Flare kernels may be smaller than you think: modelling the radiative response of chromospheric plasma adjacent to a solar flare (2022)

First Author: Osborne C

Attributed to: SASHA Simulations of alvenic solar heating funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stac2570

Publication URI: http://dx.doi.org/10.1093/mnras/stac2570

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 4