Statistics – Computation
Scientific paper
Aug 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985azh....62..768g&link_type=abstract
(Astronomicheskii Zhurnal, vol. 62, July-Aug. 1985, p. 768-775) Soviet Astronomy (ISSN 0038-5301), vol. 29, July-Aug. 1985, p. 4
Statistics
Computation
4
Polarization Characteristics, Solar Atmosphere, Solar Magnetic Field, Solar Radio Emission, Bremsstrahlung, Computational Astrophysics, Integral Equations, Solar Temperature, Spectral Energy Distribution, Temperature Distribution
Scientific paper
A theory of the formation of the polarization of radio bremsstrahlung in an atmosphere with nonuniform distributions of temperature and magnetic field strength is constructed. The possibility of reconstructing the magnetic field distribution from spectral observations of flocculi is evaluated. It is shown that the results of observations of the radio emission of flocculi do not fit into the framework of a plane-layered model chromosphere with a monotonic height distribution of electron temperature, requiring a significant reexamination of the well-known simple estimate of the magnetic field strength in flocculi.
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