{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:G7R5ZMKWPSDUKFD5CNVYIJP4EE","short_pith_number":"pith:G7R5ZMKW","schema_version":"1.0","canonical_sha256":"37e3dcb1567c8745147d136b8425fc211f42e01ddd218f493511008520e53b21","source":{"kind":"arxiv","id":"1707.00414","version":1},"attestation_state":"computed","paper":{"title":"Polarization Characteristics of Zebra Patterns in Type IV Solar Radio Bursts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"F. Tsuchiya, H. Misawa, Kazutaka Kaneda, K. Iwai, S. Masuda, T. Obara, Y. Katoh","submitted_at":"2017-07-03T06:19:00Z","abstract_excerpt":"The polarization characteristics of zebra patterns (ZPs) in type IV solar bursts were studied. We analyzed 21 ZP events observed by the Assembly of Metric-band Aperture Telescope and Real-time Analysis System between 2010 and 2015 and identified the following characteristics: a degree of circular polarization (DCP) in the range of 0%-70%, a temporal delay of 0-70 ms between the two circularly polarized components (i.e., the right- and left-handed components), and dominant ordinary-mode emission in about 81% of the events. For most events, the relation between the dominant and delayed component"},"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":"1707.00414","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-07-03T06:19:00Z","cross_cats_sorted":[],"title_canon_sha256":"023245220f3b6a0cd9fe49d617d6c00ccf49616f336b34febab0fbe2d1193e97","abstract_canon_sha256":"ab1b4e9f25670c78564eca7bc3877db93c25eba737f490cf6881490f22def8f4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:41:03.452076Z","signature_b64":"0hu49e+8tmwGEIu1bf/2nAgsZw3IWK1sfgMawKYgCZun2w9EW9HCod9oMzORYOCd64obhz2x63OqovV1GybtCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"37e3dcb1567c8745147d136b8425fc211f42e01ddd218f493511008520e53b21","last_reissued_at":"2026-05-18T00:41:03.451366Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:41:03.451366Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Polarization Characteristics of Zebra Patterns in Type IV Solar Radio Bursts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"F. Tsuchiya, H. Misawa, Kazutaka Kaneda, K. Iwai, S. Masuda, T. Obara, Y. Katoh","submitted_at":"2017-07-03T06:19:00Z","abstract_excerpt":"The polarization characteristics of zebra patterns (ZPs) in type IV solar bursts were studied. We analyzed 21 ZP events observed by the Assembly of Metric-band Aperture Telescope and Real-time Analysis System between 2010 and 2015 and identified the following characteristics: a degree of circular polarization (DCP) in the range of 0%-70%, a temporal delay of 0-70 ms between the two circularly polarized components (i.e., the right- and left-handed components), and dominant ordinary-mode emission in about 81% of the events. For most events, the relation between the dominant and delayed component"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1707.00414","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":"1707.00414","created_at":"2026-05-18T00:41:03.451477+00:00"},{"alias_kind":"arxiv_version","alias_value":"1707.00414v1","created_at":"2026-05-18T00:41:03.451477+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1707.00414","created_at":"2026-05-18T00:41:03.451477+00:00"},{"alias_kind":"pith_short_12","alias_value":"G7R5ZMKWPSDU","created_at":"2026-05-18T12:31:15.632608+00:00"},{"alias_kind":"pith_short_16","alias_value":"G7R5ZMKWPSDUKFD5","created_at":"2026-05-18T12:31:15.632608+00:00"},{"alias_kind":"pith_short_8","alias_value":"G7R5ZMKW","created_at":"2026-05-18T12:31:15.632608+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/G7R5ZMKWPSDUKFD5CNVYIJP4EE","json":"https://pith.science/pith/G7R5ZMKWPSDUKFD5CNVYIJP4EE.json","graph_json":"https://pith.science/api/pith-number/G7R5ZMKWPSDUKFD5CNVYIJP4EE/graph.json","events_json":"https://pith.science/api/pith-number/G7R5ZMKWPSDUKFD5CNVYIJP4EE/events.json","paper":"https://pith.science/paper/G7R5ZMKW"},"agent_actions":{"view_html":"https://pith.science/pith/G7R5ZMKWPSDUKFD5CNVYIJP4EE","download_json":"https://pith.science/pith/G7R5ZMKWPSDUKFD5CNVYIJP4EE.json","view_paper":"https://pith.science/paper/G7R5ZMKW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1707.00414&json=true","fetch_graph":"https://pith.science/api/pith-number/G7R5ZMKWPSDUKFD5CNVYIJP4EE/graph.json","fetch_events":"https://pith.science/api/pith-number/G7R5ZMKWPSDUKFD5CNVYIJP4EE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/G7R5ZMKWPSDUKFD5CNVYIJP4EE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/G7R5ZMKWPSDUKFD5CNVYIJP4EE/action/storage_attestation","attest_author":"https://pith.science/pith/G7R5ZMKWPSDUKFD5CNVYIJP4EE/action/author_attestation","sign_citation":"https://pith.science/pith/G7R5ZMKWPSDUKFD5CNVYIJP4EE/action/citation_signature","submit_replication":"https://pith.science/pith/G7R5ZMKWPSDUKFD5CNVYIJP4EE/action/replication_record"}},"created_at":"2026-05-18T00:41:03.451477+00:00","updated_at":"2026-05-18T00:41:03.451477+00:00"}