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

Magnetic reconnection is a fundamental process whereby microscopic plasma processes
cause macroscopic changes in magnetic field topology, leading to explosive energy release …

The description of the local turbulent energy transfer and the high-resolution ion distributions
measured by the Magnetospheric Multiscale mission together provide a formidable tool to …

Whistler waves that can produce anomalous resistivity by affecting electrons' motion have
been suggested as one of the mechanisms responsible for magnetic reconnection in the …

In the present review we survey space plasma systems where the nonlinear resonant
interaction between charged particles and electromagnetic waves plays an important role …

We briefly review helicity dynamics, inverse and bidirectional cascades in fluid and
magnetohydrodynamic (MHD) turbulence, with an emphasis on the latter. The energy of a …

Whistler-mode waves are one of the most important plasma waves potentially affecting the
triggering and development processes of magnetic reconnection. They are widely present in …

A range of nonlinear wave structures, including Langmuir waves, unipolar electric fields, and
bipolar electric fields, are often observed in association with whistler-mode chorus waves in …

Abstract We present Magnetospheric Multiscale (MMS) mission measurements during a full
magnetopause crossing associated with an enhanced southward ion flow. A quasi‐steady …

Whistler mode waves are among the most intense electromagnetic emissions and play an
important role in the energy redistribution between electron populations in the Earth inner …