{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:6IRPJE6DKKHOEXC7VIVLIDWT6C","short_pith_number":"pith:6IRPJE6D","schema_version":"1.0","canonical_sha256":"f222f493c3528ee25c5faa2ab40ed3f09696c388aaa2f4555a8ce105839df2b6","source":{"kind":"arxiv","id":"1201.5391","version":2},"attestation_state":"computed","paper":{"title":"The Effects of Irradiation on Hot Jovian Atmospheres: Heat Redistribution and Energy Dissipation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Frederic Pont (U. of Exeter), Kevin Heng (ETH), Rosalba Perna (JILA/Colorado)","submitted_at":"2012-01-25T21:08:15Z","abstract_excerpt":"Hot Jupiters, due to the proximity to their parent stars, are subjected to a strong irradiating flux which governs their radiative and dynamical properties. We compute a suite of 3D circulation models with dual-band radiative transfer, exploring a relevant range of irradiation temperatures, both with and without temperature inversions. We find that, for irradiation temperatures T \\lesssim 2000 K, heat redistribution is very efficient, producing comparable day- and night-side fluxes. For Tirr \\approx 2200-2400 K, the redistribution starts to break down, resulting in a high day-night flux contra"},"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":"1201.5391","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2012-01-25T21:08:15Z","cross_cats_sorted":[],"title_canon_sha256":"34b367947a03ec3a64885e045db8459197c2ee2236cd099840690e41fe174de0","abstract_canon_sha256":"45ce27d6edf8dbd54a79440a650c235c43afe99eeb3a7860de43bf9c5c4a8758"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:58:41.868306Z","signature_b64":"1aciwHyhGt+qwMJGcFV6BUMiI9fT1JJ3XZQ4cWodx1WbmSHUsuNlz/PVZJsssGnRfl4DGD9OMMfCLUWrSGHfCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f222f493c3528ee25c5faa2ab40ed3f09696c388aaa2f4555a8ce105839df2b6","last_reissued_at":"2026-05-18T01:58:41.867426Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:58:41.867426Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Effects of Irradiation on Hot Jovian Atmospheres: Heat Redistribution and Energy Dissipation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Frederic Pont (U. of Exeter), Kevin Heng (ETH), Rosalba Perna (JILA/Colorado)","submitted_at":"2012-01-25T21:08:15Z","abstract_excerpt":"Hot Jupiters, due to the proximity to their parent stars, are subjected to a strong irradiating flux which governs their radiative and dynamical properties. We compute a suite of 3D circulation models with dual-band radiative transfer, exploring a relevant range of irradiation temperatures, both with and without temperature inversions. We find that, for irradiation temperatures T \\lesssim 2000 K, heat redistribution is very efficient, producing comparable day- and night-side fluxes. For Tirr \\approx 2200-2400 K, the redistribution starts to break down, resulting in a high day-night flux contra"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1201.5391","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":"1201.5391","created_at":"2026-05-18T01:58:41.867576+00:00"},{"alias_kind":"arxiv_version","alias_value":"1201.5391v2","created_at":"2026-05-18T01:58:41.867576+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1201.5391","created_at":"2026-05-18T01:58:41.867576+00:00"},{"alias_kind":"pith_short_12","alias_value":"6IRPJE6DKKHO","created_at":"2026-05-18T12:26:56.085431+00:00"},{"alias_kind":"pith_short_16","alias_value":"6IRPJE6DKKHOEXC7","created_at":"2026-05-18T12:26:56.085431+00:00"},{"alias_kind":"pith_short_8","alias_value":"6IRPJE6D","created_at":"2026-05-18T12:26:56.085431+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/6IRPJE6DKKHOEXC7VIVLIDWT6C","json":"https://pith.science/pith/6IRPJE6DKKHOEXC7VIVLIDWT6C.json","graph_json":"https://pith.science/api/pith-number/6IRPJE6DKKHOEXC7VIVLIDWT6C/graph.json","events_json":"https://pith.science/api/pith-number/6IRPJE6DKKHOEXC7VIVLIDWT6C/events.json","paper":"https://pith.science/paper/6IRPJE6D"},"agent_actions":{"view_html":"https://pith.science/pith/6IRPJE6DKKHOEXC7VIVLIDWT6C","download_json":"https://pith.science/pith/6IRPJE6DKKHOEXC7VIVLIDWT6C.json","view_paper":"https://pith.science/paper/6IRPJE6D","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1201.5391&json=true","fetch_graph":"https://pith.science/api/pith-number/6IRPJE6DKKHOEXC7VIVLIDWT6C/graph.json","fetch_events":"https://pith.science/api/pith-number/6IRPJE6DKKHOEXC7VIVLIDWT6C/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6IRPJE6DKKHOEXC7VIVLIDWT6C/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6IRPJE6DKKHOEXC7VIVLIDWT6C/action/storage_attestation","attest_author":"https://pith.science/pith/6IRPJE6DKKHOEXC7VIVLIDWT6C/action/author_attestation","sign_citation":"https://pith.science/pith/6IRPJE6DKKHOEXC7VIVLIDWT6C/action/citation_signature","submit_replication":"https://pith.science/pith/6IRPJE6DKKHOEXC7VIVLIDWT6C/action/replication_record"}},"created_at":"2026-05-18T01:58:41.867576+00:00","updated_at":"2026-05-18T01:58:41.867576+00:00"}