A comprehensive three-dimensional radiative magnetohydrodynamic simulation of a solar flare-Reference-Cited by-同舟云学术

A comprehensive three-dimensional radiative magnetohydrodynamic simulation of a solar flare

Published:2018-11-26 Issue:2 Volume:3 Page:160-166
ISSN:2397-3366
Container-title:Nature Astronomy
language:en
Short-container-title:Nat Astron

Author:

Cheung M. C. M.^ORCID,Rempel M.,Chintzoglou G.,Chen F.^ORCID,Testa P.,Martínez-Sykora J.,Sainz Dalda A.,DeRosa M. L.^ORCID,Malanushenko A.,Hansteen V.,De Pontieu B.,Carlsson M.,Gudiksen B.,McIntosh S. W.^ORCID

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

http://www.nature.com/articles/s41550-018-0629-3.pdf

Reference50 articles.

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2. Shibata, K. & Magara, T. Solar flares: magnetohydrodynamic processes. Living Rev. Solar Phys. 8, 6 (2011).

3. Schrijver, C. J. Driving major solar flares and eruptions: a review. Adv. Space Res. 43, 739–755 (2009).

4. Fisher, G. H. et al. The coronal global evolutionary model: using HMI vector magnetogram and Doppler data to model the buildup of free magnetic energy in the solar corona. Space Weather 13, 369–373 (2015).

5. Amari, T., Canou, A. & Aly, J.-J. Characterizing and predicting the magnetic environment leading to solar eruptions. Nature 514, 465–469 (2014).

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