{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:TXGJWZATO2ZDOEES4HWFA6XW6G","short_pith_number":"pith:TXGJWZAT","schema_version":"1.0","canonical_sha256":"9dcc9b641376b2371092e1ec507af6f1b0e014f96997f42cde7dbf1ee6fc2c8d","source":{"kind":"arxiv","id":"1703.10273","version":1},"attestation_state":"computed","paper":{"title":"Zonal Flow Magnetic Field Interaction in the Semi-Conducting Region of Giant Planets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"David J. Stevenson, Hao Cao","submitted_at":"2017-03-29T23:53:06Z","abstract_excerpt":"All four giant planets in the Solar System feature zonal flows on the order of 100 m/s in the cloud deck, and large-scale intrinsic magnetic fields on the order of 1 Gauss near the surface. The vertical structure of the zonal flows remains obscure. The end-member scenarios are shallow flows confined in the radiative atmosphere and deep flows throughout the entire planet. The electrical conductivity increases rapidly yet smoothly as a function of depth inside Jupiter and Saturn. Deep zonal flows will inevitably interact with the magnetic field, at depth with even modest electrical conductivity."},"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":"1703.10273","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2017-03-29T23:53:06Z","cross_cats_sorted":[],"title_canon_sha256":"3844d2dd1428d0800738de1ee6041f9136c8a3f17f7096a08d170f5dabe7cd16","abstract_canon_sha256":"8e1354b31ce79ffa26d6cbd97a66e3ec5ec6eca53973d624d71e18c078f67e4f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:42:04.777935Z","signature_b64":"+MeNHAIkzongTUhi41v5QwgVrwU4yWR0PTGmajrmWRD3tadfoSwoG4r39Xq4Qb9RsdO+FNBYCQg9N+/fNoUVCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9dcc9b641376b2371092e1ec507af6f1b0e014f96997f42cde7dbf1ee6fc2c8d","last_reissued_at":"2026-05-18T00:42:04.777303Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:42:04.777303Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Zonal Flow Magnetic Field Interaction in the Semi-Conducting Region of Giant Planets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"David J. Stevenson, Hao Cao","submitted_at":"2017-03-29T23:53:06Z","abstract_excerpt":"All four giant planets in the Solar System feature zonal flows on the order of 100 m/s in the cloud deck, and large-scale intrinsic magnetic fields on the order of 1 Gauss near the surface. The vertical structure of the zonal flows remains obscure. The end-member scenarios are shallow flows confined in the radiative atmosphere and deep flows throughout the entire planet. The electrical conductivity increases rapidly yet smoothly as a function of depth inside Jupiter and Saturn. Deep zonal flows will inevitably interact with the magnetic field, at depth with even modest electrical conductivity."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1703.10273","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":"1703.10273","created_at":"2026-05-18T00:42:04.777407+00:00"},{"alias_kind":"arxiv_version","alias_value":"1703.10273v1","created_at":"2026-05-18T00:42:04.777407+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1703.10273","created_at":"2026-05-18T00:42:04.777407+00:00"},{"alias_kind":"pith_short_12","alias_value":"TXGJWZATO2ZD","created_at":"2026-05-18T12:31:46.661854+00:00"},{"alias_kind":"pith_short_16","alias_value":"TXGJWZATO2ZDOEES","created_at":"2026-05-18T12:31:46.661854+00:00"},{"alias_kind":"pith_short_8","alias_value":"TXGJWZAT","created_at":"2026-05-18T12:31:46.661854+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/TXGJWZATO2ZDOEES4HWFA6XW6G","json":"https://pith.science/pith/TXGJWZATO2ZDOEES4HWFA6XW6G.json","graph_json":"https://pith.science/api/pith-number/TXGJWZATO2ZDOEES4HWFA6XW6G/graph.json","events_json":"https://pith.science/api/pith-number/TXGJWZATO2ZDOEES4HWFA6XW6G/events.json","paper":"https://pith.science/paper/TXGJWZAT"},"agent_actions":{"view_html":"https://pith.science/pith/TXGJWZATO2ZDOEES4HWFA6XW6G","download_json":"https://pith.science/pith/TXGJWZATO2ZDOEES4HWFA6XW6G.json","view_paper":"https://pith.science/paper/TXGJWZAT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1703.10273&json=true","fetch_graph":"https://pith.science/api/pith-number/TXGJWZATO2ZDOEES4HWFA6XW6G/graph.json","fetch_events":"https://pith.science/api/pith-number/TXGJWZATO2ZDOEES4HWFA6XW6G/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TXGJWZATO2ZDOEES4HWFA6XW6G/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TXGJWZATO2ZDOEES4HWFA6XW6G/action/storage_attestation","attest_author":"https://pith.science/pith/TXGJWZATO2ZDOEES4HWFA6XW6G/action/author_attestation","sign_citation":"https://pith.science/pith/TXGJWZATO2ZDOEES4HWFA6XW6G/action/citation_signature","submit_replication":"https://pith.science/pith/TXGJWZATO2ZDOEES4HWFA6XW6G/action/replication_record"}},"created_at":"2026-05-18T00:42:04.777407+00:00","updated_at":"2026-05-18T00:42:04.777407+00:00"}