An Observationally-Constrained Model of a Flux Rope that Formed in the Solar Corona (2018)

First Author: James A

Attributed to: MSSL Solar & Planetary Physics Consolidated Grant 2016-2019 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1802.07965

Publication URI: https://arxiv.org/abs/1802.07965

Type: Other