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