{"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"}