{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:2DHT7VUBZ3Z4NERF5QXS73N27G","short_pith_number":"pith:2DHT7VUB","schema_version":"1.0","canonical_sha256":"d0cf3fd681cef3c69225ec2f2fedbaf98adec6540c529f37aee9731611538641","source":{"kind":"arxiv","id":"2009.10130","version":1},"attestation_state":"computed","paper":{"title":"Forward modelling of particle acceleration and transport in an individual solar flare","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Eduard P. Kontar, Grigory E. Vekstein, Kanya Kusano, Mykola Gordovskyy, Philippa K. Browning, Satoshi Inoue","submitted_at":"2020-09-21T18:48:52Z","abstract_excerpt":"The aim of this study is to generate maps of the hard X-ray emission produced by energetic electrons in a solar flare and compare them with observations. The ultimate goal is to test the viability of the combined MHD/test-particle approach for data-driven modelling of active events in the solar corona and their impact on the heliosphere. Based on an MHD model of X-class solar flare observed on the 8th of September 2017, we calculate trajectories of a large number of electrons and protons using the relativistic guiding-centre approach. Using the obtained particle trajectories, we deduce the spa"},"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":"2009.10130","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2020-09-21T18:48:52Z","cross_cats_sorted":[],"title_canon_sha256":"fa8d283e618bbecd190d03d3deb53077400f9563236b68dd37938593e5caaa63","abstract_canon_sha256":"d96a78bc0a2f02c09d09e52622c734da5364b39c1519e0c02b11747aa7ea2f55"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:48:55.104625Z","signature_b64":"Nbz4YoY/KHtzMyq7dUd4YdxWFZKd1uHn38f39PYl1xhiW4ISziHivzyIcbFEgx+Rwz8JWmi8eLJMwobjbqUxDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d0cf3fd681cef3c69225ec2f2fedbaf98adec6540c529f37aee9731611538641","last_reissued_at":"2026-07-05T01:48:55.104232Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:48:55.104232Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Forward modelling of particle acceleration and transport in an individual solar flare","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Eduard P. Kontar, Grigory E. Vekstein, Kanya Kusano, Mykola Gordovskyy, Philippa K. Browning, Satoshi Inoue","submitted_at":"2020-09-21T18:48:52Z","abstract_excerpt":"The aim of this study is to generate maps of the hard X-ray emission produced by energetic electrons in a solar flare and compare them with observations. The ultimate goal is to test the viability of the combined MHD/test-particle approach for data-driven modelling of active events in the solar corona and their impact on the heliosphere. Based on an MHD model of X-class solar flare observed on the 8th of September 2017, we calculate trajectories of a large number of electrons and protons using the relativistic guiding-centre approach. Using the obtained particle trajectories, we deduce the spa"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2009.10130","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2009.10130/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2009.10130","created_at":"2026-07-05T01:48:55.104289+00:00"},{"alias_kind":"arxiv_version","alias_value":"2009.10130v1","created_at":"2026-07-05T01:48:55.104289+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2009.10130","created_at":"2026-07-05T01:48:55.104289+00:00"},{"alias_kind":"pith_short_12","alias_value":"2DHT7VUBZ3Z4","created_at":"2026-07-05T01:48:55.104289+00:00"},{"alias_kind":"pith_short_16","alias_value":"2DHT7VUBZ3Z4NERF","created_at":"2026-07-05T01:48:55.104289+00:00"},{"alias_kind":"pith_short_8","alias_value":"2DHT7VUB","created_at":"2026-07-05T01:48:55.104289+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/2DHT7VUBZ3Z4NERF5QXS73N27G","json":"https://pith.science/pith/2DHT7VUBZ3Z4NERF5QXS73N27G.json","graph_json":"https://pith.science/api/pith-number/2DHT7VUBZ3Z4NERF5QXS73N27G/graph.json","events_json":"https://pith.science/api/pith-number/2DHT7VUBZ3Z4NERF5QXS73N27G/events.json","paper":"https://pith.science/paper/2DHT7VUB"},"agent_actions":{"view_html":"https://pith.science/pith/2DHT7VUBZ3Z4NERF5QXS73N27G","download_json":"https://pith.science/pith/2DHT7VUBZ3Z4NERF5QXS73N27G.json","view_paper":"https://pith.science/paper/2DHT7VUB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2009.10130&json=true","fetch_graph":"https://pith.science/api/pith-number/2DHT7VUBZ3Z4NERF5QXS73N27G/graph.json","fetch_events":"https://pith.science/api/pith-number/2DHT7VUBZ3Z4NERF5QXS73N27G/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2DHT7VUBZ3Z4NERF5QXS73N27G/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2DHT7VUBZ3Z4NERF5QXS73N27G/action/storage_attestation","attest_author":"https://pith.science/pith/2DHT7VUBZ3Z4NERF5QXS73N27G/action/author_attestation","sign_citation":"https://pith.science/pith/2DHT7VUBZ3Z4NERF5QXS73N27G/action/citation_signature","submit_replication":"https://pith.science/pith/2DHT7VUBZ3Z4NERF5QXS73N27G/action/replication_record"}},"created_at":"2026-07-05T01:48:55.104289+00:00","updated_at":"2026-07-05T01:48:55.104289+00:00"}