{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:OFD4H2WJWTLZSB4WQ6AKSH7XWT","short_pith_number":"pith:OFD4H2WJ","schema_version":"1.0","canonical_sha256":"7147c3eac9b4d79907968780a91ff7b4f0319047e310f023eec88e032fda1998","source":{"kind":"arxiv","id":"1401.4761","version":1},"attestation_state":"computed","paper":{"title":"Simulations of Accretion onto Magnetized Stars: Results of 3D MHD Simulations and 3D Radiative Transfer","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Marina Romanova, Ryuichi Kurosawa","submitted_at":"2014-01-20T00:22:39Z","abstract_excerpt":"We discuss the results of modelling of young magnetized stars, where matter flow is calculated using the three-dimensional (3D) magneto-hydrodynamic (MHD) \"Cubed Sphere\" code, and the spectra are calculated using the 3D Monte Carlo radiative transfer code \"TORUS\". Two examples of modelling are shown: (1) accretion onto stars in stable and unstable regimes, and (2) accretion to a young star V2129 Oph, modelled with realistic parameters."},"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":"1401.4761","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-01-20T00:22:39Z","cross_cats_sorted":[],"title_canon_sha256":"1aa6cdd645c1bbadcb60a241022c3030d252c037842b14238ee4902fef390244","abstract_canon_sha256":"dfd0d0f3ef0c014e2266564fecf99406d0f9dcd27c1b153d4eac0346a50e7061"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:01:44.695077Z","signature_b64":"ShhfcAUDW3EA1dI7d1nNSivKYmkO0UF/1sioPFy52GeOBM/zGfEDMX2HizDnvBr8YU9fnoAXHuNxGK5QWXQhBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7147c3eac9b4d79907968780a91ff7b4f0319047e310f023eec88e032fda1998","last_reissued_at":"2026-05-18T03:01:44.694494Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:01:44.694494Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Simulations of Accretion onto Magnetized Stars: Results of 3D MHD Simulations and 3D Radiative Transfer","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Marina Romanova, Ryuichi Kurosawa","submitted_at":"2014-01-20T00:22:39Z","abstract_excerpt":"We discuss the results of modelling of young magnetized stars, where matter flow is calculated using the three-dimensional (3D) magneto-hydrodynamic (MHD) \"Cubed Sphere\" code, and the spectra are calculated using the 3D Monte Carlo radiative transfer code \"TORUS\". Two examples of modelling are shown: (1) accretion onto stars in stable and unstable regimes, and (2) accretion to a young star V2129 Oph, modelled with realistic parameters."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1401.4761","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":"1401.4761","created_at":"2026-05-18T03:01:44.694593+00:00"},{"alias_kind":"arxiv_version","alias_value":"1401.4761v1","created_at":"2026-05-18T03:01:44.694593+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1401.4761","created_at":"2026-05-18T03:01:44.694593+00:00"},{"alias_kind":"pith_short_12","alias_value":"OFD4H2WJWTLZ","created_at":"2026-05-18T12:28:41.024544+00:00"},{"alias_kind":"pith_short_16","alias_value":"OFD4H2WJWTLZSB4W","created_at":"2026-05-18T12:28:41.024544+00:00"},{"alias_kind":"pith_short_8","alias_value":"OFD4H2WJ","created_at":"2026-05-18T12:28:41.024544+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/OFD4H2WJWTLZSB4WQ6AKSH7XWT","json":"https://pith.science/pith/OFD4H2WJWTLZSB4WQ6AKSH7XWT.json","graph_json":"https://pith.science/api/pith-number/OFD4H2WJWTLZSB4WQ6AKSH7XWT/graph.json","events_json":"https://pith.science/api/pith-number/OFD4H2WJWTLZSB4WQ6AKSH7XWT/events.json","paper":"https://pith.science/paper/OFD4H2WJ"},"agent_actions":{"view_html":"https://pith.science/pith/OFD4H2WJWTLZSB4WQ6AKSH7XWT","download_json":"https://pith.science/pith/OFD4H2WJWTLZSB4WQ6AKSH7XWT.json","view_paper":"https://pith.science/paper/OFD4H2WJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1401.4761&json=true","fetch_graph":"https://pith.science/api/pith-number/OFD4H2WJWTLZSB4WQ6AKSH7XWT/graph.json","fetch_events":"https://pith.science/api/pith-number/OFD4H2WJWTLZSB4WQ6AKSH7XWT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OFD4H2WJWTLZSB4WQ6AKSH7XWT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OFD4H2WJWTLZSB4WQ6AKSH7XWT/action/storage_attestation","attest_author":"https://pith.science/pith/OFD4H2WJWTLZSB4WQ6AKSH7XWT/action/author_attestation","sign_citation":"https://pith.science/pith/OFD4H2WJWTLZSB4WQ6AKSH7XWT/action/citation_signature","submit_replication":"https://pith.science/pith/OFD4H2WJWTLZSB4WQ6AKSH7XWT/action/replication_record"}},"created_at":"2026-05-18T03:01:44.694593+00:00","updated_at":"2026-05-18T03:01:44.694593+00:00"}