Abstract
We examined records of the radiation of three flare processes obtained in the Nobeyama observatory in 1992, 2001, and 2003. Observations with the Nobeyama radio heliograph at the frequencies 17 and 34GHz were performed with a sufficient spatial resolution to determine the physical nature of the radiation source. In the first two cases, the radiation source appeared to be a coronal magnetic loop; in the third case, a group of sunspots. In the spectra of the first two events a characteristic modulation was detected, with the frequency that increased by a factor of 2–3 for a fairly short period immediately before the beginning of the flare and later decreased gradually to the initial value. In the spectrum of the event on June 17, 2003 (the radiation source were the sunspots), no modulation of such a type was seen.
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Acknowledgements
This work was partially supported by the Russian Foundation for Basic Research (project Nos. 10–02–00265-a, 08–02–00119-a, and 09–02–00226-a), as well as by the contract KD NK-21P with the Federal Agency of Education of the Russian Federation and the project No. 228319 of the European Union within the framework of the project “EuroPlanet”-RI FP7.
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Zaitsev, V.V., Kislyakova, K.G., Altyntsev, A.T., Meshalkina, N.S. (2012). Dynamics of the Electrical Currents in Coronal Magnetic Loops. In: Obridko, V., Georgieva, K., Nagovitsyn, Y. (eds) The Sun: New Challenges. Astrophysics and Space Science Proceedings, vol 30. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-29417-4_5
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