Recent near-Sun solar-wind observations from Parker Solar Probe have found a highly
dynamic magnetic environment, permeated by abrupt radial-field reversals, or" switchbacks." …

Direct evidence of an inertial-range turbulent energy cascade has been provided by
spacecraft observations in heliospheric plasmas. In the solar wind, the average value of the …

Abstract Properties of the turbulent cascade from fluid to kinetic scales in collisionless
plasmas are investigated by means of large-size 3D hybrid (fluid electrons, kinetic protons) …

We investigate properties of plasma turbulence from magnetohydrodynamic (MHD) to sub-
ion scales by means of two-dimensional, high-resolution hybrid particle-in-cell simulations …

Using a three-dimensional compressible magnetohydrodynamic (MHD) simulation, we have
reproduced the fast solar wind in a direct and self-consistent manner, based on the …

For the solar wind, a wealth of observational evidence indicates that turbulence is an
important dynamical process for velocity (v), magnetic (b), and other related fluctuations at …

We investigate properties of large-scale solar wind Alfvénic fluctuations and their evolution
during radial expansion. We assume a strictly radial background magnetic field B∥ R⁠, and …

Switchbacks—abrupt reversals of the magnetic field within the solar wind—have been
ubiquitously observed by Parker Solar Probe (PSP). Their origin, whether from processes …

Magnetic switchbacks are rapid high-amplitude reversals of the radial magnetic field in the
solar wind that do not involve a heliospheric current sheet crossing. First seen sporadically …

We present results from a high-resolution and large-scale hybrid (fluid electrons and particle-
in-cell protons) two-dimensional numerical simulation of decaying turbulence. Two distinct …