{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:CROW2YQ4IST7WEWBGWZGG3TNAD","short_pith_number":"pith:CROW2YQ4","schema_version":"1.0","canonical_sha256":"145d6d621c44a7fb12c135b2636e6d00da7904d9cd28ca8b37113e171bd6eff4","source":{"kind":"arxiv","id":"1110.5901","version":1},"attestation_state":"computed","paper":{"title":"Analytic and numerical models of the 3D multipolar magnetospheres of pre-main sequence stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"(2) Toulouse), J.-F. Donati (2) ((1) Caltech, S. G. Gregory (1)","submitted_at":"2011-10-26T19:57:16Z","abstract_excerpt":"Traditionally models of accretion of gas on to T Tauri stars have assumed a dipole stellar magnetosphere, partly for simplicity, but also due to the lack of information about their true magnetic field topologies. Before and since the first magnetic maps of an accreting T Tauri star were published in 2007 a new generation of magnetospheric accretion models have been developed that incorporate multipole magnetic fields. Three-dimensional models of the large-scale stellar magnetosphere with an observed degree of complexity have been produced via numerical field extrapolation from observationally "},"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":"1110.5901","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-10-26T19:57:16Z","cross_cats_sorted":[],"title_canon_sha256":"3f4e6d124e1000b6d1ba200c971017cb420c30c11f871a4ba04837df94529ad7","abstract_canon_sha256":"065934746d86c569c1eb77452893ac223bc516c1e654902c719998c3335344b3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:00:03.452828Z","signature_b64":"hQHaO94auAsytcQWZvt/XGt80kmEWaUhQCL24d46UVysEVoumsTE8JYjKMhjlSt9/vifqNWel0EXeYDb+bOYCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"145d6d621c44a7fb12c135b2636e6d00da7904d9cd28ca8b37113e171bd6eff4","last_reissued_at":"2026-05-18T02:00:03.452338Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:00:03.452338Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Analytic and numerical models of the 3D multipolar magnetospheres of pre-main sequence stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"(2) Toulouse), J.-F. Donati (2) ((1) Caltech, S. G. Gregory (1)","submitted_at":"2011-10-26T19:57:16Z","abstract_excerpt":"Traditionally models of accretion of gas on to T Tauri stars have assumed a dipole stellar magnetosphere, partly for simplicity, but also due to the lack of information about their true magnetic field topologies. Before and since the first magnetic maps of an accreting T Tauri star were published in 2007 a new generation of magnetospheric accretion models have been developed that incorporate multipole magnetic fields. Three-dimensional models of the large-scale stellar magnetosphere with an observed degree of complexity have been produced via numerical field extrapolation from observationally "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1110.5901","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":"1110.5901","created_at":"2026-05-18T02:00:03.452417+00:00"},{"alias_kind":"arxiv_version","alias_value":"1110.5901v1","created_at":"2026-05-18T02:00:03.452417+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1110.5901","created_at":"2026-05-18T02:00:03.452417+00:00"},{"alias_kind":"pith_short_12","alias_value":"CROW2YQ4IST7","created_at":"2026-05-18T12:26:26.731475+00:00"},{"alias_kind":"pith_short_16","alias_value":"CROW2YQ4IST7WEWB","created_at":"2026-05-18T12:26:26.731475+00:00"},{"alias_kind":"pith_short_8","alias_value":"CROW2YQ4","created_at":"2026-05-18T12:26:26.731475+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/CROW2YQ4IST7WEWBGWZGG3TNAD","json":"https://pith.science/pith/CROW2YQ4IST7WEWBGWZGG3TNAD.json","graph_json":"https://pith.science/api/pith-number/CROW2YQ4IST7WEWBGWZGG3TNAD/graph.json","events_json":"https://pith.science/api/pith-number/CROW2YQ4IST7WEWBGWZGG3TNAD/events.json","paper":"https://pith.science/paper/CROW2YQ4"},"agent_actions":{"view_html":"https://pith.science/pith/CROW2YQ4IST7WEWBGWZGG3TNAD","download_json":"https://pith.science/pith/CROW2YQ4IST7WEWBGWZGG3TNAD.json","view_paper":"https://pith.science/paper/CROW2YQ4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1110.5901&json=true","fetch_graph":"https://pith.science/api/pith-number/CROW2YQ4IST7WEWBGWZGG3TNAD/graph.json","fetch_events":"https://pith.science/api/pith-number/CROW2YQ4IST7WEWBGWZGG3TNAD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CROW2YQ4IST7WEWBGWZGG3TNAD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CROW2YQ4IST7WEWBGWZGG3TNAD/action/storage_attestation","attest_author":"https://pith.science/pith/CROW2YQ4IST7WEWBGWZGG3TNAD/action/author_attestation","sign_citation":"https://pith.science/pith/CROW2YQ4IST7WEWBGWZGG3TNAD/action/citation_signature","submit_replication":"https://pith.science/pith/CROW2YQ4IST7WEWBGWZGG3TNAD/action/replication_record"}},"created_at":"2026-05-18T02:00:03.452417+00:00","updated_at":"2026-05-18T02:00:03.452417+00:00"}