{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2016:SV3CWBAESON7DHIBS3HUHYZX32","short_pith_number":"pith:SV3CWBAE","canonical_record":{"source":{"id":"1605.08130","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-05-26T03:01:58Z","cross_cats_sorted":["physics.space-ph"],"title_canon_sha256":"67fe8fefbe5a6affd88fb92b568d5d6394775016556325a26cfe5a22b0d90e29","abstract_canon_sha256":"9979ed7d88a7e15d449dbac565125c43ecce9be53608497cb27f2cded5e0667b"},"schema_version":"1.0"},"canonical_sha256":"95762b0404939bf19d0196cf43e337dea63b3051ea9c73365abbb1345ec5ec4a","source":{"kind":"arxiv","id":"1605.08130","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1605.08130","created_at":"2026-05-18T01:09:34Z"},{"alias_kind":"arxiv_version","alias_value":"1605.08130v2","created_at":"2026-05-18T01:09:34Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1605.08130","created_at":"2026-05-18T01:09:34Z"},{"alias_kind":"pith_short_12","alias_value":"SV3CWBAESON7","created_at":"2026-05-18T12:30:44Z"},{"alias_kind":"pith_short_16","alias_value":"SV3CWBAESON7DHIB","created_at":"2026-05-18T12:30:44Z"},{"alias_kind":"pith_short_8","alias_value":"SV3CWBAE","created_at":"2026-05-18T12:30:44Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2016:SV3CWBAESON7DHIBS3HUHYZX32","target":"record","payload":{"canonical_record":{"source":{"id":"1605.08130","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-05-26T03:01:58Z","cross_cats_sorted":["physics.space-ph"],"title_canon_sha256":"67fe8fefbe5a6affd88fb92b568d5d6394775016556325a26cfe5a22b0d90e29","abstract_canon_sha256":"9979ed7d88a7e15d449dbac565125c43ecce9be53608497cb27f2cded5e0667b"},"schema_version":"1.0"},"canonical_sha256":"95762b0404939bf19d0196cf43e337dea63b3051ea9c73365abbb1345ec5ec4a","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:09:34.347685Z","signature_b64":"L6N7D5tgnxI5JqFzn9Rab8yWh2ZFW+bfDWSEz92T4vjmwcT989H7VYI2PnsbseovE8T+soe+VqG4RwVBgtfnBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"95762b0404939bf19d0196cf43e337dea63b3051ea9c73365abbb1345ec5ec4a","last_reissued_at":"2026-05-18T01:09:34.347284Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:09:34.347284Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1605.08130","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":"2026-05-18T01:09:34Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"uleDEbGVHzIaSX/mX68TpGHkD2593QDru32ZBE/JZWnEFm3hTxJqYcxdPMTyHbHS9s30YS+Si6c4H3rovaG7Cg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T22:24:26.329804Z"},"content_sha256":"61096d5e85c3eb0050f0958af967f500653cc4dd24cea14fa9237c0bbb2ede45","schema_version":"1.0","event_id":"sha256:61096d5e85c3eb0050f0958af967f500653cc4dd24cea14fa9237c0bbb2ede45"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2016:SV3CWBAESON7DHIBS3HUHYZX32","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Superposed epoch study of ICME sub-structures near Earth and their effects on galactic cosmic rays","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"J.J. Mas\\'ias-Meza, L. Rodriguez, M. Janvier, P. D\\'emoulin, S. Dasso","submitted_at":"2016-05-26T03:01:58Z","abstract_excerpt":"Interplanetary coronal mass ejections (ICMEs) are the interplanetary manifestations of solar eruptions. The overtaken solar wind forms a sheath of compressed plasma at the front of ICMEs. Magnetic clouds (MCs) are a subset of ICMEs with specific properties (e.g. the presence of a flux rope). When ICMEs pass near Earth, ground observations indicate that the flux of galactic cosmic rays (GCRs) decreases. The main aims of this paper are to find: common plasma and magnetic properties of different ICME sub-structures, and which ICME properties affect the flux of GCRs near Earth. We use a superposed"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1605.08130","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":"2026-05-18T01:09:34Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"FeK0crWjxlb0SXtBi3mp+lE+RVEC1teH3dbNK20BVjZ9E2e5VXaS6Dhxm3MkP8ySxfLp6ppE0XBqdSNVTPbMBg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T22:24:26.330500Z"},"content_sha256":"4831a2a39d8d20681fbd72fb20e03e6984803c12d2745f403720a60a2ff4bb02","schema_version":"1.0","event_id":"sha256:4831a2a39d8d20681fbd72fb20e03e6984803c12d2745f403720a60a2ff4bb02"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/SV3CWBAESON7DHIBS3HUHYZX32/bundle.json","state_url":"https://pith.science/pith/SV3CWBAESON7DHIBS3HUHYZX32/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/SV3CWBAESON7DHIBS3HUHYZX32/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":"2026-05-25T22:24:26Z","links":{"resolver":"https://pith.science/pith/SV3CWBAESON7DHIBS3HUHYZX32","bundle":"https://pith.science/pith/SV3CWBAESON7DHIBS3HUHYZX32/bundle.json","state":"https://pith.science/pith/SV3CWBAESON7DHIBS3HUHYZX32/state.json","well_known_bundle":"https://pith.science/.well-known/pith/SV3CWBAESON7DHIBS3HUHYZX32/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2016:SV3CWBAESON7DHIBS3HUHYZX32","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":"9979ed7d88a7e15d449dbac565125c43ecce9be53608497cb27f2cded5e0667b","cross_cats_sorted":["physics.space-ph"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-05-26T03:01:58Z","title_canon_sha256":"67fe8fefbe5a6affd88fb92b568d5d6394775016556325a26cfe5a22b0d90e29"},"schema_version":"1.0","source":{"id":"1605.08130","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1605.08130","created_at":"2026-05-18T01:09:34Z"},{"alias_kind":"arxiv_version","alias_value":"1605.08130v2","created_at":"2026-05-18T01:09:34Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1605.08130","created_at":"2026-05-18T01:09:34Z"},{"alias_kind":"pith_short_12","alias_value":"SV3CWBAESON7","created_at":"2026-05-18T12:30:44Z"},{"alias_kind":"pith_short_16","alias_value":"SV3CWBAESON7DHIB","created_at":"2026-05-18T12:30:44Z"},{"alias_kind":"pith_short_8","alias_value":"SV3CWBAE","created_at":"2026-05-18T12:30:44Z"}],"graph_snapshots":[{"event_id":"sha256:4831a2a39d8d20681fbd72fb20e03e6984803c12d2745f403720a60a2ff4bb02","target":"graph","created_at":"2026-05-18T01:09:34Z","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":"Interplanetary coronal mass ejections (ICMEs) are the interplanetary manifestations of solar eruptions. The overtaken solar wind forms a sheath of compressed plasma at the front of ICMEs. Magnetic clouds (MCs) are a subset of ICMEs with specific properties (e.g. the presence of a flux rope). When ICMEs pass near Earth, ground observations indicate that the flux of galactic cosmic rays (GCRs) decreases. The main aims of this paper are to find: common plasma and magnetic properties of different ICME sub-structures, and which ICME properties affect the flux of GCRs near Earth. We use a superposed","authors_text":"J.J. Mas\\'ias-Meza, L. Rodriguez, M. Janvier, P. D\\'emoulin, S. Dasso","cross_cats":["physics.space-ph"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-05-26T03:01:58Z","title":"Superposed epoch study of ICME sub-structures near Earth and their effects on galactic cosmic rays"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1605.08130","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":"sha256:61096d5e85c3eb0050f0958af967f500653cc4dd24cea14fa9237c0bbb2ede45","target":"record","created_at":"2026-05-18T01:09:34Z","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":"9979ed7d88a7e15d449dbac565125c43ecce9be53608497cb27f2cded5e0667b","cross_cats_sorted":["physics.space-ph"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-05-26T03:01:58Z","title_canon_sha256":"67fe8fefbe5a6affd88fb92b568d5d6394775016556325a26cfe5a22b0d90e29"},"schema_version":"1.0","source":{"id":"1605.08130","kind":"arxiv","version":2}},"canonical_sha256":"95762b0404939bf19d0196cf43e337dea63b3051ea9c73365abbb1345ec5ec4a","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"95762b0404939bf19d0196cf43e337dea63b3051ea9c73365abbb1345ec5ec4a","first_computed_at":"2026-05-18T01:09:34.347284Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:09:34.347284Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"L6N7D5tgnxI5JqFzn9Rab8yWh2ZFW+bfDWSEz92T4vjmwcT989H7VYI2PnsbseovE8T+soe+VqG4RwVBgtfnBg==","signature_status":"signed_v1","signed_at":"2026-05-18T01:09:34.347685Z","signed_message":"canonical_sha256_bytes"},"source_id":"1605.08130","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:61096d5e85c3eb0050f0958af967f500653cc4dd24cea14fa9237c0bbb2ede45","sha256:4831a2a39d8d20681fbd72fb20e03e6984803c12d2745f403720a60a2ff4bb02"],"state_sha256":"c861c86e0135498d3111d2a94b574f322dee7e25c447c7bef28916c6a1ec45d3"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"3uNIiiqlrLDC2+x67IvXMM5k7ZiDyYoRXCi1weLrOtUgAaxOSV+RjwHfZXuu4/ZN2Maxk/40/CEf8DDhQVsMAA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-25T22:24:26.333637Z","bundle_sha256":"e9651cfbd1ed32fbc1d05104fa493e7e0e2bce0f9bc9212db0a1cd5eaf4ec64c"}}