{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:IFMEKHSKCA7O2N73KZT3SAXNCV","short_pith_number":"pith:IFMEKHSK","schema_version":"1.0","canonical_sha256":"4158451e4a103eed37fb5667b902ed154108ce00f9e997535000f6e0a73f54dc","source":{"kind":"arxiv","id":"2502.19394","version":1},"attestation_state":"computed","paper":{"title":"Limited hysteresis in the atmospheric dynamics of hot Jupiters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.ao-ph"],"primary_cat":"astro-ph.EP","authors_text":"Thaddeus D. Komacek","submitted_at":"2025-02-26T18:38:00Z","abstract_excerpt":"Over the past two decades, a coherent picture has emerged of the atmospheric dynamics of hot Jupiters from a combination of three-dimensional general circulation models (GCMs) and astronomical observations. This paradigm consists of hot Jupiters being spin-synchronized due to their close-in orbit, with a resulting large day-to-night irradiation gradient driving a day-to-night temperature contrast. This day-to-night temperature contrast in turn raises day-to-night pressure gradients that are balanced by a circulation with wind speeds on the order of km~s$^{-1}$. The dominant feature of this cir"},"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":"2502.19394","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2025-02-26T18:38:00Z","cross_cats_sorted":["physics.ao-ph"],"title_canon_sha256":"1649f70fd9463a4a8be78e85a9151e5a9d30bd5c6c1ad09b8b2c9f266c641bc5","abstract_canon_sha256":"8ddf34d20abe909e96dd41e68d65b70be299f66f9554ee7e7f1112d3947751a0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:20:31.456018Z","signature_b64":"m74nK5ifx8tctNbJqqa3Jd5wdFgj/i9KB+oUVlIgO6N7VfiuriaJId6VEgA/U5gNEf9WGMa9OufnSKcyJEGbBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4158451e4a103eed37fb5667b902ed154108ce00f9e997535000f6e0a73f54dc","last_reissued_at":"2026-07-05T10:20:31.455511Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:20:31.455511Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Limited hysteresis in the atmospheric dynamics of hot Jupiters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.ao-ph"],"primary_cat":"astro-ph.EP","authors_text":"Thaddeus D. Komacek","submitted_at":"2025-02-26T18:38:00Z","abstract_excerpt":"Over the past two decades, a coherent picture has emerged of the atmospheric dynamics of hot Jupiters from a combination of three-dimensional general circulation models (GCMs) and astronomical observations. This paradigm consists of hot Jupiters being spin-synchronized due to their close-in orbit, with a resulting large day-to-night irradiation gradient driving a day-to-night temperature contrast. This day-to-night temperature contrast in turn raises day-to-night pressure gradients that are balanced by a circulation with wind speeds on the order of km~s$^{-1}$. The dominant feature of this cir"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2502.19394","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2502.19394/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":"2502.19394","created_at":"2026-07-05T10:20:31.455571+00:00"},{"alias_kind":"arxiv_version","alias_value":"2502.19394v1","created_at":"2026-07-05T10:20:31.455571+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2502.19394","created_at":"2026-07-05T10:20:31.455571+00:00"},{"alias_kind":"pith_short_12","alias_value":"IFMEKHSKCA7O","created_at":"2026-07-05T10:20:31.455571+00:00"},{"alias_kind":"pith_short_16","alias_value":"IFMEKHSKCA7O2N73","created_at":"2026-07-05T10:20:31.455571+00:00"},{"alias_kind":"pith_short_8","alias_value":"IFMEKHSK","created_at":"2026-07-05T10:20:31.455571+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2505.01397","citing_title":"Bridging the Atmospheric Circulations of Hot and Warm Giant Exoplanets","ref_index":29,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/IFMEKHSKCA7O2N73KZT3SAXNCV","json":"https://pith.science/pith/IFMEKHSKCA7O2N73KZT3SAXNCV.json","graph_json":"https://pith.science/api/pith-number/IFMEKHSKCA7O2N73KZT3SAXNCV/graph.json","events_json":"https://pith.science/api/pith-number/IFMEKHSKCA7O2N73KZT3SAXNCV/events.json","paper":"https://pith.science/paper/IFMEKHSK"},"agent_actions":{"view_html":"https://pith.science/pith/IFMEKHSKCA7O2N73KZT3SAXNCV","download_json":"https://pith.science/pith/IFMEKHSKCA7O2N73KZT3SAXNCV.json","view_paper":"https://pith.science/paper/IFMEKHSK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2502.19394&json=true","fetch_graph":"https://pith.science/api/pith-number/IFMEKHSKCA7O2N73KZT3SAXNCV/graph.json","fetch_events":"https://pith.science/api/pith-number/IFMEKHSKCA7O2N73KZT3SAXNCV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IFMEKHSKCA7O2N73KZT3SAXNCV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IFMEKHSKCA7O2N73KZT3SAXNCV/action/storage_attestation","attest_author":"https://pith.science/pith/IFMEKHSKCA7O2N73KZT3SAXNCV/action/author_attestation","sign_citation":"https://pith.science/pith/IFMEKHSKCA7O2N73KZT3SAXNCV/action/citation_signature","submit_replication":"https://pith.science/pith/IFMEKHSKCA7O2N73KZT3SAXNCV/action/replication_record"}},"created_at":"2026-07-05T10:20:31.455571+00:00","updated_at":"2026-07-05T10:20:31.455571+00:00"}