Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2660
Title: The radio brightness of the undisturbed outer solar corona in the presence of a radial magnetic field
Authors: Golap, K
Sastry, Ch. V
Keywords: Brightness;Brightness Distribution;Brightness Temperature;Coronal Holes;Magnetic Field Configurations;Magnetic Flux;Radio Astronomy;Solar Corona;Solar Limb;Solar Magnetic Field;Solar Radio Emission;Absorptivity;Circular Polarization;Density Distribution;Electron Density (Concentration);Optical Thickness;Radio Bursts;Refractivity;Runge-Kutta Method
Issue Date: Mar-1994
Publisher: Springer
Citation: Solar Physics, Vol. 150, No. 1-2, pp. 295 - 304
Abstract: The radio brightness of the quiet outer solar corona at a frequency of 35 MHz in the presence of a radial magnetic field is computed. It is found that the brightness temperature of the ordinary radiation increases significantly. It is also found that in the presence of a radial magnetic field, coronal holes will appear as bright emission regions on the disk and as depressions at the limb.
URI: http://hdl.handle.net/2248/2660
ISSN: 0038-0938
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http://adsabs.harvard.edu/abs/1994SoPh..150..295G
Appears in Collections:IIAP Publications

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