Magnetic reconnection converts magnetic field energy into particle energy by breaking and
reconnecting magnetic field lines. Magnetic reconnection is a kinetic process that generates …

Dayside transients, such as hot flow anomalies, foreshock bubbles, magnetosheath jets, flux
transfer events, and surface waves, are frequently observed upstream from the bow shock …

Magnetic reconnection converts, often explosively, stored magnetic energy to particle
energy in space and in the laboratory. Through processes operating on length scales that …

Magnetic reconnection is known to be an important process for coupling solar wind mass
and momentum into the Earth's magnetosphere. Reconnection is initiated in an electron …

One of the major questions about magnetic reconnection is how specific solar wind and
interplanetary magnetic field conditions influence where reconnection occurs at the Earth's …

The Earth's magnetopause is an ion‐scale boundary that separates the magnetosphere
from the shocked solar wind. At such boundary, energy‐conversion processes frequently …

A concise review is given on the past two decades' results from laboratory experiments on
collisionless magnetic reconnection in direct relation with space measurements, especially …

We review the range of applications and use of the curlometer, initially developed to analyze
Cluster multi‐spacecraft magnetic field data; but more recently adapted to other arrays of …

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 …

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 …