Simulation of generation and transfer of polarized gyrosynchrotron radiation in the solar corona

Details Simulation of generation and transfer of polarized gyrosynchrotron radiation in the solar corona Simulation of generation and transfer of polarized gyrosynchrotron radiation in the solar corona

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..500k&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.500

Physics

Scientific paper

We perform 3D simulations of gyrosynchrotron emission from solar flaring loops. The full polarization transfer equation is solved; the radio brightness maps and spectral dependences of the Stokes parameters of the emission are obtained. We discuss the conditions required to detect the linear polarization of the solar microwave emission by the existing and perspective instruments, as well as the information that could be inferred from such observations. The numerical codes for calculating the radio emission are available online.

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