Three Types of Solar Coronal Rain during Magnetic Reconnection between Open and Closed Magnetic Structures
Coronal rain (CR) is a crucial part of the mass cycle between the corona and chromosphere.It includes flare-driven CR and two types of quiescent CR, along nonflaring active region closed loops and along open structures, separately, labeled as type I, type II, and type III CR, respectively.Among them, type I and type III CR are generally associated