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

Golap, K; Sastry, Ch. V

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dc.contributor.author	Golap, K
dc.contributor.author	Sastry, Ch. V
dc.date.accessioned	2008-07-14T06:12:37Z
dc.date.available	2008-07-14T06:12:37Z
dc.date.issued	1994-03
dc.identifier.citation	Solar Physics, Vol. 150, No. 1-2, pp. 295 - 304	en
dc.identifier.issn	0038-0938
dc.identifier.uri	http://hdl.handle.net/2248/2660
dc.description.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.	en
dc.format.extent	689039 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Springer	en
dc.relation.uri	http://www.springerlink.com/content/9j408544t4v5l14x/	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1994SoPh..150..295G	en
dc.subject	Brightness	en
dc.subject	Brightness Distribution	en
dc.subject	Brightness Temperature	en
dc.subject	Coronal Holes	en
dc.subject	Magnetic Field Configurations	en
dc.subject	Magnetic Flux	en
dc.subject	Radio Astronomy	en
dc.subject	Solar Corona	en
dc.subject	Solar Limb	en
dc.subject	Solar Magnetic Field	en
dc.subject	Solar Radio Emission	en
dc.subject	Absorptivity	en
dc.subject	Circular Polarization	en
dc.subject	Density Distribution	en
dc.subject	Electron Density (Concentration)	en
dc.subject	Optical Thickness	en
dc.subject	Radio Bursts	en
dc.subject	Refractivity	en
dc.subject	Runge-Kutta Method	en
dc.title	The radio brightness of the undisturbed outer solar corona in the presence of a radial magnetic field	en
dc.type	Article	en