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Quasi-Thermal Noise in Bernstein Waves

The calculation of the QTN in Bernstein waves [Sentman, 1982] can be generalized to the case where the dispersion equation has multiple solutions. In that case, using (22) of [Meyer-Vernet, Hoang and Moncuquet, 1993], we deduce an approximate expression for the noise measured by an antenna in the plasma frame

  eqnarray97

where tex2html_wrap_inline779 denotes the multiple solutions of Bernstein's dispersion equation for the angular frequency tex2html_wrap_inline769 , L is the antenna length (35 m), tex2html_wrap_inline807 is the angle between the antenna and tex2html_wrap_inline715 , tex2html_wrap_inline811 is the antenna response to Bernstein waves, tex2html_wrap_inline813 is the real part of the dielectric function, and tex2html_wrap_inline815 is Boltzmann's constant. Since the antenna moves with respect to the plasma, we must add to (2) an integration over the direction of tex2html_wrap_inline779 with respect to tex2html_wrap_inline767 , involving the solutions of the Doppler-shifted dispersion equations [Moncuquet, Meyer-Vernet and Hoang, 1995]. The term tex2html_wrap_inline821 is the (small) range in parallel wave vector for which the hot population makes a dominant contribution to the QTN. This term vanishes at gyroharmonics where thermal electrons damp Bernstein waves, resulting in the well-defined noise minima observed at gyroharmonics during the Io torus traversal [Meyer-Vernet, Hoang and Moncuquet, 1993].
Equation (2) does not hold near resonant solutions where tex2html_wrap_inline823 . In this case, the spectral density increases until the first-order approximation of tex2html_wrap_inline825 used to derive (2) breaks down [Sentman, 1982], then the maximum voltage is set by the second derivative tex2html_wrap_inline827 . Here we shall not try to compute tex2html_wrap_inline829 at resonances (below we show it is not necessary), but we note that since the energy flux is expected to remain constant, the noise level should continue to increase as the group velocity vanishes, reaching a maximum at resonances. Equation (2) and the above remark allow us to summarize two important properties of the QTN, which the observed spectra should exhibit: (1) In the upper hybrid gyroharmonic band, the spectral density tex2html_wrap_inline829 should reach high levels at each resonance and in some frequency band around it, since the tex2html_wrap_inline611 and tex2html_wrap_inline653 peaks are smoothed out by the Doppler shift corresponding to different tex2html_wrap_inline779 directions. Note that since tex2html_wrap_inline811 vanishes for small argument ( tex2html_wrap_inline841 ), the peak at tex2html_wrap_inline761 (where tex2html_wrap_inline759 ) could be attenuated, and if the range of variation of tex2html_wrap_inline807 is large enough, the noise should be spin modulated. (2) The signal should plummet in the forbidden bands between the largest Doppler-shifted tex2html_wrap_inline615 of the considered harmonic band and tex2html_wrap_inline789 (or slightly below that gyroharmonic, because of the Doppler shift as explained in section 2).


next up previous
Next: Observations and Discussion Up: Detection of Bernstein wave Previous: Theoretical Bernstein Q Resonances

Michel Moncuquet
Tue Nov 18 19:11:02 MET 1997