{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:I76MLT3Z3RD7NVC4FN5BIMIYOQ","short_pith_number":"pith:I76MLT3Z","schema_version":"1.0","canonical_sha256":"47fcc5cf79dc47f6d45c2b7a1431187439677448d6febb94e86ff61f4eb8b0d4","source":{"kind":"arxiv","id":"2305.19479","version":1},"attestation_state":"computed","paper":{"title":"A Shallow Water Model Exploration of Atmospheric Circulation on Sub-Neptunes: Effects of Radiative Forcing and Rotation Period","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Alice Nadeau, Ekaterina Landgren, Nikole Lewis, Peter Hitchcock, Tiffany Kataria","submitted_at":"2023-05-31T01:14:02Z","abstract_excerpt":"Sub-Neptune type exoplanets are abundant in our galaxy yet have no solar system analogs. They exist in a broad range of stellar forcing and rotational regimes that are distinctly different from solar system planets and more commonly studied hot Jupiters. Here we present simulations that explore global atmospheric circulation of sub-Neptunes generated with a two-dimensional shallow-water model, SWAMPE. We explore the circulation regimes of synchronously rotating sub-Neptunes with a focus on the interaction of planetary rotation rate and radiative timescale in a variety of stellar insolations. I"},"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":"2305.19479","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.EP","submitted_at":"2023-05-31T01:14:02Z","cross_cats_sorted":[],"title_canon_sha256":"46cf951ce28010c2612ec15bf229357e8875ea9683c2297ee1835159ba5096cb","abstract_canon_sha256":"72163a71bf612f1ec355455e240c6105a2b3cb6b71ac7fb3787bf5d718719067"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:15:50.655349Z","signature_b64":"GM8gvy5538DcTPSWFuBWOj2cNQr35CIIcs8yCf7YVLXzx5paIM1BPeQH905ULQcJyym1o9w59IfIz208yAw2Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"47fcc5cf79dc47f6d45c2b7a1431187439677448d6febb94e86ff61f4eb8b0d4","last_reissued_at":"2026-07-05T06:15:50.654820Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:15:50.654820Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Shallow Water Model Exploration of Atmospheric Circulation on Sub-Neptunes: Effects of Radiative Forcing and Rotation Period","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Alice Nadeau, Ekaterina Landgren, Nikole Lewis, Peter Hitchcock, Tiffany Kataria","submitted_at":"2023-05-31T01:14:02Z","abstract_excerpt":"Sub-Neptune type exoplanets are abundant in our galaxy yet have no solar system analogs. They exist in a broad range of stellar forcing and rotational regimes that are distinctly different from solar system planets and more commonly studied hot Jupiters. Here we present simulations that explore global atmospheric circulation of sub-Neptunes generated with a two-dimensional shallow-water model, SWAMPE. We explore the circulation regimes of synchronously rotating sub-Neptunes with a focus on the interaction of planetary rotation rate and radiative timescale in a variety of stellar insolations. I"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2305.19479","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/2305.19479/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":"2305.19479","created_at":"2026-07-05T06:15:50.654891+00:00"},{"alias_kind":"arxiv_version","alias_value":"2305.19479v1","created_at":"2026-07-05T06:15:50.654891+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2305.19479","created_at":"2026-07-05T06:15:50.654891+00:00"},{"alias_kind":"pith_short_12","alias_value":"I76MLT3Z3RD7","created_at":"2026-07-05T06:15:50.654891+00:00"},{"alias_kind":"pith_short_16","alias_value":"I76MLT3Z3RD7NVC4","created_at":"2026-07-05T06:15:50.654891+00:00"},{"alias_kind":"pith_short_8","alias_value":"I76MLT3Z","created_at":"2026-07-05T06:15:50.654891+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/I76MLT3Z3RD7NVC4FN5BIMIYOQ","json":"https://pith.science/pith/I76MLT3Z3RD7NVC4FN5BIMIYOQ.json","graph_json":"https://pith.science/api/pith-number/I76MLT3Z3RD7NVC4FN5BIMIYOQ/graph.json","events_json":"https://pith.science/api/pith-number/I76MLT3Z3RD7NVC4FN5BIMIYOQ/events.json","paper":"https://pith.science/paper/I76MLT3Z"},"agent_actions":{"view_html":"https://pith.science/pith/I76MLT3Z3RD7NVC4FN5BIMIYOQ","download_json":"https://pith.science/pith/I76MLT3Z3RD7NVC4FN5BIMIYOQ.json","view_paper":"https://pith.science/paper/I76MLT3Z","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2305.19479&json=true","fetch_graph":"https://pith.science/api/pith-number/I76MLT3Z3RD7NVC4FN5BIMIYOQ/graph.json","fetch_events":"https://pith.science/api/pith-number/I76MLT3Z3RD7NVC4FN5BIMIYOQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/I76MLT3Z3RD7NVC4FN5BIMIYOQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/I76MLT3Z3RD7NVC4FN5BIMIYOQ/action/storage_attestation","attest_author":"https://pith.science/pith/I76MLT3Z3RD7NVC4FN5BIMIYOQ/action/author_attestation","sign_citation":"https://pith.science/pith/I76MLT3Z3RD7NVC4FN5BIMIYOQ/action/citation_signature","submit_replication":"https://pith.science/pith/I76MLT3Z3RD7NVC4FN5BIMIYOQ/action/replication_record"}},"created_at":"2026-07-05T06:15:50.654891+00:00","updated_at":"2026-07-05T06:15:50.654891+00:00"}