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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/10.1051/0004-6361/201833421

Publication URI: http://dx.doi.org/10.1051/0004-6361/201833421

Type: Journal Article/Review

Parent Publication: Astronomy & Astrophysics