{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:C3L2I2FUFSTDG5743VU4GE5HHU","short_pith_number":"pith:C3L2I2FU","schema_version":"1.0","canonical_sha256":"16d7a468b42ca63377fcdd69c313a73d24277f9b1bb81dc6f2fa64ca03886911","source":{"kind":"arxiv","id":"2311.04376","version":2},"attestation_state":"computed","paper":{"title":"Planetary Radio Interferometry and Doppler Experiment (PRIDE) of the JUICE mission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM","physics.space-ph"],"primary_cat":"astro-ph.EP","authors_text":"Alexander Akins, Bert L.A. Vermeersen, Claire Vallat, Dmitry A. Duev, Dominic Dirkx, Giuseppe Cimo, Guifre Molera Calves, Judit Fogasy, Konrad Willner, Krisztina Perger, Kuo-Nung Wang, Leonid I. Gurvits, Marie S. Fayolle, Nicolas Altobelli, N. Masdiana Md Said, Patrick Charlot, Pieter N.A.M. Visser, Sandor Frey, Sergey V. Pogrebenko, Stephanie M. Cazaux, Tatiana M. Bocanegra-Bahamon, Valery Lainey, Vidhya Pallichadath","submitted_at":"2023-11-07T22:40:32Z","abstract_excerpt":"Planetary Radio Interferometry and Doppler Experiment (PRIDE) is a multi-purpose experimental technique aimed at enhancing the science return of planetary missions. The technique exploits the science payload and spacecraft service systems without requiring a dedicated onboard instrumentation or imposing on the existing instrumentation any special for PRIDE requirements. PRIDE is based on the near-field phase-referencing Very Long Baseline Interferometry (VLBI) and evaluation of the Doppler shift of the radio signal transmitted by spacecraft by observing it with multiple Earth-based radio teles"},"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":"2311.04376","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2023-11-07T22:40:32Z","cross_cats_sorted":["astro-ph.IM","physics.space-ph"],"title_canon_sha256":"20e432eb715979d68ae90713a40d373beea792da249375e891f4d2bd665c484b","abstract_canon_sha256":"2cd0ec31b2931b66e6b01d4363eda497101118944cad16ecb3e067605a0e82f9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:17:33.893807Z","signature_b64":"FF3qTamKL7LvasiaSbAN5DMSkYki9gQ8Xy0D34cnCTSxm0EgABMinLM1VKQGI/7TU0Kb7eL+Vx5Y05YXAOtYBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"16d7a468b42ca63377fcdd69c313a73d24277f9b1bb81dc6f2fa64ca03886911","last_reissued_at":"2026-07-05T07:17:33.893293Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:17:33.893293Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Planetary Radio Interferometry and Doppler Experiment (PRIDE) of the JUICE mission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM","physics.space-ph"],"primary_cat":"astro-ph.EP","authors_text":"Alexander Akins, Bert L.A. Vermeersen, Claire Vallat, Dmitry A. Duev, Dominic Dirkx, Giuseppe Cimo, Guifre Molera Calves, Judit Fogasy, Konrad Willner, Krisztina Perger, Kuo-Nung Wang, Leonid I. Gurvits, Marie S. Fayolle, Nicolas Altobelli, N. Masdiana Md Said, Patrick Charlot, Pieter N.A.M. Visser, Sandor Frey, Sergey V. Pogrebenko, Stephanie M. Cazaux, Tatiana M. Bocanegra-Bahamon, Valery Lainey, Vidhya Pallichadath","submitted_at":"2023-11-07T22:40:32Z","abstract_excerpt":"Planetary Radio Interferometry and Doppler Experiment (PRIDE) is a multi-purpose experimental technique aimed at enhancing the science return of planetary missions. The technique exploits the science payload and spacecraft service systems without requiring a dedicated onboard instrumentation or imposing on the existing instrumentation any special for PRIDE requirements. PRIDE is based on the near-field phase-referencing Very Long Baseline Interferometry (VLBI) and evaluation of the Doppler shift of the radio signal transmitted by spacecraft by observing it with multiple Earth-based radio teles"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2311.04376","kind":"arxiv","version":2},"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/2311.04376/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":"2311.04376","created_at":"2026-07-05T07:17:33.893358+00:00"},{"alias_kind":"arxiv_version","alias_value":"2311.04376v2","created_at":"2026-07-05T07:17:33.893358+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2311.04376","created_at":"2026-07-05T07:17:33.893358+00:00"},{"alias_kind":"pith_short_12","alias_value":"C3L2I2FUFSTD","created_at":"2026-07-05T07:17:33.893358+00:00"},{"alias_kind":"pith_short_16","alias_value":"C3L2I2FUFSTDG574","created_at":"2026-07-05T07:17:33.893358+00:00"},{"alias_kind":"pith_short_8","alias_value":"C3L2I2FU","created_at":"2026-07-05T07:17:33.893358+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/C3L2I2FUFSTDG5743VU4GE5HHU","json":"https://pith.science/pith/C3L2I2FUFSTDG5743VU4GE5HHU.json","graph_json":"https://pith.science/api/pith-number/C3L2I2FUFSTDG5743VU4GE5HHU/graph.json","events_json":"https://pith.science/api/pith-number/C3L2I2FUFSTDG5743VU4GE5HHU/events.json","paper":"https://pith.science/paper/C3L2I2FU"},"agent_actions":{"view_html":"https://pith.science/pith/C3L2I2FUFSTDG5743VU4GE5HHU","download_json":"https://pith.science/pith/C3L2I2FUFSTDG5743VU4GE5HHU.json","view_paper":"https://pith.science/paper/C3L2I2FU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2311.04376&json=true","fetch_graph":"https://pith.science/api/pith-number/C3L2I2FUFSTDG5743VU4GE5HHU/graph.json","fetch_events":"https://pith.science/api/pith-number/C3L2I2FUFSTDG5743VU4GE5HHU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/C3L2I2FUFSTDG5743VU4GE5HHU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/C3L2I2FUFSTDG5743VU4GE5HHU/action/storage_attestation","attest_author":"https://pith.science/pith/C3L2I2FUFSTDG5743VU4GE5HHU/action/author_attestation","sign_citation":"https://pith.science/pith/C3L2I2FUFSTDG5743VU4GE5HHU/action/citation_signature","submit_replication":"https://pith.science/pith/C3L2I2FUFSTDG5743VU4GE5HHU/action/replication_record"}},"created_at":"2026-07-05T07:17:33.893358+00:00","updated_at":"2026-07-05T07:17:33.893358+00:00"}