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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/641
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dc.contributor.authorShelke, R. N-
dc.contributor.authorPande, M. C-
dc.date.accessioned2005-12-07T05:47:07Z-
dc.date.available2005-12-07T05:47:07Z-
dc.date.issued1984-12-
dc.identifier.citationBASI, Vol. 12, No. 4, pp. 404-410en
dc.identifier.urihttp://hdl.handle.net/2248/641-
dc.description.abstractAssociation 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 boundaryen
dc.format.extent647355 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectMagnetic regionsen
dc.subjectCoronal holesen
dc.subjectThe Sunen
dc.titleCoronal holes and long-lived unipolar magnetic regionsen
dc.typeArticleen
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