Observation of All Pre- and Post-reconnection Structures Involved in Three-dimensional Reconnection Geometries in Solar Eruptions

0521172 - ASÚ 2020 RIV US eng J - Článek v odborném periodiku
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
Grant CEP: GA ČR(CZ) GA17-16447S
Institucionální podpora: RVO:67985815
Klíčová slova: solar coronal mass ejections * solar corona * solar coronal loops
Obor OECD: Astronomy (including astrophysics,space science)
Impakt faktor: 5.746, rok: 2019
Způsob publikování: Omezený přístup
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.
Trvalý link: http://hdl.handle.net/11104/0305811