Effect of pressure pulse on geomagnetic field oscillations

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DC Field	Value	Language
dc.contributor.author	Sinha, Ashwini K.
dc.contributor.author	Rajaram, R.
dc.date.accessioned	2015-09-08T07:01:55Z
dc.date.accessioned	2021-02-12T09:29:11Z	-
dc.date.available	2015-09-08T07:01:55Z
dc.date.available	2021-02-12T09:29:11Z	-
dc.date.issued	2006
dc.identifier.citation	ILWS Workshop 2006, Goa, 2006	en_US
dc.identifier.uri	http://localhost:8080/xmlui/handle/123456789/353	-
dc.description.abstract	The effect of solar wind pressure pulse on geomagnetic field oscillations has been computed by using Green’s function technique. The dominance of toroidal oscillations during dawn/dusk sectors appears to be natural consequences of solar wind pressure pulse and may not be attributed to K-H instability at the magnetopause boundary caused by velocity shear. Pressure pulse generates surface waves at the magnetopause boundary and couples to the field oscillations to give rise such effects. The paper adopts the 3-dimensional approach to explain the phenomena.	en_US
dc.language.iso	en	en_US
dc.subject	Field line response	en_US
dc.subject	Geomagnetic pulsations	en_US
dc.subject	Solar wind impulse	en_US
dc.subject	Standing waves	en_US
dc.subject	Geomagnetic field	en_US
dc.title	Effect of pressure pulse on geomagnetic field oscillations	en_US
dc.type	Article	en_US
dc.identifier.accession	090846
Appears in Collections:	UAS_Reprints

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