{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:CZILNRXCOJ5IHNIPKKFYYQDLPR","short_pith_number":"pith:CZILNRXC","schema_version":"1.0","canonical_sha256":"1650b6c6e2727a83b50f528b8c406b7c52ecbad0772bab6cf2e573d15f9873ba","source":{"kind":"arxiv","id":"1803.02635","version":1},"attestation_state":"computed","paper":{"title":"Energetic gamma-ray emission from solar flares","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Andrew M. Taylor, Carlo Romoli, Ervin Kafexhiu, Felix Aharonian","submitted_at":"2018-03-07T13:20:16Z","abstract_excerpt":"Recent advances in the $\\gamma$-ray observations of solar flares by the \\textit{Fermi} satellite, demand revisions in the hadronic $\\gamma$-ray flux computation below 1 GeV. In this work we utilize recently updated pion production cross sections, along with an accurate description of low energy nuclear interactions. Applying these new interaction descriptions to model the \\textit{Fermi} Large Area Telescope (LAT) solar flare data, we infer the primary particle spectral parameters. Application of this new cross section description leads to significantly different spectral parameters compared to"},"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":"1803.02635","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2018-03-07T13:20:16Z","cross_cats_sorted":[],"title_canon_sha256":"42569db9be1403050d4a5aaa380624abeb0b1274463a0741f271117908830361","abstract_canon_sha256":"69264f4c0ee75a1e728cf73eadc74be7ec43aaf1b4e8dc7593fdcd66a232c791"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:05:31.904495Z","signature_b64":"W59LuuoG1eNkYPN7ylDLozseseXla5jVtDGTYzqR1UjBjH7jtClYPhv8jRMGJ5euG4qtmtCloXZH7J4duOopBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1650b6c6e2727a83b50f528b8c406b7c52ecbad0772bab6cf2e573d15f9873ba","last_reissued_at":"2026-05-18T00:05:31.903924Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:05:31.903924Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Energetic gamma-ray emission from solar flares","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Andrew M. Taylor, Carlo Romoli, Ervin Kafexhiu, Felix Aharonian","submitted_at":"2018-03-07T13:20:16Z","abstract_excerpt":"Recent advances in the $\\gamma$-ray observations of solar flares by the \\textit{Fermi} satellite, demand revisions in the hadronic $\\gamma$-ray flux computation below 1 GeV. In this work we utilize recently updated pion production cross sections, along with an accurate description of low energy nuclear interactions. Applying these new interaction descriptions to model the \\textit{Fermi} Large Area Telescope (LAT) solar flare data, we infer the primary particle spectral parameters. Application of this new cross section description leads to significantly different spectral parameters compared to"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1803.02635","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":"1803.02635","created_at":"2026-05-18T00:05:31.904023+00:00"},{"alias_kind":"arxiv_version","alias_value":"1803.02635v1","created_at":"2026-05-18T00:05:31.904023+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1803.02635","created_at":"2026-05-18T00:05:31.904023+00:00"},{"alias_kind":"pith_short_12","alias_value":"CZILNRXCOJ5I","created_at":"2026-05-18T12:32:19.392346+00:00"},{"alias_kind":"pith_short_16","alias_value":"CZILNRXCOJ5IHNIP","created_at":"2026-05-18T12:32:19.392346+00:00"},{"alias_kind":"pith_short_8","alias_value":"CZILNRXC","created_at":"2026-05-18T12:32:19.392346+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/CZILNRXCOJ5IHNIPKKFYYQDLPR","json":"https://pith.science/pith/CZILNRXCOJ5IHNIPKKFYYQDLPR.json","graph_json":"https://pith.science/api/pith-number/CZILNRXCOJ5IHNIPKKFYYQDLPR/graph.json","events_json":"https://pith.science/api/pith-number/CZILNRXCOJ5IHNIPKKFYYQDLPR/events.json","paper":"https://pith.science/paper/CZILNRXC"},"agent_actions":{"view_html":"https://pith.science/pith/CZILNRXCOJ5IHNIPKKFYYQDLPR","download_json":"https://pith.science/pith/CZILNRXCOJ5IHNIPKKFYYQDLPR.json","view_paper":"https://pith.science/paper/CZILNRXC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1803.02635&json=true","fetch_graph":"https://pith.science/api/pith-number/CZILNRXCOJ5IHNIPKKFYYQDLPR/graph.json","fetch_events":"https://pith.science/api/pith-number/CZILNRXCOJ5IHNIPKKFYYQDLPR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CZILNRXCOJ5IHNIPKKFYYQDLPR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CZILNRXCOJ5IHNIPKKFYYQDLPR/action/storage_attestation","attest_author":"https://pith.science/pith/CZILNRXCOJ5IHNIPKKFYYQDLPR/action/author_attestation","sign_citation":"https://pith.science/pith/CZILNRXCOJ5IHNIPKKFYYQDLPR/action/citation_signature","submit_replication":"https://pith.science/pith/CZILNRXCOJ5IHNIPKKFYYQDLPR/action/replication_record"}},"created_at":"2026-05-18T00:05:31.904023+00:00","updated_at":"2026-05-18T00:05:31.904023+00:00"}