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The solar corona is extremely dynamic. Every leap in observational capabilities has been accompanied by unexpected revelations of complex dynamic processes. The ever more sensitive instruments now allow us to probe events with increasingly weaker ene
Externí odkaz:
http://arxiv.org/abs/2306.15104
Publikováno v:
Astronomical Data Analysis Software and Systems XXX, 532, 211 (2022)
The perplexing mystery of what maintains the solar coronal temperature at about a million K, while the visible disc of the Sun is only at 5800 K, has been a long standing problem in solar physics. A recent study by Mondal(2020) has provided the first
Externí odkaz:
http://arxiv.org/abs/2103.05371
Publikováno v:
ASP Conference Series; 2022, Vol. 532, p211-214, 4p