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Submitted on 1 Jan 1990
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Relativistic effects on the TM-modes of one boundary
corrugated parallel plate waveguide filled with uniaxial
warm drifting plasma
Rajendra Prasad, Ramjee Prasad, A.N. Mantri
To cite this version:
Relativistic effects
onthe
TM-modes
of
oneboundary
corrugated parallel plate
waveguide
filled
with uniaxial
warmdrifting plasma
Rajendra
Prasad(1),
Ramjee
Prasad(2)
and A. N. Mantri(3)
(1)
Department
of Natural Sciences, MutahUniversity,
P.O. Box 7, Mutah, Karak, Jordan(2)
Faculty
of ElectricalEngineering,
DelftUniversity
ofTechnology,
P.O. Box 5031, 2600 GADelft,
The Netherlands(3)
Department
ofPhysics,
Banaras HinduUniversity,
Varanasi-221005, India(Reçu
le 24 janvier 1990, révisé le 23 mars 1990,accepté
le 3 avril1990)
Abstract. - The relativistic effects
on the TM-modes of one
boundary corrugated parallel plate
waveguide
filled with uniaxial warmdrifting plasma
have beeninvestigated.
Thedispersion
relation for the TM-modes has been derived and the numerical
computations
have been carriedout to
study
the effects of increased(relativistic)
driftvelocity
and the temperature under this condition. The effects of driftvelocity
arequite
distinct andsignificant
over the non-relativistic case. The effect of temperature in the relativistic case isremarkably insignificant
unlike thenon-relativistic case where it was
quite pronounced.
Classification
Physics
Abstracts52.40D
1. Introduction.
In a recent paper
[1] we
studied the characteristics of theelectromagnetic
wavepropagation
through
oneboundary corrugated parallel plate waveguide
filled with warm uniaxialdrifting
plasma, using purely
non-relativistic treatment.However,
to simulate the actual behavior of theplasma
and to obtaingreater
insight
of theproblem,
the more realisticapproach
wouldobviously
be the relativistic one. The relativistic effect has now been included in thissequel
toreference
[1].
In thepresent
paper, the driftvelocity
of the boundedplasma along
the axis of thewaveguide
has been assumedlarge enough
to be treated as a relativisticparameter.
The effects of the relativistic driftvelocity
andtemperature
of theplasma,
under thiscondition,
on the TM-modes of thewaveguide
have been studied in detail. These results are ofgreat
importance
due to their wideapplication
inplasma diagnostics
[7].
2. Basic theoretical
concept.
Referring
to thegeometry
of theproblem
(one
boundary corrugated parallel plate
waveguide)
described in reference[1], consider,
two frames ofreference,
S and S’.Let,
S be attached(stationary)
to thewaveguide
and be describedby
thespace-time
coordinates(X,
Y,
1510
Z,
t).
S’ is fixed to theplasma
mediummoving
with a constantvelocity, Vo
withrespect
toS,
and is described
by
the coordinates(X’,
Y’,
Z’,
t’).
The frame S’ movesonly along
thelongitudinal
Z-axis withvelocity, Vo
=ho à,.
The field vectors vary
harmonically
as,
-where,
w’ is theangular
wavefrequency
andy’
is thecomplex propagation
constant.2.1 LORENTZ TRANSFORMATION EQUATIONS. - The Lorentz transformation for the
space-time coordinates is well known and is
given [2] by,
and
where,
r =( 1 -
a 2)- 1/2
with a =VOIC
and C is thevelocity
oflight
infree-space.
The Lorentz transformation
equations (without rotation)
for the electric(E)
and themagnetic
(H)
field vectors infree-space
aregiven
[3, 4]
by,
and
where,
J.Lo and Eo arepermeability
and thepermittivity
of thefree-space, respectively.
The Lorentz transformations for the wave vector,frequency
andplasma
parameters
aregiven [4, 5] by,
where,
p,py,
pz are the wave numbersalong
X, Y,
Zdirections,
Pz= - j y,
a is the electron thermalvelocity
indicative of the averagetemperature
of theplasma,
cv p
is theangular
plasma frequency,
defined asco p
=(Ne2/mëo)1/2, N
is the electrondensity,
and m and e are the mass andcharge
of theelectron,
respectively.
In view of
equation (2.1.3),
we canwrite,
2.2
EQUATIONS
IN UNBOUNDED PLASMA MEDIUM. - Maxwellequations [6] describing
the time harmonic fields in an unbounded warmplasma
medium(in
the frameS’)
can be writtenas,
where,
s’ is the dielectric tensor of theplasma
medium and isgiven [1]
by,
where,
It is
imperative
to note that theexpression
fore;z
does not contain thevelocity
term[1]
because the
plasma
is attached to the S’-frame.Now,
using equations (2.2.1 )
to(2.2.6),
the waveequations
and the fieldexpressions
can be derived and are obtained as,where,
kô
= cv’/C
and thesubscript
T denotes the transversecomponents
of the field vectors.3. TM-modes
(11;
= 0 ) dispersion
relation.The wave
equation (2.2.7),
in this case, takes theform,
The
boundary
conditions to beapplied
are as referred in reference[1]
and aregiven by,
where,
X = 0 is the lowerboundary
surface,
X= e
(Z’ )
is the upperboundary
surface, b
andL are the
amplitude
and thewavelength
of theperiodic
function,
respectively,
and d is the average distance between the twoplates.
Thus,
in view ofequation (3.2),
the solution ofequation (3.1 )
is obtained as,where,
h =n -ff / e (Z),
with n =0, 1,
2,
3,
... and
Eo
is constant.1512
where,
(ù c is the cut-offfrequency
of theparallel
plate waveguide
filled withfree-space
and isexpressed
as,Now,
transforming equation (3.4)
from S’ to S frameby
using
Lorentz transformationequations (2.1.1), (2.1.3)
and(2.1.4)
andnormalizing
the variables as,after a rather
lengthy algebra,
we obtain thedispersion
relation as,where,
Since,
we aredealing
with the lossless case, we assume, G= j B
inequation (3.7)
and rewriteit as,
It can
easily
be seen thatfor
1 a
1
«1,
thatis,
1 il a 1 z
1 BI,
equation (3.9)
reduces to theequation (29)
of reference[1].
This confirms the exactness of the derivation of
equation (3.9)
for the relativistic case.Further,
using equations (2.1.3), (2.1.4), (2.1.5), (2.2.9), (2.2.10)
and(3.4)
thefollowing
fieldcomponents
of TM-modes in S frame are obtained as,where,
4. Numerical results and discussion.
In order to
study
the relativistic effects on thephase
characteristics of the TM-modes of oneboundary corrugated waveguide
[b/d = 0.01
and(Z-Vot)/L=O.5],
thedispersion
Fig.
1. - Phase characteristics of thecorrugated
waveguide
filled with uniaxialplasma, il c
= 2.0,a = 0.4, 8 = 0.03,
b/d
= 0.01 and(Z - Vo
t)/L
= 0.5.Fig.
2. - Phase characteristics of the fast and the slowwaves
showing
the effect of relativistic driftvelocity.
5 = 0.03,ne
= 2.0,b /d
= 0.01 and1514
Fig.
3. - Phase characteristics of the fast and the slow wavesshowing
the effect of temperature.a = 0.5,
ne
= 2.0,b/d
= 0.01 and(Z - Vo
t)/L
= 0.5.Figure
1represents
the f2 - B characteristics for warm(8 = 0.03 ),
uniaxial(Bo =
ooâz)
anddrifting ( a
=0.4) guided
wave(f2c
=2.0) propagation.
As before[1],
onemay
identify
infigure
1,
HGI as the« waveguide
wave », ABOC as the « fast wave », DE as the« slow wave » and BG as the
non-propagating
mode. Theportion
AB of the « fast wave » is termed as the « backward wave »(the slope
dn IdB
being negative).
Oncomparing
the non-relativistic results of reference[1]
with those offigures
1 to 3 for the relativistic case, we notice thefollowing
remarkable distinction between the two results.In
figure
1,
the« waveguide
wave » becomes wider and the vertex remains at almost the samepoint.
The « slow wave » becomes almost linear(straight).
The effects of increased driftvelocity
is shown infigure
2. The « slow wave »approaches
theorigin
as a increases and at a = 0.5 itoriginates
at theorigin.
The « backward wave »disappears
at a = 0.5. For a> 0.6,
both the « fast » and the « slow » wavesjoin together
at the start andoriginate
at thesame
point (origin).
At a = 0.8(dashed curve),
the « slow wave » becomesexactly
linear(straight line).
The effect of the driftvelocity
on the OCportion
of the « fast wave » is the same as before.Figure
3 exhibits the effect oftemperature
(under
relativistic driftvelocity condition)
on the« fast » and the « slow » waves. It can be noticed in the
figure
3 thatpractically
there is no effect oftemperature.
For 8 =0.0,
0.01 and0.02,
the curves areexactly
the same. For 8 =0.03,
there is aslight
deviationbut,
within statistical error, the curves(fast
and slowwaves)
occupy almost the samerespective
positions
as thosecorresponding
to the other valuesReferences