2D fully kinetic simulations establish that reconnection in current sheets during nonlinear KHI drives localized anisotropic electron energization with suprathermal tails.
43(11):5606--5615
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MMS observations document turbulence spectra and electron-scale reconnection signatures inside Kelvin-Helmholtz waves during a geomagnetic storm.
This review summarizes the basic principles of electron transport in inhomogeneous and tangled magnetic fields through gyro-centre trajectories, kinetic instabilities, trapping, and diffusion processes.
citing papers explorer
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Reconnection-induced electron energization in magnetospheric Kelvin-Helmholtz dynamics
2D fully kinetic simulations establish that reconnection in current sheets during nonlinear KHI drives localized anisotropic electron energization with suprathermal tails.
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Turbulence properties and kinetic signatures of electron in Kelvin-Helmholtz waves during a geomagnetic storm
MMS observations document turbulence spectra and electron-scale reconnection signatures inside Kelvin-Helmholtz waves during a geomagnetic storm.
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Transport of electrons in tangled magnetic fields
This review summarizes the basic principles of electron transport in inhomogeneous and tangled magnetic fields through gyro-centre trajectories, kinetic instabilities, trapping, and diffusion processes.