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omputing an
pp e Ma ematics enter
AEC ! ESEA! CH AN! ! EVELOPMENT ! EPO ! T
T I ! -LLSOO N i co
1333 Ed e PHY S ICS
NOTE S ON MA! NETO -HY ! ! O ! Y NAMICS
VI I
F L UI ! ! Y NAMICAL ANAL O ! IES
by
A 0 A 0 Bl a n k and Haro ld ! rad
Ju ly 1 5 ,1958
Inst itute ofMathemat icalSc ien ces
N E ! Y O ! ! UN I V E ! S I T Y
N E ! Y O ! ! , N E ! Y O ! !
The general s e t o f e qu at ions wh i c h i s under cons iderat ion
i s
p div u 0
p22 gr ad p
l- c ur1 B x Bd B
p p d iv u O,or
! B( 1 0h ) curl ( u X B ) O
, l B 0
to ge ther w i th the aux i l i ary r e l a t ions
E - u . x B
J curl B
q x div E .
! e us e the no tat i on d/dt to deno te the L agrang i an der ivat ive
d
5875+ u -V .
The sound spe e d ,a1
i s de f ine d by
32
p f ( p 9 6A
where p i s a g iven func t ion o f p and o f V1 ( the entropy p er
ma s s ) . For an incompre s s ibl e fluid,we repl a c e by
dd%' O
,d iv u 0
2Se e MH-VI
, Flui d Magne t i c Equat i on s ! ener al Prop er t i e s .
p c o n s t ant throughout r ather than cons t ant on e ach p ar t i cl e
path . S imil ar ly) i i
‘
a cons t ant through out t h e fluid we
c all t h e flow i s entrop i c ,wher e a s und er the cond i t ion the
flow i s c all e d ad i abat i c .
In the s e e q uat ion s we have a s sumed inf ini t e c onduc t ivi ty
have o m i t t e d_d i s p l a c em e n t current e l e c tro s t at i c for c e s .
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A s used in the above,“person acti ng on beha lf of the Commiss ion " i n c l u des
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UNC L AS S IF IE!
AEC C omput ing and App l i e d Mathema t i c s C ent erIns t i t ut e o f Mathemat i c al S c i enc e s
by
A . A . Bl ank and Haro ld ! rad
1 5 , 19 58
C ontr ac t N0 0
The r e sul t s g iven in thi s r eport ar e,in large p art ,
i dent i c al t o tho s e pr e s ent ed in number I V o f the o r ig inal
s e r i e s o f mime ographe d l e c tur e no t e s on magne to -hydro dynami c s
i s sued in l9 5h . The c l a s s o f p ar alle l flow s cons i der e d in
S e c t ion 2 o f th i s r epor t ha s b e en ext ende d d S e c t ion 5
h a s be en add ed .
Pre fac e
1 . Introduc t ion‘
2 . P ar alle l Flows
3 . Two - ! imen s ional
C ons erv at ion o fL aw
One - ! imens i onal
Tr ansver s e Flow s
C ir cul at i on and Bernoull i ' s
Tr ans ver s e Flows
NY O -ou8 6
A . A . Bl ank and Harol d ! rad
1 . Intro duc t i on
Al though the comb ine d fluid and el e c tromagne t i c e quat ions
gener ally r epr e s ent a f ar more compl ex sy s t em than that o f
c la s s i c al fluid dynami c s,there ar e a number o f import ant
ins t anc e s for wh i ch the two sy s tems are mathemat i c ally ident i c al
upon appropr iat e ident if i c at ion o f symbol s . The exi s t enc e of
the s e exac t mathemat i c al analogi e s p erm i t s the immedi a t e appl i c a
t ion o f a we al th o f known re sul t s in fluid dynami c s to the
r e l at ive ly new and unexplor ed f ie ld o f fluid magne t i c s ° One
o f the s e analog i e s i s suff i c i ently ra n i f i e d to be tr e a t e d
s ep ar a t e ly .
1The re sul t s given in thi s repor t are mi s l e adingly
br i e f ; they allow the app l i c at ion o f many known t e chni q ue s and
r e sul t s to appropr iat e probl ems in fluid magne t i c s .
The fluid dynami c al a sp e c t o f one o f the s e analog ie s,i . e . two °
d imens ional non- s t e ady flow , inc lude s the ma ! or por t ion o f the
ent ire l i t er atur e o f fluid dynami c s . On the o ther hand,the
mathemat i c al ly ident i c al fluid magne t ic a sp e c t i s much more o f a
sp e c ial c a s e . Thi s r emark i llus tr at e s the far gr e at er compl exi ty
o f the to t al i ty o f flui d magne t i c theory a s comp ar e d to convent i onal
fluid dynami c al the o ry .
The general s e t o f e qu at ions whi ch i s under cons i derat ion
i s
d tp div u o
p Q% gr ad p fiv c u rl B x B
de dapdt
' + p div u O , ord?
0
6 E( l . h ) '
dtcurl ( u . x B ) O
,d iv B 0
to ge ther w i th the aux i l i ary r e l a t ions
( 1 0 5 ) E : -U. X B
J = .l curl Bp
q x div E .
! e us e the no tat i on d/dt to deno t e the L agrang i an der ivat ive
du -V .
The sound sp e ed,
al
i s de f ine d by
'g% r p
where p i s a g iv en func t ion o f p and o f Vi ( the entropy per u ni t
ma s s ) . For an incompre s s ibl e fluid,we repl a c e by
o,
d iv u 0
2Se e MH-VI
,Fluid Magne t i c Equat ion s ! ener al Proper t i e s .
p c on s t ant throughout r a t her than cons t ant on e ach p ar t i c l e
A
path . S imil a rly,i f V
! c ons t ant through out t h e flui d we
flow 1 8 c all e d ad i abat i c .
In the s e e q uat i on s we have a s sumed inf ini t e c o nduc t ivi ty
and have omi t t e d di sp l ac ement current e l e c tro s t at i c for c e s .
2 . P arall e l Flows
The momentum e quat ion c an be wr i t t en
Q J )
The form of thi s e quat i on sugge s t s that we lo ok for s t e ady flows
in whi ch B i s p ar all e l t o u,
B Au ;
in addi t i on , we cons i der only an incompr e s s ib l e flow , div u 0,
from whi ch it fo llow s that l i s con s t ant on e a ch s tre aml ine
( magne t i c l ine )
gg ( U n i 7 ll 0 .
S inc e e quat ion ( 1 . h ) i s s at i sf i e d ident i c ally,all that remains
i s to s at i s fy e quat i on whi ch t ake s the form
( 2 . h ) p ( u -l7 ) n gr ad p 0
wher e p i s a cons t ant on e ach s tr e aml ine,
p p iz/u
and p i s g iven by
p"
p
we re c all tha t ( a . h ) t o ge ther wi t h div u o,dp
*
/d t o
de f ine s an incompre s s ibl e s t e ady flow wi th d en s i ty p*
and
pre s sur e p%
.
3 To e very s uch flow,there ex i s t s a s t e ady
,
inc ompre s s ibl e,p ar all e l magne tohydro dynami c flow ; bo th p and
A c an b e arb i tr ar ily sp e c i f i e d on e a ch stre aml ine in t he magne t i c
analo gue . Bernoull i ' s l aw ho ld s,
v i z . the quant ity
i s con s t ant on e ach s tre aml ine .
The s t ab i l i ty o f the de gener at e c a s e p%
O, p
*c ons t ant
,
under the homogene i ty condi t i on p con s t ant ha s b e en tre at e d
by Chandr a s ekhar ( Pro c . Na t . Ac ad . S c i . , pg ,
I t should b e remar ked that no e quat ion o f s t at e i s re quir ed
0
b e twe en pw
and p*
.
Two - ! imens ional Tr an sver s e Flows
! e cons ider flow s i n whi ch all quant i t ie s are indep endent
of 2 but may dep end on x , y , and t . The magne t i c f i e ld i s
B, z
re s tr i c t e d to the z-dir e c t ion,
and the v elo c i ty i s two - d i m e n
s i o n a l in the p l ane I t
i s convenient to u se two —d i m e n
s i o n a l ve c tor no t at ion,int erpre t ing
the s ingl e component of B a s a
s c al ar . Equat i on ( l . n ) then t ake s
the form
dB0 1
F t 1( 3
3 !B d i v u 0.
In o ther words , c ons ervat ion of f l
t ake s the s ame form as c on s ervat ion o f mas s in thi s geome try .
The r e a son i s intui t ive ly c l e ar; in a plane flow,the e lement of
are a, dx dy ,
acro s s whi ch the flux i s conserve d i s the s ame as the
two -d imens ional "volu m e " e lement on whi ch ma s s i s c on s erved .
Equat i on c omb ined wi th yi e ld s thi s re sul t in the
form
dEE( B/p ) O ,
the r at io of B to p i s c on s t ant fo l lowing an e l eme nt o f fluid .
The e qu at i ons and may b e rewr i t t en in t erms of the
"to t al pre s sur e
p*
p
\0
B w ld q de p d ( -
p( 3 0 8 ) Td tz
+
3
The analogy c an be made exac t by impo s ing addi t i onal
re s tr i c t ions
a u p p o s e con s an oug ou c an e e m i na ed romS t t t hr h t B b l i t f
the e quat ion of s t at e t o ob t ain
N e w) (32
Thi s e quat ion o f s t at e s at i s fie s t he usual thermodynami c
convex i ty r e quir ement s ; in p ar t i cul ar we have
5 r
"7
de pTdn
and
( ii i
)2
l
lm
"!
I
!l
l
S! “
4
"0
FS
' Nno
an N
1: !
( b ) Suppo s e Q cons t ant throughout . ! e int erpre t Q*
a s the
thermodynami c entropy and obt a in the e quat ion o f s t at e
vii
) mm 51
;
From the re l at ion
2n 1
d e p (NE)
(1.(i i?
we s e e that , by t aking
T B/p ,
we obt a in a convent ional thermodyn ami c s truc ture . The
sound spe e d ,a*
,i s given by the s ame formula , a s
previously .
11
( 0 ) Suppo s e that q? f (n ) . Mor e pre c i s e ly,suppo s e t hat the
cu rve s Ygx ,y ) c ons t ant c o inc ide wi th the curve s
a the ini t i al ins t ant ; we de s cr ib e thi s by s aying that v5"i s a
( po s s ibly mul t i - valued ) func t ion o f Q ini t i al ly . S inc e the value s
o f nand V?ar e c arr i e d w i th the fluid el ement
,the r e l at ion
e7) f (Q) p er s i s t s for all t ime . Ei ther
2or lz
k
c an b e cho s en
a s the entropy ; l e t us t ake The pre s sur e e quat ion o f s t at e i s
l
7 ) p ( p , q )“
! ?
the sound sp e e d i s a s b e for e,and the thermodynami c ident i ty
3 7. 1( 3 Q
e p d (p)
fo llows wh en we t ake
x lt
T Tup
( d ) In a one - d imens i onal flow ( var iable s x and t ) , the re la t ion
!?
f (7)i s s at i sf i e d for arb i trary ini t i al dat a , and the form u a
l at i on ( 0 ) fo llow s .
All c onvent ional two - d imens ional ga s dynami c al the ory appl ie s
t o the abo ve magne t i c analogue s , pro v i de d that no sp e c ifi c a s s u mpo
t ions have b e en made r egard ing the e qu at ion o f s t at e . One of the
int er e s t ing fe atur e s o f the s e hydromagne t i c flows would s e em to
b e the po s s ib i l i ty of cre at ing arb i tr ary e qua t ions o f s t at e at
will by the proper cho i c e o f in i t i al confi gur at ion . Ano ther way
o f lo oking at thi s i s tha t one c an constru c t a fluid w i th a s ound
sp e e d whi ch i s an arb i trary func t ion of po s it ion much more e a s i ly
than in a convent ional gas .
- 12
S inc e the pr e v ious ly de s cr ibed analog i e s ar e exac t,the
convent ional r e sul t s on int e gr al s o f the mo t ion fo llow under the
s ame condi t ions a s quo te d for the c onvent ional fluid s . However,
it i s i l luminat ing to der iv e the s e re s ult s d ire c t ly .
The c ir cul at ion a s s igned t o a clo s e d curve rfl
i s de fined by
( LL . 1 ) C u o dx
where 0‘ i s a p ar ame tr i z at i on of r“ . For a curve
, ra ( t ) , whi ch
i s mov ing wi th t he flui d ( 0‘ i s f ixe d to a fluid element ) we have
Thi s w i ll no t b e z ero and yet admi t any s igni f i c ant
exc e p t in the two ~ d i men s i onal tr an s ver s e flow s ! us t
In that c a s e ( B o V )B O and
dc 3p
0
! t )
C ir culat i on will b e c ons erve d con s t ant ( homogeneous
incompre s s ible flow ) or if pi,c
func t ion o f p alone . The
lat t er wi ll be the c a s e when b o th l and n?are c on s t ant through
out the flow ( of . e quat ions and The
general c ond i t ion for c ons ervat ion o f c ir cul at ion ( o f . e qua t ion
i s that a po t ent ial, ( 2 ex i s t s at i s fying
(m i ) Tl53 dvf
‘
d ( e*
pei
/p ) -1-dp
*d ( 2
u !
I f the flow i s irro t at ional,
(M 5 ) u Vfl
and if the po t ent i al 2 exi s t s i f 7 and a?are cons t ant ) ,
then,u s ing ( u o V ) u curl u X u V (%—u
2), we f ind that
( L h é )
or ( Bernoull i ' s l aw )
I
t
co c
t
( it -7 ) gr+ 512
h*
-_ fl _
wher e the " to t al enthalpy" h*
i s
M
( u . 8 ) h*
ew
p%
/P ~
For a s t e ady irro t at i onal flow wi th a po t ent i al 2, we have
wéuz) %vp
*0.
from which,t ak ing the do t pro duc t w ith u and us ing 5% u
° ‘7 ,
we obt a in
gi
gdg u
zh""
Q ) o .
In th i s c as e, % u
?h*
2 i s c on s t ant on e ach s tre aml ine .
One -! imens ional Tran sver s e Flows
Thi s geome try i s,in a s ens e , the dual of the one tre at e d
Se c t i on 3 . a s sume that all quant i t i e s ar e ind ependent o f
x and y ( the r e l evant var iabl e s are z
and t ) , that B ha s two component s,Bx
and By!and u ha s only a z - component .
! e again have ( B o V )B O,and c an wr it e
the momentum e quat ion in the fo rm
Bu au 1 n 0
Fig . The e quat ion for B , int erpre t ing u a s
a s c al ar , i s
-a—B a
0.
a t
For the magni tude o f B we ob t a in
a 6
Thi s to ge ther wi th and the c ons ervat i on o f ma s s i s a
de t ermined sy s t em ( only the magni tude of B ent er s in More =
over,i t i s exac tly the s ame sys t em that wa s tre ated in Se c t ion 3 ,
spe c i al i z e d to one sp ac e d imens ion , 2 ,ins t e ad of two
,To
comp le t e the so lut ion o f the or iginal probl em,we no t e tha t
impl i e s that the dire c t ion o f the ve c tor B i s a cons t ant follow
ing a fluid e lement .