{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2017:SOJEGPZPTD3LUHGH47D5UFUPC2","short_pith_number":"pith:SOJEGPZP","canonical_record":{"source":{"id":"1705.07190","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-05-16T09:32:54Z","cross_cats_sorted":[],"title_canon_sha256":"c36e39ec2414921d852aa8fb8510dfac3c7f042a713f0855436fcd074c49c21d","abstract_canon_sha256":"bba41837725ed3b68405615944158c3770ff0acadadc58cf44b9e6e5292903c5"},"schema_version":"1.0"},"canonical_sha256":"9392433f2f98f6ba1cc7e7c7da168f16852ffb009da5295e2631304effc7203c","source":{"kind":"arxiv","id":"1705.07190","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1705.07190","created_at":"2026-05-18T00:39:34Z"},{"alias_kind":"arxiv_version","alias_value":"1705.07190v2","created_at":"2026-05-18T00:39:34Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1705.07190","created_at":"2026-05-18T00:39:34Z"},{"alias_kind":"pith_short_12","alias_value":"SOJEGPZPTD3L","created_at":"2026-05-18T12:31:43Z"},{"alias_kind":"pith_short_16","alias_value":"SOJEGPZPTD3LUHGH","created_at":"2026-05-18T12:31:43Z"},{"alias_kind":"pith_short_8","alias_value":"SOJEGPZP","created_at":"2026-05-18T12:31:43Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2017:SOJEGPZPTD3LUHGH47D5UFUPC2","target":"record","payload":{"canonical_record":{"source":{"id":"1705.07190","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-05-16T09:32:54Z","cross_cats_sorted":[],"title_canon_sha256":"c36e39ec2414921d852aa8fb8510dfac3c7f042a713f0855436fcd074c49c21d","abstract_canon_sha256":"bba41837725ed3b68405615944158c3770ff0acadadc58cf44b9e6e5292903c5"},"schema_version":"1.0"},"canonical_sha256":"9392433f2f98f6ba1cc7e7c7da168f16852ffb009da5295e2631304effc7203c","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:39:34.930721Z","signature_b64":"lpPUBSZP0HszG2OTo+a/Ye09seulbUwGvO6/T3aA49lsu4WObMOUDmvwTA2tMQ2xLb2zVvH4R+tcvT6zHKVCDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9392433f2f98f6ba1cc7e7c7da168f16852ffb009da5295e2631304effc7203c","last_reissued_at":"2026-05-18T00:39:34.930143Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:39:34.930143Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1705.07190","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:39:34Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"m0nDGRCv1PHZ+hXee/bP4+4rmp6foka4bJh2wR7h42cr10hJog607eXCIA7MUICbFlCD4qNRiJww3BLZOf6ZDw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-09T09:16:24.434699Z"},"content_sha256":"da5097baca4807a5efe4e9862c5c0a12a78c71420c7bf94e6dfb04c5c4a3cdba","schema_version":"1.0","event_id":"sha256:da5097baca4807a5efe4e9862c5c0a12a78c71420c7bf94e6dfb04c5c4a3cdba"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2017:SOJEGPZPTD3LUHGH47D5UFUPC2","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"How does an asymmetric magnetic field change the vertical structure of a hot accretion flow?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Maryam Samadi, Richard Lovelace, Shahram Abbassi","submitted_at":"2017-05-16T09:32:54Z","abstract_excerpt":"This paper explores the effects of large-scale magnetic fields in hot accretion flows for asymmetric configurations with respect to the equatorial plane. The solutions that we have found show that the large-scale asymmetric magnetic field can significantly affect the dynamics of the flow and also cause notable outflows in the outer parts. Previously, we treated a viscous resistive accreting disc in the presence of an odd symmetric $\\textbf{B-}$ field about the equatorial plane. Now we extend our earlier work by taking into account another configuration of large-scale magnetic field which is no"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.07190","kind":"arxiv","version":2},"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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:39:34Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"QgAWPffhLiFS+oHyzx5BG6KwT0YnuezPJ+pQSAEvhgn5CF+vwqSbr7ARRLlNv/KpSHPCUD1WgNT/WcLk4Pb6Ag==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-09T09:16:24.435439Z"},"content_sha256":"f56602e2522b8b1bdbdb67586a6daaec3efdda745e578880e5099072ea293e48","schema_version":"1.0","event_id":"sha256:f56602e2522b8b1bdbdb67586a6daaec3efdda745e578880e5099072ea293e48"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/SOJEGPZPTD3LUHGH47D5UFUPC2/bundle.json","state_url":"https://pith.science/pith/SOJEGPZPTD3LUHGH47D5UFUPC2/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/SOJEGPZPTD3LUHGH47D5UFUPC2/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-06-09T09:16:24Z","links":{"resolver":"https://pith.science/pith/SOJEGPZPTD3LUHGH47D5UFUPC2","bundle":"https://pith.science/pith/SOJEGPZPTD3LUHGH47D5UFUPC2/bundle.json","state":"https://pith.science/pith/SOJEGPZPTD3LUHGH47D5UFUPC2/state.json","well_known_bundle":"https://pith.science/.well-known/pith/SOJEGPZPTD3LUHGH47D5UFUPC2/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2017:SOJEGPZPTD3LUHGH47D5UFUPC2","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"bba41837725ed3b68405615944158c3770ff0acadadc58cf44b9e6e5292903c5","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-05-16T09:32:54Z","title_canon_sha256":"c36e39ec2414921d852aa8fb8510dfac3c7f042a713f0855436fcd074c49c21d"},"schema_version":"1.0","source":{"id":"1705.07190","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1705.07190","created_at":"2026-05-18T00:39:34Z"},{"alias_kind":"arxiv_version","alias_value":"1705.07190v2","created_at":"2026-05-18T00:39:34Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1705.07190","created_at":"2026-05-18T00:39:34Z"},{"alias_kind":"pith_short_12","alias_value":"SOJEGPZPTD3L","created_at":"2026-05-18T12:31:43Z"},{"alias_kind":"pith_short_16","alias_value":"SOJEGPZPTD3LUHGH","created_at":"2026-05-18T12:31:43Z"},{"alias_kind":"pith_short_8","alias_value":"SOJEGPZP","created_at":"2026-05-18T12:31:43Z"}],"graph_snapshots":[{"event_id":"sha256:f56602e2522b8b1bdbdb67586a6daaec3efdda745e578880e5099072ea293e48","target":"graph","created_at":"2026-05-18T00:39:34Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"This paper explores the effects of large-scale magnetic fields in hot accretion flows for asymmetric configurations with respect to the equatorial plane. The solutions that we have found show that the large-scale asymmetric magnetic field can significantly affect the dynamics of the flow and also cause notable outflows in the outer parts. Previously, we treated a viscous resistive accreting disc in the presence of an odd symmetric $\\textbf{B-}$ field about the equatorial plane. Now we extend our earlier work by taking into account another configuration of large-scale magnetic field which is no","authors_text":"Maryam Samadi, Richard Lovelace, Shahram Abbassi","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-05-16T09:32:54Z","title":"How does an asymmetric magnetic field change the vertical structure of a hot accretion flow?"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.07190","kind":"arxiv","version":2},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:da5097baca4807a5efe4e9862c5c0a12a78c71420c7bf94e6dfb04c5c4a3cdba","target":"record","created_at":"2026-05-18T00:39:34Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"bba41837725ed3b68405615944158c3770ff0acadadc58cf44b9e6e5292903c5","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-05-16T09:32:54Z","title_canon_sha256":"c36e39ec2414921d852aa8fb8510dfac3c7f042a713f0855436fcd074c49c21d"},"schema_version":"1.0","source":{"id":"1705.07190","kind":"arxiv","version":2}},"canonical_sha256":"9392433f2f98f6ba1cc7e7c7da168f16852ffb009da5295e2631304effc7203c","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"9392433f2f98f6ba1cc7e7c7da168f16852ffb009da5295e2631304effc7203c","first_computed_at":"2026-05-18T00:39:34.930143Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:39:34.930143Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"lpPUBSZP0HszG2OTo+a/Ye09seulbUwGvO6/T3aA49lsu4WObMOUDmvwTA2tMQ2xLb2zVvH4R+tcvT6zHKVCDg==","signature_status":"signed_v1","signed_at":"2026-05-18T00:39:34.930721Z","signed_message":"canonical_sha256_bytes"},"source_id":"1705.07190","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:da5097baca4807a5efe4e9862c5c0a12a78c71420c7bf94e6dfb04c5c4a3cdba","sha256:f56602e2522b8b1bdbdb67586a6daaec3efdda745e578880e5099072ea293e48"],"state_sha256":"91e50ebb8f446e59f6e347803386361cb79142d7cfba4c96bb213822929c82fc"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"wyxOESdbvbUYEKRctUFxnPevL99wa9WMjB07WCACVefAWFC1hXCX6r4NsmBC+pgrhYPYa+uMfJpLJLC4/CTAAA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-09T09:16:24.439447Z","bundle_sha256":"b8915d500eb0941c09390dad2b1518d0d41dfc5d697e08d3fe82190c7193bece"}}