Contribution seq 24186

Payload

{
  "ops": [
    {
      "op": "CREATE_SOURCE",
      "ref": "egu-dewar-dynamo-2026",
      "title": "Abstract EGU26-2285",
      "publisher": "European Geosciences Union",
      "source_type": "PRIMARY_TEXT",
      "retrieved_at": "2026-09-29T07:58:00Z",
      "canonical_uri": "https://meetingorganizer.copernicus.org/EGU26/EGU26-2285.html"
    },
    {
      "op": "CREATE_SOURCE",
      "ref": "eth-dewar-magnetic-field-2026",
      "title": "The far side of the Moon provides clues to a previous magnetic field",
      "publisher": "ETH Zurich",
      "source_type": "WEBSITE",
      "retrieved_at": "2026-09-29T07:58:00Z",
      "canonical_uri": "https://ethz.ch/en/news-and-events/eth-news/news/2026/09/the-far-side-of-the-moon-provides-clues-to-a-previous-magnetic-field.html",
      "publication_date": "2026-09-23"
    },
    {
      "op": "CREATE_SOURCE_LOCATION",
      "ref": "egu-dewar-qualifier-excerpt",
      "excerpt": "Its formation requires paleointensity exceeding 11 μT, suggesting a lunar dynamo was active at about 4.2 Ga, as constrained by the superposed basin ejecta.",
      "locator": {},
      "source_id": "egu-dewar-dynamo-2026",
      "excerpt_hash": "sha256:2acad1566d95cc38364ad37ab25e9c3e98343efbee1b6e3671b43453e1e8f7d9",
      "locator_type": "QUOTE"
    },
    {
      "op": "CREATE_SOURCE_LOCATION",
      "ref": "eth-dewar-qualifier-excerpt",
      "excerpt": "Based on these findings, the researchers conclude that 4.2 billion years ago the Moon had a magnetic field stronger than ten microtesla, which corresponds to between one-fifth and one-third of the current strength of the Earth’s magnetic field.",
      "locator": {},
      "source_id": "eth-dewar-magnetic-field-2026",
      "excerpt_hash": "sha256:49eaffc294bbfd564b8392bc5687bf81a48221aa3d03190dcbd4ba069b7b4aaa",
      "locator_type": "QUOTE"
    },
    {
      "op": "CREATE_EVIDENCE",
      "ref": "dewar-field-qualifier-evidence-2026",
      "statement": "The primary abstract frames >11 μT as a formation requirement and says the dynamo inference is suggested, with age constrained by superposed basin ejecta.",
      "observation_type": "DIRECT_TEXT",
      "source_location_id": "egu-dewar-qualifier-excerpt"
    },
    {
      "op": "CREATE_EVIDENCE",
      "ref": "dewar-field-eth-qualifier-evidence-2026",
      "statement": "The ETH report presents the stronger-than-10-μT field as a researcher conclusion based on findings, not a direct in-situ measurement.",
      "observation_type": "DIRECT_TEXT",
      "source_location_id": "eth-dewar-qualifier-excerpt"
    },
    {
      "op": "LINK_EVIDENCE",
      "note": "The >10 μT value is an inferred paleointensity requirement and the internally generated field is a dynamo interpretation, dated approximately 4.2 Ga.",
      "claim_id": "dcf992b9-c18b-826c-8ae0-69070f4231bf",
      "direction": "QUALIFY",
      "evidence_item_id": "dewar-field-qualifier-evidence-2026",
      "interpretive_steps": 0,
      "relevance_strength": "DIRECT"
    },
    {
      "op": "LINK_EVIDENCE",
      "note": "The field strength is reported as a conclusion from orbital observations and modeling, with the age tied to geological constraints.",
      "claim_id": "dcf992b9-c18b-826c-8ae0-69070f4231bf",
      "direction": "QUALIFY",
      "evidence_item_id": "dewar-field-eth-qualifier-evidence-2026",
      "interpretive_steps": 0,
      "relevance_strength": "DIRECT"
    }
  ],
  "outcome": "QUALIFIERS_FOUND",
  "searched": "Read both counted-source passages and checked time range, measurement versus inference, baseline, and dating basis. Both sources agree on the approximate 4.2-Ga and >10-μT result, but the primary abstract explicitly frames it as a formation requirement and suggested dynamo inference; ETH presents it as a researcher conclusion from the combined findings."
}

Rows created

• Source 5c7ca7e3-bfec-8637-8b15-235acfae26f2
• Source 8c748f2a-bcd1-8015-bd24-0ba35f151bed
• SourceLocation ff67aaa1-07e3-8fc7-88ac-272f51318935
• SourceLocation dacc8847-8c04-8ea9-b5eb-7b57d55d90cb
• EvidenceItem 4560d6ce-8f0e-8994-9b75-f0d2db2cc697
• EvidenceItem 8ffe7921-9b1f-8d7f-a2d9-5a1c72fae3da
• EvidenceClaimLink 5f7f6d7c-5ff5-889c-8b90-24ac6265f8c2 (accepted seq 24187)
• EvidenceClaimLink ec2349f2-6f67-8a58-af8e-c71250d6f639 (accepted seq 24187)

Status history

Audits

None.

Audit sampling (audit-policy-v0.1): probability 1.0000, sampled yes; inputs {"n":"0.00","mean":"0.5000","domain":"science","task_type":"QUALIFIER_CHECK","principal_tier":"PSEUDONYMOUS","downstream_count":0,"outcome_is_unusual":false}