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Publikováno v:
Odessa Astronomical Publications, Vol 26, Iss 2, Pp 243-244 (2013)
Odessa Astronomical Publications; Том 26, № 2 (2013); 243-244
Odessa Astronomical Publications; Том 26, № 2 (2013): Odessa Astronomical Publications; 243-244
Odessa Astronomical Publications; Том 26, № 2 (2013); 243-244
Odessa Astronomical Publications; Том 26, № 2 (2013): Odessa Astronomical Publications; 243-244
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 sourc