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Astrophysics/cut-off frequency v. resonant frequency

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Question
For parallel propagation in an EM field, how can one *quantitatively* distinguish the cut-off plasma frequency from the resonant one?

Answer
Hello,

In your parallel propagation (3D) case, we assume: w >> W _i

(e.g. plasma electron frequency much higher than ion cyclotron frequency) and for our fields:

B1  =  k X  E1  = (B_x, B_y, 0)


E1 =  (E_x, E_y, 0)

Curl B = 4 pi J1/c  +  E1'/c


where E1' denotes a time derivative and in the high frequency regime one has: J1 = - en_o v1

In terms of the E-field components (E_x, E_y) one can set out a matrix:

( [1 + k^2c^2/w^2 - w^2/w_e^2) (i W_e/w_e^2(w - k^2c^2/w))

(-i W_e/w_e^2(w - k^2c^2/w)  (1 + k^2c^2/w_e^2 - w^2/w_e^2))

=  0


from which we can simplify key quanitites in each of the brackets, viz.

w* = w/W_e,   b^2 = (k^2c^2/w_e^2), a^2 = W_e^2/w_e^2

From this we can write the matrix eqn. out:


a^2 w*^2 (w* +/- 1) - w* - b^2(w* +/- 1)  = 0


It can easily be seen from the above that one gets an equation in w* with order 3 (w*^3) so there must be three roots for the plasma frequency w* and hence for w.

The one called "cut-off frequency" is that for which k = 0, this implies b = 0 (since as we saw: b^2 = (k^2c^2/w_e^2)) so: the root for plasma frequency obtained (call it w_k) is the cut-off frequency. (For the other roots, one finds w* = 0, and w* = w_L denoting left hand circular polarized wave)

The "resonant frequency" for the same conditions (parallel propagation in E, B field as defined) can simply be found by noting that the same disperson relation (eg. in w, k) applies but in the limit k -> oo. For which one will find:

w =  W_e

Hope this helps, and isn't too complicated!  

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Philip A. Stahl

Expertise

I specialize in stellar and solar astrophysics. Can answer any questions pertaining to these areas, the spectroscopic analysis of stars – as well as the magneto-hydrodynamics of sunspots and solar flares. Sorry – No homework problems done or research projects! I will provide hints on solutions.

Experience

Have published papers on the relationship between sunspot morphology and solar flares; discovery of SID flares related to this, constructed computerized stellar models; MHD research.

Organizations
American Astronomical Society (Solar physics and Dynamical astronomy divisions), American Geophysical Union, American Mathematical Society, Intertel.

Publications
Solar Physics, Journal of the Royal Astronomical Society of Canada, Journal of the Barbados Astronomical Society, Meudon Solar Flare Proceedings (Meudon, France). Books: 'Selected Analyses in Solar Flare Plasma Dynamics', 'Physics Notes for Advanced Level'.

Education/Credentials
B.A. degree in Astronomy; M.Phil. degree in Physics - specializing in solar physics.

Awards and Honors
Postgraduate research award- Barbados government; Studentship Award in Solar Physics - American Astronomical Society

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