Repeated Coronal Condensations Caused by Magnetic Reconnection between Solar Coronal Loops

We recently presented coronal condensations, caused by magnetic reconnection (MR) between coronal loops from extreme ultraviolet observations, over the course of one day, on 2012 January 19. In this paper, by investigating the loops over an extended period of time from January 16 to 20, we present a...

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Veröffentlicht in:	The Astrophysical journal 2019-10, Vol.884 (1), p.34
Hauptverfasser:	Li, Leping, Peter, Hardi, Chitta, Lakshmi Pradeep, Zhang, Jun, Su, Jiangtao, Song, Hongqiang, Hou, Yijun, Xia, Chun
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Closed loops Condensation Cooling Corona Coronal loops magnetic fields Magnetic reconnection plasmas Solar corona Sun: corona Sun: UV radiation
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