2021
DOI: 10.5194/egusphere-egu21-8830
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Vlasov simulation of electrons in the context of hybrid global models: An eVlasiator approach

Abstract: <p>Modern investigations of dynamical space plasma systems such as magnetically complicated topologies within the Earth's magnetosphere make great use of supercomputer models as well as spacecraft observations. Space plasma simulations can be used to investigate energy transfer, acceleration, and plasma flows on both global and local scales. Simulation of global magnetospheric dynamics requires spatial and temporal scales achievable currently through magnetohydrodynamics or hybrid-kinetic simulat… Show more

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(8 citation statements)
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“…In this work, we employed the novel eVlasiator method (Battarbee et al., 2021) to model electron distributions in a global magnetosphere simulation, using an ion‐scale, geomagnetically active background from a previous Vlasiator 2D‐3V simulation. We present VDFs at the dayside magnetopause, the tail current sheet, and the PSBL and show that they have a remarkable agreement with MMS observations.…”
Section: Summary and Discussionmentioning
confidence: 99%
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“…In this work, we employed the novel eVlasiator method (Battarbee et al., 2021) to model electron distributions in a global magnetosphere simulation, using an ion‐scale, geomagnetically active background from a previous Vlasiator 2D‐3V simulation. We present VDFs at the dayside magnetopause, the tail current sheet, and the PSBL and show that they have a remarkable agreement with MMS observations.…”
Section: Summary and Discussionmentioning
confidence: 99%
“…Only the electron distributions are propagated according to the Vlasov equation, which is solved in a leapfrog fashion, alternating spatial translations and velocity space accelerations. In addition to magnetic force and convective and electron pressure gradient electric fields, the electrons experience electric fields EJnormale ${\vec{E}}_{{J}_{\mathrm{e}}}$ as a result of their oscillations, solved in tandem with the electron bulk velocity Ve ${\vec{V}}_{\mathrm{e}}$ (Battarbee et al., 2021): δEJnormale=δt0.17emc2()×trueB+μ0e()neVenpVp $\delta {\vec{E}}_{{J}_{\mathrm{e}}}=\delta t\,{c}^{2}\left(\nabla \times \vec{B}+{\mu }_{0}e\left({n}_{e}{\vec{V}}_{e}-{n}_{p}{\vec{V}}_{p}\right)\right)$ δVe=δt0.17ememeEJnormale $\delta {\vec{V}}_{e}=\delta t\,\frac{e}{{m}_{e}}{\vec{E}}_{{J}_{\mathrm{e}}}$ in a coupled Runge‐Kutta 4 scheme, with EJe,t0=0 ${\vec{E}}_{{J}_{\mathrm{e}},{t}_{0}}=0$ for the initial eVlasiator step, δt the Runge‐Kutta timestep, and c the speed of light. See Battarbee et al.…”
Section: Model and Methodsmentioning
confidence: 99%
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