L Comisso, L Sironi - The Astrophysical Journal Letters, 2022 - iopscience.iop.org
Turbulence is often invoked to explain the origin of nonthermal particles in space and astrophysical plasmas. By means of 3D fully kinetic particle-in-cell simulations, we …
Our understanding of processes occurring in the heliosphere historically began with reduced dimensionality-one-dimensional (1D) and two-dimensional (2D) sketches and …
Nonthermal acceleration of particles in magnetohydrodynamic (MHD) turbulence plays a central role in a wide variety of astrophysical sites. This physics is addressed here in the …
We present the first plasma simulations obtained with the code dHybridR, a hybrid particle-in- cell code with fluid electrons and both thermal and energetic ions that retain relativistic …
Context. Plasma turbulence can be viewed as a magnetic landscape populated by large- and small-scale coherent structures. In this complex network, large helical magnetic tubes …
The microphysical, kinetic properties of astrophysical plasmas near accreting compact objects are still poorly understood. For instance, in modern general-relativistic …
We present an event observed by Parker Solar Probe (PSP) at∼ 0.2 au on 2022 March 2 in which imaging and in situ measurements coincide. During this event, PSP passed through …
Energetic particle transport in the interplanetary medium is known to be affected by magnetic structures. It has been demonstrated for solar energetic particles in near-Earth orbit studies …
A novel technique is presented for describing and visualizing the local topology of the magnetic field using single-spacecraft data in the solar wind. The approach merges two …