Low Frequency Radio Emission from the 'Quiet Sun'

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