The First 3D Coronal Loop Model Heated by MHD Waves against Radiative Losses (2021)

First Author: Shi M

Attributed to: STFC Consolidated Grant for the Solar Physics Group at Northumbria University funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2101.01019

Publication URI: https://arxiv.org/abs/2101.01019

Type: Other