{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:TQXXLC4UCFS5PTYRSIMQWJ4HAZ","short_pith_number":"pith:TQXXLC4U","schema_version":"1.0","canonical_sha256":"9c2f758b941165d7cf1192190b2787067eeca6eb111adff731ee9ede9e8b9e85","source":{"kind":"arxiv","id":"1402.1966","version":1},"attestation_state":"computed","paper":{"title":"Dispersion-like phenomena in Jovian decametric S-bursts: Tabooed Facts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"astro-ph.EP","authors_text":"Helmut O. Rucker, Oleksiy V. Arkhypov","submitted_at":"2014-02-09T17:16:43Z","abstract_excerpt":"The dominant viewpoint on Jovian decametric S-burst emission neglects the time delay of the radiation, although its base theory of electron cyclotron maser instability allows a significant decreasing of X-mode group velocity near the cutoff frequency at the bottom of source region. We searched for effects of the frequency-related delay of radiation in broadband Jovian radio storms consisting of periodic S-bursts (S-burst trains) at 16 to 30 MHz. It was found that up to 1% of bursts in a train are of distorted meandering shape in dynamic spectrum, where the emission from one radio source was ob"},"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":"1402.1966","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2014-02-09T17:16:43Z","cross_cats_sorted":["physics.space-ph"],"title_canon_sha256":"933ab26c375494a53fc91e0128b8ff3fc16e00052a221291d422d36c1363b1dd","abstract_canon_sha256":"891e6e6b23b67435f0f72838b2a2016f0b7ee7dab60ef0d0c611145d46032959"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:59:32.858017Z","signature_b64":"bcCSawJao+BSGu9NAmFR5QXK8shFOhJdcclzNT0kKRa4mK5JlECTce3s7anzGTHbpRyFeNymp6F2bq8wNFlrCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9c2f758b941165d7cf1192190b2787067eeca6eb111adff731ee9ede9e8b9e85","last_reissued_at":"2026-05-18T02:59:32.857142Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:59:32.857142Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dispersion-like phenomena in Jovian decametric S-bursts: Tabooed Facts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"astro-ph.EP","authors_text":"Helmut O. Rucker, Oleksiy V. Arkhypov","submitted_at":"2014-02-09T17:16:43Z","abstract_excerpt":"The dominant viewpoint on Jovian decametric S-burst emission neglects the time delay of the radiation, although its base theory of electron cyclotron maser instability allows a significant decreasing of X-mode group velocity near the cutoff frequency at the bottom of source region. We searched for effects of the frequency-related delay of radiation in broadband Jovian radio storms consisting of periodic S-bursts (S-burst trains) at 16 to 30 MHz. It was found that up to 1% of bursts in a train are of distorted meandering shape in dynamic spectrum, where the emission from one radio source was ob"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1402.1966","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":"1402.1966","created_at":"2026-05-18T02:59:32.857288+00:00"},{"alias_kind":"arxiv_version","alias_value":"1402.1966v1","created_at":"2026-05-18T02:59:32.857288+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1402.1966","created_at":"2026-05-18T02:59:32.857288+00:00"},{"alias_kind":"pith_short_12","alias_value":"TQXXLC4UCFS5","created_at":"2026-05-18T12:28:49.207871+00:00"},{"alias_kind":"pith_short_16","alias_value":"TQXXLC4UCFS5PTYR","created_at":"2026-05-18T12:28:49.207871+00:00"},{"alias_kind":"pith_short_8","alias_value":"TQXXLC4U","created_at":"2026-05-18T12:28:49.207871+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/TQXXLC4UCFS5PTYRSIMQWJ4HAZ","json":"https://pith.science/pith/TQXXLC4UCFS5PTYRSIMQWJ4HAZ.json","graph_json":"https://pith.science/api/pith-number/TQXXLC4UCFS5PTYRSIMQWJ4HAZ/graph.json","events_json":"https://pith.science/api/pith-number/TQXXLC4UCFS5PTYRSIMQWJ4HAZ/events.json","paper":"https://pith.science/paper/TQXXLC4U"},"agent_actions":{"view_html":"https://pith.science/pith/TQXXLC4UCFS5PTYRSIMQWJ4HAZ","download_json":"https://pith.science/pith/TQXXLC4UCFS5PTYRSIMQWJ4HAZ.json","view_paper":"https://pith.science/paper/TQXXLC4U","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1402.1966&json=true","fetch_graph":"https://pith.science/api/pith-number/TQXXLC4UCFS5PTYRSIMQWJ4HAZ/graph.json","fetch_events":"https://pith.science/api/pith-number/TQXXLC4UCFS5PTYRSIMQWJ4HAZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TQXXLC4UCFS5PTYRSIMQWJ4HAZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TQXXLC4UCFS5PTYRSIMQWJ4HAZ/action/storage_attestation","attest_author":"https://pith.science/pith/TQXXLC4UCFS5PTYRSIMQWJ4HAZ/action/author_attestation","sign_citation":"https://pith.science/pith/TQXXLC4UCFS5PTYRSIMQWJ4HAZ/action/citation_signature","submit_replication":"https://pith.science/pith/TQXXLC4UCFS5PTYRSIMQWJ4HAZ/action/replication_record"}},"created_at":"2026-05-18T02:59:32.857288+00:00","updated_at":"2026-05-18T02:59:32.857288+00:00"}