11 citations · 36 across the 7 of their papers we have counts for
7 papers
Preferential acceleration of heavy ions in magnetic reconnection: Hybrid-kinetic simulations with electron inertia
Neeraj Jain, Jörg Büchner, Miroslav Bárta +1
Solar energetic particles (SEPs) in the energy range 10s KeV/nucleon-100s MeV/nucleon originate from Sun. Their high flux near Earth may damage the space borne electronics and gene…
Electron inertia effects in 3D hybrid-kinetic collisionless plasma turbulence
Patricio A. Muñoz, Neeraj Jain, Meisam Farzalipour Tabriz +2
The effects of the electron inertia on the current sheets that are formed out of kinetic turbulence are relevant to understand the importance of coherent structures in turbulence a…
Importance of accurate consideration of the electron inertia in hybrid-kinetic simulations of collisionless plasma turbulence: 1. The 2D limit
Neeraj Jain, Patricio Muñoz, Meisam Farzalipour Tabriz +2
The dissipation mechanism of the magnetic energy in turbulent collisionless space and astrophysical plasmas is still not well understood. Its investigation requires efficient kinet…
Ion acceleration in non-relativistic quasi-parallel shocks using fully kinetic simulations
Cedric Schreiner, Patrick Kilian, Felix Spanier +2
The formation of collisionless shock fronts is an ubiquitous phenomenon in space plasma environments. In the solar wind shocks might accompany coronal mass ejections, while even mo…
Electron-magnetohydrodynamic simulations of electron scale current sheet dynamics in the Vineta.II guide field reconnection experiment
Neeraj Jain, Adrian von Stechow, Patricio A. Muñoz +3
Three dimensional electron-magnetohydrodynamic (EMHD) simulations of electron current sheet dynamics in a background of stationary and unmagnetized ions and the subsequent generati…
Turbulent Plasmoid Reconnection
Fabien Widmer, Jörg Büchner, Nobumitsu Yokoi
The plasmoid instability may lead to fast magnetic reconnection through long current sheets(CS). It is well known that large-Reynolds-number plasmas easily become turbulent. We add…