{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:LMM5IVSYACXIALWOEMXJNOK4D7","short_pith_number":"pith:LMM5IVSY","schema_version":"1.0","canonical_sha256":"5b19d4565800ae802ece232e96b95c1fca908ab5bc217459028f08f57a4c51cf","source":{"kind":"arxiv","id":"2502.04169","version":1},"attestation_state":"computed","paper":{"title":"The Effects of Kinematic MHD on the Atmospheric Circulation of Eccentric Hot Jupiters","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Hayley Beltz, Joseph R. Livesey, Juliette Becker, Laura C. Mayorga, Thaddeus D. Komacek, Willow Houck","submitted_at":"2025-02-06T15:53:58Z","abstract_excerpt":"Hot Jupiters are typically considered to be tidally locked due to their short orbital periods. The extreme irradiation can result in atmospheric species becoming thermally ionized on the dayside, which then interact with the planet's magnetic field by resisting flow across magnetic field lines, shaping the atmospheric structure. However, an eccentric orbit results in temporally dependent irradiation and a non-permanent dayside, as the planet-star distance can change drastically during its orbit. In this paper, we present 3D atmospheric models of TOI-150b, an eccentric (e=0.26), Jupiter-mass 1."},"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":"2502.04169","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.EP","submitted_at":"2025-02-06T15:53:58Z","cross_cats_sorted":[],"title_canon_sha256":"c36e941924437fe4a26e9b84f9eb275b35fe7de58746d9014f3ba3fcdf1cdbe0","abstract_canon_sha256":"255156b114734d97cacb06cfa01f61206fa6c2dd702f51e7269ec2591cd498a0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:10:34.878653Z","signature_b64":"ufFM5dZAy2AGrtlyMrLR8PPvoE3R7RGfWedo764OqotYUhmGGLAy94tnrtZv7TCJV7AVuASyMpqpqoG1dVJ6Bw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5b19d4565800ae802ece232e96b95c1fca908ab5bc217459028f08f57a4c51cf","last_reissued_at":"2026-07-05T10:10:34.878215Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:10:34.878215Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Effects of Kinematic MHD on the Atmospheric Circulation of Eccentric Hot Jupiters","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Hayley Beltz, Joseph R. Livesey, Juliette Becker, Laura C. Mayorga, Thaddeus D. Komacek, Willow Houck","submitted_at":"2025-02-06T15:53:58Z","abstract_excerpt":"Hot Jupiters are typically considered to be tidally locked due to their short orbital periods. The extreme irradiation can result in atmospheric species becoming thermally ionized on the dayside, which then interact with the planet's magnetic field by resisting flow across magnetic field lines, shaping the atmospheric structure. However, an eccentric orbit results in temporally dependent irradiation and a non-permanent dayside, as the planet-star distance can change drastically during its orbit. In this paper, we present 3D atmospheric models of TOI-150b, an eccentric (e=0.26), Jupiter-mass 1."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2502.04169","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/2502.04169/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":"2502.04169","created_at":"2026-07-05T10:10:34.878265+00:00"},{"alias_kind":"arxiv_version","alias_value":"2502.04169v1","created_at":"2026-07-05T10:10:34.878265+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2502.04169","created_at":"2026-07-05T10:10:34.878265+00:00"},{"alias_kind":"pith_short_12","alias_value":"LMM5IVSYACXI","created_at":"2026-07-05T10:10:34.878265+00:00"},{"alias_kind":"pith_short_16","alias_value":"LMM5IVSYACXIALWO","created_at":"2026-07-05T10:10:34.878265+00:00"},{"alias_kind":"pith_short_8","alias_value":"LMM5IVSY","created_at":"2026-07-05T10:10:34.878265+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/LMM5IVSYACXIALWOEMXJNOK4D7","json":"https://pith.science/pith/LMM5IVSYACXIALWOEMXJNOK4D7.json","graph_json":"https://pith.science/api/pith-number/LMM5IVSYACXIALWOEMXJNOK4D7/graph.json","events_json":"https://pith.science/api/pith-number/LMM5IVSYACXIALWOEMXJNOK4D7/events.json","paper":"https://pith.science/paper/LMM5IVSY"},"agent_actions":{"view_html":"https://pith.science/pith/LMM5IVSYACXIALWOEMXJNOK4D7","download_json":"https://pith.science/pith/LMM5IVSYACXIALWOEMXJNOK4D7.json","view_paper":"https://pith.science/paper/LMM5IVSY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2502.04169&json=true","fetch_graph":"https://pith.science/api/pith-number/LMM5IVSYACXIALWOEMXJNOK4D7/graph.json","fetch_events":"https://pith.science/api/pith-number/LMM5IVSYACXIALWOEMXJNOK4D7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LMM5IVSYACXIALWOEMXJNOK4D7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LMM5IVSYACXIALWOEMXJNOK4D7/action/storage_attestation","attest_author":"https://pith.science/pith/LMM5IVSYACXIALWOEMXJNOK4D7/action/author_attestation","sign_citation":"https://pith.science/pith/LMM5IVSYACXIALWOEMXJNOK4D7/action/citation_signature","submit_replication":"https://pith.science/pith/LMM5IVSYACXIALWOEMXJNOK4D7/action/replication_record"}},"created_at":"2026-07-05T10:10:34.878265+00:00","updated_at":"2026-07-05T10:10:34.878265+00:00"}