{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2009:WT4C52ML532N52QCD5YMFQFWLP","short_pith_number":"pith:WT4C52ML","schema_version":"1.0","canonical_sha256":"b4f82ee98beef4deea021f70c2c0b65bf9882138a427bce44676b3f20b376837","source":{"kind":"arxiv","id":"0910.1346","version":2},"attestation_state":"computed","paper":{"title":"Radiation-Hydrodynamics of Hot Jupiter Atmospheres","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Emily Rauscher (Columbia), Kristen Menou","submitted_at":"2009-10-07T20:08:35Z","abstract_excerpt":"Radiative transfer in planetary atmospheres is usually treated in the static limit, i.e., neglecting atmospheric motions. We argue that hot Jupiter atmospheres, with possibly fast (sonic) wind speeds, may require a more strongly coupled treatment, formally in the regime of radiation-hydrodynamics. To lowest order in v/c, relativistic Doppler shifts distort line profiles along optical paths with finite wind velocity gradients. This leads to flow-dependent deviations in the effective emission and absorption properties of the atmospheric medium. Evaluating the overall impact of these distortions "},"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":"0910.1346","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2009-10-07T20:08:35Z","cross_cats_sorted":[],"title_canon_sha256":"500cb8cd4aa4bdfeb24c6a9f508d0e5400ed21c929fee3969d74971101045e05","abstract_canon_sha256":"56c01f88a2995d60b9b6869b65be18aa9e7faf2fe9d9c47bfded862c0cffa8df"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:34:19.793993Z","signature_b64":"KaZjLcls6j2FRaiHDL9FYP8/9pBvDUOz/3nKPCV0iu5hkm02sNTdC2t/DEUrUWbW5DlXZmMF3VjnmpUjBTubDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b4f82ee98beef4deea021f70c2c0b65bf9882138a427bce44676b3f20b376837","last_reissued_at":"2026-05-18T02:34:19.793550Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:34:19.793550Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Radiation-Hydrodynamics of Hot Jupiter Atmospheres","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Emily Rauscher (Columbia), Kristen Menou","submitted_at":"2009-10-07T20:08:35Z","abstract_excerpt":"Radiative transfer in planetary atmospheres is usually treated in the static limit, i.e., neglecting atmospheric motions. We argue that hot Jupiter atmospheres, with possibly fast (sonic) wind speeds, may require a more strongly coupled treatment, formally in the regime of radiation-hydrodynamics. To lowest order in v/c, relativistic Doppler shifts distort line profiles along optical paths with finite wind velocity gradients. This leads to flow-dependent deviations in the effective emission and absorption properties of the atmospheric medium. Evaluating the overall impact of these distortions "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0910.1346","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":"0910.1346","created_at":"2026-05-18T02:34:19.793617+00:00"},{"alias_kind":"arxiv_version","alias_value":"0910.1346v2","created_at":"2026-05-18T02:34:19.793617+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0910.1346","created_at":"2026-05-18T02:34:19.793617+00:00"},{"alias_kind":"pith_short_12","alias_value":"WT4C52ML532N","created_at":"2026-05-18T12:26:02.257875+00:00"},{"alias_kind":"pith_short_16","alias_value":"WT4C52ML532N52QC","created_at":"2026-05-18T12:26:02.257875+00:00"},{"alias_kind":"pith_short_8","alias_value":"WT4C52ML","created_at":"2026-05-18T12:26:02.257875+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/WT4C52ML532N52QCD5YMFQFWLP","json":"https://pith.science/pith/WT4C52ML532N52QCD5YMFQFWLP.json","graph_json":"https://pith.science/api/pith-number/WT4C52ML532N52QCD5YMFQFWLP/graph.json","events_json":"https://pith.science/api/pith-number/WT4C52ML532N52QCD5YMFQFWLP/events.json","paper":"https://pith.science/paper/WT4C52ML"},"agent_actions":{"view_html":"https://pith.science/pith/WT4C52ML532N52QCD5YMFQFWLP","download_json":"https://pith.science/pith/WT4C52ML532N52QCD5YMFQFWLP.json","view_paper":"https://pith.science/paper/WT4C52ML","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0910.1346&json=true","fetch_graph":"https://pith.science/api/pith-number/WT4C52ML532N52QCD5YMFQFWLP/graph.json","fetch_events":"https://pith.science/api/pith-number/WT4C52ML532N52QCD5YMFQFWLP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WT4C52ML532N52QCD5YMFQFWLP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WT4C52ML532N52QCD5YMFQFWLP/action/storage_attestation","attest_author":"https://pith.science/pith/WT4C52ML532N52QCD5YMFQFWLP/action/author_attestation","sign_citation":"https://pith.science/pith/WT4C52ML532N52QCD5YMFQFWLP/action/citation_signature","submit_replication":"https://pith.science/pith/WT4C52ML532N52QCD5YMFQFWLP/action/replication_record"}},"created_at":"2026-05-18T02:34:19.793617+00:00","updated_at":"2026-05-18T02:34:19.793617+00:00"}