{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:LTPYAVYXS7WBTAWPZBQEMRQ75O","short_pith_number":"pith:LTPYAVYX","schema_version":"1.0","canonical_sha256":"5cdf80571797ec1982cfc86046461feba1af4bbdd7fc0dea57258e1964cad9af","source":{"kind":"arxiv","id":"2305.02089","version":1},"attestation_state":"computed","paper":{"title":"Self-consistent propagation of flux ropes in realistic coronal simulations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Lani, B. Kuzma, B. Perri, B. Schmieder, F. Regnault, L. Linan, M. Brchnelova, S. Poedts","submitted_at":"2023-05-03T12:50:48Z","abstract_excerpt":"The aim of this paper is to demonstrate the possible use of the new coronal model COCONUT to compute a detailed representation of a numerical CME at 0.1~AU, after its injection at the solar surface and propagation in a realistic solar wind, as derived from observed magnetograms. We present the implementation and propagation of modified Titov-D\\'emoulin (TDm) flux ropes in the COCONUT 3D MHD coronal model. The background solar wind is reconstructed in order to model two opposite configurations representing a solar activity maximum and minimum respectively. Both were derived from magnetograms wh"},"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":"2305.02089","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2023-05-03T12:50:48Z","cross_cats_sorted":[],"title_canon_sha256":"7be1e5fb6f42764e68e189f233cfad7ac823316cb2a383dbce0bb1aca6091d36","abstract_canon_sha256":"cba0a2ea24de29f142bf29a4142bdb94de3c339bd130a4b7cab6fec29d7b3d56"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:29:47.919939Z","signature_b64":"PHrFmSwU7vS9oTk6Rq2UZ7yCWj04Cp1UZhN/fROYeYv1no1vzbhHxzmpfL5ve9F79xL2p2glot4iS6304llVBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5cdf80571797ec1982cfc86046461feba1af4bbdd7fc0dea57258e1964cad9af","last_reissued_at":"2026-07-05T06:29:47.919459Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:29:47.919459Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Self-consistent propagation of flux ropes in realistic coronal simulations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Lani, B. Kuzma, B. Perri, B. Schmieder, F. Regnault, L. Linan, M. Brchnelova, S. Poedts","submitted_at":"2023-05-03T12:50:48Z","abstract_excerpt":"The aim of this paper is to demonstrate the possible use of the new coronal model COCONUT to compute a detailed representation of a numerical CME at 0.1~AU, after its injection at the solar surface and propagation in a realistic solar wind, as derived from observed magnetograms. We present the implementation and propagation of modified Titov-D\\'emoulin (TDm) flux ropes in the COCONUT 3D MHD coronal model. The background solar wind is reconstructed in order to model two opposite configurations representing a solar activity maximum and minimum respectively. Both were derived from magnetograms wh"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2305.02089","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2305.02089/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2305.02089","created_at":"2026-07-05T06:29:47.919527+00:00"},{"alias_kind":"arxiv_version","alias_value":"2305.02089v1","created_at":"2026-07-05T06:29:47.919527+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2305.02089","created_at":"2026-07-05T06:29:47.919527+00:00"},{"alias_kind":"pith_short_12","alias_value":"LTPYAVYXS7WB","created_at":"2026-07-05T06:29:47.919527+00:00"},{"alias_kind":"pith_short_16","alias_value":"LTPYAVYXS7WBTAWP","created_at":"2026-07-05T06:29:47.919527+00:00"},{"alias_kind":"pith_short_8","alias_value":"LTPYAVYX","created_at":"2026-07-05T06:29:47.919527+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/LTPYAVYXS7WBTAWPZBQEMRQ75O","json":"https://pith.science/pith/LTPYAVYXS7WBTAWPZBQEMRQ75O.json","graph_json":"https://pith.science/api/pith-number/LTPYAVYXS7WBTAWPZBQEMRQ75O/graph.json","events_json":"https://pith.science/api/pith-number/LTPYAVYXS7WBTAWPZBQEMRQ75O/events.json","paper":"https://pith.science/paper/LTPYAVYX"},"agent_actions":{"view_html":"https://pith.science/pith/LTPYAVYXS7WBTAWPZBQEMRQ75O","download_json":"https://pith.science/pith/LTPYAVYXS7WBTAWPZBQEMRQ75O.json","view_paper":"https://pith.science/paper/LTPYAVYX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2305.02089&json=true","fetch_graph":"https://pith.science/api/pith-number/LTPYAVYXS7WBTAWPZBQEMRQ75O/graph.json","fetch_events":"https://pith.science/api/pith-number/LTPYAVYXS7WBTAWPZBQEMRQ75O/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LTPYAVYXS7WBTAWPZBQEMRQ75O/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LTPYAVYXS7WBTAWPZBQEMRQ75O/action/storage_attestation","attest_author":"https://pith.science/pith/LTPYAVYXS7WBTAWPZBQEMRQ75O/action/author_attestation","sign_citation":"https://pith.science/pith/LTPYAVYXS7WBTAWPZBQEMRQ75O/action/citation_signature","submit_replication":"https://pith.science/pith/LTPYAVYXS7WBTAWPZBQEMRQ75O/action/replication_record"}},"created_at":"2026-07-05T06:29:47.919527+00:00","updated_at":"2026-07-05T06:29:47.919527+00:00"}