Flows and magnetic field structures in reconnection regions of simulations of the solar atmosphere: Do flux pile-up models work?

Shelyag, Sergiy; Litvinenko, Y E; Fedun, V; Verth, G; González-Avilés, J J; Guzmán, F S

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Flows and magnetic field structures in reconnection regions of simulations of the solar atmosphere: Do flux pile-up models work?

journal contribution

posted on 2018-12-01, 00:00 authored by Sergiy ShelyagSergiy Shelyag, Y E Litvinenko, V Fedun, G Verth, J J González-Avilés, F S Guzmán

Flows and magnetic field structures in reconnection regions of simulations of the solar atmosphere: Do flux pile-up models work?

History

Journal

Astronomy and astrophysics

Volume

620

Article number

A159

Publisher

EDP Sciences

Location

London, Eng.

Publisher DOI

https://doi.org/10.1051/0004-6361/201833752

Link to full text

https://www.aanda.org/articles/aa/pdf/2018/12/aa33752-18.pdf

ISSN

0004-6361

eISSN

1432-0746

Language

eng

Publication classification

C Journal article; C1 Refereed article in a scholarly journal

Copyright notice

2018, EDP Sciences

Flows and magnetic field structures in reconnection regions of simulations of the solar atmosphere: Do flux pile-up models work?

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