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Pith Number

pith:X4AWOIIT

pith:2026:X4AWOIITQ2SHEBI6WAFDDLK7G6
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Direct Evidence of Non-Ideal Dissipative Dynamics in Solar Wind Magnetic Switchbacks

Forrest Mozer, Kyung-Eun Choi, Oleksiy Agapitov, Richard Sydora

Parker Solar Probe measurements reveal non-zero electric fields inside solar wind switchbacks in the plasma frame, proving they are Hall-MHD structures.

arxiv:2605.14114 v1 · 2026-05-13 · astro-ph.SR

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\usepackage{pith}
\pithnumber{X4AWOIITQ2SHEBI6WAFDDLK7G6}

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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

Parker Solar Probe electric field measurements show that switchbacks have non-zero electric fields in the plasma frame, definitively proving that switchbacks are Hall-MHD, not Ideal MHD, structures.

C2weakest assumption

The transformation to the plasma frame accurately captures the true electric field without significant instrumental or spacecraft velocity errors, and that non-zero E directly implies Hall-MHD dominance over ideal MHD.

C3one line summary

Parker Solar Probe data reveals non-zero electric fields in the plasma frame of magnetic switchbacks, proving they are non-ideal Hall-MHD structures undergoing active evolution.

References

4 extracted · 4 resolved · 0 Pith anchors

[1] Properties of Magnetic Switchbacks in the Near-Sun Solar Wind 2026 · doi:10.1007/s11214-026-
[2] Magnetic switchback formation: a review of proposed mechanisms 2026 · doi:10.1007/s11214-
[3] Magnetic Reconnection: MHD Theory and Applications 2000 · doi:10.1017/cbo9780511525087
[4] Measuring the Coronal Plasma and Magnetic Field, Plasma Waves and Turbulence, and Radio Signatures of Solar Transients 2016 · doi:10.1007/s11214-016-0244-5

Formal links

2 machine-checked theorem links

Receipt and verification
First computed 2026-05-17T23:39:11.966863Z
Builder pith-number-builder-2026-05-17-v1
Signature Pith Ed25519 (pith-v1-2026-05) · public key
Schema pith-number/v1.0

Canonical hash

bf0167211386a472051eb00a31ad5f37ac423f539f4af280933271d923436e4b

Aliases

arxiv: 2605.14114 · arxiv_version: 2605.14114v1 · doi: 10.48550/arxiv.2605.14114 · pith_short_12: X4AWOIITQ2SH · pith_short_16: X4AWOIITQ2SHEBI6 · pith_short_8: X4AWOIIT
Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/X4AWOIITQ2SHEBI6WAFDDLK7G6 \
  | 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: bf0167211386a472051eb00a31ad5f37ac423f539f4af280933271d923436e4b
Canonical record JSON
{
  "metadata": {
    "abstract_canon_sha256": "fb67ef851b6a075760ae1479235943135153e8cb1c2af9e462ee1bc7ccb38382",
    "cross_cats_sorted": [],
    "license": "http://creativecommons.org/licenses/by/4.0/",
    "primary_cat": "astro-ph.SR",
    "submitted_at": "2026-05-13T21:01:54Z",
    "title_canon_sha256": "b2ccea22ea37a64ac947e41564223be58e319a74faf312e31ad1444dc776818a"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2605.14114",
    "kind": "arxiv",
    "version": 1
  }
}