Cyclotron Line in Solar Microwave Radiation by Radio Telescope RATAN-600 Observations of the Solar Active Region NOAA 12182


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This paper presents the results of observation of a rare phenomenon—a narrowband increase in the brightness of cyclotron radiation of one of the structural details of a radio source located in the solar corona above the solar active region NOAA 12182 in October 2014 at a frequency of 4.2 ± 0.1 GHz. The brightness of radiation in the maximum of the phenomenon has reached 10 MK; its duration was equal to 3 s. The exact location of the source of the narrowband cyclotron radiation is indicated: it is a corona above a fragmented (4-nuclear) sunspot, on which a small UV flare loop was closed.

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N. Peterova

St. Petersburg Branch of Special Astrophysical Observatory

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Email: peterova@yandex.ru
俄罗斯联邦, St. Petersburg, 196140

N. Topchilo

St. Petersburg State University

Email: peterova@yandex.ru
俄罗斯联邦, St. Petersburg

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