pith:UDP6EX4L
The Role of Magnetic Reconnection in Energizing Protons and Heavier Ions at the Heliospheric Current Sheet
Simulations show magnetic reconnection at the heliospheric current sheet energizes protons and heavier ions to energies observed by Parker Solar Probe.
arxiv:2605.15068 v1 · 2026-05-14 · astro-ph.SR · physics.plasm-ph
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Claims
Multiple ion species develop power-law distributions with both spectral index and high-energy cutoff Emax consistent with in-situ data, and Emax scales as (Q/M)^alpha with alpha approximately 0.8-1.1.
The injection physics (initial energy and location of ions) is taken from separate kinetic simulations and assumed to hold when coupled to the large-scale MHD field; if the actual injection differs significantly, the predicted Emax scaling and spectral indices would change.
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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| First computed | 2026-05-17T21:40:26.045837Z |
|---|---|
| Last reissued | 2026-05-17T21:57:19.348875Z |
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | unsigned_v0 |
| Schema | pith-number/v1.0 |
Canonical hash
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Canonical record JSON
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