Low frequency radio emission from the &#x2018;quiet&#x2019; Sun
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We present observations of the &#x2018;quiet&#x2019; 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.
Key wordsSun corona radio observations streamers scattering
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- Ramesh, R. 1999,Ph.D. thesis, Bangalore University.Google Scholar