{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:6IXN2SCB2AELK7VIJN4AOVHX4M","short_pith_number":"pith:6IXN2SCB","schema_version":"1.0","canonical_sha256":"f22edd4841d008b57ea84b780754f7e32139b91570457fa739ab2c0d0f3e37b5","source":{"kind":"arxiv","id":"1204.0743","version":1},"attestation_state":"computed","paper":{"title":"Resistive and magnetized accretion flows with convection","license":"http://creativecommons.org/licenses/by/3.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Kazem Faghei, Mobina Omidvand","submitted_at":"2012-04-03T17:32:22Z","abstract_excerpt":"We considered the effects of convection on the radiatively inefficient accretion flows (RIAF) in the presence of resistivity and toroidal magnetic field. We discussed the effects of convection on transports of angular momentum and energy. We established two cases for the resistive and magnetized RIAFs with convection: assuming the convection parameter as a free parameter and using mixing-length theory to calculate convection parameter. A self-similar method was used to solve the integrated equations that govern the behavior of the presented model. The solutions showed that the accretion and ro"},"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":"1204.0743","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/3.0/","primary_cat":"astro-ph.HE","submitted_at":"2012-04-03T17:32:22Z","cross_cats_sorted":[],"title_canon_sha256":"6ddb59fa5d50164aa1baf14fa793e2bd9c000abba82a7b0ca5af8dc639a93834","abstract_canon_sha256":"cd16bb72b9edd4a98b24a8b98e6edd0fc14019038aa5031e635404ee600ba307"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:57:57.570376Z","signature_b64":"n5u+/QDqCh2dR9ez2J1ZOOntenPNupAYpm86fu/fNiM+8WdghpQuvnMawh3EZlfvacOHhr/AWpdHOE3ZyGMtBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f22edd4841d008b57ea84b780754f7e32139b91570457fa739ab2c0d0f3e37b5","last_reissued_at":"2026-05-18T01:57:57.569879Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:57:57.569879Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Resistive and magnetized accretion flows with convection","license":"http://creativecommons.org/licenses/by/3.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Kazem Faghei, Mobina Omidvand","submitted_at":"2012-04-03T17:32:22Z","abstract_excerpt":"We considered the effects of convection on the radiatively inefficient accretion flows (RIAF) in the presence of resistivity and toroidal magnetic field. We discussed the effects of convection on transports of angular momentum and energy. We established two cases for the resistive and magnetized RIAFs with convection: assuming the convection parameter as a free parameter and using mixing-length theory to calculate convection parameter. A self-similar method was used to solve the integrated equations that govern the behavior of the presented model. The solutions showed that the accretion and ro"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1204.0743","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":"1204.0743","created_at":"2026-05-18T01:57:57.569956+00:00"},{"alias_kind":"arxiv_version","alias_value":"1204.0743v1","created_at":"2026-05-18T01:57:57.569956+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1204.0743","created_at":"2026-05-18T01:57:57.569956+00:00"},{"alias_kind":"pith_short_12","alias_value":"6IXN2SCB2AEL","created_at":"2026-05-18T12:26:56.085431+00:00"},{"alias_kind":"pith_short_16","alias_value":"6IXN2SCB2AELK7VI","created_at":"2026-05-18T12:26:56.085431+00:00"},{"alias_kind":"pith_short_8","alias_value":"6IXN2SCB","created_at":"2026-05-18T12:26:56.085431+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/6IXN2SCB2AELK7VIJN4AOVHX4M","json":"https://pith.science/pith/6IXN2SCB2AELK7VIJN4AOVHX4M.json","graph_json":"https://pith.science/api/pith-number/6IXN2SCB2AELK7VIJN4AOVHX4M/graph.json","events_json":"https://pith.science/api/pith-number/6IXN2SCB2AELK7VIJN4AOVHX4M/events.json","paper":"https://pith.science/paper/6IXN2SCB"},"agent_actions":{"view_html":"https://pith.science/pith/6IXN2SCB2AELK7VIJN4AOVHX4M","download_json":"https://pith.science/pith/6IXN2SCB2AELK7VIJN4AOVHX4M.json","view_paper":"https://pith.science/paper/6IXN2SCB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1204.0743&json=true","fetch_graph":"https://pith.science/api/pith-number/6IXN2SCB2AELK7VIJN4AOVHX4M/graph.json","fetch_events":"https://pith.science/api/pith-number/6IXN2SCB2AELK7VIJN4AOVHX4M/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6IXN2SCB2AELK7VIJN4AOVHX4M/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6IXN2SCB2AELK7VIJN4AOVHX4M/action/storage_attestation","attest_author":"https://pith.science/pith/6IXN2SCB2AELK7VIJN4AOVHX4M/action/author_attestation","sign_citation":"https://pith.science/pith/6IXN2SCB2AELK7VIJN4AOVHX4M/action/citation_signature","submit_replication":"https://pith.science/pith/6IXN2SCB2AELK7VIJN4AOVHX4M/action/replication_record"}},"created_at":"2026-05-18T01:57:57.569956+00:00","updated_at":"2026-05-18T01:57:57.569956+00:00"}