{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:3LM4SHYEFO73X4GIS6SUV5TXW2","short_pith_number":"pith:3LM4SHYE","schema_version":"1.0","canonical_sha256":"dad9c91f042bbfbbf0c897a54af677b6b5d2099eda5fb0308d0bb64ec3bb867b","source":{"kind":"arxiv","id":"1202.6010","version":1},"attestation_state":"computed","paper":{"title":"Cross-Field Transport of Solar Energetic Particles in a Large-Scale Fluctuating Magnetic Field","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"James Kelly, Silvia Dalla, Timo Laitinen","submitted_at":"2012-02-27T17:41:11Z","abstract_excerpt":"The trajectories of Solar Energetic Particles (SEPs) in an Interplanetary Magnetic Field (IMF) exhibiting large-scale fluctuations due to footpoint motions originating in the photosphere, are simulated using a full-orbit test-particle code. The cross-field transport experienced by the particles in three propagation conditions (scatter-free, with scattering mean free path lambda=0.3 AU and lambda=2 AU) is characterized in the Parker spiral geometry. The role of expansion of the magnetic field with radial distance from the Sun is taken into consideration in the calculation of particle displaceme"},"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":"1202.6010","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2012-02-27T17:41:11Z","cross_cats_sorted":[],"title_canon_sha256":"73d7bfa3ae360db1a50d9b6fb39fa4c36509536aa83f64bdb6789df67f4da4a8","abstract_canon_sha256":"2af8fd13fff92f4783144681611cf9277139e167a7462bb7f9716d5140b2d12f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:58:19.132359Z","signature_b64":"/aw0uqUFsOWXh5VkgUBVczS/9pTePfaxI8GAwaBWX6AgWujNBpSxGurICgM5jxe1gpJkrhwKYQ3IvRUqQjyCAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"dad9c91f042bbfbbf0c897a54af677b6b5d2099eda5fb0308d0bb64ec3bb867b","last_reissued_at":"2026-05-18T01:58:19.131818Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:58:19.131818Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cross-Field Transport of Solar Energetic Particles in a Large-Scale Fluctuating Magnetic Field","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"James Kelly, Silvia Dalla, Timo Laitinen","submitted_at":"2012-02-27T17:41:11Z","abstract_excerpt":"The trajectories of Solar Energetic Particles (SEPs) in an Interplanetary Magnetic Field (IMF) exhibiting large-scale fluctuations due to footpoint motions originating in the photosphere, are simulated using a full-orbit test-particle code. The cross-field transport experienced by the particles in three propagation conditions (scatter-free, with scattering mean free path lambda=0.3 AU and lambda=2 AU) is characterized in the Parker spiral geometry. The role of expansion of the magnetic field with radial distance from the Sun is taken into consideration in the calculation of particle displaceme"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1202.6010","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1202.6010","created_at":"2026-05-18T01:58:19.131888+00:00"},{"alias_kind":"arxiv_version","alias_value":"1202.6010v1","created_at":"2026-05-18T01:58:19.131888+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1202.6010","created_at":"2026-05-18T01:58:19.131888+00:00"},{"alias_kind":"pith_short_12","alias_value":"3LM4SHYEFO73","created_at":"2026-05-18T12:26:50.516681+00:00"},{"alias_kind":"pith_short_16","alias_value":"3LM4SHYEFO73X4GI","created_at":"2026-05-18T12:26:50.516681+00:00"},{"alias_kind":"pith_short_8","alias_value":"3LM4SHYE","created_at":"2026-05-18T12:26:50.516681+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/3LM4SHYEFO73X4GIS6SUV5TXW2","json":"https://pith.science/pith/3LM4SHYEFO73X4GIS6SUV5TXW2.json","graph_json":"https://pith.science/api/pith-number/3LM4SHYEFO73X4GIS6SUV5TXW2/graph.json","events_json":"https://pith.science/api/pith-number/3LM4SHYEFO73X4GIS6SUV5TXW2/events.json","paper":"https://pith.science/paper/3LM4SHYE"},"agent_actions":{"view_html":"https://pith.science/pith/3LM4SHYEFO73X4GIS6SUV5TXW2","download_json":"https://pith.science/pith/3LM4SHYEFO73X4GIS6SUV5TXW2.json","view_paper":"https://pith.science/paper/3LM4SHYE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1202.6010&json=true","fetch_graph":"https://pith.science/api/pith-number/3LM4SHYEFO73X4GIS6SUV5TXW2/graph.json","fetch_events":"https://pith.science/api/pith-number/3LM4SHYEFO73X4GIS6SUV5TXW2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3LM4SHYEFO73X4GIS6SUV5TXW2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3LM4SHYEFO73X4GIS6SUV5TXW2/action/storage_attestation","attest_author":"https://pith.science/pith/3LM4SHYEFO73X4GIS6SUV5TXW2/action/author_attestation","sign_citation":"https://pith.science/pith/3LM4SHYEFO73X4GIS6SUV5TXW2/action/citation_signature","submit_replication":"https://pith.science/pith/3LM4SHYEFO73X4GIS6SUV5TXW2/action/replication_record"}},"created_at":"2026-05-18T01:58:19.131888+00:00","updated_at":"2026-05-18T01:58:19.131888+00:00"}