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Analysis of polarized microwave emission of Flare-Productive Active Region 9415

V. M. Bogod·G. B. Gelfreikh·F. Ch. Drago·V. P. Maximov·A. Nindos·T. I. Kaltman·B. I. Ryabov·S. Kh. Tokhchukova
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Abstract

The results of the microwave observations of the Sun made with the RATAN-600 have shown the existence of many types of spectral peculiarities in polarized emission of active regions, which produce powerful flares. These phenomena happen at microwaves and reflect inhomogeneous structure of magnetic field in magnetospheres of flaring active regions in wide range of heights above the photosphere. In this presentation we demonstrate an analysis of the AR 9415 during all the period of its passage across the solar disk. Results of the study point out to existence of different scenarios of circular polarization variations in the radio wave band. Here, we separated the phenomenon of the cyclotron emission passage through the quasi-transverse magnetic field (QT-region) and several effects connected with flare activity of active region. New observational data are presented and compared with the data of several observatories: SSRT, NoRH, MDI SOHO, GOES and MEES. The preliminary interpretation of the phenomena are given.

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V. M. Bogod, G. B. Gelfreikh, F. Ch. Drago, V. P. Maximov, A. Nindos, T. I. Kaltman, B. I. Ryabov, S. Kh. Tokhchukova. 2003-09-16. Analysis of polarized microwave emission of Flare-Productive Active Region 9415. https://arxiv.org/abs/astro-ph/0309444

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