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physics.space-ph2022
Electron-driven instabilities in the solar wind
Daniel Verscharen, Benjamin D. G. Chandran, Elisabetta Boella +9
The electrons are an essential particle species in the solar wind. They often exhibit non-equilibrium features in their velocity distribution function. These include temperature an…
physics.space-ph2022
Anisotropic electron heating in turbulence-driven magnetic reconnection in the near-Sun solar wind
Luca Franci, Emanuele Papini, Alfredo Micera +5
We perform a high-resolution two-dimensional fully-kinetic numerical simulation of a turbulent plasma system with observation-driven conditions, in order to investigate the interpl…