Dayside magnetopause reconnection results in significant plasma heating and particle acceleration. In collisionless plasmas, velocity distribution fun...

Kinetic processes in collisionless plasmas, such as magnetic reconnection, create highly structured distribution functions, which are key to identifyi...

Magnetic flux ropes are columns of plasma with axial and azimuthal magnetic fields and are commonly observed in the solar corona, magnetotail reconnec...

Energy conversion in many space plasmas, due to their weak collisionality, produce velocity-space distribution functions (VDFs) that are far from loca...

Magnetic reconnection occurs throughout the heliosphere and has a major impact on the morphology of plasmas in this system. However, recent Parker Sol...

The ability to predict the fraction of magnetic energy converted during magnetic reconnection into plasma heating is crucial to assess its impact on t...

Pressure-strain interaction has emerged as an important channel of energy conversion in collisionless plasma. On the one hand, it describes the pathwa...

The NASA Magnetospheric Multiscale (MMS) mission explores the boundary regions of the Earth's magnetosphere with high-accuracy measurements of charged...