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 |
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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 |