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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2660
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dc.contributor.authorGolap, K-
dc.contributor.authorSastry, Ch. V-
dc.date.accessioned2008-07-14T06:12:37Z-
dc.date.available2008-07-14T06:12:37Z-
dc.date.issued1994-03-
dc.identifier.citationSolar Physics, Vol. 150, No. 1-2, pp. 295 - 304en
dc.identifier.issn0038-0938-
dc.identifier.urihttp://hdl.handle.net/2248/2660-
dc.description.abstractThe 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.extent689039 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherSpringeren
dc.relation.urihttp://www.springerlink.com/content/9j408544t4v5l14x/en
dc.relation.urihttp://adsabs.harvard.edu/abs/1994SoPh..150..295Gen
dc.subjectBrightnessen
dc.subjectBrightness Distributionen
dc.subjectBrightness Temperatureen
dc.subjectCoronal Holesen
dc.subjectMagnetic Field Configurationsen
dc.subjectMagnetic Fluxen
dc.subjectRadio Astronomyen
dc.subjectSolar Coronaen
dc.subjectSolar Limben
dc.subjectSolar Magnetic Fielden
dc.subjectSolar Radio Emissionen
dc.subjectAbsorptivityen
dc.subjectCircular Polarizationen
dc.subjectDensity Distributionen
dc.subjectElectron Density (Concentration)en
dc.subjectOptical Thicknessen
dc.subjectRadio Burstsen
dc.subjectRefractivityen
dc.subjectRunge-Kutta Methoden
dc.titleThe radio brightness of the undisturbed outer solar corona in the presence of a radial magnetic fielden
dc.typeArticleen
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