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Published in 2021 at "Astronomy and Astrophysics"
DOI: 10.1051/0004-6361/202040254
Abstract: In solar physics, a severe numerical challenge for modern simulations is properly representing a transition region between the million-degree hot corona and a much cooler plasma of about 10000 K (e.g., the upper chromosphere or…
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Keywords:
transition region;
transition;
mhd;
adaptive conduction ... See more keywords