Predicting the time variation of radio emission from MHD simulations of a flaring T-Tauri star (2020)

First Author: Waterfall C

Attributed to: Multi-scale modelling of heating and particle acceleration in twisted magnetic fields in solar flares and coronal heating funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2006.05570

Publication URI: https://arxiv.org/abs/2006.05570

Type: Other