{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:XNS5ITOX3SKKZZI4NVVC7DCQS2","short_pith_number":"pith:XNS5ITOX","schema_version":"1.0","canonical_sha256":"bb65d44dd7dc94ace51c6d6a2f8c509685e76190d213a3e017dd439e10f6b34c","source":{"kind":"arxiv","id":"1007.2735","version":2},"attestation_state":"computed","paper":{"title":"Synthetic solar X-ray flares time series since AD 1968 /s2","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"B. Komitov, K. Koleva, M. Dechev, P. Duchlev","submitted_at":"2010-07-16T10:32:30Z","abstract_excerpt":"On the base of the most qualitative GOES satellites data for the period AD 1980-2009 and multiple regression model the \"synthetic\" series of the monthly numbers of soft X-ray flares (separately for the classes C, M, X and total numbers) were built for the epoch AD 1968-2009. The earlier parts of the series before AD 1980 were derived on the base of the mentioned model . The monthly numbers of radio bursts at four frequencies (29-33, 609, 8800 and 15400 MHz) and the radio flux at 2800 MHz (F10.7) are used as factors. The relationships are very strong (correlation coefficients R are from 0.79 to"},"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":"1007.2735","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2010-07-16T10:32:30Z","cross_cats_sorted":[],"title_canon_sha256":"aab1719c00a96a51f1bf8fa142ddb9da720d9b4dd01211470d508ee75584ce59","abstract_canon_sha256":"dc5aa74a6fa6c11326ef16f97d38af6359e1830ce61f0071f141e5d9d951a384"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:34:36.998377Z","signature_b64":"JzeS6ygWAfws1zicooyN2Db6vlg8HST//1ZOygkXKtFvGP6GFaTR4nlqPdd1pR6EHbj++c2oJVeE3YyoZ+G3Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bb65d44dd7dc94ace51c6d6a2f8c509685e76190d213a3e017dd439e10f6b34c","last_reissued_at":"2026-05-18T04:34:36.997875Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:34:36.997875Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Synthetic solar X-ray flares time series since AD 1968 /s2","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"B. Komitov, K. Koleva, M. Dechev, P. Duchlev","submitted_at":"2010-07-16T10:32:30Z","abstract_excerpt":"On the base of the most qualitative GOES satellites data for the period AD 1980-2009 and multiple regression model the \"synthetic\" series of the monthly numbers of soft X-ray flares (separately for the classes C, M, X and total numbers) were built for the epoch AD 1968-2009. The earlier parts of the series before AD 1980 were derived on the base of the mentioned model . The monthly numbers of radio bursts at four frequencies (29-33, 609, 8800 and 15400 MHz) and the radio flux at 2800 MHz (F10.7) are used as factors. The relationships are very strong (correlation coefficients R are from 0.79 to"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1007.2735","kind":"arxiv","version":2},"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":"1007.2735","created_at":"2026-05-18T04:34:36.997949+00:00"},{"alias_kind":"arxiv_version","alias_value":"1007.2735v2","created_at":"2026-05-18T04:34:36.997949+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1007.2735","created_at":"2026-05-18T04:34:36.997949+00:00"},{"alias_kind":"pith_short_12","alias_value":"XNS5ITOX3SKK","created_at":"2026-05-18T12:26:17.028572+00:00"},{"alias_kind":"pith_short_16","alias_value":"XNS5ITOX3SKKZZI4","created_at":"2026-05-18T12:26:17.028572+00:00"},{"alias_kind":"pith_short_8","alias_value":"XNS5ITOX","created_at":"2026-05-18T12:26:17.028572+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/XNS5ITOX3SKKZZI4NVVC7DCQS2","json":"https://pith.science/pith/XNS5ITOX3SKKZZI4NVVC7DCQS2.json","graph_json":"https://pith.science/api/pith-number/XNS5ITOX3SKKZZI4NVVC7DCQS2/graph.json","events_json":"https://pith.science/api/pith-number/XNS5ITOX3SKKZZI4NVVC7DCQS2/events.json","paper":"https://pith.science/paper/XNS5ITOX"},"agent_actions":{"view_html":"https://pith.science/pith/XNS5ITOX3SKKZZI4NVVC7DCQS2","download_json":"https://pith.science/pith/XNS5ITOX3SKKZZI4NVVC7DCQS2.json","view_paper":"https://pith.science/paper/XNS5ITOX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1007.2735&json=true","fetch_graph":"https://pith.science/api/pith-number/XNS5ITOX3SKKZZI4NVVC7DCQS2/graph.json","fetch_events":"https://pith.science/api/pith-number/XNS5ITOX3SKKZZI4NVVC7DCQS2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XNS5ITOX3SKKZZI4NVVC7DCQS2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XNS5ITOX3SKKZZI4NVVC7DCQS2/action/storage_attestation","attest_author":"https://pith.science/pith/XNS5ITOX3SKKZZI4NVVC7DCQS2/action/author_attestation","sign_citation":"https://pith.science/pith/XNS5ITOX3SKKZZI4NVVC7DCQS2/action/citation_signature","submit_replication":"https://pith.science/pith/XNS5ITOX3SKKZZI4NVVC7DCQS2/action/replication_record"}},"created_at":"2026-05-18T04:34:36.997949+00:00","updated_at":"2026-05-18T04:34:36.997949+00:00"}