Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4162
Title: Observations and interpretation of the slowly varying component of solar radio emission at decameter wavelengths
Authors: Sastry, Ch. V
Dwarakanath, K. S
Shevgaonkar, R. K
Krishan, V
Keywords: Brightness Temperature;Decametric Waves;Radio Astronomy;Solar Radio Emission;Brightness Distribution;Electron Density (Concentration);Electron Energy;Solar Corona;Solar Magnetic Field;Thermal Emission
Issue Date: Oct-1981
Publisher: D. Reidel Publishing Co.
Citation: Solar Physics, Vol. 73, No. 2, pp. 363 - 377
Abstract: We have observed the slowly varying component of solar radio emission at a frequency of 34.5 MHz with half power beam widths of 26/40 in the east-west and north-south directions, respectively. It is found that the observed brightness temperatures vary within the limits of 0.3×106K to 1.5×106K, and the average half power widths of the brightness distribution on the Sun is about 3R . Thermal emission from coronal regions of various electron densities and temperatures with and without the magnetic field has been computed and compared with the observed results.
URI: http://hdl.handle.net/2248/4162
ISSN: 0038-0938
???metadata.dc.relation.uri???: http://dx.doi.org/10.1007/BF00151687
http://adsabs.harvard.edu/abs/1981SoPh...73..363S
Appears in Collections:IIAP Publications

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