1917, @1967 d - dtic · it may br released to the clearinghouse, department of commerce, for sale...
TRANSCRIPT
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TDFTD-HT-23-671-67
* FOREIGN TECHNOLOGY DIVISION
PROPAGATION OF WAVES IN PLASMA ACROSS THE
MAGNETIC FIELD
by
A. B. Kitsenko andX. N. Stepanov
/UDC
r p flrrv;ript
9 @1967 D1917,2 ' GO LDE[N A NNIV R ARIY
FOREIGN TECHNOLOGY DIVISION
Distribution of this document is unlimited'.It may br released to the Clearinghouse,Department of Commerce, for sale to thegeneral public.
Reproduced by tho,,oCLEARINGHOUSEi.IM E for Federal Scientific & Technical -"--- -
Information Springfield Va. 22151
77 -_ _. . . . . ' . . . . . - - - _2 2 . _ ' _ _ -- 2 -2
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UNEDITED ROUGH DRAFT TRANSLATION
PROPAGATION OF WAVES IN PLASMA ACROSS THE MAGNETICFIELD
By: A. B. Kitsenko and K. N. Stepanov
English pages: 22
SOURCE: Yademyy Sintez (Nuclear Synthesis), No. 4, 1964,pp. 272-278.
Translated by: L. Marokus/TDBXT"
TT700i819
135 TRAWSAT3N X A R6ISON O W OW,N&,,,3 ""T --W A-. A.ALY. ." ....KorOAL WSMIiT STATAMWI 66 •hU3 PIPAIII SYo.
wvA6Qw AUflffM 1W66P NS CI IAIOWT ImmILaI p"Sq TH P NY TIAW1 DWII
1Tfofl - 23-671-67 W 2 7 Oct. 19 67
,? *n.,tllmmm
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-ITIS -INDEX C1TR FM~i01 c 8Tra~slatwion N__ XR~c~ 76CCrW
97, Header C1&s 63 Cti 164 Cotitrol Maxicings 94 O"pas 40 Ctzy Infur~CL~ UNCL, 0U
02: rM; 'OSRef 04Yz' 05 Vol O16 Isx ]07 BE .- 1.45L P. [0 tTR0000- 64 000 004 0272 0278 NONE
RASIROSTRIINYE VOLN, V PLAZME POPEREK MAGNITNOGO POLYA09 Bi~lish Titli.PROPAGATION~ OF' WAVES IN -PT.ASMA- ACROSS THE -MAGNETIC FIELD
-43- Source-YA2DERIIYY SINTEZ (USPJ ___________________i
,0,:Atlwr 98 D ocunent Lic&tion
aITSENKOJ A. -R'.16-C~to --47- Subet-Codet
STEPA19V K-. "N. 20_____________
16Cb- uthor - .39, TOic Tagsi waI proation, magneticNOWE f ield, xied iistic pl1a si oscilato, !
l6':TCo-Authokr cycatonfrquc, -dispersion equation,plas.a atn
-NONE _ _ _ _ _ _ _ _ _ _ _ _
'AS7A:T-,*prh -pagaton of Waves in a plasma across a magnetic field is 4beJ:ng chatracteriied -by intere',ting featdires -hear gyro-frequencies of electronsand ions,, as well as frequencies5 multiple to them. Frequencies of ordinaryand extraordinar'y waves which propagate across a magnetic field in a non- jrelatiistc plasma are determined, and tha excitation of high frequencybiian~hes of thesep os'C'illations are investigated when an ion cyclotron wavepasses, through the IlasmaL. Various dispersion equations for extraordinary'waves are~giyen. Thei behavioral frequency of various branches of extra-ord'inricy wave, i" -hot -plasma 'are described-.(E,-.gih, tii~lation:- 22' pages.
FTD ES 07 0-90 f
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PRO ATION OF WAVES IN PLASM ACROSS, THE MAGNEIC FIED
A. B. Kitsenko and K. N. Stepanov
I
-I
IThe effect of the thermal movement of plasma electronsiiand ions on wavre propagation of a low pressure nonrelativis tic
plas a t_ 47rf n0 TajHi2 ;S i) acrose a magnetic field is iti-
vestigated. The dispersioni equation for ahX -ordinlary wave hassolutions-co%(k)-. iimilar to k sw a ;2,u. at any given
wavelength ratio (A . i/k) to the Larmorlan radius Ioa ype particles having a thermal velocity (see Fig. i).
(c% and mi gyro-frequency of electrons and ions,)eiThe dZ'spersion e4uation for an extra&ordinary wave also
has Val aalogoua so) ution in the field of high frequenciis(CO ftce), (see Fig. 5), as well as a solution,, correspornding
at k I 2 .> , o the longitudinal. plasma oscillations.
FreauencJ.es of longitudinal oscillations, in the case of a
Langmuirs frequency of electrons) as a function of the wavevector, decreaae at a rise in kt e1 decreasing from a value
a) a e( s - 2, 3,,.. at k to w ft (s i)We at*
(%Sl e be the behavior of plasma frequencies is shown inFig, 2 and 3.
In the field of, low frequencies (w < mi) the dispersion
equation for en extraordinary wave (in case of a cold lasma)dote rmines the frequency w - kV~j which cor.kespond to hmagneto-sonic wave (Vi - is the Alfven velocity). This
expression appears to be unacceptable at kQ i o s(s n-opos.when co~ a mi~. 121 this field it is necessary to compute the
FTD-HT-23-67h-67! ____ _ _ __ _
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71
thermal movement of the ions. The behavior frequency ofvarious branches of the extraordinary wave in a hot plasma at
w S i is shown in Fig. 6.
The auto-excitation of the electron (high frequency)branches of the eyAmined oscillations, when an ion cyclotronwave passes through 'bhb plasma, due to bunched instabilitywas investigated.
i. Introduction
I*The propagation of waves in a ylasma across a magnetic field
is characterized by interesting features near the gyro-frequencies
of the electrons and ions, and freniencies multiple to them. In
spite of the investigation -of this question by a whole series of
works [i--i3], it cannot be consldred fully explained. In the
present work, the frequt.ncies t of ordinaiy and extraordinary waves
which propagate across a magnetic field in a nonrelativistic plasma,
are determined and also the excl' ;ion of high-frequency (electronic)
branches of these oscillations when an ion cyclotron wave passes
through the plasma is ini;estigated. As is known, in the case of a
transverse propagation of waven in a plasma situated in an outer
magr.etic field HO, the dispersion equation, which determines the
frequencies t of these wwvez as a function of the jave vector k,
breaks into two equk1 .ions
(2)
where)
, . .. .....,,.(3 )
7r=-T- 3-67167.
*e4.4Z: 7i ~2
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k c/-- is the index of refraction. -a = (i4ve2n0/ma)/2, to
- eH0/mac -- is the Langmuirian and cyclotronic frequencies of parti-
cles of type -a, e = -- 1, s1 i, )n - Int) -- is the Bessel
function from 'he imaginary arguement, v, (Tama) I /2 -- is the
th~1e~c~y,= 2 2 ,2 2thermal/ velocity, pa = k V 2/a k Q a a -- is the Larmorian
radius of particles with thermal velocity.
Equation (i) determines the frequencies of an ordinary wave
which appears to be purely transverse (the intensity of the electric
field of this wave is perpendicular to the direction of propagation
and paiallel to the outer magnetic field H0 ). Equation (2) deter-
mines the frequencies of an extraordinary longitudinal-transverse
wave (the intensity of the electric field of that wave is perpen-
dicular to K and has a different (f.om zero) projection in the
direction of propagation).
Let us note, that the expressions of (3), for the tensor of
dielectric permeability Eij, can be used only for the fulfillment
of the inequality
where P - va/c. This condition denotes, that the dispersion of
frequencies of the cyclotron radiaticni particles with thermal
velocity, due to the relativ.stic (transverse) Doppler effect, is
small in comiparison with w When fulfilling the conditions of
(4), the cyclotron oscillation damping is exponentially small.
Below, we will investigate plasma oscillations close to
gyroreoonances. If the length of the wave is on the order of the
Larmorian radius of electrons or ions (P e i orp a"i), then the
square of the refractive index, when w f Wa is on the order c
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2 2
' Values aij $I ADc2/-2 if (D is not close to sto. It is obvious
i1 the resonances co so~a, are separated only when c,- A> m
in the case when the gas kinetic pressure of the plasma is consider-
Sably lower than the magnetic pressure,
LI (5)
'We w5-ll confine ourselves to the investigation of this case.
When i, the qualitative pattern of the frequency depend-
ence wc the wave vector is also the same when it, i; however, for
the determination of frequencies m(k), a numerical solution of
eq. i and 2 is needed. Upon the fulfillment of condition (5) it
is possible to obtain simple expressions for frequencies w(k), which
are close to s(Da -
2. Ordinary Wave Frequencies
Let us first of all examine Equation i in the case of high
frequency (electronic) oacillations when the movement of ions can
be disregarded. In the case of low density plasma (a. < ,a) the
value F.3 is comparable to w ,e* Pe ' i with (kc/) 2 c2 2/2
only when 1 -- sw / a PC But in this case the nonrelativistic
expressions of equation 3 for sEj cannot be used. Therefore, we
will examine the case of dense plasma (Se A-me). In this casemaintaining only a resonance component in the expression for e33'
we will obtain
(,.-4 )I,=-.,,Ij) (m,,, ...4 (6)
where
h C) f(7)
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Expression 6 can be used only for Le W xe' if Pe < Xe then in E.,
it is also necessary to maintain that a conrPonent with n = 0 in
addition to the resonance member. Then we will obtain
where (8)
The behavior of frequencies depending on the wave vector is
shown' schematically in Fig. io The frequency close to We at low
'e < xe±/2 decreases (Aml'%e - ee[ue + PJ)p it reachese~iunt e ~ t e
minimum at e %e/2 (LM/ e W -. eLI), and then it increases,
approaching asymptotically to we at pe * i. Frequencies close to
S e(s m 2,3, ...), decrease upon an increase in pe. reaching a
minimum at k . kmn nI/Q e, and then increase, approaching se
With an increase in the number s of branch oscillations, value k nin'
increases, and value Ia - soI) e/coe decreases in a minimum, whereby
functions (to -Se)/Ae change slowly at k eft.
I
L --
Fig. i.~ (a) uVo b & e
5-
-- -- "'Ole
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I N
Clear expressions for the refraction index as a frequency
functions a w *a se can be obtained in case of long wave oscilla-
t.ions (Pe- i) at s 1 1, 2 and in case of short wave oscillations
( e : i) for any sq j e
If co ce* Pe- , then
At xli i we will thus obtain
-- 0 -' ,.+ U- 'IIkell as olitl - (10)
If w 2 We 'and Pe i, then
2 ( 2 (1 - 2c*i/:WI
At w ace and ILLej' i the refraction index equals
The conclusion about the poa& lf-ty crf wave propagation in
plasma with a greater density at w - we was made by Drummond (i],
who obtained expression 10. (Formula iO was already obtained in
Gershman's work [2). Let us note that the numerical results for
k c/o. pbtained in report I from formula 10, are erroneous, i.e.
they lie outside the applicability area o' expression ±0 either
condition pe i i awrWy from frequency t wo is disrupted, or
6
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condition 1 Ix I -- wIIe3/2 W I close to )W
Expredsions 9 and ii were obtained in Stepanov's work [3], and
expression i2 were obtained in Ramashvili and Rukhadze's report [4],
and with the consideration of collisions, they were obtained in the
report by Demidov and Frank-Kamenetskiy [5] also.
An analysis of equation i without decomposition by degreen
Pe 0z- iie for plasma with an arbitrary ratio of gas kinetic pressure
to the magnetic pressure was mentioned in the report by Dnestrov-
skiy and Kostomarov [6], in which the appearance of new brnches
for the index of refraction at c - s'oe was indicated, and the
entire picture of the behavicr of refraction indices is explained
depending on the frequency. Let us note that the results of numeri-
cal calculations of the refraction index in the area com c se , given
in report 6 are incorrect, i.e. they belong to the case 1e < we and
lie outside of the area of applicability of the initial dispersion
equation.
In the low frequency area at a)o sci and.p e4 i we will obtain
the following expresr'on for the frequency from equation i.
The schematic behavior of the frequencies depending on k i is
shown in Fig. I for which it' is necessary to replace we by c i and
e by 'e
3. High-Frequency Longitudinal Oscillations
We will now go to the investigation of equation 2 in the caoe
of high-fr _ency (electronic,) oscillations. If the refraction
index is great (kc/c) 2 rw LJxe > 1, then in equation 2 a branch
of longitudinal oscillations, whose dispersion equation e,, 0O,
7
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will be presented in form of the following can be separated
'0'l ey - Pi i o.W .
As is evident from Fig. 2, on which the form of the function
y = f (w) is shown schematically, this equation has solutions
Fig. 2 5
N - t
2 Irk-
e: eIn_ jhe are pe; rm(4)w ilot
(b) L t 0 , /-,.
Fig. 2.
oKEY: (a) o+where
2 CO- . s(k) (s -1i, 2, ... ) corresponding "to intersection points
1, 2, ... of curves y = f '(,O) with a stra ht line y = e e
In the area I e 1. from (hf) we will •obtain
• -o . , ,,.., (o=,, ,..) (15)
or om ab (i + ), where
1 t. 8.3' w' '1 ' -, ')' (16)
v 8
:}-
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I.
If Le 1 1. then for frequencies close to s me, we will obtain
the expression
(w- ,,)l ,, aA'sO,.(s2x#,"*()') ..
The behavior of frequencies ,wo = cs(k) is shown schematically in
Fig. 3. at Ifl/we < 3 and in Fig. 4 f2 < 112 2 + f+j2.
As is evident from Fig. 4, frequencies as(k) at s < f decrease
monotonrically upon an increase of k, tending pe k i and s < f
toward s we" Frequency wi(k) (f we <'(fe2 + Me2)i/2 < ( + ) We)
at low pe rises with an increase of k, if J > i, it reaches
maximum at k Qe - i, then it monotonrically decreases, tending
toward f ae" At f = i, this frequency monotonrically decreases,
approaching we with a rise in k Qe" Frequencies greater than )s(k).
at s > f increase at low k e, reaching maximum at k e f i, and
then again approach s we. Expressions 15 s - f or s - f + i and
equation 16 are inapplicable, when the hybrid frequency 'o0 is close
to (f + i) we. In this case, maintaining the components in equation
14 with n -+ i and the resonance member n -f or n f + i, we will
obtain0m- .(1+e) (±7)
where
' *T\ _ .. WL .. 1)'(±8)
,,?; equations 17 and ±8 it follows, that frequency Wo, as well
.4 9 _
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iii
,i ____
Fig. 3.KEY: (a) frequency; (b) wave
"vec o.I
o|
(b) HiSH .. ,,d~ . ,
~Fig. .E:. (a) requcy (b)_wave
~vector.
wer obaied n Gos reot[]ada I ,3 . -i h
Siteko nd tep nrert[]
; iO
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The expressions for the refraction index of longitudinal
oscillations can be obtained in a clear form at p i and e )b i.
If CD sw, e then,.e e
kc - 1'- 2.-- ,- o -ts I I
At ae kiand w s w we have[l]e e
--- ge (20)
4. An Extraordinary Wave (High Frequencies)
Let us now examine equation 2 in the general case of plasma with f
greater density in the field of high frequencies. At p N e in
expressions 3 for 6iW. E22 and s12$ it is possible to leave only
the resonance components -/(,-- s coe)" Then we will obtain
"- = : ,() 1, ,,.. (21)
where
97, (;k) = 8 (MP - 1) VOW1 + 1 ) 1, - zI, 1] ( 22) :
At small pe the function ys( e) a P IeS/2E (s + l)1 increase
in ±.eI reaching maximum at ILe i i, and then decreases, approachingTs (Pe) - s/(27)i/2,3/2. (At pe > i function % (pe) and f
coincide asymptotically, therefore the refraction indeu of the
extraordinary and ordinary wave is determined by one and the very
same formula 12 [1]).
Li
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II
in the area p e hen e tensor Eij it is necesry to
consider also the components with n =+ i in addition to the resonance
wo.on nts N / _s to In this case we will obtain
• , o,, .,,)(23),+)
At 4 Le Xe this formula coincides with formula 21
In addition to the oscillations branch in the field of low
there is still another branch, whose frequency is determined by
expression
.,-,,,.. , . +.) + i,. )(.] ,3(24)me (Xe
The frequency of that branch settles away much farther from s eethan the frequency determined by formula 21. In the area mt
e efexpression 24 transforms into expression 15 for a frequency of
longitudinal waves (in the denominator of equation i5 in the case
question of dense plasma e 2e in comparison with i/(s2 - i)in 2/(
can be disregarded. In this way waves with the frequencies of
equation 24 are the long wave part of the branch of plasma
oscillations.
The behavior of frequencies w (k) depending on kQe for both
branches is shown schematically in Fig. 5.
Equation 2 has been numerically solved at low ILe and W f e
in Drummond's report (i], which mentioned the possibility of wave
passage with a frequency of w P we through dense plasma. (The
numerical results of the report [i] are erroneous, because at pe ± 1
for calculations a formula suitable only for p 4 i is used). The
expressions for the refraction index of an extrordinary wave at
12........
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I
Fig. 5.
wave vetor.
e e n e I were obtained
in report [3.
Dnestrovski-Kctmarov report [9] a-- analys-is of equation 2 in
the
general case (g" < is em. i, le > i) was made and
shown for the
existence- of n . oscil -lation branches at a) s we Let us note,
that the numrical calculations of the refraction index, dvlpd
in report 9 at - s we are invalid, i.e. for them ondition 4 of
the applicability of the expressions 3 for sij used in this case
is disrupted, Schematic graphs for" k c/, which correspond to
waves with the frequencies equation 21 are given in the Demidov
report CIO].
5. Low-Frequancy Pdazma "Oscillations
In case of low frequenc pIasma oscillations
( << e equation
-. 0 has the following form at e 'ci
0A
I t i n o b v o u s t h a t oe ff 5. a n w e l l a n e q u a t i o n 1 .4 h a s a
number'of olut o ns W m (k) ( mi, 2, 3, .. ) IyLn g in the interval
.33
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I
f C., <CD< (S, i .
in case of long wave oscillations (kQ i-C 1) we finid from
equation 25
J, ,.g. . . (26)
1or
* or 0 aw4f- I) (+(27)
where
" N- 0 + Iw') S-4.S JM
Expression 27 for a plasma oscillation frequency at Ta - 0
was derived by Koerper [ii]. A consideration of the thermal
movement of plasma particles, which leads to the limitation of
refraction indices of an unusual wave at w -.*ai, is given in report
3, £2, and £3. (Let us note, that in report 3 the thermal movement
of electrons was not considired; in report £2 the thermal movement
of ions was n)t considered; in addition the coefficient at N in
formula 12 of report [£2] should be mfltiplied by 2.)
In the area of short wave oscillations (Pi > i) from eq. 25,
we have
The dependence of the frequencies ws(k) on kQ i is schemtically
represented in Fig, 3 and Fig. 4 (it iz only necessary to make a
replacement of we by ci e by i and a0 by wk).
'1 1
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If the hybrid frequency wk is close to s ci then expressions
26 and 27 are inapplicable. In this case
-* (29)
where
itsp (30)
6. The Extraordinary Wave (Low Frequencies)
Let us first of all mention, that eq. 2 in a hydrodynamic
approximation (PeC i., P - i) has a solution w wc in the area
corresponding to a magnetic audio wave
W k -A (3:)
where
(3ia)
On the other hand, maintaining the rbsonance components in eij' we
will obtain
M-ee~~~4 1 eq(pf 0- - p..u -+-. (,.,,,0 ...) (32)
where function Ts(Li) is decermined by foryule. 22, or (at low Ii)
..-.. .*(..)a,i CM- ) (* z2, 3, ,..) (
~T~F~L(33)
Funtction 33 has an extirvu at points i "+ where
15
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.P4. function 32 -- has in points pi = 2 s i(s, 1,2, ... ),
The branch of oscillations with a frequency of eq,, 33 passes in the
area pi oti into longitudinal oscillations, investigated above(see formula 26).
Expressions 31 and 33 are applicable in the narrow area at2
Pi s 2 i . In this case instead of eq. 31 and 33 we will obtain
WZ2W+, where
--,-- .. = _1r,,i1/3 i](., - j[ 1l"-']
+,-412 8i 1 zi , ..l8 (34)
+ }' ( I-i) ( -. (,
At an increase in differentl I(l!t)"'2 -i formulas
34 and 34, change respectively into formulas 31, 33 and 31, 32.
M .1 + )IIIZ' A V~t W(35)
where91:t WZ=_ W. + [ V18l
8" /' +)! (/4 - 1A,)I//40
Formulas 35 at IxI l 1changes into formulas 32 and 33°
The dependence of frequencies %(k), determined by formulas
31-36, on the wave vector k is shown in Fig. 6. Let us discuss the
individual sections of curves 1, 2, 3; ... in Fig. 5 in greater de-
tail, Curve 1 in area pi < Y. corresponds to magnetic audio
oscillations with the frequency of eq. 31. In the area p. 0 xi the
frequency of this wave is determined by formula 34) for w+ ( in this
- i16 -
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6.t
... y; (a) f-requency; b rv -,-tiector.
case w - i ft -- X ii/2 W if < X- l 2) and at Ii > xi (l iXil Y- i ) by formula 32. Curve i reaches maximum at P, s- 2x, (in
2A
this case w - i- -- ii and then drops, At PiI i curve I has
a minimum a) - i -i ) With a further increase of p. curve
i approaches asymptotically to ai.
The frequency of the branch of ohcillations corresponding to
curve 2 is determined by formulas: 32 at p. < xij at Ii " Ili 34'
f or w+, (in this case u>- u m xi i/2wi, if lI .- " Xi < Xi 2 ) ; 31 -
In area x, < Pi < 4 i; 34 for w_ (s - 2) and 33 in the area 4xi <
< i (s 2 ). Curve 2 reaches maximum -;L Pi= P+ - 6.3x,; (in
this case w - 2 11i " - 1 ) -' and then decreases, converting.
into a branch of longiudinal oscillations, whose frequency tends
towar'd w., when pi e 1o
Curves -2 s - i - 3P 5o 7 whose form at i (0 are
22
ftrmined by formula 32. dCrve i reach maximum at 1 Xi (in
' in this case . - U and then drops.eAty cure hase
A i = 0hefrofteecurves2 is determined by formulas 2 t 35<~~ a
i/2fo 1(nthscs if''~i
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32. That curve rt-hehes maximum at + (in this - s mi
Xj s+i wi); it then dec -eases, reaching minimum at pi g 1," (co-s
s ii ED and then approaches s Wi"
Point p is displaced to the right with an increase of s, and
value a2 at an increase of s decreases).
Curves f - 2 s 4 1, 6, ... are determined by formulas: 32
i at i-i < P0 ' 35 fol-J at P, " o (in this case c - s '0m S wi ) ,
33 at <s 2 g' <.x s )3 for a+t at p s Xi;II2 (s± 2 ,3atS (si 2
3iat s (i < (B + i) 34 at p - (s + i)2 i (in this case
it is necessary to replace s by s + i in formula 34, 33 at (s + 1)
x i < Pi i (here it is also necessary to replace s by s + i). in
this area gi %i this curve determines the frequency of plasma
oscillations which decreases with an increase in pi approaching
s co Curve f = 2 s has a maximum at pi. p+ (in this case c -
(s + i) y! - X s + i co). which lies below the minimum of curve
= s + i at point pi. p_, where p_ is determined by formula 33,
in which s should be replaced by s + i.
The obtained expressions for frequencies can be used only at
s2 2 2
Let us note that for curve sections w(k), which decrease with
an increase in k, group and phase velocities of the waves are
directed in opposite directions.
7. Excitation of Electronic Oscillations When Ions CyclotronIJ Waves Pass Through Plasma
When an ion cyclotron wave passes through plasma, electrons
and ions acquire a relative velocity u in the field after that
wave has passed, If u W v., then in the plasma beam instability
may originate [i4]. We will examine the excitation of extraordinary
18
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and ordinary waves in dense plasma investigated above by an ion
stream caused by the field of a cyclotron wave. We will assume
that the wave length of.the excited waves.is considerably smaller- .
than the length of an ion-cyclotron wave and the time of develop-
ing the instability is considerably less than the time of turning
the ions in the magnetic field H.. Then the value u(t) can be
considered as a constant value and the effect of the magnetic
field on the perturbed movement of ions may be disregarded.
The contribution of ions into the tensor eiJ in the reading
system in which electrons rest, equals
_____Dig Dk it,i'C(w-kux)'+k'Ui'J w{ -k _)'
f2
Disregarding the components C Eij, we will obtain from the
dispersion equation
dot [(h ( -V 6) + (a"@ + 0)J O (36a)
two equations
(kc*~ (37)L
(c,= +'.ll') (,ko/o)'- (ell + #I&,) (#g. +eo.') - ,, 0 (8
where ii Es 2 2 J s33 and E12 are determined by formulas 3, in which
i9
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ii[
I
it is only necessary to consider the contribution of the electrons.
Let us first of all examine the excitation of a usual wave.
Assuming
where ,%(k) is a solution of eq. 37 at i= 0, determined by
formula 6, we will obtain w(k) = kxu, at resonance which
-I + i31, -,.k,,,.,(o,- ev,.} 111 (4 0)E = 2 Llm, (1rP - 0Is m) as '"
At ve (kq e" i) by the order of magnitude e (Xe2m/mi)i/3
5.
In case of the excitation of a longitudinal-transverse extra-
ordinary wave, whose frequency is determined by formula 21, we will
find w s(k) - k ux , in resonance conditions that
a ((-1 +i3,)l2] (,,.,,w/,d)1yl~) @.(11_-,7,), (.4 1 )
At uxft Ves X e± we have e 2 me/mi)/we.
Let us now investigate the excitation of longitudinal
oscillations. The dispersion equation of these oscillations, E.l
+ - 0, has the form
o'i'( l-u. ) - ,_,' (42)
a--r ,. .._,-
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The component M fl, plays a substan-i.! role Ln equation 42 at a )
k . Assuming cD = k ux+, we will fid thatx
___ __ (413)
Hence it is evident that the exciiation of oscillations (IM r > 0)
takes place at s toe <k ux <ms, where -s is the frequency of M
longitudinal oscillations (E,= 0 at w - (k)). The increment of
increase in expression 43 increases at k ux -0 s. However, ex-
pression 43 can be utilized only at Im - k u~I >Is;4" At Ic -
k Uxj j a the increment reaches a maxiium value
.4 +ia2 P(,i y 08itv (44)-s-IX
If i, Ux' Ve, then E (mem i/ic e At vi qux, ve and
11e 3pi formula 44 coincides with the result of report 14.
In conclusion the authors thank A. I. Akhiezer for evaluating
the work and for useful council.
Literature
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2. Gershman, B. N. "Zh. eksp. teor. Fiz." (Journal ofExperimental and Theoretical Physics.) 24 (1953) 659.
3. Stepanov, K. N. "Doklad na i konterentsii Fizikotekhicheskogo Ingtituta Akademli Nauk Ukrainskoy SSR po fizike plazmy iprobleme ypravlyaemykh termoyadernyx reaktsiy (Khar'kov, iyun,-iyul,±959); v sbornike Fizika Plazmy i ProbleaW Ypravlyaemogo Termoyadernopo Sinteza (K. D. Sinel'nikov, red.). Izdatel'stvo Akademii NaukUSBR, riev i (962) 52" (Report at the ist Conference of the Physics-Technicil Institute of the Academy of Sciences of the UkrainianSSR for Plasma Physics and the Problem of Controlled Thermonuclear
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Reactions (Khar'kov, June-July 1959); in the Collection of PlasmaPhysics and the Problems of Controlled Thermonuclear Synthesis(K. D. Sinel'nikov, editor). Publiehing House of the Academy ofSciences of the Ukrainian SSR. Kiev i (1962) 52.
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Academy of Sciences of the USSR) 139 (i9jI) 1342.
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Sinel'nikov, red.). Izdatel'stvo Akademi- Nauk USSR, Kiev"(In the Report of Plasma Physics and Problems of Controlled Ther-monuclear Synthesis (K. D. Sinel'nikov, editor). PublishingHouse of the Academy of Sciences of the Ukrainian SSR, Kiev 3.(±963) 3.
14. Kurilko, V. I., Vi I. Miroshnichenko. "v sbornikeFizika Plazmy i Problemy Upravlyayemogo Termoyadernogo SintezaK. Do Sinel'nikov, red). Izdateltstvo Akademii Nauk USSR. Kiev"(n the Report of Plasma Physics and the Problems of ControlledThermonuclear Synthesis (K. D. Sinel'nikov, editor). PublishingHouse of the Academy of Sciences of the Ukrainian SSR. Kiev 3 (1963)
Manuscript submitted 4/6/64
FTD-HT-23-671-67 22
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