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Observation of All Pre- and Post-reconnection Structures Involved in Three-dimensional Reconnection Geometries in Solar Eruptions
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SYSNO ASEP 0521172 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title Observation of All Pre- and Post-reconnection Structures Involved in Three-dimensional Reconnection Geometries in Solar Eruptions Author(s) Dudík, Jaroslav (ASU-R) RID, ORCID
Lörinčík, Juraj (ASU-R) ORCID
Aulanier, G. (FR)
Zemanová, Alena (ASU-R) ORCID, RID
Schmieder, B. (FR)Article number 71 Source Title Astrophysical Journal - ISSN 0004-637X
Roč. 887, č. 1 (2019)Number of pages 8 s. Publication form Online - E Language eng - English Country US - United States Keywords solar coronal mass ejections ; solar corona ; solar coronal loops Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics OECD category Astronomy (including astrophysics,space science) R&D Projects GA17-16447S GA ČR - Czech Science Foundation (CSF) Method of publishing Limited access Institutional support ASU-R - RVO:67985815 UT WOS 000506001500071 EID SCOPUS 85077308304 DOI 10.3847/1538-4357/ab4f86 Annotation 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. Workplace Astronomical Institute Contact Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2020 Electronic address https://doi.org/10.3847/1538-4357/ab4f86
Number of the records: 1