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HAL Id: jpa-00219281

https://hal.archives-ouvertes.fr/jpa-00219281

Submitted on 1 Jan 1979

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ELECTROSTATIC TRIVELPIECE-GOULD MODES IN A TORUS

F. Stössel

To cite this version:

F. Stössel. ELECTROSTATIC TRIVELPIECE-GOULD MODES IN A TORUS. Journal de Physique

Colloques, 1979, 40 (C7), pp.C7-603-C7-604. �10.1051/jphyscol:19797292�. �jpa-00219281�

(2)

JOURNAL DE PHYSIQUE CoZZoque C7, suppZ6ment au n07, Tome 40, JuiZlet 1979, page C7- 603

ELECTROSTATIC TRIVELPLCE-GOWD MODES

IN

A TORUS

F.P. Stksel.

I n s t i t u t e for l'heoreticaZ Physics, Universi.ty- o f Innsbruck, Innrain 52, A-6020 Innsbruck/Austria, Europe.

Abstract: Electron plasma waves are treated in a V ~ Y = 4x en 1 torus of square cross section with an infinitely

aE

-

(k,~/m)"~ is the velocity of sound. This strong azimuthal magnetic field. Eigenfrequencies

leads to the following equation for the electrosta- and eigenfunctions are calculated numerically.

tic potential:

Although many experiments were performed in to- -v2y

a

- a2 12 E o v ~ +ylo2 e a2 ~ r = 0 y roidal devices a well-developed theory of toroidal

a

t2 r2 a@2 r a@2 waves is not available as yet. As a step in that

Variahles can be separeted by the following ansatz:

direction electron plasma waves are investigated in

iwt iknz im@

a toroidal cavity of square cross section, i.e. the Y = e e e Tl(r) same configuration as used by Swanson (1) in dis.-.

cussing ion cyclotron and fast waves. Cylindrical coordinates r,

9,

z are used. The torus has a major radius R and a square of lateral length 2ro

.

The cavity is completely filled with a homogeneous plasma, and the walls are ideal conductors. In con- trast to the original paper by Trivelpiece and Gould (2), where the magnetic field has only a com- ponent in the z-direction, the magnetic field here lies in the $-direction. A linearized fluid descrip- tion is used (3).

The uniqueness-condition restricts the mode numbers m to integers; m=O describes the steady-state solu- tion. The perfectly conducting walls require that Y vanishes at the walls, i.e. Y(r, z=0) =

= Y(r, z=2r ) = 0, which results in a sinusoidal z-dependence (u sin k z with k = n?r/2ro) and in

n n

the conditions y(r=R-ro, z) = Y(r=R+ro, z) = 0 whence we obtain boundary conditions for the radial eigenfunctions T (r) which obey the following dif-

1 ferential equation:

The magnetic field is assumed to be infinitely 1 m2 w2

TI''

+ 7

TI' + ( pe

- - -

m2 k:) .TI = 0 strong, so that the r- and z-components of the ve- r2U2 - m2ai r

locity can be neglected. Thus the system of line- Primes denote derivatives with respect to r. This arized equations consists of the equation of con- eigenvalue problem with w as the eigenfrequency was ti nu it^, the $-.component of the equation of motion, solved numerically by a shooting method. Numerical and Poisson's equation: values typical of large present-day experiments

were chosen. E.g,, the Debye-length was set equal to 7.43xl0-' x R. The figures below show some I a examples of the eigenfunctions T, for an inverse

a

= - a 2 L ? L n l + e n --y

"0

TF

$ E r a$ rn era$

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphyscol:19797292

(3)

aspect ratio a = 0.3. The eigenfunctions are nor- malized by setting dT/dr = I at r = R

-

r The

0'

first six modes in 1 (1 = 1

-

6 ) are plotted one over another in each figure for mdl, n=l in Fig.1, for m=3, n=3 in Fig.2,and for m=5, n=5 in Fig.3.

Fig. 1

The eigenfrequencies w / w for these cases are:

Pe

From the figures one can clearly see the deviation of the radial eigenfunctions from symmetry about r = Rwhich should obtain for linear geometries.

For the appropriate linear geometry, a parallelepi- ped of length ZrR, and side-length 2ro, the eigen- functions are sinusoidal. The deviation increases with the inverse aspect ratio, i.e. with the cur- vature of the torus. However, as can already be suspected from the three examples given here, it turns out that the mode number n has much more in- fluence on the shape of the eigenfunctions than the aspect ratio. On the other hand variation of m changes the eigenfrequencies but does not alter the shape of the eigenfunctions.

The eigenfrequencies for linear geometry are generally somewhat smaller than those for the to- xus, For the above-mentioned examples, the devia- tion lies within 1

-

4 % for most of the modes and reaches a maximum of 23 % for the 1=1, m=5, n=5 mode.

This work bas been supported by the Gsterreichi- scher Ponds zur Farderung der Wissenschaftlichen Forscfiung Grant Nr. 2781/S.

References

(1) Swanson B.G., Phys.Fluids

2,

1974, 2241 (2) Trivelpiece W., Gould R.W., J.Appl.Phys.

30

1959, 1784

(3) Cap F.F., Handbook on Plasma Instabilities, Academic Press London, 1978, vo1.2, p.817

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