{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:UTULDVXIFAZIRBMPKO5QIRDFJ3","short_pith_number":"pith:UTULDVXI","schema_version":"1.0","canonical_sha256":"a4e8b1d6e8283288858f53bb0444654ed0f736cc4921700a6a20bbe82384f1d5","source":{"kind":"arxiv","id":"1705.08728","version":1},"attestation_state":"computed","paper":{"title":"Synthetic IRIS spectra of the solar transition region: Effect of high-energy tails","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"C. Vocks, E. Dzifcakova, J. Dudik","submitted_at":"2017-05-24T12:37:47Z","abstract_excerpt":"The solar transition region satisfies the conditions for presence of non-Maxwellian electron energy distributions with high-energy tails at energies corresponding to the ionization potentials of many ions emitting in the EUV and UV portions of the spectrum. We calculate the synthetic Si IV, O IV, and S IV spectra in the far ultra-violet (FUV) channel of the Interface Region Imaging Spectrograph (IRIS). Ionization, recombination, and excitation rates are obtained by integration of the cross-sections or their approximations over the model electron distributions considering particle propagation f"},"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":"1705.08728","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-05-24T12:37:47Z","cross_cats_sorted":[],"title_canon_sha256":"5a6080ab73a0383a1d72084e366a0ea3b9fafdca97537629cf0037886ec72f1b","abstract_canon_sha256":"9de52c5c44d6ceed90dd089150cae56180b41dd0f48d8a969d3337ead835a4f8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:40:03.417774Z","signature_b64":"BkdN5rOtlQU42EK81ON/cUTHGAmJ2HtUmcuJ0zjFUKwYCXUfDhJfgoskmSodkNwtYLQ9+DI3Egm8q8q+r30TBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a4e8b1d6e8283288858f53bb0444654ed0f736cc4921700a6a20bbe82384f1d5","last_reissued_at":"2026-05-18T00:40:03.417075Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:40:03.417075Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Synthetic IRIS spectra of the solar transition region: Effect of high-energy tails","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"C. Vocks, E. Dzifcakova, J. Dudik","submitted_at":"2017-05-24T12:37:47Z","abstract_excerpt":"The solar transition region satisfies the conditions for presence of non-Maxwellian electron energy distributions with high-energy tails at energies corresponding to the ionization potentials of many ions emitting in the EUV and UV portions of the spectrum. We calculate the synthetic Si IV, O IV, and S IV spectra in the far ultra-violet (FUV) channel of the Interface Region Imaging Spectrograph (IRIS). Ionization, recombination, and excitation rates are obtained by integration of the cross-sections or their approximations over the model electron distributions considering particle propagation f"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.08728","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":"1705.08728","created_at":"2026-05-18T00:40:03.417144+00:00"},{"alias_kind":"arxiv_version","alias_value":"1705.08728v1","created_at":"2026-05-18T00:40:03.417144+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1705.08728","created_at":"2026-05-18T00:40:03.417144+00:00"},{"alias_kind":"pith_short_12","alias_value":"UTULDVXIFAZI","created_at":"2026-05-18T12:31:49.984773+00:00"},{"alias_kind":"pith_short_16","alias_value":"UTULDVXIFAZIRBMP","created_at":"2026-05-18T12:31:49.984773+00:00"},{"alias_kind":"pith_short_8","alias_value":"UTULDVXI","created_at":"2026-05-18T12:31:49.984773+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/UTULDVXIFAZIRBMPKO5QIRDFJ3","json":"https://pith.science/pith/UTULDVXIFAZIRBMPKO5QIRDFJ3.json","graph_json":"https://pith.science/api/pith-number/UTULDVXIFAZIRBMPKO5QIRDFJ3/graph.json","events_json":"https://pith.science/api/pith-number/UTULDVXIFAZIRBMPKO5QIRDFJ3/events.json","paper":"https://pith.science/paper/UTULDVXI"},"agent_actions":{"view_html":"https://pith.science/pith/UTULDVXIFAZIRBMPKO5QIRDFJ3","download_json":"https://pith.science/pith/UTULDVXIFAZIRBMPKO5QIRDFJ3.json","view_paper":"https://pith.science/paper/UTULDVXI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1705.08728&json=true","fetch_graph":"https://pith.science/api/pith-number/UTULDVXIFAZIRBMPKO5QIRDFJ3/graph.json","fetch_events":"https://pith.science/api/pith-number/UTULDVXIFAZIRBMPKO5QIRDFJ3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UTULDVXIFAZIRBMPKO5QIRDFJ3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UTULDVXIFAZIRBMPKO5QIRDFJ3/action/storage_attestation","attest_author":"https://pith.science/pith/UTULDVXIFAZIRBMPKO5QIRDFJ3/action/author_attestation","sign_citation":"https://pith.science/pith/UTULDVXIFAZIRBMPKO5QIRDFJ3/action/citation_signature","submit_replication":"https://pith.science/pith/UTULDVXIFAZIRBMPKO5QIRDFJ3/action/replication_record"}},"created_at":"2026-05-18T00:40:03.417144+00:00","updated_at":"2026-05-18T00:40:03.417144+00:00"}