Pith Number

pith:5SBY4LRZ

pith:2026:5SBY4LRZE7VPETLWRNRJMEPFMW

not attested not anchored not stored refs resolved

A view of the evolution of a CME and the associated wave-trains at high spatial and temporal resolution

A. Burtovoi, C. Sasso, F. Frassati, F. Landini, G. Jerse, G. Russano, H. Cremades, L. Abbo, M. Pancrazzi, M. Romoli, M. Temmer, M. Uslenghi, R. Susino, S. Mancuso, V. Andretta, Y. De Leo

High-resolution Metis images reveal distinct plasma motions inside a coronal mass ejection and fast circular wavefronts at 500 km/s on its flank.

arxiv:2604.12836 v1 · 2026-04-14 · astro-ph.SR

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Add to your LaTeX paper

\usepackage{pith}
\pithnumber{5SBY4LRZE7VPETLWRNRJMEPFMW}

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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

Metis observations resolve the CME's fine structure and internal plasma motions. The detection of circular, fast-propagating wavefronts (500 km/s, 3 minute period) at the western flank suggests wave excitation and magnetic reconfiguration processes.

C2weakest assumption

The identification of the wavefronts as quasi-periodic propagating fast modes assumes a specific magnetic field geometry and plasma beta regime in the middle corona that is not directly measured in the data.

C3one line summary

High-resolution coronagraph images resolve CME substructures and fast circular wave-trains interpreted as quasi-periodic propagating fast magnetosonic modes.

References

48 extracted · 48 resolved · 0 Pith anchors

[1] 2025, A&A, 701, A199 2025

[2] 2020, A&A, 642, A10 Auchère, F., Soubrié, E., Pelouze, G., & Buchlin, É 2020

[3] 2025, ApJ, 985, 145 2025

[4] Brueckner, G. E., Howard, R. A., Koomen, M. J., et al. 1995, Sol. Phys., 162, 357 1995

[5] M., Temmer, M., V ourlidas, A., et al 2024

Receipt and verification

First computed	2026-06-10T14:10:49.671816Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

ec838e2e3927eaf24d768b629611e56590695e19b44f9ad0b868e1395f1de1c3

Aliases

arxiv: 2604.12836 · arxiv_version: 2604.12836v1 · doi: 10.48550/arxiv.2604.12836 · pith_short_12: 5SBY4LRZE7VP · pith_short_16: 5SBY4LRZE7VPETLW · pith_short_8: 5SBY4LRZ

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/5SBY4LRZE7VPETLWRNRJMEPFMW \
  | 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: ec838e2e3927eaf24d768b629611e56590695e19b44f9ad0b868e1395f1de1c3

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "d82cb0b07f97b20e2026f53e28b2ee1816a73990ecce195ee15253ffaf5750ef",
    "cross_cats_sorted": [],
    "license": "http://creativecommons.org/licenses/by/4.0/",
    "primary_cat": "astro-ph.SR",
    "submitted_at": "2026-04-14T14:56:30Z",
    "title_canon_sha256": "53ad060fc71e44316b782777c194fbf92dc47f148d8428faefed5b8ab15b771b"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2604.12836",
    "kind": "arxiv",
    "version": 1
  }
}