Association of Coronal holes with large scale Solar Magnetic fields

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/636

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DC Field	Value	Language
dc.contributor.author	Shelke, R. N	-
dc.contributor.author	Pande, M. C	-
dc.date.accessioned	2005-12-07T05:04:46Z	-
dc.date.available	2005-12-07T05:04:46Z	-
dc.date.issued	1984-12	-
dc.identifier.citation	BASI, Vol. 12, No. 4, pp. 357-363	en
dc.identifier.uri	http://hdl.handle.net/2248/636	-
dc.description.abstract	Association of coronal holes with large scale solar magnetic fields has been investigated. It is concluded that coronal holes always form in the large unipolar megnetic field patterns, and no specific polarity rule holds true for low-latitude coronal holes. The coronal holes show a strong tendency to bypass the opposite polarity regions in their location. Coronal holes get fragmented into pieces, if opposite polarity flux enroaches and/or erupts into their boundaries. Migration of coronal holes or their fragments and the growth of coronal holes out of hole fragments are also discussed.	en
dc.format.extent	632971 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Astronomical Society of India	en
dc.subject	Coronal hole	en
dc.subject	Solar magnetic fields	en
dc.title	Association of Coronal holes with large scale Solar Magnetic fields	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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