{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:BW3BN5LHS3P4XFLKFJSAP54LDQ","short_pith_number":"pith:BW3BN5LH","schema_version":"1.0","canonical_sha256":"0db616f56796dfcb956a2a6407f78b1c1fa377b51c4ccb394086da538ec7f507","source":{"kind":"arxiv","id":"1407.7838","version":1},"attestation_state":"computed","paper":{"title":"Variations in Abundance Enhancements in Impulsive Solar Energetic-Particle Events and Related CMEs and Flares","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Donald V. Reames, Edward W. Cliver, Stephen W. Kahler","submitted_at":"2014-07-29T19:37:11Z","abstract_excerpt":"We study event-to-event variations in the abundance enhancements of the elements He through Pb for Fe-rich impulsive solar energetic-particle (SEP) events, and their relationship with properties of associated coronal mass ejections (CMEs) and solar flares. Using a least-squares procedure we fit the power-law enhancement of element abundances as a function of their mass-to-charge ratio A/Q to determine both the power and the coronal temperature (which determines Q) in each of 111 impulsive SEP events identified previously. Individual SEP events with the steepest element enhancements, e.g. ~(A/Q"},"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":"1407.7838","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-07-29T19:37:11Z","cross_cats_sorted":[],"title_canon_sha256":"fe51745a1288143467ddc93345d7ad29de7afa0b39683ec4d36bdb74588101ab","abstract_canon_sha256":"f7ad85842a9d086dd07f7fbf580a92702f44f81f75c3d7b566f775310246347c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:30:08.077575Z","signature_b64":"Ot/JQcGgcOH4iAy2g4jxsdOfNkKnB+ogaxgN7Uarhl28SxraLbxaUh8kE13/x6EubBjAYZd1bz5afKztblYqBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0db616f56796dfcb956a2a6407f78b1c1fa377b51c4ccb394086da538ec7f507","last_reissued_at":"2026-05-18T02:30:08.077050Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:30:08.077050Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Variations in Abundance Enhancements in Impulsive Solar Energetic-Particle Events and Related CMEs and Flares","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Donald V. Reames, Edward W. Cliver, Stephen W. Kahler","submitted_at":"2014-07-29T19:37:11Z","abstract_excerpt":"We study event-to-event variations in the abundance enhancements of the elements He through Pb for Fe-rich impulsive solar energetic-particle (SEP) events, and their relationship with properties of associated coronal mass ejections (CMEs) and solar flares. Using a least-squares procedure we fit the power-law enhancement of element abundances as a function of their mass-to-charge ratio A/Q to determine both the power and the coronal temperature (which determines Q) in each of 111 impulsive SEP events identified previously. Individual SEP events with the steepest element enhancements, e.g. ~(A/Q"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1407.7838","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":"1407.7838","created_at":"2026-05-18T02:30:08.077123+00:00"},{"alias_kind":"arxiv_version","alias_value":"1407.7838v1","created_at":"2026-05-18T02:30:08.077123+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1407.7838","created_at":"2026-05-18T02:30:08.077123+00:00"},{"alias_kind":"pith_short_12","alias_value":"BW3BN5LHS3P4","created_at":"2026-05-18T12:28:22.404517+00:00"},{"alias_kind":"pith_short_16","alias_value":"BW3BN5LHS3P4XFLK","created_at":"2026-05-18T12:28:22.404517+00:00"},{"alias_kind":"pith_short_8","alias_value":"BW3BN5LH","created_at":"2026-05-18T12:28:22.404517+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/BW3BN5LHS3P4XFLKFJSAP54LDQ","json":"https://pith.science/pith/BW3BN5LHS3P4XFLKFJSAP54LDQ.json","graph_json":"https://pith.science/api/pith-number/BW3BN5LHS3P4XFLKFJSAP54LDQ/graph.json","events_json":"https://pith.science/api/pith-number/BW3BN5LHS3P4XFLKFJSAP54LDQ/events.json","paper":"https://pith.science/paper/BW3BN5LH"},"agent_actions":{"view_html":"https://pith.science/pith/BW3BN5LHS3P4XFLKFJSAP54LDQ","download_json":"https://pith.science/pith/BW3BN5LHS3P4XFLKFJSAP54LDQ.json","view_paper":"https://pith.science/paper/BW3BN5LH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1407.7838&json=true","fetch_graph":"https://pith.science/api/pith-number/BW3BN5LHS3P4XFLKFJSAP54LDQ/graph.json","fetch_events":"https://pith.science/api/pith-number/BW3BN5LHS3P4XFLKFJSAP54LDQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BW3BN5LHS3P4XFLKFJSAP54LDQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BW3BN5LHS3P4XFLKFJSAP54LDQ/action/storage_attestation","attest_author":"https://pith.science/pith/BW3BN5LHS3P4XFLKFJSAP54LDQ/action/author_attestation","sign_citation":"https://pith.science/pith/BW3BN5LHS3P4XFLKFJSAP54LDQ/action/citation_signature","submit_replication":"https://pith.science/pith/BW3BN5LHS3P4XFLKFJSAP54LDQ/action/replication_record"}},"created_at":"2026-05-18T02:30:08.077123+00:00","updated_at":"2026-05-18T02:30:08.077123+00:00"}