Peculiarities of the development of active regions on the Sun prior to strong X-class flares: Joint analysis of data from the RATAN-600 radio telescope and SDO space observatory

Author:

Abramov-Maximov V. E.,Borovik V. N.,Opeikina L. V.,Tlatov A. G.

Publisher

Pleiades Publishing Ltd

Subject

Space and Planetary Science,Astronomy and Astrophysics,Aerospace Engineering

Reference27 articles.

1. Akhmedov, Sh.B., Bogod, V.M., Borovik, V.N., et al., The structure of active regions on the Sun as observed by VLA and RATAN-600 in July 1982, Astrofiz. Issled. (Izv. SAO), 1987, vol. 25, p. 105.

2. Bogod, V.M., Alesin, A.M., and Pervakov, A.A., RATAN-600 radio telescope in the 24th solar-activity cycle. II. Multi-octave spectral and polarization high-resolution solar research system, Astrophys. Bull., 2011, vol. 66, no. 2, pp. 205–214.

3. Bogod, V.M., Kal’tman, T.I., and Yasnov, L.V., On properties of microwave sources above the magnetic field neutral line, Astrofiz. Byull., 2012, vol. 67, no. 4, p. 441.

4. Borisevich, T.P., Il’in, G.N., Peterova, N.G., et al., The Tanaka-Enome criterion and solar activity in October–November 2003 as observed by the Large Pulkovo Radio Telescope, Kosm. Issled., vol. 42, no. 6, pp. 585–594. [Cosmic Research, pp. 561–570].

5. Borovik, V.N., Vatrushin, S.M., and Korzhavin, A.N., Radio characteristics of the active region associated with the proton flare on April 24, 1985 according to RATAN-600 observations, Astrofiz. Issled. (Izv. SAO), 1987, vol. 28, p. 123.

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