Radio emission from coronal streamers

Details Radio emission from coronal streamers Radio emission from coronal streamers

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ssrv...70..279d&link_type=abstract

Space Science Reviews, Volume 70, Issue 1-2, pp. 279-282

Computer Science

Sun: Corona, Sun: Radio Emission, Sun: Streamer

Scientific paper

Different models of coronal streamers are used to calculate the radio brightness temperature at the wavelengths of observation of the Nançays Radioheliograph. Calculation are performed assuming the location of the streamer both on the disk and at the limb. Their comparison with observations show that a satisfactory agreement with a particular model can be found in the shape and in the relative enhacement of the streamer with respect to the quiet Sun, although the absolute values of the computed brightness temperatures are much higher than the observed ones.

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