Determination of the Coordinates of Radio Sources on the Sun from RATAN-600 Observations in Multiazimuth Mode
Published: 09/2020
(a) Image of the leading part of NOAA 11520 on July 11, 2012, acquired with SDO (AIA/4500 Å). The cross indicates the position of source2 according to the coordinates determined in this study; (b) Radio scans of NOAA 11520 obtained with RATAN-600 at the frequency of f = 12.9 GHz. The solid and dashed lines show the scans obtained in the R and L polarization, respectively.
Astrophysical Bulletin, Volume 75, Issue 3, p.350-359
Opeikina L. V., Abramov-Maximov V. E., Borovik V. N., Chernenkov, V. N.
We provide an analytical description of the method for the determination of the coordinates of solar radio sources from multi-azimuth observations on RATAN-600. We analyze models of the displacement of the object across the scan depending as a function of azimuth taking into account solar rotation and suggest a method for estimating the rate of displacement due to rotation. We demonstrate the results of the application of the method using the determination of the coordinates of a radio source in the active region NOAA 11 520 as example. After eliminating gross scan referencing errors we obtained the coordinates, which agree well with observational data. We discuss the scan coordinate reference errors.
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