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

Shelyag, S., Litvinenko, Y. E., Fedun, V., Verth, G., González-Avilés, J. J. and Guzmán, F. S. 2018, Flows and magnetic field structures in reconnection regions of simulations of the solar atmosphere: do flux pile-up models work?, Astronomy and astrophysics, vol. 620, doi: 10.1051/0004-6361/201833752.

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Title Flows and magnetic field structures in reconnection regions of simulations of the solar atmosphere: do flux pile-up models work?
Author(s) Shelyag, S.ORCID iD for Shelyag, S. orcid.org/0000-0002-6436-9347
Litvinenko, Y. E.
Fedun, V.
Verth, G.
González-Avilés, J. J.
Guzmán, F. S.
Journal name Astronomy and astrophysics
Volume number 620
Article ID A159
Total pages 7
Publisher EDP Sciences
Place of publication London, Eng.
Publication date 2018-12
ISSN 0004-6361
Keyword(s) Science & Technology
Physical Sciences
Astronomy & Astrophysics
Sun: atmosphere
Sun: magnetic fields
Sun: photosphere
Sun: chromosphere
STEADY-STATE
EXPLOSIVE EVENTS
CANCELLATION
EVOLUTION
PHOTOSPHERE
FEATURES
ENERGY
Language eng
DOI 10.1051/0004-6361/201833752
Field of Research 0201 Astronomical And Space Sciences
HERDC Research category C1 Refereed article in a scholarly journal
ERA Research output type C Journal article
Copyright notice ©2018, EDP Sciences
Persistent URL http://hdl.handle.net/10536/DRO/DU:30116109

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