This paper reviews Vlasov-based numerical methods used to model plasma in space
physics and astrophysics. Plasma consists of collectively behaving charged particles that …

In this paper, the particle acceleration processes around magnetotail dipolarization fronts
(DFs) were reviewed. We summarize the spacecraft observations (including Cluster …

Upstream Plasma Waves and Downstream Magnetic Reconnection at a Reforming Quasi-parallel
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Using high‐resolution data from the Magnetospheric Multiscale mission, an electron‐only
reconnection current sheet is found between two successive dipolarization fronts (DFs). The …

We report in situ observation of magnetic reconnection between magnetic flux rope (MFR)
and magnetic hole (MH) in the magnetosheath by the Magnetospheric Multiscale mission …

Magnetic reconnection underlies the physical mechanism of explosive phenomena in the
solar atmosphere and planetary magnetospheres, where plasma is usually collisionless. In …

Dipolarization fronts (DFs) are important for energy conversion, particle acceleration, and
flux transport in the magnetotail. The partition of energy conversion between ions and …

This review paper summarizes the research of Mercury's magnetosphere in the Post-
MESSENGER era and compares its dynamics to those in other planetary magnetospheres …

Within dipolarization fronts (DFs) in the Earth's magnetotail, significant magnetic energy is
converted to plasma energy, and a significant portion of the electrons and ions therein are …

In the last decades, a few spacecraft missions have been launched to investigate the
process of magnetic reconnection in space, during which magnetic free energy is …