dc.contributor.author |
Ramesh, R |
|
dc.contributor.author |
Subramanian, K. R |
|
dc.contributor.author |
Sastry, Ch. V |
|
dc.date.accessioned |
2005-01-28T06:01:58Z |
|
dc.date.available |
2005-01-28T06:01:58Z |
|
dc.date.issued |
1997 |
|
dc.identifier.citation |
Kodaikanal Observatory Bulletins Series A, Vol. 13, pp. 143-145 |
en |
dc.identifier.issn |
0374-3632 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/252 |
|
dc.description.abstract |
We have observed radio emission from the solar corona at a frequency of 77 MHz during the total solar eclipse on October 24, 1995 from our observatory at Gauribidanur. Sources of angular sizes less than or equal to 1.5' have been found to exist at height 0.4Ro above the photosphere. |
en |
dc.format.extent |
64178 bytes |
|
dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en |
|
dc.publisher |
Indian Institute of Astrophysics, Bangalore |
en |
dc.subject |
Solar eclipse |
en |
dc.subject |
Radio emission |
en |
dc.subject |
Scattering |
en |
dc.title |
Radio Observations of Compact Sources in the Outer Solar Corona |
en |
dc.type |
Article |
en |