A new technique to study the variability of the Sun

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/197

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DC Field	Value	Language
dc.contributor.author	Singh, J	-
dc.date.accessioned	2005-01-08T06:29:01Z	-
dc.date.available	2005-01-08T06:29:01Z	-
dc.date.issued	1988	-
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 9, pp. 159-164	en
dc.identifier.issn	0374-3632	-
dc.identifier.uri	http://hdl.handle.net/2248/197	-
dc.description.abstract	A method has been developed to take the high resolution spectra in ionized calcium K line at different latitudes and integrated over visible 180/sup0/ longitude. These spectra have been analysed to study the variability of the line profile as a function of latitude. The spectra are being obtained on regular basis and large data base will be used to study rotation, differential rotation, activity and variability of K-line parameters in various latitudes with the phase of solar cycle.	en
dc.format.extent	196027 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Calcium K line	en
dc.subject	Solar cycle	en
dc.title	A new technique to study the variability of the Sun	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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