{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:BYUKZCKBSOPYRJITMLJMU7SI3E","short_pith_number":"pith:BYUKZCKB","schema_version":"1.0","canonical_sha256":"0e28ac8941939f88a51362d2ca7e48d922d724684f5e75af0abb85daf1fbfcb3","source":{"kind":"arxiv","id":"2405.07755","version":1},"attestation_state":"computed","paper":{"title":"Searching for evidence of subchromospheric magnetic reconnection on the Sun","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. S. H. To, A. W. James, D. Baker, D. H. Brooks, D. M. Long, G. Valori, H. Kuniyoshi, J. McKevitt, J. M. Laming, L. M. Green, L. van Driel-Gesztelyi, M. Murabito, P. Demoulin, S. A. Matthews, S. L. Yardley, T. Mihailescu","submitted_at":"2024-05-13T13:53:36Z","abstract_excerpt":"Within the coronae of stars, abundances of those elements with low first ionization potential (FIP) often differ from their photospheric values. The coronae of the Sun and solar-type stars mostly show enhancements of low-FIP elements (the FIP effect) while more active stars such as M dwarfs have coronae generally characterized by the inverse-FIP (I-FIP) effect. Highly localized regions of I-FIP effect solar plasma have been observed by Hinode/EIS in a number of highly complex active regions, usually around strong light bridges of the umbrae of coalescing/merging sunspots. These observations ca"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2405.07755","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2024-05-13T13:53:36Z","cross_cats_sorted":[],"title_canon_sha256":"9b02b4d875e0141f21738778c50f1b33757619d185d55b5396d1501f54cafb1e","abstract_canon_sha256":"3e8f0220de677c9ff68fc9fe20bb2eeb74e399c223532c5599968361e2506aa8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:18:34.234453Z","signature_b64":"ZcWxh8Yvi4ZwAv7jwjF3vJqVg9GwqFv1u/23G5eUAEKmsy0H07+bOvdG+00hb+kQyUgEDb/FGPvPGdLPm+1PCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0e28ac8941939f88a51362d2ca7e48d922d724684f5e75af0abb85daf1fbfcb3","last_reissued_at":"2026-07-05T08:18:34.233882Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:18:34.233882Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Searching for evidence of subchromospheric magnetic reconnection on the Sun","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. S. H. To, A. W. James, D. Baker, D. H. Brooks, D. M. Long, G. Valori, H. Kuniyoshi, J. McKevitt, J. M. Laming, L. M. Green, L. van Driel-Gesztelyi, M. Murabito, P. Demoulin, S. A. Matthews, S. L. Yardley, T. Mihailescu","submitted_at":"2024-05-13T13:53:36Z","abstract_excerpt":"Within the coronae of stars, abundances of those elements with low first ionization potential (FIP) often differ from their photospheric values. The coronae of the Sun and solar-type stars mostly show enhancements of low-FIP elements (the FIP effect) while more active stars such as M dwarfs have coronae generally characterized by the inverse-FIP (I-FIP) effect. Highly localized regions of I-FIP effect solar plasma have been observed by Hinode/EIS in a number of highly complex active regions, usually around strong light bridges of the umbrae of coalescing/merging sunspots. These observations ca"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2405.07755","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2405.07755/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"2405.07755","created_at":"2026-07-05T08:18:34.233941+00:00"},{"alias_kind":"arxiv_version","alias_value":"2405.07755v1","created_at":"2026-07-05T08:18:34.233941+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2405.07755","created_at":"2026-07-05T08:18:34.233941+00:00"},{"alias_kind":"pith_short_12","alias_value":"BYUKZCKBSOPY","created_at":"2026-07-05T08:18:34.233941+00:00"},{"alias_kind":"pith_short_16","alias_value":"BYUKZCKBSOPYRJIT","created_at":"2026-07-05T08:18:34.233941+00:00"},{"alias_kind":"pith_short_8","alias_value":"BYUKZCKB","created_at":"2026-07-05T08:18:34.233941+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BYUKZCKBSOPYRJITMLJMU7SI3E","json":"https://pith.science/pith/BYUKZCKBSOPYRJITMLJMU7SI3E.json","graph_json":"https://pith.science/api/pith-number/BYUKZCKBSOPYRJITMLJMU7SI3E/graph.json","events_json":"https://pith.science/api/pith-number/BYUKZCKBSOPYRJITMLJMU7SI3E/events.json","paper":"https://pith.science/paper/BYUKZCKB"},"agent_actions":{"view_html":"https://pith.science/pith/BYUKZCKBSOPYRJITMLJMU7SI3E","download_json":"https://pith.science/pith/BYUKZCKBSOPYRJITMLJMU7SI3E.json","view_paper":"https://pith.science/paper/BYUKZCKB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2405.07755&json=true","fetch_graph":"https://pith.science/api/pith-number/BYUKZCKBSOPYRJITMLJMU7SI3E/graph.json","fetch_events":"https://pith.science/api/pith-number/BYUKZCKBSOPYRJITMLJMU7SI3E/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BYUKZCKBSOPYRJITMLJMU7SI3E/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BYUKZCKBSOPYRJITMLJMU7SI3E/action/storage_attestation","attest_author":"https://pith.science/pith/BYUKZCKBSOPYRJITMLJMU7SI3E/action/author_attestation","sign_citation":"https://pith.science/pith/BYUKZCKBSOPYRJITMLJMU7SI3E/action/citation_signature","submit_replication":"https://pith.science/pith/BYUKZCKBSOPYRJITMLJMU7SI3E/action/replication_record"}},"created_at":"2026-07-05T08:18:34.233941+00:00","updated_at":"2026-07-05T08:18:34.233941+00:00"}