{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2003:IACC3XMQHVVARTQNSBUAVM43XC","short_pith_number":"pith:IACC3XMQ","schema_version":"1.0","canonical_sha256":"40042ddd903d6a08ce0d90680ab39bb89508333861d3090b13dd5d66ac3b98da","source":{"kind":"arxiv","id":"cond-mat/0310272","version":2},"attestation_state":"computed","paper":{"title":"Influence of twin structure on flux turbulence near the front of vortex annihilation","license":"","headline":"","cross_cats":[],"primary_cat":"cond-mat.supr-con","authors_text":"A.A. Zhokhov, I.G. Naumenko, L.S. Uspenskaya","submitted_at":"2003-10-12T15:11:00Z","abstract_excerpt":"The remagnetization of YBCO single crystals is studied by magneto-optical technique. Different behavior of the annihilation flux front in twinned and twin-less samples is observed. The specific induction distribution, called Meissner hole, is found to be necessary forerunner of turbulence development."},"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":"cond-mat/0310272","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"cond-mat.supr-con","submitted_at":"2003-10-12T15:11:00Z","cross_cats_sorted":[],"title_canon_sha256":"ff94a91c64cce4d62ca7d46e425ccc5867ab5545b794a601dbbc49f6cef1e579","abstract_canon_sha256":"b1fca3bfddae4892d17b724c89dacb5d7715321d47e1d3d8868386d22fa40206"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:39:59.046626Z","signature_b64":"9cVvHmOofZY4CetC/7IsW1scwRKMx8GgeVYK7UtMTLZpzD+tT2b0OStfOhl+i9eNXUgE207hRY71ca21SgdnCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"40042ddd903d6a08ce0d90680ab39bb89508333861d3090b13dd5d66ac3b98da","last_reissued_at":"2026-05-18T01:39:59.046155Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:39:59.046155Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Influence of twin structure on flux turbulence near the front of vortex annihilation","license":"","headline":"","cross_cats":[],"primary_cat":"cond-mat.supr-con","authors_text":"A.A. Zhokhov, I.G. Naumenko, L.S. Uspenskaya","submitted_at":"2003-10-12T15:11:00Z","abstract_excerpt":"The remagnetization of YBCO single crystals is studied by magneto-optical technique. Different behavior of the annihilation flux front in twinned and twin-less samples is observed. The specific induction distribution, called Meissner hole, is found to be necessary forerunner of turbulence development."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"cond-mat/0310272","kind":"arxiv","version":2},"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":"cond-mat/0310272","created_at":"2026-05-18T01:39:59.046242+00:00"},{"alias_kind":"arxiv_version","alias_value":"cond-mat/0310272v2","created_at":"2026-05-18T01:39:59.046242+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.cond-mat/0310272","created_at":"2026-05-18T01:39:59.046242+00:00"},{"alias_kind":"pith_short_12","alias_value":"IACC3XMQHVVA","created_at":"2026-05-18T12:25:52.051335+00:00"},{"alias_kind":"pith_short_16","alias_value":"IACC3XMQHVVARTQN","created_at":"2026-05-18T12:25:52.051335+00:00"},{"alias_kind":"pith_short_8","alias_value":"IACC3XMQ","created_at":"2026-05-18T12:25:52.051335+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/IACC3XMQHVVARTQNSBUAVM43XC","json":"https://pith.science/pith/IACC3XMQHVVARTQNSBUAVM43XC.json","graph_json":"https://pith.science/api/pith-number/IACC3XMQHVVARTQNSBUAVM43XC/graph.json","events_json":"https://pith.science/api/pith-number/IACC3XMQHVVARTQNSBUAVM43XC/events.json","paper":"https://pith.science/paper/IACC3XMQ"},"agent_actions":{"view_html":"https://pith.science/pith/IACC3XMQHVVARTQNSBUAVM43XC","download_json":"https://pith.science/pith/IACC3XMQHVVARTQNSBUAVM43XC.json","view_paper":"https://pith.science/paper/IACC3XMQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=cond-mat/0310272&json=true","fetch_graph":"https://pith.science/api/pith-number/IACC3XMQHVVARTQNSBUAVM43XC/graph.json","fetch_events":"https://pith.science/api/pith-number/IACC3XMQHVVARTQNSBUAVM43XC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IACC3XMQHVVARTQNSBUAVM43XC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IACC3XMQHVVARTQNSBUAVM43XC/action/storage_attestation","attest_author":"https://pith.science/pith/IACC3XMQHVVARTQNSBUAVM43XC/action/author_attestation","sign_citation":"https://pith.science/pith/IACC3XMQHVVARTQNSBUAVM43XC/action/citation_signature","submit_replication":"https://pith.science/pith/IACC3XMQHVVARTQNSBUAVM43XC/action/replication_record"}},"created_at":"2026-05-18T01:39:59.046242+00:00","updated_at":"2026-05-18T01:39:59.046242+00:00"}