{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:7PVBX6CSHB324W2YBG4SBDQUG4","short_pith_number":"pith:7PVBX6CS","schema_version":"1.0","canonical_sha256":"fbea1bf8523877ae5b5809b9208e143712693f739f08b179d29dc5e9ab967548","source":{"kind":"arxiv","id":"1603.05397","version":1},"attestation_state":"computed","paper":{"title":"Formation and plasma circulation of solar prominences","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Chun Xia, Rony Keppens","submitted_at":"2016-03-17T09:20:49Z","abstract_excerpt":"Solar prominences are long-lived cool and dense plasma curtains in the hot and rarefied outer solar atmosphere or corona. The physical mechanism responsible for their formation and especially for their internal plasma circulation has been uncertain for decades. The observed ubiquitous down flows in quiescent prominences are difficult to interpret as plasma with high conductivity seems to move across horizontal magnetic field lines. Here we present three-dimensional numerical simulations of prominence formation and evolution in an elongated magnetic flux rope as a result of in-situ plasma conde"},"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":"1603.05397","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-03-17T09:20:49Z","cross_cats_sorted":[],"title_canon_sha256":"f23a9ac7fb7662e3914c791f2d9d213c9b1571ee0fb36130b5a056b3148fd258","abstract_canon_sha256":"6c1ec3066a187f056f2302a928a33118d8488027cce37ab2e163d67704271514"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:13:53.978582Z","signature_b64":"Rl5zpwf55UOVIvoaFqL5ccL3GsLhuYXrwVkSuTIMzWyViACnTBdm6sVnTA0dDUMKTHLBf7MGnBPOIa2NACw9Cg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fbea1bf8523877ae5b5809b9208e143712693f739f08b179d29dc5e9ab967548","last_reissued_at":"2026-05-18T01:13:53.977870Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:13:53.977870Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Formation and plasma circulation of solar prominences","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Chun Xia, Rony Keppens","submitted_at":"2016-03-17T09:20:49Z","abstract_excerpt":"Solar prominences are long-lived cool and dense plasma curtains in the hot and rarefied outer solar atmosphere or corona. The physical mechanism responsible for their formation and especially for their internal plasma circulation has been uncertain for decades. The observed ubiquitous down flows in quiescent prominences are difficult to interpret as plasma with high conductivity seems to move across horizontal magnetic field lines. Here we present three-dimensional numerical simulations of prominence formation and evolution in an elongated magnetic flux rope as a result of in-situ plasma conde"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1603.05397","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":"1603.05397","created_at":"2026-05-18T01:13:53.977965+00:00"},{"alias_kind":"arxiv_version","alias_value":"1603.05397v1","created_at":"2026-05-18T01:13:53.977965+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1603.05397","created_at":"2026-05-18T01:13:53.977965+00:00"},{"alias_kind":"pith_short_12","alias_value":"7PVBX6CSHB32","created_at":"2026-05-18T12:30:04.600751+00:00"},{"alias_kind":"pith_short_16","alias_value":"7PVBX6CSHB324W2Y","created_at":"2026-05-18T12:30:04.600751+00:00"},{"alias_kind":"pith_short_8","alias_value":"7PVBX6CS","created_at":"2026-05-18T12:30:04.600751+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/7PVBX6CSHB324W2YBG4SBDQUG4","json":"https://pith.science/pith/7PVBX6CSHB324W2YBG4SBDQUG4.json","graph_json":"https://pith.science/api/pith-number/7PVBX6CSHB324W2YBG4SBDQUG4/graph.json","events_json":"https://pith.science/api/pith-number/7PVBX6CSHB324W2YBG4SBDQUG4/events.json","paper":"https://pith.science/paper/7PVBX6CS"},"agent_actions":{"view_html":"https://pith.science/pith/7PVBX6CSHB324W2YBG4SBDQUG4","download_json":"https://pith.science/pith/7PVBX6CSHB324W2YBG4SBDQUG4.json","view_paper":"https://pith.science/paper/7PVBX6CS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1603.05397&json=true","fetch_graph":"https://pith.science/api/pith-number/7PVBX6CSHB324W2YBG4SBDQUG4/graph.json","fetch_events":"https://pith.science/api/pith-number/7PVBX6CSHB324W2YBG4SBDQUG4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7PVBX6CSHB324W2YBG4SBDQUG4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7PVBX6CSHB324W2YBG4SBDQUG4/action/storage_attestation","attest_author":"https://pith.science/pith/7PVBX6CSHB324W2YBG4SBDQUG4/action/author_attestation","sign_citation":"https://pith.science/pith/7PVBX6CSHB324W2YBG4SBDQUG4/action/citation_signature","submit_replication":"https://pith.science/pith/7PVBX6CSHB324W2YBG4SBDQUG4/action/replication_record"}},"created_at":"2026-05-18T01:13:53.977965+00:00","updated_at":"2026-05-18T01:13:53.977965+00:00"}