{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:HQEALUEJGB4KIO7K3OTE7RODTL","short_pith_number":"pith:HQEALUEJ","schema_version":"1.0","canonical_sha256":"3c0805d0893078a43beadba64fc5c39accc150037787f44ab4537a2ec9ecfa13","source":{"kind":"arxiv","id":"1110.5699","version":1},"attestation_state":"computed","paper":{"title":"Magnetospheric launching in resistive MHD simulations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Hsien Shang, Miljenko Cemeljic","submitted_at":"2011-10-26T04:18:01Z","abstract_excerpt":"We perform numerical simulations in the close vicinity of a slowly rotating young stellar object. Using our own resistive MHD Zeus347 code in 2D axisymmetry, magnetospheric interaction experiences four robust stages in evolution. Quasi-stationary axial and conical streams of outflowing matter can last many orbital periods as results of the resistivity-facilitated magnetic reconnections. The shape of the magnetic field depends on resistivity in the magnetosphere."},"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":"1110.5699","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-10-26T04:18:01Z","cross_cats_sorted":[],"title_canon_sha256":"f6ac4b0d4a60b0d4df991622484ba4b87072cfd516e8c43b0373933cf10063db","abstract_canon_sha256":"a00c86b56eb2cae1c687c2ffd5b452b5670ff0e1e0550ef29d0ab4a55657a24a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:10:11.587200Z","signature_b64":"Pb6tmyIkZIqrmigiXuWIJPjRaEguoXfLXviw08Q7o91VI7WFrMlZ6l9qFv+2fa7LgBc7RuxclMvHLfahhuL0Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3c0805d0893078a43beadba64fc5c39accc150037787f44ab4537a2ec9ecfa13","last_reissued_at":"2026-05-18T04:10:11.586369Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:10:11.586369Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Magnetospheric launching in resistive MHD simulations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Hsien Shang, Miljenko Cemeljic","submitted_at":"2011-10-26T04:18:01Z","abstract_excerpt":"We perform numerical simulations in the close vicinity of a slowly rotating young stellar object. Using our own resistive MHD Zeus347 code in 2D axisymmetry, magnetospheric interaction experiences four robust stages in evolution. Quasi-stationary axial and conical streams of outflowing matter can last many orbital periods as results of the resistivity-facilitated magnetic reconnections. The shape of the magnetic field depends on resistivity in the magnetosphere."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1110.5699","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":"1110.5699","created_at":"2026-05-18T04:10:11.586512+00:00"},{"alias_kind":"arxiv_version","alias_value":"1110.5699v1","created_at":"2026-05-18T04:10:11.586512+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1110.5699","created_at":"2026-05-18T04:10:11.586512+00:00"},{"alias_kind":"pith_short_12","alias_value":"HQEALUEJGB4K","created_at":"2026-05-18T12:26:30.835961+00:00"},{"alias_kind":"pith_short_16","alias_value":"HQEALUEJGB4KIO7K","created_at":"2026-05-18T12:26:30.835961+00:00"},{"alias_kind":"pith_short_8","alias_value":"HQEALUEJ","created_at":"2026-05-18T12:26:30.835961+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/HQEALUEJGB4KIO7K3OTE7RODTL","json":"https://pith.science/pith/HQEALUEJGB4KIO7K3OTE7RODTL.json","graph_json":"https://pith.science/api/pith-number/HQEALUEJGB4KIO7K3OTE7RODTL/graph.json","events_json":"https://pith.science/api/pith-number/HQEALUEJGB4KIO7K3OTE7RODTL/events.json","paper":"https://pith.science/paper/HQEALUEJ"},"agent_actions":{"view_html":"https://pith.science/pith/HQEALUEJGB4KIO7K3OTE7RODTL","download_json":"https://pith.science/pith/HQEALUEJGB4KIO7K3OTE7RODTL.json","view_paper":"https://pith.science/paper/HQEALUEJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1110.5699&json=true","fetch_graph":"https://pith.science/api/pith-number/HQEALUEJGB4KIO7K3OTE7RODTL/graph.json","fetch_events":"https://pith.science/api/pith-number/HQEALUEJGB4KIO7K3OTE7RODTL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HQEALUEJGB4KIO7K3OTE7RODTL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HQEALUEJGB4KIO7K3OTE7RODTL/action/storage_attestation","attest_author":"https://pith.science/pith/HQEALUEJGB4KIO7K3OTE7RODTL/action/author_attestation","sign_citation":"https://pith.science/pith/HQEALUEJGB4KIO7K3OTE7RODTL/action/citation_signature","submit_replication":"https://pith.science/pith/HQEALUEJGB4KIO7K3OTE7RODTL/action/replication_record"}},"created_at":"2026-05-18T04:10:11.586512+00:00","updated_at":"2026-05-18T04:10:11.586512+00:00"}