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Hans Publishers, Astronomy & Astrophysics, (575), p. A47

DOI: 10.1051/0004-6361/201424548

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Perturbations of gyrosynchrotron emission polarization from solar flares by sausage modes: Forward modeling

Journal article published in 2015 by V. E. Reznikova, T. Van Doorsselaere ORCID, A. A. Kuznetsov ORCID
This paper is made freely available by the publisher.
This paper is made freely available by the publisher.

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Abstract

We examined the polarization of the microwave flaring emission and its modulation by the fast sausage standing wave using a linear 3D magnetohydrodynamic model of a plasma cylinder. We analized the effects of the line-of-sight angle on the perturbations of the gyrosynchrotron intensity for two models: a base model with strong Razin suppression and a low-density model in which the Razin effect was negligible. The circular polarization (Stokes V) oscillation is in phase with the intensity oscillation, and the polarization degree (Stokes V/I) oscillates in phase with the magnetic field at the examined frequencies in both models. The two quantities experience a periodical reversal of their signs with period equal to a half of the sausage wave period when seen at a 90 • viewing angle, in this case, their modulation depth reaches 100%.