Simulations of particle acceleration in turbulent plasma regions with multiple contracting and
merging (reconnecting) magnetic islands emphasize the key role of temporary particle …

Magnetic reconnection is an important process in space,,,, and laboratory plasmas that
effectively converts magnetic energy into plasma kinetic energy within a current sheet …

ABSTRACT In 2010 May 23–24, Solar Dynamics Observatory (SDO) observed the launch of
two successive coronal mass ejections (CMEs), which were subsequently tracked by the …

Previous application of our focused transport equation for energetic ion test particle
acceleration by numerous active small-scale flux ropes to solar wind conditions near 1 au …

We report unambiguous in situ observation of the coalescence of macroscopic flux ropes by
the magnetospheric multiscale (MMS) mission. Two coalescing flux ropes with sizes of∼ 1 …

A major discovery of Parker Solar Probe (PSP) was the presence of large numbers of
localized increases in the radial solar wind speed and associated sharp deflections of the …

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 …

Computational and observational evidence is accruing that heliospheric shocks, as emitters
of vorticity, can produce downstream magnetic flux ropes and filaments. This led Zank et al …

The occurrence of spatially and temporally variable reconnection at the Earth's
magnetopause leads to the complex interaction of magnetic fields from the magnetosphere …

Magnetic flux ropes (MFRs) are significant regions for the production of energetic electrons
in space and astrophysical plasmas. However, the research on electron heating and …