{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:SV3CWBAESON7DHIBS3HUHYZX32","short_pith_number":"pith:SV3CWBAE","schema_version":"1.0","canonical_sha256":"95762b0404939bf19d0196cf43e337dea63b3051ea9c73365abbb1345ec5ec4a","source":{"kind":"arxiv","id":"1605.08130","version":2},"attestation_state":"computed","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"},"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":"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"},"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"},"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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1605.08130","created_at":"2026-05-18T01:09:34.347358+00:00"},{"alias_kind":"arxiv_version","alias_value":"1605.08130v2","created_at":"2026-05-18T01:09:34.347358+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1605.08130","created_at":"2026-05-18T01:09:34.347358+00:00"},{"alias_kind":"pith_short_12","alias_value":"SV3CWBAESON7","created_at":"2026-05-18T12:30:44.179134+00:00"},{"alias_kind":"pith_short_16","alias_value":"SV3CWBAESON7DHIB","created_at":"2026-05-18T12:30:44.179134+00:00"},{"alias_kind":"pith_short_8","alias_value":"SV3CWBAE","created_at":"2026-05-18T12:30:44.179134+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/SV3CWBAESON7DHIBS3HUHYZX32","json":"https://pith.science/pith/SV3CWBAESON7DHIBS3HUHYZX32.json","graph_json":"https://pith.science/api/pith-number/SV3CWBAESON7DHIBS3HUHYZX32/graph.json","events_json":"https://pith.science/api/pith-number/SV3CWBAESON7DHIBS3HUHYZX32/events.json","paper":"https://pith.science/paper/SV3CWBAE"},"agent_actions":{"view_html":"https://pith.science/pith/SV3CWBAESON7DHIBS3HUHYZX32","download_json":"https://pith.science/pith/SV3CWBAESON7DHIBS3HUHYZX32.json","view_paper":"https://pith.science/paper/SV3CWBAE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1605.08130&json=true","fetch_graph":"https://pith.science/api/pith-number/SV3CWBAESON7DHIBS3HUHYZX32/graph.json","fetch_events":"https://pith.science/api/pith-number/SV3CWBAESON7DHIBS3HUHYZX32/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SV3CWBAESON7DHIBS3HUHYZX32/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SV3CWBAESON7DHIBS3HUHYZX32/action/storage_attestation","attest_author":"https://pith.science/pith/SV3CWBAESON7DHIBS3HUHYZX32/action/author_attestation","sign_citation":"https://pith.science/pith/SV3CWBAESON7DHIBS3HUHYZX32/action/citation_signature","submit_replication":"https://pith.science/pith/SV3CWBAESON7DHIBS3HUHYZX32/action/replication_record"}},"created_at":"2026-05-18T01:09:34.347358+00:00","updated_at":"2026-05-18T01:09:34.347358+00:00"}