Non-linear high-frequency waves in the magnetosphere

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DC Field	Value	Language
dc.contributor.author	Moolla, S.
dc.contributor.author	Bharuthram, R.
dc.contributor.author	Singh, S.V.
dc.contributor.author	Lakhina, G.S.
dc.date.accessioned	2015-08-25T08:53:28Z
dc.date.accessioned	2021-02-12T10:11:11Z	-
dc.date.available	2015-08-25T08:53:28Z
dc.date.available	2021-02-12T10:11:11Z	-
dc.date.issued	2003
dc.identifier.citation	Pramana-Journal of Physics, v.61/6, p.1209-1214, 2003, doi: 10.1007/BF02704418	en_US
dc.identifier.uri	http://localhost:8080/xmlui/handle/123456789/278	-
dc.description.abstract	Using fluid theory, a set of equations is derived for non-linear high-frequency waves propagating oblique to an external magnetic field in a three-component plasma consisting of hot electrons, cold electrons and cold ions. For parameters typical of the Earth’s magnetosphere, numerical solutions of the governing equations yield sinusoidal, sawtooth or bipolar wave-forms for the electric field.	en_US
dc.language.iso	en	en_US
dc.subject	Magnetosphere	en_US
dc.subject	Bipolar	en_US
dc.subject	Sawtooth wave-forms	en_US
dc.subject	Electric fields	en_US
dc.subject	Non-linear high-frequency waves	en_US
dc.title	Non-linear high-frequency waves in the magnetosphere	en_US
dc.type	Article	en_US
dc.identifier.accession	090767
Appears in Collections:	UAS_Reprints

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