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pith:UDP6EX4L

pith:2026:UDP6EX4LN25AYBHTAUBE3ISDEU
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The Role of Magnetic Reconnection in Energizing Protons and Heavier Ions at the Heliospheric Current Sheet

Colby Haggerty, Fan Guo, Giulia Murtas, Giuseppe Arr\`o, Jeongbhin Seo, Xiaocan Li

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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\pithnumber{UDP6EX4LN25AYBHTAUBE3ISDEU}

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Record completeness

1 Bitcoin timestamp
2 Internet Archive
3 Author claim open · sign in to claim
4 Citations open
5 Replications open
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The bundle contains the canonical record plus signed events. A mirror can host it anywhere and recompute the same current state with the deterministic merge algorithm.

Claims

C1strongest claim

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.

C2weakest assumption

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.

C3one line summary

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.

References

50 extracted · 50 resolved · 0 Pith anchors

[1] F., Swisdak, M., et al 2021 · doi:10.1103/physrevlett.126.135101
[2] Blandford \ and\ author D 1987 · doi:10.1016/0370-1573(87)90134-7
[3] 2023a, in EGU General Assembly Conference Abstracts, EGU General Assembly Conference Abstracts, EGU–3494, doi: 10.5194/egusphere-egu23-3494 · doi:10.5194/egusphere-egu23-3494
[4] Desai, M. I., Mitchell, D. G., McComas, D. J., et al. 2022, ApJ, 927, 62, doi: 10.3847/1538-4357/ac4961 2022 · doi:10.3847/1538-4357/ac4961
[5] Desai, M. I., Drake, J. F., Phan, T., et al. 2025, ApJL, 985, L38, doi: 10.3847/2041-8213/ada697 2025 · doi:10.3847/2041-8213/ada697

Formal links

1 machine-checked theorem link

Receipt and verification
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

a0dfe25f8b6eba0c04f305024da243252bb137890cc614d470a03157ca375b98

Aliases

arxiv: 2605.15068 · arxiv_version: 2605.15068v1 · pith_short_12: UDP6EX4LN25A · pith_short_16: UDP6EX4LN25AYBHT · pith_short_8: UDP6EX4L
Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/UDP6EX4LN25AYBHTAUBE3ISDEU \
  | jq -c '.canonical_record' \
  | python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
# expect: a0dfe25f8b6eba0c04f305024da243252bb137890cc614d470a03157ca375b98
Canonical record JSON
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    ],
    "license": "http://creativecommons.org/licenses/by/4.0/",
    "primary_cat": "astro-ph.SR",
    "submitted_at": "2026-05-14T16:57:04Z",
    "title_canon_sha256": "dc8dcbe7e4d85e7ad6d79816cd79fdd97a5c921b608299a87394696835073e57"
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}