{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:JR5VG3MALTB6HOHI3SJHFUEU5S","short_pith_number":"pith:JR5VG3MA","schema_version":"1.0","canonical_sha256":"4c7b536d805cc3e3b8e8dc9272d094ec9909698f71a3a48fb7f10110a9bc328d","source":{"kind":"arxiv","id":"1502.05157","version":1},"attestation_state":"computed","paper":{"title":"The Confined X-class Flares of Solar Active Region 2192","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. M. Veronig, J.K. Thalmann, M. Temmer, Y. Su","submitted_at":"2015-02-18T08:46:48Z","abstract_excerpt":"The unusually large NOAA active region 2192, observed in October 2014, was outstanding in its productivity of major two-ribbon flares without coronal mass ejections. On a large scale, a predominantly north-south oriented magnetic system of arcade fields served as a strong, also lateral, confinement for a series of large two-ribbon flares originating from the core of the active region. The large initial separation of the flare ribbons, together with an almost absent growth in ribbon separation, suggests a confined reconnection site high up in the corona. Based on a detailed analysis of the conf"},"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":"1502.05157","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2015-02-18T08:46:48Z","cross_cats_sorted":[],"title_canon_sha256":"596b94fbf85839e073a1de3b74d28516bc84a4118052019035646cbc6cdb905e","abstract_canon_sha256":"ee71c8d0c0090c2b12c7928e6cbbccfda0ad86c15d709b97c4cfcf4756880bcb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:01.000398Z","signature_b64":"Qbwg/JsoXuBPpX4cfBWBedE09YpAZTflOl1vL5V0KLjm70f5W1RIJ1b5Xxb7QScvBAsoItlG388WEI4pu9ooAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4c7b536d805cc3e3b8e8dc9272d094ec9909698f71a3a48fb7f10110a9bc328d","last_reissued_at":"2026-05-18T01:41:00.999701Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:00.999701Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Confined X-class Flares of Solar Active Region 2192","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. M. Veronig, J.K. Thalmann, M. Temmer, Y. Su","submitted_at":"2015-02-18T08:46:48Z","abstract_excerpt":"The unusually large NOAA active region 2192, observed in October 2014, was outstanding in its productivity of major two-ribbon flares without coronal mass ejections. On a large scale, a predominantly north-south oriented magnetic system of arcade fields served as a strong, also lateral, confinement for a series of large two-ribbon flares originating from the core of the active region. The large initial separation of the flare ribbons, together with an almost absent growth in ribbon separation, suggests a confined reconnection site high up in the corona. Based on a detailed analysis of the conf"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1502.05157","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":"1502.05157","created_at":"2026-05-18T01:41:00.999800+00:00"},{"alias_kind":"arxiv_version","alias_value":"1502.05157v1","created_at":"2026-05-18T01:41:00.999800+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1502.05157","created_at":"2026-05-18T01:41:00.999800+00:00"},{"alias_kind":"pith_short_12","alias_value":"JR5VG3MALTB6","created_at":"2026-05-18T12:29:27.538025+00:00"},{"alias_kind":"pith_short_16","alias_value":"JR5VG3MALTB6HOHI","created_at":"2026-05-18T12:29:27.538025+00:00"},{"alias_kind":"pith_short_8","alias_value":"JR5VG3MA","created_at":"2026-05-18T12:29:27.538025+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2501.11345","citing_title":"CME Observations -- from Sun to Impact on Geospace","ref_index":62,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/JR5VG3MALTB6HOHI3SJHFUEU5S","json":"https://pith.science/pith/JR5VG3MALTB6HOHI3SJHFUEU5S.json","graph_json":"https://pith.science/api/pith-number/JR5VG3MALTB6HOHI3SJHFUEU5S/graph.json","events_json":"https://pith.science/api/pith-number/JR5VG3MALTB6HOHI3SJHFUEU5S/events.json","paper":"https://pith.science/paper/JR5VG3MA"},"agent_actions":{"view_html":"https://pith.science/pith/JR5VG3MALTB6HOHI3SJHFUEU5S","download_json":"https://pith.science/pith/JR5VG3MALTB6HOHI3SJHFUEU5S.json","view_paper":"https://pith.science/paper/JR5VG3MA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1502.05157&json=true","fetch_graph":"https://pith.science/api/pith-number/JR5VG3MALTB6HOHI3SJHFUEU5S/graph.json","fetch_events":"https://pith.science/api/pith-number/JR5VG3MALTB6HOHI3SJHFUEU5S/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JR5VG3MALTB6HOHI3SJHFUEU5S/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JR5VG3MALTB6HOHI3SJHFUEU5S/action/storage_attestation","attest_author":"https://pith.science/pith/JR5VG3MALTB6HOHI3SJHFUEU5S/action/author_attestation","sign_citation":"https://pith.science/pith/JR5VG3MALTB6HOHI3SJHFUEU5S/action/citation_signature","submit_replication":"https://pith.science/pith/JR5VG3MALTB6HOHI3SJHFUEU5S/action/replication_record"}},"created_at":"2026-05-18T01:41:00.999800+00:00","updated_at":"2026-05-18T01:41:00.999800+00:00"}