{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:RKTJ6ZQ4ANMSQ7AQBKTQSJ3DYX","short_pith_number":"pith:RKTJ6ZQ4","schema_version":"1.0","canonical_sha256":"8aa69f661c0359287c100aa7092763c5f101017c0bfe2612eabc18bb813e31b4","source":{"kind":"arxiv","id":"1112.1319","version":1},"attestation_state":"computed","paper":{"title":"Magnetic confinement of the solar tachocline: The oblique dipole","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Brun Allan Sacha, Strugarek Antoine, Zahn Jean-Paul","submitted_at":"2011-12-06T15:51:08Z","abstract_excerpt":"3D MHD global solar simulations coupling the turbulent convective zone and the radiative zone have been carried out. Essential features of the Sun such as differential rotation, meridional circulation and internal waves excitation are recovered. These realistic models are used to test the possibility of having the solar tachocline confined by a primordial inner magnetic field. We find that the initially confined magnetic fields we consider open into the convective envelope. Angular momentum is transported across the two zones by magnetic torques and stresses, establishing the so-called Ferarro"},"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":"1112.1319","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-12-06T15:51:08Z","cross_cats_sorted":[],"title_canon_sha256":"b8a79b386707a8831a3145bf7e8fc27c30a33bebed1562dd5b186ba526e529f9","abstract_canon_sha256":"e232074942e707f8056304902fd71ba6aa02ccf5ee432d346714001bb6f518dd"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:21:27.715206Z","signature_b64":"gpgM5St2sJZ82lj9Gh7JD0W+gLv9/S1K1RbSh9wyVbv8HhYwkB0FoLH+bk0/w0mPN+sLqY2JIoyCFOrEF7PqCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8aa69f661c0359287c100aa7092763c5f101017c0bfe2612eabc18bb813e31b4","last_reissued_at":"2026-05-18T02:21:27.714590Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:21:27.714590Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Magnetic confinement of the solar tachocline: The oblique dipole","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Brun Allan Sacha, Strugarek Antoine, Zahn Jean-Paul","submitted_at":"2011-12-06T15:51:08Z","abstract_excerpt":"3D MHD global solar simulations coupling the turbulent convective zone and the radiative zone have been carried out. Essential features of the Sun such as differential rotation, meridional circulation and internal waves excitation are recovered. These realistic models are used to test the possibility of having the solar tachocline confined by a primordial inner magnetic field. We find that the initially confined magnetic fields we consider open into the convective envelope. Angular momentum is transported across the two zones by magnetic torques and stresses, establishing the so-called Ferarro"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1112.1319","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":"1112.1319","created_at":"2026-05-18T02:21:27.714698+00:00"},{"alias_kind":"arxiv_version","alias_value":"1112.1319v1","created_at":"2026-05-18T02:21:27.714698+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1112.1319","created_at":"2026-05-18T02:21:27.714698+00:00"},{"alias_kind":"pith_short_12","alias_value":"RKTJ6ZQ4ANMS","created_at":"2026-05-18T12:26:41.206345+00:00"},{"alias_kind":"pith_short_16","alias_value":"RKTJ6ZQ4ANMSQ7AQ","created_at":"2026-05-18T12:26:41.206345+00:00"},{"alias_kind":"pith_short_8","alias_value":"RKTJ6ZQ4","created_at":"2026-05-18T12:26:41.206345+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/RKTJ6ZQ4ANMSQ7AQBKTQSJ3DYX","json":"https://pith.science/pith/RKTJ6ZQ4ANMSQ7AQBKTQSJ3DYX.json","graph_json":"https://pith.science/api/pith-number/RKTJ6ZQ4ANMSQ7AQBKTQSJ3DYX/graph.json","events_json":"https://pith.science/api/pith-number/RKTJ6ZQ4ANMSQ7AQBKTQSJ3DYX/events.json","paper":"https://pith.science/paper/RKTJ6ZQ4"},"agent_actions":{"view_html":"https://pith.science/pith/RKTJ6ZQ4ANMSQ7AQBKTQSJ3DYX","download_json":"https://pith.science/pith/RKTJ6ZQ4ANMSQ7AQBKTQSJ3DYX.json","view_paper":"https://pith.science/paper/RKTJ6ZQ4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1112.1319&json=true","fetch_graph":"https://pith.science/api/pith-number/RKTJ6ZQ4ANMSQ7AQBKTQSJ3DYX/graph.json","fetch_events":"https://pith.science/api/pith-number/RKTJ6ZQ4ANMSQ7AQBKTQSJ3DYX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RKTJ6ZQ4ANMSQ7AQBKTQSJ3DYX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RKTJ6ZQ4ANMSQ7AQBKTQSJ3DYX/action/storage_attestation","attest_author":"https://pith.science/pith/RKTJ6ZQ4ANMSQ7AQBKTQSJ3DYX/action/author_attestation","sign_citation":"https://pith.science/pith/RKTJ6ZQ4ANMSQ7AQBKTQSJ3DYX/action/citation_signature","submit_replication":"https://pith.science/pith/RKTJ6ZQ4ANMSQ7AQBKTQSJ3DYX/action/replication_record"}},"created_at":"2026-05-18T02:21:27.714698+00:00","updated_at":"2026-05-18T02:21:27.714698+00:00"}