no code implementations • 10 Mar 2021 • G. Del Zanna, V. Andretta, P. J. Cargill, A. J. Corso, A. N. Daw, L. Golub, J. A. Klimchuk, H. E. Mason
We discuss the diagnostics available to study the 5-10 MK plasma in the solar corona, which is key to understanding the heating in the cores of solar active regions.
Solar and Stellar Astrophysics
