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Electron Signatures of Reconnection in a Global eVlasiator Simulation
M Alho1, M Battarbee1, Y Pfau-Kempf1
1Department of Physics University of Helsinki Helsinki Finland.
Summary
The eVlasiator model simulates electron dynamics in geospace plasma, revealing ion-scale processes drive electron kinetic signatures observed by Magnetospheric Multiscale (MMS) spacecraft during magnetic reconnection.
Area of Science:
- Space Physics
- Plasma Physics
- Computational Astrophysics
Background:
- Geospace plasma simulations advance solar wind-magnetosphere interaction modeling.
- Electron scales remain computationally challenging in global simulations.
Purpose of the Study:
- Introduce eVlasiator, a novel submodule for global hybrid-ion kinetic simulations.
- Investigate electron scale dynamics influenced by ion-driven electromagnetic fields.
- Compare simulated electron distributions with Magnetospheric Multiscale (MMS) observations.
Main Methods:
- Utilized the Vlasiator model with its new eVlasiator submodule.
- Simulated global hybrid-ion kinetic plasma dynamics.
- Analyzed electron distribution functions at reconnection sites.
- Compared simulation results with MMS spacecraft data.
Main Results:
- eVlasiator successfully reproduces kinetic electron signatures.
- Simulated electron features (inflows, outflows, distributions, streaming) match MMS observations.
- Key reconnection phenomena are captured despite truncated electron physics and ion-scale resolution.
Conclusions:
- Ion-scale dynamics and ion-generated magnetic fields are crucial for electron dynamics in near-Earth plasmas.
- eVlasiator demonstrates the capability to simulate electron-scale phenomena in a global context.
- The study validates the importance of ion kinetics in shaping observable electron behavior.
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