{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:ZUDZW6HILLQBDQQZTQDQMXJACA","short_pith_number":"pith:ZUDZW6HI","schema_version":"1.0","canonical_sha256":"cd079b78e85ae011c2199c07065d20101c0bf20a7143b02eb00c1d6218890065","source":{"kind":"arxiv","id":"1710.02908","version":1},"attestation_state":"computed","paper":{"title":"Global solar magnetic field organization in the outer corona: influence on the solar wind speed and mass flux over the cycle","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Allan Sacha Brun, Victor R\\'eville","submitted_at":"2017-10-09T01:59:29Z","abstract_excerpt":"The dynamics of the solar wind depends intrinsically on the structure of the global solar magnetic field, which undergoes fundamental changes over the 11-yr solar cycle. For instance, the wind terminal velocity is thought to be anti-correlated with the expansion factor, a measure of how the magnetic field varies with height in the solar corona, usually computed at a fixed height ($\\approx 2.5 R_{\\odot}$, the source surface radius which approximates the distance at which all magnetic field lines become open). However, the magnetic field expansion affects the solar wind in a more detailed way, i"},"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":"1710.02908","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-10-09T01:59:29Z","cross_cats_sorted":[],"title_canon_sha256":"05670959ce7e93d55a7fa842de91ea57bd51c539f27f6189496f33c03ebc53bd","abstract_canon_sha256":"7add942135548e75b7d87a76a0cdcc4ce10d4eb017caa9fd2f57067fe0a17fa1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:29:28.140080Z","signature_b64":"iTWlgKXmRgHRqaGgTCaWbF+KKygZkg1tCGR2Z18tddMuyO4I8yaEjqZvSVQQBQgR8AilXxfbLE6dqJkcRueNAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cd079b78e85ae011c2199c07065d20101c0bf20a7143b02eb00c1d6218890065","last_reissued_at":"2026-05-18T00:29:28.139528Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:29:28.139528Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Global solar magnetic field organization in the outer corona: influence on the solar wind speed and mass flux over the cycle","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Allan Sacha Brun, Victor R\\'eville","submitted_at":"2017-10-09T01:59:29Z","abstract_excerpt":"The dynamics of the solar wind depends intrinsically on the structure of the global solar magnetic field, which undergoes fundamental changes over the 11-yr solar cycle. For instance, the wind terminal velocity is thought to be anti-correlated with the expansion factor, a measure of how the magnetic field varies with height in the solar corona, usually computed at a fixed height ($\\approx 2.5 R_{\\odot}$, the source surface radius which approximates the distance at which all magnetic field lines become open). However, the magnetic field expansion affects the solar wind in a more detailed way, i"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1710.02908","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":""},"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":"1710.02908","created_at":"2026-05-18T00:29:28.139597+00:00"},{"alias_kind":"arxiv_version","alias_value":"1710.02908v1","created_at":"2026-05-18T00:29:28.139597+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1710.02908","created_at":"2026-05-18T00:29:28.139597+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZUDZW6HILLQB","created_at":"2026-05-18T12:31:59.375834+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZUDZW6HILLQBDQQZ","created_at":"2026-05-18T12:31:59.375834+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZUDZW6HI","created_at":"2026-05-18T12:31:59.375834+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/ZUDZW6HILLQBDQQZTQDQMXJACA","json":"https://pith.science/pith/ZUDZW6HILLQBDQQZTQDQMXJACA.json","graph_json":"https://pith.science/api/pith-number/ZUDZW6HILLQBDQQZTQDQMXJACA/graph.json","events_json":"https://pith.science/api/pith-number/ZUDZW6HILLQBDQQZTQDQMXJACA/events.json","paper":"https://pith.science/paper/ZUDZW6HI"},"agent_actions":{"view_html":"https://pith.science/pith/ZUDZW6HILLQBDQQZTQDQMXJACA","download_json":"https://pith.science/pith/ZUDZW6HILLQBDQQZTQDQMXJACA.json","view_paper":"https://pith.science/paper/ZUDZW6HI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1710.02908&json=true","fetch_graph":"https://pith.science/api/pith-number/ZUDZW6HILLQBDQQZTQDQMXJACA/graph.json","fetch_events":"https://pith.science/api/pith-number/ZUDZW6HILLQBDQQZTQDQMXJACA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZUDZW6HILLQBDQQZTQDQMXJACA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZUDZW6HILLQBDQQZTQDQMXJACA/action/storage_attestation","attest_author":"https://pith.science/pith/ZUDZW6HILLQBDQQZTQDQMXJACA/action/author_attestation","sign_citation":"https://pith.science/pith/ZUDZW6HILLQBDQQZTQDQMXJACA/action/citation_signature","submit_replication":"https://pith.science/pith/ZUDZW6HILLQBDQQZTQDQMXJACA/action/replication_record"}},"created_at":"2026-05-18T00:29:28.139597+00:00","updated_at":"2026-05-18T00:29:28.139597+00:00"}