dc.contributor.author |
Ramesh, R |
|
dc.date.accessioned |
2008-08-12T08:55:01Z |
|
dc.date.available |
2008-08-12T08:55:01Z |
|
dc.date.issued |
2000-12 |
|
dc.identifier.citation |
Journal of Astrophysics and Astronomy, Vol. 21, No. 3 – 4, pp. 237 - 240 |
en |
dc.identifier.issn |
0250-6335 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/3070 |
|
dc.description.abstract |
We present observations of the 'quiet' Sun close to the recent
solar minimum (Cycle 22), with the Gauribidanur radioheliograph. Our
main conclusion is that coronal streamers also influence the observed
radio brightness temperature. |
en |
dc.format.extent |
333230 bytes |
|
dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en |
en |
dc.publisher |
Indian Academy of Sciences |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/2000JApA...21..237R |
en |
dc.subject |
Sun |
en |
dc.subject |
Corona |
en |
dc.subject |
Radio Observations |
en |
dc.subject |
Streamers |
en |
dc.subject |
Scattering |
en |
dc.title |
Low Frequency Radio Emission from the 'Quiet Sun' |
en |
dc.type |
Article |
en |