The bright points in the Ca II K-line and their relation to the inner network magnetic structures

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4776

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DC Field	Value	Language
dc.contributor.author	Sivaraman, K. R	-
dc.date.accessioned	2009-08-28T14:59:33Z	-
dc.date.available	2009-08-28T14:59:33Z	-
dc.date.issued	1991	-
dc.identifier.citation	Ulmschneider, P., Priest, E. R and Rosner, R. eds., Mechanisms of chromospheric and coronal heating: Proceedings of the International Conference, Heidelberg, 5 - 8 June, 1990., pp. 44 - 47	en
dc.identifier.isbn	0-540-53436-9	-
dc.identifier.uri	http://hdl.handle.net/2248/4776	-
dc.description.abstract	We present observational evidence to show that the K/sub2v points bear a one to one correspondence with the inner network magnetic elements when the quiet sun is viewed under good spatial resolution. This would have implications on the theories of chromospheric heating over quiet regions on the sun.	-
dc.language.iso	en	en
dc.publisher	Springer-Verlag	en
dc.subject	Ca II K-Line	en
dc.subject	Network Magnetic Structures	en
dc.title	The bright points in the Ca II K-line and their relation to the inner network magnetic structures	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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