{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:FKIVNVAQZH3ECGUW44HVGHD4G3","short_pith_number":"pith:FKIVNVAQ","schema_version":"1.0","canonical_sha256":"2a9156d410c9f6411a96e70f531c7c36e556df1fc3cc8a93b5af930d64cd4fef","source":{"kind":"arxiv","id":"astro-ph/0609197","version":2},"attestation_state":"computed","paper":{"title":"Different Power-law Indices in the Frequency Distributions of Flares with and without Coronal Mass Ejections","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"N. Gopalswamy, R. A. Howard, S. Akiyama, S. Yashiro","submitted_at":"2006-09-07T14:09:07Z","abstract_excerpt":"We investigated the frequency distributions of flares with and without coronal mass ejections (CMEs) as a function of flare parameters (peak flux, fluence, and duration of soft X-ray flares). We used CMEs observed by the Large Angle and Spectrometric Coronagraph (LASCO) on board the Solar and Heliospheric Observatory (SOHO) mission and soft X-ray flares (C3.2 and above) observed by the GOES satellites during 1996 to 2005. We found that the distributions obey a power-law of the form: dN/dX~X^-alpha, where X is a flare parameter and dN is the number of events recorded within the interval [X, X+d"},"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":"astro-ph/0609197","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-09-07T14:09:07Z","cross_cats_sorted":[],"title_canon_sha256":"6c48678c5554986242cbfe475ae28d5cc1d3155797b8e1fe6a7e7d325086776b","abstract_canon_sha256":"696eb25010920cc713af1b6c9bea97a81039c91144ca05dac19ee9898ffb76fe"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:28:57.844143Z","signature_b64":"bfhulnRFbmF2aHF2Mu5iF3bLMHJOHrldu7vMUdqnCSnB/tL4yCHxfWCn6Scaupkp3/UHPw/0wEL4zJ7YdIUGBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2a9156d410c9f6411a96e70f531c7c36e556df1fc3cc8a93b5af930d64cd4fef","last_reissued_at":"2026-05-18T04:28:57.843645Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:28:57.843645Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Different Power-law Indices in the Frequency Distributions of Flares with and without Coronal Mass Ejections","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"N. Gopalswamy, R. A. Howard, S. Akiyama, S. Yashiro","submitted_at":"2006-09-07T14:09:07Z","abstract_excerpt":"We investigated the frequency distributions of flares with and without coronal mass ejections (CMEs) as a function of flare parameters (peak flux, fluence, and duration of soft X-ray flares). We used CMEs observed by the Large Angle and Spectrometric Coronagraph (LASCO) on board the Solar and Heliospheric Observatory (SOHO) mission and soft X-ray flares (C3.2 and above) observed by the GOES satellites during 1996 to 2005. We found that the distributions obey a power-law of the form: dN/dX~X^-alpha, where X is a flare parameter and dN is the number of events recorded within the interval [X, X+d"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0609197","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":"astro-ph/0609197","created_at":"2026-05-18T04:28:57.843718+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0609197v2","created_at":"2026-05-18T04:28:57.843718+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0609197","created_at":"2026-05-18T04:28:57.843718+00:00"},{"alias_kind":"pith_short_12","alias_value":"FKIVNVAQZH3E","created_at":"2026-05-18T12:25:53.939244+00:00"},{"alias_kind":"pith_short_16","alias_value":"FKIVNVAQZH3ECGUW","created_at":"2026-05-18T12:25:53.939244+00:00"},{"alias_kind":"pith_short_8","alias_value":"FKIVNVAQ","created_at":"2026-05-18T12:25:53.939244+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/FKIVNVAQZH3ECGUW44HVGHD4G3","json":"https://pith.science/pith/FKIVNVAQZH3ECGUW44HVGHD4G3.json","graph_json":"https://pith.science/api/pith-number/FKIVNVAQZH3ECGUW44HVGHD4G3/graph.json","events_json":"https://pith.science/api/pith-number/FKIVNVAQZH3ECGUW44HVGHD4G3/events.json","paper":"https://pith.science/paper/FKIVNVAQ"},"agent_actions":{"view_html":"https://pith.science/pith/FKIVNVAQZH3ECGUW44HVGHD4G3","download_json":"https://pith.science/pith/FKIVNVAQZH3ECGUW44HVGHD4G3.json","view_paper":"https://pith.science/paper/FKIVNVAQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0609197&json=true","fetch_graph":"https://pith.science/api/pith-number/FKIVNVAQZH3ECGUW44HVGHD4G3/graph.json","fetch_events":"https://pith.science/api/pith-number/FKIVNVAQZH3ECGUW44HVGHD4G3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FKIVNVAQZH3ECGUW44HVGHD4G3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FKIVNVAQZH3ECGUW44HVGHD4G3/action/storage_attestation","attest_author":"https://pith.science/pith/FKIVNVAQZH3ECGUW44HVGHD4G3/action/author_attestation","sign_citation":"https://pith.science/pith/FKIVNVAQZH3ECGUW44HVGHD4G3/action/citation_signature","submit_replication":"https://pith.science/pith/FKIVNVAQZH3ECGUW44HVGHD4G3/action/replication_record"}},"created_at":"2026-05-18T04:28:57.843718+00:00","updated_at":"2026-05-18T04:28:57.843718+00:00"}