Generation and Amplification of HM Emissions by Ion-Cyclotron Instabilities

Details Generation and Amplification of HM Emissions by Ion-Cyclotron Instabilities Generation and Amplification of HM Emissions by Ion-Cyclotron Instabilities

Aug 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973ap%26ss..23..269s&link_type=abstract

Astrophysics and Space Science, Volume 23, Issue 2, pp.269-273

Astronomy and Astrophysics

Astrophysics

Scientific paper

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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