dc.contributor.author |
Shanmugaraju, A |
|
dc.contributor.author |
Umapathy, S |
|
dc.date.accessioned |
2005-01-28T06:11:39Z |
|
dc.date.available |
2005-01-28T06:11:39Z |
|
dc.date.issued |
1997 |
|
dc.identifier.citation |
Kodaikanal Observatory Bulletins Series A, Vol. 13, pp. 147-149 |
en |
dc.identifier.issn |
0374-3632 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/253 |
|
dc.description.abstract |
A solar radio spectrograph has been developed to observe the transient solar radio emissions in the band of 30 MHz at our School of Physics. A non trackable log periodic antenna having beam of 60 degree in E-W and 90 degree in N-S is being used. The recent solar eclipse of October 24, 1995 was observed with maximum obstruction of sun's disc by moon to the tune of 40% using the above radio spectrograph. The initial results have been reported in this paper. |
en |
dc.format.extent |
65574 bytes |
|
dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en |
|
dc.publisher |
Indian Institute of Astrophysics, Banglaore |
en |
dc.subject |
Solar eclipse |
en |
dc.subject |
Radio spectrograph |
en |
dc.title |
Radio spectrograph observations of the recent soalr eclipse on October 24, 1995 |
en |
dc.type |
Article |
en |