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Observation of All Pre- and Post-reconnection Structures Involved in Three-dimensional Reconnection Geometries in Solar Eruptions
- 1.0521172 - ASÚ 2020 RIV US eng J - Journal Article
Dudík, Jaroslav - Lörinčík, Juraj - Aulanier, G. - Zemanová, Alena - Schmieder, B.
Observation of All Pre- and Post-reconnection Structures Involved in Three-dimensional Reconnection Geometries in Solar Eruptions.
Astrophysical Journal. Roč. 887, č. 1 (2019), č. článku 71. ISSN 0004-637X. E-ISSN 1538-4357
R&D Projects: GA ČR(CZ) GA17-16447S
Institutional support: RVO:67985815
Keywords : solar coronal mass ejections * solar corona * solar coronal loops
OECD category: Astronomy (including astrophysics,space science)
Impact factor: 5.746, year: 2019
Method of publishing: Limited access
https://doi.org/10.3847/1538-4357/ab4f86
We report on observations of the two newly identified reconnection geometries involving erupting flux ropes. In 3D, a flux rope can reconnect either with a surrounding coronal arcade (recently named “ar-rf” reconnection) or with itself (“rr-rf” reconnection), and both kinds of reconnection create a new flux-rope field line and a flare loop. For the first time, we identify all four constituents of both reconnections in a solar eruptive event, the filament eruption of 2011 June 7 observed by Solar Dynamics Observatory/Atmospheric Imaging Assembly.
Permanent Link: http://hdl.handle.net/11104/0305811
Number of the records: 1