Physics
Scientific paper
Mar 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993soph..144..199b&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 144, no. 1, p. 199-202.
Physics
4
Brightness Temperature, Microwave Emission, Solar Atmosphere, Solar Physics, Solar Prominences, Solar Radio Emission, Chromosphere, Microwave Absorption, Solar Corona
Scientific paper
The physical conditions causing the appearance of the low brightness temperature regions at 37 and 22 GHz are discussed. The source radiation stems from free-free processes (bremsstrahlung), and passes through the transparent chromosphere and corona. The absorption occurs either in the prominences or in coronal condensations with physical parameters between those of prominences and corona. A deficit in emission of the chromosphere-corona transition region in the vicinity of the inversion lines of the longitudinal component of the photospheric magnetic field could also result in the appearance of low temperature region.
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