Coronal holes and long-lived unipolar magnetic regions

dc.contributor.author	Shelke, R. N.
dc.contributor.author	Pande, M. C.
dc.date.accessioned	2010-03-09T06:59:50Z
dc.date.available	2010-03-09T06:59:50Z
dc.date.issued	1984
dc.identifier.citation	This article is downloaded for ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/623
dc.description.abstract	Association of coronal holes with long-lived unipolar magnetic regions (LLUMRs) which survived for four solar rotations is examined. It is noticed that every coronal hole fits in well within the LLUMR. The coronal holes are also seen to dissolve as a consequence of the LLUMR boundary zone evolution and emergence of opposite polarity regions with in coronal hole boundary.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	basi12-404
dc.subject	Magnetic regions, Coronal holes - The Sun	en_US
dc.title	Coronal holes and long-lived unipolar magnetic regions	en_US
dc.type	Article	en_US