Measuring magnetic fields in the solar corona by radio emissions

Details Measuring magnetic fields in the solar corona by radio emissions Measuring magnetic fields in the solar corona by radio emissions

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994r%26qe...37..533z&link_type=abstract

Radiophysics and Quantum Electronics, Volume 37, Issue 7, pp.533-542

Physics

Scientific paper

Some ways of identifying magnetic fields in the solar corona using the observed properties of solar radio emissions are discussed. Examples are given for measuring the magnetic field in the active region atmosphere (in the chromosphere-corona transition region) based on spectral observations of microwave radiation from local sources associated with sunspots. Ways of determining the magnetic field in hot coronal loops in the case of recording cyclotron lines in solar microwave radiation are considered. It is shown that polarization of the second harmonic in Type III bursts testifies to a magnetic field on the track of electrons accelerated in the flare region and moving outward.

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