{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2014:IXCJJ2VIVAXKNJFGHR2UTRKXO4","short_pith_number":"pith:IXCJJ2VI","canonical_record":{"source":{"id":"1410.3303","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-10-13T13:38:58Z","cross_cats_sorted":["physics.space-ph"],"title_canon_sha256":"8a4721baada9b1501fc4bc1bef78ee083439390e9f5f1aded7bd454575ee474a","abstract_canon_sha256":"7f79238e5c52689595effa3b00cb906498f37a0f5d4a60f09a379c8b752e31d1"},"schema_version":"1.0"},"canonical_sha256":"45c494eaa8a82ea6a4a63c7549c55777187618ba29d14e2ff4b976c3375980cf","source":{"kind":"arxiv","id":"1410.3303","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1410.3303","created_at":"2026-05-18T01:41:48Z"},{"alias_kind":"arxiv_version","alias_value":"1410.3303v1","created_at":"2026-05-18T01:41:48Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1410.3303","created_at":"2026-05-18T01:41:48Z"},{"alias_kind":"pith_short_12","alias_value":"IXCJJ2VIVAXK","created_at":"2026-05-18T12:28:33Z"},{"alias_kind":"pith_short_16","alias_value":"IXCJJ2VIVAXKNJFG","created_at":"2026-05-18T12:28:33Z"},{"alias_kind":"pith_short_8","alias_value":"IXCJJ2VI","created_at":"2026-05-18T12:28:33Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2014:IXCJJ2VIVAXKNJFGHR2UTRKXO4","target":"record","payload":{"canonical_record":{"source":{"id":"1410.3303","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-10-13T13:38:58Z","cross_cats_sorted":["physics.space-ph"],"title_canon_sha256":"8a4721baada9b1501fc4bc1bef78ee083439390e9f5f1aded7bd454575ee474a","abstract_canon_sha256":"7f79238e5c52689595effa3b00cb906498f37a0f5d4a60f09a379c8b752e31d1"},"schema_version":"1.0"},"canonical_sha256":"45c494eaa8a82ea6a4a63c7549c55777187618ba29d14e2ff4b976c3375980cf","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:48.872349Z","signature_b64":"lFRyuEWV/Z7pcg7kvuMPQyAlAHY1dXBAEMIiIR6fU4E9ykRjdemfD710DOpUenhvuqskVUNVId/etZ1ShdKWAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"45c494eaa8a82ea6a4a63c7549c55777187618ba29d14e2ff4b976c3375980cf","last_reissued_at":"2026-05-18T01:41:48.871874Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:48.871874Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1410.3303","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:41:48Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"BarFxWok0JGqPqlF/VEH0rHZIbxt6UEMxUh10PEAc14iKpxZ1l++zmbmb1bv1kQX24+HHxtLy+0kTRASJ1TUCQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-06T20:07:49.906560Z"},"content_sha256":"60160b028adabf5fe067e96de36024ddda37cdccfe669b3da0bfe928aca38432","schema_version":"1.0","event_id":"sha256:60160b028adabf5fe067e96de36024ddda37cdccfe669b3da0bfe928aca38432"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2014:IXCJJ2VIVAXKNJFGHR2UTRKXO4","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Geoeffectiveness of Coronal Mass Ejections in the SOHO era","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"Andy Devos, Astrid Veronig, Bojan Vrsnak, Davor Sudar, Domagoj Ruzdjak, Kristoffer Leer, Luciano Rodriguez, Mateja Dumbovic, Susanne Vennerstrom","submitted_at":"2014-10-13T13:38:58Z","abstract_excerpt":"The main objective of the study is to determine the probability distributions of the geomagnetic Dst index as a function of the coronal mass ejection (CME) and solar flare parameters for the purpose of establishing a probabilistic forecast tool for the geomagnetic storm intensity. Several CME and flare parameters as well as the effect of successive-CME occurrence in changing the probability for a certain range of Dst index values, were examined. The results confirm some of already known relationships between remotely-observed properties of solar eruptive events and geomagnetic storms, namely t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1410.3303","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:41:48Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"QSWnZkvDYnPy3leJ+9mvg0MAu+oJGE9FVO8PwHdSq9JUKkiGPE5KSFE1he30qVN4tF4OR+fWsZbR7bLjf4BUDA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-06T20:07:49.907226Z"},"content_sha256":"91d9a2d7e629c1e9322bd5cdd9d34e892893bb7b08c2f5f6566d01deb1239ba9","schema_version":"1.0","event_id":"sha256:91d9a2d7e629c1e9322bd5cdd9d34e892893bb7b08c2f5f6566d01deb1239ba9"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/IXCJJ2VIVAXKNJFGHR2UTRKXO4/bundle.json","state_url":"https://pith.science/pith/IXCJJ2VIVAXKNJFGHR2UTRKXO4/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/IXCJJ2VIVAXKNJFGHR2UTRKXO4/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":"2026-06-06T20:07:49Z","links":{"resolver":"https://pith.science/pith/IXCJJ2VIVAXKNJFGHR2UTRKXO4","bundle":"https://pith.science/pith/IXCJJ2VIVAXKNJFGHR2UTRKXO4/bundle.json","state":"https://pith.science/pith/IXCJJ2VIVAXKNJFGHR2UTRKXO4/state.json","well_known_bundle":"https://pith.science/.well-known/pith/IXCJJ2VIVAXKNJFGHR2UTRKXO4/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2014:IXCJJ2VIVAXKNJFGHR2UTRKXO4","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":"7f79238e5c52689595effa3b00cb906498f37a0f5d4a60f09a379c8b752e31d1","cross_cats_sorted":["physics.space-ph"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-10-13T13:38:58Z","title_canon_sha256":"8a4721baada9b1501fc4bc1bef78ee083439390e9f5f1aded7bd454575ee474a"},"schema_version":"1.0","source":{"id":"1410.3303","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1410.3303","created_at":"2026-05-18T01:41:48Z"},{"alias_kind":"arxiv_version","alias_value":"1410.3303v1","created_at":"2026-05-18T01:41:48Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1410.3303","created_at":"2026-05-18T01:41:48Z"},{"alias_kind":"pith_short_12","alias_value":"IXCJJ2VIVAXK","created_at":"2026-05-18T12:28:33Z"},{"alias_kind":"pith_short_16","alias_value":"IXCJJ2VIVAXKNJFG","created_at":"2026-05-18T12:28:33Z"},{"alias_kind":"pith_short_8","alias_value":"IXCJJ2VI","created_at":"2026-05-18T12:28:33Z"}],"graph_snapshots":[{"event_id":"sha256:91d9a2d7e629c1e9322bd5cdd9d34e892893bb7b08c2f5f6566d01deb1239ba9","target":"graph","created_at":"2026-05-18T01:41:48Z","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":"The main objective of the study is to determine the probability distributions of the geomagnetic Dst index as a function of the coronal mass ejection (CME) and solar flare parameters for the purpose of establishing a probabilistic forecast tool for the geomagnetic storm intensity. Several CME and flare parameters as well as the effect of successive-CME occurrence in changing the probability for a certain range of Dst index values, were examined. The results confirm some of already known relationships between remotely-observed properties of solar eruptive events and geomagnetic storms, namely t","authors_text":"Andy Devos, Astrid Veronig, Bojan Vrsnak, Davor Sudar, Domagoj Ruzdjak, Kristoffer Leer, Luciano Rodriguez, Mateja Dumbovic, Susanne Vennerstrom","cross_cats":["physics.space-ph"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-10-13T13:38:58Z","title":"Geoeffectiveness of Coronal Mass Ejections in the SOHO era"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1410.3303","kind":"arxiv","version":1},"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":"sha256:60160b028adabf5fe067e96de36024ddda37cdccfe669b3da0bfe928aca38432","target":"record","created_at":"2026-05-18T01:41:48Z","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":"7f79238e5c52689595effa3b00cb906498f37a0f5d4a60f09a379c8b752e31d1","cross_cats_sorted":["physics.space-ph"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-10-13T13:38:58Z","title_canon_sha256":"8a4721baada9b1501fc4bc1bef78ee083439390e9f5f1aded7bd454575ee474a"},"schema_version":"1.0","source":{"id":"1410.3303","kind":"arxiv","version":1}},"canonical_sha256":"45c494eaa8a82ea6a4a63c7549c55777187618ba29d14e2ff4b976c3375980cf","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"45c494eaa8a82ea6a4a63c7549c55777187618ba29d14e2ff4b976c3375980cf","first_computed_at":"2026-05-18T01:41:48.871874Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:41:48.871874Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"lFRyuEWV/Z7pcg7kvuMPQyAlAHY1dXBAEMIiIR6fU4E9ykRjdemfD710DOpUenhvuqskVUNVId/etZ1ShdKWAQ==","signature_status":"signed_v1","signed_at":"2026-05-18T01:41:48.872349Z","signed_message":"canonical_sha256_bytes"},"source_id":"1410.3303","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:60160b028adabf5fe067e96de36024ddda37cdccfe669b3da0bfe928aca38432","sha256:91d9a2d7e629c1e9322bd5cdd9d34e892893bb7b08c2f5f6566d01deb1239ba9"],"state_sha256":"7ebf691b0d0ae166ff37315b1306931639b1aba219fd51a1390378ba67334499"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"lgbQEsbm13oHqJ5dit7U+/guBOtlwB0oqTYmwSxNFXnSERaUwtT9b4t13ZpseCw9IqSbkhK4bqxoJfZwdUWGAw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-06T20:07:49.911151Z","bundle_sha256":"512b0d456e1817cacd0bdc027c73cc76aa2a52b8bf58cf036b77d6204d10fd43"}}