Study of whistler mode instability in Saturn's magnetosphere

dc.contributor.author	Singhal, R.P.
dc.contributor.author	Tripathi, A.K.
dc.date.accessioned	2021-09-15T05:34:25Z
dc.date.available	2021-09-15T05:34:25Z
dc.date.issued	2006
dc.identifier.issn	09927689
dc.identifier.uri	http://localhost:8080/xmlui/handle/123456789/1680
dc.description.abstract	A dispersion relation for parallel propagating whistler mode waves has been applied to the magnetosphere of Saturn and comparisons have been made with the observations made by Voyager and Cassini. The effect of hot (suprathermal) electron-density, temperature, temperature anisotropy, and the spectral index parameter, κ, on the temporal growth rate of the whistler mode emission is studied. A good agreement is found with observations. Electron pitch angle and energy diffusion coefficients have been obtained using the calculated temporal growth rates.	en_US
dc.description.sponsorship	Annales Geophysicae	en_US
dc.language.iso	en	en_US
dc.publisher	Copernicus GmbH	en_US
dc.relation.ispartofseries	Issue 6;Volume 24
dc.subject	anisotropy;	en_US
dc.subject	dispersion;	en_US
dc.subject	electron density;	en_US
dc.subject	growth rate;	en_US
dc.subject	instability;	en_US
dc.subject	magnetosphere;	en_US
dc.subject	Saturn;	en_US
dc.subject	spectrum;	en_US
dc.subject	temperature	en_US
dc.title	Study of whistler mode instability in Saturn's magnetosphere	en_US
dc.type	Article	en_US