Can coronal magnetic structures be quasi-static?

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4291

Full metadata record

DC Field	Value	Language
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
Appears in Collections:	IIAP Publications

Files in This Item:

File	Description	Size	Format
Can coronal magnetic structures be quasi-static?		175.36 kB	Adobe PDF	View/Open

DSpace JSPUI