Calculations of Coronal Magnetic Field Parallel and Perpendicular to Line-of-Sight in Microwave Bursts

Details Calculations of Coronal Magnetic Field Parallel and Perpendicular to Line-of-Sight in Microwave Bursts Calculations of Coronal Magnetic Field Parallel and Perpendicular to Line-of-Sight in Microwave Bursts

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006soph..237..173h&link_type=abstract

Solar Physics, Volume 237, Issue 1, pp.173-183

Physics

4

Scientific paper

Based on the approximations of the non-thermal gyro-synchrotron radiation used by G.A. Dulk, and K.A. Marsh, Astrophs. J. 259, 350, 1982, the author analyses calculations of the propagation angle and coronal magnetic field self-consistently with brightness temperature, spectral index, frequency, turnover frequency, and polarization degree in solar microwave bursts. Hence, the coronal magnetic fields parallel and perpendicular to the line-of-sight in the sources of microwave bursts are calculated theoretically, and discussed in an event observed by the Nobeyama Radio Polarimeters (NoRP).

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