Magnetic reconnection at the heliospheric current sheet produces power-law ion distributions whose spectral index and Emax scaling with charge-to-mass ratio are consistent with Parker Solar Probe data.
13(1):9--49
2 Pith papers cite this work, alongside 1,395 external citations. Polarity classification is still indexing.
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The paper reviews electron transport in tangled magnetic fields, including creation via turbulence, modulation by instabilities, trapping, cross-field diffusion, and energization.
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The Role of Magnetic Reconnection in Energizing Protons and Heavier Ions at the Heliospheric Current Sheet
Magnetic reconnection at the heliospheric current sheet produces power-law ion distributions whose spectral index and Emax scaling with charge-to-mass ratio are consistent with Parker Solar Probe data.
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Transport of electrons in tangled magnetic fields
The paper reviews electron transport in tangled magnetic fields, including creation via turbulence, modulation by instabilities, trapping, cross-field diffusion, and energization.