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Electromagnetic Ion Cyclotron Waves in Multi-Ions Hot Anisotropic Plasma in Auroral Acceleration Region-Particle Aspect Approach

机译:极光加速区域中多离子各向异性热等离子体中的电磁回旋波-粒子长宽比方法

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摘要

Using particle aspect approach, the effect of multi-ions densities on the dispersion relation, growth rate, perpendicular resonant energy and growth length of electromagnetic ion cyclotron wave with general loss-cone distribution function in hot anisotropic multi-ion plasma is presented for auroral acceleration region. It is observed that higher He+ and O+ ions densities enhance the wave frequency closer to the H+ ion cyclotron frequency and growth rate of the wave. The differential heating of He+ ions perpendicular to the magnetic field is enhanced at higher densities of He+ ions. The waves require longer distances to achieve observable amplitude by wave-particle interactions mechanism as predicted by growth length. It is also found that electron thermal anisotropy of the background plasma enhances the growth rate and reduces the growth length of multi-ions plasma. These results are determined for auroral acceleration region.
机译:利用粒子长宽比方法,提出了多离子密度对热各向异性多离子等离子体中具有一般损耗圆锥分布函数的电磁离子回旋波的色散关系,生长速率,垂直共振能量和生长长度的影响,以实现极光加速区域。观察到较高的He + 和O + 离子密度使波频率更接近H + 离子回旋加速器频率和波的增长率。垂直于磁场的He + 离子的差分加热在He + 离子的较高密度下会增强。这些波需要更长的距离才能通过生长长度所预测的波粒相互作用机制达到可观察到的振幅。还发现背景等离子体的电子热各向异性提高了生长速率并减小了多离子等离子体的生长长度。确定了极光加速区域的这些结果。

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