{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:F5VU3IHDZGSEIT7NTYN22K4HIP","short_pith_number":"pith:F5VU3IHD","schema_version":"1.0","canonical_sha256":"2f6b4da0e3c9a4444fed9e1bad2b8743cc2d8d91c119132470076db48935ed93","source":{"kind":"arxiv","id":"1601.00069","version":2},"attestation_state":"computed","paper":{"title":"Atmospheric Circulation of Hot Jupiters: Dayside-Nightside Temperature Differences","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Adam P. Showman, Thaddeus D. Komacek","submitted_at":"2016-01-01T09:59:13Z","abstract_excerpt":"The full-phase infrared light curves of low-eccentricity hot Jupiters show a trend of increasing dayside-to-nightside brightness temperature difference with increasing equilibrium temperature. Here we present a three-dimensional model that explains this relationship, in order to shed insight on the processes that control heat redistribution in tidally-locked planetary atmospheres. This three-dimensional model combines predictive analytic theory for the atmospheric circulation and dayside-nightside temperature differences over a range of equilibrium temperature, atmospheric composition, and pot"},"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":"1601.00069","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2016-01-01T09:59:13Z","cross_cats_sorted":[],"title_canon_sha256":"2e416b514f09a170b38a7459a753cc6ccef4e42a3d6c4d353321f03000471e74","abstract_canon_sha256":"916f6b1086c2c660b14df9f33f92f066a6b8d320e286f01d549ac9306a6bae3c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:02:21.079866Z","signature_b64":"wGZsFS5eCJGVg1sjJowZEYX/rm8R7Yunl1NMODtUjidQiYeqRCUJnq/btElF7uB8amdTamgFlQAWhi4sQF8rDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2f6b4da0e3c9a4444fed9e1bad2b8743cc2d8d91c119132470076db48935ed93","last_reissued_at":"2026-05-18T01:02:21.079196Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:02:21.079196Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Atmospheric Circulation of Hot Jupiters: Dayside-Nightside Temperature Differences","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Adam P. Showman, Thaddeus D. Komacek","submitted_at":"2016-01-01T09:59:13Z","abstract_excerpt":"The full-phase infrared light curves of low-eccentricity hot Jupiters show a trend of increasing dayside-to-nightside brightness temperature difference with increasing equilibrium temperature. Here we present a three-dimensional model that explains this relationship, in order to shed insight on the processes that control heat redistribution in tidally-locked planetary atmospheres. This three-dimensional model combines predictive analytic theory for the atmospheric circulation and dayside-nightside temperature differences over a range of equilibrium temperature, atmospheric composition, and pot"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1601.00069","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":""},"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":"1601.00069","created_at":"2026-05-18T01:02:21.079291+00:00"},{"alias_kind":"arxiv_version","alias_value":"1601.00069v2","created_at":"2026-05-18T01:02:21.079291+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1601.00069","created_at":"2026-05-18T01:02:21.079291+00:00"},{"alias_kind":"pith_short_12","alias_value":"F5VU3IHDZGSE","created_at":"2026-05-18T12:30:15.759754+00:00"},{"alias_kind":"pith_short_16","alias_value":"F5VU3IHDZGSEIT7N","created_at":"2026-05-18T12:30:15.759754+00:00"},{"alias_kind":"pith_short_8","alias_value":"F5VU3IHD","created_at":"2026-05-18T12:30:15.759754+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/F5VU3IHDZGSEIT7NTYN22K4HIP","json":"https://pith.science/pith/F5VU3IHDZGSEIT7NTYN22K4HIP.json","graph_json":"https://pith.science/api/pith-number/F5VU3IHDZGSEIT7NTYN22K4HIP/graph.json","events_json":"https://pith.science/api/pith-number/F5VU3IHDZGSEIT7NTYN22K4HIP/events.json","paper":"https://pith.science/paper/F5VU3IHD"},"agent_actions":{"view_html":"https://pith.science/pith/F5VU3IHDZGSEIT7NTYN22K4HIP","download_json":"https://pith.science/pith/F5VU3IHDZGSEIT7NTYN22K4HIP.json","view_paper":"https://pith.science/paper/F5VU3IHD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1601.00069&json=true","fetch_graph":"https://pith.science/api/pith-number/F5VU3IHDZGSEIT7NTYN22K4HIP/graph.json","fetch_events":"https://pith.science/api/pith-number/F5VU3IHDZGSEIT7NTYN22K4HIP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/F5VU3IHDZGSEIT7NTYN22K4HIP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/F5VU3IHDZGSEIT7NTYN22K4HIP/action/storage_attestation","attest_author":"https://pith.science/pith/F5VU3IHDZGSEIT7NTYN22K4HIP/action/author_attestation","sign_citation":"https://pith.science/pith/F5VU3IHDZGSEIT7NTYN22K4HIP/action/citation_signature","submit_replication":"https://pith.science/pith/F5VU3IHDZGSEIT7NTYN22K4HIP/action/replication_record"}},"created_at":"2026-05-18T01:02:21.079291+00:00","updated_at":"2026-05-18T01:02:21.079291+00:00"}