dc.contributor.author |
Venkatakrishnan, P |
|
dc.date.accessioned |
2009-01-28T12:38:40Z |
|
dc.date.available |
2009-01-28T12:38:40Z |
|
dc.date.issued |
1994 |
|
dc.identifier.citation |
K. S. Balasubramaniam and George W. Simon., eds., Solar active region evolution: comparing models with observations. Astronomical Society of the Pacific Conference Series, Vol. 68, Proceedings of the 14th International Summer Workshop, National Solar Observatory / Sacramento Peak, Sunspot, New Mexico, USA, 30 August - 3 September 1993, pp. 409 - 410 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/4291 |
|
dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of the Pacific |
en |
dc.relation.ispartofseries |
Astronomical Society of the Pacific Conference Series, Vol. 68 |
|
dc.relation.uri |
http://adsabs.harvard.edu/abs/1994ASPC...68..409V |
en |
dc.subject |
Coronal Magnetic Structures |
en |
dc.subject |
Quasi-Static |
en |
dc.title |
Can coronal magnetic structures be quasi-static? |
en |
dc.type |
Article |
en |