~miCS N. F. Krasnav
1
Fundamentals of Theory. Aerodynamics of an Airfoil and a Wing Translated from the Russian by
G. Leib
Mir Publishers Moscow
First puhlished 1985 Revised {rom the 1980 Russian edition
© JlaA8TeJII.CTBO .Bhlcmall ml(OJlat, t980
© English translation, !'IIir Publishers. t985
~mb>
1
H. IP. KpaCHOB
A3POAHHOMHKO YaClb
I
OCHOBbl leopHH AapOAHHaMHKa npOljJHn. H Kpblna ~3AaTenbCTBO
cBwcwB.a WKonu MoCKal.
anl:~~i~I~~~m;~i~e:~~~h:~~le~fl~:11~r~~~:tt~~~ ~~ ~t~0~~~~~;11'a,~~~kd;sf:;~f
mooeru craft. The funclnmentllb of nl'rodynamics are u~ed in stu{lyinf,;' the external Dow over \"ariou~ bodies or the motion of air (a ga~l inside various objects. Engineering success in the tields of aviation, artillery, rocketry. ~pace night, motor vehicle tran~port. nnd so on, i.I~. [ields that perlnin to the flow of air or a ~as in some form or other, depends 011 a lirm knowledge of aerodynamicti. The present textbook, in ,uldition to the general law~ of ]]o\\' of a fluid, treats the application of aerodynamics, chiefly in rocketry anll modern hi~h ,peed aviation. The book conHist.:; of tll'O parts, each forming a separlltp mlume. fhe tirst of Lllem concerns Ihl' fUlulaml'ntal concepts and definitions of nerodynamirs and tht- th(>ory of flo\\' over all airfoil alld a wing, il\cllldin~ an unstead.I' Ilo\\' (Chapter~ 1-9), while the ~C('l)nd desfTibl'~ the aerodynamic design of craft and their individual parts (Chapters 10-15). The tll'O p;lrts are (le~igned for u~e in a two-s!'mester ('our~e of aerodynamics. although the first part can be u~ec! indepcn 0 Conversion of the Pressure Coefficient from M"'l > 0 to M..,~ > 0 Determination of the Critical Number M Aerodynamic Coef6.eients flow at Supercritical Velocity over an Airfoil (M "" > M ..... cr) Supersonic Flow of a Gas with Constant Specific Heats over a Thln Plate Parameters of a Supersonic Flow over an Airfoil with an Arbitrary Configuration lise of the Method of Characteristics Hypersonic .flow over a Thin Airfoil Nearly l:niform Flow over a Thin Airfoil Aerudynamic Forces alld Their Coeflicieuts Sideslipping Wing Airfoil Dclinition of a SideslippUl~ Wing Aerodpwmic Charact('ril!.tlcs of Ii Sideslipping Wing Aidoil Suction force Linearized Theory of Supersonic Flou' OIW a Finite-Span Wing Linearil.;ltioll of the Equlltion for tile ]'oteulial Fllnction Boundar,I' Connitions
~1~;nVO~I~~f~rorp~J~u?;~:sal a~dluX~r~~
dynamic Coerticients l"eatures or S\lprr~(llli(' Flow over Wings 8.2. :'.ll!thod of Sourc,,~ fI..a. Wing with It S~mmelri~ Airfoil and Triangulu l'lanforlll. (2 -u, eYa '" U)
!~~r~ o~~~~i~ih:¥d~:nd witb It Sub· Triangular Wing Symmetrie about lhe 'x·Axis with Subsonie Leadinl~ Edges Scmi-Inlinill' Wing with a Supel'S(Jnic Edge Triangular WingSym.metrie about the x-Axis with SupersoDlc Leading Edges 8.1i. Flow over a Tetragonal Symmetrk Airfoil Wing with Subsonic Edges at II Zero Angle of 'Attack 8.5. Flow over a Tetragonal Syruruetri" Airfoil Wing with Edges~of Different Kinds (Subsonie and Supersonic)
271 272 273
274.
274 278 285 285 291 293 293 ~
299 3(l1 3(5 308 308 310 313 3t5 317 321 321 326 328 330 331
343
Contents
11
Leading aud ~Ii,]d!e Edges are Subsonic Trailing l~lIgo: 15 .supersonic :y'J3 Le~ding Ed~e is Subsonic, .\liddle and Trailing Edgo:s are Supersonic 345 Wing with ,\ll Supl'r~Ollic Edges 346 General I{el,llioll for Calculating the Drag 350 8.6. l'ic!d of Applicatiun of tht Source ~Iethod 3,ll 8.i. Doublet Vi~tributio!\ ~lptLiOJ 3,l3 So!!. fo'lo\\- OH'r .:J. Triallg"lllar Wing with SubsoniC' Lrading Eligt'~ ~ fUI. Flow o\,l'r u Ill'xagOlml Wing \\'ith :'Ilbl'uni(' LcadilJg Dild Supersoni!"onal Wing with ~npl'nllni! \lolioll !'I.~'.lU~·lIa!ni;' ~tJ.lJilit~
395 398 1,04 1,116 4,,6 411, ,i08 !itO
Uelllll\wII 4111 Stabilil,- Cllara'-tcri"lir~ 413 ItG. Ba~k l\('latiun,; for Ln>: low speeds becalL:ariug Ihe )Iallie of :\. Zh\lko\"~kr. The developmcnt of adatioll, artillery, amI rocket.I'Y. and t.he mntllring of the theoretical fllndamcntnls of aerodynamirs changed the nature of acrodynamk instal latiolls, from the first, comparath'ely small and low-speed wind tunnels up to lhe giant high-speed tunnels of TsAGI (HMO) and mocil'rn hypcrsonit" installations, and also special facilities ill whirh a snpersonir. now of a beated gas is artificially created (what wC call high-temperature t.unnels. I-tho,k tUllnels, pJasma instaJIatioJls, ek,). The nature of tbe il1terartioll between a gas and a hody moving in it may vary, At low speeds, t.he interactioll is mailll~' of a fm'('e nature. With a growth ill the speed, the force interartion is attended b~' heat.ing of the surface owing to heat transfer from the gas to the body: this gives rise to thermal interaction. At YCry high spceri1.cd by a ehango in the kinematic parameters with time is usually a \'ery intricate t.a.'lk. Simplified ways of solving this problem are used lor practical pllrposcs. Such simplification is possihle \vllen the change occllrs .~lJfJi('ienlly slowly. Thif: is chararterif:tic of IlHlIlY craft. "'hell determining thcir aerodrnamic chn.racteristits. w(' ran pro('('ed rl'om the hypolhe!iis o[ steadiness in accordanee wilh which the:-;(' dl,II'(H'tcristic~ in unsleady lIlotioll nrc assumed to be thl' ~alllC;JS ill ~teallr Illolion, ilud are determined by the kinematic pnraml'ler.i;.:ed basic scientific trends have taken shn.pe in aerodYlLamics. They are (lSSOCiflled with the aerodynamic investigations of craft as a whole and their illdi\·i~ dual structural elements, and also of the most characteristi\. kiuds of gas flows and processes attending the flow over a body. It is qnite natural that any classification of aerodynamics is conditional to a certain extent becauso all these trends or part of them are interrelated. :"-Jevcrtheless, such a "branch" specializa(.ion of the aero~ dynamic science is of a practical interest. The two main paths along which modern aerodynamics is developing can be determined. The first of them is what is called force aerodynamics occupied in solving problems connected with the 2-017\$
18
Introduction
force action of a fluid, i.e. in iillding the distribution of the pressure and shearing stress over the snrface of a craft. and also with the distribution of the resultant aerodynamic forces and moments. The data obtained are used for strength analysis of a craft as a whole and of individual elements thereof. and also for determining its flight characteristics. The second path includes problems of aerothermodynamics and aerodynamic heating-a science combining aerodynamics, thermodynamics, and heat transfer alld studying flow over bodies in connection with thermal interaction. As a result of these investigations, we find the heat nuxes from a gas to fl wal1 and determine its temperature. These data are needed in analysing the strength and designing the cooling of erflfl. At the Sflille time. the taking into account of tlte changes in the properties of fl gAS flowing over a hody under the influence of high temperatures allows us to determine moro precise!)' the quantitative criteria of force interaction of both the external flow and of the houndary layer. All these problems are of a paramount importance for very high air speeds at which the thermal processes are very illtensiv(!. Even greater complicaliolU; are introduced into the solution of sudl problems, however, because iL is associated with t.he need to take into consideration the chemical processes occurring in the gas, alld also the influence of c.hemiral interaction between the gas and the material of t.he wall. If we have in view the range of air speeds frolll low subsonic to very high supersonic ones. then, as already indieated, we can separate the followillg basic regions in the science of inve~tigatilJg flow: aerodynamics of an incompressible fluid. or fluid mechanics (the Mach number of the flow is M - 0). and high-~peed aerodynamics. The laLLer, in tllfn, is divided into subsonic (M < 1), transonic (M ~ i), supersonic (M> 1) and bypersonic (1)1 ~ 1) acrodynamics. It must be noted that each of these branches studies flow processes that are characterized by certain spedflc features of flows with the indicated :\Iac.h nnmbers. This is why the investigation of such flows can be hased on a different mathematical foulldation. 'Ve have already indicated that Aerodynamic investigatiolls fire hased on a division of the [Jow ncar bodies into two kinds: free (extE'rnal) inviscid flow and the boundary layer. An independent section of aerodynamics is devoted to each of them. AerodynamiCS of an ideal fluid st.udies a free flow and investigates the distribution of the parameters in inviscid now over a body t.hat are treated as paramet.ers 011 the boundary layer edge and, cOlisequE'lI tly, arc the bOllndary conditions for solving the differential equations of this layer. The inviscid parameters inclnde the pressure. If ,ve know it.s distribnlion. we can find t.he relevant resultant forces and moments. Aerodynamics of an ideal fluid is based on Euler's fundamental equations.
Introduction
19
Aerodynamics of a boundary layer is one of the broadest and illost dc\'e-Iopcd sect,iolls of the sden('o of a fluid in mot.iOIl, 1t. studies \'is('ous gllS now in 1\ bOlilldal'Y laym', The 1'oluliOIl of [he problem of flow in a boundary III:,-'cr makes it possihlc 10 lind Ih£' di1'tributioll of the shearing stresses and. ("onscIllIcully, of the resultant aerodynamic fof("l's IIlid momcnts (',\USNI hy fl'klion. It also make::: it. possihl(> to (",II("lIia(.r. the tra!lsfer of helll from Ihe gas nowing o\"el' a hody to a houndary, The ('on('lusi(Jn~ of t.he bOlludarr la,..'cr theory ('illl also ill.' used Cor corrL'('ting lhc ~ollllion 011 in\"iscicl now, pm'lklllarly for lililling the corrert ion to tile pre!'.'1llre distrihution rlllC 10 Ille iunllen('e of the boundm'y layer, The modC!rll Ul(!oryof tht' hOlludary layer is hased Oil fundalllental iln'csligat.ions of A, XIl"ier, G, Stokc!ot, 0, HeYl101ds, L. PI'andtl, and T, "Oil Karmali, ,\ substantifll ('outribut.ioll to the de\"elopment of the boundary Illycr theory was lUade h)' the So\'iet ~cientists A, DoI'OdnitsYII. L, Loihi,yansky, A. :'Ilelnikov, 'X, Kochin. (i, Petro,', V, SII'llminsk~'. atlll otllrol'!-', TIIC'Y !"l'eat.ed a harmouium: theol'Y of the boundary laycl' in a compl'e~sib)e gas, worked alit. method!! of ('alrlllilting til(') no\\' of a \"i!-'cou~ nuid o\"er "arious hodi('s (t\\"o- and thl't'c-dimensionlll), in\"estigilted problem!> of tJle transition of a laminill' I>oundlu'y layel' into a tlll'bulcnL one, and studied the complkalc:i pl'Ohll'llI~ of tllfhulent lIlotion. In ilel'odYlUunil' iH\'cstigatiotls in\"olving low airspeeds, the thermal proe(lSS(l!-t in the hOUtHlil!')' layer do not havC! to bro taken illio ,H'('Olltll ul'('aw<e of tlwit' low iut.enllity, "'hen high !oipl'Nis arc iuvoh-ed, howen'l', lIt'rount Illlt:-;t be taken of heat transfer and of tite influence of the high hOlllldllry layer temperatur('!'! 011 rrktioll, It i!'l quile natltral tbat abumlallt attention is being gi\"en to Ihe :'!ollltion of slldl problem!;. especially recently, In t.he SO"iet L'nion, professors L, Kalikhman, I, Kibei. V, lye\"Jev and others al'e developiug the gas-dynamic theory of Ileal. transfer, stlldying tllc ,'is('olls Row 0\'("1' ,'arious bodic!'! ot high I("mpel'ature!'! of the boundal')'layer, Similar prohlems arc also heing :o:ol\"ed by U Ilumber of foreign scienti!'!t~.
AI hypersouic flow speptls, the prohlt'ms of 1I("l'oclyuflmic heilting liot the only on(l~, That ionization Q('t'III'S fit· sneh sp('eds because of the J1igh temperat.ures and the gas begins to ("(lIuluct ele theory of 11 lifting plane in an ullsteady now. Keldysh and La\,rentre" !'o\"ed the important prohlem 011 the now over a \'ibrating airfoil by generalizing Chaplygill's method for a wing with varying circulation. Academician Sedoy estAh1i!>hec\ general formulas for ullsteady aerodynamic forr,C!'I and moments acting on :m arbitrarily moving wing. Profe!'1sol'S F. Frankl. E. Kra!>ilsllchiko\"a. and S. Falko\'ich developed the theory of steady and unstead~' supersonic now O\'er tllin wings of various conligurations. Important results in studying unsteady aerodynamic."I of a wing were obtained by professor S. Uclolserko\'sky, who widely used numerical methods and computers. The results of aerodynamic in\'estigations of wings can be applied to the calculation of the aerodynamic characteristics of the tail unit. and also of elevators and rudders shaped like a wing. The specifiC features of flow over separate kinds of aerodynamic elevators and rudders and the presence of other kinds of conlrols resulted ill the appearance of a special branch of modern aerodynamics-the aero-
dynamics or controls. Modern roc.ket-type craft often have the conliguration of bodies of revolution or are close to them. Comhined rocket systems of the type "hull-wing-tail unit" ha\'e a hull (body of revolution) as the main componellt of Lhe aerodynamic system. This explains why the aerodynamics of hulls (bodies of revolution), which has become one of the important branches of today's aerodynamic science. has seen intensive development in recent years. A major contribution to the development of aerodynamics of hodies of revolution was made by professors f'. Frankl and E. Karpovic.h. who published all interesting scientific work "The Gas I)ynamir~~ of Slender Bodies" (in Russian). Tile Soviet scientists I. Kihei alld F. Frankl. who specializefl in aerodynamic!';. developed the method of characteristic.Oj that macie it possihle to perform effective calculations of axisymmetric supersonic flow past pointed bodies of re"olutioll of an arbitrary thickness. A gl'oop of scientific workers of the Institute of Mathematics of the USSR Academy of Sciences (K. Babellko, G. Voskresensky, and others) de"eloped a method for the numerical calculation of threedimensional supersonic now o,'er slender hodies in the general case when c.hemical reactions in the now are taken into account. The important problem on the supcrsonic flow over a slender COlle was solved by the foreign specialists in aerodynamics G. Taylor (Great Britain) and Z. Copal (uSA). The intensivc dewllopment of mo(lern mathematics and computers and the illlprovemeni on Ihi~ ba~is of the methods of aerodynamic
Inb-odudion
23
in\"esligations lead to greater and greater f:ucces~ in soh-ing m.my (:omplicaled problems of aerodynamics including the determination of till' o"eralJ aerodynamic charac.teristics of a craft. Among them are the aerodynamic derh'atiYes at subsonic speeds, the finding of which a work of S. Belotserko"sky and B. Skripach 14.1 is devoted to. In addition, approximate methods came into u~e for appraising the effecl of aerodynamic interference and calculating the releyant corrections to aerodynamic characteristics when the latter were oblaim'd ill the form of an addiLi"e sum or the rde"ant characteristic's of th(' illdi\"idual (i!lolated) elements of a craft. The solution of such prohlems is the subject. of a special brand. of til(' aerodynamic
scieurc-interferenee aerodynamics. At low slLper!'onic speeds, aerod:'tr('~('s acting on 11 fa('(' 01 an ~'Iementary fluid Jlartid~'
hllvin~
Ihe ShllPI' of a tctl'ahed-
I'on
Allotlu'[' fOl'ce nctillgon the il>olatt'd tluid nllulI[e is the mass (body) force proportional [0 the mR~li of th€' particle ill Illis \'olume, \[ass forccs indude gravitatinnoi ones. 1' to the lilllit \\"itll 6.,r. !!.!I. lind j,z telldiug to zero. COllsequcutl~'. thc [('1'111:< conillilliug ~l-V/6.S,~ will 111so tend to ZPI'O b('~'1111:;(! !!.W is l\ small qllautitr or the third ()rt\C'r. while 6.S,. is a small <jlllllltity of till' :,,'ant mean square componpnts of the Ilu('tllution velocities, designated lly fJ, find 1';2 [lod determinl?d from the (Ixpr('ssion
T'"7.
V;."!",:)""
I~~II
I,
JV~·~y,t)dt I,
The concepts of IJ\li.ltiOIl!; motiOIl (11)(' Reynolds eqllation~). Sudl e!';s pressure (p - P«» dS and the tangential • Wc sllall omit the won] ·,.omponents" Jx.low for bre\'ity,
it and use fonnulo3 for scalar quantities.
hu~
shall mean
Ag.U.i ActioD of pftMurC and friction
!sr~~ar) forces on an elementary
force 't dS. The sum of the projeetions of these forces onto the x·axis ·of a wind «(]jgnt path) coordinate system is (Fig. 1.3.1) /\
/\
r(p- p",,) cos (n,x a) + "tcos (t,xo») dS (1.3 .1) where n aud t are a normal and a tangent to the olement of area, respectively. The other two projections onto the axes Ya and z. are obtained by a sirnilar formula with the corre.sponding cosines. To find the resultant forces, we have to integrate expression (1.3.1) over the entire !.urface S . Introducing inlo lhe.sc equations the pressure cOPUlcicnt p = (p - p"",)/q"" and the local friction 'actor Cj .:t = 'tlq "", where q"" = p ... V!. 12 is the velocitv head. we obtain formulas for the drag force, the IiCl force, and the side force, respectively:
x .. =
q"",Sr
~ (S)
"
y~ ,.."qocSr)
fp cos (~,~.H-c,. :tcos
(t.i.)JdSIS r /\ r-pcos(n,y.)+c,.xcos(t,Ya)]dSISr
(1.3.3)
1fPCOS (;;,~.)+c, . %cos(r.i.)ldSISr
(1.3.4)
/\
(1.3 .2)
IS)
Za = -q"",Sr
lSi
We can choose a random surface area such as that of It wing in plan view or the area of the largest cross section (the mid·section) of the fuselnge as the charactoristic area S t in these formulas. The intograls in formulas (1.3.2)-(1.3.4) are dimensionless quantities taking into account how the aerodynamic forces are aHected by the nature of the flow over a body of a given goometric configuration and by the distribution of the dimensionless coefficients of pressure and jfriction due to lhis flow . . In formulas (1.3.2) for the force X . , the dimensionless quantity ,lS usually designated by c Xa and is known as the drag coeffaclent.
Ch. 1. gasic Information from Aerodynamics
43
III the othl'r two fOI'lnulos, the corresponding symbols cUa and c'a
Za """ cZ/lqooSr
(1.3.5)
We can oLlain generol relations for tI[(~ moments in the same way 8~ formulas (1.3.2)-(1.3.4) for the forces. Let liS consider as an example slI('h a r('iation for !lu' pitching mom(,nt ,1[ •. It is evident that the e]('mentllry vallie of this moment d;\/zll is d~t.ermined by the sum of thE' morrwnLs about the axis ZII of the forclls acting on an area dS in i\ plane al right allg'ks 10 the nxi~ ZII' If the coordinat.es of t.he Ilrea dS arc Ya
JF;,dS
s,
b
and
+ C:t.b ..:... C:t.f
C.~.b ~ q:~r
where Pb = (P.b - poo)/qot> (this quantity is negative because a rarefaction appears after a bottom cut, i.e. Pb < pool. Characteristic Geometric DimE'nsions. The absolute value of an aerodynamic coefficient. which is arbitrary to a certain extent.
Ch. 1. Basic Information from Aerodynamics
:~~e~!':ic I,.-c~ntr"
45
vicw of a wing:
chord, bt-till lind b-Iocal chord
chord.
depends on the choice of the characterigtic geometric dimensions S rand L. To facilitat.e practical calculations. however, a characterb~ tic geometric quantity is dlOsen beforehand. In aerogpace technology, the area of the mid-section (the largest cross section) of the body Sr = SlIllri is usually chosen ag the characteristic area, and the length of the rocket is taken as the characteristic linear dimension L. In aerodynamic calculations of aircraft., t.he wing plan area S r .= = Sw, tlle wing span l (the distance between tlw wing tips) or the wing chord b arc adopted as the clHlracteristic (Iim('nsions. By the chord of a wing is meant a length equa! ") the distance between the farthest points of an airfoil (section). For n wing with a rectangular pianform, the chord equals the width of the wing. In practice, a wing usually has a chord varying along its span. Either the mean gPOmc:tric chord b = b m equal to b m ~ Swfl or the ml'an aerodynamic chord b = b A is taken as the characteristic tlimengioll for such a wing. The mean aerodynamic chorl] is determined ag the chord of the airfoil of an equivalent rectangular wing for which with an identical wing plan area the moment aerodynamic characleristics are approximately the same as of tlw given wing. The length of tile mean aerodynamic chord and the coordinate of its leading edge are determined as followg (Fig. 1.:l.2):
bA=~ Sw
1/2
I b'l.dz, u
When calculating forces and moments according to known aerodynamic coefficients, the geometric dimensions must be used for which these coefficients were evnluated. Should guch calculations have to be performed for other geometric dimensions, the aerodynamic coefficients must be preliminarily converted to the relevant geometric dimension. For this purpose, one mnst use the relations C1Sl = C 2 S 2 (for the force coeflicients). and TnISIL I = Tn 2S 2 {'2 (for the moment coefficients) obtained from tilC conditions of th(' constancy
46
Pt. I. Theory. Aerodynemics 01 en Air/oil end eWing
Fill. t.3.l Constructing 8 "polar of the first kind of a craft: a-e'l'a vs. a: /.I-Cyll. vs. a; c-polsr ot hrst kind
of the forces and moments acting on the same craft. These relations are used to fmd the coefficients C 2 and m 2 , respectively, converted to the new characteristic dimensions 8 2 and L 2: c2
=
c1
(8 1 /8 2 ),
m 2
=
ml
(8 1 L I /8 2L 2)
where the pr~vious dimensions 8 1 , L] and aerodynamic coefficients c1 ' ml , as well as the new dimensions 8 2 , L2 are known. Polar of a Craft A very important aerodynamic characteristic
~h:;af~~i \.f:~;atl~~~~s~r~:I~tf:~ ~~t=Zea~ t~e ~?f~~~da~r~~e f:r~:: o~~ which is the same, between the lift and drag coefficients in a flight path coordinate system. This curve, called a polar or the first kind (Fig. 1.3.3c) is the locus of the tips of the resultant aerodynamic force vectors Ro acting on a craft at various angles of attack lor of the vectors of the coefficient ella of this force determined in accordance with the relation en~ = RII./(S rq (m)1. A polar of the first kind is constructed with the aid of graphs of C!f A versus ct and cVa versus ct so that the values of C!fa and cJlll Me laid off along the axes of abscissas and ordinates, respecth·ely. The relevant angle of attack ct, which is a parameter of the polar in the given case, is written at each point of the curye. A polar of the first kind is convenient for practical use because it allows one to readily flDd for any angle of attack such a very important aerodynamic characteristic of a craft as its lift-to-drag ratio (1.3.10)
(or Y a) and C!fa (or X.) are the same, the quantity K equals the slope of a vector drawn from the origin of Coor(JiIf the scales of
eVA
Ch. I. Basic Information from Aerodynamics
47'
.'
~ "
'.
o
Flg.UA
'x
))rag polar or the second kind
nates (the pole) to the point of the polar diagram corresponding to the· chosen angle of attack. We can usc a polar to determine tbe optimal angle of attack "oPt corresponding to the maximum lift·lo-drag ratio: K maz = tan "oPt
(CUO')·
if we draw a tangent to the polar from the origin of coordinates. The characteristic poinls of a polar include the point cllamaz corresponding to the maximum Jifl force th.d is achieved nl. tIle critical angle of attack Ct cT ' We can mark n point on the- curve determining the minimllm drag coefficient cX.amlll and tht' corresponding values of the angle of all lick and the lift coeflicient. A polar is symroetl'k llbout the axis of ah::cissas if a craft has· horizontal symmetry. For .such n craft, the vattIC of ex min ('orresponds to a zero lift force, c lla = O. ' .• In addition to a polar of the flrst kind. a polar or the second kind is sometimes used. It dWers in that it is plolLecl iii a bo(ly axis coordinate system along \.... bose axis of abscissas the \"alues of the longitudinal-force coefficient COl' arc laid off. and along the axis of ordinates-the normal-force coefficients cy (Fig. Ut4). This curv6 is used, particularly, in the strength analysis of craft. Theoretical anel experimental investigation~ show that in the most general case, the aerodynamic coefficients depclul ror a given body configuration and angle of attack on dimensionless variables such as the Mach number Moo = V oolaoo and the Rernolds number Beoo = V ooLPoo/p,oo. In these expressions, a_ is the speed of sound in the oncoming Dow, poo and ~oo arc the density and dynamic viscosity of the gas, respectively, and L is the length of the body. Hence. a multitude of polar curves exists for each gh'cn craft. For example, for a definite number Be oo • we can construct a family of such curves ench of which corrC!>ponds to a definit.e value of the
48
PI. I. Theory. Aerodynamics of an Airfoil arKt a Wing
Fig. U.S Determination of the centre of pressure (a) and aerodynamic centre (b)
velocity Moo. The curves in Figs. 1.3.3 and 1.3.4 corrospond to a fixed value of Re"", and determine the relation between cYa and cra. for low-speed nights (of the order of 100 mis) when the aerodynamic coeflicients do not depend on Moo. Centre of Pressure and Aerodynamic Centre. The centre of pressure (CP) of a craft is the point through which the resultant of thc aerodynamic forces passes. The centre of pressure is a conditional poinL because actually the action of fluid results not in a concentrated force, but in forces distributed over the surface of the moving body. It is customarily assumed that for symmetric bodies or ones close to them this conditional point is on one of the following axesthe longitudinal axis of the craft passing through the centre of mass, the axis of symmetry of a body of revolution, or on the chord of an airfoil. Accordingly, the longitudinal force X is arranged along this axis, while the centre of pressure when motion occurs in the pitching plane is considered as the point of application of the normal force Y. The position of this centre of pressure is usually determined by the coordinate xp moasured from the front point 011 the contour of the body in a [Jow. If the pitching moment ill: about this point and the normal force Yare known (Fig. 1.3.5a), tho coordinate of the centre of pressure (1.3.11) A moment Mz tending to reduce the angle of attack is considered to be negative (Fig. 1.3.5a); hence the coordinate xp is positive. Taking into account that
M:=mzqooSrb we obLain
and
Y=cyqooSr
Ch, 1. Buic In/ormation from Aerodynamics
49
wheuce
(LUI') The dimensionless quantity Cp dermed as the ratio belwcell the distance to the centre of pressure and the characLerisLic length of a body (in the gi ....en case the wing chord b) is called tlte centre-ofpl'e~ure coefficient. With small angles of attack, wlten the lift and nOl'mal-force coefficients are approximately equal (c Ya ~ c y ), we have (1,3.12)
In the case heing considered of a two-dimensional fio\\' past a body, Lh(' pitcldng-molllent cocfflcieuts in wint.l (Right path) and body axis coordinate sy. all zero Y[llnes in accordance with the expressions
=
Cy
= (iJc,/oa) a,
lnz
= (ilmz.:aa.)
IX
holding at small angles of attack (llCl'e the (leri\'llti\'es (jcl/.'O(l. and omz'da are COJlstant qU normal force dm' to the cle ...·atol defit;'('U(}TI angle nud proportional to this angle is known as the t'lcutor·dt'11ection aerodynamic ct'ntre. The moment of the forces about. a lateral axi~ pa~sing through lhis centre is e"ideutly indL"pendent of the anglo be' In the geJleral ense for nil o:-;ymmelric. configuration, its centre of pressure coincides with none of the aero~ d~·lul.mic centres (based on a or B,,). In a particular case, in a sym~ melrk crnft at« --; D. the centre of pressure coincides with the aerod~"Tlamir centre based on Bel'silll! the definition of the aerodynamic centres hased 011 the angle of attack "lid the elevator deflection angle and introducing the corr~pollding coordinates XFa, and X"'II' we find the ("oelflciellt of the moment ahout tile centre of mass. This ('oemcienl is evaluated by formula (L:l.22), iu which (1.3.24)
where XF~ = x,/b and X-;6 = the aerodynamic centres.
xF/b
are the relathe coordinat~s- of
1!i2
PI. I. 1I':eory.
Aeroclyn~mics
of en Airfoil end I Wing
t .... Static Equilibrium and Static Stability CDncept of Equilibrium and Sfilllility
The stllte of static equilibrium is determined by the flight conditiol\;:; and the corresponding force action at which the overall aerodynllluic moment abont the centre of mass in the absence of rotation and wHh the angle of attack and the sideslip angle remaining constant is zel'O (l'1 = 0). Such equilibrium l·orresponds to conditions of steady rectilinear motion of a craft, when the pal·amete!·s of this motion do IIOt depend 011 the time. It is eddelll that for axisymmetric configuration!' over ,,"!lich the fluid 110w:; in Ok longitudinal dil'ection, the equality)1 .= 0 is arhie\·ed ,vith IIlIIlenel'te« ",le,'ators and l'ndder~ and wilh zero angles of aLta.k and :::id~1ip, Hence, ill this rnse, equilibrium, ('allcrllhe trim equilibrium of a craH. sets in tlt the balanc(' angl(' of aHat:k and sidt·slip angle (cz.blll' ~blll) equal to zero. The Med to halallce Ilight al olher angles (0: =F ablll aud ~ =F ~I>III) requil'es the cOl'respouding turniug of Ihe elevators. EquilibriullI of a. craft (pal'licuhu'ly. with the elevators I'xed in place) may be stahle or Ilnstable, Equilibrium of a Cl'I1ft b; considel'ed t.o he stable if arter lhe introduction of a random r;horl-Lil11c (I\."turhance it retnrns to its initial pO!'lition. If these distlll'bnlLcc" cal1se it to delleI'I ~lill more from the initial position, eqllilibrium is said to he l.IIIstabl('. The nature of t.he equilihrium of a. cl'aft is dctcnnirwtl hy its static stability Ol' instability. To rcycal the l'sscnce of slat ic stahility, we call consider the Oow of ail' in a wiud tunnel PMt a c.raft lixed at its ceutre of lDass and capable of turning abottt it (Fig, 1.4.1). For a given elevator angle 6"" a definite value of the aerodynamic nloment :1l z ('orresponds to each value of lhe ungle or del1ectioll of tile craft Ct (the angle o[ attnck). A pos."ible relation between Ct and :Ifz for n c,erLAi .. angle 6(" is showu iu Fig. 1.4.1, where points 1, 2, and 3 det('rmiuillg t.he balance angles Ctlbtll, Ct~bal' and a;3b~1 at which tile aerodynamic moment equal:,; zero correspond to the equilibrium positiolls. The ligure also ~hows two other moment clIr,'cs for the Gh~','alor angle." li,: and a;. Let HS ,'oll."idor equilibrium at floint 1. If UtC craft is de\'iated tbrough nil 1111~k' smaller or lat'ger than a.'bal' the iuduced momenls, positivI) 01' !Lpnnth'c, l'esp('!~th·ol:t', will result ill tm incrensc (reduction) of this mlg-Io to it.;; previolls ,'aille alh,al' i.e. these momonts nrc stahilizin.e; on('.-=. Con~equ(lntlr, lhe po~itioll of eflniliill'ium at point 1 is stahle (thf' ('!':lft is sLatknlly sllIhle). It can he showll !'imilarly that sneh a po~itit)1I of stable c'luilibduln also (,_ol'l'esponds to point 3.
Ch. 1. Basic Information from Aerodynamics
1!13
Fig. tA.t
Dependence of the aerodynamic
~~~~~n~ ~y ~ :'~ftt~~d~~e u~~
rRection of the eh!\'alorl:l lie:
2, 3, ,,_.polnls or inlel'lH't'tion of
In the Ii!':.;t C!l!"C, fl'cc rot.ation or lhc l'l'nh rOlltilllle:o; IIlIlil it o('('lIpie:; the clplilibrimn po~i!ioli ai, point 1. /In(1 ill the sel'ontl ('il~e-at poiut 3, At. point 2 (a 21'nl) the equilihrium i:-; lJIlst;lbll'. I IHlcpd , eXiuuiu· .. Iloll of I"ig, 1..1.1 1'(>\'(,.. 1:-1 Ihnl at nllues of 111(' angle a lilrgN or slllall(,I' than ct 2La l' momellt~ al'(' iJ1(illl't,tI, po~iti\'e or negatiH'. re· sperlively. thai lend 10 illrl'l~fl~e (01' I'et!ul'e) ct. IIt'nre. these mmnents
arC' destabilizing, flnd tlw !'raft. will be
~Iiltis insignificantly. The constancy of the angular velocity is dl1e to the eqllilibriulll of the pitching moments about the lateral axis, i.e. to longitudinal baloncing of the craft at which the ('qnoli!y JI z :...:' 0 hold.", i.e. m: o -:" m~O::bal
+ m~1!6~ -j- m?,Qz =
0
This equation allows us to find the elevator angle needed to balanced flight at the given values of o:.onl and Qz; 6c .bal = -(1Im~.) (mto
+ m~o;Lal
..:..
m;:Q%)
eJ\~ure
(1.4.3)
For conditions of a high static stability, we have m~'Qz -%:: mfa: bal ; consequently 6~.bal = (-1/m~e) (mzo ..!- m~abal) (1.4.3') For a craft with an axisymmetric configuration, mzo = 0, therefore 6~.bal = -(m~/m~e) abal (1.4.4) The normal (lift) force coefficient corresponds to the balance nugle of attack and elevator angle, namely, cV• bal = cvo
+ (c: + c:e6e.bal/abal) abal
(1.4.5)
Ch. I. Basic Information from Aerodynamics
5T
The "alues of c yo are usually very small even for as~'mmetri('. COIJfigurations (at low be and a) and equal zero exaet1~' for craft wilh axial symmetry. lIellce, with a sllffIcient degree of nccurary, we can write
Static Lateral Shlbliity
To analyse the lateral stability of a craft. one mus!. con.s Ill} lind III~ coincide. li0n('c. ill 1\1I,,1~'~ilJg roJlilig motion. we ran lise the derivativc m~ kno\\'1l as the ('o('rfll'h'nt (df'gred of static rolling stabiJHy. Static directional stability is eiJaractNi1.C'd hy 11 cO('i"fIdl'Il1 (dl'gTl'e) dl;ltermincd by the derivative il.lIy/i.i~ {or (/fII!liuf1 .. 11I~:). If Lhe CIuantity //IV < 0, the craft has statir directional ."tabilitr: al /liD> > o. il has static instability. and when =-- O. l1('utrality. The {'oncept of directional stability is af':soriated with the pl"Opertr of a ('fflet to eliminate an appearing side!'Jip unglll~. .At lhe same time. a crail doe,.: not maintain the .g· sible nHil1 at illlillih'l~' hi!!h l'p('('(1 IIncl, ('nll!'l'cllIl'nlly, thc I'atio of the night ~p('t'd to thai of !'ol1lul t('lId!' to 7.t'I'O, :\1odel'Jl ('I";\ft lli!\'t' high llirl'p('('(I:< at whilltlll'!'!' of Ilil!i1-!'Jl('('d ;ll'l'flIl~,t1;l111ic:1lt'rJrr of ol'dt'reIlIJWl'atlll'c of till! ol'{h.'I· nf I;JlJ(J I" ('xcitalion of th(' \'ibra· tional It\'l'is I)f till' inlf'I'llill (,Il(lrgr of Ih(> O:.:~·gt'll nud llitl'Og('U mole("ul('s ill th(' I~ir hl"collll'~ noticl'ilhle. AI a Ipmpl'I'llhll'l' of I\bnut. 3(100 K illlli a prl'~~\Il'l' of IO~ Pa, llit' yibrational degrl'l'l' of freedom of the oxrgl'll moit,t"I1I(',«. m'(' f'ompll'tl'\r ('will'd, and further e(e\'atioll of til(' it'llIJlt'l"atlll'(' allow." llil' atolll." to SlIl'TllOlUl1 th(' m'lion
eo
Pt. I. Theory. AerodynlmiCs 01 In Airfoil lind II Wing
of the intramolecular forres. As a re.~tJlt, f01" example, a dilllomic molecule breaks up into two individual atoms. This proress is known as dh_socialion. The latter is attended by J"('combination-the formation of a Ilew molecule when two atoms collide (0 2 ~ 20), This heat-producillg reaction is 8('companied b)' the collision of t.wo I'Itoms with a t.hird partide that carries on part of the released energy and t.hus ensures the creation of a stable molecule. In addition, ('.hemical reactions occur ill the air that result in the appearam',eof a ('ertain amonnt of nitrogen Illonoxide ~O. The latter also di5.~ oi intt'raclioll helw(>('u al()nl~ lI[lnll lite di~.'ratll!'(J, Till' atul'c on the spf'ritk IWllt nl il ,'011"(,1111 pl'('_-~II1'1' ("Ill i,\'
the
(01'01111.1
where Ille e,'ipf)llelit 'f'
ill IU1'n. ,11'PC'lIli.-< 1,; ill, Ihe .'-:pc(ilic Ilrat d('pelHb 1I0t oaly 011
thc Icm"('I'III11n~_ IJlII ;11.~0 on tlu! p.'t':;SIII'C, Thc ~I)f'dfll' hCill~ and thc adi11' and (curl V)z = 2wJ:
Ch. 2. Kinematics of ,. Fluid
79
U. VOIteI·Free
MotIon of • Fluid
When investigating the motion of a fluid, we may often take nl) account of rotation because of the negligibly small angular velocities of the particles. Such molion is called vortex-free (01' irrotational). For a vortex-free flow, (0 = 0 (or curl V = 0), and, consequently, the vortex components 00;.;, OO Ut and 00: equal zero. Accordingly, from formulas (2.2.3) and (2.2.6) we obtain aVxliJy = aVuJax. aVz1iJy = aVulaz, 8V x!{)z = dV:,'8z (2.3.1) These equations arc a necessary and sufficient condition for the
~i~e~~~t}~~~~~~~~lil~~:Cte~z~g ~ft:Kot :r:ad~l;i~ I;~ :h~o::~~i,~:~e~; th~e:~:;~:lngC~~;of~~nc~~o~:Ci~ ~~~ :~r~ ~z'(x, y, z, t) and considering the time t as a parameter, we can write the expression dq> = Vxdx
+-
l!.,dy
+ l':dz
On the other hand, the same differelltial is d~ ~ (8~Jax) dx -i- (8~J8y) dy + (a~,a,) dz Comparing the last two expressions, we fmd Vx o'fiiJz, VII = oqJJag, V: = {)cp/iJz
(2.3.2)
The function qJ is called a velocity potential or a potential function, and the "ortex-free flow characterized by lhis function is called a potential ftow. Examination of relations (2.3.2) reveals that the partial derivath'c of thc potential
V.=" rs:nlj . ::
(2.4.39)
Contfnulty Equation 01 Gas flow .1.,. • Curved Surt.ce
Let us consider a particular form of the continuity equation in .curvilinear orthogonal coordinates that is used in studying flow over a curved wall. The x-axis in this system of coordiuates coincides with the contour of the wall, and the y-axis with a normal to this wall at
Ch. 2. Kinematics of
/I
Fluid
B7
Fig.l.U
To the derivation of the
COli
tinuily equation in curvilinl'.1r coordinalA's
the point being considered. The coordinates of point P 011 the plane (Fig. 2.4.3) equal the length x measllred ~dong the wall and the distance y measured along a normal to it.. respectively. Assume that the wall is a surfRce of revolut.ion in an Rxisymmetric flow of a gas. The curvilinear coor(linates of point. Pare:
ql = X, q2 = y, q, = )'
(2.4.40)
The elementary lengths of the coordinate line arcs are ds1 = (t
+ ylH) dx,
ds z = dy, ds a = r d)'
where r is the radial coordinate of point P measured along a normal to the axis of the surface of reyoilltion, and R is the radius of curvature of the surface in the section being considered. ConsequenLly, Lame's coefficients are hi = t -I- y/ll, h z = I, h3 .= r (2.4.42) Let us llSC formula (2.4.21t)Jor div V in which the velocity components arc VI = V:r = ds1idt = (t .:" y/ll) dx/dt. tt"2 = Vy = dy/dt. V3 = 0 (2.4.43) Substitution yields divV=
(1+~_R)r {8(;;"r)
+ iJll'-yr~:7U!R)I}
(2.4.44)
Let us calculate tile total derivathe for the densit.y:
*-0'=*+*-.*+-*.*
=-"*"1- 1;=/ll ."*-7- Vy"*
(2.4.45)
88
PI. I. Theory. Aerodynllmic$ of !In Airfoil and a Wing
Introducing expre!;sions (2.4.14) and (2.4,45) into (2.4.1), after !;imple transformations we obtain the continuily C'quat.ion *r(t....!...y/R) + iJ(r;xv -,\,) ~ arpr(I-~-:!R)Y'l/1
(2.4..46)
When studying the motion of a gas ncar a wall with a small curvature or in a thin layer adjacent to a surface (for example, in a houndary layer). the coord in ale y« R. Consequently (Op/ot) r
-+
iJ (prV3C)/OX
+ iJ (prVy)/oy
'""- 0
(2.4.47)
The form of the obtained equation is the same as for a surface with a straight generatrix. For steady now d (prV.,JIOx
+ a (prVy)/OY
= 0
(2..1.48)
For two-dimensional flow near a curved wall (a cylindrical surface), the continuity equation has the form *(1-:-yJR)+
For y
«R.
a(~:.\.)
+
arpV'/~y-i
ViR)!
-.0
(2.4.49)
we approximately have op/ot -t- u (p V;c)/ux -/. u (p V y)/uy --. 0
(2.4.50)
Hence, for flow near a wall, the continuity equation in curvilinear cootdinates has the same form as in Cartesian coordinates. For steady flow, aplat -= 0; in thi!; case the continuity equation is D (pV.)IDx + D (pV,)18y _ 0 (2.4.50') Equations (2..1..18) and (2.4.50') can he combine(1 into a single one: d/(pv,..r8)Jax a (pVyr8)/ay 0 (2.4.48')
+
0....
where E = 0 for a two-dimensional plane flow and e = 1 for a threedimensional axisymmetric flow. Flow bte Equation
Let us consider a particular form of the continuity equation for a steady fluid flow having the shape of a !;tream filament. The mass of the fluid in a fixed volume confllled within the surface of the filament and the end plAnE" ('.ross sections docs not change in time because the condition that up/at 0 is observed at every point. Hence the mass of the fluid entering the volume in unit time via the end cross section with an area of 8 1 and equal to PI VIS 1 is the same as the mass of the fluid P2 V 28 2 leaving through the opposite cross seclion willi an area of S2 (Pt and P2 are the densities, Vl and T'2 are the speeds in the firsl and second cross seclions of the lilamenl, respectivE'!0-
Ch. 2. Kinematics of a Fluid
89
Iy). We thus have PIV1St ., P2V2Sl. Since this equation can be related to any cross secLion, in Lhe general form we have p VS = const (2.4..51) This is the flow rale equation. 1.5. Stream Function
The studying of II ,·ortex-rree gas flow is simplilied because it can be reduced to the fmding of one unknown potential fUllction completely determining the flow. We shall show that for certain kinds of a vortex flow there is also a function determining its killemath: characteristics. Let 115 cOllsider a two-dimensional (plane or spatial axisymmetric) steady vortex now of II fluid. It call be established lrom continuity equation (2.4.32') that there is a lunction 'If; of the coordinates x and y determined by the relations a¢lax c -PII'V,; 8¢lay ~ PY'V. (2.5.1) Indeed, introriucing these relations inlo (2.4.32'), we ohtllin ax) ,- 82¢/(8x ay), i.e. an identity. Substituting (2.5.1) into t.he equation of slr('amliu('s Vyl8y .. , V:Jlldx wriLten in the form
8~1J;/(ay
pytVy dx - flytV:Jl dy '""" 0
(2.;").2)
we obtain the expression (a'i'iax) dx -i. (a¢lay) dy = 0
from which it follows that (2.5.2) is a dWerelltial of the fUllcliol! '" and, consequently, Integrating (2.5.3), we find an equation of stream lilies in the form 1f (or, y) """ const (2.;JA,) The function1p, called the stream function, completely determines the velocity of a vortex flow in accordance with the relations V. (l/py') 8¢lay, V, - - (1/py') O¢iaz (2.;'.0) We remind our reader that for a two-dimensional flow, we hav~ to assume in these expressions that e ,. . ,. , 0, while for a threc-diml'lIsional axisymmetric flow e = 1 and y = r. A lamily of streamlines of a potential flow can also be charact('rized by the function '" "'- const that is aSSOciated with the velocity potential by the relations a'Piax ~ (lil'lI') 8¢lay,
a
(2.8.1)
The function W (0) that is determined if the fUllction of two real variables If ::-; If (x, y) and W=: W(x, y) satisfies differential equations (2.5.9) is called a complex potential. If we recall that the values of the functions If (x, y) or~ (x, y) allow one to determine the velocity field in a moving fluid unambiguously, then, (',onsequently, any two-dimensional flow can be set by a complex potential. Hence, the problem on calculating such a flow can be reduced to finding the function W (0). Let us ('alculate the derivative of the function W (0) with respect to the complex variable cr: dWId0) ~ (qI2,,) (111 r + tel
en. 2. Kinem!ltics of II Fluid
99
v,
Flg.l.9.t
General view of II forward plane-parallel now
Flg.l.9.l
A two-dimeDSional point source
where r is the distance to a point with the coordinates x and y (the polar radins), anti 0 is the polar angle. It follows [rom the obtained equation that ~ ~ (qI20)
In r
~ (q/2n)
'" ~ (qI20)
In V x' -\- y'
e
(~.U.8) (~.9.9)
'Ve find from (2.9.8) that the radial velocity ('omponent (in the direction of the radius r) is iJcp/iJr = V~ = q/(21(r)
(~.9.!O)
and the componellt along a normal to this radius is Vs = O. We thus obtain a flow whose streamlines (pathlines) are a family o[ straight lines passing through the origin of coordinates (this also follows from the equation of a streamline 1j> = const). Such a radial flow issuing from the origin of ('oordinates is called a two-dimensional point source (Fig. 2.9.2). The rate of flow of a fluid through a contour of radius r is 2:nrl'r = = Q. Introducing into this eqllat.ion the value of V~ from (2.9.10),
100
pt. I. Theory. Aerodyn~mi(;$ of ~n Airfoil ~nd ~ Wing
we fmd Q = q. The constant. q is thus determined by the rate of flow of t.he fluid from the source. This quantity q is known as the intensity or strengtb of tbe source. In addition to a source, there is a kind of motion of a Ouid called a two-dimensional point sink. The complex potential of a sink is W (0) = - (qI2~) In 0 (2.9.11) The minus sign indicates that unlike a source, motion occurs toward the centre. A sink, like a source, is characterized by its intensity, or strengt.h, q (the rate of flow). !hree·m.enslon.r Source and Sink
In addition to two-dimensional ones, there also exist three-dimen· sional point sources (sinks). The flux from them is set by the following conditions:
V~= 4~
'7;
Vu= ,~ . ~:;
v¥=
4~' ~
(2.9.12)
whore R = V Xl + y2 + z.2 aud q is the strength of the source (plus sign) or sink (minus sign). The strengl.h of a source (sink) equals the quantity q defined as the flow rate (per second) through the surface of a sphere of radius R. The resultant velocity is V=VV~+V:+V:=±q/(4nR')
(2.9.13)
and coincides with the direction of the position vector R. Conseqnentl~·. the velocity potential depends only on R and. therefore.
8 't zx = G'V:,; (3.1.15) where 'VIIX' yy:. and 'Vu are the angles of shear in the directions of the axes z, x, and y, respectively. A comparison of formulas (3.1.15) with the corresponding relations (3.1.5) for a viscous fluid reveals that these formulas can be obtained from one another if the shear modulus G is replaced by the dynamic viscosity Il, and the angles of shear y by the relevant values of the speeds of distortion e of the angles. In accordance with this analogy, when substituting Il for G in formulas (3.1.14) and have to (3.1.14'), the strains (relative elongations) e,;.6 11 , and be replaced with the relevant values of the rates of strain 9" = by = lJV,;llJx, 9 11 = lJVyllJy. 9: = aV:llJz, and the volume strain the rate of the volume strain 9=fJV:/lJx+lJV ll lay + lJVz/Jz =div V. The relevant substitutions in (3.1.14) and (3.1.14') yield:
a
a
a
e:.
e
P,;:r:=-p+v.(Z 0:Xx --}divV) pyy=-p+.v.(2 0:VY --}divV) PZI= -P+1l
(z
O~' --}div V)
(3.1.16)
Ch. 3, Fundlimenfliis 01 Fluid Dynllmics
111
The second terms on the right-hand sides of expressions ,(3.1.t6} determine the additional stresses due to viscositv. By using relations (3.1.4), (3.1.4'), (3.1.5), and (3.1.16), we can evaluate the quantities P x , PilI find Pl' For example, for P x from (3.1.4) we obtain
Px=-*+*[~(2 8Jxx -{-divV)J+*[~l( &::11 + a~x)J +*[~ (a~z + a:z%)]= -*+~liV. +t-~ div V + :~
(2 aJ.x --}diV v)
where
li
+*
(a:ux + 8:: ) +~ (a:sx +8;;)
is the Laplacian operator: li iP/ax'J. + a'J./ay1.
+ 82/az"
Particularly, liV.~
-eo
a2VxiaX~
+ iPVx /{Jy2 + a2v.",'oz'J.
In a similar way, we ran lind the expressions for P II and Pz' The relations for the stresses due to the surface forces in a fluid have been obtained here by generalizing the laws relating stressesand strains in solids for a fhlid having the property of elasticity and viscosity. We shall obtain the same relations proceeding from a number of hypothetic notions on the molecular forces acting in • fluid (see [9, 1\1). By compiling projections or the total accelef; apply the Lap/adall operator to the vector V, and use the expression
,
.6,V= ~ l!Vnin=graddivV-cllrlcllriV ,,=1
(3.1.33)
where dF n arc the projeetions of Ihe vector along the coordinatelines qn'
Pt. I. Theory. Aerodynam!c$ of lin Airfoil and a Wing
116
The first vector on the right-hand side of (3.1.33) has been determined in the form of (3.1.25), while for calculating the second one Eq. (3.1.28) should be used. Taking the curl of both sidos of this equation. we obtain
, ,
curl curl V = ~ (curl curl V)"i n
._1
=~ "~hJ{ Lapiaciull opel'alor in spherical coo['dinalc-s is 11
-~ ~ . .;.;. (r~
-:r) + r~
$:11 t:I •
-to (sin 0 -k) . r! ,'1111" o· ~ (a.1.4,'f)
For lwo-dimellsiollal l-lpatial gas nO\\'5 charal"terizNI uy a change in the parameters (\'elodty, pressUI'e, density. e\c.) in the riirection of only two {~oordilJale lines, let liS write the eqllation of motioll - a simpler form:
aV r
.
dt~~-
+v
--.;..~ _
~-
au .
21'; _ 21'ge~)tO) r • r
-I-...!..... &div V
~-i ~.~+ VrVO ... .~ ~-.-V at r ar r ali r -
+v
1
' \'(1 in', \"~ l"p ra, r-;:-'&o--,=-p'o,
V ar r
(CiV r _
_..!....21I
3
br
rp
(CiVo -:--'}. a~j -r2~~20) +*.bd~;\"
bO
J
(3_t.45)
HIO
Pt. I, Theory. Aerodynamics of an Airfoil and a Wing
where
Il=-J,.f, (r2
-!r) +
r<si1nll
.-:0 (sin e ~)
diVV"""~. U{~;r2) i ~.a(\'9a~inO)
(3.1.46) (3.1.47)
Equations of Two·Dlmenslonal Flow
of a Gas Hellr II Curved Surface
For the Case I eing ton..,idereu, the curvilinear coordinates. Lame coefficients, 311d Yelo('ily ("omponents are determined by formulas (2.4.40), (2.4.12), and (2.4.43), respeC'th·ely. We shall adopt the further condition that motion occurs near II. wall. and. consequently. y« R. Accordingly, q1 = X, 12 = y, q3 = y. hI = 1, h, = 1. h$ = r VI = dx/dt = V=, V, = V r, V, = 0 With a view to these data, the acceleration component is
W,
OV,lal
+ V, OV';O$ + V, aV,;ay
and the projection of the preSfmre gradient is (grad ph = fJplfJx
(3.1.48) (3.1.49)
In addition, (grad div Vh
=
(3.1.50)
iJ div V/iJx
where the divergence of the velocity has been determined by relation (2.4.44). Consequently, (graddiVV)I=-1;{+[O(:x"r),.
O(;r
l ]}
(3.1.51)
We use (3.1.28) to calculate the projections 01 the velocity curl vector: (3.1.52) (curl V), = fJV/fJx - iJV,,/fJy, (curl Vh = 0 Introducing these expressions into (3.1.34), we obtain
(curl curl V),=+.fu-[r (~_
U;y=)]
(3.1.53)
With a view to relations (3.1.51) and (3.1.53lt we have (.6.V), = (grad divV)I- (curl curl V),
=fz{+ [u(::r) (3.1.54)
Ch. 3. Fundamentals of Fluid Dynamics
Similarly, when considering the coordinate line
Q2,
+ v x aVylax + l'y av /ay = aplay
W z = aV,,,at
(3.1.55) (3.1.56) (:·U.57)
(grad ph (~Vh
(grad div Vh --: a div v/ay = (grad eli\' Vh - (nl1'l curl
12t
we have
vh
(::r) ]}-+.:z [r (a:: _":;T) J(3.1.58)
= -i;-{+ [8 Eq. (3.2.10), we cnn no longer take into account separately the release or absorption of heat because of chemical reactions. Introducing into (3.2.10) the expressions for the st.resses (3.1.5) and (3.1.16) and excluding the term taking into account the work done by the mass forces, after transformations we obt.ain an energy equation for a gas: p
1t (~-!. u)
= -
div (pV)_.. -} div (jlV div V)
+-f; (~~) +fu- (~
u:;) +-i; (~ u:!)
*
Ch. 3. Fund"mentals of Fluid Dyn"mics
2
-tx
f,!{VyCt7 Vzcy)I-i- 2
127
IfL (V."€l ;. V.f x)]
:- 2 "';;'I~ (V.~ey -; Vllc:rl/·;...div (Agraa T) +~ ijdiv(pDgradc/)+€
(3.2.11)'
Equation (3.2.11) sl10ws what causes the kinetic energy of a nuid to change. III addilion to conduction, {Jifrllsion, alld nuliatiotl. this energy changes at the expense of the work of comprC'ssion di,· (pV) and tho work of tho friction forces (the tcrJII~ of t.ho eqllation ("ontaining the dynamie viscosity pl. The di!'sipatioll of ell('I'gy i.'" 1ISSOciated with the losses of mechani(:l1I en('rgy ror on'('{'ollling the friction forces. j':nergy dissipation {'onsists in that the mcehanica\ energy in part tram;forms il'l'eYersihJy into heat. Accordingly. the friction forces arc ('alled dissipath·e. The terms on till' right-hand side of (3.2.11) ('ontaining 11 form the dissipative fUllction. For two-dimellsiollal plnllC' molioll of a \'i!'colls nuid. thC'· energy equation is p
~ (~-;. u) =
-div (pV)-i- div
(~lV div V)
+fx(~l~)~*(~W) 2 -if; (~lVllez) ._- 2
i; (fLV ",ell.1- div (Agrad T)
+ ~ i l div (pDgl'ad ci ) -: where grad T
V "'" V.ti (oT/B.d i
€
(0.2.12)1
+ V"/L di\' V '"'" iJV)iJx + (}r"ldy, + (oT/uy)j, grad C; -" (8c;:(h)i ~- (IJc;lay)j
Let us transform the energy eqllation (:~.2.12). To do this, we' multiply the first equation (3.1.20) hy V", the second olle hy V", and sum up the results. \Ve obtain
p
_ Vx~[~(2
-t- (~).~ - (V"~'.Vy*)
u:~~-+diVV)]'i-Vyi;[~(2 U~',_~ di\"V)]. -: 2
[l"o~ ~ (j.l€z) -I· VII
-;;. (Il€.) ]
We can show by simple tran.!'fol'mations thnt l'" up/ax VII iJp/ay = di" (pV) - P (Jiv V
+
(3.2.13)-
128
Pt. l. Theory. Aerodynemics 01 en Airfoil end eWing
where we find p div V by using the continuity equation p div V ~ -(pip) dpld" or p d'v V ~ P (dldt) (pip) -
dpldt
We transform the sum of the other two terms on the right-hand side of the equation to the form
V%.:x[~ (2 ;t--}diV v)] +V.. ';; [~
(2 ~ --} div V) J
~ -h (~~) +.:,- (~W)-2~[( '::)' +( '::
n
-{-diV (~V div V) ++~(divV)t For the last term in (3.2.13), we have the expression 2
[v" ;;'(fJo!,;z) l· V y ';;
(!-LBz)]
=2* (I-'V"e
l )
+~ (",V:t:ez) - 4",e~
Let us make the relevant substitution in (3.2.13) and subtract the obtained equation from (3.2.12). Having in view that i = = It + pIp, we obtain
p~=*+21-'{[(~r
+ea;y" r]-i- (divV)2+4e~}
-I- div ().grad T) + h i, div (pDgrad cI ) + e
(3.2.14)
In the absence of heat transfer by diffusion and radiation. we can write the energy equation in the form
p~
=%+21-'{[( 0;; r + ( 0;,;1 rJ --} (div V)Z+!ie~} +div{).gradT)
(3.2.15)
At low gas velocities. when the work of the friction forces is not great. we may disregard the dissipative terms. In addition. the work done by the pressure forces is also insignificant (dp/dt 1::J ~ 0). In the given case, instead of (3.2.15), we have dTld'
(Alpc,) d'v (grad T)
(3.2.16)
The quantity A/(pC p ) = a, called the thermal dillusivity,characterizes the intensity of mol ocular heat transfer.
Ch. 3. Fundllmenlotls or Fluid Dynllmics
129
3.3. System 01 Equations of Gas Dynamics. Initial and Boundary Conditions
The investigation of the motion of a gas, Le. the determination of the para.meters characterizing this motion for each point of space, con~ists in soiYing the relevant eqnations that relate these parameters to one another. All these equations are independent and form a system of equations of gas dynamies. We determine the number of independent equations by the number of unknown parameters of the gas being sought. Let us consider the motion of an ideal compressible gas. If the velocities of the Row are not high. we may ignore the change in the specific.' heats with the temperature and take 110 account of radiation. In this case. the gas How is a thermodynamically isolated system and is adiabatic. The unknown quantities for the now being considered arc the three "elocity component$ l'x, VII' and V z• and also the pressure p, dl>Jlsitr p, nnd temperilture T. Consequently. the system of equations of gas dynamics must include six independent- onc.'i. Among them arc the eqllation~ of motion, continllity. slate, IIlld ell(>rgr. which art' ('USlomllrily called the fundamental equations of gas dynamics, B(>fore compiling this s-y:-;(ern of equations, let us cOIl~idel' separately the energy eq1lation. III ac('onlnncc willi ollr m':-;umption on the nrliabatif: nature of (he Ilo\\", we \I'Hn:-;fol'lll til(' ('1I('rgy equation (:1.:!,14) tI!! follows: di
= dp/p
(3.3.1)
If we take into cOII$lideralioli the cquatiorl di -, c/• dT, aud also the ('xpressions el' - C p ..." Rand p -'" RpT. from which we can nnd
then (3.3.1) is reduced to the form dp/p = k drIp. Hence (3.3.2)
where A is a constant characteristic of the given conditions 01 gas flow. Equation (3.3.2), is known as the equation of an ndiabat (isentrope). Hence. in the case being considered, the energy equation coin('ides with that of an adiabat. Having the energy equatioll in t.his
130
Pt, I. Theory. Aerodynamics 01 an Airfoil and" Wing
form, we shall write all the equations of the system: 1
dV:\, _
8p
-p'Tz'
---cit-
dV lI ~=
1
ay
-p'Tu
~~:=-+,~, -*+pdivV=O p=RpT.
(3.3.3)
Aph-I=RT
Let 11S ('.onsider the system of equations for the more general case of the motion of an inviscid gas at high speeds when the specific heats change with the temperature, and dissoC'-iation and ionization may orcur in the gas. For generality, we shall retain the possibility of the heated gas radiating energy. ~ow the thermodynamic process in the gas flow will not be adiabatic. Accordingly, the quantity £ determining the radiation heat flllx remains on the right-hand side of energy equation (3.2.14). We shan note that the equation of state must be adopted in the form of (1.5.8) taking into ft(',count the change in the mean molar mass Ilm with the temperature and pressure. In accordance with the above. and also taking into ar,r.ount that the equations of motion and continuit.y do not change in form. we shall give the fundamental equations of the system: dV."\"
_
I
8p
8V"
1
8p,
(ii"'=--p'&%' d't-:'-p'Ty
d!'t%
:;;~
-+'*: ~+pdiVV=O
p=!;-pT,
f (3.3.4)
p-¥:-=*+e
We can see that in the given system in addition to the six unknown quantities indicated above (V", V y • V z • p, p, and T) three more have appeared: the enthalpy i, mean molar mass of the gas 11ru. and the heat flux e: produced by radiation. Besides these quantities. when studying the flow of a gas, we must also determine the entropy S and the speed of sound a. Hence. the total number of unknown parameters characterizing a gas flow and being additional1y sought is five. Therefore. we must add this number of independent relations for the additional unknowns to the system of hlndamental equations. These expressions can be written in the form of general relations determining the unknown quantities as functions of t.he pressure and temperature: i ~ /, (p, T) (3.:1.5) (3.3.6) S = t. (p, T) (3.3.7) ~m = t. (p, T) (3.3.8) • =t.(P, T) (3.3.9) • = t. (p, T)
Ch. 3. Fund~ment~l$ of Fluid Dynllmics
131
The linding of these functions is tlte subject of special branches of physics and thermodynamics. The solution of Eqs. (:1.3.1)-(3.3.0) determines the parameters of flow of an inviscid dissociating and ionizing gas with account taken of the radiation effect. Snch flow is studied by the uerodynamics of a radiating gas. Let us consider a more general clIse of flow chara(·tcrized hy the action of friction forces and heat transfer. \Ve shall assume that chemical reactions occur ill the gas. Therefore. Llw fllndamental equations of th(' sYiitcm (for simplirlcation we shall ("onsider twodimensional plane flow) will include two differential equations (3.1.20) of motiou of a yisrous compressible fluid \vith a varying dynamir viscosity (Il =t= cOllsI), and also l'ontinuity e(Iuation (2.4.1). These equations mUl'it be l'iupplcmented \vail equation of slate (1.5.8) relating to the general cuse of a dis~ociated and ionized gas, and with expression (3.2.11) that iii the ('nergy equation for a two-dimensional compressible gas rlow in which heat transfer by diffusion anc1 radiation occur. These equations describe the gelleral case of unsteady motioll and characterize the unsteady thermal processes orcufring ill a ga~ now. !fence, we have
~== _+.~++'~['I (2
iI;;. --}diV v)J
++~(Ile:)
~
=
-+.* r+'+v [~(2 a{~;1 ._+ div v)] +4·*(~eJ
(3.3.10)
47-, pdivV=O; fJ%=~
-'-2M
{[(~r .L(~r]-+{clh'VP· 4e~}
+div ("-grad T)+ ~ i, div (pD~rad cJ) :.
t·
This system mllst be slIpplelllelltf'd with relations n.3.5)-(:·I.~Ul), and: also with tbe gener,]} relations for the thermal conductivit.y
).
~!. (p, T)
"
~
(3.3.11)
the dynamic viscosity
!,
(3.3.12)
(p, T)
.md the specific heats
c,.
= /,
(p, T),
C1'
'-'
/9
(p, T)
(3.3.13)
182
PI. I. Theory. Aerodynamics of an Airfoil and a Wing
The last t\\'o quantities are not contained explicitly in Eqs. (3.a.10). but they fire RCvertheless used in solving them because when studying the flow of a gas its th(>rmociynamic characteristics are determined. Since the energy equation also t.akes into account heat transfer by diffusion. equation (3.2.5) has to be included additionally. It must be taken into accollnt simultaneollsly that the COIlcentration Cj in the energy and diffusion equations is a function of the pressure and temperature, and it can be written in the form of the general relation
c,
~
/" (p, T)
(3.3.14)
The abo\'e system of equations including the fundamental equations of gas dynamics and the corresponding number (according to the number of unknowns being sought) of additional relations is considered in the aerodynamics of a viscous gas and allows one to fmd the dist-ribution of the normal and shear streiises, and also the aerouynamic heat nnXeii from the heated gas to the wall over which it Hows. In spedflc ("aRCS, for which a definite schematization of the now process is possible, the above system is simplifled, and this facilitates the solution of the differential equations. When soh'jng the equations, it becomes necessary to in\'olve additional relations used for determining the characteristic parameters of motion. Among them are. for example, relations for determining the ~pE"cinc heats and the degree of dissociation depending on the pressure and tcmpcrature, 0.11(1 formulas for calculating the shear stress depcnding on lhc \'clocity. The solution of a system of gaswdynamic equations describing the flow onr a given snrfarc mustsatis[y defInite initial ami boundary conditions of this now. The initial conditions al'e determined by Lhe values of the gas parametcl'!'! for a certain instant and ha\'e sense, evidently, for unsteady motion. The boundary conditions arc superposed on Lhe solution of the problem both for steady and [or unsteady motion and must be obsen'ed at eury ins/ant of this motion. According to one of them, the solution must be SUeil that the parameters determined by it equal the values of the parameters for the undisturbed Dow at the boundary separating the disturbed and undisturbed now regions. The second boundary c.onditioll is determined by the nature of gas flow oyer the rele\'sllt :"urfnce. If the gas is in viscid and does not penetrate through such II surface. the flow is said to be without separation (a fre{' streamliop. now). In accordance with this condition, the normal velocity component at eac·h point of the surface is zero, while the vect.or of the total velocity coincides with the direction of a tangent to the surface.
Ch. 3. Fundamel'ltals of Fluid DYl'Wllmics
133
It is general knowledge that-the "ector grad F [nerc F (qt. q'J' q3) = = 0 i,!l the equation of the sllrfaC'c in the 00\..... and qh q'J' q3 are the generalizcII C'urvilinear C'ool'(linat~l coincides in dircction with a normal to the snrlaC'e. lIen(,f-, ror conditions of Row without sep· aralion. the dot prodnel of 111i~ vcC'tor and the "clority vector V is zero. Conseqllcmtly. the condition of Row withont separation can be written in a mathematical form ,IS follows: VgradF ·0 Taking into account that gradF
""-&. :~ i
l • -/;;.
;~
i'J
~-*. :~
13
(3.3.15)
the ('ondition of Row without separation can be wl'iUcn as
-&' :~ VI+i· :~ V2~-*' :~ V =O 3
(3.3.16)
For Cartcsian coorninate."', we haye grad F , . (iJF.'iJ,r) i l + (;)F.'iJy) i'J -:- (iJpiiJz) i.1 COII!lt'qllcntly. r.r (3.3.16) i'.,. ilFliJx ~- 1'" OFhJy --:- 1": flF/i)z ,... ()
(:1.3.17)
For two-dimensional plane flow 1""
V;"". -
aF/iJ.r; aFlog
(3.3.17')
If the equation of lhc surface is gh'en in q;lindrical ('oordiIl8tes. we haye
gradF-:-~il+*j'J-:-
+.*i
3
thererm'f', the ('omlilion of flow wilholll scpal"ulioll has Illc rorm (3.3.18) In a particulllr case. whNI a :'lUl'face of rc\'olnt.ioli is ill the flow, we obtain the equation Fx OF/O:r -;... {)F/i)r - 0 (:3.:3.18')
'·r
froll1 whieh we find the condition for the vclo('itr ratio:
f.; - ~~~:;
(3.3. "19)
Other bOlilldal'Y cOlldilioll~ ('an also he rormulated. They are determined for each spccinc problem, the boundary conditions ror
1.34
Pt. I. Theory. Aerodynamics of an Airfoil and a Wing
a viscous gas differing from the cOlHlitions for an ideal fluid. ParliClllarIy, witli'll studying the flo,v of a viscolls gas in a boundary layer, the solutions of the pertinent equations must satisfy the conditions on the sllrface of the body and at the edge of the boundary layer. According Lo experimental data, the gas partides adhere, as it were, to the sllrface, and therefore the velocity on it is zero. At the boundary layer edge, the velocity be{'~omcs the sallie as in free (inviscid) flow, and the shear stress equals zero.
3.4. Integrals of Motion for an Ideal Fluid The differential equations deriver! for the general case of motion of a gas are non-integrable ,in the finite form. Integrals of these equations can be obtained only for Lhe particular case of an ideal (inviscid) gas flow. The equation of motion of an ideal gas ill the vector form is 8V/fJt + grad (V2/2) + cud V x V = -(tip) grad p (3.4.1) This equation can be obtained from vector relation (3.1.22') in which the terms on the right-hand side taking into acconnt the influence of the viscosity should he taken equal to zero. In its form (3.4.1), the equation of motion was first obtained by the Rmisian scientist prof. I. Gromeka. With a view to the mass forces, Gromeka's equation becomes 8V/8t -;- grad (V2/2) eurI V X V ~ G - (lIp) grad p (3.4.2)
+
Let us assume that the unsteady now will he potential, hence curl V = 0 and V = grad 'P. In addition. let us assume that the mass forces have the potential U, therefore the vector G = -grad U
+
where grad U = (8U/ax)1 (aU/uyH --1_ (uUliIz)k. If a fluid has the property of barotropy characterited by an unambiguous relation between the pressure and density (this occurs, for example, in an adiabatic flow, for which p -:-:: Ar"), then the ratio dp/p equals the differential of a certain function P and, therefore, (lIp) grad p = grad P \Vith a view to this equation, expression (3.4..2) becomes 8 (grad rp)18t grad (1'1/2) = -grad L: - grad P
+
Substituting the quantity grad (8(r/8t) for the deri"ali\"e ,ve obtain grad (8rpI8t) grad (V212) = -grad U - grad P (3.4.~)
u (grad amlincs (pathlines) find the vortex through whose points a slrenmline pfl~~(lS. One must deflrly understand Ihe distinction between the Grollleka and Bernoulli equations con~idcred abo\'(·. TIley nrc both derived for a vortex (non-potential) nO\\', howen~r the iiI'S!. of them reJ1p(,\.f'. the fact that the totfll energy of a IIllit llli1~S 01' the IS in the entire region where the \'orlex liHl'S and while the second equation ('."'tabl [ghes Ihe law this energy is constant along fI giH'n streamline lIr L·or/c.! ingly. in the Gromeka equation. tlw COll;.:talll, is thp ."amp entire flow region being consi(ll:'red. wllere'"c(., we lilld i ~ lk/(k - 1)1 pip (3.1,.15) Con~equently,
V'/2 V 2/2
+ [k/(k -
1)[ pip ~ C
+ kRT/(k -
1) --" C
(H.16) (3.4.16')
The Bernoulli equation for an ideal compressihle gas is the theoretical foundation for investigating the laws of isentropic flows of a gas. 3.5. Aerodynamic Similarity Concept 01 SlmUlrHy
The aerodynamic characteristics of craft or their individual elements can be determined twlh theoretically and experimentally. The theoretical approaches are hased on t.he llse of a system of equations of gas dyuamics that is solved as applied to a hody in a flow, the hody ha\Oing a given configuration and arhitrary absolute dimensious. \Vhen rUllning experiments intended for obtaining aerodynamic parameters that can he used directly for further ballistic calculations or for verifyiug the resnlts of theoretical investigations. it is not always possible to use a fnll-scale body because of its large size, and a smaller-size mod "I of the body has to be used. In tlds con-
Ch, 3, Fundamentals 01 Fluid Dynamics
139
Jl('ction, Ihe question appem's on Ihe poss.ihility of trans.fel'fing the l'xpl'rimental 1'('''-lIitS obtained 10 full-scllle ])o of aerodynamil's. Con..-iderLng the expression rOt' the ll(']'()(lyuamic coefiieiellt
(fx,,)1*
C'\·8= ) [iJeos(Il.T D )·;·(',."cos (3 ..'5.2) <s, Qhtnined from (1.3.2), we can !':'CE.' Ihat this coefficienl depends on dim('n~ionless gcomet!'ir parllnlell'I's. and also on (limensionless qlllllltities sudL as th(' pl'eSSlll'(' rQPllidont 11IIt! Jocal fricLion facioI'. Hellc(' it follows Ihat thc aerO(IYllllmic co('ffirienl..- fol' a fuJl-sclIle ohjed [lIHI an eXpl'fillll'lltal onl' with diffNent ahsolute dimell!: with 11 gi\'en configuration
p
140
PI. I. Theory. Aerodynllmics of an Airfoil and a Wing
of the body in the flow known \"alues of the angle of attack lind the sideslip ,mgle. as of the rudder and elevator angles, will be functiolls of the stream velocity l' the pressure poc, the density p "', lIH: dynamic yj~co!>ity .~oe. the specilic heats c" "" and C,,(IO of the gas, as \I'cll as of a certain characteristic (reference) linrar dimension of thf' hody L ConsequenLly. the drag coefficient will also depend all tltese parameters, and we can compile a functional relation for it in the form ex:...: t (V"',, p"", p"" fl=, c)lx" C,._. L). Since this coefficient is a dimensionless quantity, it mnsl also be a function of dimensionless parameters. From the general considerations or the dimensional method. it follows thnt the seven different argnments of the funclion C x call be reduced to three. The latter are dimensionless combhHltiolls compiled from V.", p"", poo, fix-, cl'''''' c,_ ,." and L because there arc fOllr independent units of measnrement, namely, mass, lcngth, time, ancl temperaturE'. These dimensionless combinations h,,\'E' the following form: II "" Vk~pnsionie:o;s comLinntion~ forming what is called a bns(>, i.e. a system of dimellsionless ql1antilies determining all the other parametPfs of a flow The~e (lirnensionless combinations are ("died Similarity eritNia. (10,
Ch, 3, FUfldamentab 01 Fluid Dynamics
141
The ~imilaritr critt'ria gi\'t~n above have a delillite phrsical meaning, In accordance with the e:o.:pression a:! = dp/dp, the speed of sound can be considered as a criteriou tlcpeuding 011 the property of compressibility, i.e. on the ability of a gas to change its densit}' with a change ill the pressure. Consequently, the Mach number is the similarity criterion that is used to characterize the influence oj compressibility 011 the flow of a gas, The Heynolds number is a parameter used to appraise the influence of ~'I$C'osily Oil a gas ill motion, while Lhe parameter k _ = cp ""fc r "" determines the features of a flow due to the thermodynamic properties of Q gas. Similarity (rU.ria Taking Account of
the VIKGsU, and Heat Conduction
In the more genernl conditions of flow characterized by the influence of a number of other physical and thermodynamic parametel's on the aerodYllamic properties of craft, the drnamic similm'ily criteriA are more complicated and diverse. To establish these criteria, we can usc a different approach of the dimensional analysis and similarity method based on lh(> use of the eqUAtion of motion of a "bcons Iwnl-conducting ga~, Lel us wrile these (!qtUltioll~ in the dimclI:-:iolli(>ss form, i.e, in a form such that the paramett'fs (vciociLr, presslIre, temperature. etc,) in the equations arc rclal('d to I'd('rt'llco panUl1l'lt'I'S. The illtter arc constants for f\ gh'en flo\\' alHl dl'lt'rmillt' iLs scal(>. \\'e shall take as references the paramnlers of lhl' (1'(>(' stream: it,;; Yeioci~y r ... , pressure p_, dCllsitr p_. lempf.'l'al1ll'C T...,. f[YIlss equations [provided that Eqs. (3.5.13)-(;~.3.Hi) determine il'm, [, ~, and Cp as a function of 11 depend on the dimensionless cool'dinates anu the time. and also on the similarity criteria (3.5.17)-(3.5.10). Particu· Jarly, the dimensionless pressure can he represent~d a~ the (ulldion pip. = CJll (F,., Re, M, Sk, p,., k.,
Tw ,
XI
y, Z, t)
(:~.5.21)
We can \l.SC the known pressure distrihuLion to dctC'l'lIIine the dimensionless drag force coerrident for a gh'ell inslanl: c:C" = X./(q_S) = S2' ant} S3 have been chOSl'n as these slIrfflceg. Taking logarithms, wc obtain In p In V :- In S = = const. Differentiation of this l'xprl'ssion yields
,I
+
dpip
-;~
dvrV -;- dSIS
= 0
whence
(J.G.I) Le~
us use relation (3..1.11), by dilTcrentiation of which we have
IT. dV = -di
(3.6.:.!)
Substituting dp r for di. we fmd VdV ,-' -dp/p
(3.6.3)
Taking the speed of sount! fl :-..= V dpldp into accollut 1IIul llsing r~lalioll (3.0.3). we transform (;{.6.1) to the form dS;dV \\'hel'(' M
'-~
~
(Sir) (M' -
1)
(3.0..1)
V,'a is the }Iach Ilumber in the given cross section of
the jet. LeL lIS IlSS11lnC! (hot l.hl' vclocity along the jet grows (dV> 0), 1mt, remains subsonic and. CO[]~l·q1Lent.ly, M < 1. A glance at (:':1.0.4) rcyeals that for Illis caSt' the derivative dS/dV < O. This indicntes that the jet couverges downstream. COIl\'('rsciy, for a subsonic
1~O
Pt. I. Theory. Aarodynolllmics of an Airfoil and
0lil
Wing
V.p.~
p.r.d
v,;
''Fig. U.t
Parameters of
d
p~
to
Po '.
gas flowing over a body
Dow with a diminishing velocit.y (M < 1. dY < 0). the cross section increases. which is indicated br the inequality dS > 0 following from (3.6.4). Let us consider a supersonic Row (M> 1). If the velocity decreases, then. as can be seen from (3.6.4). the differential dS < 0, and. consequently. the jet converges. Conversely, when the velocity grows. the value of dS > O. Le. the jet diverges. Let us take a nozzle that first has the shape of a converging. and then of a diverging channel. In defmite conditions in the converging part of the nozzle. a subsonic now is accelerated, reaching the speed of sound in the narrowest cross section [here dS """ 0 and, as follows from (3.6.4), M = 1J, and then becomes supersonic. This is how nozzles are designed in rocket engines, gas turbines, and wind tunnels intended for obtaining supersonic flows. Flow V.locHy
Let us consider a gas jet Rowing oyer a surface (Fig. 3.6.1). We shall denote the free-stream parameters by Y .... P 00. P 00, T ,." L.,. and a .... and the parameters for the part of the jet in the disturbed region by the same symbols without subscripts. To lind the \'elocity in an arbitrary cross section of the jet. we shall lise Eq. (3.4.14) in which we shall determine the constant C according to the preset parameters of the frce stream: C = Y!.12 1~ (3.6.5)
+
Wit.h this in view. we have yIl2 i = V!./2 .:. too whence
+
V-VV:.-,.2(1~
I)
(3.6.G)
At the stagnation point. V:....: 0, consequently the enthalpy is t = io = V!..:·2 -:- i... (3.0.7)
Ch. 1. fynd~m.,nt.ls of Fluid Dyn~mics
151
Hence. t.he constant C as regards its physical meaning lcan be considE!red as the stagnation enthalpy. With a "iew to this valne of C. the "elocit r in t he jet is V~V2(i,-i)
(3.6.8)
The stagnation pressure Po and density Po correspond to the enthalpy i o• They are determined from the condition i o"'""
k:1'~'=- ~~~~. i ..
=.x;.+ k~l
.
~:
(3.6.9)
We can rewrite Eq. (3.6.9) as follows:
';:+ k~1 ·f:·
k~l .~
Sillce the flow is isentropic, we have pip' .~ p,lp\
(3.6.10) (3.6. \I)
consequently (3.6.12) Seeing that for conditions of stagnation the speed of sound is ao = VkPo/po. we fmd (3.6.13) Examination of (3.6.8) reveals that the velocitylalong the jet grows with diminishing of the enthalpy, and therefore more and morc or the heat is convcrted into kinetic energy. The maximum velocity is reached pro\'ided that the entbalpy i = 0, i.e. all the heat is spent to accelerate the gas. The \'alue of this velocitr is Vmu:= V2i;,
(3.6.14J
or with a view to (3.6.9):
VIPU=Vk~1·~=ao l/k~l
(3.6.15)
Accordingly, the velocity in an arbitrary section is V~Vm .. VI-iii,
(3.6.16)
V=Vmu. 'Vi_(pIPo)(II.-t)ill.
(3.6.17)
or In the narro'.... est. critical, cross section of the jet, the ,·elocity equals the local speed of sound. The latter is caUed critical nnd is
162
Pt. I. Theory. Aerodynillmics of ilIn Airfoil lind II Wing
designated by a*. The critical pressure p* and density p* correspond to the critical speed. It follows from the Bernoulli equation that for the critical section we have a· 2 , k
p.
-y -.- k=T' p* =
Po
k
-r=T 'P;-
Having in view that kp*/p* = a*z, the critical speed is a*=
V k~1 '*=00l / k!l
(3.6.18)
or, taking into account (3.6.15),
a* ~ Vron Y"(k:---C1")!"'(k"~c"1)
(3.6.19)
To determine the local ~ound speed a, we shall use Eq. (3.6.10). Performing thc substitutions a2 = kp/p and ~ = kpo/Po in it, we obtain (3.6.20) or a'1=
k-;i
a*'1_
k"2l
V2
(3.6.21) (3.6.22)
a2= k-;l (vfullJ.- V2)
Let us introduce the velocity ratio (relatiw ,'elocity) '}. = Via"'. Dividing Eq. (3.6.21) by VZ and having ill view that the ratio Via = = M, we can establish the relation between'}. and M: 1.' ~ I(k
+ 1)/2IM'/{1 + I(k -
1)/2IM')
(3.6.23)
Hence it follows that in the cross section of the jet where Vmu is reached, the number M = 00. We find the corresponding value of '}. = Amal< from (3.6.23) pro·vided that i.V -+ 00: 1.ruu~ Y(k '1)/(k
1)
(3.6.24)
Evidently, in the critical section where M = 1, we rature 1'*: P* = Po ( k~t )"/{h_l) P*=Po
(k!t
= Port (1)
(3.636)
)t/(Il-t)=P08(l)
(3.6.37)
T·~T.( k~1
)=T.T(I)
(3.6.38)
where n (1). e (1), and 1" (1) are the yalues of the gas-dynamic functions at M = 1. The above formulas, suitable for ally speeds, can give us approximate relations for cases when the numbers M arc very large. A glance at (3.6.30) reveals that when M>- 1 a.nd M - 1. we have (3.6.39) Similar relations for the density and temperature have the form plp_ = (M .IM),,,h-.) (3.6.40) TiT _ - (M .IM)' (3.6.41) Using relation (3.6.27) for the velocity of the free-stream flo ...... ,
(3.6.27') for the conditions Moo >- t and M >- 1, we obtain the following .approximate formula for the local velocity:
(3.6.42) Flow of • O.s from • Reservoir
Formula (3.6.12) allows us to determine the velocity of a gas .flowing out through a noule from a reservoir (Fig. 3.6.2) in which the parameters arc determined by the conditions of st.agnation corresponding to a velocity of the gas in the reservoir of V ~ O. Such conditions are ensured in practice if the critical cross section of the nozzle is suffiCiently small in comparison with the cross:iectional dimension of the reservoir. In the critical section of the nozzle, which the value of the derivative dS!d~' = 0 corresponds
Ch. 3. Fund.ment.1s of Fluid DyMmic'
Fig. 3.6.1
Paramett'fs of
It
1I!1f~
gas nowiog from a res('n·oir
to, the Ma ch H1Imber, as can be seen from (a.!i.4), equals unity. i.e. Lit£' \'elocity in this section equals the local speed of sound:
V=a*=
V
k::J·
~:
"-'no
l/·I"-~ 1 ··'l /" 2:~~o
Such n speed is ensllred providc(1 t hat the pressure in t he reservoi r accordiug to (~.(l.3G) is not lower than thc vaillc
Po .• p*(¥)I,(I'-I)
(3.6.103)
If the nozzle communicatt>s with the utmospheric air whose prelSSure is p,. ,-: 1O~ Pa (this pressu.·e is call1'd the backpressure), now through the uonlc is possible whcll p* ;;;;:, 1O~ 1',1. Assuming that p* =- 10:' Pa and k = 1.1, we obtain the pre5sIIre needed to ensure the sp('('d of sound at the ant let of a eO[l\-erging nozzle:
1'0 = 10"( 1.4;-1 )1 ."(t.'-t)~".fI :-: J(lS Pa When the critical partuncters are re-uelle-d in the throat of a nozzle, a further reduction of thl' bnckpressure (pa < p*) no longer nfleets the \·;IIIIt'S of a* und 1'*, whi el. Ilepclld on the stAte of the gas in the reservoir. But Ill're conciitiolls (\fl' crl:'ated fot' the nppearance of a s uprrsonic specil of th e gAS in the diYergillg port of the TlO1.zil'. In Fig. ;Uj.2 . tllt'se c()J\d iHo[1~ of iscutropic motion are charaet('rhed br l' IIt'VPS 1 d(·termilling thr cilaugc ill tlt~ ralio " lpo and in the lIumber M
p(~l at ,,,hlCh the pressure p~~' at the exit reaches the same value as pi:). The subsonic flo,,, formed in thill case is characterized by curves 2 shown in Fig. 3.6.2. We find the veloci\.y ratio').. (M) of this flow by Eq. (3.6.23), choosing from the two solutions for').. the one that is less than unity. Upon a further increase ill the ll1lckpressure to the value pl~), conditions appear in which the pressllre p(~) at the exit will equal the backpressure, i.e. p(:) = p(~>, while the pre~sure in tl1('. throat will exceed the critical pressure p*; the rel~'vant speed in this croSs section is subsonic (1" < a*). Consequently, in the diverging part of the nozzle, the speed lowers, remaining suhsonic (curve 3 in Fig. 3.G,2). At pressHrf's at the ('xil smaller tILall p(~) and larger then p(~l, the isentropic uature of the flow is disturbed. At a certllin cross section of the !lolzle. a jump (di~contill\lily of the parmncters) occurs, the trnm;ition thl'ougl, which is attended by sharp deceleration of the flow. As a result of Ihis ciece\(»'atioll, having an irreLwsible adiabatic /lature, the supersonic. flow trallsjorms abruptly into a subsonic one. Till' change in the prcssure and in the number .}1 along the nozzle in these flow cOlulilions is characterized by curves 4 (Fig, 3,G.2). The surface of discontinuity of the parameters (shock) must be in a cross section with a 1Iach number M sucl) tltllt would correspond to the pressurc ps past this surface ensuring a gas pressnre of p~l' (p(Jl < plJ> < ps propagate ill a gal" at re!'lL in all (jir(>ctions at tlJC I"peC'd of sonnd a ill Ihe form of sphl'ricaJ waws in space or circnlM waves ill fI plane (Fig. 4.1.20). AI the instant I. thr. rndbls of a wave is r = (It. If fl. suhsonic glls fiow is
=
n-;--
160
PI. I. Theory. Aerodynamics of ~n Airfoil and a Wing
fig..U.t
,shocks; a-attaCMd curved shock;
b-d~!aclled
cur~d
sboC'k: e-attacMd straight .hock
(6)
(aJ
'fi,.4.t.l
Propaga tion of disturbance. in a gaB: a.-g.s at rest;
b-!lub~onll!
OOWI e-supt'rsonlc flow
incident on a source (V < a, Fig. 4.1.2b), the waves are carried downstream: the centre of a wavc travels at a speed of V < a. while tile wave propagates at the speed of sound. During a certain time t, the centre of tile ",,,ve tra\'els tile distance Vt, wlLilc the radius of the wave r = at, here at > Vt. Hellce, in a subsonic !low, disturbances also propagate up!;tream. In the particular case of a sOllic velocity (V = al, the front of spherical or circular disturbance waves is limited by a flAt vertical surFace or straight line tangent to a sphere or circle, respectively, and passing through point 0 because in this case the distance over which the centre of the wave travels dnring the time t equals its radiu!; at the same instant t. Let 11S assume that the free-stream velocity is supersonic (V> a). During' the time t. the centre of the wave travels the distance Vt, while a sound wave covers the distance at. Since at < Vt, [or all the spherical sound waves we can draw an enveloping conical snr[ace (Fig. 4.t.2c), Le. a disturbance cone (or !tfach con~). On a plane, disturbance lines (or Mach lint's) are envelopes of the family of circular waves. Tho di!'t\lrhancc~ arc the densest on the disturbance
Ch. 4. Shock Wave Theory
161
Fitl· U •1
OriglnatioD of a shock
cone or lines that are boundaries of a disturbed ann uodisturbed region because all the sound waves on this cone are in the same phase of oscillation-the compression phase. Such disturbed regionsr.onica. or plane waves confined within straight Mach lines, are called simple pressure waves or Maeb waves. The angle Il formed by the generatrix of a conical wave or line of disturbances i~ determined from the cond ition (Fig. 4.1.2c) that sin Il = at/(Vt), whence sin J.1
=
1/lW
(1,.1 .1)
The angle J.1 is called the Mach angle. A ~mpersonic flow carries all the sound disturbances downstream, limiting their propagation by the Mach cone or lines inclined at the angle ~L The front of a pres~ ure wave propagates at the same speed of ~o\lnd as Lhe front of a spherical (or circular) wave. This is why the projection of the freestream velocity onto a normal to the WII.\'C' front equals the speed of sound (Fig. 4.1.2c). In a simple pres~ure wave, a~ in a soun(1 one, the gas parameters (pressure, density, etc.) change by an infinitely small magnitude, which is indicated, particularly, by the relaLioli for the speed of sound a = 11 dp/dp known from physic~ . In the disturbed region. the velocity remains virtually the same a~ in the undislurbed flow. Therefore, a simple pressure wa ve can be con ~ idered as a shock (or shock wave) of all infinitely small strength, and we can assume for practkal purposes that the paramelers do not change when traversing it. This is why such a simple pressure wa.ve is al so called a weak sboek wave, while its front (Mach line) is called a. line of weak disturbances or a wavelet. It is natural to assume that the formation of a shock of a finite strength is associated with the superposition of simple pressure waves and, as a result, with their mutual amplification. Let us consider the process of formation of such a shock taking an oblique shock as an example. Let us assume that a supersonic flow initially travels along a level and smooth surface (Fig'. 4.1.3). We create artiflcially a 10rnl pressure increment at point A hy turning the flow through the inrlllitely small angle d~. This prodll r e~ a simple pres.q-
162
Pt. I. Theory. Aerodynamics of an Airfoil and a Wing
ure wa"e AR emerging from point A as from the source of clisturbam'c and inclined to the surface at the angle }1. If we again tUrn th(' flow slightly through the angle 6~, a new simple wav" AC is fOI'llH'd that emerges from the same point A. but iii higher tllfln the Jirst wave, But in II. supersonic flow, as shown above, waves ('an not propagate upstream. therefore the wave AC will drift downslream until it coincides with the first one, A more intensive wave is formed that if; considerably amplifled upon a furt.her turning of the flow. The shock of a finit.e strength formed in this way hali a speed of propagation higher than the speed of sound at whkh the simple prelisure wave travels. Therefore, the lihock of fmite strength nllliit deviate from the liimple wave AD to the }t'ft and occupy the new pOliition AD. Here it is kept in equilibrinm because the speed of its propagation equals the component of the free-stream "elocity along a normal to the shock front V sin a" where as is the angle of inclination of tht' shoc_k. It follows that the angle of inclination of a f;hock of finite strength is larger than that of the Mach line (cone), Le. 9s »!.
".1.
Genera. Equations
'or. Shock
We shall consider the more general rase when the ga.~ behind a shock, owing to substantial heating, experienr.es physicochemical transformations and changes its specific heat. Of major signific,anco whell f;tudying shockli behind which oscillations are generated and dissociation, ionization, and chemical reactions occur are the rates of the physicochemical transformations. Proref;ses hehind shock waves arc characterized by a fraction of the kinetic. energy of the moving gas virtually instantaneously transforming into the internal energy of the gas. In these conditions, we cannot ignore the fact that thermodynamic equilibrium is achieved after a certain time elapses only in conditions of such equilibrium do all the parameters experiencing discontinuities (the pressure, density, temperature) become time-independent. The analysis of these phenomena is a more involved problem and is associated primarily with studying of the mechanism of non-equilibrium processes, and with a knowledge, particularly, of the rates of c,hemical rear"tions in the air, The simplelit case is characterit.ed by an infinitely high rate of the physicochemical transformations and, consequently, by the inst.antaneous setting in of thermodynamic equilibrium. Such processes behind shock waves are pOlisible physically, which is confirmed by experimental studies. Let llS ronsider the basic theoretical relations allowing one to evaluate the equilibrium parameters behind a shock wave.
Ch.... Shock Wive Theory
169
Obll... Shock
A J;hock formed ill real conditions is charact('rized by a certain The parameters of t.he gas in sllch 1I ~hock change not inshntflllconsly. but during a certain time intel'\'ul. As .c:hown by theoretical alld C!xperimentlll in\'estigations, howe\'er, the thickness of a shock is \'ery small and i.e: of the order of the mean free path of the lllolerulct:. Fot· IItlllosphel'i(' condilions, calculations yielded the following vallle:-: of the thickness of a shock measured in the direction of the frce-l:::tl'enm .... t'locity: thid,:ues~.
:\Iach nnmb('r Moo . . . , ' . Thicklll's!!. nun
t.5 . . . . . , . 4.5xtO-·
1.2xH\'"~
to' l).7xto-' 1I.2xt()-&
For M oc- = 2. t.he thickness of a shock equals about four molecular free pnth:-:, and for M co .... 3-about three. Therefore, when studying a shocl< in an ideal fluid, this thickness may be disregarded and the shock represented in the form of a geometric discontinuity surface for the gnJ; paramcters. assuming these parameters to change inst.ant:meously. 0111' t.ask con~~ts in determining the unknown parameters of a gas hehind II shock aecording to the preset parameters c,harartflrizing 1he now of Ihe gas ahead of the ,c:hock. For lin oblique shock formed in a dis~ocitlting and ionizing gas, there tire nine lInknown parameters: the pres~ure Pz, density Pz. tempt"l'fl.lnr£' T:?" nlocity V'l , enthalpy f z. ('ntrop~' S2' .c:peed of .e:oulHl 1I2' the mean molar mas..'!ses, the former is attenderl by greater heating of the gas, and this is just. what facilitates a certain drop in the density.
174
PI. 1. Theory. Aerodynemics of en Airfoil and eWing
Formula (4.:i.16) determines the raLio of t.he squares of the sound speed in accordance with t.he relation a!la~ = TzlT l (4.3.17) Using tllis relaLion, and also Eq. (4.2.18'), we can determine the number M2 behind a shock. Inserting expression (4.2.21) for LlVn into (/1.2.18'), we find V:/V~ = cos 2 as + (P l/p2)Z sin z 6s (4.3.18) Dividing Eq. (4.3.18) by (4.3.17), we obtain an expression for the ratio of the squares of the Mach numbers: M!/~ = (TIIT z ) [cosZas + (P l/p2)2 sin 2 as] (4.3.19) where TIlT'). and Pl/pz are found from formulas (4.3.113) and (4.3.13), respectively. The formula for calculating M 2 can be obtained in a sOme\Vllat different form with the aid of momentum equation (4.2.4"). Let liS writo it in the form
*
("1 + ~ VisinZas) =
1+
1;- V;sin2 (as-i-f}s)
Taking into account that kplp = [(1 + 6)/(1 - 6)] pIp, and determining P21Pl by the Hugoniot equation (4.3.13'), we obtain
1-;;2~~~~~J)
(1 -I- :~~ M; SioZ6s) = 1+ !~~ Misin2(9s-f}~)
After sub5tituting for we obtain the relation
M~
sin'). 6s its value found from (4.3.13), (4.3.19')
Let us determine the stagnation pressure for the conditions of a flow behind a shock. Considering the Dow of a gas behind a shock and ahead of it to he isentropic, we can compile the thermodynamic relations: p2/p~ = p~/p'~,
Pl/p~ = Po/p~
where Po and p;, Po and p~ are the stagnation pressure and density in the regions of the flow ahead of the shock and behind it, respectively. These relations yield the pressure recovery ratio across a shock wave: "0 = p~/po = (PiPl) (Pl/pz)" (p~/p()" Multiplying both sides of this equation by the ratio obtain
(Polp~)I>..
we
Ch, 4. Shock Wave Theory
17~
Let us use the energy equation y2/2'7 cpT = const and write it for the conditions ahead of and behind a shock: V:i~ + cpT, = V:12 + c"T 2 At pOints of stagnation, V, = V 2 = O. 1L follo\\'s from the energy equation that the temperatures at these points are identical, i.e. Tn = T~ or, which is the same, Po/Po = p~.(l~. Consequently. 14.:UO) (4.3.20')
w11ere P1ip2 and P2/Pl arc found by (4.3.15) and (4.3.13), respectively. By (3.6.28), the stagnation pressure is (4.:3.21)
*
Consequently, 1(1 -:. 6) Mi sin 2 9~_6J(6-1)/20 (.U, sin 9~)(J.r6)"o'
'(1_6)-(IT6)/26
.
d by an increase in the strength of a shock, a greatt>l' density behind it. and, as a result, hr the shock coming close (0 the> surface of the bOlly, which leads to dellection of the flow through a larger angle. At u still larger no,~e ungil:', t.he now ul'hind Illl attached shock becomes unstahle, as a resllit or which the shock 1II0Y('S away from the nose, Behind such it (ldnched shock, n new ~lIthle flow region appears. It is chul'aclcrizcli hr tieflt'clioll thl"Ough 1111 illig-Ie also less than the critical one. Bill unlikell suhcriti('ai now, 1I1i~ one i!l- called sup P~ and, .:onscquently, 8 2 - 8 1 > O. This conchlsioll cortl>sponds to the second law of thermodynami('~. ac('ording Lo which the cntrop)" of an i~olated sy!'!tem with ('omprl'ssion shocks increases. Let U!l !lOW considl'r the reverse l'ituatioll \\hetl n gus passes from fI statr characterized by Ihe slagnation pressure p~ (the parampll!rS wilh the subscript 2) into a stat.e with the stagnation pressure Po (the pnrameters with Ihl! subscript 1) through all expansion shock. In this case, by flnalogy wilh (4.·i.,;;), the challbJ{' in lIle entropy is SI -
S1.
. R III
(p~/po)
Benel'. whell the coudition p~ < Po is retailled. the entrop), should diminish. but this contradicts the second law of thermodynamics. It thus foJlows Ihat expansion 8hocks cannol appear, In accordance wilh Ihe above. Ihf' passage of a gas through a shock, which is adiabatic in its 1I111111'e becall:'m it uccurs in a thermally in~lIlaLed ~ysl('m, is 8n irreversible adiabatic non·isentropic process. Equation (4.:i,(i) cau he uscil to wrify tha.t a real process of an increase in the entropy (S2 - 8 1 > 0) corresponds to a supersonic
182
Pt. I. Theory. Aerodynamics 01 an Ai,foil and " Wing
flow [M 1 > 1 (a Ilormal shock). HI sill Os > 1 (all oblique shock)], while the physically impossible phenomenon of a decrease in the entropy (S2 - SI < 0), to a subsonic flo\\' (MI < 1 ilnd MI sin Os < < 1). Hence, shucks can appear only in a supersonic f/ow. We must note (hal the relations obtained for the change ill the entropy are valid when an irreversible process of transition through a shock attended by an isentropic flo\\ ~tr, we eannot find a graphical solution for a slwck with the aid of a shock polar. This is due to the fact that the inequality ~s > ~or does not correspond to the assumptions (on the basis of which we obtained equations for a shock) consisting in that a shock is straight and sholtld be attached to a nose. Physi~ caUy-ill the given case of the wedge anglo ~s exceeding the eriticai deflectiou angle fie r-the compression shock detaches and becomes cUl'verl, The determination of the shape of such a cuned shock and of its distance to the bod~r is the task of 11 special problem of aerodynam· ics associated, particularly, with the conditions of supercritical flow past a wedge. If such a problem is not selved, then with the aid of a polar in the field of defmition from point D to A we can give only a qualitative appraisal of the change in tbe parameters in a re~ gion ahead of the surface in the flow, If, on the other hand, the shape of the shock is determined for presot fiow conditions (in addition to calculations, this can also be done with the aid of blowing in a wind tunnel), it is possible to establish quantitative eorrespondence between the points of a shock polar and the shock surface. Assume. for example, that we have set the angle Pa and points E and N on a shock polar (Fig. 4.1.2). The shock angle 6$N = LANG corresponds to point X, and the angle SsE = LAEK (EK ..L OB) to point E. If the configuration of the shock wave front is known, then by direct measurement \"e can lind on it a point N' with the wne angle SsN" and a point E' with the angle 6 5 1:;' (see Fig. 4.3.4). [n tht! ~aJLle way, we can find II. puillt C' 011 the shock that corresponds to the critical (maximum) denection angle Per. On a preset surface of a detached shock, point D on the shock polar corresponds to the shock apex (a normal shock), and terminal point A of the polar corresponds to the remotest part of the shock that has transformed into a line of weak disturbances. For an attached shock (Ps < ~ef)' we can indicate two solutions, as can be seen on the shock polar. One of them (point E) corresponds to a lower velocity behind the shock, and the other (point N), to 8 higher one. ObservaLions show that attached shoe-ks with a higher velocity behind them, i.e. shocks with a lower strength are possible physical b'. If we dra'.... on the graph the arc of a circle whose l'adius is unity (in the dimensional axes wand u this corresponds to a radius equal to the critical speed of sOltnd a*), we can determiue the regions of the now-subsonic and supersonic-which points on the shock polar to the left and right of the arc correspond to. In Fig. 4.3.4, the section of the flow corresponding to a subsonic velocity is hate·hed. A close look at the shock polar reveals lhat the yelocity is always
184
PI. I. Theory. Aerodyn./lmics of .!In Airfoil .!Inc! .!I Wing
subsonic behind a normal shock. On the other hand, behind an ob· lique (curved) shock, the velocity may be either sllper~onic (the rei· evant points on the shock polar are to the righl of point S) or subsonic (the points on the polar arc to th~ left of point S). Points on the polar between Sand C corre.spond to an attached shock behind which the velocities arc subsonic. Experimental investigations show that for wedge angles ~s less than the critical one ~cr or larger than L SOB, a shock remains attached, but it hecome!i curved. The theoretical values for the angle as and the gas velocity AZ on the entire section behind such a curved shock fOllnd on the polar accord· ing to the wedge angle B~ do not correspolld to the actnal values.
4.5. A Hormal Shock In the Flow of a Gas with Constant Speclfc Heats We shall obtain the corresponding relations for a normal shock from the condition that 6s ---: ,,/2 and. consequently, Vnl = VI and V n2 = V~. Basic eqnation (4.3.10) becomes (4.0.1) '(4.5.1') where Al = 1'1Ja* and A2 = V 2Ja*. We find the relative change in the velocity from (4.3.11'):
Ii iT ~ (V, -
V,)/V, ~ (1 -
6) (1 -
11M:)
(4.5.2)
We obtain the corresponding relation~ for the ratios of thE' densities, pressures, and temperatures from (4.3.13), (4.3.15), and (4.3.16): P2/PI = M:/(1 - 6 6M~) (4.5.3) P2iPI = (1 + 6) M: - 6 (4.5.4) T,fT, ~ [(1 6) M: - 6[ (1 - 6 6M:)fbP, (4.5.5)
+
+
+
By eliminating M~ from (4.5.3) and (4.5.4), we obtain an equation of a shock adiabat for a normal shock that in its appearance differs in no way from the similar equation for an oblique shock [see (4.3.13')[. Assuming in (4.3.19) that as = nl2, we find the relation for the Mach' number behind a normal shock: .V:iM: = (TilT 2) (P IJp2)2 (4.5.6) Let us consider the parameters of a gas at the point of stagnation (at the critical point) of a blunt surface behind a normal !ihock (Fig. 4.5.1). The pressure p~ at this point is determined by formula
Ch. 4. Shock W~ve Theory
18~
(4.3.20') in which the ralio." P2 PI allci P~ PI are found from (·'J.5.8}· and (1.5.4), respccliH·ly. With this in view. we han p~fpo =
[(1 -;- 6)
M~
61("-1)/~"
-
fM;/(t - 6 ...
6M~)JCh~)/~"
(4.:1.7)
Determining Po by (4.3.21), we fmd P;/Pl =
[(1 -;- 6) M; -
61(&-1)/~"
..tt(~'6)/6 (I -
6)-(14&J/~6
(4.5.8)
Knowing the absolute pre~surt! p~, we can determine I he dimE'lIsionless quantity = (p~ - PI) (h-the pressure coeflicient fit the stagnat.ion point. Taking into account that the velocity head is
Po
ql:"'"
kP~l/I
2(11-.'_°6 ) filM:
we obtain
Po=
(~.~6~~~ {1(1--· 6) M~ _61(6 - J)/~\ JI I (I i 61/6 x(1_6)-(1+6)/2~_
.. }
(1.'=-dl)
It is proved in Sec. 4.3 that the stagnalion temperature behind a shock does not change, i.e. T~ = To. Consequenlly. at the ;;tilgllation point. we have
T~'-' Td 1 + I~b
.un
(0.10)
Let us usc the expression i~ :..::... cpTo aIH) il = c,,TI 10 determine the enthalpy. Acconlingly. at the stagnation point. we haw
186
Pt. I. Theory. Aerodyn~mjcs of an Airfoil ~nd • Wing
4.6. A Shock at Hypersonic Velocities and Condanf Specific Heals
0'.
Gas
At hypersonic (very high) velocities, which values of MI sin O. >::> t correspond to, the dimensionless parameters of a gas behind .a shock are very close to their limiting values obtained at HI sin Os __ __ 00. It follows from (4.3.11') that for this condition, we have
(4.6.1) Consequently, the limiting ratio of the densities by (4.2.13) is
p,/p,' - 1- ~V.
- 6
(4.6.2)
Introducing this ..-alue into (4.3.27), we obtain the following ex;pression at. the limit when MI sin 8, __ 00:
tan e.= (cotJl,/U) [I-b ± ]f"'(1-'6"')';-4n;67ta"'n"'~"'.1
(4.6.3)
Let us lind the limiting value of the pressure coeffIcient. For the ·conditions directly behind a shock. as follows from (4.3.15~), when MI sin Os -- 00 and MI __ 00, we have
(4.6.4) We obtain the corresponding quanlity for the point of stagnation
f'om (4.3.23):
Po =
2 (1 -
6)(6-1)126
(1
+ 6)-{1.")!'.!" sin as 2
(4.6.5)
The ratio of the pressure coefficients is
(4.6.6)
Poipz
In the particular case when 6 = 1/13 (k '-' 1.4), the ratio = = 1.09. The limiting value of the llumber M2 can be found from (4.3.19), using relation (4.3.16) for TzIT 1 • A passage to the limit when MI sin 0, __ 00 and HI __ 00 yields
M:- {II [6 (I ~.6)J) (cot' e,+6')
(4.6.7)
To lind the limiting parameters behind a normal shock, we must assume that 9 s = :t/2 in the above relations. As a result, from (4.6.4) and (1.6.5) WC" h8\'e:
Po =
p, 2 (1 -
2 (1 - 6) 6)lll-il/26 (1 -i- 6)-(l+W26
(I,.G.·1') (4.6.;;')
en.
4. S~ock Wdve T~.eory
181
We C(ln :;ec that the ratio Po'I-;~ i:-: the .':'amea~ ror i1n olJliqut' Sllotl;. The limiting Milch lIumhel' behind OJ JI()l"m~d ~hock is
For 6;;;....; 1,'(j (k --: 1.4), the 11\11111)('1' M ~ - 1/"[7 :::::: O.3t\. The actual v(lllies of the dilnensionle-s5 parrlrnelf'I's behind a shock fit linitl:!. nlthough very large', Mnch I\Ulll!wr." depC'nd on M l · Let \I.':' considf!l' the corrl!sponding' worki1lg rrlation:-: fOl" lilt' r.a.':'e when !lUnched ;.;hock.'< originalr ahead or ;.;h'uder \\·('cigcs. ami the .sllOek angles ,"lrP thcrd"ol'C' low. A~"nlllillg ill (!I.~-t:!;;) Ihal tan s ~ .~ e~ nll(l tall ~J :::::: 0, - ~,. w(' oblai"
e
(e, -
(0, - ~,) 0, ~ (l - b ., 6M;O~)(,I1;O;) Introducing Ihe syrnbol K ~ Ml~~' art('r Il'all.' of the (jU,Hltilies chal'acterizing h~'persouiC' nO\\·.~. \\"11('(1 Sill·1I rlo\\"s han> identical partlinett'I's K, the ratios of the angl('s e~;ll., r parameters, namely, p~, T~, p~, etc. The results of the calculations correspond to the preset flight altitude. A change in the altitude is at.t.ellllf!'d by a changc ill the conditions of flow past. a body and, consequently. in the paralllcters at t.he point of stagnation. This relation is shown graphically in Fig. 4.7.4. The curves allow us to determine the temperat.ure T~ and pressure p~ as a function of the veloci\.~' V, and the flight altitude H. The value of p~, in turn, can he used to ca!r.ulate the pressnre coefficient at the point of stagnat.ion: Po = O.'skM;'. (p~/p "" - 1). Its value grows somewhat in a di.!'50ciating flow. For exam piC', at an altitude of 10 km at M~ = ifi.7, its valne is Pi) '""'" ~.08, whereas without account taken of dissociation = 1.83 (for k =- cJ'.·c,. = = 1.4). The pressure coefficient can be seen to grow by abOHt 1R%_
Po
192
Pt. I. Theory. Aerodyntlmics of an Airfoil 1:3. when the dissocialioll of the nitrogen becomes appreciable. the dependence of fl~lpoo on M"" for air reminds one of the similar relation for gaseolls nitrogcll bccause the iatter is the predominating component. in tile air. The C;llcnlation of the parameters of a gas behind a shock ,vith a vicw to the varying na~llre of l!le specifiC heats is Ilescribed in greater detail in [141. 4.8. Relaxation Phenomena Sectioll 1.7 deals with ways o[ calculating the parameters of a gas behind a shock with account taken of tile physicochemical transformations for conditions of equilibrium of the thermodynamic processes. In a more general case, however, these processes are characterized by non-pquilibrium, which has a delluite innuence 011 the gas flo\\' behind shocks. Non-Equilibrium Flows
It is known from thermodynamics that the ilssumption of thermodynamic equilibrium consist.s in agreement brt,veen the le,-els of the internal degrees of freedom and the parameters characterizing the state of a gas, For example, at comparati\'ely low temperatures (low velocities), equilibrium sets in between the temperature and the vibrational degree of freedom, which corresponds to equilibrium l.Jet,veen the temperature and till} specirlc heat. At high temperatur(}s (high velocities), when a gas diSSOCiates, the equilibrium state is reached as follows. As diSSOCiation develops, the probability of triple collisions grows (for a binary mixture of diatomic gases) because the numher of gas particles increas(}s. This leads to the acceleration of recombination and the retardation of the rate of dissociatioll. At a certaill instant and t(}mperature, the rates of the direct and reverse r(}actious become equal, and the gas arrives at an equilibrium state. The latter is characterized by a constant composition and agreement between the degree of dissociation, on the one hand, and the temperature and pressure, on t.he other. At still higher temperatures (very high velocities), equilibrium processes of excitation of the electron levels and ionizatiOIl can be considered. Upon a sudden change in the temperature in an equilibrium flow, the corresponding internal degrees of freedom also set in instantaneously; dissociation~and ionization call be considered as the manifestation of new degrees of freedom. Consequently, in these cases, there is'no delay in establishing the degrees of freedom, i.e. the time needed for achieving equilibrinm is zero.
194
Pt. I. Theory. Aerodynamics 01 an Airfoil and a Wing
In practice, an equilibrium flow is observed under supersonic Dows past bodies at Mach numbers of M CO> = 4-5 in conditions corresponding to altitudes of 10-15 km and less. The explallillion is that at the maximum temperatures of the order of 1000-1500 K appearing in these conditions, the main part of the intemal energy falls to the share of the translational and rotational degrees of freedom, which upon sudden changes in the temperature are established virtually instantaneously because only a few molecular collisions are needed to achieve equilibrium. This is wby the transl;ltionai and rotational degrees of freedom arc usually called "active" degrees. With an increase in the velocities and, conseqllently, in tlie temperatnres, a substantial part of the internal energy is spent on vibrations, then on dissociation, excitation of the electrolL levels, and ionization. Actnal processes are such that these energy levels set in more slowly than the translational and rotational ones beciluse a mtlch greater number of collisions is needed. For this reason, thE' vibrational and dissociative degrees o[ fl'C'edom are sometimes called "inert" degrees. Hence, the inert degrees arc featured by a delay in the achievement o[ equilibrium called relaxation. The time in which equilibrium sets in, i.e. correspondence between the temperature and the energy level is established, is callC'd the relaxation time. The relaxation time charactertzes the rate oj attenuation oj depa1'lures oj a gas state from an equilibrtum one, which in a general case manijests itself in the jorm of a change in the energy distribution limong the di/Jerent degrees 0/ freedom. Relaxation processes are determinl'd by whal degreE' of freedom is excited. If upon a sudden change in the tempf'rilture, vibrations appear, the corresponding nOll-equilibrillm process is callC'd vibrational relaxation. It is characterized by a lag in the specific heat when the temperature changes. If the temperature rise!', the specific heat grows because of the appearance of vibrations of the atoms in the molecules. The time during which vibrational motion renclles equilibrium is called the vibrational relaxation time. In a non-equilibrium dissociating gas upon a sudden change in the temperature, a delay occurs in the change in the degree of dis!'ociation. This phenomenon is called dissociative relaxation. Owing to the difference between the rates of formation of the aloms and their vanishing (the rate of dissociation is higher than that of recombination), a gradual increase in the degree of dissociation occurs. The equilibrium value of the degree of dissociation is achieved at the instant when the rates of the direct and reverse reactions become equal. The time needed to obtain an equilibrium degree of dissociation is called the dissociative relaxation time. Experimental data on the relaxation time for oxygen and nitrogen are given in Fig. 4.8.1.
Ch, 4, Shock. WlJve Theory
195
~I~p:;~ental (I, 2) curves of the vibrationaL relaxation time
and calculated (,1, 4) curves of the relaxation timc for the dissociation or oxygcn and nitrogpn, re-spectively, at atrnosphe-ric prcssure
At. tcmperaturcs approximaLely lip to 10 000 K, the \'ibrational and dissociative relaxation proces~ws are the nlilin ones, Tht' rl'iaxalion phenoJUpna a~sociateu wiLh the excitation of the elecLro" Il'yels o[ the Illoipcldes and nlomO', and also wiLh ionizAtion, may 1)(' 4ii~re gardc41 because a small fraction of the internal energy fallO' to Ihe shal'c ot' t\Jef':e 4legret's of freedom at the indicated t('mpf'l'atllres. A nOll-equililJl'illnl slate has a substantial influence on the Yal'iollS pl'ocess('s attending the flo\\' of a gns at \'Cry high \'e1ocities, l\'l'lic1(lady, vibrational and dissociativc relaxations change t1l(' parameters of a ga!; ill a trall!;itioll throllgh shock \\'n\'('s and in the fin\\' past bodi('s, This, ill turn, aHrcts the JlrOCe~Sl'S of friction, heat exchange, and abo the redistribution of thn pr('ssurp. The studying of nOll-cquilibrium flo\\'s consists ill the joiHt investigation of the motion of the fluid and of the chemical pro('(''!:ses occuning at Hnite ,,('Ioeities. Thi~ is ex:pl'essed formally in Ihnl an eqllatioll for the rate of chemical reactions is adcle{l to till' m:nal system of equal ions of gas dynamic'!:, EquilibrIum Processes
Equilibrium flows have been studied better than non-equilibrium ones both from the qualitative and the qnantitfltive ~t 0), It decreases in tlH' real cO\Hlitions of a gradualtrl.lllsit.ion from a nonequilibrium state to RIl equilibrium flow behind a shock wave, i.e. when the degree of dissociation ehRnges from 0 behind tile wave to the equilibrium value '"1. , ..:: etc at the ell~1 of the relaxation zone.
5 Method of Characteristics
5.1. Equlflons for !he velocity Potential and Stream Funcffon
An important place in aerodynamics is occupied by the method of characteristics, which allows one to calculate the disturbed flow of an ideal (inviscid) gas, This method make~ it possible to design correctly the contours of nozzles for supersonic wind tunnels, determine the parameters of supersonic flow over airfoils and craft bodies. The method of characteristics has been developed comprehensively for solving the system of equations of steady supersonic two-dimensional (plane or spatial axisymmetric) vortex and vortex-free gas flows. Investigations associated with the lISC of the method of characteristics for calculating the three-dimensional flow over bodies 8fC being performed on a broad scale. Below we consider the method of characteristics and its application to problems on supersonic twodimensional flows. Equations for a two-dimensional plane steady Dow of an illViscid gas are obtained from (3.1.20) provided that 1.1. = 0, 8V,/8t = = 8V,/8t = 0 anel hAve the following form: V
oV", '"
V:c
oz
~~. _..!..~ }
+l' g
8y
P
iJz
(;"'d.1)
0:; + V, ~:' =, _~. ~~
For a two-dimensional axisymmetric flow, the equations of motion obtained from (3.1.36) for similar conditions (v = 0, 8V,/8t = = 8V,IOt = 0) can be wriLten in the form
'V~=-..!.'..!f....}
Vx
DV", ilz
V:c
o~r + Vr :~r
I
r
p
or
=
iJz
(5.1.2)
_~.*
The conLinuity equlltions for plune and axisymmetric Dows .having
r('~pcctively the form of (2.4.5) Rnd (2.4.32) can be generalIzed as
Ch. 5. Method 01 Characteri~tic~
20t
follows: a (pV""yt),()x -j d (rVyye),'uy
~-
0
(5.t.3}
When e = 0, this equalion coincides with the continuity equation for a two-dimensional plane now in the Carlesian coor(linates x and y. If e = 1. we have a continuity equation for a two-dimensional axisymmetric Dow in the cylindrical coordinates y (r), I. Accordingly,. for both kinds of flow, we may consider that the equatiolls of mot ion Fd.1) arc written in a gent'ralized form. Having determined the partial derivative!> ill continuity equation (5.1.3), we obtain
(v~ ~~
+ V" !~
)ye+pyt ( a;~x.1
{}~1I) ~pVyf:yF-l
.. 0
(5.1.4}
V'le can replace the partial derivative ap./oJ: wiLh lhe expression Dp/ax = (ap/Elp) aplfJx, in which Elp/fJp = La:!, while the derivative &p/&x is found from (5.1.1) in the form
-r (Vo. o~:
_;
Vy (.~;Ix)
\\'jth this in view, we have
;~ '-- -%(Vx
{}fJi:x -:
Vy
(5.1.5)
An expression fo!" the del'ivat ivl' rlp/oy is way:
~';
,;, -7 (V
x
rJ~;"
f()lItHI
+ V~, ;',~> )
similar
(5.1.6)
Substitution of the vnluC's of th('!ie d(>ri\"{\ti\"t.~ into (:U.4) yields
This cqualioll is thC' fundam(>ntal differential equation of gas dynamics for a two-dimensional (plane or spatial axis~ mmelric) steady tlow which the velocity cOlilponelll~ and mllst satisfy. Since this equation reJatr:i the \"('Ioritie~, it is {liso 1'C'Cerrcd to a~ the fundamental kinematic {'(Iuation. If a flow ii' potential, tllell
r ..
l:x'-- dq,u,t·, VII :."': oq uy, dVx/{Jy thcrc!ort·, Ey. F).l.7) (Vi-a2)
~"j:~
.j
l:U!l
2V.Y'J
ry
= 8J'v·lIJ' = (P!p.'ih ay
he transformed as follows:
(:'.1.8)·
PI. I. Theory. Aerodynamics of an Airfoil and. .e. Wing
202
where
Equation (5.1.8) is the fundamental differential equation of gas dynamics for a two-dimensional potential stead)' flow and is called an equation for the vcloeity potential. Hence, unlike (5.1.7), Eq. (5.1.8) is used only for studying vortex-free gas flows. If a two-dimensional gas now is a vortex one, the stream function 1Jl lias to be used for studying it. The velocity components expressed in terms of the function 1Jl have the form of (2.5.5). Replacing p in accordance with formula (3.G.31) in which the stagnation density PI! along a given streamline is assumed to be constant, expressions (2.5.5) can be written as follows: Vol = y-t (1 _
f1)-1/(4-1)
o1jJloy,
VII = _y-. (1 _ y2)
_1/(4_1)
o¢/ox (5.1.9)
where j7 = VIV,u:\~. The cRlculaLion of a vortex gas flow consists in solving a differelltial equation for the stream function "p. To obtoin tllis equation, let tiS rUffprentiate (5.1.9) with respect to y and to x:
"~;'
= _ey-e-l (1_V"2tli(4-1l : :
(1- yttl/(A-Il-1
":~"
.. _ y-e
a~2 . ::
-j_
+y-e~
y-e (1- VZ)-I/(k-I)
~ (1- V2tl/(h-1)-1 ~~2
.
~~
~:~
_ y-e (1- Vit1(1t-1l
~
T,1king into account expression (3.0.22) for the square of the speed of sound, and also relations (5.1.9), we can write the expressions obtained for the derivatives oV,)oy and oV,/ox as follows:
J:;
'--co
_+ v.,.,-
~:~. "~2 +y-e(l_V2)-,/(h-1l ~:~
":;"~, :a~. a~2 _y-e(1_Y2)-I/(h-1l ~:~
(5.1.10)
(5.1.11)
We shall determine the derivatives oV2loy and oV'llox in Eqs. (5.1.10) and (5.1.11) with the aid of relations (5.1.9). Combining these relations, we obtain (5.1.12)
Ch. S. Method of Chllrllcteristics
203
By difierent.iating (5.1.12) with respect to x anti y, we lind the relevant relations: 2 :~ . ~:~. -t- 2 ~,!
2
~;
.
.a~:fJ~
~. ~ t
_ P y 2f
yte
. ~:~ _, ~~2 y2"
a~~~y .:- 2 ~!
2eV2 y 2e -1 (1 _
~~:
--.-
Y2)2/(/'-t) _ 1'2y2e
V2)~/(~-L)
(t -
('I _ V2)10l/(I!-I)-I
(~~2
(1 ._-
V?)'~I(I!-I)
~ 0 - i12.)2/(I
(5.1.23)
Since a Z = kRT, then, taking (3.6.22) into account, we fl"!ld an expression for the temperature: Tc.""",
;~ ,_ k~1 .*(V~lax-V2.)= k~t. V~nJ! (1--V2)
Introducing this relation into (5.t.23), we obtain
o~,:
_o~:
.=
~. 1~1~~~
(1- V~)
~:
(5.1.24)
By introducing the vortex according to this expression into (5.1.15), we lind a differential equation for tile sLream function:
(Vi-a 2 ) ~:~ +2V:'Yllo!~o~ L(V~_a2) ~~l;
+ yt'-e a2V
%
(1- V2 ),/(h-1)
= k;;1 • V;;'J! (1- V2).\/(.\-O ye (02 _
V~) ~:
(5.1.2:1)
5.2. The Cauchy Problem
Equations (5.-1.8) for the velocity potential and (5.1.25) for the stream function are inhomogeneous nonvlinear second-order partial differential equations. The soilltion~ of these equations cp = cp (x, y) and W= W(x, y) are depicted geometrically by integral surface~ in a space determined by the coordinate systems x, g, cp or x, y, 1p. In these systems, the plane x, y is considered as the basic one and is called the pbysical plane or tile planc of independent varlableA.
206
pt.
I. Theory. Aerodynamic, of In Airfoil Ind
I,
Wing
r!'ii!f'~urve AB; the required function and its first derivatives witil respect to:e and y are on it
known
Tho Cauchy problem consists in finding snch solutions in the vicinity of all initial curve y = y (x) satisfying the additional conditions set Oil this curve. The values of the required function (jl (x, g)
~i~~alx~~?d~~i~r~!~e -fll~:~ d::!v~~i:\~~ ~1~S (t;'~hY~: ~~~t:~e ~~~Jlit~~:~!~ From the geometric viewpoint, the Cauchy problem consists in finding nn integral surface in the space x, y, cp (or x, y, 'lJl) that passes through a preset spatial curve. It is just the projection of this curve onto the plnno g, x that is the initial curve y = y (x) on this plane. The solution of the Cauchy problem as applied to the investigation of supersonic gas flows and the development of the corresponding method of characteristics arc t.he results of work performed by the Sovict scientist, prof. F. Frankl. To consider the Cauchy problem, let us write Eqs. (5.1.8) and (5.1.25) in the general form Au
+ 2Bs + Ct + H =
0
(5.2.1)
:~~~ed up:rtT:i J~~i~;t~~:s:=\:;V v~Ol::rV~f ~,d ~,=a:dv Jo:qt"a'l' :~: coefficients of the corresponding second partial derivatives, and the quantity H is determined by the free terms in Eqs. (5.1.8) and (5.1.25). We shall find a solution of Eq. (5.2.t) in the vicinity of the initial curve AB (Fig. 5.2.t) in the form of a series. At a point M (x o, Yo). the required function is
~ (x"
y,)
~ ~ (x, y)+ ~
+, [(dx)' ::~
n=f
+f (L\X}fl-J 6y 8.t:~~~8v + X
m::'·,.'
n
(~~1) (6x)n-2 (6y2)
+ ... + (dy)' ~:n
(5.2.2)
Ch. S. Method of Characteristics
207
where IP (x, y) is the value of this function at the given point A (x, y)on the initial curve, fix = ;:j';1J - x, fUnl fly = YIJ - y. The function 'If may be used ill (5.2.2) instead of IP. Series (5.2.2) yields the required ~olution if values of Lh(' [HIl('Lions IP (or 'If) and also their derivatives of any order exist on a gin'n curve and arc known. Since the flrst derh'alives on this curve [\\'(' shall denote them by p = (fx (or 'fr) and q "-' lPu (or 1f,)} arc gin'lI. our task consists in fmding the second derivatives on it, and ul!'o clt'rh'utives of a higher order. lIcmce. the solution of tlu' Cau(,hy prohlem is associat~d wilh flUding of the conditions in which til(' higlwr (l('ri\·.:I.' tives 011 the givl'1l curvl' ('UIl b(' delermilled. shalilimiL (lul'~('IYCS to determination of thc second derinth"es. Since these cic'rh-ilLiYes are three in numbel' (u, s. rille! t), we ha"'(' to compih· Ihl' !'ame lIumber of indl'Jll'II O. Such curves, at each point of which the principal determinant of system (5.2.3) is zero, are called characteristics, and Eq. (5.2.5) is called a characteristic one. From the above, there follows a condition in which the unambiguous determination of the second derivatives on the initial curve is possible: no arc element of this curve should coincide with the characteristics. The same condition .1. 'ji::O holds for the unambiguous determination of tile higher derivatives in series (5.2.2). Consequently, if .1. 'ji::O, all the coenicients of series (5.2.2) are determined unambiguously according to the data on the initial curve. Consequently, the condition .1. =I=- 0 is necessary and sufficient t.o solve the Cauchy problem. This problem has a fundamental significance in the theory of partial dinerential equations. and formula (5.2.2) can be used to calculate the flow of a gas. Dut from the viewpoint of the physical applications, particularly of the calculation of supersonic gas flows, of greater interest is the problem of determining the solution according to the characteristics, i.o. the method of characteristic'S. This method can be obtained from an analysis of the Cauchy problem and consists in the following. Let us assume that the initial curve An coincides with one of tho characteristics. and not only the principal determinant of the system (5.2.3) equals zero along it. but also the partial determinants .1." = d, = .1., = O. It. can be proved here that if, lor example. the determinants !J. and A, equal zero, i.e. (5.2.5') Ay" - 2By' + C ~ 0 (5.2.7) A (y'q' - p') - 2Bq' - H = 0 where p' = dpldx. q' = dq/dx. then the equality to zero of the other determinants is satisfied automatically.
Ch. S. Method or Cherecteristics
209
Ar.cording to the theor~' of s)'stems of algebraic equations, the equality to zero of the principal and all the partial determinants signifies that solutions of system (5.2.3), although they are ambiguous. can exi.,t. If one of the solutions. for example, that for u, is fmite. then the 801lltions for sand t are also tinite. 5.3. Characteristics CompatlbllHy Conditions
Equations (5.2.5) and (5.2.7) (1 by differential eqllation (j.LH) ('orrc."lpolld to points of the CUf\'e~ determined hy differl:'nlial eqlHlt-ion (5.1.25). Hence, II definite point 011 a duu·ac_teristic ill the plane p, q corresponds to direcLion of the chflracteristics in the plane p. 1 if the direction or. the conjll~ate characteristics in the phYl'lirlll pl-- k;;.1
~~~;x
(1_YZ)k/(I,-uye(a2_V2)
~~
]
,-,0
After cancelling quantities where possible and inLroducing the dimensionless variables
Vx
-= V.JV.nnx' fy = l'yfVmu.
V
= V/Vmu ' VIa -=
M
we ean wriLe this equation in thf' rorm
f A1 .2tV')'2.1- Vy)!
(d~'(~.I_d;:)
r!I-Vx1l' .J/r,. flow uefleciioll angle ~e. entropy Sc. etc.) at. the inter~ectioll of clements of charfl('.tcristirs 01' the lil'st anti gccond families drawll from points A and JJ (Fig. 5.4.10). At these points~ whirh arc on diffl'rent strealillille~. we know the velocities VAt Vo• and other parameters, including the cntropie. element Dr fl' of it characteristic of the ~econd famiJy ill 0. hodograph ("orrl'spond~ to all element of n ('.hafnrteri~tic of the same family in n physicnl pI nne. The third problem consist~ in calculating the YP\ocity at the interl'prtioll of the charartE'ristics with a ."hod, alld in determilling the rhl'lnge in t.he inclinatiOIl of the shock at. this point. Since a characteristic in its nature is a line of weak di.~lllfhan('e.", Ihis illtersectioll physically ('orrc!'iponds 10 the inlcraclion of a wpal, w(\\-e \\"lth a compression shark. Assume that closely arrangpd expan"ioll wa\"('~, ""hi('\l rharacteril'tics of the first family ('orrespolld to. fnll at points J and H on ('omprc~sioll shock A· of a preset shape!J ..,.t tl") (Fig. 5.4.3a). As a rcsult, the streng!11 dimillishL's. as dol'S the inclination angle of the shock_ Sin('c points.r nnd Jl :lr(' SOllrces of (Iistllrbanccs. expansion wa\"C~ appear, AJI(I ('h~facteristics of thc .~ecOl\d bmily ran he drawn through these point". Olle of stich rharartl'fistics, pa.sumed to be linear. The angle of inclinl'llion of thc »ilo('k on this section and the corresponding pa-
228
pt, I. Theory. Aerodynamic.s of an Airfoil and a Wing
(6)
(•.1
~y
rameters of t.he gas are approximately equal Lo their values at inLersection point II of clement FH of a first family characteristic with the shock. One or the unknown parameters is the angle of indinatioll ~H of the velocity vector at this point. which can be written as ~H = = A~p + ~p, where A~Ji' ~H - ~F. and ~F is the known angle of inclination of the velocity vector at point F. To evaluate the second unknown (the number MH at the same point) we shall use the formula MH ~ MJ -I- (dMld~)JA~JH (5.4.32) in whicb (dMld~)J is a derivative calculated with the aid of the relevant expressions for a compression shock according to the known parameters at point J, and the quantity A~JH determined by the change in the angle ~ along a shock element equals the dirt:erence ~H - ~J. We may assume that this quantity approximately equals the change in the angle ~ along the element FH of a characteristic of the lirst family A~PH --' L1~p PH - PF' The derivative dMldP is evaluated as a result of difterentiation of (4.3.19'), 00
of the families AAn (let us consider it to be a characteristic of the sl;lcond family) emerging from point A on all arc of radius rA (Fig. 5.5.3). Point Al is at the intersection of ray r 1 = = OA I with the element of characteristic AA I drawn at an angle of ~"" -- _Sill- I (11M ",,). We fwd the number MI at point Al \vitl! thp aid of the expression 91 = 8*IS1 • Since 8 1 = 2ar1 ,1 (21'/360), and S* -= :!nr*·1 (2yl360), we have ih = r*lrI . Employing (3.6.·'.6), \ve can lind Al and the corre~ponding number MI' We determine in a similar way the coordinates of intersection point A z of the adjacent ray rz = 0.1 2 with the element of character· istic AIAz inclined to straight line OA I at the angle ~(l = = _sin- l (1IM I ), the number M2 at point A2\ and so on. As a result, wo can construct a characterist.ic of the secolJd family in the form of broken line AA1 ... An_tAn int('r~ect.ing straight wall BAn of the nozzle at point An. For this point, as for the other points An_2' An_I' and An of intersection of the characteristic wit.h the straight lines emerging from source 0, we r.an calculate the relevant Mach numbers and the angles fL = -sin-l (11M). The flow region OAAn with a known velocity field confllled by the characteristic AAn and the straight walls of the nozzle is called a triangle of definiteness. The shape of this flow is preserved if we change the wall behind point An so that the radial flow on the Mach line gradually transforms into a plane parallel flow at the exit.
Ch, 5, Method of Characteristics
\'"ith a "iew to
thi~
'233
ronciilioll, we can
of the nr!'t family eml'l'ging from point ~traight lirH', If we now determine the the ehMueteristie!' AA" /Iud ADm' we lillc~. I t is exactly the .streamline pa. wloeit\' field, \\.(' dimensional tlow being (,(;ll:"idl'r('ri the rhara('1l'ristic.'< of theftr.!'t family elll(,l'ging from point,;.: /t" -2 ... 1". l' ilS \\'('11 as the rhnraeteristir .. iD m art' slraight lillc.s Wig, :;,5,:~), Till' inclination of ead( charartN'islic 10 a radial line is II(>terlllin('d by thcenrri'5pOndIng ~!ar1t anglc jl( _. sin- J (J'Il!I). ~12 sin· 1 (t/M 2 ), C!t cx.Ii)' Figure 6.5.2 shows graphically how the coellicients c,III ant! Cx,1 are converted from the aspect ratio AWl to Aw2 in accordance with formulas (6.5.5) and (6.5.6). First the curves c'a "" II (al) and CUll = = Cfl (cx,n) are plotted for a wing with the given aspect ratio AWl' Next. setting ~ number of values of c,Ia' we lise the plot to determine the correspondmg values of a 1 and c;.;.Il' and then calculate l.he angles of attack a2 and the coefficients c.~ 12 for the second WHlg by formulas (6.5.5) and (6.5.6). The corresponding points are laid off, and the curves C,I. = h. (0:.2) arId c,In -= (f2 (c x.l2) are plotted, For wings with smaller aspect ratios ().w:z < AWl)' these l'Uf\'eS will be to the right of those of tile ratio Awl because with the same true angle of attack, tIle incrcage in the downwash angle €w2 [Ol' the second wing with a smaller A,,2 is compensated by the growth in the setting angle of attack (a2 > a 1); ill turn, all illcreased coefiici('nt C.~.12 corresponds to tho greater downwash angle 1:'''''2, and this i:5 exactly what is shown in Fig. 6.5.2. The plots in Fig. 6.5.2 can be llsed to convert clla and Cx .! to a wing with an infini tely large aspect ratio (airfoil). For this pt1rpose,
262
Pt. I. Theory. Aerodynamics of an Airfoil and a Wing
the second terms in the brackets in formulas (6.5.5) and (6.5.6) must be taken equal to zero. The converted curves Clla ~-..: 12 (a2) and clla = = 1"f2 (C~.I2) will occupy a position at the extreme left of the corresponding curves clI , = h (al) and cu, = 'PI (c~.Il). Mean Aerodynamic ChoM. When performing aerodynamic calculations of finite-span wings. the mean aerodynamic clIord is selected as the characteristic geometric dimension of the span. Such a chord belongs to a conditional wing having a rectangular planform for which the planform area. the aerodynamic force, and the pitching moment are the same as for a wing of the given planform. The mean aerodynamic chord allows us to compare the moment characteristics of various wings with a varying chord along their span. One of such characteristics is the pitching moment coefticient determined as mlA = Mz/(bAqSw). where bA is the mean aerodynamic chord. The quantity mzA is sufficiently stable when the planform of a wing and its dimensions change. The value of the chord h. and those of the coordinates of its leading point XA. YA (relative to coordinate axes passing through the apex of the given wing), are usually determined approximately assuming equality of the aerodynamic coefficients (of the moment, drag, and lift) of a wing as a whole and its individual section (profile). Accordingly. we have
bA=S~
'/'
1/'
) b2 (z)dz,
o
1
z·--i;-I%b(Z)d'l
(6.5.7)
'/2
YA-
L Jo yb('Jd,
J
where x, yare the longitudinal and vertical coordinates of the leading point of a section with the varying chord b (z). Evidently, knowing and the equation of the leading edge of a given wing, we can determine the lateral coordinate ZA of the mean aerodynamic chord. Formulas (6.5.7) make it possible to calculate the magnitude of the chord bA, by numerical or graphical integration and determine its position. The middle of bA coincides with the centre of gravity of the wing area. For a broad range of wings having a trapezoidal planform, we can find analytical relations for bAr xA. NA' and ZA' For such wings
XI.
b(.)-bo[I-(~w-IJ'/~wJ } Sw-b,l(~w+I)/(2'1w)
z=ztan"o;
y=ztan1p
(6.5.8)
Ch. 6. Airloil and Finite-Span Wing in Incompressible Flow
263
where f). = bJb A is the taper ratio of the wing, XI' is the sweep angle of the leading edge. ~: is the dihedral angle. and i""" 2-;11. Introduction of (6.5.8) inlo «(i.5.7) yields
bA =4Sw [1-~"/(tl"+ 1)'[/(31) } ZA,= 1(f)w+ 2) tan xo/rO (11,,·+ 1)1 YA=I(~w" 2)1.n~·/[6(~ .. -< 1)[
(U.5.U)
'fhe lateral coordinate of the (.hord bit, is found from the formula ZA ..." XIt, !tan Xo_ [f 8 wing tla:o; no dihedral, the coordinate YA, is evidently zero.
An Airfoil in a Compressible Flow
7
7.1. Subsonic Flow over
iI
Thin Airfoil
LInearization of the Equation lor the Velocity Potential
The calculation of a subsonic flow over an airfoil i.e; associated with solution of the equation for the velocity potential of a plane two~ dimensional flow that is obtained from (5.1.8) provided that e = 0 and has the form (Vi-a 2)
;;~
+2V:rVII a!2:y
+(V~-a2) :~ s::::0.
(7.1.1)
This partial differential equation of the second order is non-linear in the unknowll function o. The Khristianovich method is sllitable provided that- the velocity is suhsunic o\"er the enlil'tl airfoil. This condition is satisfied if the Mach number of the oncoming now is les.." thnll the critical value M cr' Conseqllently, hefore p(>rfol'ming calculations, one mllst find tlds criticnl value nnd determine the numbf'r M"" < M "-'. er for whirh calculations are possible. The critical 1lI1l11bN Moo .... , can also be found by the Khristianovich method. 0O
Assume that we know thr {listrilmtiOIl of the pressure coefficient over an airfoil in Iln incompressible flow, i.e. we know the form of thC' function Pic c- Pie (x) (Fig. 7.2.2). This fnnction is converted to the number M"",.er > Moo > 0 n~ follows. We determine the speed ratio accorciillg to the given number M~>O:
A"" _=
Ikt I M;, (1-1- k-;t .ill;' r!r 2
(7.2.J)
From Tahle 7.2.1, we (ind the i'lflitioH$ speed ralio .\"" of an ill_ eOlllprf'ssible flmv corresponding to the value ;."'" and for tl\{> choSE'Q value of frolll th(> Bernoulli e(lllation
Pic
(7.2.2) we determine the local fictitious speed ratio
(7.2.2') Kllowing A, we usc Table 7.2.1 to find t.he loeal trlle ! M"" > 0, we Cllll determine the value of Pte, mIll by the COH\'ersion of Pic. min to the number Moo = O. Assume tha~ we know the value of lhe maximullI rarefaction P1C. IHln' Since}, -""", 1 \....here a sonic velocity appears, from Table i .2.1 we can find the corresponding value of the local spe(>.d ratio of the fictitiouS incompressible flow, i.e. A ~ 0.7577. Gsing the Bernoulli equation mIn = 1 - (A/.\",,)2 we can find the speed ratio for the fktitiollS oncorning flow:
Pic.
1\00
=
A/I ' 1- Pic, mill =. 0.7577 / I·
'1-
Pic,
mIll
(i .2.5)
while H~illg Table 7.2.1 and the value of .\"" we can deterrnine the critical speed ratio A",_ cr of the compre~sihle flow. The corresponding critical Mar-h number is
M",. cr =
"00, cr (k-~-1_ 1.:-;-1 A~, er) -1.'2
(i .2.G)
A plot of the critical Mach number "erslls "I~' 111111 con.slructed ae.cording to the results of the above calculation isshown in Fig. 7.2.3. An increase in the airfoil thickness is attended hy a decrease in the IIl1mber M Cr' The explanation i~ that such all inr-rease leads to contraction of tlte stream lilament and to an increase in the local flo\\' velocily. Conseqnently, sonie "elocity on a thickened airfoil is achie"ed at a lower fr('e-~tl"eam velocity. i.e. at a lower value of M 1'1"". cr- This conclusion follows (liree.tly frolll Fig. 7.2.3 in acconlnnce with which at all illcreased local yelodty lower Yulues of M",.cr correspond to a lower value of the coeffirient Pte. ml,,' Upon an inet'ease in the angle of attack, the /lumber M "". cr diminishes, which is also explained by tlw greater contraction of the streO'l.rn HIaments and by the 'ls.sociated increase in the loc.al subsonic velocity. QQ.
oX
-:
274
'·m
PI. I. Theory. Aerodynemics of en Airfoil end eWing
M_.,r
'-'
I .
a., I.a
a.8
I:---r-
0.7
0.6 Flg.7.:U A Khristianovich curve for determining .the crHical ~18ch number
a.5 M
-0.5 -'.'0 -,.~ Jii(.nri~
....rodynamlc Coefficients
Khristianovich's investigations made it possible to obtain more accurate relations for the lift and moment r.oefticients than relations (7.1.1'1) found on tlle basis of the Prandtl-Glauert formula for the pressure coefficient. These relations are as follows:
clIa=cy.lcL/V1-M!o;
ml:a=m%alcL2/V1-M!.,
(7.2.7)
where
L = 1-f- O.05M;'1 M!."
cr
Compressibility changes the position of the centre of pressure of an airfoil (the coordinate xp of this centre is measnred from the leading edge along the chord). It follows from (7.2.7) that in a compressible flow, the coefficient of the centre of pressure is (7.2.8) where Cp = xplb = -m 2/c!la' c".ie = -m'alc/cYalC
Examination of (7.2.8) reveals that the centre of pressure in a compreS!>ible flow ill c.omparisoll with an incompressible one is displaced toward the trailing edge. This is explained by the increase in the aerodynamic load on the tail sections of an airfoil at increased flow speech; and. as a consequenc.e, by the appearance of an additional stabilizing effect.
7.3. Flow at Supercrifical Velocity oYer an Airfoil (Moo>,ll"",cr)
Sn bsonic flow over an airfoil can be characterized by two cases. In the flrsl one, the local velocity of the flow on a surface does not exceed the speed of sound anywhere. This case is purely subsonic
Ch. 7. An Airfoil in • Compressible Flow
271!.
~~\~'~i~ flow over an airfoil at a supercritical ve1ocill': ,,-diagram or H," Row U5('d ror ealculllli("'~ ,,'hN' • local norlllal shuck Is p",~nl; bdi~lrfb"li"n 01 Ilw Jlrcssuro' ov .. r Ihr llirl"iI wb"n II local }.'$hap ~ PI~l (1-\'o)d. < < iVCF• lI • The pr(':-;surc in the region abovc line CF will he greater than in that helow it. A pressure jump rannol be rehlill('(1 on a houndary i'lll'fac(' in
11
gas flow. althouglt the velodties may remain different. Tllerefore, itl real conditioll~. the diredion of :o.trPHmlinc CF differ.~ from that of the free-stream velocity. i.t'. a downwash of thc flow forms behind the pl Ph .=-: /JOC.b on the bottom side- is (".~pouding \',ducs of !he }-,'(q",,/,) :1ud cx" . Xa'(q",).)·
r" .-
Intro("\ioll of the shock and the characteristic. Downstream. cHrving of the shock is due to its intt'l"
Hypersonic Flow over a Thin Airfoil
U a thin sharp-nosed airfoil (sec Fig. 7.5.1) is in n hypersonic flow at such small angles of attack that the local :\.fach numbers on its upper and bottom surfaces at all points c~onsi,snre on a thin eirfoil in a nearly uniform flow. The aecuron! of these calculations can be increased by usillg lhe second-order aerodynamic theory. Ac('ording to the lattPl', the pressure coeRicient is (7.5.21) where C1
= 2(M!, -
1)-I/z.
C2
=
0.5 (JU;'" -
1)-~
[(;11;" - 2)2
+ kIlI!:.1 (7.5.22)
The pIllS sign in (7.5.21) relatcs 10 the bottorl1 ..,ide of the plate CPL; 0 "-~ a - ~iJ, and the minus Sig:ll, to the upper one (PN.; e = ~,,- ~N)'
Aerodynamic Forces and Their Coetllclents
To determine tile llerodYllflmic prc!;!;urc forcos. we sha! I use formulaa (1.3.2) and (1.3.3), relating them to the body axes x, y (seo Fig. 7.5.1) and assuming that c,.x ,--- O. In this condition, formula (1.3.2) determine.., the 10llgitudinal force X for an airfoil. and (1.3.3), the normal force Y produced by the pressuro:
X = q",,8 r
.~ (5)
peos (n",'x)
ff-,
Y = - q«>Sr \ (8)
pcos (~:y)-¥r
294
pt. I. Theory. Aerodynamics 01 an AIrfoil and eWing
Flg.7.U
Aerodynamic forces for an airfoil in a body axil and flight path coordinate systems
Adopting the quantity S r = b X 1 as the characteristic area and taking into account that dS = dl X 1 (b is the chord of the airfoil, and dl is an arc element of the contour), we obtain the following expressions for tho aerodynamic coefficients: XI(q..,Sr)
Cx =
=
c, ~YI(q~Sc)~
~ peas (h,i> dT.
-fiicos (,;','y)
dT
where dt = dUb, while the cllrvilinear integrals are taken along the contour of the airfoil (counterclockwise circumvention of the contour is usually taken as positi vel. Let us introduce ...............
-
into
-
this
-
-
expression dl = dx/sin
/'-. x),
(fl,
-
cos (n, y) dl -= dx, where dx = dx/b. Next passing over from curvilinear integrals to ordinary ones, we obtain 1
1
c,~ -.i Pb (*)b dx + Jp" (*)"dx o
1
(7.5.23)
"
j (Pb-pJdz
(7.5.24) o where Ph and Pu are the pressure coefficients for the bottom and upper sides of the airfoil, respectively. Using the formula for con version [see formula (1.2.3) and Table 1.2.11, we obtain the aerodynamic coefficients in a wind (flight path) coordinate sy.< = Cr cos! it, = cos! x, m~,;( = m~ COS·" (7.6.3)
C",.
C,
Evidently. by (7.5.25'), we have c~a'" =
(c:c
+ c,a) cos! " = crr, cos
2
x
Since the drag force is determined not in the direction of the velocity component V"" cos x, but in the direction of the free-stream velocity V... , the coellicient of this drag is
c:c:;( = c~a"
COS" =
c:c. cosS "
(7.6.4)
All these coellicients arc determined for a velocity head of q"" = = O.5p""P"". Inspection of formulas (7.6.3) for c,.,. and mz,l< reveals that the coefficient of the centre of pressure c p = -m,.,./c,.y' corresponding to small angles of attack does not depend on the angle of attack, i.e. C p = -m~/c/l' Compressible Flow. According to the linearized theory, the pressure coefficient for the airfoil of a sideslipping wing in a subsontc compressible flow can be obtained from the corresponding coe1licient for the same '.... ing in an incompressible flllid by the Prandtl-Glauert formula (7.1.14), substituting the number Moo cos x for Moo in it:
p,.=P",teIV1-M!.cos2x
(7.6.5)
or, with a view to (7.6.2)
p,.
=
Pic cos
2
xlVi
M:" cos2 it
(7.6.5')
The relevant aerodynamic coefficients are obtained from (7.5.23). (7.5.24), and fI.5.26), and are found with the aid of formulas (7.6.3)
Ch. 7. An Airfoil in .. Compressible Flow
:~ (M""~~W':~--V_:_;___ i",
303
(b)
~
'iC-Si,2-,u_
~i~~:itp'Ping
wing with slIhsonic (a) and supersonic (b) leadintt c(lgros
and
(7.5.4) whose right-hand sides contain the qnantity Vi M!o cos2 x in the denominaLor. Particularly. the coerricieillsof the normal force and the longiludinal moment. are Cll.~ =cu cos2.xf1/1
M:" cos2.x; m1 , >! = rn; cos2.;;JV 1-· M~ cos:! % (7.6.6)
It follows from t.hese relations that for thin airfoils, the coeITicient of the centre or pressure c p = -m 1 ,)I,lcy,)I, depends neither on the sideslip (sweep) angle nor on tho eomprr.ssihility (the number ill ",,). The usc of a sideslipping wing produces the same flow efT('ct that appears when the frcc-stream velocity is lowered from F to V ... cos x (or the Mnch number from M ... to M"" cos Yo). HC're, Ilalurally. the local velocities on an airfoil or the shlcslipping wing also decrease, and this, in turn. le8tls to diminishing of tho rarl'r;lction and. as n result-. to an increase in the critical Milch nnmber. The Jatter call be dc.termined from its ]mown v31ue JH eo C r for a straight wing of the same shape and flngle of aLtack as 11m airfoil of Ill(' sideslipping wing in a normal seclion:
Moo cr,"
= M ... cr/cos'fl. x
(i.G.7)
Supersonic Velocities. Let us llSl'umc that aL a ~upcr!'=ollie frcestream velocity (V ... > a .... Moo> 1), tbe sweep angle satislips the inequality )t > n/2 - ..... , according to which cos x < sin 1-1"" and, consequently. Vn"" < a,., = V"" sin ]l ... , Le. the normal component to the leading edge is subsonic. lIence. the flow over the seclious of a sideslipping wing is subsonic in its nature. In the case beiug considered. the swept edge is called suhsonic (Fig. 7.6.1a). At increased Dow veloeitie!'=. the normal velocily component may become higher than the speed of sound (Vn... > a ... = V"" sin 1-1 ....). so that x < n/2 - 1-' ... and cos x > sin 1-'00' In this case, the Dow
304
Pt. I. Theory. Aerodynamics 01 an Airfoil and a Wing
over the airfoils of a sideslipping wing is supersonic. Accordingly, the leading edge of such a wing is called supersonic (Fig. 1.6.4b). Let us consider the calculation of the supersonic Dow over a sideslipping wing in each of these cases. Supersonic Leadlng Edge. The Dow over such a wing can be calculated by the formulas obtained for an infinite-span thin plate provided that the free-stream velocity is V n"" = V"" cos x > a"", and the corresponding number M 0. "" = M "" cos x > t. The angle of attack of the plate aD is related to the given angle of attack a of the Sideslipping wing by expression (7.6.1). or at small angles of attack by (7.6.1'). Using formula (7.4.9) and substituting aD. = a/cos x for ~ and MD"" = M "" cos x for M "" in it. we obtain a relation for the pressure coofficient in a plane perpendicular to the leading edge:
j;-I± 2a/(eosjx V M'.eos'x-I) In this formula. the pressure coefficient Ii is rolated to the velocity hoad qn = O.5kp....M1D oo. To obtain the value of the pressure coefficiont rolated to the froe-stream volocity head q"" = O.5kp...,M1"", we must use formula (7.6.2) according to which p,. _ ± 2a eoslxtV M"':'-:Cco:-:s"'.c-'I (7.6.8) In (7.6.8). the plus sign determines the pressure coefficient for the bottom sido of a wing. and the minus sign for the upper side. In accordanco with formulas (7.4.20)-(7.4.22) (replacing a with aD and M ... with M"" cos x in them). and also with a view to relations (7.6.3) and (7.6.4). wo find a rolation for the aerodynamic coefficients of a sideslipping wing airfoil cll
.,.= 4(111 cos2 x/V M!,cos:l.x-1
C=.1C=
4a.~cossx/VM!. cos2 x-1
') (7.6.9)
m"a>l= -2a"coszy'/V M!,cos 2 x-1 Upon analysing these relations. we can establish a feature of swopt wings consisting in that in comparison with straight ones (x = 0). the lift force and drag coefficients, and also the coelliciont of the longitudinal moment of airfoils (in tlteir magnitude) are smaller at identical angles of attack an along a normal to the leading edge. The physical explanation is that in now over a Sideslipping wing Dot tho total volocity head g... = 0.5p ... V!. is realized, but only a part of it. gO. = g ... cos2 x, and flow in the direction of the oncoming stream occurs at a smallor angle of attack than in the absonce of sideslip (a < an. aa = a/cos x). Subsonic Leading Edge. The Dow over sections (',orresponding to the motion or a straight wing with the number Mn_ < 1 is investi-
Ch, 7. An Airfoil in
II
Compressible Flow
305
gated with tlle aid of the subsonic or transonic (combined) theory of flow over an airfoil. The drag and lift forceg arc determined by the laws of subsonic flows cllar;lcterizcd by interaction of the flows on the upper and bottom sides of a wing that manifest.s itself in thE! gas flowing ovcr from a region of lligll pressure into a zone \\'itll reduced pressure values, V\'U\'C losses may appear olily in sllpcrcritical flow (Mno > M «> cr) when shocks form on the surface, If M" '" < lW 00 c r, then shocks and, therefore, \\'ave drag are absent. This conclusion relates to an inlinite-span wing, For lillite-span wings, wave losses are always prescnt because flow O\'er their tips is allccted by the velocity component V sin %, A result is the appearance of supersonic flow properties and of a wayc drag, The three-dimcnsional theory of supersonic flow has to be llsed to study this drag. 00
Suction Force
As we have established in Sec. 6.3, a ~mctioll force appears on the leading edge of an airfoil over which an incompressible fluid is flowing. The same effect occllrs when an airfoil is in It subsonic flow of a compressible gas. The magnitude of tile snction force is affected by the sweep of the leading edge of the wing. To calculate this force, we shall use expression (o.il.25), which by meallS of the corresponding transformations can be made to cover the more general case of the tlow over an airfoil of a wing \vith a swept leading edge (Fig. 7.6.5). Let us consider this transformation. In au iu\'iscid flow, the free-stream velocity component tangent to the leading edge of a sideslipping wing docs )lot change the Iield of the disturbed velocitics, and it remains the sume as for a straight wing in a l10w at the velochY V n "" ,.., V"" cos %. The forces acting on the wing also remain unchanged. Therefore, the following suet ion force acts on a wing element dz o with a straight edge (in the coordinates .1'0' zo): dl'o = ;tpc! dz o (7.G.1D) where in accordance with (6.3.28') c~= lim lu:(xo-x~.eo)l Xo-Xs .eo
A glance at Fig. 7.6.3 reveals that dT o = dT/cos = u/cos~, and Xo - Xs.eo = (x- x~.e) cos ~. Insertion of these values into (7.6.10) yields
~,
dz o = dz/cos
~,
Uo
dT/dz=npc:z.V1-i- tan:z.x
(7.().ll)
c:z.,._", lim fu 2 (x-xs,e}J
(7.().12)
where Z-X s . r 20-01715
FIg. 7.6.5
Suction force of a sidellipping wing
Expressions (7.6.11) and (7.6.12) can be generalized for compressible Dows. For this purpose, we shall use expressions (8.2.4) relating the geometric characteristics of wings in a compressible and an incompressible Dows. It follows from these relations that all the linear dimensions in the direction of the x-axis for a wing in a compressible Dow are 'V 1 - M!, limes smaller than the relevant dimensions for a wing in an incompressible Dow. whereas the thickness of the wing and its lateral dimensions (in the direction of the z-axis) do not change. Accordingly. we have
x=xlc'Vl-M!... bdz=b1c dz 1C 'V1-M!, tanx=tanx!c'V1-M;' From the conditions that x find
= XIC 'V 1 -
M~ and
(aq>'iiiy), __o
(8.1.15)
in which the left-hand side corresponds to the velocity Vn directly above the vortex sheet (y = +0), and the right-hand side, to the velocity under it (y = -0). Hence, condition (8.1.15) expresses the continuity of the function orr-'lfJy when passing through a vortex sheet. In addition, the condition of the continuity of the pressure is satisfied on a vortex sheet. According to (7.1.5'), we obtain the relation (8.1.16) that also expresses the continuity of the partial derivative fJcp'18x when passing through a vortex sheet. Let us consider the fiow over a wing with a symmetric airfoil (yu = -Yb) at a zero angle of attack. In this case, there is no lift force and. consequently, no vortex sheet. Owing to the wing being symmetric, the vertical components of the velocity on its upper and bottom sides are equal in magnitude and opposite in sign, i.e. v (x, +y, z) = -v (x, -Y, z). On plane :cOz outside the wing, the component v = 0, therefore a~'liiy ~ 0 (8.1.t7) Let us assume further that we have a zero-thickness wing of the same planform in a flow at a small angle of attack. The equation of the wing's surface is y = f (x, z). A glance at (8.1.12) reveals that the vertical velocity components Vn = 8cp'/oy on the upper and bottom sides of the wing are identical at corresponding points. Since we arc dealing with a sufficiently small angle of attack of the wing, the same condition can be related to the plane y = O. At the same time, such a condition can be extended to the vortex sheet bebin" the wing, which is conSidered as a continuation of the vortices in the plane y = O. Therefore, at points symmetric about this plane, the
Ch. 8, A Wing in
at a zero angle of attack and 11 given concavity of a wing. A lift force due to the angl!' of at.lack is p~oduced by wing 4- and, therefore, depends on the planform of the wlIlg.
The iindillg of tile pressure distribution, the resultant forces, and the releyant aerodynamic coefficients with a ,'ie\\, to their possible resolution into components according to formulas (8.1.27) and (8.1.29) is the basic problem of the aerodynamiCS o[ a finite-span wing in a nt'ariy uniform supersonic now. Features 01 Supersonic Flow over Wings
When determining the aerodynamic characteristics of wings, we mnst t.ake acconnl of the features of the supersonic flow over them. These features are due to the specifiC property of supersonic flo\\'s in which the disturbancps propagate only downstream and within tile con(ines of a disturbance (Mach) cone with all apex angle of f-l "" = sin -l (1/Jl1 00)' Let us consider a supersonic flow oyer a thin wing having an arbitrary plan form (Fig. 8.1.3). Point 0 on the leading edge is a source of disturbance!' propagating dow.nslream within the conlines of a Mach cone. The Macll lines OF and OG are both ahead of tile leading edges
318
Pt. I. Theory, Aerodynamics of an Airfoil and a Wing
Supersollic flow over n wing: G-wlng with subsonic
rdgr~;
b- wing with
sll~l'$onlc
cdg\"s
(Fig. 8.1.3a) and behind them Wig. 8.1.3b). The arrangement of the Mach Jines at a given wing planform depends on the number M .... In the Jirst case, the nnmbcr M ... is smaller than in the second one, and the angle of inclination of the Mach line ""OIl > nl2 - x (x is the sweep angle). The normal velocity component to the leading eelge is Vn ... =V""cosx. Since cosx<sin 11 ... = 11M"" and V OIl/a ... = = M ... , the normal component V n... is evidently smaller than the speed of sound. The flow of a gas in the region of the leading edge of a swept wing for this case was considered in Sec. 7.6. This flow corresponds to the sllbsonic flow over an airfoil that is characterized by interaction between the upper and bottom surfaces occurring through the Jearling edge. Such a leading edge is called 8ubsonic (Fig. 8.U.). Upon an increase in the now velocity, wben the tone of disturbance propagat.ion narrows and the Mach lines are behind the leading edges as shown in Fig. 8.1.3b, the normnl velocity component becomes supersonic. Indeed, examination of Fig. 8.1.3b reveills that the angle of inclination of the Mach line /1 ... < rr./2 - 1(, bence sin ~ ... = = 11M ... < cos Y., anti therefore V n_ = V a-. Such a leading edge ucalled 8uperBonic. The now over airfoils in the region of the leading edge is of a ~upersonie nature whose feature is the ab~ence of interaction between the hottom and the \lpper surfaces. If the l-loch line coincides with the leading edge (x = ';[/2 - ~ ... ), such an edge is sonic. It is quite evident that in thiscilse the magnitude of the normal velocity componen t to the edge equall'! the speed of sound. Let us introduce the leading edge sweep paralllf'!ter n :"'- tan xl Icot /1 .... For a supersonic. Jeading edge, cot ~l"" > tan x, therefore
Ch. 8. A Wing in a Supersonic Flow
317
1. For suhsonic. and SOllie lending edges. we have n > 1 and It -= 1. respectively. hecause! in the first rase rot !J."" < tan x and in the second one rot J.l "" -- tan x. By analogy with thli' J(lading edges, we can inlrodllce Ihe ronrept n
rsollie lips (side edgcs) and trailing edges of a wing, Tip CD wilh all allale of illclinaion Vt to the direclion of the free-stream relocity smaller tlutn the Mach anale (Fig. 8.1.3a) ig called subsonic. The velorilycompollent normal to a lip CInd equal to = l' "" sin Vt is lower thnn the speed of SOl1nd ill the giYen case. Indeed. sincu a x ,V .'>in p"" nnd Pox» Vt. we ha\'c Vn < a"". It is ohvious that the leading edge sweep parameter II > 1. The part of the wing surface with a sllhsonic tip is inside !.he region cut ()[( by the 1I.-[ach rones is.'-~1
s
This expression i~ similar to (8.3.6) with the djfference that the coordinate zJ is taken as the upper limit of the integraL By calculating tlte derivative UIfJ'/ux and integraLillg, we obtain relation (8.3.9) for the component of the additional velocity. We must assume in it that cr < 0 because the coordinatezN is negath. e. In calculations, the coordinate ZN may be assumed to be positive, and, consequently, 0> O. If we take the magnitudGS of tan x, then to determine the
Ch. 8. A Wing in
f~'riu~~~
oBI
Supersonic Flow
S2ij
"
of sources on the velocity oulside a wing
induced ... clority we may use Eq. (H.3J) in whidl 0 ~hoilltl he taken with the opposite sign. The \vorking relalion 1I0W be('ome;o. We lISC thc value of this vclocity to fllld the pressurc coeflidcnt:
p= - ;:
=
;1'];'
:~
cosh- t
:Ita--:.at)
(8.3.17)
Figurc 8.3.4 shows the ficld of pressur('. a>
L
U.
:1(1.·yn~-l
eosh- 1 1/r 1I~-1
r
0 1 -1
(8.3.21)
328
Pt. I. Theory. Aerodynllmics 01 lin Airfoil lind
II
Wing
Seml·lnfinPe Wing with • Supersonic Edge
For such a wing (Fig. 8.3.6), Mach line OK issuing from a vertex is on its surface. Consequently,
n/2-x>ll.." taox and take absolute values for n, the additional \'clocity is u=
-
:let'
~~; __ II:
COS-I l"t,"':"'..(JO)
(8.3.3!)
and the pressure coefficient is
p= - ~:
= na'
~
cos- J
:'tl_':_(J(J)
(8.3.32)
The pressure field for a semi-infinite triangular wing with a supersonic leading edge is shown ill Fig. 8.3.7. Between the leading edge and the internal Mach line, the pressure is constant, then it lowers, and on the external l\-lach line reaches the value of the free-stream pressure (jj = 0). TrlaJtlulu WIng 5,......rfc about the ,x.AliI with Supenonlc LeitClllJtl Edges
The velocity and the pressure coefficient at point L (Fig. 8.3.8) between !\lach wave OK and the leading edge are determined by formulas (8.3.22) and (8.3.23), respectively, because the now at this point is affected only by edge OR. These formulas may be applied for the conditiolls n < 1 and 1 > (J > n.
Ch. 8. A Wing in " Supersonic Flow
331
Fig. 8.].8
Triangular winq symmetric about thl' .r-axis with Supl,!f$onic leading etlges: J-/lfacll hrw: 2-mnximuln thickness I",,,
The v('locity
(lzil
80';:~\~A,:;~~n ~2
__
CO.~h-1
)
V :~=! . ~~2
(8.4.5)
°:oG
where 0"2H and 02G are cvaluated relative to point II.
Slimming (8.4.3) and (S.Ll) and tnking into account that 0IP'"""' z,
02G = :, 1;(:
%2
~~~x' "-'
c-,-, L
om
tan 11.", tan )(2
-=
_~
III t;:X\
== X:~~:~l~'XI
I";.XB =~,
(J~H"""
z. ;; x~ = 1
we obt~in Cx, }'H
-= Cx, Fe: ·rex. all II tlln)(l
.Tn+71 tlln )(2
8J·fz, tall XI
b:ta'
Xd:r, Let us
Ylli--l
r
~
,
coc;h-I
'V '~i-=-;.f
--
8(A:.'1-:~!~n)(1) casICt}/'" :~=~
a~ that ;,' A~. u "3' illHI (1 (1:1' Silmmilig 1I1(' pre:-sllrc coefficients due to all three soul'ce disll'iblltiolls, we obtnill
n.
Poll =, •
yeos
4AI
:w;' y'1I~-1
h-I"/
V
cosh-!
V" 1'11-
(Iii -t (11
~ ().,~-).,1)
"o;t' ~
n~-fJi .!i).,l 1-1"'/"'iii'=T t_()'I-l'1a,~cosl V 0:-1
8411
( ••
)
336
Pt. I. Theory. Aerodynlmics of an Airfoil and a Wing
where n:') = tan ;(:,)/(1.': the values of 01' 02, and 0, are calculated nllative to points O. Band D. Introducing the value of P-;L into formula (8.4.2) and substituting A!! for AI in it, we obtain _
cr ,
JL = -
r
:r~~:~
(/IL
(1-
~;n~
•
d:~l
~I ~1::a~; . ~~'
oosh-(
'u
+ ;. V:J)(~l
V ~~I1~t
--
j
1
__
COJlh- 1
',J
'IL
t~n;; n~
r (1
j
',L
__
)" COSh-I V =:=: .d;.a J
(8.4.12)
',J
Summing (8.4.10) and (8.4.12). we have _
[
!:~. HL= - :t.~:I,
(/IL
(I
_~n~
j ',"
(/2L
r(1
__
cosh- t
V ~f~:l- da;1
,/_. __ •
)
t~;~ co.~h-I V ~'-=-:i' ~2 ',L '," __
+ ;. ~~ J cosh-t V :i=! .~ ]
(8.4.13)
'oJ
In this expression 'I tanK 1 • (t-;:)bO+.31 tanxa
0'2H-1, C13J=
1:1
x,
rbo~::~:~xa
0'2L
tan X, zj
0'11a= ~l bO+=1 tan
I
=n,.
0'3L=
SI
tan x,
zi,
I }
=
1.
(8.4.13')
where xJ = Zt cot fl ... = ZI(1.'. and xi, = Zt tan )(3' We take the integrals in formulas (8.4.8) and (8.4.13) by parts. These formulas hold (see Fig. 8.4.1) when (8.4.14)
where zlh
=
(1 - r) bo/(tan
Xl -
ex'}.
Zo.
= rbJ(tan
X2 -
a') (8.4.15)
Ch. 8. A Wing in a Supeunnic Flow
SS7
or (Fig. 8.4.2) when (8.1.16) The drag cocfficicnt of th(' airfoil dctcrmined by formula (8.4.13) has been relntcd to the local chord 1,. We calculatc the value or the drag ('oellicicnt. Cx.o relatcd to t1l(' rcntral cliord lIo by thf' fornmln C:l',fI = C:r: (blb o)· Airfoil in the :\1id-Span Section (z = 0). We determine the \'alucs of the aerodynamic coefficients for this airfoil ns 10110\\,5. 011 nirfoil sec·tion OB (sec Fig. 8.4.1) with a 1f'ngth of (1 - ii boo thc "clarity is indllr.ed hy ~ollrc.es having' i1 strcngth of Q.-, 2i'Il"." distrihutrd in trianglc Accordinglr. we evaluatE' the pressure coerti~~i,Z\~:tKI1 ,\
--
cosh-I
"1F t
8().::~t~n}(2
-
•
"2H1
.\'
V '~'-='a~~' (~att
V ~:=: .d:i~ --
cOsh-I
(SA.21)
"21'1
where 0"1 and 0"2 nicient c.",,",!., from expression (8,4.-13) in which we replace the limits 0ln and <JIL with the quantities <J1H, and O"IL" the limits 0"2H and 0"21, wilh the quanLities 0"2H, and 0"21.., and the limits 0"3.1 and 0"31. with the quantities 0"3J, and <JJL" respectively. determined by formulas (8.4.13'). The overlween points D. and B. (Fig. 8.4.2) with the coordinate ZI satisfying the inequality zD, < < Zt < Zn,. The flow over this airfoil is of a more intricate nature. The velocity on section F 2G2 is indneed by sources having the strength Q ,.-.:: 21l, V distributed in triangle OCC'. Consequently, the pressure coefficient on this section is determined with the aid of formula (8.4.1), and the corresponding drag coeITieient Cx • l'-.G, from expressioD (8.4.3) in which the integral is taken between the limits O"IF , and OIG,. 00
Ch. 8. A Wing in e Supersonic Flow
aag
The pressure OIL scction G2.H z depends on the influencc of sources having a strength of Q -"- 21..1 Y 00 distributeel oyer section OCC', and also of sonrces having a strength of Q = 2 (Az - 1..\) Y 00 in region BCG'. Conseql1ently. we cakulHte the pressure roeITicient by formula (8.4.4), and the drag coefficient c,\:. ("H, from ('xpre.!'sion (8.4.:)) in whkh we take the first inlrgral hetween the limits OIG, anti OtH,. an(l the second between (J~G and O"~II • Section II zJ2. experiellrcs'lhc si~ultaneolls actiou of sources distrillllted in region OCC' (Q . . , 2"11"00), and also in triangle RCC' IQ --: 2 (A2 - AI) Fool and 011 sl1rfflre [JCC', where the strength Q = = -2A21'oo. The first. distribution re!'.lIils in a pressure coefficient determined by formula (8.:tHl), alill thr se('ond two distributions resulL in the roefiicienl calcl11ated by expression (8.3.21). The total vallie of the pressure coerfLcient 011 this section of the airfoil is PHzJz
,
~
:vx'
1-1
',COSI
~;:ti-1
c05h- 1 1-/
'~i~:/ .~ .1~/'~-;:;·~1
1.~.2 :t~' l/n~-1
/III=T J; o~-I -
]-1' /
COSI
V
n:f= I
(J~-I
(8422) ..
where 01' 02' and 0"3 arc determined relative to points 0, 8, and D, respectively. By using the formula
') Xft _
C.", 112J, =
i;:.\
P1I2J2AZ
dx
(8.4.23)
'H,
we can calculate the drag coefficient ror lhe sectioll of the airfoil being considered relate!l to the length bo of the centre chord. The flow over the last airroil sect-ion J 2L'J is the result of indllction by the sources distribnted in tlte sallle regions of the wing as for airfoil section II ~J~. lIere accouut must be taken of the feature that the velocity induced by the sources in region ReG' is determined by formula (8.3.1R), where A is replaced by the ,",ngular coefficient A~ - At. Therefore, the pressure coefficient should be calculated by formula (8.4.11). and the drag cocrncient ex, J,I .• trom expression (8/1.12) in which we take the integrals between the limits onJ, and (Jnl., (n = 1, 2, :~). We obtain the total drag coefficient by summation of the coeffi~ dents for all four sections of the airfoil: ex.
F,L,
= ex, F.G,
provided that the value of tao
+ cx. G,H, -!- ex .II,J, + c:t, J.l. Zt
satisfies the inequality
~~O_ct' < Z1 < t~~-;:~b~,
340
Pt. I. Theory. Aerodynamics 01 an Airfoil arld a Wirl9
Airroil FaLa. Let us consider seclion F3La (Fig. 8.4.2) with the coordinate Zl satisfying the inequality (8.4.24) where (8.4.25) Tho pressure on section F aJ a of tho airfoil is due to the action of sources distributed on the triangular surfaces OCC' (Q = 2A1 V .,.,) and BCC' lQ = 2 (All - A,) Vool. We shall therefore calculate the pressure coefficient by expression (8.4.4), and the drag coefficient by formula (8.4.5) in which we replace the limits all, G and an, H with the values On,!'. and on, J. (n = 1, 2). Airfoil section J 3H 3_ in addition to the indicated source distributions in regions OCC' and BCC', also experiences the action of sources having a strength of Q = -2A\I VL distributed in triangle DCC'. Consequently, the pressure coefficient equals the value calculated by formula (8.4.4) plus the additional value calculated by formula (8.3.21) in which we assume that A = -At. Flow over section H 3£3 is characterized by the induction of sources distributed in three regions of the wing, namely, OCC', BCC', and DCC'. Accordingly, the pressure coefflcient on this section should be calculated with the aid of formula (8.4.11). By calculating the relevant components of the drag coeflicient for all three SGctions and summing them, we obtain the total drag coefficient: c%:. F.r.. = C:c. P,J. C.'C.J.H. + C%:, H,I.. The relevant expression is suitable for calculating the drag coeffI~ cient of the airfoil between points DI and D2 (Fig 8.4.2) with the coordinate Zl that satisfies the inequality
+
tao
y.:;~~, < Zt
zD,
(8.4.27)
Three source distributions simultaneously act on this section, namely, OCC' (Q - 2~, V ~), BCC' [Q - 2 lA, - ~.) V ~l. and DCC' (Q = -2A2V ooJ. Airfoil section F,H, is behind Mach line OKo within the confIDes of the wing, therefore to calculate the pressure produced by the distribution of lhe sources in OCC' we must use formula (8.3.19) in which wo assume that A = AI' The second distribution of the sources in BCC' acts on section F ,H, located beyond the conilnes of the surface between the Mach line and edge BC. Therefore, to calculate the additional pressure dlle to the influence of the distribution of the sources in BCC'. we must use formula (8.3.2t) with the substitution of At - A)' for A..
Ch. 8. A Wing in a Supersonic Flow
a41
Fi,.8.4.3
Distribution of the drag coerrl-
~~~~a~~e~h~hred S~~~g o~\"i~hs~~~~ sonic edges (tbr dasbeLl
Un~
sholl's an unswrJ,1
~·lng·
The second seclion of airfoil H4L~ is located within the confine., of the wing surface, i.e, at the same side from the Mach lines and the relevant edges OC and BC, Consequently, to determine the pre~~ure coefficient resulting from the dislribntions of the sources in OCC' and BCC', we use formula (8.3.19) in which the value A. = ;.., corresponds to the distribution in OCC', and the value A. = 1.2 - Al to the distribution in BCG'. Section H4L4 is at both sides of Mach line DKo and trailing edge DC, Le. it is beyond the contines of triangular surface DCC' where the strength of the sources is Q = -2A. 2 V"". Hence, to calculate the pressure coefficient produced by these sources, we should use formula (8,3.21) with the substitution of -1.2 for A., Using the obtained value of the pressure coefficient, we can determine the relevant drag coefficient for airfoil F4L4: Figure 8.4.3 shows the results of calculating the distribution of the drag coefficient c:r/lJ.2 (3. = I1lb) over the span of a swept constant chord (b) wing (Xl = X, = X3 = 60°) with a symmetric rhombiform airfoil (r = 112) for M"" = 1.8 and 1.9. A glance at the figure reveals that with an increase in the distance from the centre chord, the drag coefflcient riist grows somewhat, and then sharply drops. For purposes of comparison, the figure shows the value of the func~ tion c,/ t;, for an airfoil belonging to an unswcpt wing. To determine the total drag coefficient of the wing, we must integrate the distribution of the drag coefficients Cx ." of the airfoils over the span, using the formula It'
cX
=7- Jc:r,,,dz
(8.4.28)
342
Pt. I. Theory. Aerodynemics of en Airfoil end eWing
Influence of a Side Edge on the Flow over a Wing. If a wing has a wide tip or side edge (Fig. 8.4.4), its influence on the pressure distribution and the drag coefficient must be taken into account. The flow over such a hexagonal wing is calculated as follows. First the velocities and pressures in region 00' D' D produced by the distri· bution of the sources on triangular area OCD are calculated. The calculations in this case are performed similar to those of a wing with a tetragonal planform (see Fig. 8.4.1) having no side edges. Next the calculated velocities and pressures are determined more precisely with account taken of the influence of side edge O'C', which is oquivalent to the action of sources distributed in triangle O'CD'. The strength of these sources has a sign opposite to that of the sources corresponding to a wing of area O'CD'. The action of the sources distributed in triangle O'CD' extends to the wing within the area O'TnD' confined by Mach line 0' K', the side edge, and the trailing edge. For example, for airfoil F 2L21 the action of the sources is confmed by section F~L2 (point F~ is at the intersection of chord F2L2 and Mach line 0' K'). Let us see how the pressure is evaluated on section J 2L2 of this airfoil. Taking into consideration only the distribution of the sources in region OCC', we can determine the pressure coefficient by for· mula (8.4.11). We can introduce the correction IJ.p-for the action of sources of opposite signs in triangle O'CD', so that (8.4.29)
When fmding the correction IJ.p we must take account of the posi· tion of airfoil section J 2L2 relative to Mach line O~K; that passes through point 0; belonging to the opposite side edge (Fig. 8.4.4). If this line does not intersect J 2L2' the latter is influenced only by the distribution of the sources in region O'CD' of one side of the
a.
Ch.
A Wing in ~ SupersoniC Flow
343
wing. whereas the influence of the sources ill O;C'U; is excluded. The induced velocity is calcuh\led by formula (8.3.13), and the corresponding additional value of the pressure cocITieient b~' the formula !!.p = -2u/V .... We shall write this a(lditional nlluf' in the form of the slim (8.4.:l0) where !!.Pl depends on the distriblltion of the sources ill O'CC' (Q = 2"'1 V 00), while IlP2 and IlPa depend on the distribution of the sources in B'CC" IQ = 2 (!,~ - AI) v ... 1 and [)'CC~ (Q = -2"'21' ,.,). Hence, by using formula (8.a.14). we obtain
D.p=
.10:'
~::f-I
cosh-
l n;l~~~(f~I)
+ ~~~}.; ~;'l~ 1 cosh- n:'l;~_(f;~) t
_ :-(0;'
n~ )1"1-1
cosh-!
1I~·;-1]3 " 3 {1-i- 0 3)
(H.Io.:311
°
where 1, 02 and 03 arc calculated relative to points 0'. /J', and [)'. If Mach line O~K; intersel.'ts chord F2 L l • then simult.aneously with the action of sources 0' CC account must also be taken of th.e influence of t.he sources distributed in triangle O;C'C; at the opposite side of the wing. The same formula (8.:·U:~) is used to c~lc\llate tile induced velocity. N
B.S. Flow over a Tetragonal Symmetric Airloil Wing with Edges 01 Different Kinds (Subsonic and Supersonic I Leading and Middle Edges Are Subsonic T'llIing Edge Is Supersonic
The disturbances from the trailing supersonic edges of a wing (Fig. 8.5.1a) propagate downstream \\'ithin the confines of the Mach cone with the g(lneratrix DKD and therefore do not affect the flow ovor the wing surface. The velocities and pressures depend on the influence of the leading and middle subsonic edges. Let us consider profile FL with the coordinate ZI < 200,. The pressure coefficient on section FC, which depends on the action of sources having a strengtll of Q = 2"'lV.... that are distributed in triangle OCC'. is determined from (8.4.1). and the corresponding drag coefficient c"'. n. from (8.4.3). On t.he following section GH experiencing the influence of the sources distributed in triallgles OCC' (Q = 21.1 V..,) and BCC' IQ..." 2 ("'2 - AI) V .... 1. the pressure
344
Pt. I. Theory. Aerodynamics of an Airfoil a"d a Wing
«)
(h)
Fig. '.S.t
Tetragonal wing in a supersonic Dow:
rng~h:.!cr;d~L:~rc.u:t~::I~:f:~:~t~lm~l~i~e a~a!~~~~~;I:~~\1~~1':'a~es~~
Ionic
coefficient is calculated by (8.4.4). The con'esponding value of the drag coefficient c~. GH for this section is determined from (8.4.5). The action of the same source distributions is observed on section HL as on section GH. But taking into account that section HL is below Mach line BKB (on the wing sudace), the pressure coefficient PHI. must be calculated from (8.4.9). and the drag coefficient C~, HL. from (8.4.10). The total drag coefficient of the aidoil is c~, FL = cjC, PO c~, GH c~, HL (8.5.t)
+
+
When considering section FILl with the coordinate %1 > %8,. account must be taken simultaneously of the source distributions in OCC' and BCC'. For section FlHl • the drag coefficient c~, P,H, is determined by formula (8.4,21). For section H1L" the drag coeffieient Cit, H,L, is found by expression (8.4.13) in which the third term in the brackets is taken equal to zero, while the limits Gn.H and a p ,1,
Ch. 8. A Wing in a Supersonic. Flow
34lS
are replaced with the values Gn, H, and Gn, L,(n = 1,2), respectively. The total drag coefficient for airfoil FlLI is (8.5.2) Leading Edge Is Subsonic, Middle and Trailing Edges lire Supersonic
A feature of the flow over the wing (Fig. 8.5.1b) consists in that the sources distributed in region BDD t do not affect the distribution of the velocities and pressures on the remaining part of the wing above Mach line BK D• Let us considor airfoil F L with the coordinate Xl < ZD,. Section FH of this airfoil is acted upon hy the sources distributed in triallglo OCC' (Fig. 8.5.ia); consequently. the pressure distribution can bu found from (8.4.1), and the corresponding drag coefficient C:E.l in drug {unction I, by Tormuln (8.5.t6) saliant point corresponds to the tl'ansformalion of the I.railing edge,. and til(! second. of the leading edge into a sonic one.
8.6_ Field of Application of the Source Method The method of sources, as we already know. is used to calculatu· the flow in order to fmd the drag forc~ of a wing with a symmetric Airfoil at a zero angle 0/ aUack, i.e. in the absence of a lift force. In,,-e1ltigations reveal that the fiCld of application or this metilOu ill ap.rodynamic research call be extended. Let \loS consider case::; when the method of sources can be used to determin0 a nearly uniform flow over a thin wing at u non-zero angle of attack, and we CMI thus lind the lift force in addition to the drag. Let us take two wings with different leading edges. One of them lias a curved edge wi til a nnite sllpersonic section (Fig. 0.Li.l), while the other has completely subsonic leading edges (Fig. 8.6.2). In Fig. 8.6.1, the supersonic section is bounded I;y points E and t'r at which a tangent to the contour coillcides with the genera trices of the Mach cones. Let us con~ider tlw velocily potential at a point .H in the region confined by euge!; ED and the Mach lines dmwn in plane xOz from points E, J), (Jr, and E'. By formula (8.2.16) in which the integration region f'1 shouleJ bo taken equal to (J " - SI S~, the velOCity potential at the point being considered is
+
JJ y (~1 ('i):) d~z~~ t)2 --irt JJ V(Z~I(~)II;)~ld~
cp' = -
2~
5,
t;)i
5,
(8.6.1)
atl2
Pt. I. Theory. Aerodynamics of lin Airfoil and a Wing
~~~n;'~1tb
a finite section of a supel'3onic leading etlge
'F1,.I.6.l
Wlng witb subsonic leading
edges
In (S.6.1), the function Ql (x. z) = 2 (OI.p'!oY)II'-'o' This follows from (8.2.17). This function is determined from the condition of flow over the wing surface without separation (8.1.12). Since the equation of this surface is given, the function Ql (x. z) is known. In the particular case of a wing in the form of a plate in a flow at the angle of attack IX, the function Ql = 2V""IX. Hence, the determination of !p' by formula (8.6.1) is associated with the finding of the unknown function Q2 determining the intensity of sonrce distribution on section S •. To find this function Q" let us take an arbitrary point N (x 0, z) in the region between the Mach lines issuing from points E and D . At this point, according to (8.1.20). the velocit}' potential is zero, therefore in accordance with the notation (sec Fig. 8.6.1), we have t
0= -
it- JJ y' (~I (ti);) d~J:~~ S,
+ -it .\ .f -V (~2 (~t)a~) ~~ ~)1 S,
t)! -
(R.6.2)
Ch. 8. A Wing in " Super~onic Flow
3~3
The ftrst term on the right-hand side of this int.egral equation is a known function of the coordinates of a point because the strength Q1 on area S3 has been determinerl from the boundary conditions. We can therefore use the equation to determine the unknown function Q~ that is the strength of the sources in region 8 4 , Hence, if the leading edge of a symmetric airfoil wing is completely or partly supersonic, the metlwd of sources is suitable for investigating tM flow over tM wing at a non-zero angle of attack. The same conclusion evidently also relates to a wing with similar edges and a nonsymmetric airfoil in a Gow either at the angle 0: =#:0 or at ct = O. I\ow let us consider a wing with subsonic leading edges. We can derive the following relation for a similar point N (Fig. 8.6.2):
0= -
2~
.\.\
s,
y(~3(~)2~)'~:ld~ I;l~
-
~ JJ 1/(~d~)2{:)~~~
1:)1
~-
(8.6.3) We have obtained an equation with two unknown functions Q, and Q2' Similar to Q2, the rnnction Q3 is the strength of the sources on area 8 s belonging to the region located between the left-hand leading edge and the Mach line issuing from the wing vertex. Hence, if a wing has a subsonic leadirl{! edge, the source method cannot be used to investigate the flow oeer a thin symmetric airfoil wing at an angle of attack, or the flow over a non-symmetric airfoil wing at a zero angle of attack or when 'J. =#: O. '.7. Doublet Distribution Method It has been establishod that the application or the source method for investigating supersouic flow is restricted to wings with completely or partly supersonic lending edges. In other cases associated with the investigation of the supe-rsonic aerodynamic characteristics of wings with subsonic leading edges wit.h a non-zero angle of attack (or of similar non-symmetric airfoil wings and at a = 0), the doublet distribution PlE:lbod mllst be llsed. Let us consider a doublet in a supersonic flow. To do this. we shall determine the velocity potential of the Dow produced by an elementary source and an elementary sink of the same strength Q having coordinates x = ;, z = t y = 8, and:x = ~,z = t. y = -e. respectively. The chosen source is located above the plane 11 = 0 at the small distance I:: from it, and the sink is under this plane at the same small distance -e. Expressing (8.2.11) as a differenceequation, we shall write the potential produced by the source and sink
354
Pt. I. Theory. Aerodynlmic5 of on Airfoil lind 0 Wing
in the form AI= 4nM ... E(k)
II a
dr ds VrA-r' VSA-S
(8.9.14)
Let us use Eq. (8.9.14) to determine the potential function at point A in region II that is conHned by the Mach lines issuing from points D and G, the tips, (side edges) and partly the trailing edges. We shall write Eq. (8.9.14) in the following form: q>II = B~'
~:;~~~k~)
rA
"A
rK
sD'
J vr~r_r J
Vs:S_s
(8_9_15)
analogy with (8.9.8): SB' =
TB,m = TAm
(8_9_16)
eh.
8. A Wing in e Supersonic Flow
869
Point K is on a tip whose equation is z = U2. In the coordinates rand s, the equation of a tip in accordance with (S.9.4W) is
r - S - -M .li2 Therefore, for point K, the coordinate is
(8.9.17)
rx - SK - M.li2 - SA - M.1I2 (8.9.18) Taking also into account that SB' = 'Am, after integration of (8.9.15) we obtain
fJI[I= 1X:;~~t:) J./[rA-(sA- M;')] (sA-rAm)
(8.9.19)
Introducing instead of rA, SA and m the relevant values from (8.9.4') and (8.9.10), we find
Til = I::~~)
V
n"';c,1'--(l---2-'-A)""("':"'~-T-'
-n-,."")'-
(8.9.20)
The velocity potential for point A in region III is ~A
r ..\
Till
~~:;::.;;;
J
II
"I('
r~r_r
I
l"s~:-$
(8.9.21)
'0'
Points K' and G' are on thn tips whose equations are z = ±1I2 (the plus sign is for the starb031'(1 find the minus sign is for the port tip). In the cooruinates r Vcoi2 is the \-elocity hea(I, anf!' S", is the> area of the wing planform.
3B2
pt. I. Theory. Aerodynllmics of lin Airfoil lind II Wing
~:. tt-:'~~leulation of the suc· tion force for a triangular wing with subsonic leading edgl!s To detarmine the force T, we can use tbe relations obtained in Sec. 7.6 for an infinite-span swept wing. This follows from the fact that in accordance with (7.6.18) and (7.6.19), the suction force depends on the change in the axial component of the velocity in the close vicinity of the leading edge of tile airfoil being considered, and also on the lOCK 1 sweep angle, and lloes not depend on the behaviour of this velocity far from the leading edge. t:sing (7.6.18), we obtain T-2:tp_ V Tl_7;.7'.=n"'''"x---;M''';''
'I" c'.!dz
(8.11.3)
where c is a coefficient determined from (7.6.19). Let liS determine the drag for a triangular wing. For this purpose, we shall lIse expression (8.8.39) for the disturbed volocity. Assuming that cot~ = z, xJ.e. we fi1ld
u where xJ.e is the
di~tallce
to the leading edge, z and x are the coor-
diI~i~~d~fci~:~i:~t :~u~h~f'~:rrn~:if7.g:1~)1~~d taking into
that
lim
c1
account
(xlxl.,) = 1. we have
r-%).e
=[ :~';,
r :c~~ll,.. ~:;:rl~;~~)~(~_~':'~:')
-+[ ;~~~
rzeotx
Introducing this expression into (7.6.18) and integrating. we find
T~ ~po.:'lt~ [~~.~
r2V'l-."7""","",'-".---;M;, but also on the t (side edges) on the disturbed now Ilear
the surface. The simultaneous influence of the leading edge nnd one tip is present within the limits of Mach cones issuing from wing corners 0 and 0' (Fig. 8. t2.1a) if the generatrices of tllCSC cones intersect outside the wing. If these generatl'ices intersect on the surface of the wing (Fig. 8.12.1b), in addition to regions II and 1/' where the in4 nuence of one tip is obsef\·ed. zone [II appears in which both tips act Simultaneously on the disturbed flow. In region I on the wing between the leading edge and the Mach cones, the disturbed fiow is due to the influence of only the leading edge. Here the pressure cocfficiC'ol is determined br the formula for a flat plate: (8.12.1) p, = ±2«IVM!. - 1 We shall use the method or sources to calculate the disturbed flow in region II (Fig. 8.12.1a). The \'elocity at point A in this region is induced by sources distributed OVCI' wing section ACOE. The total action 01 sources BCO lind OBD 011 point A is zcro, and, consequently, integration in (8.10.3) \llust or performed OY('!' region ABDE. Aecordingl~', the velocity potential at. point A is
=
rr _d_,_
-al·...
.\~
:l.U""
,.~ l/~":'$ r~,
_d'_
r";.\-r
(8.12.2)
Point F is on the leading edge whose equation is x = O. Hence, by (8.9.4), for this edge we have r
= -(M .,/2).,
8
= (M ./2) •
(8.12.3)
Consequently. the equation of the leading edge in the coordinates r and 8 has the form r =-8 (8.12.4) Therefore, for point F. the coordinate rp = l' = -So Point B is on the Up whose equation is z = O. Hence, by (8.9.4), for this tip we have (8.12.5)
a8S
Pi.
I.
Fig.8.n.t Heclangular
Theory. Aerodynamics of an Airfoil lind II Wing
wing
ill
a
linearized :>upersollic now
We can thus write the equation or the tip in the form
(8.12.6) For point n. the coordinate Sn"""' rll' - r;... Performing intcgration in (B.12.2) with a vicw to the limits rl' =" = -s and Sa ,-. r.\, after introducing the values of r,\ and S;.. from (8.9.1'), we obtain
cpil
~- -~~roo
[V,.. %(xA-a'z.d
'~'7 t,Ill- 1 V.r.\(t~~~'zJ (8.12.7)
Let
liS
calculate the corr{'sponding pressme coefficient:
PII -. _. (2/V....,) dq;h
iJx,\,'
::a~(l.
lan-I! /
J' \
~'~~\.\
(iU 2.8)
On the houndary of Lhe Lwo rcgiou. liFt cot'fricicllt fOI' this St'c1ioll I"t'lalvd tn
face
lot,lI \\"itl~ Slll"-
Lilt)
is
(:II·-·C,~ .~:,
"
(':,
S\\- .. ('~\,I\:
'I'll(' 1011\1 lift cuelTici('1I1 ('11,,·-
Cull
('Ill
.
}/.,:Z-I
The wave th',lg coeITicil'll1
"'"H
'3CII "
=
SII')
c.; (1-
1..)
;.,,1..
(H.12.13)
j,-;
(1-
~;"\\" I?J'~ -t)
(8.12.11,)
/IJ~,,-.I
) (8,12.J5)
i,~
(J:t
I
(1-
2;. ....
ass
Pt. I. Theory. Aerodyn"mics of an Airfoil and a Wing
FiCl···tl.l
To tbe determination of the aerodynamic moment for a rectaDgular willII'
We can calculate the cocrricienl of the moment about the z-axis according to the known data on the pressure distrihution and the lift coefficients for individual parts of the wing: Ill.,. = Mz/(q ... Swb) (8.t2.1U) The moment Jlz. of the pressure forces distributeu over the surface of tbe wing can be found as the sum of the moments of the lift forces about the z-axis acting on variolls parts of the wing (Fig. S.12.2). Taking into account that on the trhmgnlar parts of the wing the point of application of the lift force coincides with the centre of mass of the area of the relevant part. we hAve the following expression for the moment:
(8.12.17) where yep, yep, and Y n are the values of the lift force calculated for parts CDB (IlEF), EFCH, and ADB (GHE), respectively. By (S.12.ft) and (8.12.12), we ha,'e
Y'l':." c~ P"'~';;" '1'
Y1
:":CIl
(J-~';;"
SII '- -*'
,pooV!.
1
Sll
Ija;
p... v!.
.
poo~!, Su
-,-Sf:t,cn :'-: ""(i7"'"'-2-(SW-.'Js n
Yll-=c~ r ...~';;"
SI1"--'
~
)!I ..
(S 12 IS)
Introducing (8.12.7) and (S.12.1S) into (S.12.16) and taking into account the value S II = Sw/(2'J..w a'), we have
m,"~
jI';:''::'
(1- JAw
v~~-,
)
(8.12.19)
Ch. 8. A Wing in a Supersonic Flow
389
The coeffieient. of Ihe centre of presSUI"e is
e ., "
-11
:li.,,-
.T;' _ ~.'~
V:ur=T _.:!
3(2i, ... ,1.11;'.-1-1)
(R.t2.20)
If the number iff '"' for the flow oyer the wing shown in Fig. 8.12.1a is reduced. then Ilt a certAin nine of this /lumher the lip )l;lch cones int.ersect inside Ihe wing. Here regioll 1/1 appear::: (see Fig. 8.1!!.1b) in which the disturbcd flow i!< 11ff('{'ted hy Ihe )eiltlillg supersonic edge (Inti both subsonic tips. The nature of the fluw ill rcgiolls I and II (/I') is the liamc m: ill the corre!lpolldillg zolles I and II (II') of the wing ,.... hose diagralll is shtJ\\'II in Fig. 8."12.1C1. Let us consider the now ilt point ;I of region I I I (sec Fig. 8. U.lb). 'fhe region o( iufluencc of the sOIll't·e.'> 011 thi~ now coillddcs with wing s(.'('tion ABDD' IJ', The )AUer can be l'cpl'f!Senled il!< the Slim of area~ IIIJDD' ami A Hn' /I'. With this in view aud 3t'cortlillg to (8.10.3), the velodty polenti:'!.1 at point Ii is
We can (lelerllline tho integl·a!.ioll limits directly from Fig. 8.11.1b. Hence,
We c-8lcltlate the lirst two integrals by 811alogy wilh (8.12.i), and the othcr two independent I~' of each other because the regioll of integration is a pllralll'liogram (see Fig. B.12.1b). \\,ith this ill view, we have
f~ill"".o ~'t:::'"'
{-V('A .. SH)(SA
+ V2r.A(SA -'A) -(·'A·
t
I'A)
_tan-ll/8";,~A) -:-2V{SA
(tan-I
$}I)
V~
SU)('A 'D')}
(8.·12.21)
Examination of Fig. S.1:1.1b reveals that thc coordinate Slf ~-' SD' and in accordance with (B.t2.1), the quantity SlY :- -'0" Consequently, 8H -- -I'D' '"=, -I'D"
390
Pro I. Theory. Aerodynemks of en Airfoil end eWing
Poinl 8' is 011 the starboard lip whose equation is z : , l. From (8.9.4~), we can lind the equation of thb; tip in the coordinates T and $:
T-s-=-M""l
(8.12.22)
lIen('e for point 8' TD'
M...,l
'': $0' -
s,-\..;..
M",,/
(8.12.23)
Ar.cordingly, we have SI-[ .• ~
-TD' -- -SA
I- M ool
(8.12.24)
Introducing into (8,12.21) the ('oordinales TA and $,\ from (8,9.4') and TD' and SJt from (B.12.23) and (8.12,24). we find
tal.c hehind lhc wiug mHl Ihe dl'ag force, Particulclor~' for \,ol·\1ident being c.on:
(9.1.5)
where qi is the set of dimensionless kinematic variables, qi is tho amplitl!de, and Pi is the circular frequency of the oscillations. In accordance with (1J.1.5), the time derivative is
q,
= dq,ldt = -qlpj sill Pit where we hflve introduced the Stroubal number
pt
= PllIV ...
(9.1.6) (9.1.7)
398
Pt. I. TI-.eory. Aerodynamics 01 an Airfoil and a Wing
For cxample, it l/;
• a, qi .- aD (thc amplitude of the o~dllatioll~
with rc!!pect to the angle of atlilck), ,..- p;, and Pi PI1.' thCII
is a!'sodated with the simultaneous rotation of a craft abont two axes and is of a gyroscopic nature. Gyroscopic forces and moments are pro-
".
404
PI. I. Theory. Aerodynamics of en Airfoil and
1I
Wing
fIg. 9.3.t
To the conversion of the aerodynamic coefficients and their stability derivatives from one reduction centre to nnother
portional to the product of two angular velocities. For example. upon the simultaneous rotation about the axes Ox and Oy. these additional forces and moments are proportional to the product Q."Qy. and the corresponding aerodynamic coefficients. to the product of the dimensionless variabJes CilxW v ' This is why the derivatives of a coeHicient with respect to Cil:.:Cil Il (c~~~jl" m~,~Wrl. etc.) are known as the gyroscopic stability derivatives. 9.3. Conversion 01 stability Derivatives upon a Change in the Position of the Force Reduction Centre
Let us consider the conversion of the pitching moment and normal force coefficients, and also of the releYantstability derivatives calculated with respect to a reduction centre at point 0 for a new position 0 1 of this centre atadistanco of x from 0 (Fig. 9.3.1). A similar problem is solved, particularly, when determining the aerodynamic eharacteristics of an empennage relative to the centre of mass that is the centre of rotation of a craft in flight and coincides, consequently, with the centre of moments. Assuming that the pitching moment (',oefficient at Ct = Q% = 0 .aquals zero (m:o = 0) and that the airspeed is constant, let us form a general expression for this coefficient relative to the lateral axis passing through poiDt 0:
mz=m~Ct-i-m.~~+ m~)~wz+ m;'z~z
(9.3.1)
in whichl thel derivatives m~, m~ • ••.• are known. We can obtain a similar expression for the new reduction centre: mzt =
+ +m:r1(j)d +m.:;l~~~
m~}al m~f~1
(9.3.2)
Here the nerivatiYes m~!, m~ll • • . • are to be found in terms of their corresponding values obtained ror the reduction centre O.
405
Ch. 9. Aerodynamic Charflcieridics in Unsteady Motion
For this purpose. let us first consider the relations between a.
~I" and
al'
~I'
OOll'
ii,
001"
;'%1' A glance at Fig. 0.3.1 reveals that
'XI = ex
+ l1ex =
ex -
(I):;;
x
where = xII, 001' = Q;lIV., and, consequent.Jy, ~I = ~ - ~:;.. The angular velocities and their derivatives do not change upon a change in the reduction c.eotres, i.e. 00:1 = 00 •• and ~:I := (.,1" Using these relations. let us reduce the formula for the moment coefficient: mz =
m~lexl + m~I~1 ~- m~%IOOIi + m~':I~'1
(0.3.3)
expressed in t.erms of the new kinematic pal'ametcl's (for point 0 1) to the form m%
= m~la ....,... m~l~ + (m;:1 - nl~lx) 00. -;. (m~'zl - m~;) ~z
(9.3.4)
By comparing (0.3.1) and (9.3..'..) we find
With this in viow, expression (9.3.3) acquires the form mz =
m~al -T m~1 -i- (m:'z 7 m~x) WZ1 -:-. (m~)z -T- m~.i) ~zt
(U.3.S)
The obtained moment coeftident can be expressed in terms of its value found for the now centre 0 1 by means of the formula m. = = mn + e,i' (Fig. 9.3.1). Here formula (9,3.2) ca.n be substituted for mu. and C,l written in the form of a relation similar to (9.3.5):
e" = c;al-:-'
e:a
l .;..
(e:" -: e~x) 00:1 ...;. (e:'" .~. e:z) W.t
(9.3.6)
By comparing tile expression obt.ained fol' In: = m%l T cux with the corresponding relation (9.3.6), we find formulas for the stability derivatives relative to point 01: m~l=m~-e::X. m:{J=m::+(m~_c;·")X-C~2. } • . •• ••• m~l= m~- ~r. nl~ft=m:~z + (m:-e;")"i-c:x~
(9.3.7)
The new stability derivatives of the normal force coefficient are obtained by comparing Eq. (9.3.6) and ao equation similar to (9.3.2): CIII
=c;lal ~.e:~~1 -j.c;pOOzt + e'~il;"1
406
PI. I. Theory. Aerodynamics of an Airfoil and • Wing
in which we assume that cY1 = cy (because upon a change in the redu('tion centre the aerodynamic force does not change). The coroparbson yields c:l=c
y.
ci,=~, c(:u = yl
8
c;ll=c: z +c:x
C;I • ..!....
yl
I
JX' Y
(9.3.8)
Similarly, we can convert the aerodynamic characteristics for rear arrangement of the new reduction centre. 9.'. Particular Cues of Motion Lon.WI.... and Latera. MotIons
To simplify our investigation of the moliOIl ofa controllable craft and farilitate the finding of the required aerodynamic characteristics. including the stability derivatives. we shall usc the method of resolving the total motion into individual components. The possibility of resolution into longitudinal and lattoral motions in principal is due to the symmetry of a craft about its longitudinal axis. The longitudinal motion (pitching motion), in turn, consists of the translational displacement of the centre of mass in the vertical flight plane (the trajectory differs only slightly from a plane one) and rotation about the lateral axis Oz. In stich motion, good stability in roll is ensured. and variables such as~. '\'. COX' and COy may be considpred negligibly small (the surfaces controlling rolling and yawing are virtually 110t deflected). Upon lateral motion in the direction of the axis Oz, the centre of mass moves. and the craft experiences rotation about the axes Ox and Og (here the control surfaces function that ensure yawing and rolling motion). When investigating longitudinal motion, we usually consider the aerodynamic coefficients in the form of the following functions: cx=cx(M •• a, 6e). c,=O.
cu=·c!I(.IJI_, a, 6e)
}
.:..
(9.4.1)
m:-==O, m,,=O. m,=mz(M ... a. 6e, a. 6,)
To study lateral motion. we use the coeBicients in the form of cu=c,,(Moo. a, 6e), m~=m:r:(Mool a. mil
=
mil (M ...
P.
P. 6n
c,=cz(M ... ,
P.
6 r)
btl br • bat CO,r, Wg , Wz> W X1
wy •
W. 01')
(9.4..2)
Ch. 9. Aerodynamic Ch3r ... cle,i$flc~ in Unsle ... dy Molion
407
It mus\. be had ill view that longiLudillal motiolL is studied ilJde~ -pendently of lateral motioll, whereas the latter i.tigation. we ~hall wrile the aerodynamic coefficients ill the form c_~=c",(,Uo O. Solution of (9.5.4) yields a relation for C/.. lndiratillg the undamping aperiodic nature of motion. Hence, static in~t8bilitr also gi\"es rise to inst.ability of Illotion. In this case, agreement ran beobsel"Yed bet,,'eenstatic ouri dynamic stability or instability. Such agreemE'nt is not obligflt.oI'Y. ho,Ye\"er, for the g(1Tleral rase of motion of a craft. One Illny lJave a statically stable (Taft thnt, howewr, doC'!<nothavedynamic stability and in its telH..Iellry to the position of eqnilibrium will perform oscillat.ions with an incrE'm:ing amplitude. S1]ch cases are observed in practice in some airrraft at 10\\'-spce(! flight. and al~o in flying wings with a small sweep of thfl leading edge. It ron:::t be notcd that tllC overwhelming majoriLy of aircr ...ft owing to special devices have static st.ability, i.e. the ability to respond to distmbau('es so as t.o reduce their magnitude at the initial instant. This property is of Illnjor practical sigllil]rance regardless of how an aircraft behaves in the process of di::tllrbed motion. Free development of the Jisturbances ifi lIsnally attellded by denection of the control surfaces to retmn the ,,-raft to its preset flight condiliolls. The use of these control ~l1rfaces ifi a necessary condition for ensllring the preset motiOH of a statically unstnble (with fixed control surfares) aircraft. The concept of stability presumes the existence not of two separat.e kinds of stability-static and d:ynamic, but of a single stability renecting the real motion of a craft in time and its abUity to retain the initial flight c.onditions. Since the dynamic coefficients of the eqllations depend on the parameters of the undisturbed flight, tho s1lme aircraft can have different dynamic properties along a tra~ jC'clory, for example, its motion may be stable on some sections of the trfljectory and unstable Oil others. unsteady motion is described by equations whose dynamic coefficients depend on the design of the craft. Unlike craft of the aeroplane type, such coefficients for bodies without an empennage. or with all only slightly developed empennage (fin assembly), correspon and the dimensionless coordinates
=
£=
xIx,. and ~
=
zlx,.
=
(9.6.2)
related to the length XI!. of the Iifti ng surface. Now we obtain the following relations for the force and moment coefficients at any unsteady motion of a lifting surface with the dimensions l:
Ch. 9. AerodYnAmic Characteristics in Unste.!dy Motion
417
FI,. U.t
To the determination of the aerodynamic coefficients for a lUUng surface
Here So and ~I are the dimensionless coordinates of the leading and trailing edges of the lifting surface, respecth·ely. For a non-standard coordinate system in which the axis Ox is directed from the leading edge to the trailing one, the signs in formulas (9.6.3) should be reversed. Let us fmd relations for the aerodynamic characteristics of the lifting surface cross sections. For the normal force, longitudinal moment, and rolling moment of a section, we have, respectively dY=
r
6.pdxdz,
:l:"n
dM:T = -
dJlz = )ll.pxdxclZ,
..y
:TQ
6.pz dx dz
(9.6.4)
The corresponding coeffidents are as follows:
1
I
(9.6.5)
where x' is a chord of a lifting surface element in the section z = = const being considered. We calculate the integral in (9.6.5) over a given section from the trailing (Sl = XI/XII) to the leading (So = XO'XII) edges. W:, . . .
m:1 = m~,
m:)z .
m::E, m:z
Assuming that the craft length XII has been adopted as the characteristic geometric dimension, we obtain from (9.6.3), (9.6.7) and (9.6.8) expressions for the derivatives of the aerodynamic coefficients
in terms of the derivatives of the difference of the pressure coeffi-
Ch. 9. Aerodynamic Ch",racieristics in Unsteady Motion
419
cients: 2.x 2
1/(2.~1r.)
1=p
o
~I
C:i=-t
J
2.J2 1/(2... /1) ~o
•
J
JP~id~d{, C~'=7
0
.
JP"id~d~
~I
li(2J:/I)i o
m;i~-~ ~
jp'Il~dsd!;,
~l
ii
m~i~
-
~Z
J Jp;lsd~ds o
2.x 2
m~i=--f-
IIIZs/,) i.~
I o
19.6.9)
iG
li(2~·k)
~l
.
"x 2 1/(2.th);0
1p'/iSd~dt;,m:i.o.--;' ~l
J 0
•
JP?i~d~tl~
!1
The above expressions are linear relations between the aerodynamic deriv~tives and the dimensionless kinematic vDriables gj and go that ensure quile reliable results provided that the values of these variables are small in romparison with unity. III linearized problems 011 the IInsteady flow O\'er lifting :"lIrfares, such relations are exact for a harmonic law of the change in the kinematic variables (see 14, HI]). Let us consider some features of the slability derivaU\·cs. Sinre we arc dealing with motion in the absence of sideslip and an angular veioeity about the axis Oy (~ ,..-. 0, Q v = 0), here the deri-..'atives of the aerodYOiunic coefficients wi th respect to the parametl?rs ~ and Q y evidently eqllal zero. In addition. we have excluded the coeHiciellts of the longitudinal and lateral forces (c,., c,) and also the yawing moment coefficient m" from our analysis because inde· pendent in\'cstigations arc devoted t.o thew. It mllst be had in vjew here that when analysing the stability of a craft, these qualltitief-' are of a smaller practical significance. For a lifting surfaco that is symmetric about plane xOy and movE'S translationally in the absenr.e of rotation (Q x = 0), the prcssure is distributed symmetrically; therefore, the corresponding derivatives equal zero: m'l/ = 0, = (i = 1, 3). With rotation about the axis Ox, the pressure is distributeu asym· metrically about symmetry plane xOy, hence the aerodynamic loads produced by the angular velo("ily ul.~ are also asymmetric, and, consequently, the following stability deri-vatjy(,s eqllal zero in this case:
mil
c:·~ = 0,
°
c~ ... = o~
m~·t = 0,
m~'·'· = 0
420
Pt. t Theory. AerodynamiC5 of an Airfoil and a Wing
C.uchy-LilFilnge IntaFill
Let us consider the basic expression of the theory of unsteady now relating the parameters of the disturbed now (the velocity. pressure. density) and the potential function . With this in view. the equation of motion (3.1.22") can be given thus
a g~~d (lJ -+- grad X; =
_
+
grad p
(9.6.10)
Considering that the gas flowing over a body is a barotropic ftuid whose density depends only on the pressure. i.e. p = p (P), we can introduce a function P, assuming that P
= Jdp/p (p)
(9.6.11)
Accordingly.:
(9.6.12)
(lip) grad p = grad P We can therefore write (9.6.10) as grad (iJed of sound a:! = dp/dp. By (9.6.25), the continuity equation becomes
+.-%_: a~ (iJ~;y _~.~+~)+~.~ +~,*+~.~-=O
(9,6.26)
Let liS exclude the dynamic variables from Ihis equation, ret.aining only the kinematic ones, To do this, we shall use the Cauchy· Lagrange integral (9.G.18') from which we shall find expressions for the pressure derivat.iv(>s with respect to the corresponding cOordinates x, y, oZ, a.nd also the time t related to the df>nsity: (lip) opfax, (lip) opioy, O/p) apia, For this purpose. with respect to x, 1/,
\\'C
Z,
sholl differentiate (9.6.18) consecutively and t:
+·*~e;rV~ ~~~-~~)
+.-%£-
=~(V= d:2:y
+'*-=Pf(V~ iJ:~t +.*--,~(Voo
-
aaY~I)
;,":t)
(1l.6.27)
u:;t - ~~~)
We shall write the relation for the square of the speed of sound at; in a linearized fiow on the basis of the Cauchy-Lagrange integral. Since P-P.
424
Pt. 1. Theory. Aerody"~mics of an Airloll "nd a Wing
then with a view to (9.6.17) and (9.6.i8'), we have aZ = a!, (k - i) (V"" acp/ax - 8cplat)
+
(9.6.28)
We can represent the velocity components in (9.6.26) in the form
V. _ V _
+ &~/&X,l
V, -
a~iay,
V, -
a~/a,
(9.6.29)
Let us introduce (9.6.27)-(9.6,29) into continuity equation (9.6.26). Disregarding second-order infmitesimals and assuming that the density ratio p,,jp ~ 1, we obtain (i--M!')
~:;
-I ::; 7
~:; + 2~:oo .~-
aL . ::~ =0
(9.6,30)
where M"" = V ""Ia"", is the Mach number for an undisturbed Dow. The obtained equation is called the wave one. It satislles the velocity potential III of an unsteady linearized flow. If in a body-axis system of coordinates, the longitudinal axis 0:& is directed from the nose to the tail, the sign of the term (2M ",,/a .... ) a'1.~/8x 8t in (9.6.30) must be reversed. With a view to the notation (9.6.19), the wave equation in the dimensionless form can be written as follo'\\'s: (1-M;,)
~~~ + ::~ + ~;% -,2M~ iJ~~'f
-M:O
~~
=0
(9.6.31)
To determine the aerodynamic characteristics of a craft. it is sufficient to solve wave equation (9.6.31), finding the potential of the disturbed velocities Ylt " can be written itS q.>(XI'
Ylt
Z't
t)= })
'(;T.~. ~1)d1"rJ"~.
J.\' ='-"'-""'= ,,~
IJI
wllere r = V (Xl xr'" ,,'2 Iy~ (Zl 411 is a conditioliRl elistance between the points (Xl' JIl. Zl) Rnd (:1', 0, z). The integration regions 0"1 (Xl' Yt. ztJ find 02 (Xl' Yh ZI) are the parts of plane ;1.;OZ confined within the hranch of the ~1Rch (characteristic) cone issuing from the poinl (Xl' Yh Zl)' This branch is determined by the equation a'2y i :...= (Xl - X)! - a'2 (ZI _ Z)2
As a result of dHferentiating *-0
0)
(9.8.19) (9.8.20)
The last derivative is used directly for calculation of unsteady now parameters. The rmding of this derivative, and also of other functions determining the dimensionless induced velocities is described in (4), vortex Model 01 • Wing
A vortex model of a wing in the form of a nat lifting surface in an unsteady circulatory flow is shown in Fig. 9.8.3. If a wing has curved edges, they are replaced approximately with a contour formed of segments of straight lines. Hence, in a most general case, a lifting surface has breaks. Let us divide the entire area of a wing into zones by drawing sections parallel to the axis Ox through the breaks in the contour. Let us further divide each segment l6 between the breaks into strips and number their boundaries from right to left (the boundary having the number p = 0 coincides with the tip of the wing, and having p = N with the longitudinal axis). Usually the values of the width of a strip lp,"_l differ only slightly from one another. Let us consider the strip between the sections p and p - 1 in any of the zone.'i 6. We shall denote the dimensionless coordinate of the leading edge in the secHon p by So. p, Ilnd of the trailing one by The relative chord of the section is
No
G.,.
s.p -
bp = bplbo = So l' Lel us assume that a strip consists of n cells. For this purpose, we shall divide each chord in the relevant section into n parts by means of points with the coordinates ' •• P '~".p~0.5b. (1-
hy \I {for the leadillg edge 'I' """" 0, for the tl'uiling one v = "J. We shall designate the coordinates of points at till' intersections of the lines v and p by the subscripts v and p. Hydrodynamically, the plane of the wing is eqlli\'alent to a Yortex surface that is approximately depicted by a system of bound discrete vortices. Each of sl1ch vortices evidently consists of oblillu('" horseshoe vortices adjoining one alJother, while the total number of these vortices coincides with the number of cells in whicll they are accommorlatcd. We shall characterize the bound vortex filaments by a serial number fL counted from the lIose. Let liS introdll!:e (or the sections dividing the plane of the wing along its span, ill additiOIl to the numbers p, the serial number k conn ted from a tip where \\'e a~sume that k = O. Accorrlillgly, O:::;;;;k ~ ,y, We shall denote the points of intersection of the lines fl and k by the SIII1IO subscripts, \\.'e consider here tllllt the coordinates of points on the leadillg edge ill St"!ction k and the magnitude of the chord in this section bk (pl of each lOne 6 arc known. We shall determine the posit.ion of discreLe YorLices a:o follo\\"s. We separate the chords in the sections ilnd ~"_I with points haYing the (:oordinates
;h
~p." . So.I:-:· O.5b" (l-cos 2!~n·I:1)
~Il'''-I ~c ~o.h-I -- O.;)b"_l ( 1·- cos 2~~:- I j.I ~--'
I, 2, ... ,
It
:1)
(9.8.22)
488
Pt. I. Theory. Aerodynamics of an Airfoil and 011 Wing
Poinls with identical !J.'s coincide with the ends of discrete VOl'· tic.~s. WI' hal'e the followillgrelatiolls for the dimensionless coordinates of the middles of the oblique bound vortices, tlu'!ir spall lA'''-l' and sweep illlgl('s tan x~: L,:
~::tl
05(~h
S)II, •• )-=O.5(£oh..j~h_l)
o 2;) (b" ; b,,_11(1-cos t:,~_,=-O.5(l:"
1,.J..t,I.It_I)'
2"'2:;1
1
n)
i~'h_'- I~b:-l =tJl,"-I-~)1 I,
I
(9.8.23)
tan x~: ~_I' - (~. "_I-~" ,,)l(bll, "-1- bll,") jJ.~··1. 2, ... , Il; k,...·l, 2, ... , N The coordinates of the centre of another vortex symmetriC about plane xOy 011 the port half of the craft and also the sweep angle arc as follows:
o~: t.1
=s:: ~-Io crb~: L. =. -t:: L'}
crt h . h-I "".. l h . 1,_1. crx:::t_."""-'X~:tl
(9.8.24)
where the l'ariables for the port side of the wing al'e designated by the faclor o. For a wing with rectangular edges, the sweep angles of the bound vortices arc constant (x ... : const.) , and each of t.hem transforms into an ordinary straight horseshoe vorlex. H a wing plane has breal(s in its contour, then the corresponding breaks are present in the vorLex filaments too. The circulation of obliq\le and conventional (straight) horseshoe vortices along tile spall is constant, while Iree filaments parallel to the axis Ox are shed off the ends of the bound vortices. The free filaments propagRte downstream, and when the flow is circulaton' they pass away to iurmity. In addition, when the circulation of the bOllnd vortices changes with lime, free vortices of the relevant strength are shed off tltem. The vortex model being considered is very convenient for computerized calculations of a Oow. This is due, flrst, to the suffkiently simple relations describing the disturbed Oow near a wing. and, second. to a number of important properties of the system of algebraic equations which the solution of the problem is reduced to. One of these properties is that the diagonal terms in the matrix of the equAtion coefficients play a dominating role; the solutions themselves hllve a great stability relative to the initial conditions. A significant Ieature of computerized calculations is also the fact that the usc of oblique horsesl1oe \'orUces instead of the cOllventional ones leads to suhst.antiall'limpliflcation of the calculations and to more accurate r('slilts.
Ch. 9. Aerodynamic CharacieristiC$ in Unsteady Motion
439
Calculation of Circulatory Flow
System of Equations. Let u:; JT'p['esl'lIl the dimensionless cil'clIlation of the oblique hOl'scshoe \"Orte:\: rl"~' 11_\ = r~. I;, /,_11 (1'"",bo) in the following form:
1'".,.. A-I ('1')",,"
~t [1':1, h. II-I qi (Tl ; r~i.~. II-I ql ('tl]}
q, ....... ct.
(1)."(",
(9.8.25)
(Il,,; T=l'",I-'bo,
or in the expanded form f ... , II. II-I
(T).~'~ r~, Ii. II-I a..!. r~. h. h- I ~+. r:~ II. II-I (O).'(}
+ r:~II. 11_\ wx-:-l':~ II. h-I
(I).
:..
(9.8.26)
r;~ II, II_I ~z
where r:~ Ii. A-I arc dimensionless functions not. depending on the time; the only Hme-dependent \'ariables are qi and q~. We shall assume that tbe kinematic variables change according to harmonic rl'lalions (9.1.5) and (9.1.6) which CIUI be represented in terms of t.he dimensionless Lime T as follows: qi :..: cos prT, -q'{pr sin ptT (9.8.27) wllcre qT are the amplilllfle \·a.llIes o[ the yuriables not depcnding on lhe time, pi '-' P1bo:l l "" is the StroulHd nllmber (Pi is the angular frequencr), and T '--' tV",lb o' With a view to (0.8.27). the circulation (9.8.25) is expressed as follows:
q;
qr
r ll . h. 1,_1 (-t) =
f q1 [r~i. k.
k-I
1-=-\
cos ptT
-r~~ II, Ir-l pt sin pr"t] (9.8.28)
Ily (9.8.6) 3
'\'(s~: ~_I, "t)= V"'" ~... f/Tpi {r~i. II, II-I sin (pt (T-~~: :_1) 1 j'l
(9.8.29) where S~:hlt_l is the longit.udillul coordinate or the middle of nn oblique bound vortex. The expressions fol' the circuh\lion of the rree \'orlic.es (9.8.7) have the rorm
,
r 1 (:!) (6~::- t."t) :b r'~.It.h_I=-1
11 (011(2)11-, A, A-I
~ ~
v,
p~Pt-l
.a
c.lJ.2)1\, h,
v,
It-I)
P8pr- 1
(9.8.47)
k=IIo1=1
;.;
r'~,
h, 1:-1
p=1. 2, .. " N; k,..-=l. 2, ... , iY
r:,II,:k-ll"'=II.=O;
,\,.=1.2, ...• n-1;
We use a third system to find the derivative r:~Jt;.Jt;-I: 1
N
4i" ~
,11,1:-1 ",,11.,11-1 0; v,p \ hn (~.JI.JI_l+(JVV.p.p_l)rll.II •• _l=-SV.P_l I
'~I .~I
r~~
II,II-dll
~II- •..:: 0;
p=1,2• .•• ,1'f; v=1. 2• ...• n-l; k=1.2, ...•
I
.vJ
(9.8.48)
446
Pt. I. Theory, AerodYnllmics or an Airfoil "nd a Wing
A fonrth system of equations is intended for cair.ulClting
r~~II.II-1:
(9.8.49)
r~: 1s or Do\\' that is characterized by low Strouhal numbers (pi ~ 0), inste;'1I1 of Eq (0.8.83) we obtain (').8.84)
Let us consider a rigid lifting sHriace. Instead of the flow of a compressible fluid over it, we sha11 study the flow of an incompressible fluid over the transforme(\ surface. The coordinates of points in the incompressible flow are related to the coordinates of the space of the compressible gas hy the expressions XIC ,...,.
xlk,
YIC
= y,
Zic
=
(9.8.85)
Z
in the dimensionless form tiC =
Ile/bo.le =
£.
Tllc
~IC -= Zie/bo· Ic
= '=
Ylcfbo,lC
= 11k,
(9.8.86)
i;Je
Let us change the pl;Ulform of the given lifting surface. nsing the relations between the coordinates in the form of (9.S.S6). In accordance with these relations. the dimenSionless geomotric variables of the transformed surface can be written as follows' (U.S.87)
where edge;
£0
and ~a are the dimensionless coordinates of the leading
blc = bIClbo.lc. b = blb o, blc = b/k For the centre and running chords in (9.8.87), we have introduced the symbols bo and b, respectively. For wings with straight edges, the planform is usually set by dimenSionless parameters, namely. the aspect ratio Aw = lo:'bm, the taper ratio 11,,· bolb l • and the sweep angle of the leadillg edge la. The corresponding dimensionless geometric vari(lbles of the transformed wing in an incompressible Oow are: =0
Alc•w = /cAw. 11IC,"'" = 11"" Ale ....- tan Xo,le = Aw tan
xo
t) of a transient (pulsating) source (9.7.7) satisfying the wave equation (9.6.30). Let us consider the expression for such a potential for harmonic oscillations of a wing when the kinematic parameters vary in accord-
Ch. 9. Aerodynamic Characteristics in Unsteady Motion
4'57
ance with the general relation q,
=
q; exp Opt)
(j
=.0
cr, l'J.~,
fJ)1)
W.n.!}
It follows from (9.6.32) that the h011ndary conriiliOlls 011 a wing
also vary harmonically. The derivative of the velocity potential on a wing (9.7.8) (let liS call it the now Jown\\"ash) om he expressed by the harmonic function (0.\J.2)
The required disturballcc potf'ntial is related to the downwashes.
~~rJ~~~~ul~i~~'~~~~~~: (~.~~~~ti:: f~l'~~~~: t~
are determined in ac-
: =t/21 =/~\~l~ ~ ~/:,~::!'~i ~jJ~~'(aa]'2)}
~~ ~
(9.9.3)
After introducing (9,9.2) and (g,9.3) into (9,7.7) for a wing (assuming that y -'.co 0), we obtain Ip(XJ, Yl' ZjI
,I
rr JJ
t)=, _ _ Hee iP1 ~
eI(%"
[.:;;t(;t.,.1/. Z)] pO vy
to)
Xe- jP(.~'~~:'::"'" (eiP ":C!.""! e-;P .,,,,-:~,,.1 dJ/= Taking into account that the sum in paTell theses on the righthand side equals 2 cos (pr,a",a'Z), aIHI the (]lIantilies p* = pbo/V""
(I)
= p*Jl;,'-x"1
(9.9.4)
we obtain the foHowing expression for tile velocity potentia!: fP (xt. X
Yll %1'
t) = -
rr ['. au (x,
JJ a(x"
-k He q$e ]
y, z) y=l
iN
- ,....:.'cos -,) ('"') d, d, "oJlx> - , -
(8.Y.5)
:,)
whel'e r = V (Xl x)Z a'Z [y~ -;- (ZI Z)2J. With a view to the harmonic uature of llloLion of the wing, wecan write the potential function as follo'..-~: fP(x. y, Z,
t)=V""bO.~(Ql"jqJ ;=,1
= V""bo He eil'!
.
L
j~l
l-rp1j9J)
.
q; lip"} (x, y. z) -;-- ip*Ql"j (x, y, %)1
(9.9.6;
4ea
PI. !. Theory. Aerodynemic5 01 en Airfoil and ... Wing
where qJ -= qje iP !,
1j '""" dqJldr:= (dqj/dt) b,/V"" =
ipjqje iP !
(9.9.7)
In accordance with (9.9.6). the partial derivative of the potential function with respect to y is a'l'
Ty (I, y,
Z,
. t) = V""ho Re e'p!
h3
_[ flIp'll
qj --ay(x, y, z)
;=1
+ip*
&:!I~j
(x, y, z)J
(9.9.8)
Inserting this ucrivatiye into the left~hand siue of (9.9.2), we .obtain the following relation for [OIP (x, y. z)/oyly=o: [ ;: (x, y.
+ip* 8:U'" (x, y,
Z)]
(9.9.9)
Introducing this expression into (9.9.5). substituting (9.9.6) for the velocity potential on the left~hand side, and taking into account that e - ;"'~,-l;) = cos CIl (:t"l -x) _ i sin W (Xl-X) b~
bo
obtain relations for the derivatives of the potential function:
XCOSW(.1'I;:.1'),p*[ uti (x.
y. z)Jv=o sinw (:t";,;.1')}
x Cos ( "'(s, . 0, "q,(.)[ =
±
['1'"
i""l
(s',
0,
"q'(")e-cpo, (s',
0,
"q,(.,)]
(9.9.18)
where by (0.9.1), we have gJ (t) = qje iPt , qj ("C"') ,,-, qje;P{l-(X*-X)}VooJ;
qj ('t) = iqjpe iPt 9} ("C*) = igj p*eiPlt-(Z.-Z)/Vool
After introducing the values of qj and their derivatives into (9.9.18), we obtain (without the summation sign) ( used for small Strouhal numbers (p* -+ 0):
~'I(s" 0, ,,) - F'I (s" 0, ,,)
q>~J(£1>
0,
S!)=~J (Sh
0. t;,,)-
M;~t ~J(Sh
} 0, SI)
(9.9.25)
After inserting the value of CPqj (9.9.25) into the first of Eqs.(9.9.24). we obtain an integral equation for determining the derivative pqj:
F"i(t
_t, I,
0, )__ -'-rr[.!!:.!...] JJ ,
1, t
8'1t
"
11t=O
d',dC, rt
(9.9.26)
" Let us introduce (9,9.25) into the second of Eqs. (9.9.24): rJ (SI, h 0,
~t. 1)-
M!,;,t.
t
pqJ(£I,
It
0,
~I,,)
M!,(St',t- St )
[.!:L!...]
Ct
81)1
} dS!dtt Tlt-O
rt
Substituting for the derivative Fl J on the left-hand side of the equation its value from (9.9.26) and having in view that by (9.9.25)
""] "I-O=-= [""] [~ ~ T1t=o we obtain an expression for finding the derivative Fqj:
F~J (t_1,
to
0') = • .",1.
t
_..!.. f r [~] d~!r,d~t IE J J 8Tl' Tlt~O
(9 9 27)
..
"
We perform our further transformations in characteristic coordinates (Fig. 9.9.1). namely,
+"
r - Is, - s",,') - ,,, s - (S, - s"",) (9.9.28) selected so thal only positive values of the variables will be used in the calculations. The value of ~o.o.t representing the displacement of the characteristic system of coordinates is determined as shown in Fig. 9.9.1 (the coordinate lines from the displaced apex 0' pass through breaks of the wing at the tips).
Ch. 9. Aerodynamic Characteristic$ in Unsteady Motion
463
Fig. 9.9.1
To the Dumerical calculation of a wing with combined leading and supersonic trailiDg edges in an unsteady Row: I . JI-resions 101 fmdlnG: HlP down.
wa~ h
Equations (9.9.26) and (9.9.27) acquire the following form in thecharacteristic coordinates:
;, F) (rjt
&F~) i i~'[.~
1 "..
0, $j) =-
-z;:
(9.9.29) ] 11,=0
drtls V(r1-r) ($I-S)
For further transformations allowing us to eliminate the singularity in Eqs. (9.9.29), we shall introduce the variables
v = Vr
1 -
T,
U
=
VSl -
S
(0.9.30)
Equations (9.9.29) acquire the following form in the variables (9.9.30)
(0.Y.31)
where (9.0.32) To perform numerical calculations, we shall divide the region. occupied by the wing into separate cells as shown in Fig. 9.9.2.
464
Pt. l. Theory. Aerodyn
St
d£t dt t
~,
1 J" x.~:. ~.) t.'. d•• dt.]
(9.9.75)
It must be taken into consideration that the velocity potential cOn the leading edge is zero. Consequently. (9.9.76)
Accordingly,
it )
q
aF
Ja~tlo 'I)
ds, = Ft , (st. ~t)
~~. t
i~
J
" of
J~i:·~t) StdSt=stF'Ij(st,
St)
!io.t
.t
-J
F"J (St. i;;d
dS t
lo.t
(9.9.77)
'J~
ilF'I J (st>
~t)
,.,.. A: _,. t;-F" (t.
--.;-,-'ot5tu'et-~tSt
lo.t
., -
\ F'J (S" ~o: t
t.) t. dS.
.)
'=" ...t
Ch. 9. Aerodyni!lmic Chi!lri!lcteristics in Unstei!ldy Motion
..
) of'' i ~~:'
471i
~I) sf d~t .= ~t~F'I j (st, ttl
,:
lo.t
-
) Stp"J (s" ~t) d61
to.t
In a similar way, we shall writ.e the relevant. expressions related to the derivatives pili. Let us go over in (9.9.70H9.9.75) to the characteristic coordinates sand r (9.9.28). Assuming that the velocity potential (or the [unction D) is const.ant in the cells and replacing the integrals with sums, with a view to (9.9.77) we obtain relations for numerical calculations of the derivatives of the aerodynamic coefficients. These relations, used for finding by (9.9'(i7) t.he correspondin.g derivatives of the aerodynamic coefficients of t.he lift. force ~. ~, C~I, and also for determining from (9.9.68) the derivatives of
c::,
the pitching moment coefficients sented by the relations: C:. t = 4bg~'"",,. h
h
m:;, mi, m~·;. m~;:
FrJ. Cr*,
can be repre-
s*)
;. C:t, t = -
4bg~~~;.w
liZ ~
~ pi" (T, $)
I
s
~
4I>!a"),.. h Cy,2t=--,,-
{a' ",.,i -, M!, f.C'. ~r,
- ~ [(;:'+S*)hI2+s.", .• i F"f',
r.
-') S
(9.9.78)
[
s') +h ~ ~ F"(r, s)} s ,
C;,'t = 4b3~';"w h ~ p"'z (r*.
s*)
;.
c;t, c:i.
t
= -
t
=
4bB~~~l.w
h'1.
~ hPj,), (r, "$) s
4bB~~11...
h {;:
~
"" ;:-
i'z (r*. $*)
t
(9.9,79)
476
PI. I. Theory. Aerodynsmics of an Airfoil and sWing
,. +h~~F"'(;:, SI}
,
m~. 1 = 4b~~~%}'w h {h «r* +8*) h/2 -:-~. o. tJ Fo. cr*, $*)
"-h~,~r(;, S)} m:I,t= - 4b~~:'AW h'l ~,~ [(r~s)hJ2-:-£o.o. t1 r(r, "8) ;
_
~hJo.'JAw h { +
m,2.t- - - , , -
a'
M:7.,
'"
1-* +s-"') h/2
~ (r
(9.9.80)
"
- ~ ((r* + 5*) h/2+~. o. t]2 F~(r", s*)}
,.
The aerodynamic derivatives of the rolling moment coefficient are calculated by the following formulas:
m::t= m~f.
t
=
m~:Il = x2, t
4b~;S).w h
h rls.-r*)h!2j F'"x(r*.
;*)
" 4b~~:3)...... h h h ({s-r) hJ21 F\i):Il (r, S) Z
_
4.f;~o.'3"W I~
,
h {~ 'V [(s*-r*) h:2J M~ LJ .'
,.
F~X(r* • :;*)
- h [($*- r-*) 1I/2J [(r* + ;-*) h/2 +~. o. tJ F"'x (T*, 'i-h ~ ~ s
l(s-,)h!2J FO, (r',
,O)}
s*)
(9.9.81)
Ch. 9. Aerodynamic Ch~racteristic5 in Unsteady Motion
477
If we take the wing span l as the eharacteristic dimension when calculating the rolling moment coefrlcient, and the half-span lI2 when determining the kinematic parameter {J)z, then the new values of the rolling moment coefficient and the corresponding derlvatives are determined by the relations
mz1 = Inzboll. m~fl = 2m~:t:: :'0 and 11,," If a rectangular wing is being considered, it is necessary to assume that Aw tan XO = 0 and fill' = 1; for a triangular wing. flw = 00. Diagrams characterizing the dependence of the stability derivatives on the similarity criteria for wings with a taper ratio of 11w = 2 in a subsonic flow are shown in Figs. 9.10.1-9.10.10 as illustrations. The mean aerodynamic chord bA has been taken as the characteristic dimension when_ calculating the data in these figures (the kinematic variables ;"A, W:.A, c:,z.A, the coefficient mt.A)' This makes the dependence of the aerodynamic derh'atives on the geometric parameters of the wing more stable, the results approaching the relevant quantities for rectangular wings. When CAlculating the rolling moment m:tl, we chose the wing span l as the characteristic geometric dimension, while for the kinematic variables W.xl and ~Xl we took the half-span l/2. The origin of coordinates is on the axis of symmetry, while the axis Oz passes through the beginning of the mean aerodynamic chord bA • When nece5sary. w(' can convert the obtained (lerivatives to another characteristic dimension and to a new position of the axis Oz.
Ch. 9. Aerodynllmic Chllrllcterisiics in Unstelldy Motion
Fig. Uo.t
~~ea:~~: i~al~buela~~~n~t: s~t'it ity derivative c~ for a wing in a subsonic Dow
Fig. '.to.l Change in the quantity kC:,z'AA detennining the derivative
~~;i~~t~~~
Fig. '.to.l
a wing at subsonic
.
.
valuesofyc:~At and k Sc:6.z ~g:rd~:r;~~i~~ o~h:he c~o~~~~ie~~ 'with respect to oX..%. !for a lifting surface at M"" < 1.
clI
479
-480
Pt. I. Theory. Aerodynamics of .an Airfoil "nd " Wing
'flg.9.1G.A
k't:'
k't;,t.
ValUE>9 of ,z:..1 and A determining the derivative of Cy, A with respect to (l)t, A for a !!Ubsooic now over a wing
'flg.9.to.S -Change in the variable kmx~3.:1 determining the derivative of the rolling moment coefficient with respect to (l)xl for a wing at M",, I
a.'m:?'
Flg.9.f0.t6
Values of ',/.'2
a'2(m~'I\]h
and
(m;jqh characterizing the
change in the ucrivathc of the rolling moment coefficient with
~~~~~~nl~ 81;~ ror 11 wing in a
-O.1J'
486
Pt. I. Thllory. Aerodynamic5 of an Airfoil and a Wing
Flg.9.tO.t7 Variable a'"t~.A determining the derivative m~A for a wing atMoo > 1
-J r---t---' 1 grow with an increase in the aspect ratio. although to a smaller extent than at subsonic velocities. Particularly, for a rectangular wing (XO = 0), the increase in ~ wben M">O > 1 occurs only up to Aw = 3-4, and then the derivative ~ remains virtually c·ollstant. For triangular wings. the constancy of t1, is. observed beginning from ct'}.", ;:e, 4, Le. when the leading edgi-s transform from subsonic into supersonic ones. The derivatives of longitudinal and lateral damping (m~.·AA and m~"\al"ized Dow over a thin sharp-nosed airfoil, the pressure coefficient at a certain point is determined according to the local angle of inclination of a tangent to the airfoil contour ex - ~=-- (for the upper ~ide). and a. - ~J. (for the bottom side), Le. the corresponding yalue of this coefficient is the same as that of a local tangent surface of a wedge. By formulas (7.5.20) and (7.5.20'), in which we assume that ~N = ~ on the bottom and ~1. = -~ on the upper side of tht' uirfoil, at the corresponding points we have ;;b-2("+~)Il'M~-I. p.~-2("-~)!VD1~-·1
(~.11.3)
where ~ is the local angle of inclination of the contour calculated with a view to the sign fol' the upper side of the airfoil. With account taken of these data, the differencl' of the pressure coefficients on the bottom an(1 upper sides is
!ip = where ex' = VM!. - 1.
Pb -
Pu =
4a./ex'
(9.11.4)
490
Pt. I. Theory.....1I,ocIyn.. mics of lin .... irfoil lind II Wing
tJ.p can also be applied to non-stationary fiow if instead of a we adopt the value of the local summary angle of attack determined from boundary conditioll (9.6.32) in the form It is presumed that formula (9.11.4) for
as = -v/V ... = a + 00••:;; - oo;X (9.11.5) where; = x/b o, "i = 2zll, and 00:1:1 = O:l,U(2V ... ) [with a view to the chosen coordinate system, the sign of OO~X has been changed in -comparison with (9.6.32)1. Let us write tJ.p in the form of a series:
tJ.p =
+ p«lXlOO:l:l + p«l~ooz
pGa.
(9.11.6)
Substituting for tJ.p in (9.11.6) its value from (9.11.4), but using from (9.11.5) instead of a, we find the aerodynamic derivatives:
al:
po. = 4/a',
=
p«lXI
4Z1a', pf>lz
= -tU/a'
(9.11.7)
According to the tangent-wedge method. for all wings we have (9.11.8)
Knowing the quantity (9.11.7), we can find the stability derivatives:
c~=
1~ j j tpd'iii;
Awlb o
o
c;~~
rI?-
'.v.;bo J l~'dxdz
x~
m A t ij.
mlCfJ =
__ -
--f- j j pmJ,'lzdzdz
(9.11.9)
Oi"o
A6
m~='~
ri"r pGrdzdz.; -- - '"
J
).6
mz~=~
ll·i'l~ p"'--zxdxdz. o~o
OiQ
We locate the origin of the coordinates at the nose of the centre chord of a wing (Fig. 9.11.1). We adopt the centre chord bo as the characteristic dimension for m~ and OOz. and the span land halfspan u2, respectively. for m X1 and 00:.: 1, For such a wing. the equations of the leading and trailing edges in the dimensionless form are all follows: x_·_~ (t)u.+t)71",otan'l.. :Z }
__
0 - 110 -
(9.11.10)
4'1U'
XI=1!-= -1 + (l1;~t _
IJ~;:-t '-.,ot:nX·)i
cn. 9. Aerodynllmk Ct-lIrllcleri$tics in Un$leady Motion
491
fig. '.H.t Diagram of a wing ill the calculation or stability rlerintiVl's accord in\.! to the mcthorl 0[' i(lcul w~'dgcs
Let us write the ratio of the ccntrp chord to the span and the aspect rat io of a wing: b,ll~
2'lw'['w (~w -i- 1)1,
Aw ~ 1',8 - 2~wl1l(~w+ 1) b,l (9.11.11)
The tungl'nt of the sweep angle along the trailing edge is tan Xl = tan 'l.o -
(2b o") (1 - 1hl",)
Introducing (9.11.10) and (9.11.7) Into m.11.9). stability derivatives of a wing:
+
tl:....+,~~"'~3 (
i.\\
t~1I '/ n ) ~J
(9.11.12) W('
obtain the
(9.11.13)
III the part.icular C(lH' of rectangu lar wings for which tan Xo = 0 and 1'jw = 1, we ha .... e
(9.11.16) m~f' = -2/(3a'}
(9.11.17)
m~~= -2la', m~·= -4/(3et'}
(9.11.18)
492
PI. I. Theory. Aerodynamics of an Airfoil method makes it possible to determine only the aerorlynnmic derivatives without dots. The results obtained coincide with the accurate solutions according to the linear theory for inl'lniLc-span rectangnlar wings, and also for triangular wings with supersonic leading edges, at small Strouhal numbers (p* _ 0). For linitc-aspect-ratio wings, the tangent-wedge method yields more accurate solutions when the numbers M.",. and the aspect ratios ).w are larger.
1. Se.d,?v, L:1. Sirn~lari!y and JJtmeM,tJllal .1Iet/jod.< !II Jlechal!!(~, tran;:. by Klsln, \ltr Publtsbers, \Ioscow (1982). 2. Sedov, L.1. A Course Of ConUJII./Um .1fecllanics, ,"ols. 1-1\-. Croningen, Wolters-NoorthoH (1971-1972). 3. Kbrislianovkh, 5.A. Ob/ekanie tel guzolll lirl baLldkh skorustyakh (HighSpeed Flow of a Gas over a Bodr), !'\auch. trudy IsAGI. vyp. 481 (194U). 4. Bclotserkovsky, 5.:\1. and Skripach. A.K. AerodLnamiclll.'s1rit protZIJOd/!!le
~!~~~~~t,~:s :f~aC:!ft ~n~{~/\Vr;~ a~"s~~Ub~~IJ~!~'v~~~i:~::t\!~~~~~i:~:~
(1975). 5. Loitsyansky, L.G_ Mtkhallika ~hidk('s1i i ga:a U'luid \lC{'hanics), Xauka, Mosco",' (1970). 6. Pred\'oditelev, A.S., Stupochenko, E.\"., 10110\", V.P., Pil'!Shanov, A.5., Rozhdestvensky, LB., and SamuIJov, E.\'. Termodir/llmid~l'skfl' funk/sit vozdukha dli/a temperatur ot 1001) do It 0')1) K i datl"flil nt O.U(}l dft 1000 atmgratiA-i luakt.ii (Thermodynamic Functions of .\ir lor Tcmperatures from lova lu 72 01)0 K and Pres~ures irom 0.001 to tOOO atm -Graphs of Functionsl, Izd. AN SSSR, Moscow (1960). 7. Prerlvoditelev, A,S., Stupocbenko, E.V., Samu"1lov, E_V_. Stakhanov, J.P .• Pleshanov, A.S., and Rozhdestvensky, LB. 1'llv/ilsy fl'rmJdinamlc!teskikh fu.nktsii vozdukha (dlya temperatur 01 61)(}() do 121/1)'1 K r dav/tali ot 0.001 do IIJ(hI atm) [Tables of Thermodynamic Functions of Air (for Temperatures from 6000 to 12 000 K and Pressurcs from U.001 to 1000 atmll. lzd, .'\N 5SSR, Moscow (1957). 8. Kibardin, Yu.A., Kuznetsov, S.I., Lyubimov, :\. :'01"., andShumyatsky, 11. Ya. Atlas ga:odinamiclltsklJ.-'/ funktsit pri hol'slti!.:11 skor08tyakll i vysokikh temperdturakh lJosd/Uhnogo potokll (A tlas of Gas-Dynamic Functions at High Velocities and High Temperatures of an Air Stream), Goscnergoizdat,
ltloscow (t961). 9. Kochin:N.E" KibeI, LA" and Roze, ~.V. Teordi(/reskdya gidromekhanika (Theoretical Hydromechanics), Parts I, II, Fizmatgiz, Mo!lCOW (1963). 10. Fabrikant, I.Yn. Aerodinamika (Aerodynamics), Nauka, \losco\\' (t964). 11. Arzhanikov, N.S. and 5adekova, G.S. Aerodinamlka hol'shikh skorQstel (High-Speen Aerodynamics), Vysshaya shkola, Moscow (1965). 12. Irov, Yu.D., Keil, E.V., Pavlukhin, B.N., Porodenko, V.V., and Stepanov, E.A. Gazodiaamicheskie Junktsii (Gas-Dynamic Functions), lI-Iashinostroenie, Moscow (1965). 13. :,!khitaryan, A.:'>1. Aerodinamika (Aerodynamics), \lasninostroenie, :\Ioscow (1!"!jfi).
494
References
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dYllamic~,
fundamental, 12!J, 201, 3119 syH"nl, 1291(, ilI4 Grollll'ka's, UIII, 3G JlOdognlph. 180 J1ugolliol. 172{ itltl'l!rn-difTt'rctltial, 25/1 kinpm;ltifs, fundanlC'nlal, 201 La1!ran!{I', 135 Lapla'orce{s), aerodynamic, airfoil, 293f body, 27 comrlex. 246f conversion to another coordinate sY,'ltem, ItOf dissipative, t27 drag, 38, 42, see also Drag gyroscopic, 403f
l'orctI{s). lateral. :~,:) lift. 38 . .'.::!. ::!;iOr. :.!54 ((at pl;.ltc. 248, 3113 muimum. 47 Dearly uniform Dow. 236 . ,386
(;a5, equa\.i()ll~, l2\lif. l·'~') [low from res(!l'\'oil·, 1SllT heating, 58ff ideal, 134, 149, see 1Il.,;(> Gas, perfect interaction with body, 15r, 18 ioniz.ation, tWf
ri;c~i~f~go~rff\~~1~,~,!)~g3!
mass, :.!7 extern;.ll, work, t2ii OD rnOViu!! body, 25ff normal, 38, 416[ producl!d by pressure, 293 ponderomotive, 27 side, 38, 42 suction, 24~. 382fI correction factor, 383[ sideslipping wing. 305fi triangular winq, 362 surface, 25f. iOil work. 12-41 viscous. Viti ForJ!lula. see also Equation(s) Blot-5avart. 05 conversion, coordinate sy~tem9, 82ij
Euler. 117 Karman-T$ien, 268 Prandtl-Glauert, 26B. 302, 306 Reynold~ generalized, 33r Sutherland's. 63 Zhukovsky. 248 Zhukovsky-Chaplygin, 247 Frequency, oscillations, 414 Friction, $I!t a/so Viscosity in turbulent flow, 3211 Function, conformal, 2'.Of
~~~tY:iidf~trt:Jtion. 354, 358, 360f
potontial. 79, 243, 354f, 367{1, 457, see also Velocity potential derivatives. 458 doublet, 3541 gradient, 80 stream, 89f, 9B, 202 Gas, see; also
Air,
Flow(s), Fluid
::l~~r~~ili:r' el!~tr~~ity~8f1945211
diatomic, mean molar rna9S, 70 diffusion, 121 dissociation, 60, tB9H dynamics, Hi, see alsQ Aerodynamics, high-speed
mixture, 67 mean molar ru;J.~, 70 parameters, at stagnation point. 191 perfect, see olso Gas, ideal calorically, 65 equO-tion of state, 65 thermally. GS recombination, 60 stream, configUration, 149f viscous. (low in boundary layer,
'34
Gradient,
~~~::r 've1!~ity,
32
potential function, 80 pressure, 107 velocity, 34
Half-wing,. inllnile triangular, rn Heat. speclrlC, 61£ Heating, acrodyn:;l1oic, 15, 18, .-':\ Hodograpb, t 7\)fi
H~b~~~~!iS~f
reverse influence, 17 continuum, 16, 20 harmonicity, rm~, intl'raction, 402
ir!~~~~:l.an s:~;:~f;o~tc
supel's