dc.contributor.author |
Raju, K. P |
|
dc.contributor.author |
Srikanth, R |
|
dc.contributor.author |
Singh, J |
|
dc.date.accessioned |
2008-09-02T14:35:25Z |
|
dc.date.available |
2008-09-02T14:35:25Z |
|
dc.date.issued |
1998-06 |
|
dc.identifier.citation |
Solar Physics, Vol. 180, No. 1/2, pp. 47 - 51 |
en |
dc.identifier.issn |
0038 - 0938 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/3331 |
|
dc.description |
Restricted Access |
en |
dc.description.abstract |
Calcium K line spectroheliograms obtained during the solar minimum phases at Kodaikanal between 1913–1974 have been used to study the network cell sizes. The autocorrelation is calculated for two-dimensional strips at 5° interval up to ±50° latitude. The average size of the network cells was found to have a dependence on solar latitude with a maximum variation of about 7%. The pattern shows an apparent north–south symmetry with two minima at about 20° N and S. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Springer |
en |
dc.relation.uri |
http://dx.doi.org/10.1023/A:1005072907000 |
en |
dc.subject |
Chromospheric CA II K |
en |
dc.subject |
Solar Latitude |
en |
dc.title |
The Dependence of Chromospheric CA II K Network Cell Sizes on Solar Latitude |
en |
dc.type |
Article |
en |