Solar limb brightening at millimeter wavelengths

Details Solar limb brightening at millimeter wavelengths Solar limb brightening at millimeter wavelengths

Dec 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974soph...39..315k&link_type=abstract

Solar Physics, vol. 39, Dec. 1974, p. 315-322.

Physics

6

Brightness Temperature, Millimeter Waves, Solar Limb, Solar Radio Emission, Spicules, Astronomical Models, Microwave Emission, Ray Tracing, Statistical Analysis

Scientific paper

The radio brightness distribution wavelengths of 9, 3.5, and 1.2 mm is calculated employing a statistical technique to account for the presence of spicules randomly occurring along the ray path. The results indicate limb brightening at each wavelength when the Avery and House (1969) spicule model is employed. This contradicts the results of Lantos and Kundu (1972), whose method of computation is shown to be inadequate.

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