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Published in 2018 at "Solar Physics"
DOI: 10.1007/s11207-017-1228-7
Abstract: Models of the upper transition region of sunspots have been derived based on the observed radio spectrum between 3 and 18 GHz from Radio Astronomical Telescope of the Academy of Sciences 600 (RATAN-600) observations. Our objective…
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Keywords:
observations modeling;
transition region;
ratan 600;