Non-thermal line broadening due to braiding-induced turbulence in solar coronal loops (2020)

First Author: Pontin D
Attributed to:  Dynamics of Complex Magnetic Fields: From the corona to the solar wind funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/202037582

Publication URI: http://dx.doi.org/10.1051/0004-6361/202037582

Type: Journal Article/Review

Parent Publication: Astronomy & Astrophysics