Analysis of unresolved photospheric magnetic field structure using Fe I 6301 and 6302 lines (2018)

First Author: Gordovskyy. M

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.1808.06862

Publication URI: https://arxiv.org/abs/1808.06862

Type: Other