{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:IOIDJRSA5VM24XSCHLFRPJYK3U","short_pith_number":"pith:IOIDJRSA","schema_version":"1.0","canonical_sha256":"439034c640ed59ae5e423acb17a70add38fe66003ea65f548d163c05eb3660ca","source":{"kind":"arxiv","id":"2506.05170","version":1},"attestation_state":"computed","paper":{"title":"Extending near-axis equilibria in DESC","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"physics.plasm-ph","authors_text":"Daniel Dudt, Dario Panici, Eduardo Rodriguez, Egemen Kolemen, Rory Conlin","submitted_at":"2025-06-05T15:45:29Z","abstract_excerpt":"The near-axis description of optimised stellarator fields has proven to be a powerful tool both for design and understanding of this magnetic confinement concept. The description consists of an asymptotic model of the equilibrium in the distance from its centermost axis, and is thus only approximate. Any practical application therefore requires the eventual construction of a global equilibrium. This paper presents a novel way of constructing global equilibria using the \\texttt{DESC} code that guarantees the correct asymptotic behaviour imposed by a given near-axis construction. The theoretical"},"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":"2506.05170","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"physics.plasm-ph","submitted_at":"2025-06-05T15:45:29Z","cross_cats_sorted":[],"title_canon_sha256":"264437e5c870947e193cc8489f9e7499bb8d4d0fbb7249fbd248b9aa19b9bfeb","abstract_canon_sha256":"63f36fdaf6097845230d2c23da45b2eef90436792505a9993dcc1941121efa36"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:16:43.598736Z","signature_b64":"/YZhLjyU86sd5bBXBkRgLgHZQb1qk2jlK7vQLjis49didsZPGBydOONojOyw0jjuwgElY0yoZTUYEWC8szoADQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"439034c640ed59ae5e423acb17a70add38fe66003ea65f548d163c05eb3660ca","last_reissued_at":"2026-07-05T11:16:43.598207Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:16:43.598207Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Extending near-axis equilibria in DESC","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"physics.plasm-ph","authors_text":"Daniel Dudt, Dario Panici, Eduardo Rodriguez, Egemen Kolemen, Rory Conlin","submitted_at":"2025-06-05T15:45:29Z","abstract_excerpt":"The near-axis description of optimised stellarator fields has proven to be a powerful tool both for design and understanding of this magnetic confinement concept. The description consists of an asymptotic model of the equilibrium in the distance from its centermost axis, and is thus only approximate. Any practical application therefore requires the eventual construction of a global equilibrium. This paper presents a novel way of constructing global equilibria using the \\texttt{DESC} code that guarantees the correct asymptotic behaviour imposed by a given near-axis construction. The theoretical"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2506.05170","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/2506.05170/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":"2506.05170","created_at":"2026-07-05T11:16:43.598274+00:00"},{"alias_kind":"arxiv_version","alias_value":"2506.05170v1","created_at":"2026-07-05T11:16:43.598274+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2506.05170","created_at":"2026-07-05T11:16:43.598274+00:00"},{"alias_kind":"pith_short_12","alias_value":"IOIDJRSA5VM2","created_at":"2026-07-05T11:16:43.598274+00:00"},{"alias_kind":"pith_short_16","alias_value":"IOIDJRSA5VM24XSC","created_at":"2026-07-05T11:16:43.598274+00:00"},{"alias_kind":"pith_short_8","alias_value":"IOIDJRSA","created_at":"2026-07-05T11:16:43.598274+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2505.20475","citing_title":"Numerical asymptotics of near-axis expansions of quasisymmetric magnetohydrostatic equilibria with anisotropic pressure","ref_index":2025,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/IOIDJRSA5VM24XSCHLFRPJYK3U","json":"https://pith.science/pith/IOIDJRSA5VM24XSCHLFRPJYK3U.json","graph_json":"https://pith.science/api/pith-number/IOIDJRSA5VM24XSCHLFRPJYK3U/graph.json","events_json":"https://pith.science/api/pith-number/IOIDJRSA5VM24XSCHLFRPJYK3U/events.json","paper":"https://pith.science/paper/IOIDJRSA"},"agent_actions":{"view_html":"https://pith.science/pith/IOIDJRSA5VM24XSCHLFRPJYK3U","download_json":"https://pith.science/pith/IOIDJRSA5VM24XSCHLFRPJYK3U.json","view_paper":"https://pith.science/paper/IOIDJRSA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2506.05170&json=true","fetch_graph":"https://pith.science/api/pith-number/IOIDJRSA5VM24XSCHLFRPJYK3U/graph.json","fetch_events":"https://pith.science/api/pith-number/IOIDJRSA5VM24XSCHLFRPJYK3U/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IOIDJRSA5VM24XSCHLFRPJYK3U/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IOIDJRSA5VM24XSCHLFRPJYK3U/action/storage_attestation","attest_author":"https://pith.science/pith/IOIDJRSA5VM24XSCHLFRPJYK3U/action/author_attestation","sign_citation":"https://pith.science/pith/IOIDJRSA5VM24XSCHLFRPJYK3U/action/citation_signature","submit_replication":"https://pith.science/pith/IOIDJRSA5VM24XSCHLFRPJYK3U/action/replication_record"}},"created_at":"2026-07-05T11:16:43.598274+00:00","updated_at":"2026-07-05T11:16:43.598274+00:00"}