Solar wind is probably the best laboratory to study turbulence in astrophysical plasmas. In
addition to the presence of magnetic field, the differences with neutral fluid isotropic …

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 …

Context. Fast radio bursts (FRBs) are transient sources of unknown origin. Recent radio and
optical observations have provided strong evidence for an extragalactic origin of the …

Fast radio bursts are mysterious transient sources likely located at cosmological distances.
The derived brightness temperatures exceed by many orders of magnitude the self …

The accuracy of quasilinear theory applied to the electron bump-on-tail instability, a classic
model problem, is explored with conservative high-order discontinuous Galerkin methods …

All the bodies of the solar system are embedded in the supersonic flux of energetic particles
emitted by the Sun. Since the advent of the space age, the models to describe the interaction …

Context. Coherent radiation of pulsars, magnetars, and fast radio bursts could, in theory, be
interpreted as radiation from solitons and soliton-like waves. Solitons are meant to contain a …

Mutual impedance (MI) experiments are a kind of plasma diagnostic techniques for the
identification of the in situ plasma density and electron temperature. These plasma …

High time resolution observations from the STEREO spacecraft show that in solar type III
radio bursts, Langmuir waves often occur as very intense one‐dimensional magnetic field …

Intense localized Langmuir waves in the solar wind are often associated with type III solar
radio bursts. Wave packets with a Gaussian fall‐off of electric field with distance are shown …