Association of coronal holes with large scale solar magnetic fields

dc.contributor.author	Shelke, R. N.
dc.contributor.author	Pande, M. C.
dc.date.accessioned	2010-03-10T05:29:44Z
dc.date.available	2010-03-10T05:29:44Z
dc.date.issued	1984
dc.identifier.citation	This article is downloaded for ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/625
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 magnetic 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 encroaches 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_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	basi12-357
dc.subject	Coronal holes	en_US
dc.title	Association of coronal holes with large scale solar magnetic fields	en_US
dc.type	Article	en_US