{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:3FJFPRCLP2NTMBZTOSEQ7HUDYC","short_pith_number":"pith:3FJFPRCL","schema_version":"1.0","canonical_sha256":"d95257c44b7e9b36073374890f9e83c0ac02e352b457d76b3a89609de0217ae5","source":{"kind":"arxiv","id":"1711.00622","version":1},"attestation_state":"computed","paper":{"title":"Observation of a Large-scale Quasi-circular Secondary Ribbon associated with Successive Flares and a Halo CME","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Chaowei Jiang, Eun-Kyung Lim, Heesu Yang, Jeongwoo Lee, Jongchul Chae, Kyuhyoun Cho, Kyung-Suk Cho, Pankaj Kumar, Sujin Kim, Vasyl Yurchyshyn","submitted_at":"2017-11-02T06:02:19Z","abstract_excerpt":"Solar flare ribbons provide an important clue to the magnetic reconnection process and associated magnetic field topology in the solar corona. We detected a large-scale secondary flare ribbon of a circular shape that developed in association with two successive M-class flares and one CME. The ribbon revealed interesting properties such as 1) a quasi-circular shape and enclosing the central active region; 2) the size as large as 500\\arcsec\\, by 650\\arcsec\\,, 3) successive brightenings in the clockwise direction at a speed of \\kms{160} starting from the nearest position to the flaring sunspots, "},"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":"1711.00622","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-11-02T06:02:19Z","cross_cats_sorted":[],"title_canon_sha256":"0042678b61c1371116d5393a45455ce5f52b91a9b8cf64c3731af10abefd29ee","abstract_canon_sha256":"ebe24c42b5ba04f9aeb187247a377b0b644e7ffdca02dc45b18f10422597e28a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:28:12.879691Z","signature_b64":"wtUaEsExZzzYx6tzYLVXVkjQTTcxKd7/J/+OLJd6n9fqygZhNVWg/VYgit8nthJ2G8LQQjsiQb+UDErhlf8CAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d95257c44b7e9b36073374890f9e83c0ac02e352b457d76b3a89609de0217ae5","last_reissued_at":"2026-05-18T00:28:12.879150Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:28:12.879150Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Observation of a Large-scale Quasi-circular Secondary Ribbon associated with Successive Flares and a Halo CME","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Chaowei Jiang, Eun-Kyung Lim, Heesu Yang, Jeongwoo Lee, Jongchul Chae, Kyuhyoun Cho, Kyung-Suk Cho, Pankaj Kumar, Sujin Kim, Vasyl Yurchyshyn","submitted_at":"2017-11-02T06:02:19Z","abstract_excerpt":"Solar flare ribbons provide an important clue to the magnetic reconnection process and associated magnetic field topology in the solar corona. We detected a large-scale secondary flare ribbon of a circular shape that developed in association with two successive M-class flares and one CME. The ribbon revealed interesting properties such as 1) a quasi-circular shape and enclosing the central active region; 2) the size as large as 500\\arcsec\\, by 650\\arcsec\\,, 3) successive brightenings in the clockwise direction at a speed of \\kms{160} starting from the nearest position to the flaring sunspots, "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.00622","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":"1711.00622","created_at":"2026-05-18T00:28:12.879221+00:00"},{"alias_kind":"arxiv_version","alias_value":"1711.00622v1","created_at":"2026-05-18T00:28:12.879221+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.00622","created_at":"2026-05-18T00:28:12.879221+00:00"},{"alias_kind":"pith_short_12","alias_value":"3FJFPRCLP2NT","created_at":"2026-05-18T12:30:58.224056+00:00"},{"alias_kind":"pith_short_16","alias_value":"3FJFPRCLP2NTMBZT","created_at":"2026-05-18T12:30:58.224056+00:00"},{"alias_kind":"pith_short_8","alias_value":"3FJFPRCL","created_at":"2026-05-18T12:30:58.224056+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/3FJFPRCLP2NTMBZTOSEQ7HUDYC","json":"https://pith.science/pith/3FJFPRCLP2NTMBZTOSEQ7HUDYC.json","graph_json":"https://pith.science/api/pith-number/3FJFPRCLP2NTMBZTOSEQ7HUDYC/graph.json","events_json":"https://pith.science/api/pith-number/3FJFPRCLP2NTMBZTOSEQ7HUDYC/events.json","paper":"https://pith.science/paper/3FJFPRCL"},"agent_actions":{"view_html":"https://pith.science/pith/3FJFPRCLP2NTMBZTOSEQ7HUDYC","download_json":"https://pith.science/pith/3FJFPRCLP2NTMBZTOSEQ7HUDYC.json","view_paper":"https://pith.science/paper/3FJFPRCL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1711.00622&json=true","fetch_graph":"https://pith.science/api/pith-number/3FJFPRCLP2NTMBZTOSEQ7HUDYC/graph.json","fetch_events":"https://pith.science/api/pith-number/3FJFPRCLP2NTMBZTOSEQ7HUDYC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3FJFPRCLP2NTMBZTOSEQ7HUDYC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3FJFPRCLP2NTMBZTOSEQ7HUDYC/action/storage_attestation","attest_author":"https://pith.science/pith/3FJFPRCLP2NTMBZTOSEQ7HUDYC/action/author_attestation","sign_citation":"https://pith.science/pith/3FJFPRCLP2NTMBZTOSEQ7HUDYC/action/citation_signature","submit_replication":"https://pith.science/pith/3FJFPRCLP2NTMBZTOSEQ7HUDYC/action/replication_record"}},"created_at":"2026-05-18T00:28:12.879221+00:00","updated_at":"2026-05-18T00:28:12.879221+00:00"}