In this review we focus on the fundamental theory of magnetohydrodynamic reconnection,
together with applications to understanding a wide range of dynamic processes in the solar …

In this study, we apply a new method—the first‐order Taylor expansion (FOTE)—to find
magnetic nulls and reconstruct magnetic field topology, in order to use it with the data from …

Theoretically, magnetic reconnection—the process responsible for solar flares and
magnetospheric substorms—occurs at the X‐line or radial null in the electron diffusion …

Magnetic reconnection is a fundamental process in laboratory, magnetospheric, solar and
astrophysical plasmas, whereby magnetic energy is converted into heat, bulk kinetic energy …

The Geotail spacecraft made in situ observations of magnetic reconnection on 15 May 2003
in the near‐Earth magnetotail at a radial distance of 28 RE when a moderate substorm …

Magnetic nulls are believed to play important roles in the energy dissipation during
reconnection. Such nulls have been observed in reconnection at the magnetopause …

A magnetic reconnection event detected by Cluster is analyzed using three methods: Single‐
spacecraft Inference based on Flow‐reversal Sequence (SIFS), Multispacecraft Inference …

While the plasma in the Earth's magnetotail predominantly consists of protons and electrons,
there are times when a significant amount of oxygen is present. When magnetic …

The interaction between interplanetary small-scale magnetic flux ropes and the magnetic
field in the ambient solar wind is an important topic in the understanding of the evolution of …

Magnetic reconnection is an important process in astrophysical, space and laboratory
plasmas. The magnetic null pair structure is theoretically suggested to be a crucial feature of …