Abstract
We studied a number of solar active regions using two-dimensional spatially resolved microwave observations. Data from the Nobeyama Radioheliograph and the Siberian Solar Radio Telescope together with observations by the Michelson Doppler Imager (MDI) onboard the Solar and Heliospheric Observatory (SOHO) have allowed us to identify long-lived intersunspot sources (ISSs) in most of the investigated active regions. Their centers are often located above the line-of-sight magnetic field inversion line that separates the leading and following polarities of a full active region (first type of ISS) or above the inversion line that separates magnetic polarities inside of a complex of sunspots (second type of ISS). ISSs of the first type are extended and, in general, they are sources of bremsstrahlung emission. ISSs of the second type are compact and are, most likely, sources of gyroresonance or gyrosynchrotron emission. We propose a qualitative model involving three types of magnetic connectivity to explain how long-lasting ISSs may be generated.
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Acknowledgements
This work was partly supported by the Russian Foundation for Basic Research (projects No. 13-02-00656, 13-02-00586, 13-02-00714, and 14-02-00924), the Presidium of Russian Academy of Sciences (program No. 22) and by the European Commission Exchange Program MC FP7-PEOPLE-2011-IRSES-295272 RADIOSUN. We are grateful to the SOHO team, TRACE team and NoRH team for allowing us to use the data. The RATAN-600 observations were carried out with the financial support of the Ministry of Education and Science of the Russian Federation (state contract 14.518.11.7054). We would also like to thank the anonymous referee for useful comments.
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New Eyes Looking at Solar Activity: Challenges for Theory and Simulations
Guest Editors: Silja Pohjolainen and Marian Karlický
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Bakunina, I.A., Melnikov, V.F., Solov’ev, A.A. et al. Intersunspot Microwave Sources. Sol Phys 290, 37–52 (2015). https://doi.org/10.1007/s11207-014-0614-7
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DOI: https://doi.org/10.1007/s11207-014-0614-7