OBSERVATION ON THE RADIO TELESCOPE URAN-4 OF RADIO SOURCES, CONNECTED WITH THE CORONAL MASS EJECTION ON THE SUN

Автор(и)

  • V. V. Galanin Institute of Radio Astronomy of National Academy of Science of Ukraine, Україна
  • V. G. Derevjagin Institute of Radio Astronomy of National Academy of Science of Ukraine, Україна
  • R. O. Kravetz Institute of Radio Astronomy of National Academy of Science of Ukraine, Україна

DOI:

https://doi.org/10.18524/1810-4215.2013.26.83757

Ключові слова:

radio source, solar corona

Анотація

In 2012 and 2013 the observations of radio sources covering by the solar corona was conducted on the radio telescope URAN-4. Inobtained data there was fixed the records of the strong radio sources, which had flow level comparable with the 3c461 source. As a result of information analysis from miscellaneous observatories about the solar activity conditions there is done the conclusion that they are connected with the coronal mass ejections which was took place that time.

 

Посилання

Galanin V.V. et al.: 1989, Kinematics and Physics of celestial bodies, 5, 5, 87.

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Опубліковано

2013-11-18

Номер

Том 26 № 2 (2013)

Розділ

Статті

Ліцензія

Авторське право (c) 2016 Odessa Astronomical Publications

Creative Commons License

Ця робота ліцензується відповідно до Creative Commons Attribution-NonCommercial 4.0 International License.

Відповідно Закону України про авторське право і суміжні права N 3792-XII від 23 грудня 1993 року