{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:3IBO4MJSRGSUBAEYO3NPZ2WTYH","short_pith_number":"pith:3IBO4MJS","schema_version":"1.0","canonical_sha256":"da02ee313289a540809876dafcead3c1ce5e402f944aec9cf2a232c275934b08","source":{"kind":"arxiv","id":"1711.11287","version":1},"attestation_state":"computed","paper":{"title":"Winds of Massive Magnetic Stars: Interacting Fields and Flow","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Ian Stevens, Simon Daley-Yates","submitted_at":"2017-11-30T09:45:19Z","abstract_excerpt":"We present results of 3D numerical simulations of magnetically confined, radiatively driven stellar winds of massive stars, conducted using the astrophysical MHD code Pluto, with a focus on understanding the rotational variability of radio and sub-mm emission. Radiative driving is implemented according to the Castor, Abbott and Klein theory of radiatively driven winds. Many magnetic massive stars posses a magnetic axis which is inclined with respect to the rotational axis. This misalignment leads to a complex wind structure as magnetic confinement, centrifugal acceleration and radiative drivin"},"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":"1711.11287","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-11-30T09:45:19Z","cross_cats_sorted":[],"title_canon_sha256":"4ff2900b3d0cd12a75374768c9a6125d916f797c6dc74dece83c9e321bf8fd04","abstract_canon_sha256":"7d1071fa1ecfe9c85164d25e1c38f0c2e59a45273a168b24d2c8d386f2edcc1f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:29:11.952142Z","signature_b64":"IOj5837q5rjvUokZ3bGt91UUTJbEm+DqdxIBS3rYoXS90LU3yOI2a07EIKjHT3Y+nopVQU0XPKrj4lP+FkM0DQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"da02ee313289a540809876dafcead3c1ce5e402f944aec9cf2a232c275934b08","last_reissued_at":"2026-05-18T00:29:11.951487Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:29:11.951487Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Winds of Massive Magnetic Stars: Interacting Fields and Flow","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Ian Stevens, Simon Daley-Yates","submitted_at":"2017-11-30T09:45:19Z","abstract_excerpt":"We present results of 3D numerical simulations of magnetically confined, radiatively driven stellar winds of massive stars, conducted using the astrophysical MHD code Pluto, with a focus on understanding the rotational variability of radio and sub-mm emission. Radiative driving is implemented according to the Castor, Abbott and Klein theory of radiatively driven winds. Many magnetic massive stars posses a magnetic axis which is inclined with respect to the rotational axis. This misalignment leads to a complex wind structure as magnetic confinement, centrifugal acceleration and radiative drivin"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.11287","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":"1711.11287","created_at":"2026-05-18T00:29:11.951601+00:00"},{"alias_kind":"arxiv_version","alias_value":"1711.11287v1","created_at":"2026-05-18T00:29:11.951601+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.11287","created_at":"2026-05-18T00:29:11.951601+00:00"},{"alias_kind":"pith_short_12","alias_value":"3IBO4MJSRGSU","created_at":"2026-05-18T12:30:58.224056+00:00"},{"alias_kind":"pith_short_16","alias_value":"3IBO4MJSRGSUBAEY","created_at":"2026-05-18T12:30:58.224056+00:00"},{"alias_kind":"pith_short_8","alias_value":"3IBO4MJS","created_at":"2026-05-18T12:30:58.224056+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/3IBO4MJSRGSUBAEYO3NPZ2WTYH","json":"https://pith.science/pith/3IBO4MJSRGSUBAEYO3NPZ2WTYH.json","graph_json":"https://pith.science/api/pith-number/3IBO4MJSRGSUBAEYO3NPZ2WTYH/graph.json","events_json":"https://pith.science/api/pith-number/3IBO4MJSRGSUBAEYO3NPZ2WTYH/events.json","paper":"https://pith.science/paper/3IBO4MJS"},"agent_actions":{"view_html":"https://pith.science/pith/3IBO4MJSRGSUBAEYO3NPZ2WTYH","download_json":"https://pith.science/pith/3IBO4MJSRGSUBAEYO3NPZ2WTYH.json","view_paper":"https://pith.science/paper/3IBO4MJS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1711.11287&json=true","fetch_graph":"https://pith.science/api/pith-number/3IBO4MJSRGSUBAEYO3NPZ2WTYH/graph.json","fetch_events":"https://pith.science/api/pith-number/3IBO4MJSRGSUBAEYO3NPZ2WTYH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3IBO4MJSRGSUBAEYO3NPZ2WTYH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3IBO4MJSRGSUBAEYO3NPZ2WTYH/action/storage_attestation","attest_author":"https://pith.science/pith/3IBO4MJSRGSUBAEYO3NPZ2WTYH/action/author_attestation","sign_citation":"https://pith.science/pith/3IBO4MJSRGSUBAEYO3NPZ2WTYH/action/citation_signature","submit_replication":"https://pith.science/pith/3IBO4MJSRGSUBAEYO3NPZ2WTYH/action/replication_record"}},"created_at":"2026-05-18T00:29:11.951601+00:00","updated_at":"2026-05-18T00:29:11.951601+00:00"}