{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:XMZ4YWLAXSYK7J2AUDMTHCPUL2","short_pith_number":"pith:XMZ4YWLA","schema_version":"1.0","canonical_sha256":"bb33cc5960bcb0afa740a0d93389f45eb9355cbac7f1b1163506607cb6889e2a","source":{"kind":"arxiv","id":"1507.07655","version":4},"attestation_state":"computed","paper":{"title":"Numerical simulations of solar energetic particle event timescales associated with ICMES","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"G. Qin, S.-Y. Qi, Y. Wang","submitted_at":"2015-07-28T05:59:19Z","abstract_excerpt":"Recently, S.W. Kahler studied the solar energetic particle (SEP) event timescales associated with coronal mass ejections (CMEs) from spacecraft data analysis. They obtained different timescales of SEP events, such as TO, the onset time from CME launch to SEP onset, TR, the rise time from onset to half the peak intensity (0.5Ip), and TD, the duration of the SEP intensity above 0.5Ip. In this work, we solve SEPs transport equation considering ICME shocks as energetic particle sources. With our modeling assumptions, our simulations show similar results to Kahler's spacecraft data analysis that th"},"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":"1507.07655","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2015-07-28T05:59:19Z","cross_cats_sorted":[],"title_canon_sha256":"d8338befef0e60b3a08e85f199cb85e448756c30f6f28084047d3431268f3046","abstract_canon_sha256":"7356dcd9dd32ae05ce2ef26e8456387ea5047a77ff0d9ff8bc2ad7912efede4f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:00:40.478927Z","signature_b64":"HlOElErPmgOVI9BgkH1CisnwJUiaCfbl8zi1Ej/ppDGCTBaT/RpAyDVMV95IU1F5orTtdd+KadtSZSgDvKTyCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bb33cc5960bcb0afa740a0d93389f45eb9355cbac7f1b1163506607cb6889e2a","last_reissued_at":"2026-05-18T01:00:40.478478Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:00:40.478478Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Numerical simulations of solar energetic particle event timescales associated with ICMES","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"G. Qin, S.-Y. Qi, Y. Wang","submitted_at":"2015-07-28T05:59:19Z","abstract_excerpt":"Recently, S.W. Kahler studied the solar energetic particle (SEP) event timescales associated with coronal mass ejections (CMEs) from spacecraft data analysis. They obtained different timescales of SEP events, such as TO, the onset time from CME launch to SEP onset, TR, the rise time from onset to half the peak intensity (0.5Ip), and TD, the duration of the SEP intensity above 0.5Ip. In this work, we solve SEPs transport equation considering ICME shocks as energetic particle sources. With our modeling assumptions, our simulations show similar results to Kahler's spacecraft data analysis that th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1507.07655","kind":"arxiv","version":4},"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":"1507.07655","created_at":"2026-05-18T01:00:40.478551+00:00"},{"alias_kind":"arxiv_version","alias_value":"1507.07655v4","created_at":"2026-05-18T01:00:40.478551+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1507.07655","created_at":"2026-05-18T01:00:40.478551+00:00"},{"alias_kind":"pith_short_12","alias_value":"XMZ4YWLAXSYK","created_at":"2026-05-18T12:29:50.041715+00:00"},{"alias_kind":"pith_short_16","alias_value":"XMZ4YWLAXSYK7J2A","created_at":"2026-05-18T12:29:50.041715+00:00"},{"alias_kind":"pith_short_8","alias_value":"XMZ4YWLA","created_at":"2026-05-18T12:29:50.041715+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/XMZ4YWLAXSYK7J2AUDMTHCPUL2","json":"https://pith.science/pith/XMZ4YWLAXSYK7J2AUDMTHCPUL2.json","graph_json":"https://pith.science/api/pith-number/XMZ4YWLAXSYK7J2AUDMTHCPUL2/graph.json","events_json":"https://pith.science/api/pith-number/XMZ4YWLAXSYK7J2AUDMTHCPUL2/events.json","paper":"https://pith.science/paper/XMZ4YWLA"},"agent_actions":{"view_html":"https://pith.science/pith/XMZ4YWLAXSYK7J2AUDMTHCPUL2","download_json":"https://pith.science/pith/XMZ4YWLAXSYK7J2AUDMTHCPUL2.json","view_paper":"https://pith.science/paper/XMZ4YWLA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1507.07655&json=true","fetch_graph":"https://pith.science/api/pith-number/XMZ4YWLAXSYK7J2AUDMTHCPUL2/graph.json","fetch_events":"https://pith.science/api/pith-number/XMZ4YWLAXSYK7J2AUDMTHCPUL2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XMZ4YWLAXSYK7J2AUDMTHCPUL2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XMZ4YWLAXSYK7J2AUDMTHCPUL2/action/storage_attestation","attest_author":"https://pith.science/pith/XMZ4YWLAXSYK7J2AUDMTHCPUL2/action/author_attestation","sign_citation":"https://pith.science/pith/XMZ4YWLAXSYK7J2AUDMTHCPUL2/action/citation_signature","submit_replication":"https://pith.science/pith/XMZ4YWLAXSYK7J2AUDMTHCPUL2/action/replication_record"}},"created_at":"2026-05-18T01:00:40.478551+00:00","updated_at":"2026-05-18T01:00:40.478551+00:00"}