The radio brightness of the undisturbed outer solar corona in the presence of a radial magnetic field

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
Appears in Collections:	IIAP Publications

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