Proton imaging has become a key diagnostic for measuring electromagnetic fields in high-
energy-density (HED) laboratory plasmas. Compared to other techniques for diagnosing …

Quasiperiodic erupters are a remarkable class of objects exhibiting very-large-amplitude
quasiperiodic X-ray flares. Although numerous dynamical models have been proposed to …

This review of scaling theories of magnetohydrodynamic (MHD) turbulence aims to put the
developments of the last few years in the context of the canonical time line (from Kolmogorov …

The physics of astrophysical jets can be divided into three regimes:(i) engine and launch (ii)
propagation and collimation,(iii) dissipation and particle acceleration. Since astrophysical …

Magnetic fields in several astrophysical objects are amplified and maintained by a dynamo
mechanism, which is the conversion of the turbulent kinetic energy to magnetic energy. A …

Turbulence in a conducting plasma can amplify seed magnetic fields in what is known as the
turbulent, or small-scale, dynamo. The associated growth rate and emergent magnetic-field …

Interaction of an ultrastrong short laser pulse with nonprepolarized near-critical density
plasma is investigated in an ultrarelativistic regime, with an emphasis on the radiative spin …

The turbulent dynamo is a powerful mechanism that converts turbulent kinetic energy to
magnetic energy. A key question regarding the magnetic field amplification by turbulence, is …

In conventional gases and plasmas, it is known that heat fluxes are proportional to
temperature gradients, with collisions between particles mediating energy flow from hotter to …

The origin of the cosmic magnetic field remains an unsolved mystery, relying not only on
specific dynamo processes but also on the seed field to be amplified. Recently, the diffuse …