Saturation of electron cyclotron maser by lower-hybrid waves

被引:0
|
作者
Fleishman, G
Arzner, K
机构
[1] Inst Extraterr Phys, D-85740 Garching, Germany
[2] Ioffe Inst Phys & Technol, St Petersburg 194021, Russia
来源
ASTRONOMY & ASTROPHYSICS | 2000年 / 358卷 / 02期
关键词
Sun : radio radiation; masers;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We perform a numerical study on the quasilinear relaxation of an electron cyclotron maser on the initially dominant mode. We focus thereby on a situation where the initially dominant modes are quasi-electrostatic lower hybrid (1h) waves, which have not been treated in preceding studies. To this end, we chose 0.2 less than or equal to omega(p)/omega(Be) < 0.5 (omega(p): plasma-, omega(Be): electron cyclotron frequency) and an initial losscone distribution of energetic electrons of the form f(p, mu) similar to p(-xi)e(-mu 2/mu 02) (p: momentum, mu: pitch angle cosine). Superimposed on this is a damping Maxwellian background. From our calculations, we find that multiple peaks in the lower-hybrid wave intensity can occur if the initial loss cone distribution is sufficiently broad. We also find that quasilinear relaxation with respect to lower-hybrid waves does not destroy the capability of the electron distribution to amplify transverse (XOZ) waves, which therefore become dominant at a later stage. The comparison with observations shows that the calculated shape of a single peak in the lower-hybrid energy density displays a remarkable similarity to solar radio spikes.
引用
收藏
页码:776 / 788
页数:13
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