Web13 apr. 2024 · The key ingredients that make Vlasov simulations at magnetospheric scales possible are the sparse velocity space implementation and spatial adaptive mesh refinement. ... “ The dynamic quasiperpendicular shock: Cluster discoveries,” in Microphysics of Cosmic Plasmas ( Springer US, Boston, MA, 2014), pp. 459 ... WebTo investigate the possible magnetospheric source of this structure, we simulate the entire process with the Rice Convection Model coupled with an MHD code (RCM-MHD). After the long-lasting low-entropy plasma is supplied from the tailward boundary, frequent drippings and the accompanying oscillations in the near-Earth plasma sheet are reproduced.
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X-Ray Emission of Auroral Electrons and Magnetospheric …
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