Low frequency waves in plasmas with spatially varying electron temperature

被引:8
作者
Guio, P
Borve, S
Pécseli, HL
Trulsen, J
机构
[1] Univ Oslo, Inst Theoret Astrophys, N-0315 Oslo, Norway
[2] Univ Tromso, Auroral Observ, Inst Phys, N-9037 Tromso, Norway
[3] Univ Oslo, Dept Phys, N-0316 Oslo, Norway
来源
ANNALES GEOPHYSICAE-ATMOSPHERES HYDROSPHERES AND SPACE SCIENCES | 2001年 / 18卷 / 12期
关键词
ionosphere; plasma temperature and density; radio science; waves in plasma; space plasma physics; numerical simulation studies;
D O I
10.1007/s005850000299
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Low frequency electrostatic waves are studied in magnetized plasmas with an electron temperature which varies with position in a direction perpendicular to the magnetic field. For wave frequencies below the ion cyclotron frequency, the waves need not follow any definite dispersion relation. Instead a band of phase velocities is allowed, with a range of variation depending on the maximum and minimum values of the electron temperature. Simple model equations are obtained for the general case which can be solved to give the spatial variation of a harmonically time varying potential. A simple analytical model for the phenomenon is presented and the results are supported by numerical simulations carried out in a 21/2-dimensional particle-in-cell numerical simulation. We find that when the electron temperature is striated along Bo and low frequency waves (omega much less than Omega (ci)) are excited in this environment, then the intensity of these low frequency waves will be striated in a manner following the electron temperature striations. High frequency ion acoustic waves (omega much greater than Omega (ci)) will on the other hand have a spatially more uniform intensity distribution.
引用
收藏
页码:1613 / 1622
页数:10
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