Onset of Hydrodynamic Non-Equilibrium in Helmet Streamers

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2856

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DC Field	Value	Language
dc.contributor.author	Venkatakrishnan, P	-
dc.date.accessioned	2008-07-23T11:30:24Z	-
dc.date.available	2008-07-23T11:30:24Z	-
dc.date.issued	1996-06	-
dc.identifier.citation	Solar Physics, Vol. 166, No. 1, pp.195 - 200	en
dc.identifier.issn	0038-0938	-
dc.identifier.uri	http://hdl.handle.net/2248/2856	-
dc.description.abstract	The steady-state solar wind solution is examined for different geometries of the flow tube that mimics a helmet streamer. Onset of non-equilibrium is seen whenever the spatial variation of the flow geometry crosses critical values. It is suggested that the dynamical response of the flow to the onset of non-equilibrium can manifest as a coronal mass ejection.	en
dc.format.extent	537532 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Kluwer Academic Publishers	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1996SoPh..166..195V	en
dc.subject	Helmet streamers	en
dc.subject	Geometries	en
dc.subject	Solar wind solution	en
dc.title	Onset of Hydrodynamic Non-Equilibrium in Helmet Streamers	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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