{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2018:JIVGIJTFKBZOFME27P5OVIN2HI","short_pith_number":"pith:JIVGIJTF","canonical_record":{"source":{"id":"1802.03026","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2018-02-08T19:13:23Z","cross_cats_sorted":[],"title_canon_sha256":"6d850a6d7e8007f52b970ee0ee9f2e2fe59e7b3b46bd650389cafcaacc7906af","abstract_canon_sha256":"c6d856fbefe6e51d1d411c7a78d389104508fcf71a28602dc76d48ec86a29b37"},"schema_version":"1.0"},"canonical_sha256":"4a2a6426655072e2b09afbfaeaa1ba3a2a778b061235a7ce43cd7b5e4e578d63","source":{"kind":"arxiv","id":"1802.03026","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1802.03026","created_at":"2026-05-18T00:24:02Z"},{"alias_kind":"arxiv_version","alias_value":"1802.03026v1","created_at":"2026-05-18T00:24:02Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1802.03026","created_at":"2026-05-18T00:24:02Z"},{"alias_kind":"pith_short_12","alias_value":"JIVGIJTFKBZO","created_at":"2026-05-18T12:32:31Z"},{"alias_kind":"pith_short_16","alias_value":"JIVGIJTFKBZOFME2","created_at":"2026-05-18T12:32:31Z"},{"alias_kind":"pith_short_8","alias_value":"JIVGIJTF","created_at":"2026-05-18T12:32:31Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2018:JIVGIJTFKBZOFME27P5OVIN2HI","target":"record","payload":{"canonical_record":{"source":{"id":"1802.03026","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2018-02-08T19:13:23Z","cross_cats_sorted":[],"title_canon_sha256":"6d850a6d7e8007f52b970ee0ee9f2e2fe59e7b3b46bd650389cafcaacc7906af","abstract_canon_sha256":"c6d856fbefe6e51d1d411c7a78d389104508fcf71a28602dc76d48ec86a29b37"},"schema_version":"1.0"},"canonical_sha256":"4a2a6426655072e2b09afbfaeaa1ba3a2a778b061235a7ce43cd7b5e4e578d63","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:24:02.207332Z","signature_b64":"Et+G6FDFJicJNlhibVflmtOCYeEVnD/zYrDUqXhYYAaoKf0LeqJ7kwo+EFgkyD2wi4yTECD7m1AX0N2NI7bNBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4a2a6426655072e2b09afbfaeaa1ba3a2a778b061235a7ce43cd7b5e4e578d63","last_reissued_at":"2026-05-18T00:24:02.206677Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:24:02.206677Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1802.03026","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:24:02Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"WkxoDyCfvgDe9N4UQlI9iXSf2R7NAxkU9b4wYFPW/OQZSDE8+P7oxzh4oGE6+acqNLbgsrGfoVzPjgCwyLRGCw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-11T04:16:51.836809Z"},"content_sha256":"e22dc33d0563af6a50da8d83fe756dc1a0cd20496ca09bddb0f0e349b2de1305","schema_version":"1.0","event_id":"sha256:e22dc33d0563af6a50da8d83fe756dc1a0cd20496ca09bddb0f0e349b2de1305"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2018:JIVGIJTFKBZOFME27P5OVIN2HI","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Convective dynamics and disequilibrium chemistry in the atmospheres of giant planets and brown dwarfs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Baylee Bordwell, Benjamin P. Brown, Jeffrey S. Oishi","submitted_at":"2018-02-08T19:13:23Z","abstract_excerpt":"Disequilibrium chemical processes have a large effect upon the spectra of substellar objects. To study these effects, dynamical disequilibrium has been parameterized using the quench and eddy diffusion approximations, but little work has been done to explore how these approximations perform under realistic planetary conditions in different dynamical regimes. As a first step in addressing this problem, we study the localized, small scale convective dynamics of planetary atmospheres by direct numerical simulation of fully compressible hydrodynamics with reactive tracers using the Dedalus code. U"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1802.03026","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":""},"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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:24:02Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"cVCcuAQfx//ccjDoEjB6jTTzrBKoAvijGHDwpTcxCy1TVsNwVpNreVRwa9Husy6ar9Y64dBqBTpPMrZZLhB1AA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-11T04:16:51.837552Z"},"content_sha256":"1d84d05940656db3a70262b813fd8797cbdb559e1e441dbb315b632ceffde00d","schema_version":"1.0","event_id":"sha256:1d84d05940656db3a70262b813fd8797cbdb559e1e441dbb315b632ceffde00d"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/JIVGIJTFKBZOFME27P5OVIN2HI/bundle.json","state_url":"https://pith.science/pith/JIVGIJTFKBZOFME27P5OVIN2HI/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/JIVGIJTFKBZOFME27P5OVIN2HI/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-06-11T04:16:51Z","links":{"resolver":"https://pith.science/pith/JIVGIJTFKBZOFME27P5OVIN2HI","bundle":"https://pith.science/pith/JIVGIJTFKBZOFME27P5OVIN2HI/bundle.json","state":"https://pith.science/pith/JIVGIJTFKBZOFME27P5OVIN2HI/state.json","well_known_bundle":"https://pith.science/.well-known/pith/JIVGIJTFKBZOFME27P5OVIN2HI/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2018:JIVGIJTFKBZOFME27P5OVIN2HI","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"c6d856fbefe6e51d1d411c7a78d389104508fcf71a28602dc76d48ec86a29b37","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2018-02-08T19:13:23Z","title_canon_sha256":"6d850a6d7e8007f52b970ee0ee9f2e2fe59e7b3b46bd650389cafcaacc7906af"},"schema_version":"1.0","source":{"id":"1802.03026","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1802.03026","created_at":"2026-05-18T00:24:02Z"},{"alias_kind":"arxiv_version","alias_value":"1802.03026v1","created_at":"2026-05-18T00:24:02Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1802.03026","created_at":"2026-05-18T00:24:02Z"},{"alias_kind":"pith_short_12","alias_value":"JIVGIJTFKBZO","created_at":"2026-05-18T12:32:31Z"},{"alias_kind":"pith_short_16","alias_value":"JIVGIJTFKBZOFME2","created_at":"2026-05-18T12:32:31Z"},{"alias_kind":"pith_short_8","alias_value":"JIVGIJTF","created_at":"2026-05-18T12:32:31Z"}],"graph_snapshots":[{"event_id":"sha256:1d84d05940656db3a70262b813fd8797cbdb559e1e441dbb315b632ceffde00d","target":"graph","created_at":"2026-05-18T00:24:02Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"Disequilibrium chemical processes have a large effect upon the spectra of substellar objects. To study these effects, dynamical disequilibrium has been parameterized using the quench and eddy diffusion approximations, but little work has been done to explore how these approximations perform under realistic planetary conditions in different dynamical regimes. As a first step in addressing this problem, we study the localized, small scale convective dynamics of planetary atmospheres by direct numerical simulation of fully compressible hydrodynamics with reactive tracers using the Dedalus code. U","authors_text":"Baylee Bordwell, Benjamin P. Brown, Jeffrey S. Oishi","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2018-02-08T19:13:23Z","title":"Convective dynamics and disequilibrium chemistry in the atmospheres of giant planets and brown dwarfs"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1802.03026","kind":"arxiv","version":1},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:e22dc33d0563af6a50da8d83fe756dc1a0cd20496ca09bddb0f0e349b2de1305","target":"record","created_at":"2026-05-18T00:24:02Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"c6d856fbefe6e51d1d411c7a78d389104508fcf71a28602dc76d48ec86a29b37","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2018-02-08T19:13:23Z","title_canon_sha256":"6d850a6d7e8007f52b970ee0ee9f2e2fe59e7b3b46bd650389cafcaacc7906af"},"schema_version":"1.0","source":{"id":"1802.03026","kind":"arxiv","version":1}},"canonical_sha256":"4a2a6426655072e2b09afbfaeaa1ba3a2a778b061235a7ce43cd7b5e4e578d63","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"4a2a6426655072e2b09afbfaeaa1ba3a2a778b061235a7ce43cd7b5e4e578d63","first_computed_at":"2026-05-18T00:24:02.206677Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:24:02.206677Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"Et+G6FDFJicJNlhibVflmtOCYeEVnD/zYrDUqXhYYAaoKf0LeqJ7kwo+EFgkyD2wi4yTECD7m1AX0N2NI7bNBw==","signature_status":"signed_v1","signed_at":"2026-05-18T00:24:02.207332Z","signed_message":"canonical_sha256_bytes"},"source_id":"1802.03026","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:e22dc33d0563af6a50da8d83fe756dc1a0cd20496ca09bddb0f0e349b2de1305","sha256:1d84d05940656db3a70262b813fd8797cbdb559e1e441dbb315b632ceffde00d"],"state_sha256":"33ce6d0df38f18ab4a60568466588474da6dd0e0aa9a97d2d2eb32c5c78fe3f8"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"sgmzTSA9DfCTpItd2v23HdaFbZ4H82eQ+ECx1cn4YCbxAUIuJPkuB6oSMUmM5KSp33SPmrw+EpqrKjo7O3yfBg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-11T04:16:51.841241Z","bundle_sha256":"c2696e0146d11e5bbccd159dee131f5fe2851792dc84dbbd1c87e93c2c68cda0"}}