{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:7KXNUG5UHIWL6GLS2C5SXKTKBA","short_pith_number":"pith:7KXNUG5U","schema_version":"1.0","canonical_sha256":"faaeda1bb43a2cbf1972d0bb2baa6a082266a311ff575ca5a2a27251e15d9796","source":{"kind":"arxiv","id":"1603.08857","version":1},"attestation_state":"computed","paper":{"title":"Self-consistent Monte Carlo simulations of proton acceleration in coronal shocks: Effect of anisotropic pitch-angle scattering of particles","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"physics.space-ph","authors_text":"Alexandr Afanasiev, Astronomy, Finland), Markus Battarbee, Rami Vainio (Department of Physics, Turku, University of Turku","submitted_at":"2016-03-29T17:36:24Z","abstract_excerpt":"Context. Solar energetic particles observed in association with coronal mass ejections (CMEs) are produced by the CME-driven shock waves. The acceleration of particles is considered to be due to diffusive shock acceleration (DSA). Aims. We aim at a better understanding of DSA in the case of quasi-parallel shocks, in which self-generated turbulence in the shock vicinity plays a key role. Methods. We have developed and applied a new Monte Carlo simulation code for acceleration of protons in parallel coronal shocks. The code performs a self-consistent calculation of resonant interactions of parti"},"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":"1603.08857","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.space-ph","submitted_at":"2016-03-29T17:36:24Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"2b139b45b5f713637e2f7066c49412aa50c2a133133ce289b3182c1af70e4528","abstract_canon_sha256":"429832f6ab3f9a706394d61c0223633d8ccd570a7fa53e4877e6e1749a345375"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:18:05.140939Z","signature_b64":"/TIhrNC5U+n3jUmNXhqwJgEf6W55XFMssWmv+qsyPaWZuv0N9BhUlypWED9VH6PoLEigcWhWxTrilm4H1TPNCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"faaeda1bb43a2cbf1972d0bb2baa6a082266a311ff575ca5a2a27251e15d9796","last_reissued_at":"2026-05-18T01:18:05.140402Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:18:05.140402Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Self-consistent Monte Carlo simulations of proton acceleration in coronal shocks: Effect of anisotropic pitch-angle scattering of particles","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"physics.space-ph","authors_text":"Alexandr Afanasiev, Astronomy, Finland), Markus Battarbee, Rami Vainio (Department of Physics, Turku, University of Turku","submitted_at":"2016-03-29T17:36:24Z","abstract_excerpt":"Context. Solar energetic particles observed in association with coronal mass ejections (CMEs) are produced by the CME-driven shock waves. The acceleration of particles is considered to be due to diffusive shock acceleration (DSA). Aims. We aim at a better understanding of DSA in the case of quasi-parallel shocks, in which self-generated turbulence in the shock vicinity plays a key role. Methods. We have developed and applied a new Monte Carlo simulation code for acceleration of protons in parallel coronal shocks. The code performs a self-consistent calculation of resonant interactions of parti"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1603.08857","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":"1603.08857","created_at":"2026-05-18T01:18:05.140465+00:00"},{"alias_kind":"arxiv_version","alias_value":"1603.08857v1","created_at":"2026-05-18T01:18:05.140465+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1603.08857","created_at":"2026-05-18T01:18:05.140465+00:00"},{"alias_kind":"pith_short_12","alias_value":"7KXNUG5UHIWL","created_at":"2026-05-18T12:30:04.600751+00:00"},{"alias_kind":"pith_short_16","alias_value":"7KXNUG5UHIWL6GLS","created_at":"2026-05-18T12:30:04.600751+00:00"},{"alias_kind":"pith_short_8","alias_value":"7KXNUG5U","created_at":"2026-05-18T12:30:04.600751+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/7KXNUG5UHIWL6GLS2C5SXKTKBA","json":"https://pith.science/pith/7KXNUG5UHIWL6GLS2C5SXKTKBA.json","graph_json":"https://pith.science/api/pith-number/7KXNUG5UHIWL6GLS2C5SXKTKBA/graph.json","events_json":"https://pith.science/api/pith-number/7KXNUG5UHIWL6GLS2C5SXKTKBA/events.json","paper":"https://pith.science/paper/7KXNUG5U"},"agent_actions":{"view_html":"https://pith.science/pith/7KXNUG5UHIWL6GLS2C5SXKTKBA","download_json":"https://pith.science/pith/7KXNUG5UHIWL6GLS2C5SXKTKBA.json","view_paper":"https://pith.science/paper/7KXNUG5U","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1603.08857&json=true","fetch_graph":"https://pith.science/api/pith-number/7KXNUG5UHIWL6GLS2C5SXKTKBA/graph.json","fetch_events":"https://pith.science/api/pith-number/7KXNUG5UHIWL6GLS2C5SXKTKBA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7KXNUG5UHIWL6GLS2C5SXKTKBA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7KXNUG5UHIWL6GLS2C5SXKTKBA/action/storage_attestation","attest_author":"https://pith.science/pith/7KXNUG5UHIWL6GLS2C5SXKTKBA/action/author_attestation","sign_citation":"https://pith.science/pith/7KXNUG5UHIWL6GLS2C5SXKTKBA/action/citation_signature","submit_replication":"https://pith.science/pith/7KXNUG5UHIWL6GLS2C5SXKTKBA/action/replication_record"}},"created_at":"2026-05-18T01:18:05.140465+00:00","updated_at":"2026-05-18T01:18:05.140465+00:00"}