Power Distribution of Magnetospheric Whistler Mode Waves with Finite Electron and Ion Temperature

被引：0

作者：

Maxworth, Ashanthi ^{[1
]}

Golkowski, Mark ^{[1
]}

Malaspina, David ^{[2
]}

Jaynes, Allison ^{[2
]}

机构：

[1] Univ Colorado, Dept Elect Engn, Denver, CO 80204 USA

[2] Univ Colorado, Lab Atmospher & Space Phys, Boulder, CO 80303 USA

来源：

2017 XXXIIND GENERAL ASSEMBLY AND SCIENTIFIC SYMPOSIUM OF THE INTERNATIONAL UNION OF RADIO SCIENCE (URSI GASS) | 2017年

基金：

美国国家科学基金会;

关键词：

D O I：

暂无

中图分类号：

TM [电工技术]; TN [电子技术、通信技术];

学科分类号：

0808 ; 0809 ;

摘要：

Whistler mode waves play an important role in energy dynamics of Earth's magnetosphere. A majority of the previous work on whistler mode raytracing in the Earth's magnetosphere was done assuming a cold background plasma (0 k) even though the temperature of electrons and ions is around 1eV In this work we present our recent results on power distribution and lifetime of whistler mode waves with the inclusion of finite electron and ion temperature. The simulated power distribution results with finite temperature effects show a better agreement with the Van-Allen Probe space craft observations than the simulated results under cold plasma assumptions.

引用

页数：2

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