{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:4NCHCM5JWMW63ASLAH3USYYH2T","short_pith_number":"pith:4NCHCM5J","schema_version":"1.0","canonical_sha256":"e3447133a9b32ded824b01f7496307d4c0e198bdfbb95487da04c376189c445b","source":{"kind":"arxiv","id":"1011.4035","version":3},"attestation_state":"computed","paper":{"title":"Spontaneous current-layer fragmentation and cascading reconnection in solar flares: I. Model and analysis","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.plasm-ph"],"primary_cat":"astro-ph.SR","authors_text":"Jan Sk\\'ala, J\\\"org B\\\"uchner, Marian Karlick\\'y, Miroslav B\\'arta","submitted_at":"2010-11-17T19:41:42Z","abstract_excerpt":"Magnetic reconnection is commonly considered as a mechanism of solar (eruptive) flares. A deeper study of this scenario reveals, however, a number of open issues. Among them is the fundamental question, how the magnetic energy is transferred from large, accumulation scales to plasma scales where its actual dissipation takes place. In order to investigate this transfer over a broad range of scales we address this question by means of a high-resolution MHD simulation. The simulation results indicate that the magnetic-energy transfer to small scales is realized via a cascade of consecutive smalle"},"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":"1011.4035","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2010-11-17T19:41:42Z","cross_cats_sorted":["physics.plasm-ph"],"title_canon_sha256":"fd7bd048945b8a738968e73b2ac619b057783a00db3c59e324147a173768a714","abstract_canon_sha256":"269b85d733124e72cff044595543dbeddc1409bb2703e3a7c197347362fa8aed"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:23:36.378906Z","signature_b64":"17OQCC3c84Dn0MEnOB5IqYe/s+N9L6RZpGto/Ha8+MyxWX9dwtbuieVQWRtbDp/WAvAoWNqulQODugxy7GToDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e3447133a9b32ded824b01f7496307d4c0e198bdfbb95487da04c376189c445b","last_reissued_at":"2026-05-18T02:23:36.378230Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:23:36.378230Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Spontaneous current-layer fragmentation and cascading reconnection in solar flares: I. Model and analysis","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.plasm-ph"],"primary_cat":"astro-ph.SR","authors_text":"Jan Sk\\'ala, J\\\"org B\\\"uchner, Marian Karlick\\'y, Miroslav B\\'arta","submitted_at":"2010-11-17T19:41:42Z","abstract_excerpt":"Magnetic reconnection is commonly considered as a mechanism of solar (eruptive) flares. A deeper study of this scenario reveals, however, a number of open issues. Among them is the fundamental question, how the magnetic energy is transferred from large, accumulation scales to plasma scales where its actual dissipation takes place. In order to investigate this transfer over a broad range of scales we address this question by means of a high-resolution MHD simulation. The simulation results indicate that the magnetic-energy transfer to small scales is realized via a cascade of consecutive smalle"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1011.4035","kind":"arxiv","version":3},"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":"1011.4035","created_at":"2026-05-18T02:23:36.378343+00:00"},{"alias_kind":"arxiv_version","alias_value":"1011.4035v3","created_at":"2026-05-18T02:23:36.378343+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1011.4035","created_at":"2026-05-18T02:23:36.378343+00:00"},{"alias_kind":"pith_short_12","alias_value":"4NCHCM5JWMW6","created_at":"2026-05-18T12:26:03.138858+00:00"},{"alias_kind":"pith_short_16","alias_value":"4NCHCM5JWMW63ASL","created_at":"2026-05-18T12:26:03.138858+00:00"},{"alias_kind":"pith_short_8","alias_value":"4NCHCM5J","created_at":"2026-05-18T12:26:03.138858+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/4NCHCM5JWMW63ASLAH3USYYH2T","json":"https://pith.science/pith/4NCHCM5JWMW63ASLAH3USYYH2T.json","graph_json":"https://pith.science/api/pith-number/4NCHCM5JWMW63ASLAH3USYYH2T/graph.json","events_json":"https://pith.science/api/pith-number/4NCHCM5JWMW63ASLAH3USYYH2T/events.json","paper":"https://pith.science/paper/4NCHCM5J"},"agent_actions":{"view_html":"https://pith.science/pith/4NCHCM5JWMW63ASLAH3USYYH2T","download_json":"https://pith.science/pith/4NCHCM5JWMW63ASLAH3USYYH2T.json","view_paper":"https://pith.science/paper/4NCHCM5J","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1011.4035&json=true","fetch_graph":"https://pith.science/api/pith-number/4NCHCM5JWMW63ASLAH3USYYH2T/graph.json","fetch_events":"https://pith.science/api/pith-number/4NCHCM5JWMW63ASLAH3USYYH2T/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4NCHCM5JWMW63ASLAH3USYYH2T/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4NCHCM5JWMW63ASLAH3USYYH2T/action/storage_attestation","attest_author":"https://pith.science/pith/4NCHCM5JWMW63ASLAH3USYYH2T/action/author_attestation","sign_citation":"https://pith.science/pith/4NCHCM5JWMW63ASLAH3USYYH2T/action/citation_signature","submit_replication":"https://pith.science/pith/4NCHCM5JWMW63ASLAH3USYYH2T/action/replication_record"}},"created_at":"2026-05-18T02:23:36.378343+00:00","updated_at":"2026-05-18T02:23:36.378343+00:00"}