{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2017:NXP6O3EMXWKPHCFUSPTTQXQZBG","short_pith_number":"pith:NXP6O3EM","canonical_record":{"source":{"id":"1704.04696","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.flu-dyn","submitted_at":"2017-04-15T23:20:53Z","cross_cats_sorted":[],"title_canon_sha256":"a71f02477a4f6ede17e9a5c43c7393d732d7a807b02f348af1ff3063248f98d8","abstract_canon_sha256":"db2cb103628706e2c2893e7430cfc90ee8280a7f86fba6c5df0384737c921fc0"},"schema_version":"1.0"},"canonical_sha256":"6ddfe76c8cbd94f388b493e7385e1909895bdf16a967e7ad4122c91816580e1f","source":{"kind":"arxiv","id":"1704.04696","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1704.04696","created_at":"2026-05-18T00:35:22Z"},{"alias_kind":"arxiv_version","alias_value":"1704.04696v1","created_at":"2026-05-18T00:35:22Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1704.04696","created_at":"2026-05-18T00:35:22Z"},{"alias_kind":"pith_short_12","alias_value":"NXP6O3EMXWKP","created_at":"2026-05-18T12:31:34Z"},{"alias_kind":"pith_short_16","alias_value":"NXP6O3EMXWKPHCFU","created_at":"2026-05-18T12:31:34Z"},{"alias_kind":"pith_short_8","alias_value":"NXP6O3EM","created_at":"2026-05-18T12:31:34Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2017:NXP6O3EMXWKPHCFUSPTTQXQZBG","target":"record","payload":{"canonical_record":{"source":{"id":"1704.04696","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.flu-dyn","submitted_at":"2017-04-15T23:20:53Z","cross_cats_sorted":[],"title_canon_sha256":"a71f02477a4f6ede17e9a5c43c7393d732d7a807b02f348af1ff3063248f98d8","abstract_canon_sha256":"db2cb103628706e2c2893e7430cfc90ee8280a7f86fba6c5df0384737c921fc0"},"schema_version":"1.0"},"canonical_sha256":"6ddfe76c8cbd94f388b493e7385e1909895bdf16a967e7ad4122c91816580e1f","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:35:22.635068Z","signature_b64":"jeEgrDPPkbNIuu7/MSV6OrEXKgctEGh0GgV8EZGQ3YfP2R54y5azWNG2XKsienCM3rvzGQxlp/UJzx3zgi9HAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6ddfe76c8cbd94f388b493e7385e1909895bdf16a967e7ad4122c91816580e1f","last_reissued_at":"2026-05-18T00:35:22.634655Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:35:22.634655Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1704.04696","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":"2026-05-18T00:35:22Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"xkEk50JUBWdMUSIARcgsWQjyEkJ0Twsjxn/xyKkHnC4zvlpylTir4OFnmMtOKk6BNKr5td/eUKgxOgUKwibuBw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-23T04:44:53.719218Z"},"content_sha256":"e478da9a19a2989ce84807cbf4bfd6594b6519637dc260d13d7352464136274d","schema_version":"1.0","event_id":"sha256:e478da9a19a2989ce84807cbf4bfd6594b6519637dc260d13d7352464136274d"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2017:NXP6O3EMXWKPHCFUSPTTQXQZBG","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"The sensitivity of rapidly rotating Rayleigh--B\\'enard convection to Ekman pumping","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"physics.flu-dyn","authors_text":"Keith Julien, Meredith Plumley, Philippe Marti, Stephan Stellmach","submitted_at":"2017-04-15T23:20:53Z","abstract_excerpt":"The dependence of the heat transfer, as measured by the nondimensional Nusselt number $Nu$, on Ekman pumping for rapidly rotating Rayleigh-B\\'enard convection in an infinite plane layer is examined for fluids with Prandtl number $Pr = 1$. A joint effort utilizing simulations from the Composite Non-hydrostatic Quasi-Geostrophic model (CNH-QGM) and direct numerical simulations (DNS) of the incompressible fluid equations has mapped a wide range of the Rayleigh number $Ra$ - Ekman number $E$ parameter space within the geostrophic regime of rotating convection. Corroboration of the $Nu$-$Ra$ relati"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1704.04696","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":"2026-05-18T00:35:22Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"zXU7bNjwZtshaQ2VtBMV1la3IIUdbOZnsRvV/5y/ebRnnCpFZ0L8Hsksd7V+h+eucTPGBthiG9x2lcQ+SutmCg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-23T04:44:53.719576Z"},"content_sha256":"ecff4628e823fe3bc85674649f63ac2467bbfafe94ae2e9c60606afd34ea098f","schema_version":"1.0","event_id":"sha256:ecff4628e823fe3bc85674649f63ac2467bbfafe94ae2e9c60606afd34ea098f"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/NXP6O3EMXWKPHCFUSPTTQXQZBG/bundle.json","state_url":"https://pith.science/pith/NXP6O3EMXWKPHCFUSPTTQXQZBG/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/NXP6O3EMXWKPHCFUSPTTQXQZBG/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":"2026-06-23T04:44:53Z","links":{"resolver":"https://pith.science/pith/NXP6O3EMXWKPHCFUSPTTQXQZBG","bundle":"https://pith.science/pith/NXP6O3EMXWKPHCFUSPTTQXQZBG/bundle.json","state":"https://pith.science/pith/NXP6O3EMXWKPHCFUSPTTQXQZBG/state.json","well_known_bundle":"https://pith.science/.well-known/pith/NXP6O3EMXWKPHCFUSPTTQXQZBG/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2017:NXP6O3EMXWKPHCFUSPTTQXQZBG","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":"db2cb103628706e2c2893e7430cfc90ee8280a7f86fba6c5df0384737c921fc0","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.flu-dyn","submitted_at":"2017-04-15T23:20:53Z","title_canon_sha256":"a71f02477a4f6ede17e9a5c43c7393d732d7a807b02f348af1ff3063248f98d8"},"schema_version":"1.0","source":{"id":"1704.04696","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1704.04696","created_at":"2026-05-18T00:35:22Z"},{"alias_kind":"arxiv_version","alias_value":"1704.04696v1","created_at":"2026-05-18T00:35:22Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1704.04696","created_at":"2026-05-18T00:35:22Z"},{"alias_kind":"pith_short_12","alias_value":"NXP6O3EMXWKP","created_at":"2026-05-18T12:31:34Z"},{"alias_kind":"pith_short_16","alias_value":"NXP6O3EMXWKPHCFU","created_at":"2026-05-18T12:31:34Z"},{"alias_kind":"pith_short_8","alias_value":"NXP6O3EM","created_at":"2026-05-18T12:31:34Z"}],"graph_snapshots":[{"event_id":"sha256:ecff4628e823fe3bc85674649f63ac2467bbfafe94ae2e9c60606afd34ea098f","target":"graph","created_at":"2026-05-18T00:35:22Z","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":"The dependence of the heat transfer, as measured by the nondimensional Nusselt number $Nu$, on Ekman pumping for rapidly rotating Rayleigh-B\\'enard convection in an infinite plane layer is examined for fluids with Prandtl number $Pr = 1$. A joint effort utilizing simulations from the Composite Non-hydrostatic Quasi-Geostrophic model (CNH-QGM) and direct numerical simulations (DNS) of the incompressible fluid equations has mapped a wide range of the Rayleigh number $Ra$ - Ekman number $E$ parameter space within the geostrophic regime of rotating convection. Corroboration of the $Nu$-$Ra$ relati","authors_text":"Keith Julien, Meredith Plumley, Philippe Marti, Stephan Stellmach","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.flu-dyn","submitted_at":"2017-04-15T23:20:53Z","title":"The sensitivity of rapidly rotating Rayleigh--B\\'enard convection to Ekman pumping"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1704.04696","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:e478da9a19a2989ce84807cbf4bfd6594b6519637dc260d13d7352464136274d","target":"record","created_at":"2026-05-18T00:35:22Z","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":"db2cb103628706e2c2893e7430cfc90ee8280a7f86fba6c5df0384737c921fc0","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.flu-dyn","submitted_at":"2017-04-15T23:20:53Z","title_canon_sha256":"a71f02477a4f6ede17e9a5c43c7393d732d7a807b02f348af1ff3063248f98d8"},"schema_version":"1.0","source":{"id":"1704.04696","kind":"arxiv","version":1}},"canonical_sha256":"6ddfe76c8cbd94f388b493e7385e1909895bdf16a967e7ad4122c91816580e1f","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"6ddfe76c8cbd94f388b493e7385e1909895bdf16a967e7ad4122c91816580e1f","first_computed_at":"2026-05-18T00:35:22.634655Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:35:22.634655Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"jeEgrDPPkbNIuu7/MSV6OrEXKgctEGh0GgV8EZGQ3YfP2R54y5azWNG2XKsienCM3rvzGQxlp/UJzx3zgi9HAA==","signature_status":"signed_v1","signed_at":"2026-05-18T00:35:22.635068Z","signed_message":"canonical_sha256_bytes"},"source_id":"1704.04696","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:e478da9a19a2989ce84807cbf4bfd6594b6519637dc260d13d7352464136274d","sha256:ecff4628e823fe3bc85674649f63ac2467bbfafe94ae2e9c60606afd34ea098f"],"state_sha256":"5eda51cba06bdb7a635d84a935b048c8f8af6c7fed869d80e604be0ca3f9a374"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"TRORIpaZGnm+wEJBmmfNy82PLPF/Lou2gXUMAXNSij9Oyttb0r68oGboIhMZiFvoP2s/Xg4tf+has3q1y0CuDA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-23T04:44:53.721384Z","bundle_sha256":"1f4e9ab079853d1d8802eaa5de6c6bc2020fabdaa2418e939c55d683919abebb"}}