Revisiting the formation mechanism for coronal rain from previous studies
Leping Li, Hardi Peter, Lakshmi Pradeep Chitta, Hongqiang Song

TL;DR
This study revisits the formation mechanisms of quiescent coronal rain, highlighting the role of interchange magnetic reconnection between open and closed magnetic field lines in its development.
Contribution
It provides a detailed analysis of 15 quiescent coronal rain events, demonstrating that 40% can be explained by interchange reconnection mechanisms, thus emphasizing its significance.
Findings
40% of studied events explained by interchange reconnection
Interchange reconnection plays a significant role in coronal rain formation
Revisiting previous reports supports the importance of magnetic reconnection
Abstract
Solar coronal rain is classified generally into two categories: flare-driven and quiescent coronal rain. The latter is observed to form along both closed and open magnetic field structures. Recently, we proposed that some of the quiescent coronal rain events, detected in the transition region and chromospheric diagnostics, along loop-like paths could be explained by the formation mechanism for quiescent coronal rain facilitated by interchange magnetic reconnection between open and closed field lines. In this study, we revisited 38 coronal rain reports from the literature. From these earlier works, we picked 15 quiescent coronal rain events out of the solar limb, mostly suggested to occur in active region closed loops due to thermal nonequilibrium, to scrutinize their formation mechanism. Employing the extreme ultraviolet images and line-of-sight magnetograms, the evolution of the…
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