This paper summarises some of the recent progress that has been made in understanding
astrophysical plasma turbulence in the solar wind, from in situ spacecraft observations. At …

The near-Earth space is a unique laboratory to explore turbulence and energy dissipation
processes in magnetized plasmas thanks to the availability of high-quality data from various …

INTRODUCTION Magnetic reconnection is a physical process occurring in plasmas in which
magnetic energy is explosively converted into heat and kinetic energy. The effects of …

The Exploration of energization and Radiation in Geospace (ERG) Science Center serves
as a hub of the ERG project, providing data files in a common format and develo** the …

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 …

The Earth's magnetosphere and its bow shock, which is formed by the interaction of the
supersonic solar wind with the terrestrial magnetic field, constitute a rich natural laboratory …

Weakly collisional and collisionless plasmas are typically far from local thermodynamic
equilibrium (LTE), and understanding energy conversion in such systems is a forefront …

Abstract The Magnetospheric Multiscale (MMS) mission and operations are designed to
provide the maximum reconnection science. The mission phases are chosen to investigate …

Turbulent plasmas generate a multitude of thin current structures that can be sites for
magnetic reconnection. The Magnetospheric Multiscale (MMS) mission has recently …

How turbulent energy is dissipated in weakly collisional space and astrophysical plasmas is
a major open question. Here, we present the application of a field-particle correlation …