Fast magnetoacoustic waves steepen and dissipate nonlinearly before reaching coronal magnetic null points due to decreasing fast speed in the non-uniform magnetic field.
2022 Direct observations of anomalous resistivity and diffusion in collisionless plasma
3 Pith papers cite this work. Polarity classification is still indexing.
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3D MHD modeling of candle-flame solar flares reveals Y-points do not coincide with apparent cusp tips and observed downflow speeds underestimate reconnection Alfvén speeds by 2-10x.
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.
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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.