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Electron Signatures of Reconnection in a Global eVlasiator Simulation

Abstract Geospace plasma simulations have progressed toward more realistic descriptions of the solar wind–magnetosphere interaction from magnetohydrodynamic to hybrid ion‐kinetic, such as the state‐of‐the‐art Vlasiator model. Despite computational advances, electron scales have been out of reach in...

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Furkejuvvon:
Váldodahkkit: M. Alho, M. Battarbee, Y. Pfau‐Kempf, Yu. V. Khotyaintsev, R. Nakamura, G. Cozzani, U. Ganse, L. Turc, A. Johlander, K. Horaites, V. Tarvus, H. Zhou, M. Grandin, M. Dubart, K. Papadakis, J. Suni, H. George, M. Bussov, M. Palmroth
Materiálatiipa: Artigo
Giella:Inglês
Almmustuhtton: Wiley 2022-07-01
Ráidu:Geophysical Research Letters
Fáttát:
kinetic simulation
reconnection
electron distribution function
magnetosphere
vlasov equation
electric field
Liŋkkat:https://doi.org/10.1029/2022GL098329
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