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 |
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dc.format.mimetype |
application/pdf |
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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 |