Using the Stokes V widths of Fe I lines for diagnostics of the intrinsic solar photospheric magnetic field (2019)

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.1912.03340

Publication URI: https://arxiv.org/abs/1912.03340

Type: Other