{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:CMQSXLX4PJOECIZ7DMWCGBWINR","short_pith_number":"pith:CMQSXLX4","schema_version":"1.0","canonical_sha256":"13212baefc7a5c41233f1b2c2306c86c5b5cd65b74ab3f24ab399a049c240a86","source":{"kind":"arxiv","id":"1906.05167","version":1},"attestation_state":"computed","paper":{"title":"Effect of Star Rotation Rates on the Characteristics of Energetic Particle Events","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"Gang Li, Gary Zank, Junxiang Hu, Shuai Fu, Vladimir Airapetian, Yong Jiang","submitted_at":"2019-06-12T14:27:08Z","abstract_excerpt":"Recent detection of superflares on solar-type stars by Kepler mission raised a possibility that they can be associated with energetic coronal mass ejections (CMEs) and energetic particle events (SEPs). These space weather events can impact habitability of exoplanets around these stars. Here we use the improved Particle Acceleration and Transport in the Heliosphere (iPATH) model, to model the time intensity profile and spectrum of SEPs accelerated at CME-driven shocks from stars of different ages traced by their rotation rates. We consider a solar-like (G-type) star with 6 different rotation ra"},"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":"1906.05167","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2019-06-12T14:27:08Z","cross_cats_sorted":["physics.space-ph"],"title_canon_sha256":"eb72176ca7526b900e847dd9e897a30ac7d9d991dd941f55d0b80d126a3807ce","abstract_canon_sha256":"e33b1de34805f65c116861991ac4a44fa9518a5f85a8f9a99a28caaa404ccdd2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:42:18.512372Z","signature_b64":"7c7khfB2pYk4KobDEJCv46B97qlEnJDmpjVyeyL6Uj26H/LsJV6QiJKxv9NuGIHACuNsQ/7S5+x83tr3hfbzBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"13212baefc7a5c41233f1b2c2306c86c5b5cd65b74ab3f24ab399a049c240a86","last_reissued_at":"2026-05-17T23:42:18.511936Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:42:18.511936Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Effect of Star Rotation Rates on the Characteristics of Energetic Particle Events","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"Gang Li, Gary Zank, Junxiang Hu, Shuai Fu, Vladimir Airapetian, Yong Jiang","submitted_at":"2019-06-12T14:27:08Z","abstract_excerpt":"Recent detection of superflares on solar-type stars by Kepler mission raised a possibility that they can be associated with energetic coronal mass ejections (CMEs) and energetic particle events (SEPs). These space weather events can impact habitability of exoplanets around these stars. Here we use the improved Particle Acceleration and Transport in the Heliosphere (iPATH) model, to model the time intensity profile and spectrum of SEPs accelerated at CME-driven shocks from stars of different ages traced by their rotation rates. We consider a solar-like (G-type) star with 6 different rotation ra"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1906.05167","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":"1906.05167","created_at":"2026-05-17T23:42:18.512009+00:00"},{"alias_kind":"arxiv_version","alias_value":"1906.05167v1","created_at":"2026-05-17T23:42:18.512009+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1906.05167","created_at":"2026-05-17T23:42:18.512009+00:00"},{"alias_kind":"pith_short_12","alias_value":"CMQSXLX4PJOE","created_at":"2026-05-18T12:33:15.570797+00:00"},{"alias_kind":"pith_short_16","alias_value":"CMQSXLX4PJOECIZ7","created_at":"2026-05-18T12:33:15.570797+00:00"},{"alias_kind":"pith_short_8","alias_value":"CMQSXLX4","created_at":"2026-05-18T12:33:15.570797+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/CMQSXLX4PJOECIZ7DMWCGBWINR","json":"https://pith.science/pith/CMQSXLX4PJOECIZ7DMWCGBWINR.json","graph_json":"https://pith.science/api/pith-number/CMQSXLX4PJOECIZ7DMWCGBWINR/graph.json","events_json":"https://pith.science/api/pith-number/CMQSXLX4PJOECIZ7DMWCGBWINR/events.json","paper":"https://pith.science/paper/CMQSXLX4"},"agent_actions":{"view_html":"https://pith.science/pith/CMQSXLX4PJOECIZ7DMWCGBWINR","download_json":"https://pith.science/pith/CMQSXLX4PJOECIZ7DMWCGBWINR.json","view_paper":"https://pith.science/paper/CMQSXLX4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1906.05167&json=true","fetch_graph":"https://pith.science/api/pith-number/CMQSXLX4PJOECIZ7DMWCGBWINR/graph.json","fetch_events":"https://pith.science/api/pith-number/CMQSXLX4PJOECIZ7DMWCGBWINR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CMQSXLX4PJOECIZ7DMWCGBWINR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CMQSXLX4PJOECIZ7DMWCGBWINR/action/storage_attestation","attest_author":"https://pith.science/pith/CMQSXLX4PJOECIZ7DMWCGBWINR/action/author_attestation","sign_citation":"https://pith.science/pith/CMQSXLX4PJOECIZ7DMWCGBWINR/action/citation_signature","submit_replication":"https://pith.science/pith/CMQSXLX4PJOECIZ7DMWCGBWINR/action/replication_record"}},"created_at":"2026-05-17T23:42:18.512009+00:00","updated_at":"2026-05-17T23:42:18.512009+00:00"}