dc.contributor.author |
Raju, P. K |
|
dc.date.accessioned |
2005-01-08T05:37:01Z |
|
dc.date.available |
2005-01-08T05:37:01Z |
|
dc.date.issued |
1988 |
|
dc.identifier.citation |
Kodaikanal Observatory Bulletins Series A, Vol. 9, pp. 89-98 |
en |
dc.identifier.issn |
0374-3632 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/189 |
|
dc.description.abstract |
In this article the methods to probe the solar corona are briefly described. The discussion is confined to continuum and the "optical" wavelength region ~ 0.3 mum to 1.1 mum. |
en |
dc.format.extent |
272829 bytes |
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dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en |
|
dc.publisher |
Indian Institute of Astrophysics, Bangalore |
en |
dc.subject |
Solar corona |
en |
dc.subject |
Optical emission |
en |
dc.title |
Optical emission from solar corona |
en |
dc.type |
Article |
en |