{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2006:FKIVNVAQZH3ECGUW44HVGHD4G3","short_pith_number":"pith:FKIVNVAQ","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"},"canonical_sha256":"2a9156d410c9f6411a96e70f531c7c36e556df1fc3cc8a93b5af930d64cd4fef","source":{"kind":"arxiv","id":"astro-ph/0609197","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/0609197","created_at":"2026-05-18T04:28:57Z"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0609197v2","created_at":"2026-05-18T04:28:57Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0609197","created_at":"2026-05-18T04:28:57Z"},{"alias_kind":"pith_short_12","alias_value":"FKIVNVAQZH3E","created_at":"2026-05-18T12:25:53Z"},{"alias_kind":"pith_short_16","alias_value":"FKIVNVAQZH3ECGUW","created_at":"2026-05-18T12:25:53Z"},{"alias_kind":"pith_short_8","alias_value":"FKIVNVAQ","created_at":"2026-05-18T12:25:53Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2006:FKIVNVAQZH3ECGUW44HVGHD4G3","target":"record","payload":{"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"},"canonical_sha256":"2a9156d410c9f6411a96e70f531c7c36e556df1fc3cc8a93b5af930d64cd4fef","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"},"source_kind":"arxiv","source_id":"astro-ph/0609197","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T04:28:57Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"39fCSK3nxeCFDdNsn2Z9e4HzfdjhojdRktuO9pY43BKs/kou185uafULCW5zAMZlN8JyZyBvxXMjVlRN+w5FAw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-31T23:23:28.385685Z"},"content_sha256":"ea1366543c3a1a162df957d60c7fcae38febafcdede43be9f6cd86084299d405","schema_version":"1.0","event_id":"sha256:ea1366543c3a1a162df957d60c7fcae38febafcdede43be9f6cd86084299d405"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2006:FKIVNVAQZH3ECGUW44HVGHD4G3","target":"graph","payload":{"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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T04:28:57Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"BnGBZC58LEin4ZAfiw6k3S67Im8e7DbG2QGpNUYaVfbIqqM+wdKltFsjMx4zf3X2Oi/R8zcq38p30QTTqMGsCA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-31T23:23:28.386486Z"},"content_sha256":"9e80dbbd1818e58f7d0607be7638396b99288628caad436e723c6bcc60fb2d58","schema_version":"1.0","event_id":"sha256:9e80dbbd1818e58f7d0607be7638396b99288628caad436e723c6bcc60fb2d58"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/FKIVNVAQZH3ECGUW44HVGHD4G3/bundle.json","state_url":"https://pith.science/pith/FKIVNVAQZH3ECGUW44HVGHD4G3/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/FKIVNVAQZH3ECGUW44HVGHD4G3/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-05-31T23:23:28Z","links":{"resolver":"https://pith.science/pith/FKIVNVAQZH3ECGUW44HVGHD4G3","bundle":"https://pith.science/pith/FKIVNVAQZH3ECGUW44HVGHD4G3/bundle.json","state":"https://pith.science/pith/FKIVNVAQZH3ECGUW44HVGHD4G3/state.json","well_known_bundle":"https://pith.science/.well-known/pith/FKIVNVAQZH3ECGUW44HVGHD4G3/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2006:FKIVNVAQZH3ECGUW44HVGHD4G3","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"696eb25010920cc713af1b6c9bea97a81039c91144ca05dac19ee9898ffb76fe","cross_cats_sorted":[],"license":"","primary_cat":"astro-ph","submitted_at":"2006-09-07T14:09:07Z","title_canon_sha256":"6c48678c5554986242cbfe475ae28d5cc1d3155797b8e1fe6a7e7d325086776b"},"schema_version":"1.0","source":{"id":"astro-ph/0609197","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/0609197","created_at":"2026-05-18T04:28:57Z"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0609197v2","created_at":"2026-05-18T04:28:57Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0609197","created_at":"2026-05-18T04:28:57Z"},{"alias_kind":"pith_short_12","alias_value":"FKIVNVAQZH3E","created_at":"2026-05-18T12:25:53Z"},{"alias_kind":"pith_short_16","alias_value":"FKIVNVAQZH3ECGUW","created_at":"2026-05-18T12:25:53Z"},{"alias_kind":"pith_short_8","alias_value":"FKIVNVAQ","created_at":"2026-05-18T12:25:53Z"}],"graph_snapshots":[{"event_id":"sha256:9e80dbbd1818e58f7d0607be7638396b99288628caad436e723c6bcc60fb2d58","target":"graph","created_at":"2026-05-18T04:28:57Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"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","authors_text":"N. Gopalswamy, R. A. Howard, S. Akiyama, S. Yashiro","cross_cats":[],"headline":"","license":"","primary_cat":"astro-ph","submitted_at":"2006-09-07T14:09:07Z","title":"Different Power-law Indices in the Frequency Distributions of Flares with and without Coronal Mass Ejections"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0609197","kind":"arxiv","version":2},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:ea1366543c3a1a162df957d60c7fcae38febafcdede43be9f6cd86084299d405","target":"record","created_at":"2026-05-18T04:28:57Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"696eb25010920cc713af1b6c9bea97a81039c91144ca05dac19ee9898ffb76fe","cross_cats_sorted":[],"license":"","primary_cat":"astro-ph","submitted_at":"2006-09-07T14:09:07Z","title_canon_sha256":"6c48678c5554986242cbfe475ae28d5cc1d3155797b8e1fe6a7e7d325086776b"},"schema_version":"1.0","source":{"id":"astro-ph/0609197","kind":"arxiv","version":2}},"canonical_sha256":"2a9156d410c9f6411a96e70f531c7c36e556df1fc3cc8a93b5af930d64cd4fef","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"2a9156d410c9f6411a96e70f531c7c36e556df1fc3cc8a93b5af930d64cd4fef","first_computed_at":"2026-05-18T04:28:57.843645Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T04:28:57.843645Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"bfhulnRFbmF2aHF2Mu5iF3bLMHJOHrldu7vMUdqnCSnB/tL4yCHxfWCn6Scaupkp3/UHPw/0wEL4zJ7YdIUGBA==","signature_status":"signed_v1","signed_at":"2026-05-18T04:28:57.844143Z","signed_message":"canonical_sha256_bytes"},"source_id":"astro-ph/0609197","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:ea1366543c3a1a162df957d60c7fcae38febafcdede43be9f6cd86084299d405","sha256:9e80dbbd1818e58f7d0607be7638396b99288628caad436e723c6bcc60fb2d58"],"state_sha256":"e218d5d6da1b45d03106c808883c229f91c1786eeeab5961ae9c3fa72e4406fc"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"ZldkL+2fkikXVJTAeWIAUpyE5IGMuSqCQcebfZ2xFvMqL19Een+J6D6zu68fPLJ1tQfs+qzhX+Atp3f/QAKUBA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-31T23:23:28.390851Z","bundle_sha256":"a53968ea7cab698bd202c2ae066b111061b06be89b32e9d8a5a5e05d58ca7a7a"}}