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

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

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994soph..150..295g&link_type=abstract

Solar Physics, vol. 150, no. 1-2, p. 295-304

Astronomy and Astrophysics

Astronomy

1

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

Scientific paper

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.

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