{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:RCID34ALJ2CSIDONENYWOLJUTN","short_pith_number":"pith:RCID34AL","schema_version":"1.0","canonical_sha256":"88903df00b4e85240dcd2371672d349b492685c555a59aa2392988991cd0c106","source":{"kind":"arxiv","id":"1301.3813","version":1},"attestation_state":"computed","paper":{"title":"Cassini UVIS observations of the Io plasma torus. II. Radial variations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Ian F. Stewart, Andrew J. Steffl, Fran Bagenal","submitted_at":"2013-01-16T20:12:18Z","abstract_excerpt":"On January 14, 2001, shortly after the Cassini spacecraft's closest approach to Jupiter, the Ultraviolet Imaging Spectrometer (UVIS) made a radial scan through the midnight sector of Io plasma torus. The Io torus has not been previously observed at this local time. The UVIS data consist of 2-D spectrally dispersed images of the Io plasma torus in the wavelength range of 561{\\AA}-1912{\\AA}. We developed a spectral emissions model that incorporates the latest atomic physics data contained in the CHIANTI database in order to derive the composition of the torus plasma as a function of radial dista"},"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":"1301.3813","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2013-01-16T20:12:18Z","cross_cats_sorted":[],"title_canon_sha256":"24371cec434b3d84a146b9da26531e3dcbeba8ea116e41d63aea61d1681a26d4","abstract_canon_sha256":"133b58d33046a5f20cb7251279113e5aeac81d81b7268d6bd2aaa13ad8b951f8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:36:16.569440Z","signature_b64":"ry9nH/tpYc1Gz5QC8pCCetBYSDyjSa7LyYwFaRi2/xjAdcl4K7ZbaGI65Mqb3GS8wnjssVfm6QwCg7zYmjOLAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"88903df00b4e85240dcd2371672d349b492685c555a59aa2392988991cd0c106","last_reissued_at":"2026-05-18T03:36:16.568697Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:36:16.568697Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cassini UVIS observations of the Io plasma torus. II. Radial variations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Ian F. Stewart, Andrew J. Steffl, Fran Bagenal","submitted_at":"2013-01-16T20:12:18Z","abstract_excerpt":"On January 14, 2001, shortly after the Cassini spacecraft's closest approach to Jupiter, the Ultraviolet Imaging Spectrometer (UVIS) made a radial scan through the midnight sector of Io plasma torus. The Io torus has not been previously observed at this local time. The UVIS data consist of 2-D spectrally dispersed images of the Io plasma torus in the wavelength range of 561{\\AA}-1912{\\AA}. We developed a spectral emissions model that incorporates the latest atomic physics data contained in the CHIANTI database in order to derive the composition of the torus plasma as a function of radial dista"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1301.3813","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":"1301.3813","created_at":"2026-05-18T03:36:16.568809+00:00"},{"alias_kind":"arxiv_version","alias_value":"1301.3813v1","created_at":"2026-05-18T03:36:16.568809+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1301.3813","created_at":"2026-05-18T03:36:16.568809+00:00"},{"alias_kind":"pith_short_12","alias_value":"RCID34ALJ2CS","created_at":"2026-05-18T12:27:57.521954+00:00"},{"alias_kind":"pith_short_16","alias_value":"RCID34ALJ2CSIDON","created_at":"2026-05-18T12:27:57.521954+00:00"},{"alias_kind":"pith_short_8","alias_value":"RCID34AL","created_at":"2026-05-18T12:27:57.521954+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/RCID34ALJ2CSIDONENYWOLJUTN","json":"https://pith.science/pith/RCID34ALJ2CSIDONENYWOLJUTN.json","graph_json":"https://pith.science/api/pith-number/RCID34ALJ2CSIDONENYWOLJUTN/graph.json","events_json":"https://pith.science/api/pith-number/RCID34ALJ2CSIDONENYWOLJUTN/events.json","paper":"https://pith.science/paper/RCID34AL"},"agent_actions":{"view_html":"https://pith.science/pith/RCID34ALJ2CSIDONENYWOLJUTN","download_json":"https://pith.science/pith/RCID34ALJ2CSIDONENYWOLJUTN.json","view_paper":"https://pith.science/paper/RCID34AL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1301.3813&json=true","fetch_graph":"https://pith.science/api/pith-number/RCID34ALJ2CSIDONENYWOLJUTN/graph.json","fetch_events":"https://pith.science/api/pith-number/RCID34ALJ2CSIDONENYWOLJUTN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RCID34ALJ2CSIDONENYWOLJUTN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RCID34ALJ2CSIDONENYWOLJUTN/action/storage_attestation","attest_author":"https://pith.science/pith/RCID34ALJ2CSIDONENYWOLJUTN/action/author_attestation","sign_citation":"https://pith.science/pith/RCID34ALJ2CSIDONENYWOLJUTN/action/citation_signature","submit_replication":"https://pith.science/pith/RCID34ALJ2CSIDONENYWOLJUTN/action/replication_record"}},"created_at":"2026-05-18T03:36:16.568809+00:00","updated_at":"2026-05-18T03:36:16.568809+00:00"}