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.
The acceleration of charged particles and formation of power-law energy spectra in nonrelativistic magnetic reconnection
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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.