Two modes of ion-ion hybrid waves in magnetospheric plasma

被引:5
作者
Mikhailova, Olga S. [1 ]
Mager, Pavel N. [1 ]
Klimushkin, Dmitri Yu [1 ]
机构
[1] RAS, SB, Inst Solar Terr Phys, Irkutsk, Russia
关键词
magnetosphere; ion-ion hybrid waves; heavy ions; waves in plasma; STANDING ALFVEN WAVES; 1-2 MAGNETIC PULSATIONS; FIELD LINE RESONANCES; ULF-WAVES; EQUATORIAL MAGNETOSPHERE; SOLAR-WIND; RESONATOR; PRESSURE;
D O I
10.1088/1361-6587/ab5b32
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
This paper is concerned with the structure of ion-ion hybrid (IIH) waves in multicomponent magnetospheric plasma in the dipole geomagnetic field model. Like Alfven waves, in IIH waves the field line can oscillate in different directions: in the azimuthal direction (the toroidal modes) and in the radial direction (the poloidal modes). Contrary to Alfven waves, in IIH waves only the equatorial part of the field line can oscillate, since due to the heavy ions admixture the IIH waves are trapped in the resonator in the vicinity of the geomagnetic equator. The equatorial localization of the waves allow the calculation of the parallel structure of the toroidal and poloidal IIH modes analytically. It was found that the toroidal and poloidal modes have slightly different structures and that their frequencies are also slightly different. The difference between toroidal and poloidal frequencies (the polarization splitting) is small with respect to the basic harmonics of each mode. It was found that IIH modes have a considerable compressional component of the wave's magnetic field.
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页数:9
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