Coronal mass ejections (CMEs) are the largest-scale eruptive phenomenon in the solar
system, expanding from active region-sized nonpotential magnetic structure to a much larger …

Solar flare emission is detected in all EM bands and variations in flux density of solar
energetic particles. Often the EM radiation generated in solar and stellar flares shows a …

Observations indicate that reconnection-favored emerging flux has a strong correlation with
coronal mass ejectons (CMEs). Motivated by this observed correlation and based on the flux …

This two-part book is devoted to classic fundamentals and current practices and
perspectives of modern plasma astrophysics. This second part discusses the physics of …

Coronal bright points (CBPs) are long-lived small-scale brightenings in the solar corona.
They are generally explained by magnetic reconnection. However, the corresponding …

The dynamics of magnetic reconnection in the solar current sheet (CS) is studied by high-
resolution 2.5-dimensional MHD simulation. With the commencing of magnetic …

Solar flares are an explosive phenomenon where super-sonic flows and shocks are
expected in and above the post-flare loops. To understand the dynamics of post-flare loops …

This Letter presents a direct example of the shrinkage of flare loops from the radio
observation of a limb X3. 1 flare occurring at 00: 49 UT on 2002 August 24. The relation …

Ellerman bombs and Type II white-light flares share many common features despite the
large energy gap between them. Both are considered to result from local heating in the solar …

The aim of the present study is to investigate the reconnection jets formed during the
process of magnetic flux cancellation in the physical environment of the solar transition …