Titlebook: Microphysics of Magnetic Reconnection in Near-Earth Space; Spacecraft Observati Giulia Cozzani Book 2020 The Editor(s) (if applicable) and

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Numerical Models for Astrophysical Plasmas, kinetic description of a plasma eventually deriving the Vlasov equation. Section 5.2 discusses the different approaches that can be used to model plasma processes, notably the fluid (Magneto-Hydro-Dynamics, MHD), the hybrid model and the kinetic codes. A brief description of Particle-In-Cell (PIC)

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ViDA: A Vlasov-DArwin Solver for Plasma Physics at Electron Scales, and sub-proton spatial scales, where proton kinetic effects are dominant, while electrons can be approximated as an isothermal fluid (hybrid framework) (Valentini et?al. .). In this range of scales, both Particle-In-Cell (PIC)?and Eulerian hybrid codes?(see Sect. .) have been extensively employed t

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Fully Kinetic Vlasov Simulation of Collisionless Magnetic Reconnection,rstly, the magnetic reconnection signatures are presented. Then, the chapter focuses on the evaluation of the contribution of the terms of Ohm’s law in the EDR. It is found that the electron inertia term, and in particular the term which is proportional to the temporal variation of the current densi

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Book 2020merical simulations. Magnetic reconnection is a? fundamental process in plasma physics during which the topological reconfiguration of the magnetic field leads to energy conversion and particle energization. The book focuses on the physics of the electron diffusion region (EDR), a crucial region whe

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Fully Kinetic Vlasov Simulation of Collisionless Magnetic Reconnection,ty plays a role in sustaining the reconnection electric field. This contribution is not limited to an electron scale region around the X-point but it extends to the ion scales in the outflow direction. This feature can depend on the artificially low mass ratio adopted here.