Pith Number

pith:I3AHHIIL

pith:2026:I3AHHIILSCYHPVJXQKH337TU5H

not attested not anchored not stored refs resolved

Detector for fast wave trains in the solar radio emission

A. V. Mikhalchuk, E. G. Kupriyanova, V. A. Dmitriev

Neural network detector identifies 50 candidate fast wave trains in solar radio spectra

arxiv:2605.13728 v1 · 2026-05-13 · astro-ph.SR

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\usepackage{pith}
\pithnumber{I3AHHIILSCYHPVJXQKH337TU5H}

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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

Our automatic detector revealed 50 independent QFP-candidates events with the temporal signatures similar to that of the fast wave trains, with 13 candidates connected with the global waves.

C2weakest assumption

The neural network classifier correctly identifies true QFP wave trains based on temporal signatures in radio spectra, with the 50 global EUV waves serving as reliable independent markers for targeted search.

C3one line summary

A neural network detector applied to 2011 solar radio spectra identified 50 QFP wave train candidates, with 13 associated with global coronal EUV waves.

References

64 extracted · 64 resolved · 0 Pith anchors

[2] 2023 Requirements for Progress in Understanding Solar Flare Energy Transport: The Impulsive Phase 2023 · doi:10.3847/25c2cfeb.701e4c96

[3] 2025 UK White Paper on Magnetic Reconnection 2025 · doi:10.48550/arxiv.2512.11631

[4] 2025 Understanding Solar Flares and Energetic Events: Open questions, observational requirements, and instrumental needs over the coming decade 2025 · doi:10.48550/arxiv.2512.24479

[5] 1958a Magneto-Hydrostatic Equilibrium in an External Magnetic Field

[6] 1958b The production of high energy particles in solar flares.Il Nuovo Cimento8, 188–196 · doi:10.1007/bf02962520

Formal links

2 machine-checked theorem links

Receipt and verification

First computed	2026-05-18T02:44:16.586625Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

46c073a10b90b077d537828fbdfe74e9e5821c0d4fc641d67709df1666eeb571

Aliases

arxiv: 2605.13728 · arxiv_version: 2605.13728v1 · doi: 10.48550/arxiv.2605.13728 · pith_short_12: I3AHHIILSCYH · pith_short_16: I3AHHIILSCYHPVJX · pith_short_8: I3AHHIIL

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/I3AHHIILSCYHPVJXQKH337TU5H \
  | 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: 46c073a10b90b077d537828fbdfe74e9e5821c0d4fc641d67709df1666eeb571

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "f1a3d90dbc28f2dee0350ae70d12051e0bd5c773b883cd80b001625a74bf323f",
    "cross_cats_sorted": [],
    "license": "http://creativecommons.org/publicdomain/zero/1.0/",
    "primary_cat": "astro-ph.SR",
    "submitted_at": "2026-05-13T16:08:23Z",
    "title_canon_sha256": "608a0ccc61a5bde76844e8d041a4306539d1d56a3de2ad5c9deec5eed6a5946c"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2605.13728",
    "kind": "arxiv",
    "version": 1
  }
}