{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:7XHPE5CEVCTGSMS3HOEYPRKMW5","short_pith_number":"pith:7XHPE5CE","schema_version":"1.0","canonical_sha256":"fdcef27444a8a669325b3b8987c54cb75fa32aab069dd6a6692dfc3ed24bd54d","source":{"kind":"arxiv","id":"2303.06465","version":1},"attestation_state":"computed","paper":{"title":"The S-Web Origin of Composition Enhancement in the Slow-to-Moderate Speed Solar Wind","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"A. K. Higginson, B. J. Lynch, L. Zhao, N. M. Viall, S. T. Lepri, X. Sun","submitted_at":"2023-03-11T17:30:43Z","abstract_excerpt":"Connecting the solar wind observed throughout the heliosphere to its origins in the solar corona is one of the central aims of heliophysics. The variability in the magnetic field, bulk plasma, and heavy ion composition properties of the slow wind are thought to result from magnetic reconnection processes in the solar corona. We identify regions of enhanced variability and composition in the solar wind from 2003 April 15 to May 13 (Carrington Rotation 2002), observed by the Wind and Advanced Composition Explorer spacecraft, and demonstrate their relationship to the Separatrix-Web (S-Web) struct"},"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":"2303.06465","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2023-03-11T17:30:43Z","cross_cats_sorted":["physics.space-ph"],"title_canon_sha256":"fbfa89e68d92b7df507576af2ae1770d519d076311965780cd2d718727085d67","abstract_canon_sha256":"dc43b2c32d0e7c6613152cd120c729c259d6fc946f3964e47adfef6e039cde29"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:13:38.679133Z","signature_b64":"qSsgdCh2Ykm7rw3hgt2uI6YDZlCUrk9p3Ed2/dZw6g+tgSWPTFZaUKzC4/2kdFQsOj+cS1zKckmlaY/ip9T5Dg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fdcef27444a8a669325b3b8987c54cb75fa32aab069dd6a6692dfc3ed24bd54d","last_reissued_at":"2026-07-05T06:13:38.678629Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:13:38.678629Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The S-Web Origin of Composition Enhancement in the Slow-to-Moderate Speed Solar Wind","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"A. K. Higginson, B. J. Lynch, L. Zhao, N. M. Viall, S. T. Lepri, X. Sun","submitted_at":"2023-03-11T17:30:43Z","abstract_excerpt":"Connecting the solar wind observed throughout the heliosphere to its origins in the solar corona is one of the central aims of heliophysics. The variability in the magnetic field, bulk plasma, and heavy ion composition properties of the slow wind are thought to result from magnetic reconnection processes in the solar corona. We identify regions of enhanced variability and composition in the solar wind from 2003 April 15 to May 13 (Carrington Rotation 2002), observed by the Wind and Advanced Composition Explorer spacecraft, and demonstrate their relationship to the Separatrix-Web (S-Web) struct"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2303.06465","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/2303.06465/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":"2303.06465","created_at":"2026-07-05T06:13:38.678691+00:00"},{"alias_kind":"arxiv_version","alias_value":"2303.06465v1","created_at":"2026-07-05T06:13:38.678691+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2303.06465","created_at":"2026-07-05T06:13:38.678691+00:00"},{"alias_kind":"pith_short_12","alias_value":"7XHPE5CEVCTG","created_at":"2026-07-05T06:13:38.678691+00:00"},{"alias_kind":"pith_short_16","alias_value":"7XHPE5CEVCTGSMS3","created_at":"2026-07-05T06:13:38.678691+00:00"},{"alias_kind":"pith_short_8","alias_value":"7XHPE5CE","created_at":"2026-07-05T06:13:38.678691+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/7XHPE5CEVCTGSMS3HOEYPRKMW5","json":"https://pith.science/pith/7XHPE5CEVCTGSMS3HOEYPRKMW5.json","graph_json":"https://pith.science/api/pith-number/7XHPE5CEVCTGSMS3HOEYPRKMW5/graph.json","events_json":"https://pith.science/api/pith-number/7XHPE5CEVCTGSMS3HOEYPRKMW5/events.json","paper":"https://pith.science/paper/7XHPE5CE"},"agent_actions":{"view_html":"https://pith.science/pith/7XHPE5CEVCTGSMS3HOEYPRKMW5","download_json":"https://pith.science/pith/7XHPE5CEVCTGSMS3HOEYPRKMW5.json","view_paper":"https://pith.science/paper/7XHPE5CE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2303.06465&json=true","fetch_graph":"https://pith.science/api/pith-number/7XHPE5CEVCTGSMS3HOEYPRKMW5/graph.json","fetch_events":"https://pith.science/api/pith-number/7XHPE5CEVCTGSMS3HOEYPRKMW5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7XHPE5CEVCTGSMS3HOEYPRKMW5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7XHPE5CEVCTGSMS3HOEYPRKMW5/action/storage_attestation","attest_author":"https://pith.science/pith/7XHPE5CEVCTGSMS3HOEYPRKMW5/action/author_attestation","sign_citation":"https://pith.science/pith/7XHPE5CEVCTGSMS3HOEYPRKMW5/action/citation_signature","submit_replication":"https://pith.science/pith/7XHPE5CEVCTGSMS3HOEYPRKMW5/action/replication_record"}},"created_at":"2026-07-05T06:13:38.678691+00:00","updated_at":"2026-07-05T06:13:38.678691+00:00"}