Coronal Magnetic Field Measurements Through Bremsstrahlung Emission

Details Coronal Magnetic Field Measurements Through Bremsstrahlung Emission Coronal Magnetic Field Measurements Through Bremsstrahlung Emission

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004assl..314..115g&link_type=abstract

Solar and Space Weather Radiophysics, Astrophysics and Space Science Library, Volume 314. ISBN 978-1-4020-2813-7. Springer Scien

Astronomy and Astrophysics

Astrophysics

3

Scientific paper

Basic concepts are presented of the theory of thermal bremsstrahlung in the anisotropic plasma of the solar atmosphere. Formulas are given describing the polarization resulting from the solar magnetic field, from which the longitudinal component of the magnetic field can be found through analysis of the polarization spectra of the thermal radio emission. The application of the method is illustrated with examples pertaining to solar faculae, prominences, coronal holes and coronal loops. The observations were carried with large, modern radio telescopes such as the Nobeyama Radioheliograph (Japan) and the RATAN-600 (Russia).

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