Flare evolution and polarization changes in fine structures of solar radio emission in the 2013 April 11 event

0461402 - ASÚ 2017 RIV GB eng J - Článek v odborném periodiku
Chernov, G. - Sych, R.A. - Tan, B.-L. - Yan, I.-H. - Tan, C.M. - Fu, Q. - Karlický, Marian - Fomichev, V. V.
Flare evolution and polarization changes in fine structures of solar radio emission in the 2013 April 11 event.
Research in Astronomy and Astrophysics. Roč. 16, č. 2 (2016), 008/1-008/12. ISSN 1674-4527. E-ISSN 2397-6209
Institucionální podpora: RVO:67985815
Klíčová slova: Sun activity * flares * particle emission
Obor OECD: Astronomy (including astrophysics,space science)
Impakt faktor: 1.371, rok: 2016

For the first time, solar radio spectral fine structures (zebra patterns, pulsations and fibers) were observed simultaneously by several radio instruments at four different
observatories: Chinese Solar Broadband Radio Spectrometer at Huairou (SBRS/Huairou), Ondrejov Radio Spectrograph in the Czech Republic (ORSC/Ondrejov), Badary Broadband Microwave Spectropolarimeter
(BMS/Irkutsk), and spectrograph/IZMIRAN (Moscow, Troitsk). It gives exceptional case in determination of the plasma parameters in their radio sources.
Trvalý link: http://hdl.handle.net/11104/0261252