s. · 2020-01-17 · specific impulse the parameter linking the exterior: ballistics of vehicle and...
TRANSCRIPT
THE EFFICf OF DEPARTURE FROM IDEALiff OF A MULTIPLY IONIZED ,i
MONATOMIC GAS ON THE PERFORP..ANCE OF ROCKET ENGINES
by
John Noble Perkins "'
B. s. in Aeronautical Engineering
M. S. in Aeronautical Engineering
Thesi.s siibmitted to the Graduate Faculty the
Virginia Polytechnic Institute
in candidacy for degree of
DOCTOR OF PHILOSOPHY
AEROSPACE ENGINEERING
Apd.1 1963
Blacksburg, Virginia
3.
... z ....
INTRODUCTIO!t • • • • • • • • • • • • • • • • • • • • • .. • • • • • • • • • • • • • • • • • • • • • • • • • 5
EQUILIBRIUM TF..ERMODYli.M-UCS •...•....•..•.....•..••.....•.... 2.1
2 .. S
2.6
2.7
1
2
................................ . . . . . . . . . . . . . . . . . .. . . . . . . . . . . . . . . .
.............................................. ..............................
........................................ o • • o • • • •. • • • 1' • • • " • • • fi • 41 Ii • • II • • • • • ,i, • • ilJ
taw of .................................... •••••••••••••••••••••••••••••••••••••••
EQUATION .............. • ............................. .
.............................. for Particle
11
11
13
15
16
17
20
21
µ ................. • • • • • • • • • • • • • • • • • • • • • • 28
.3
METHOD OF
4.1
4.3
5.
5.2
µ = r •••..•••.••.•
••• Ii •••••••••••••••••••••••••••••••••••••
........................... 34
••••••••••••••••••••••••••••••• 37
...................... "' . CALCULA~IONS •••••••••••••••••••••••••••••••••••••
ti •••••••••••••••••••
•••••••••••••••••••••••••••••
Ps.ge
6.. llStlLTS .AND CONCLUSIONS ••• ,. ........... • ...... • ........... • •• • •• ,. • 46
1. smtlAll.t ••••••.••••••.•.•••.•••••.••.• --. ............... • .. _............... 49
8. PllNCtPAla: SDmoLS •• •. ~ •••• • •• ·• ........... • •••• •· •• ~ • •• • •.•. ,. ., • • • • • 50
9. ACKNOWLEDG!fBNTS ·• • , a ........ • •· • ~ • ~ •• • •••. •: •.•••.•• • • ·• • • • • • .. • • • • • • • 53
10. ~CBS •• • .-•.•.• ot1i •••• , .... • •- •. , ~ ••••• -•••• • ..... • • ••••• • ••••• , • •. 54
1.1. 171.TA ••••·••••••·•·••••-•••••~••-•··~··••••••·••••••••••••••••··•••••• 57
AitPDIJ)lX A •••••••. -. •• • • •-•• -• ,, • ........ • •••. ., •• • •• • ....... • •• ·• •••••. • • 58
A.1 Collision lntegra.1s for lnela.stic Collisions ••••••••• 58
A.2 &$action 'tem$ for µ • t:· •............................. 62
A.3 Derivation of Reaction Velocities•••••••••••••••••••• 63
AP'PBNDlX · B • ••• • ............ •· ............ • • , ·• •••• • ••••••.••• • • • • • • • • • 65
B.1 Equilibrium flow Equations••••••••••••••••••••••••••• 65
B.2 NonequiU.brium Flow Equations ••••• •• •• "........ •• • • • • • • 67
B.3 Reaction Velocities for Argon ......................... 68
,Pase
Figure l tllusttation of Convergence of Starting Procedure • • • .. 71
Figure 2
Figure 3
31igui-e 4
Figure 5
Figure 6
Figure 1
li'igute 8
1!igure 9
Figure lO
Figure 11
Figure 12
Figu'te l.3
Figure 14
Figure l5
Figure 16
Ionization fraction vs. Area Ratio
Ionization ft,;1.et;ion vs. Are.a Ratio
Ion:i.zat:i.on Fra.etiO'i.1 V$.. Area Ratio
l:onization Fraction ve. Area Ratio
Ionization lh:act:lon vs • .i;\t'ee latio
' ......... ' ... •· ....... .
.....................
.....................
.................... Temperature vs. At'e·a Ratio ................ , .............. .
'.l:eniperature vi. Area. Ratio • • ............................. ..
Teraperature v-s.. .Area Ratio ............................ .
temperature vs. At-ea Ratio•••••••••••••••••••••••••··
Tempe:1:ature vs. Ate:a '.a.atiQ ................................. .
Velocity vs. Area Ratio ................................. .
Velocity vs. Area Ratio •••••••.• , •••• • ••••••••••••••••
Velocity vs. Are$ Ratio••••••••••••••••••••••••••••••
Velocity vs. Area l:t.atio ................................... .
Velocity vs. Area Ratio •••••••••••••t•••~··••••••••••
72
73
7l~
7S
76
77
78
79
80
81
82
83
Bl~
85
86
Performance calculations rockets :ln flight show that the
velocity of the vehicle at: burnout increases linearly with the specific
impulse and decreases 1d.th an increase the inert mass. the specific
impulse, or thrust per unit rate. of flow, is determined chiefly
by thermodynamic properties of propellant gases, the operating
cu)l"lditions tdthin the motor., and geometry of the nozzle. Since the
specific impulse the parameter linking the exterior: ballistics of
vehicle and the interior design of the power plant, it is imperative
that the specific impulse developed by the rocket engine be known to a
high degree accuracy.
1:he assumption tht.tt the working subetance (propellant products)
obeys ;he perfect laws provides a &imple and rapid method for
estimating the specifi~ impulse a given tocket engine, and bas been
treated extensi:vely the literature (see, for example, refs. 1 .. 3),
While this method does not, general, yi$ld sufficiently accurate
results for practical applications; it does point out the important
fact th.at the specific impulee increases id.th an increase in the chamber
temperature and decrease$ with the :molecular weight of the combustion
product~. High $pecifie impulse thu$ results from operating at high
temperatures and/or low weight propellant gases, Since the
choice of molecula:r weight of the propellant gases is obviously limited.,
the only alternative, obtaining high specific impuhei to heat the
working subttanee to extremely
concept of tr$ating tbe propellant produ<!ts a* perfec:t gas.es 1s no
longer applicable. That is, the eltcitat.ion of dissociation and ioni•
dete:tmirling specifie impulse is no longer a simple one ..
ln there ia only a the effect::i dissociation
ot1 speeif :Le impulse and evren is known about the effects of ioni•
3 10 eeconds 1 or more, ate to oe(:Omle a reality, it will be 11ecessa:ry that
problem ionization
theory for
for the case
its ~ssociated eff~cts on rocket performance
molecular dissociation and recombination
molecular·dissoclation 's theory
adequate; however, once gas becomes ioni~ed, tbe con•
as an ideal gas is not $0 apparentj, However, Bray' s
diverge from equilibrium. was also found that emi.lt'i'Y radiated as a
from adiabatic flow.
thesis to study tbe equilibrium,
flow of an :c•times ionized gas in the nozzle
engine including
radiation. the investig:ation aasumes an ionized gas which is
in thermal equilibrium. (1.e •. , a one temperature f1u(d) and wbieh is
eleetrically neutral. Also, dis.sociati.011 of a mole~ular gas is
essentially complete before 1onizat.ion becomes ~ppa:eeiable, only mon•
atomic gases will considered.
the equilibrium flow eol.ution is used both as a refe1.;ence for
measuiing departure$ from equilib,:ium as initial conditioni for the
noneqt.tiU.brium calculations. The equiU.briwn ca.1culations are based on
a system of algebraic equations consisting of th~ isent:ropie oondition.,
law of mass atttion, an equation of etate, and the equations for the
conservation of raas& and ~nergy • 1:hie system of equations is nonlinear.,
and iterative methods solution. lquilibrium flow
calculations an upper limit speei£1c impulse since a.11 of
the energy invested in ionii.ation. ,iegained,.
The (i.e. fixed eompQsition) flow solution gives the lower
limit for the specific since none of energy invested :ti regained.
these ealcula.tiona are relatively simple since gat behaves as a
'rbe nonequilibri'U'nl solution accounts fot the fact that the internal
structure the gas lag behind that required for thermodynamic
equilibrium., and, as a result,. may be considered as the "eorreetH
solution. The ®n$quilibrium calculations differ :from equtlibi:ium or
frozen calculations in that the composition of the gas is governed by
a different:l.al equation of fi~st•order which will be referred to as the
rate equation. Thus, the calcul~tion the nonequ:Uibrium flow involves
the numerical integration ,of a system of first .. order 1 nonlinear differ
ential equations.
The derivation of the equations governing the equilibrium, frozen
and nonequilibrium flow ts based on the assumption that ionization is
due to atom•atom, atom-ion,. and atom•eleetton collisions. Since the
methods of cbemical kinetics fail iii. the ptesenee Qf Coulomb interactions,
recourS1e is made to the methods of kinetic theoey. The kinetic theory
.approach con,iats of stating the fundamental kinetic equations for the
ga.s c01.1sidered (Maxwell•Bolumann equations) .which are to be solved at
least a,pproximately. 'lhe solution of the Boltzmann equations gives not:
only the macroscopic equations of mot.ion, but also the equations of
transport for the single particle components, i.e. the rate equations.
The kinetic theory represents,. therefore, a uniform start.ing point for
nonequilibrium flow problems ... lt: tnU$t be pointed out that since quantum
statistics include Boltmnann statistics as a limit:i:ng case, it would
have been more approprLate to use quantum statistic$. 1-k)wever, their
use results in increasing the complexity of the al;eady coinplicated
expressions of the thermodynamic properties and therefore, sueb a
refinement not seem to be warranted at this stage.
The the,:modynamie variables are derived etarting from the appropriate
express.ion for the Helmholtz free energy. ln this expression two approxi•
mationa are employed. The :first assumes that the rth ionization is
complete before the r + 1 ionization starts; thus, three species exist
in the plasma at a given time. ?he second assumes that the eleetronie
partition function., which is represe11ted by e.n infinite series., can be
approximated over any temperature range by a constant. fot the singly
ionized case this constant may be taken a& the degenlt!racy of the ground
state.
rhe de.rivation of the rate equation req.uires an investigation of
the rate$ at which ioniiaation and recombination take place. Ionic
recombination is a t:eh.tively complicated process since the electrons
and ions can recombine in several ways7~ Also, the presence of Coulomb
interactions excludes the uee
kinetics 1 which assumes that
the methods of classical chemical
rate constants are independent of the
concentrations 8• Examination of the Helmholtz f1:et energy taking into
account the free energy reeulting frol'n Coulomb inte,:ac.tions showa that
the equilibrium constant is a function of both temperature and con•
centration. This implies that the reaction rate constant$ .are functions
of temperature and concentration if interaction taken into account.
ln addition to the fact that Coulomb interaction, preelude the
use of cb.uieal chemical kinetics, their presence also gives rise to
difficulties in calculating the Helmholtz free energy and certain
collision integralslt As a result of the long range Coulomb forces
there ,....,. .......... ;;;;> an energy of interaction between the eha:rged particles.
This energy of interaetion is a function only of the distanc:e between
the particles and, thus, ma.y be tt:ea~ed as a potential energy whose
total derivative defines the forces. However, the presence of this
•10•
potential causes certain integrals in the expressions for the free
energy and the scattering cross sections to diverge unless some method
the potential is etnployed. ln the present work, the
Debye ... ffuckle approximation :ts used for cut:•off distance. ?he
choice of the J)ebye•Huckle theory due to the fact that it is the
only self-consistent theory availab1e 9• Because a number of assumptions
t1ere involved in the formulation of the theory" the coriditions under
'Which valid are not well generally
believed that the Debye.,..Huekle theory is valid.as long as the Coulomb
en,~rg:y does not exceed the thermal energy 10 ..
Sample calculations are presented for an inviecid :flot1 in a
Coulomb interactions result in an increa.se the
impulse and a decrease energy, enthalpy, etc~ ;
and an ap1pa1~e11,~ decrease in the ionization potential.. However, the
specific impulse at'(! insignificant
from a practical viewpoint,
more
· to
2.1. Helmqoltz.rree Eners,:.
as the .sum of two parts: (1)
derivation of
One of the
a·gas
F. Given the free
Helmholtz free ~ergy uaa:y 'be expressed
action, FP, and (2) free en~arg;y reaulti'll8 from Coulomb interaction.,
F 1 • That is cou.
(2.1)
the an
(2.2)
where, under the assumption each proee,s of ionization is
essentially complete na,rn?~ the ne~t begins, subscriptµ tal(QS on
the values r + 1, and e. llebye•Huc.kel apprC>ximation leads to 11
263 . ·. 1/2 :, coul. • ~ ... 3 ( k:l:v ) (
µ
2 3/2 N z ) µ µ , (2.3)
for the free energy due :l:nte;1raction. ln Et.\~ (2. 3) the 1µ. are given by
=r (2.4)
Substitution of Eqs. (2 .. 2) and (2.l) i11to iq. (2.1) gives for the free
energy of including Coulomb interactions
F • ... N - k'l V.
Note the Nµ are not :Lndep$ndent of each other; electrical
neutrality requires
M.+N. 1 .. =N • r . t+'·
AU of
(2.S)
(2.6)
(2. 7)
2.,2 Partitionrunctions. :ror all cases considered herein, the total
partition fQnction may ba written as
, (2.8)
where Bi
respectively. Thus, for the atom., ion, and el.eett:on,
(2.9)
(2 .. 10)
and
V • (2.U.)
Equations (2.9) and (2.10) assume that the reference energy level is
that the neutral atom, that it the average value of er E
over temperature rang~ !n which r~ti1nes ionized atoms exist,
Note that ain.ee the Htemperatute boundariesn of the ioniting process
Ar to may be computet:121:1 it iB necessary to compute only the
first few terms tlle infinite series representing e • . rl
Using the above expr.es$10ns for partition functions in Eqs.
obtained as follows ..
defined as
, (2.12)
or,
ki' p -- v
Lett:b1g 11 = N/V be
density the
end
3 k .. ·. ·.. . ·. .f!I. (.· :It p ~ - tll (r + a ) • ~ · · ..... ) m ·· ;,r 3 ld.'
•
atomic nuclei
given by
'
(2.13)
noting
(2.14)
a.re
(2.15)
the (r + 1) .. t~es 1onU:ed
written as
(2.18)
unit mass
or
l Tr + · · · (1 "'" a"" .•. >• ·;-.· .· + t+C\,: • 4
where Tr • 11/k is a "ebaraetei:'i$tic:r temperature of the r•times
ion1eed atom. Note that Tr = 0 for r - 11 by definition.
i = u + p/p • (2.21)
Substitution Eqs. (2,18) (2.20) Eq. (2.21) yields
de.fined as
(2.23)
where r f :;: ,,_ • pV • (2.24)
Using Eq$. (2.S), (2.20), and (2 •. 24) i:n lq. (2.2.3)
k s=m.
where
(t
composition
atraint.s
Eq. (2.5)
a > r. · i • loa ( .Q , ~· S!. ··1,. + r L2 Q.1n 3..J
l•a ( ....... r) ·<'.'\·
(2.25)
(2.26)
tb~ ionizing.monatomic A$ is well known, eq,uil:tbrium
by lqs. (2,6) and (2.7). Thus, using Eqs. (2.6) and (2.7),
be ,,:d .• tten as
0r J 0fr+ll • log ( u·r·· ) + (N • N~.) log ( · < c ) ..... • N • N r
oe 2 3 . n 1/2 lr 2 ( r. N • "'r. · ) + 3 ~ ( 3 ··3 . . l (r • l) Nr. ,,~. it T. V ,
(2.27)
r 2(r + alt) . . l. I ...... · .. ·. . . a , L (t" • 1 + <-,;.-) ..J (2. 21)
or, substituting the partition functions Eqs. (2119)•(2.11)
2(r+a:r) . . a
(r~l+2 etr> J .
(2.28)
the condition equilibd.uni; is, the lali .of
mass action.
( SU?) ;Iii. ·. d . • ' I) s
(2.29)
emptoying Eq. (2.18)
l . 0 ) } +-.·(l·- . p 2 (2.30)
Taking total derivative of (2.iS) and setting the i-esult
to aero gives (dT/dp)$ of (d a1/dp)
8, which when sub•
stituted into (2.30) gives
8r o . 3 (r • '\-) log ], °'..
1 . . + 2 log (ET) + log .. ( .. 1 • . . )· -
Ot+l,Q · O!t.' t' · . T at p
( .. ) .. m
(r + (% ) ..____ .. r 3(: + a )(3 + a) a ·]. do · a -. · · r. . ·. ··. · ... · .. (l + .......__~ ........... - ) ( -. r ) J· ,
r • l, + 2 ar 6 + cr r .. 1 + 2 dp s
(2. 31)
where, for equilibrium, (d CY.rr;ldp)8
!s fou.ud from Eqjl (2. to be
! 0 + t1) ~ ~ ......... l
6(:t· + ar) a l6(r + or) . 2 -.· .. 2+·. .•... 2(5 (r .... 1 + 2 a,;.) (t • 1 + 2 ~)
1£ .. ·....L.· .. l ... ·T· • ... '···.·.?.... J'"'.' r'/' ... \.· do 1 {. . 't . ·. • ,: ,.-r • VJ (d/\ =p .c6t,>< t+\ r)•
1 . 3(r + a~) --1 •·1
[ 2 + (r .. 1 + 2 a,/ J O' J ' (2.32)
lqs. (2.18) through (2.25) shows that the effect
Coulonib interact.ions,. wu.J1.cu are represented by the quantity a 1 is to
decrease the pressure, enf!rgy, enthalpy, entropy of the gas.
Equation (2. 28) shm-ts that thete an apparent decrease in the
ionization potential.
Equations (2 ... 18) u, i, etc .. as functions
p, 'l, a.nd C\1
• In the case of equilibrium, ~ is
given by law of mass a.etion, lq •. (2.28). l.n tha presence of non•
equiU .. brittn1 an equation for '\:' whi~h the rate equation, is
obtained for the assumed ior.diation mechanism frcnn kinetic theory
considerations. This problem. the next section.
It1 ode~ to oJ,tain 4s eQmplete a picture tlf poss:tble of the flow
of tile iord.itng 34$ tkreugh the XlO~z1e of a r~t engine., it is
ntc.,,uaar;y ~t the ut11u1t to which the flw depart$ &om equilibrium
ha ~t!Uted. As wall Nntio®d previouflY, the -rate equation for the
it•f.times ionis.:tng gas will he detemin-ed from • Jyatem of equations of
the Bol.tanana ~pe~ ln add:i.tion. to col.U.aio:ns which t:esult in no
change ill the nwnber of partielest the followi:pg co1.1f.tioris, which
· at:e aa,umed to b.rtng about the ionii•tton, wi.11 b6 eonside~ed;
0 1 r ,
13·1 ,;
(3,.1)
To .deisortbe the tolU .. sion eq,u~ti~s., a eetni*'quantu:ra•mechanical de• .12 . . . · ·
sei-iption $.$ used ·• l'o; the t.rans1atiori.a1 tt10tion the c1asa:tc-.1
deJaeription ls. t.'etained; but for the 1nte.f1Ul.1 motion, the atCtlls and
ions are eontidered aa betug able. to exist in difftin:-ent iatEJmal ene"tgy
states" !he inten.ta1. energy is deuot$d by et.ti' where., a, beftn'e,
µ stands for an abbreviation for i = N, L (atoms).,
1 = N', l,i (ions). N., N' are the total quantum numbers and L, L 1 are
and
has
£or rotation.
energy eri·
advantage
course, e . ii 0. A .(v ., e . ) e1 r r ·r~ r ... tin1e.s ;,ll., .... ~ ... .,.. ... ,...,...... a.tom with velocity "r
tha state of a part:ic le
total
e,tistence of total inverse collisions
one of main assumptions in derivation the claseical
3.1. J~e Bo1t~mann Bguat;lons. With the abbreviation for the velocity
diin:ribution function
of. 1 of . c,£ . of . = ~ + v . ~ + f (;r, t) • ~--"~ = ( ·~ ) . ,
µ µ oVµ coll.
df where ( d~& ) . . is an abbreviation for the collision term.
coll ..
rate at which the velocity distribution
(3.2)
(3.3)
It
is being altered by encounters and may be exrn:essad as the sum of
collision terms,.
of . (~) =
ot coll.
of elastic
( '<,~1. ) . + · eoll • .,j
'£hat is, the eoU.ieion term may be divided into encounters tn which
the number paiticlei remains conE1.tant (defined here to be elastic
collisions), those in which the number of paiticles changea
(;i:nel~i;tic col.lis.tons).
an ela$tic eneountet, oonsidtat' the eollieion
Jlµ(vµ, ~µi) + Av(v,,., EVJ)~Aµ(Vµu ~\.i'k) + t\,(Vv" '\,p•> • (3.5)
the e~:ptession atµ, .elastic
< ot > dv di dt eoll .. .,v µ
(3.6)
$ignifies the net increase, during
A (v , e. ,.) (without restriction to µ µ. vi
in the number of particles
velocity of the latter
particles). Thi$ net inerease the difference bett1een the numbers
of particles A , within df., which during µ
Qv1ing to encountera the particles A • 'V
enter and leave the set,
nuniber Qf pattieles to the set during tim.$ d.t, owing to
the pa:rticul•r group of encounters particles 4v<vv' E11
j), i$
equal to
f . i f .~ O'(V. E . 4 • V E: ·J .... ,v ... • '.µ";. f • Vv. ·I E I ) dv dv " d:t t df dt " µ · VJ ·· µ, IJ.•' \I 11 ~ • "" ' vp ·. V µ • \I '
(3. 7)
to
fµk,i :i\,p• a(\1 €µk,H V11, 6vp'/Vµ Eµi' VV Elli dvV d~, dvV, dr dt •
(3.8)
Since, number particles
Eqs. (3 .. 7) {3.8)
(3.9)
Defining peculiar velocity of~ particle of speciesµ as the
average velocity v0
, that
...... . ..... ~ :\ .. ~ ...:a,. V (v , r, t, == v. • v , µ µ . µ 0
the velocity distribution functions may be written 14
where
u,1ng lqs. (3.11)
requires
then,
. m . .. .. ,
"'._.. . ·. ~. V . + 'i . j k! 2 µ tJ.l. [ 1 (" u .. 2 . ) l
exp ,.....,. ______ ,.,._........,....._~-
e ._ 1 exp(--~l kT
f 1 .. (v_ > • µ' ,µ <v > • µ
(3.10)
I (3.11)
(3.12)
(3.13)
q(v .. e .·..t.' µ µ ....
Usins (3.14)
(3.14)
Eq. (3. 8) ""'""'""'·"b '\-11th Eqi. (3. 6) and (3. 7), the
probabilities fQr be obtained by a
generfl~liiation of the above s.ri~~tui £0-r t.al.af.ttie encounte,:t. As an
~ampl.e of an inelastic. coll~ef.011,
By analogy with Eq. (3 .. 9), the condition for
be local ,quilibrium
(3.16)
~eaetion (3.16) to
(3.17)
Subst:t.tutins Bq.s .• (3.11) into lq. (3.17)
m · '" 2 .. . ·· )· . ( .. e 2 ) ( y(r+t)• + £(t+1)p• + 1(~1) + · .. 2 "e• • '
(3.18)
~r:~ ne • g ( 2gr:;·o·) ,:3/Z eltP • ( T~! .. Tr) .. (;~;;~) a] '
i:r r(~l)e· cr~(ttl)e = A er ,:,: . ,
where
rr c e
i-(r+l)e
I:lavi11.g established the t:eJ~a1;~or.ls between the t,!'~~'t'\a'i
probabil.itie,, £'1111 expression of 1 .
:( ?,~ · ) . . • •. . . , · may h~ written as coll.
( d.· .. f· Y .. 1 )··. at · · •· • eoll.
th~ collision
J (et) µ.i (a)•
(3.19)
(:l.20)
(3.21)
(3.22)
(3.23)
with the following abbreviation, 14 fot the elastic collision term.a;
(a) (tr) (rr) (re) J sJ.,. +J ... +Ji ,
t.i (a)' r1. (rr) • (r(r+l)e)• r (re)' (3.24)
(a) ((r+l)(:r:+l)) (r(tt-1)) 3
(rtl)t (a,),= 3
(r+1)1 ((r+l)(r+l))'+ 3
(r+-1)i (r(~l))' +
(b+l)e) J
(r+l)'i. ( (r+l)e)• ,. (3.2S)
(a) (ee) (te) ((r+l)e) J . $:=J ... +J ... +J ' a (a)' e (et) • e (re) ' · e (rt+l)e) *
(3.26)
(a) (rr) (re) (rb+l)) J ..... 1.. s 2 J + J ·. + J.. +
4'. (fl)' rt (i:(t+t)e) • J>i ((r+l)ee.) • d. ((:r+1) (t+l)e)'
(r(r+l)a)
(rit')'
(a) (r(r+l)) (r(t*l)e)
J(t+l)i (f;i)' = J(t+l)i ((r+l){r+l)e)'+ J(r+l)i ( rr)•
(h+l)ee) ((t+l)(r+l)e) J 1.~1) • · · + 2 4(.....t.l·) ." ,
\P' i ( (r+l)e). I..T. l. (r(r+1)) I
+
(a) (re) (r(r+l)e) ( (r+l) (t+l)e) J = J . + ·J . + J • e O)• - e ((r+l)ee)' e (ri-)' e (r(r+l))'
(3.29)
(3.30)
(t) (3.31)
etc. wm;r'.e ,-·; means the summ.a.tion L, (i)
taken indices except i
(of co,urse, the subscripts r., r,,t,-11 e are not .... ....,,..11,p.1.·,1.n: .. .i.,;;:.u to be indices
following properties:
(3.32)
collision integrals.
3.2.
Let fµ-1 some p,:operty of the patti.cte Aµ i fJ ,. (v , r, t" G .i) ; ..... . ', . . . . . . µ1· µ· . µ.
µ = r, t+l, Eh ''the mean value of properties iµi is d$fined by
(3.33)
r (3.34) ,J
•\1.iµ are tl1e densities of the property iµi iu f•spac,a. The
eqvations transport for mean val~e (t\,. follQW Sqs. (3. 3),
if thetse equatto.n.s are multiplied 1\.t.:tdvtJ., integrated Qver vµ, and
summed over tc
r ·. .· of i ..... J t .. 1 ( ·~ ) . .. dv.. • .
" f!'¥' · ···· coll. .f""
(3.35)
'l!he e~lUations of trmlsport fo:t the gas are thu$ obtained by subst.ttuting
f .. the quantitieEl µ1 .
2
equat:i.on
+e. 4 +1 , µ. µ. (3.36)
elf • ( ~. ~ .. 1
) . dv , 0 coll. JJ.
(3.31)
or
on. d ~. ·. . . + - • n (v + V ) ;;:· R , at ot µ · o µ µ
(3~38)
V • V • V µ µ. 0 (3.39)
is the diffusion velocity of tlle species µ 1 and
r of .· ( I ~-sM\ ) . . dV
d ot coU •. · µ (3.40)
of produetion of ps:.rticle$ of species µ. Sin.ee only
the b~e1astic colUsions, lqs. (3.1..)., eontd.bute to 1\,., Eq,. (3.40)
may be written
a • µ
of . inelastic ( ~.i >. . dV , at . 1·1. L fJ. co .. •JI.\.
(3.41)
(3.42)
The ecf!ations (3.37) are not independent $ince conserva.tion of mass
requires that
µ
•30·
tn R = 0 , µ µ
( r . .,.1.·.·) n ·. + rn ... · .. l. "" n.. = 0 • r ff e
(3.43)
(3.44)
l.l. 111.a· Rate Bquation for the Species µ = t. Since the f ·i· are . . µ
as.sumed to be Maxwellian1 V ~ 0 and lfis. (3.38) may be -written µ
(3.45)
(3.46)
(3.47)
Substituting Eq. (3~46) into lq. (3.45) gives,
D(m n ) .·.. m. ti Dp MMr .. ~~=mR
Dt p Dt µµ • (3.48)
Da .......!. = •. :Ot .. (3.49)
I ij
(3.50)
(3.51)
the "co111tant" o.f the law of mast action defined
lq. · (2. 28). the quanUtie,s urt' ut·(,utl)' ure. are the ret.t.etion
velocitiet and fit'e. g:tven by (sae Eq. (A.24))
whete la;.t-1 • lvr ~. f,r\ , tte • ., Ql)d;p the Q't •• the co1U.ston croes
-.ctions def1n$1 by
ICn:J ~ "'J '\,(=l)• .tfr; dV(r+l)' a;., , (3,SS)
rb'+l)
I '"(JM.t> I ~<i-+1> • f ct ... ·1 ·. . .•.. ,, <i.i+1> • 8<.+1). ,. "• •. ·~ . .. (t.+.)b+l)e. (3.56)
tbe crosa•sections are known for the. colU .. sions in
question, Sqs. (3 .• 52) .... (3.54) be intagt'ated to yield the reaction
velociti••· Once the ,teaetion veloc;it:les have been detet'nlined tbe
rate equation, Eq. (3.-49)., compl$tely specified. ln t;he following
seetton ineocyoi-ation of this rate equation with the quaei•one•
dimensional flow equations is along with the met.hods of
solution for equiU .. brium. and f:ctnien flow case$.
This section sets down the method of analys:h, for the quasi.""'one•
dimensional equi1ib:d.um, frozen, and nonequi1ibrium flow of the real
r--time$ io1;d.2ed gas tbr<>ugh '1 ccnvel:$ing•diverging noza1e. for each
ease conside:red, the neceeaaey system of equ.ath'>ns written down by
a suit~b1$ combination the one•dimena::lonal £low ~quat.ions with the
equations of 1ection(a) 3 and/or 2. The present investigaU.on thus
eon,ists
order.
t.h;ee separate part• which wilt be treated in the following
these flow
properties necu~s-sa~ not only to gain an understal.lding 0, depart•
u1:es equiU,brium, but to obtain ixd.i:tal conditions for the non~
equilibrium calculations.
'?he ~quilibrium calculations are l>ased on 4 system of nonlinear
algebraic eq,u~ttons c,onsisting of the one•dimensiona.l expressions for
coufJervation of mass and energy;
(4.l)
(4.2)
togetlle't with the thermodynanie t'elationships of lqs. (2.18), (2.22),
~d (1.2S)l
(4.3)
,., ... r ( ; ) • j + ! l log (DT) +
and the law mass act.ion, 2tg. (2.28)t
T .. •i 2(r+a) ( . £ti ... t ) - .. . . . ··,:
(t"• 1 + 2etr)
(4.6)
where quantitie.s at a sonic throat are denoted
:s0
are the total entbalpy and entropy, ltespeetively, which are const$:lt
for equilibrium flow.
p* v* A*, has been determined. the flow is isentropic ,.
speed sound at point.
g .·.. ··.·· 3 ( .... r,o..,_ ) + _ 2sr+. . l. ·. o a ,
where., (dar/dp)8
is
a. simultaneous Qv.i:,.u.t..11-1.1,.~
is then calculated
are
(ET)+
41 (4.3)
t:emperatute (T >
downstream of the th11oa.t)
simultaneously for a
The velocity, which
from Eq. (2 ... 31)
(4.6)
da ~1 < or:{ > s J'
(4.7)
p* are speeif:i.ed,
...,. ....... _.;-o r? and p*.
(4.4)
Eq. (4!0 S). 1111.ally, the.
the noazle
for upstream of the throat., and
solving Eqs. (4.S) and (4.,6)
$pecifie impulse,
fol.101-,s fr.om Eqs. (4.2) and (4. 4), and iq. (4.1) then gives the area A 1 •
Stagnation conditions a.re obtained from a siwltaneous solution of
Eqs. (4.4); (4.S), and (4.6).
4.2. l'ro~eil Flgw £9.taagionp. ,;b,e f~ozen f-t.ow calculations provide the
lower limit to the ~pec.ific impulse. the. composit,icm is astumed t:o
remain conftettf!, m<i thus, the f:r11n:ep. flow eal.eulations a.re identic.$l
to the pet:fect; ~u ea.1culatiQnS. !hat is, for a specified value of
11 pi& ealeulated directly from iq. (4.5),. l?he remain11,1g state an(l
flow properties folJ.ci;1 from Jqi;,. (4.1).,(4 •. 4)* Note that the ca.lculations
a~e 4a:td.ed out ouly for tbs:~ portion of the noia:ale whtch :i.$ dow&tream
of the tllJo~t., and at'e lla•~ on the equtU.brium tnaa!ll £low rate.
4.3. Hpnawail1'briµm !1• lifat,ione. Jf the ~eaetiOll t~a for the
eo1l1$1onl given by lq$... (3. l) ·l:W~ of th$ ,_. otdei as the chal!'4etertetic
tren$it time th~ugh the flow belng considered, tlle f1owwi11 depart
from e4ui11brtuin .. · As a result, th$ f \ow, while ad:btbat:tc, is no longer
isenttopic. '.thus, the eq,uatl<ms whieh de1;1cribe the nonequilib1:'ium fl.ow
through a nozie:le of ;lowly va.~tng c:toss•sectional a3i&a 4\l'.\lthe eon ..
Sliltv~tion equ$tions (4 .. 1) and (4.,2) and the equation of eonsetva..t:ion of
vdv+ldp•O I) . (4.8)
together with the t:be,:inodynamic relatienthips o.f lfis .. (4,.3) Ci\nd (4.4)
Bald the r~te eq_uat;.1® (l<b (3.49)) which., fci- •t~ady 1 one•.d:tmensiou1
fl.ow, •1 'b<! writ.ten in the fem
do: ..... p . r J=[. v dxl • (; >t, (1 • o:t) urr + o:r u-r(r:t-1) + (t: .. 1 + aJt) ut-e .. {r .. ar)
• Kt' ar (i-•1 + a,:,> J , (4~9)
where xis the ~ia1 distanc.• n,aqured from the throat.
speeified, so
the area A' Eq. (4.1).
c:!1".l!:l:nn.tll ~ in Eq. (4. 9) may 'be CQ~reb.ted with
a no~zle with tlle hypE:?rbolie
(4 .• 10)
(4.l1)
b
at large values
(4.12)
(4.13)
·[ 2 ! . . . . . . ' .. •·· . ' 'fl-... ' ·' . . ... ... J.., . ·. . · · • i - {~)c, + 3 .• · .. ·· 2 2 .··
(. .a... "" ... >· 1. 1 + .! ... )· } J!d_ {· ... ~. 1 "· ···· .... · ·., · , ik~ml ,S, £1:tt il . · [ 1 +· . t' V ""t· '\ .a . 3 V•. ·. 4' T . .. . . .. . . . . .. . . ..... · . ··. . .. _ 2
('t + ~2 ('· + _a. \:.· '1.:· j ! ,4 if! ,.
(i.J V
i . I .. f 3Et • a > 1- .. # .. !'+ , i r )·.. . . . . L l .· .. ~ .... ; ~ . . i. ·. ·.tr, =. l!ffl .. ·. . . .; ·~. ) .. · i ' · · · , · · "' r ;;.· · , + ~ "' • a "" "' ,,..r,+.l • ·~~ ""'
(4.14)
p ...... ~~~--------------~~-- ......... ....._-------------
2.. : . . k ··[ 1 ... · . . . ·. . . . 4 . . ] L112 (l+g ) 1''~·2 (;). 2 f~) + c:t,.::rt+-1 + (l~t) T'*l.• 3 (r+o:r)Er J
(4.15)
(4.13) (4.14) are .,...~ .. _._u~..,U. for ar and 'r
by nnt.1tJ.er:tclU, 11cu;;eigr,at:1kon
Eq. (4.15)
readily possibl~
difficulties
constant M
not occur at the tbl!'oat, must be
a ltunge-Kutta pr<>cetu.11:e employing
are then
must be emphasized that although this
principle, in actual pract;ie~ ce.:rtain
the solution that the
ftom a. tedious iterative
ealculatton pro¢edure 16, *?his ..... N'ol• ................ ...
that flow may be tre.ated. as a.n
equilibt'ium flow unt;il a point downstream of th.e throat reached ..
However, the :rate equation (4.14), the
above procedure gives riie to a second difficulty11 Since Kr is the
equi.libriUlT! cous~t, then ·i=. 0 for equilibrium flow. '?his conditio-u
has been to lead problems when the integration is
the equilibrium flow eonditions1 5, 16; '?his difficulty
however,
be satisfied at
tllia
s.ection in connection with
a:rgon.
conditions
(4.16)
end each integration step. A
procedure given in the next
As an, illustra.~ion of. the proposed ~naly:$if, t~ flow o~ At'gon
th.Tough a ~oi~le Q~ sl.ow'lyvaeying c~ss•$erzt:toual _.ea for the three.
cases of; equU.tbi-:tum, frl;)a@,. 4nd m;,~qutU.b~i.Utn ts con,i4e1:ed.. Since
a a~h of tbfl pteacmt day 11te~atui~ ievealed that no eoiJ;tstort
c~oss s~e;ion. data was ~vatlab1e for :more tba.u singl~~stage ionization,
all numed.cal ,;~u.tationa •e. for tha c.alffi or r • l. ~ five
txam.p 1e.s considel:'ed ¢orr~pond t<> the fo1l<>Wf.ng tempera.~,;es and
pre,,~ure$ . at the ndntnun eros$._,·•eotd.onal 4lZ.8a of the nozale:
Case. t <>(K) p (a.tm~)
1 1!000 O.\ 2 13000 0.1 3 14000 o ... i 4 14000 1,0 5 14000 10.c
tt :ts tho~t lbat thue e!($1.iplt$ give ,:epyese~•ttve ~su1.t$ for ne vwt~Uons of thE) effects of Cou10tllb i~taetiona wtt:b temperatuie and
pl'e&sur.e tor the ea~ of r • 1.
s.1. l9iillt?•,:Lmn ,.tn1J IJ;pzt1 Jo,\uti9u. tb.e equations ot Section 4.1
(Jpetd.ali:t•d for t • )*) h.ave been fll•J.ved by ite1:,-ative methods,. using
.. ~a•~•. U!h• corresponding •ttdeat.•• JOiutions (er l',9 0) have. also been
found .. ' 9\e value cf the ioutli.ltion fra,c:.t1.on va,:ied f~ appt®tf.tnat$1y
O,.S to o, and ·tae .. tmwn. value <>fa w-.s i<>u® tq b~ apptOl(imately
O .. tl2.$.. fte mt:tld:iaum n.~i-ie~l di.f.ftt'ellCe !~ the t-eal aud ideal sq1utiop;s
w~ fQuttd to be a 12 .. pf!.'.f.e(!nt vm;tat.i.~ tn the temperatutE¥. 'J:hl$ led to
f:he oonc1u;ion t.hat, for singfy,•ioniaed ~e•, tbe Pl"th!lCe Qfflo\J.lom.b
intff&etiona ean have 4 n<.J~tc.•a1>1e ,it,et on the t;:Jter:mad:vn•e,
pro~i:tf.ee if equllil.bd,\.tm flow 1, acltteved«
s.2. ~~bill!! !olP,tion. $olution; of the dif.'fer$ntial e1u-.tiqns
(4.13) and (4 .. 14) (epeeiali.z~ foi t • t•) ~re been fo\lnd numerically
t>y a foutth•ord¢r R~~kutta method, which included •trapolatic>n to
ae,:o 1ntetv$1 size as~ eonEW:tton fS¢tor, using an l»M 7890 digital
computei fen: th~ rea1 and idea:i eas$&.
!fhe coU.iston Ct:0$$ Sftct!o.ns Uled for the, atom•atoa.l,. atom-ion, ant\
atom-el~tron co1U.,ion, a.re (s1u~ AppentU.x ll)
(S.1)
(5.2)
2 ~ m le I ~
Q. = 6 0 .. · 10.., 22 I e le • T jl le · • · x · · l 2k exc . . ' (5.3)
respectively. Thus,. the reaction velocities become (see Appendix I)
3 /2 T .·· " •i' ··. 12T .. s 'k!l r .... exe .. 2 . 1 exc u12 = S.5 :& 10 ·• . 112 ( - ) + 8 j e , (5.5)
(nm) L T
and
• (5.6)
reaction velocity u18 contributes
to the rate equation. Thus, the expression for the rate. equation,
assum.ing :: 1.0 om2 and b su¢.h that e • 1.so,. is
(5.7)
.. 44 ...
As ll1eU.t1o~ bti(tfly in the plreceeding sec.tion, t:h~ equU.ibri.um
s.olut1on$ are uted to st~t; tba iid;ag;aeion. the sttartins pttQCed11re
that is u$ed to join. tb~ two solutions is as f1;>ltow,,, Ufing
eq,uil:liu:1• vatu•• cort:$$vonding to .~· point Jqs~ dowstl'eatn oi the
th1t'oat, au ~tt~t :L$ 'Ul.ade to eta.it. •ne intesx-at.tcm.. At th~ and of i:be
fltst i1tt$g1:"at:t.on $tep 1 the eo.tlditi.onf (4 .• 16) a,:,e ~becked. lf either
c,f tn,.,, C()$liti0tis it vto1a.ted1 th• :tnteg;ation :bi atoppe<J •m a
poi:nt aligbtl.; futthe~ downstreem·it: tried. It bas tlteri fomld that
onee the conditions (lh16) ~e simultaneouJly s.aitt1tfied 1 t:;Jm integration
will. proeaed d()tffl the ll()Zzle with no t$ndency :fttr tnatability to
dev&lop ..
tt: :ls to be poitd;ed cut th.at thil atQ.rtlng point ie 1 to some
extent, d$pen~ntupon 1:he number of significant ziguies eari-ied in
the comput$t:ions. Wherefore., the st:a.i:tiug pt"oetdtn:~ described above
does not a;:tve uni4ue re.$t11ts i~ the vicinity of the ste,rting point ..
Howavai, itwl:is f<1und that if the integration wa.i:t at:atted at a point
slightly downttream of the. :bd.tial starting point, .th('!· two solutions
rapidly l!!on.versed (see figure t). For the cases considered., the
aveJ:ase range of t over which t.he soltJ.tion. could 'be· st.a.rted, and sive
results independent of the stat'ting poi11t, w,1.s found to be approximately
0~06.
thiing the method tf solution described jbove fot' the non-
eq,uilibriU111 fl.ow, th~ ~i~ numerical di.f f$renees between the teal
•d :tde•l solt.ttions wete found to be. less than 3 pereent for th.e cases
'1le tesults of the analysis and catcuiations 4re p~$1;1$n~d
gr-.phi..e31ly. figu~e 1 tbows the coll'V'$t.'8G~e of the intes~ation
solution uai:ng dUfetent st~ting points fl)r a typ1c:it1 ease.
figures 2•6 show plots of a vs. A. Jigures 7.-U. give thf vafiation
of T with A, figur.e.s 12 .. 10 show plots of v vs. A,. which, since
1,, • i , itepte,sent tb• vt.riatton of $peeifie impu1ae. Xn all plots
e~lus1:ve of Figute 11 t~sults !ncludt~ the •ffeets of iatera.ction
at$ plott;:ed - ,atoU.d tines., Ca,e, whet:~ only solid lines 4ppeat
indic4te that th$ i:esults wt.th and without Coul.otid) tntei;-aetione are
ee•entia.lly td,nttea1~
!the wtesu1ts indicat• thit f<;;'t tile c:on<l:lt.1Qns und~i eons.iderat:t.on,
the speeJ.ftc 1mpub$ :l$ •1me4t ~omplettly unaffected by the. presence
of Coulomb 1nt.el:"•ct1()n6. th• ealculat.ions cattt.ed out indicate that.
the -.~:!mum eor'ttct1on ts l$s$ tbau 1 p-.rceJ*;t. Alaot since the
•f:fect of negleettag Coulomb interacti.Olltt is .to unde.te$tin.late the
.apeeific impul~, ide4l gas c•l¢u1at:tons raay be consideted to give
conservative. tesults when used to pr4dict t'Oe~t engine. performance ...
Note, h~r, that itgur~ U. shows. that 11eglecttng tnte:r:actions
for the ~quiU.b'rium flow results. in unde'testimati~ the t$1UPeJ:"at.ure
by !lppro~:bnately 12 per.cent at 1*n area i:atio of one hundred. While
this hae little or no ed:fect ot1 t;he performance of rocket engiues, it
would be of importance :ln -.11•tns data obtained from a hypersonic
arc jet facility. Figure 11 also that interaction ef:Eects are
preseu,t in nozzle flow after the deg~ee of ionization has become
negligible. That is, the two solutions do not converge as a approaches
zero. Too, it can be seen from Figure 11 that for A> 16, the equili•
br:t1trn is less t.he nonequilibrium temperature. The
e::q,lanation of: thio lies in the :fact. that since a appro,;:i,:::hes zero
there a:ce 110 J:eac tions place the equilibrium flow and, as a
result, the temperatcrte g:a:.adient is ve1:y large. The effect of th:i.s
large :i.n temper,:ature on the veloc is to mako it cipproacb. its ,.
value of ,J i 0 fa.ster.
tl1at tl1e reac tidn ty usl:'ld in the anslysis is
correct;, the wonequil:tbrium results represent the actual conditions in
the nm:~zle., and consequently the equilibr:i.um and. solutions
merely deJ:itte bm:m.daries c:>£ problem. 1'iote, however, that: for all
down.stream 0£ throat. This conclusion comes
from the of ' . t:n-e pi:ocedure for starting the integration.
Finally, the analysis ind3.catcr; that the or<lel'.' magnitude
of the Coulomb corrections. For example; at A = 100 1 Figure 11 g:i.ves
the percent correction in T too .. 5
:;; O. 20 ::t 10 to be
a.ppro:dmate:l.y 12 percent., whereas Figure lO gives the percent correction
"" .? c.orrespond:tng to a = 0. 25 x 10 '"' to. less than 1 Also, as
noted a.bove, Coulomb interactions can influence the flow of an
ionb:.ing
concluded
parameter rs
deviations
lt muse
hold only
of r n.,,.,~l!);\"'A'l"
of more
.,.,. ........ __ a has
a is
not sufficient
an ideal gas.
emph~si~ed
ease
one,
However,
small. Thus, while can be
0 smallU, t:he
actual
above results eonelusions
:ta to that for values
Coulomb inlt'ieX'.8.Ct1<)ns v:rill become
demonstration w.ust . wait ........ , ..........
multi•st:~ge ionieation crios:3•!U!!c~t:1.on data is
7. -
Vsit.ll the hi,ye-Bueki• 4Jprn,cimat1® 1 the e·ifct~ta of t:oul.omb
iti.'t'erae.tl®s on .th$· tM1u:tU.brtum" froeen, $id ~tiectuU.ib'd.um flow of
~ 1-i•ed a•1 bavt b~ uwtsttgated. ·fhe gas :ia as~d eo k
®na•te1, el.ae~~!eally neutral, and- in tbetrltd equi.U.\»rjum (i.e., •
one t!~etaturt flu.id) a but th• eompo$iti® of th~ 1• i, •td.tr~wy,
thai :ts1, tllUlUple ionuat!o~ of •:r 4egtee 1,. 4l1ov4d.
·~fil thet"mO~~ ~iil!t.b1es •~ derived iJtai-tt~ ft:a the
app1:0prlilte. exp,:esston fo:r the hlmbo:J.:tt• fr~e. eAet"BY~ Using Boltzmenn
st•tttstJ.cs ~ uawm.na that t,.,. velocity di$1!:d,bution fu®t;t-one •~
given ·'by t'ne:lr -.111an vdueJ, the tat• of twi•tion ts t.ied,ved
:for ab:ml•atQll1 atom-c1on, en4 atom~\\l'1et:ro..ti colliatona.
'?he ~$1:.tlttng ~--stone .a,;e tben employed il\ soJ.vina t~ <,tua$i•
one, .... d~t~ flow !n • con.v•si~•divfJgtq noot.e fo~ ti. equtU.ltrtum ,
fl'o•e.n, and not1tqutU.brl'Ull\ <;... lumertcal tx•1es# using &rgOIJ, as:
ti. w~1:kf.ng subs~e, fte dis~.ussed and the reeulttt pt't•t11ted St'aJ>-_:l.ea11yl'
·':ftlf\l ~suJ.tf of tbe$e 4a1.cu14ti~n$ indicate thai, fqt tiing14\ :l.otdeation.,
tbe effect of Cow.Otm) :i.nt.tu:act:Ltms cm the peitf~f.lt of to~t •~ines
iJ1 negligibt..J but that datf.t ttbtatiied fl'Ol'l.l byper$0n1e ~ jet; wiadw
tu:IU.1els e• be ti;ntftcantly inf1uell'Ced br the pt<,uuim.~e <>f tee bltet'•
t1.Ctions ..
µ
n
h
A µ
N µ
V
N
m
particle deneity,
Planck's constant
Helmholtz
particle
energy
µ
particles A µ
a pa~ticle A µ
number of atomic nuclei
1; 2; 3; •• 1 = a.toms;
rnase . of atom
ionized atoms;
g,:ound state degenercy for e1eet·~onic partition function
of a particle A µ
of
degree of :loni~ation
dimensionless 1uantity defined by ltq" (2.17)
u
i
s
D, E
a
a, f3
-V µ
e µi -r t
fµi
~
rµ
a£ .. (~)
dt colt.
(a) J;.
µ1;. o>•
(a)
Ji µ (a)'
rr at(t+l)e
specific energy
specific entropy
constants defined 'by lq. (2.26)
speed of sound
coordinate system
internal e1nn:gy af a p~rticle Aµ
a fixed Cartesian
position vector in a fixed Cartesian coordinate system
time
fµ (vµ, Eµi' $, t) distributiQn function for particle$ '\
With internal ene:rgy eµ:t
collision integrals particles A µ
abbreviation a $Unl of collision integrals belonging
to the Boltm.nann equation particles A where the µ number pai:ticle$ at encounters changes due to t:<eactions
as be.fore, but where tb.e nwnber of
eneountere
transition probability
Ar + Ar_... Ar • + Ar+1' +
v 0 ~
''t.J. Iµ
E .. µl.
l\,. t
fJ
K
u rµ
M
ielat:lon totil forward and total t'e4rwa-i-d
transition probabilities, defined by lq. (3.22)
tJ 1(v, a • :, r, t) some property of the particle A µ .. µ. ···µ1 µ
masa avetage 0£
peculiar velocity of particle
ionization energy
energy of
a particle A µ
e. particle A µ
constant
partic1El Ar relative to the
coU.ision cross-section def:t.ned by lqs. (3.S5)•(3.57)
total electronic
length along centerline throat
a particle
4 particle A µ
nozzle measured from the
<!imensiot1les$ distance along noz~le centerline defined by Eq. (4.11)
specific impulse
is desire the his appreciation
to Drt! A. Ras&an, Mechanical Engineetbtg Department at the
Notth Carolina State College., for nun1erou1 suggestion$ tnd patient
ass:tst:ar1ce in the successfu1 of proje.e.t~
'to Dt. J1l J. lades., J,:., of Aerospac.e Sn.gineering Depart•
mant at Virginia J?olytechnie Institute, wish~, to express
appreciation hi.s and consultation$.
l. f. J~ Malina ~ C1.Wast•£llt&sa 1of .Ra,ag !!qtOtE Jlei~s II,~ !J.f1 $'l
~ of ttrfesti !l41ii, Soutnal of tbe huk1ia Xaat.,. V<tl.. llO,
Ito. 4, 1!140.
~. u. s. &eifut • I!!&@ ISR!melou, John W:Ucay Ind SoM> tnc.,
New to,:kji l9S9.
3. G, ,. Sut~Oll <jl,· ltett -~11.0l'l(JJ.eaast, John Wil.$31' ,md Sou,
In¢., tiew Yo:rk, 1956.
4. a. 1. o. lray • naut5,9,r1. ,,. pisg9t9yp. ,11911,~;- in ,a
Dz2iaU2D&s lu.lkh A.a ... c. 19, 1,983, Mwch ltJa.
S .. M, I:• U$bthill • ~I gf a tis109iaJiy .111.t Part l, •
'SJ"&hJ:&• Vmt J. fluid Mech., fol. !, l'art 11 ... January l9S7.
6. It. N. t. Bway amt J~ A. w1t11on • & :,rs~ §tu!&% o.f lon&'r
~'91£~ ti .AtSQn. \1l li!!i1,lmle1 MialQi, U.S.A.A. le,t.
Uo. 14~ fell.\ 1960,
1. :,. w. sou<t 'I! !lmbn . 13i1,, t siws1 11;og1a. AJ.atn, lhysical aevtew, Vol... ios,. 19S7..
s. s.. s.. 1$nner ... ~-am~1ton t~ ea !b.tv 2S .. SJ!tekf!l: le,stw@ &a 11ft S11t1.1.1, ACA1$o&l."4Ph *· 7, lutte~~th Sct.euc1.f$.a lubl:tcattons•
1'>ndon, l.9SS.
9. R •. Fol11ex-$Ud E. A. Guggenbeim .- Statistical 'l?hE\rmodynmpic$,
Cambridge at the Unive.rsity Pre,s, New York, 1956.
10.. a. Fowl.er • Statisti~al. Mechanies, Cambridge ,t the Utd.vei.-&:tty
Press, New York, 19.55.
11. L. D. Landau and I. Lifshitz • Statiatical siot, Addison•
Wesley Publishing Company, Inc., Reading, Mass., 1958.
12. e. S. Wang Chang
Polz~tomic . Gas~s, Eng. Res. Inst., Univ. Michigan, ItepOtt CM 681,
July 1951.
13. S. Chapman and t. G. flf)wling "" ~e. ~tbet®ltical 'l'beog of. >ton•
Unive,:sity iress, New York, 1960.
14. G. Ludwig and M. Heil • :BQundaQr.-Lax;e,: .. 'tbeog. with l)isso.eiation
a:nd loni~a.tton., Advane.e$ ii,; .AppU.ed MechlUlice, Vol. 61 Academic
Prass, )iew York, 1960~
15. G. Emanuel and w. G. Vincenti • Methoc.i for .Calculation of the One•
Dimensicrnal litoneguilibrium Flow pf .. a generail Oas Mixture Tb:t'ough
a,H:z.2ersonicNozz1e, AEOO•iDl•62•Ul, Atnold lngineet'ing Devel.op•
Center, June 1962.
16. J. G~ Hall
H 1'02;;1.e , Co:rne11 Aero. Lah • ., !ept .• No.
AD•lUS•A,.6, Cont. No. Gt 18(603)-..141, 1959.
17. H. Petscbek s. Bryon• AJ.!J!?;Oach.to Jiqu:tU.brium lonima.tio:n §~bind
Strong 6-hock wa11s in Arson, Physics; Vol. 1957.
H. ~ier•Leiu,;d.tz, z. Jpys1,k., Vol. 9S, p. 499,. 19.35.
19 .. A. von Engel• ]pni2;;ed Gas~s, Oxfot"d at the Clarendon Press,
Phenomena, Qgford at the Clarendon Press,: tondon, 19S2.
21. R. w. 'tt'Uitt and J. N. :Petkins • fhermodz;nand.cs .of t:ne Ideal
r .. t.imes :toniZE Monatamic .. Gas I Developmet1t$
Plenum Press, New Yo1:k, 1961.
Mechanics, Vol. 1,
22. J. B. l(nc,ff • ?he Bo~t!!ann B9uation and Non.eguilibrium Pheno•ena
lnstitute
NQrway.
Theoretical Astrophys:tca, Oslo University,. BU.ndern.,
1:be author was born
attended schools
'!he £ollotving fall
tmbse.quently g:rl:lduated
l.l.
award Bachelor 's uej~t'e(e
school at the
on. Api;il. 7, 1934. He
completing high school in 1952.
.i..4;.i;:;.,1,.,1,;4g. Polytechnic lns.titute, and was
1956, his Bachelor of
In July, following the
he eniolled 111 the engineeii,ng graduate
In September of 19S7 he
accepted cl position as on the Aeronautical Bngineeiing Staff
a.t the Vit'ginia Polytechnic Institute, ln 1958 the e.utbor received his
Master Science degree in Aeroniuti~al Engineering, In January, l9S9
he enrolled in the engineering graduate school at the Virginia Poly•
technie At the pres~nt he bolds the position of
Assistant Professor in Aeiroi~:oit.ce !ngineeting and is completiug the
requix-ement;s the degree Doetor Philosophy Aerospace Engi'""
neering at
APPENDIX A
are revtrU.ten in the form
(A.l•b)
The colU.sion integrals, (of .• lat) . 1. 1 .. , are obtained from the eolU.sion µ1. co • equation& (A.1) by considering each react.ion foll!' each value ofµ. lot
) rr ' O'
(A.2) ;(l:+l)e
Note that lq. _(A.2) mut be m.ultiplied by 2 since each eolU.sion
results in loss of two particles
proceeding to the left gives
(A.3)
Similarly, collisions (A.l .. b) and (A.1 .... c) give fo,: µ = r
(r(t+l)) J,. • r 1 ((r+l)(r+l)e)*
(i)
(A.4)
and
dv. dv~ 1 , av • di , , e ·:;;T e· · e (A.5)
(t(r+l)e)I .-, r·. J. ·.. « =. (i\
(r+l)i .(· rr), , ,,1 . (i)
.) a ·r(t'+l)e
(A.6)
V 1
(A. 7)
J . . ((r+l)b+l)e) • \·,
(r+l)i (r(..+1))' li'J
,,) (S (r(r+1). dv P (r+l)(l:+l)e r+l
(A.8)
and ((r+l)ee)
J(r+l)i b:e)'
=
(i)
f . t t'J
..
(A.9)
E!q,, (A.2), Bq. (A.8) must be ,multiplied by 2 to
account for the loss of two
collision. lri:nally, Eq$. (A., l) give µ•e
(r(1*1)e) J •
e (r-,:)' -rr
• ~P*' er. • dv\. dv~1 dv, cf , , ... r(7N-1)e "' ,l;.T . r r
(A.l.0)
((r+l)(t+1)e) J • e (r(t"+l))t i j
(A.U.)
(re) J = e((t+l)ee)'
(A.12)
((r+l)ee) J =
e (1:e)'
(A.13)
wher~,
that the summation ove:t all indices, Eq. (A.12)
is equal to negative of iq. (A.13). 'I!herefore, it is necessary to
y"""'""'""¥l>~;;.. only lq,. (A.10') through (A.12) for the case of µ. = e.
A
J of .. inelastic < r:1) uv \ ot coll., k r
(A.14)
ri [ A (rt) .... (r(r+l)e) A (r(t+l))
lr = ~ j 2 1r1 ·· + 11:1 ·(· ) , + '~1((.-..t..1··) (·..;J;.1) )' +
(r(r+l)e), · • J:'r . . «-T '",.. e
(A.15)
sun1ned over all values of i
(rt) 3 . (r(r+l)e) rt '
(A, 16) "" J ri (r(r+l)e)' (rr)'
therefore
J .. (rr) + J (r(r+l)) + J¥.1. (re) J av ...... ri · · ri ~ ~
(t(r+l)e)• ((t'tl)(~l)e)' (h+l)ee)'
gives
dV = r
2
r "' (rr) nr . m ·. 3 /2 L Jt:i = ·z; ( 2,rl,i'f )
(r(r+l)e)'
(A.17)
(A.19)
Bq. (A.18) yields
(A.20)
(A .. 21)
in Eq. (A.20) may be t-alated to ea.eh other through the conservation of
[ r- lil • ...Lj !! (• . 2 ·. ·. •. 2)· . ~ ... 2
. 2kt .' 2 v. ' + '~1• ·· + ,, V • + L · J!' ~r 6 e
J (A.22)
JA (rr) , Jr1
(r(,r+l)e) • ... n J r (A.23)
where
~ -L -<·v• ·. 2 ..1... v· 2). ~.· "" 2· f ,.;m ... ·.. "" -:r T ~. t' . . r
rr _.... --., r1 dV l
r(r+l)e 5 f (A.24)
reaction, velocity
u are obtained re
APPENDIX B
:B. l. E.s,uilibrium Flow Equation::}. The equilibrium flow e<.Juations for
the special case of r=l are obtained fron1 section 2. These are:
Equation o~ State k (J
p l\'lO ; pT ( l + a) (l .. 3 ) , (B.1)
Spe.cific Enthalpy
i !t(l a) i 5 a 'X2 4 l = + - + - .. -cr J m I 2 1 + a T 3 ' ""
(B.2)
Specific Entropy
l·J·· rs P ai.3r 'i £1 ;::;; -m'" L (1 + a) 1,i -2. .. log ( - ) ... - J + -.. i log (DT) + o; log (ET)J! .. m 3 2 1
L
Law of Mass Action
2 2g2 T.3/2 r· T ,1 w.. l a ;O ) ...£ + (B. l}) = E ( exp ... .. IJ I 1 .. a gl,o (p/ro) L T a J '
and
(B.5)
wttb
1 i (.. 6 + cr ).· .'2 .· ( 3 + 4a ·)· ~l -;t·· 3 r· 2et· (JI· (ll.6)
the equations of conservation
03.1)
(B.8)
fcn:m the system Qf nonlinea,: elgebr.aic equations used to solve the
r=-l are
Ir- 2T ·_ .. · .. _ .... M2 - - (1 + a) cr + _ ·•··· . ·· :~
1 L 3 P .- . _ . .· (k/m) p3 (1 + t ) 2 t . . .
! (1 + a:) (1 + !16... ) ~ .
J . . -' [ f (1 + a)(3 + cr) J "
fl + a) ( l ... + 1 ... --a) } ~ + • .· · · 2 · 3 . d~
~ T
(B.9)
(B.10)
where
M
(J =:= .,_,.,.._,...,.......,._""""""'!.-. .......-. -·~···--· -· """". --· ..... """'· .--.!"""' .. --"'""*"'· .-. --· ·•· """"·-· ~ ................ """·~·--·. -1 /2 I
2 10
.. 2( ! ) [ f T(l-.()$) + (l .. a:) Tton .,. ! (lffl)cr ]}
(B.11)
B.3. leact:i.on Velocitif!1S foll'. Ar&t?J!• Since electton•atom collisions
ao1:,eaLr to be the dominant mechanism of ioniaation. 1 the reaetio.n
will discussed first.
tbe at:Qms which
ev·entually ionize, Petschek
mation fot'
is electron energy
~1a = 1.0 Jt 10 · (w • 11.S) , e
ev and the constant 11.S
(B.11)
the energy,
ev, the first excited argon. Equation (B.11) represents
a straight line fit to data obtained. by Maier•t.eibnit~ 18•
E<1uat:ton (B.11) mtpressad in ·0&. (Te,m = 1.34 ~ 105 °K)
(B.12)
-where c1e is the initial velocity of the atom relative the electton. ..... -lo.
terms of c18 and G, the mass•eente.r
. 13 SJ.nee
a. <.,r .... ,.~1> ........ ......._e~ ....... ·.· .. = l • o<v;,, ve)
, .. ' .. ·· 3 1/2 t ~ 106 I 2<kT) l ( · ~e + 2) e .. L ,t J .. '
(B.13)
(B.14)
(B.15)
11 in,'fo¥ the a$sumptton that eeeentially al.l excited atoms eventually
to twice the energy
an a:tom etrikes 191J nterefore, assuming
and using cross data given in
r,~ferences l!:1 and 20 fo-r Q11 and Q12., respectively, the following
approximations are obtained fot' atom.iiiatom and atom•ion cross
(B.16)
(B.17)
Ud~g !qi. (B.16) and (lh 17) t;.he expre11ions fQr u11 integrated to give !qst (S.4) (5.5).
-71-
0.4
Case 2
(~ i = • 22901, a:i = • 31911)
a:
T* • 14000 OK
p* • 1.0 atm~ er ,;. 0
Case 1 <~1 • .16372, 0:1 = .32455)
Equilibrium
o":'------------------~------------------,r 1 10
A
Figure 1. Illustration of Convergence of Starting Procedure
-72-
0. 8 ~------------------~------------------------------------,----------------------------------------------------------,
0.7-----
* 12000 °K T = 0.6 p* = 0.1 atm
- a :; 0
a = 0
0.5
a
0.4
---Frozen
Nonequilibrium -
o.__ ________________ ___."-------------------1 10
A
Figure 2. Ionization Fraction vs. Area Ratio
100
-73-
0--~------
T* = 13000 01(
p* = 0.1 atm
- cr,'O
cr • O
Frozen
Nonequilibrium
Equilibrium
o'-----------------.....iL.,,-----------------"'!!"!!!! 1 1 100
A
Figure 3. Ionization Fract.ioll vs. Area-Ratio
-74-
a
Frozen
Equilibrium
T* • 14000 <>K
p* • 0.1 atm
cr ., 0
cr • 0
o"'r---------------~~--------------~ 1 10 A
Figure 4. Ionization traction vs. Area Ratio
-75-
0:
Frozen
0.3
T* • 14000 OK
p* • 1.0 atm
a =I, O
(1 = 0
Nonequilibrium
Equilibrium
o'-!!-----------------__.~-----------------1 10 100
A
Figure 5. Ionization Fraction vs. Area Ratio
-76-0.8
0.7
T* = 14,000 OK
p* ... 10.0 atm 0.6
-a ,, 0
--a = 0
0.5
a
0.4
0.3
0.2
-- Frozen ~------ - '-- - -- -- -- -- -- -- ----0.1 ~
~'..;;::'! _<Equilibrium ~
~--= Nonequilibrium --.:::: --==-.;; 0
1 ll 100
A
Figure 6. Ionization Fraction vs. Area Ratio
-77-16--------------------------...-------------------------------,
T* = 12000 OK
12 p* = 0.1 atm
-{: ., 0
= 0
10
Equilibrium
it 8 (")
I 0 ,-1
>4 E-t
6
Nonequilibrium
Frozen
01----------------~~--------------~ 1 10 100
A
Figure 7. Temperature vs. Area Ratio
M I 0 ,-4
>4
E-4
Equilibrium
Nonequilibrium
T* = 13000 °K
p* • 0.1 atm
-{a=,O a = O
61-------+----....,..,..,---------+--------------------I
Frozen
4r----~~---~----------===----..;;;;;;;;::::::::::=:J
0,...---------------~----------------~ 100
A
Figure 8. Temperature vs. Area Ratio
M I
Equilibrium T* • 14000 °K
p* • 0.1 atm
_. { (J. 0
(J - 0
sa~--+~~-----------~r----------------. ,cl
rt Nonequilibrium
Frozen
o'----------------f::---------------:;;~ 10 100
A
Figure 9. Temperature vs. Area Ratio
~ 0
M
Equilibrium
Nonequilibrium
-80-
T* = 14000 °K
* p • 1.0 atm
er .;. O
er = 0
'o 8 ~---\..--------:!io.----------+------------------....:::,,::lll
,-l
Frozen
0 ~1----------------.....,.1 ..... 0 _________________ 10-0
A
Figure 10. Temperature vs. Area Ratio
-81-
T* = 14000 °K
p* = 10.0 atm
(J ., 0
er = O
Note: Frozen and Nonequilibrium
12 curves show no effects of er
CV")
~8~--~-------~~--~~------+-------------------1 .....
Equilibrium
Frozen Nonequilibrium
o.__ ________________ ...,,.j _________________ _
1 10 A
Figure 11. Temperature vs. Area Ratio
100
-82-8-----------------------------------
7t-------------------t------------------l
6t-------------------t-----------------Equilibrim
u51---------------------+------::i...-~ Nonequilibrita IJ • ...... e
T* • 12000 OK
p* = 0.1 atm
{ (J .. 0
a• 0
Frozen
2-----------------------------------1
lt---~--------------+-----------------....,
o"T----------------..,..---------------..... A
Figure 12. Velocity vs. Area Ratio
an •
-83-a---------------....----------------1
71-----------------+-----------------t
94~---~~-----------~------------------1 H
>
T'* • 13000 °K
p* • 0.1 abl
-{a•O a• 0
2.------------------+------------------t
lt-----"'lc---------------+-----------------1
o.._ _______________ .._ ______________ __.
1 10 A
ll'ipre 13. Velocity vs. Area Ratio
100
(.) G) CD -fl
Ll"I I 0 ,-1
>< >
-84-8-----------------,------------------,
Frozen
5
4
T* • 14000 OK 3 p* = 0.1 abn
{ (1 ~ 0 -(1 a 0
2
ll------3-.,._ ____________ __,1---------------------a
o'-------------------1.---------------- .. 1 10 A
Figure 14. Velocity vs. Area Ratio
100
-85-8-----------------,-----------------,
71--------------'---+---------------.
61-------------------;-- Equilibrium
Nonequilibrium ~5~------------~~~~~j==~~~~~~~--------, (I.I -5
It\ I 0 ~
Frozen
~41-----~L------------+-----------------, >
T*"" 14000 °K 3 p* = 1.0 atm
CJ :I, 0
er = 0
2
o.__---------------:-,!-----------------:~ 10 100 A
Figure 15. Velocity vs. Area Ratio
(.) <1l Cll -s (.)
in
-86-s --------------------..---------------------
7 I-------·------------------------- ----------------
6 !---------------- --- - ----- -----,f------
Equilibrium
Nonequilibrium
Frozen
6 4 1----------------i"~------------+------- -------------1 ~
T* = 14000 OK
p~' = 10.0 atm
er -:# 0
a = 0
l ,____ __ ,.. __________________ ------ -------+-----------------
o',;-------------------=-':::------------------,,-,,-,! 10 100
A
Figure 16. Velocity vs. Area Ratio
Usi11g the Debye•liuckle approximation, the effects of Coulomb
interactions Oll the equi1Un:ium.., frozen, and nonequilibrium flow of
an ioni~ed gas have been investigated. The gas i$ assumed to be
monatomic, electrically neutra.:t.,·and in thermal equilibrium (i.e., a
one temperature fluid); 'but tbe composition of the gal$ is a'tbitrary,
that :ts, multiple ionization of any degree 1s allowed.
The thermodynamic variables are derived starting from the appropri•
ate expression for the Helmholtz free energy. · U$i.ng Boltzmann
statistics and asstun.ing that the velocity distribution functions are
given by their Maxwellian va.lues, the rate of ionization is derived
for atom•atom, atom. ... ton, and atom .. electron collisions.
The resulting tmpressions are then employed in solving the
qua.$1 .. one .. dimen,eional flow in a eo'1werging ... diverging noz21le for the
equilibrium, frozen, and nonequil:i.brium eases. Numerical examples,
using argon as the working substance, are discussed and the results
presented graphically. 'the results of these calculations indicate
that, for single ionization, the effect of Coulomb inti$1taetions on the
performance of rocket engines is negligible; but that data obtained
from hypersonic arc jet wind-tunnels can be significantly influenced
by the presence of the interections ..