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Generation and amplification of HM emissions by ion-cyclotron instabilities

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Abstract

This paper describes the analysis of the growth rate of hydromagnetic waves in the magnetosphere in ion-cyclotron mode considering multicomponent thermal plasma. Effects upon growth rate have been estimated due to (a) Thermal velocity of background plasma; (b) Presence of Heliumions in background plasma; (c) Beam Velocity; (d) Beam density.

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Authors and Affiliations

  1. Electronics & Radio Physics Laboratory, Department of Physics, Banaras Hindu University, Varanasi, India

    S. N. Singh & R. Y. Prasad

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  1. S. N. Singh
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  2. R. Y. Prasad
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Singh, S.N., Prasad, R.Y. Generation and amplification of HM emissions by ion-cyclotron instabilities. Astrophys Space Sci 23, 269–273 (1973). https://doi.org/10.1007/BF00645156

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  • DOI: https://doi.org/10.1007/BF00645156

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