dc.contributor.author |
Bagchi, J |
|
dc.contributor.author |
Subramanian, K. R |
|
dc.contributor.author |
Ebenezer, E |
|
dc.contributor.author |
Gowda, N |
|
dc.contributor.author |
Abdul Hameed, A. T |
|
dc.date.accessioned |
2005-01-28T05:32:16Z |
|
dc.date.available |
2005-01-28T05:32:16Z |
|
dc.date.issued |
1997 |
|
dc.identifier.citation |
Kodaikanal Observatory Bulletins Series A, Vol. 13, pp. 133-141 |
en |
dc.identifier.issn |
0374-3632 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/251 |
|
dc.description.abstract |
The interpretation of the lunar occultation data recorded at the microwave frequencies of 2025, 3.80 and 4.20 GHz from two stations during the October 24, 1995 solar eclipse in India is presented. |
en |
dc.format.extent |
629401 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 eclipse |
en |
dc.subject |
Lunar occultation |
en |
dc.subject |
Microwave emission |
en |
dc.subject |
Active regions |
en |
dc.subject |
X-ray emission |
en |
dc.title |
Lunar Occultation Observations of the Microwave Sun During the Eclipse of October 24, 1995 |
en |
dc.type |
Article |
en |