dc.contributor.author |
Singh, G. N |
|
dc.contributor.author |
Shrivastava, P. K |
|
dc.date.accessioned |
2008-07-17T10:23:57Z |
|
dc.date.available |
2008-07-17T10:23:57Z |
|
dc.date.issued |
2002-09 |
|
dc.identifier.citation |
BASI, Vol. 30, No. 3, pp. 599 - 600 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/2728 |
|
dc.description.abstract |
High speed solar· wind streams are separated into two categories : (i)
Corotating (ii) Flare-generated streams. Resul ts based on this analysis
indicate the occurrence of large geomagnetic and interplanetary disturbances
during flare-generated streams in comparison to period of corotating
streams. |
en |
dc.format.extent |
56595 bytes |
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dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of India |
en |
dc.subject |
Solar Wind |
en |
dc.subject |
Geomagnetic Activity |
en |
dc.subject |
Interplanetary Disturbances |
en |
dc.title |
Effect of solar wind streams on interplanetary features and on geomagnetic field |
en |
dc.type |
Article |
en |