no code implementations • 24 Feb 2021 • Julia M. Riedl, Caitlin A. Gilchrist-Millar, Tom Van Doorsselaere, David B. Jess, Samuel D. T. Grant
While the analysis of the energy flux for ideal and non-ideal MHD simulations with a plane driver cannot reproduce the observed damping, the numerically predicted damping for a localized driver closely corresponds with the observations.
Solar and Stellar Astrophysics Plasma Physics
