Pith Number

pith:PAOJLW67

pith:2026:PAOJLW673ACWAZAVTVGHL4RMWK

not attested not anchored not stored refs pending

Multi-Viewpoint Observation of a Failed Prominence Eruption on the Sun

Astrid M. Veronig, Bin Chen, Bin Zhuang, Katharine K. Reeves, Peter R. Young, Sijie Yu, Tingyu Gou, Xingyao Chen

External reconnection on an erupting solar flux rope slows it down and prevents escape from the Sun.

arxiv:2604.23084 v1 · 2026-04-25 · astro-ph.SR

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\usepackage{pith}
\pithnumber{PAOJLW673ACWAZAVTVGHL4RMWK}

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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

✓ Portable graph bundle live · download bundle · merged state

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

As the high rate of external reconnection proceeds, the flux rope and embedded prominence decelerate noticeably and fail to erupt into the heliosphere, under strong magnetic confinement of overlying fields.

C2weakest assumption

The multi-wavelength signatures are produced by external reconnection occurring on the erupting flux rope rather than by other coronal processes.

C3one line summary

External reconnection on an erupting solar flux rope removes flux and decelerates the structure, preventing escape under strong magnetic confinement.

References

72 extracted · 0 resolved · 0 Pith anchors

[1] Priest, E. R. & Forbes, T. G. The magnetic nature of solar flares.Astron. Astrophys. Rev.10, 313–377 (2002) 2002

[2] Chen, P. F. Coronal Mass Ejections: Models and Their Observational Basis.Living Rev. Sol. Phys.8, 1 (2011) 2011

[3] Webb, D. F. & Howard, T. A. Coronal Mass Ejections: Observations.Living Rev. Sol. Phys.9, 3 (2012) 2012

[4] S.et al.Impact of space weather on climate and habitability of terrestrial- type exoplanets.Int 2020

[5] Lugaz, N.et al.Earth’s magnetosphere and outer radiation belt under sub-Alfv´ enic solar wind.Nat. Commun.7, 13001 (2016) 2016

Receipt and verification

First computed	2026-05-21T02:05:03.373878Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

781c95dbdfd8056064159d4c75f22cb2a0ff0495e65241ab8e2f5536c25e1550

Aliases

arxiv: 2604.23084 · arxiv_version: 2604.23084v1 · doi: 10.48550/arxiv.2604.23084 · pith_short_12: PAOJLW673ACW · pith_short_16: PAOJLW673ACWAZAV · pith_short_8: PAOJLW67

Agent API

Resolver JSON Graph JSON Events JSON Schema Signing key

Verify this Pith Number yourself

curl -sH 'Accept: application/ld+json' https://pith.science/pith/PAOJLW673ACWAZAVTVGHL4RMWK \
  | 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: 781c95dbdfd8056064159d4c75f22cb2a0ff0495e65241ab8e2f5536c25e1550

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "d67a02e1d592784bcfcad5c9d637b493c4d27d112654d88068da298e8bcaaf98",
    "cross_cats_sorted": [],
    "license": "http://creativecommons.org/licenses/by-nc-nd/4.0/",
    "primary_cat": "astro-ph.SR",
    "submitted_at": "2026-04-25T00:36:54Z",
    "title_canon_sha256": "69255c63ef8c6db95c8d567d035b2d4baf86cfe93f6148da408ff2a40115abd0"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2604.23084",
    "kind": "arxiv",
    "version": 1
  }
}