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1
Published in 2018 at "Nature Astronomy"
DOI: 10.1038/s41550-018-0590-1
Abstract: The Sun’s active corona requires an energy flux of ~103 W m−2 to compensate for radiative losses and to maintain its high temperature1. Plasma moves in the corona through magnetic loops2,3, which may be connected with the…
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Keywords:
pseudo shocks;
energy;
confined pseudo;
corona ... See more keywords