Coronal holes and long-lived unipolar magnetic regions

dc.contributor.author	Shelke, R. N
dc.contributor.author	Pande, M. C
dc.date.accessioned	2005-12-07T05:47:07Z
dc.date.available	2005-12-07T05:47:07Z
dc.date.issued	1984-12
dc.identifier.citation	BASI, Vol. 12, No. 4, pp. 404-410	en
dc.identifier.uri	http://hdl.handle.net/2248/641
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 within the coronal hole boundary	en
dc.format.extent	647355 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Astronomical Society of India	en
dc.subject	Magnetic regions	en
dc.subject	Coronal holes	en
dc.subject	The Sun	en
dc.title	Coronal holes and long-lived unipolar magnetic regions	en
dc.type	Article	en