{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:VFJIYHL5SOG34LEL5KF2HG46NX","short_pith_number":"pith:VFJIYHL5","schema_version":"1.0","canonical_sha256":"a9528c1d7d938dbe2c8bea8ba39b9e6de441a69061a775def30fe2ded6892e10","source":{"kind":"arxiv","id":"2005.09419","version":1},"attestation_state":"computed","paper":{"title":"Interferometric Imaging with LOFAR Remote Baselines of the Fine Structures of a Solar Type IIIb Radio Burst","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Andrzej Krankowski, Bartosz Dabrowski, Christian Vocks, Chuanbing Wang, Diana E. Morosan, Gottfried Mann, Jasmina Magdalenic, Mario M. Bisi, Peijin Zhang, Pietro Zucca, Sarrvesh Seethapuram Sridhar","submitted_at":"2020-05-17T14:47:50Z","abstract_excerpt":"Context. Solar radio bursts originate mainly from high energy electrons accelerated in solar eruptions like solar flares, jets, and coronal mass ejections. A subcategory of solar radio bursts with short time duration may be used as a proxy to understand the wave generation and propagation within the corona. Aims. Complete case studies of the source size, position and kinematics of short term bursts are very rare due to instrumental limitations. A comprehensive multi-frequency spectroscopic and imaging study was carried out of a clear example of a solar type IIIb-III pair. Methods. In this work"},"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":"2005.09419","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2020-05-17T14:47:50Z","cross_cats_sorted":[],"title_canon_sha256":"7c4e4e94e22691c195622171728dd42b62eacb0bd9aae2caf29e7c9eae6ce2d8","abstract_canon_sha256":"7ce48b3a7cd3f34af61bb10dfa6bb0dcfbfe6026af10cde2162a2f9b320c2b7f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:21:01.303156Z","signature_b64":"VhFDoqHT8Rn/Zby16DxFq/w/XgIzW6Yl8P6NAFs7oecLj6BKg3Euc/gM55al6klPTM6Ns9m4F9rcjppFUoltDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a9528c1d7d938dbe2c8bea8ba39b9e6de441a69061a775def30fe2ded6892e10","last_reissued_at":"2026-07-05T01:21:01.302645Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:21:01.302645Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Interferometric Imaging with LOFAR Remote Baselines of the Fine Structures of a Solar Type IIIb Radio Burst","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Andrzej Krankowski, Bartosz Dabrowski, Christian Vocks, Chuanbing Wang, Diana E. Morosan, Gottfried Mann, Jasmina Magdalenic, Mario M. Bisi, Peijin Zhang, Pietro Zucca, Sarrvesh Seethapuram Sridhar","submitted_at":"2020-05-17T14:47:50Z","abstract_excerpt":"Context. Solar radio bursts originate mainly from high energy electrons accelerated in solar eruptions like solar flares, jets, and coronal mass ejections. A subcategory of solar radio bursts with short time duration may be used as a proxy to understand the wave generation and propagation within the corona. Aims. Complete case studies of the source size, position and kinematics of short term bursts are very rare due to instrumental limitations. A comprehensive multi-frequency spectroscopic and imaging study was carried out of a clear example of a solar type IIIb-III pair. Methods. In this work"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2005.09419","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/2005.09419/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":"2005.09419","created_at":"2026-07-05T01:21:01.302709+00:00"},{"alias_kind":"arxiv_version","alias_value":"2005.09419v1","created_at":"2026-07-05T01:21:01.302709+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2005.09419","created_at":"2026-07-05T01:21:01.302709+00:00"},{"alias_kind":"pith_short_12","alias_value":"VFJIYHL5SOG3","created_at":"2026-07-05T01:21:01.302709+00:00"},{"alias_kind":"pith_short_16","alias_value":"VFJIYHL5SOG34LEL","created_at":"2026-07-05T01:21:01.302709+00:00"},{"alias_kind":"pith_short_8","alias_value":"VFJIYHL5","created_at":"2026-07-05T01:21:01.302709+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/VFJIYHL5SOG34LEL5KF2HG46NX","json":"https://pith.science/pith/VFJIYHL5SOG34LEL5KF2HG46NX.json","graph_json":"https://pith.science/api/pith-number/VFJIYHL5SOG34LEL5KF2HG46NX/graph.json","events_json":"https://pith.science/api/pith-number/VFJIYHL5SOG34LEL5KF2HG46NX/events.json","paper":"https://pith.science/paper/VFJIYHL5"},"agent_actions":{"view_html":"https://pith.science/pith/VFJIYHL5SOG34LEL5KF2HG46NX","download_json":"https://pith.science/pith/VFJIYHL5SOG34LEL5KF2HG46NX.json","view_paper":"https://pith.science/paper/VFJIYHL5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2005.09419&json=true","fetch_graph":"https://pith.science/api/pith-number/VFJIYHL5SOG34LEL5KF2HG46NX/graph.json","fetch_events":"https://pith.science/api/pith-number/VFJIYHL5SOG34LEL5KF2HG46NX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VFJIYHL5SOG34LEL5KF2HG46NX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VFJIYHL5SOG34LEL5KF2HG46NX/action/storage_attestation","attest_author":"https://pith.science/pith/VFJIYHL5SOG34LEL5KF2HG46NX/action/author_attestation","sign_citation":"https://pith.science/pith/VFJIYHL5SOG34LEL5KF2HG46NX/action/citation_signature","submit_replication":"https://pith.science/pith/VFJIYHL5SOG34LEL5KF2HG46NX/action/replication_record"}},"created_at":"2026-07-05T01:21:01.302709+00:00","updated_at":"2026-07-05T01:21:01.302709+00:00"}