{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:YOKHALGBLAGLWXT5JMP2KZ65HV","short_pith_number":"pith:YOKHALGB","schema_version":"1.0","canonical_sha256":"c394702cc1580cbb5e7d4b1fa567dd3d453e2e65192c077f69cba14d18bc8211","source":{"kind":"arxiv","id":"1308.0442","version":1},"attestation_state":"computed","paper":{"title":"The Role of a Flux Rope Ejection in Three-dimensional Magnetohydrodynamic Simulation of a Solar Flare","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.plasm-ph"],"primary_cat":"astro-ph.SR","authors_text":"Kazunari Shibata, Keisuke Nishida, Naoto Nishizuka","submitted_at":"2013-08-02T09:09:55Z","abstract_excerpt":"We investigated the dynamic evolution of a 3-dimensional (3D) flux rope eruption and magnetic reconnection process in a solar flare, by simply extending 2-dimensional (2D) resistive magnetohydrodynamic simulation model of solar flares with low $\\beta$ plasma to 3D model. We succeeded in reproducing a current sheet and bi-directional reconnection outflows just below the flux rope during the eruption in our 3D simulations. We calculated four cases of a strongly twisted flux rope and a weakly twisted flux rope in 2D and 3D simulations. The time evolution of a weakly twisted flux rope in 3D simula"},"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":"1308.0442","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2013-08-02T09:09:55Z","cross_cats_sorted":["physics.plasm-ph"],"title_canon_sha256":"7208e79e86c472475a38200c74fef13e9f98e6f30adae9ab95d80112a058d70f","abstract_canon_sha256":"c85cd0eb4747330fa2eab2c1735172edca10511d72187ce63d562af8b4ab5690"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:13:09.639645Z","signature_b64":"U4GLFvGbii7SDRznUVl/OkWdLYStGsbUVz8RWT/x7ajg3S4Ix1OuKg9BrdvnjVqP2vK402MCky5Aj5It5CJ5Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c394702cc1580cbb5e7d4b1fa567dd3d453e2e65192c077f69cba14d18bc8211","last_reissued_at":"2026-05-18T03:13:09.639229Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:13:09.639229Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Role of a Flux Rope Ejection in Three-dimensional Magnetohydrodynamic Simulation of a Solar Flare","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.plasm-ph"],"primary_cat":"astro-ph.SR","authors_text":"Kazunari Shibata, Keisuke Nishida, Naoto Nishizuka","submitted_at":"2013-08-02T09:09:55Z","abstract_excerpt":"We investigated the dynamic evolution of a 3-dimensional (3D) flux rope eruption and magnetic reconnection process in a solar flare, by simply extending 2-dimensional (2D) resistive magnetohydrodynamic simulation model of solar flares with low $\\beta$ plasma to 3D model. We succeeded in reproducing a current sheet and bi-directional reconnection outflows just below the flux rope during the eruption in our 3D simulations. We calculated four cases of a strongly twisted flux rope and a weakly twisted flux rope in 2D and 3D simulations. The time evolution of a weakly twisted flux rope in 3D simula"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1308.0442","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":"1308.0442","created_at":"2026-05-18T03:13:09.639287+00:00"},{"alias_kind":"arxiv_version","alias_value":"1308.0442v1","created_at":"2026-05-18T03:13:09.639287+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1308.0442","created_at":"2026-05-18T03:13:09.639287+00:00"},{"alias_kind":"pith_short_12","alias_value":"YOKHALGBLAGL","created_at":"2026-05-18T12:28:06.772260+00:00"},{"alias_kind":"pith_short_16","alias_value":"YOKHALGBLAGLWXT5","created_at":"2026-05-18T12:28:06.772260+00:00"},{"alias_kind":"pith_short_8","alias_value":"YOKHALGB","created_at":"2026-05-18T12:28:06.772260+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/YOKHALGBLAGLWXT5JMP2KZ65HV","json":"https://pith.science/pith/YOKHALGBLAGLWXT5JMP2KZ65HV.json","graph_json":"https://pith.science/api/pith-number/YOKHALGBLAGLWXT5JMP2KZ65HV/graph.json","events_json":"https://pith.science/api/pith-number/YOKHALGBLAGLWXT5JMP2KZ65HV/events.json","paper":"https://pith.science/paper/YOKHALGB"},"agent_actions":{"view_html":"https://pith.science/pith/YOKHALGBLAGLWXT5JMP2KZ65HV","download_json":"https://pith.science/pith/YOKHALGBLAGLWXT5JMP2KZ65HV.json","view_paper":"https://pith.science/paper/YOKHALGB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1308.0442&json=true","fetch_graph":"https://pith.science/api/pith-number/YOKHALGBLAGLWXT5JMP2KZ65HV/graph.json","fetch_events":"https://pith.science/api/pith-number/YOKHALGBLAGLWXT5JMP2KZ65HV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YOKHALGBLAGLWXT5JMP2KZ65HV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YOKHALGBLAGLWXT5JMP2KZ65HV/action/storage_attestation","attest_author":"https://pith.science/pith/YOKHALGBLAGLWXT5JMP2KZ65HV/action/author_attestation","sign_citation":"https://pith.science/pith/YOKHALGBLAGLWXT5JMP2KZ65HV/action/citation_signature","submit_replication":"https://pith.science/pith/YOKHALGBLAGLWXT5JMP2KZ65HV/action/replication_record"}},"created_at":"2026-05-18T03:13:09.639287+00:00","updated_at":"2026-05-18T03:13:09.639287+00:00"}