{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:NJSP6QCUX5SL3FATUD3MLZV6PZ","short_pith_number":"pith:NJSP6QCU","schema_version":"1.0","canonical_sha256":"6a64ff4054bf64bd9413a0f6c5e6be7e59c98720e06c88a5f7d4bdf797e22825","source":{"kind":"arxiv","id":"1601.05312","version":1},"attestation_state":"computed","paper":{"title":"Microwave Type III Pair Bursts in Solar Flares","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Baolin Tan, Chengming Tan, Guangli Huang, Hana Meszarosova, Marian Karlicky","submitted_at":"2016-01-20T15:53:23Z","abstract_excerpt":"Solar microwave type III pair burst is composed of normal and reverse-sloped (RS) burst branches with oppositely fast frequency drifts. It is the most sensitive signature of the primary energy release and electron accelerations in flares. This work reported 11 microwave type III pair events in 9 flares observed by radio spectrometers in China and the Czech Republic at frequency of 0.80 - 7.60 GHz during 1994 - 2014. These type III pairs occurred in flare impulsive and postflare phases with separate frequency in range of 1.08 - 3.42 GHz and frequency gap 10 - 1700 MHz. The frequency drift incre"},"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":"1601.05312","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-01-20T15:53:23Z","cross_cats_sorted":[],"title_canon_sha256":"417141ab46a7c1a0a2073e8281c34be18b2435a3c50a8c1eeb8631de195bf486","abstract_canon_sha256":"8840b01663675f3879c24b7aaace307dfde227e2db77bbe0547f172467178402"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:19:01.276029Z","signature_b64":"rXBf7RtyC1NeERhQTqnGBRiagi6XrO8w75ZPZjlrOtBMQG60rNfvBIM4UngDZR1UakxA0qprzlyrxW3J5eLlAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6a64ff4054bf64bd9413a0f6c5e6be7e59c98720e06c88a5f7d4bdf797e22825","last_reissued_at":"2026-05-18T01:19:01.275585Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:19:01.275585Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Microwave Type III Pair Bursts in Solar Flares","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Baolin Tan, Chengming Tan, Guangli Huang, Hana Meszarosova, Marian Karlicky","submitted_at":"2016-01-20T15:53:23Z","abstract_excerpt":"Solar microwave type III pair burst is composed of normal and reverse-sloped (RS) burst branches with oppositely fast frequency drifts. It is the most sensitive signature of the primary energy release and electron accelerations in flares. This work reported 11 microwave type III pair events in 9 flares observed by radio spectrometers in China and the Czech Republic at frequency of 0.80 - 7.60 GHz during 1994 - 2014. These type III pairs occurred in flare impulsive and postflare phases with separate frequency in range of 1.08 - 3.42 GHz and frequency gap 10 - 1700 MHz. The frequency drift incre"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1601.05312","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":"1601.05312","created_at":"2026-05-18T01:19:01.275650+00:00"},{"alias_kind":"arxiv_version","alias_value":"1601.05312v1","created_at":"2026-05-18T01:19:01.275650+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1601.05312","created_at":"2026-05-18T01:19:01.275650+00:00"},{"alias_kind":"pith_short_12","alias_value":"NJSP6QCUX5SL","created_at":"2026-05-18T12:30:32.724797+00:00"},{"alias_kind":"pith_short_16","alias_value":"NJSP6QCUX5SL3FAT","created_at":"2026-05-18T12:30:32.724797+00:00"},{"alias_kind":"pith_short_8","alias_value":"NJSP6QCU","created_at":"2026-05-18T12:30:32.724797+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/NJSP6QCUX5SL3FATUD3MLZV6PZ","json":"https://pith.science/pith/NJSP6QCUX5SL3FATUD3MLZV6PZ.json","graph_json":"https://pith.science/api/pith-number/NJSP6QCUX5SL3FATUD3MLZV6PZ/graph.json","events_json":"https://pith.science/api/pith-number/NJSP6QCUX5SL3FATUD3MLZV6PZ/events.json","paper":"https://pith.science/paper/NJSP6QCU"},"agent_actions":{"view_html":"https://pith.science/pith/NJSP6QCUX5SL3FATUD3MLZV6PZ","download_json":"https://pith.science/pith/NJSP6QCUX5SL3FATUD3MLZV6PZ.json","view_paper":"https://pith.science/paper/NJSP6QCU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1601.05312&json=true","fetch_graph":"https://pith.science/api/pith-number/NJSP6QCUX5SL3FATUD3MLZV6PZ/graph.json","fetch_events":"https://pith.science/api/pith-number/NJSP6QCUX5SL3FATUD3MLZV6PZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NJSP6QCUX5SL3FATUD3MLZV6PZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NJSP6QCUX5SL3FATUD3MLZV6PZ/action/storage_attestation","attest_author":"https://pith.science/pith/NJSP6QCUX5SL3FATUD3MLZV6PZ/action/author_attestation","sign_citation":"https://pith.science/pith/NJSP6QCUX5SL3FATUD3MLZV6PZ/action/citation_signature","submit_replication":"https://pith.science/pith/NJSP6QCUX5SL3FATUD3MLZV6PZ/action/replication_record"}},"created_at":"2026-05-18T01:19:01.275650+00:00","updated_at":"2026-05-18T01:19:01.275650+00:00"}