Solar coronal rotation and phase of solar activity cycle

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/788

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DC Field	Value	Language
dc.contributor.author	Mehta, M	-
dc.date.accessioned	2006-03-15T05:06:20Z	-
dc.date.available	2006-03-15T05:06:20Z	-
dc.date.issued	2005-09	-
dc.identifier.citation	BASI, Vol. 33, No. 3, pp. 323-325	en
dc.identifier.uri	http://hdl.handle.net/2248/788	-
dc.description.abstract	Solar rotation continues to be observed by several techniques. We have tried to study coronal rotation using radio observations. Coronal rotation and its variation with height in solar atmosphere are studied. For this, we have used 11 different frequencies of radio emissions. We have also tried to look at dependence of rotation period on phase of solar cycle. The period of analysis is four solar cycles (cycle 19 to 22). The results of analysis do not show systematic relationship between coronal rotation period and phase of isolar cycle	en
dc.format.extent	94157 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Sun	en
dc.subject	rotation-Sun	en
dc.subject	radio radiation-Sun	en
dc.title	Solar coronal rotation and phase of solar activity cycle	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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