{"as_of":"2026-08-14T07:37:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:3c32adf9138996ad47f8ab3558b251c40e88232c6c413a8cf72e7d17c34fb1a9","coverage":[{"denominator":22,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":22,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-09T17:06:16.348118Z","state":"measured"},{"denominator":24,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":24,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-14T06:32:32.682623+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-08T14:10:21.854418Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-07-10T15:27:20.192934Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2502.00974","last_updated":"2025-02-03T00:55:40Z","snapshot_observed_at":"2026-08-13T11:34:41.622007Z","submitted_at":"2025-02-03T00:55:40Z","title":"Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.00974","snapshot_observed_at":"2026-08-08T14:10:21.854418Z","title":"N., & Wray, A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.07006","last_updated":"2025-02-10T20:11:04Z","snapshot_observed_at":"2026-08-10T10:17:22.810544Z","submitted_at":"2025-02-10T20:11:04Z","title":"Properties of Turbulent Convection and Large-Scale Flows in a Rotating F-type Star Revealed by 3D Realistic Radiative Hydrodynamic Simulations","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-08T14:10:21.854418Z"},"links":{"cited_paper":"/paper/2502.00974","citing_paper":"/paper/2502.07006"},"observation_digest":"sha256:2020a330d528352deb27829234c051c0a8175f4a6e4edbd3694103ee1ed45597","observation_id":"4359521a-42c8-4c94-93a5-6a30e8b35514","resolution":{"observed_at":"2026-08-08T14:10:21.854418Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.00974","last_updated":"2025-02-03T00:55:40Z","snapshot_observed_at":"2026-08-13T11:34:41.622007Z","submitted_at":"2025-02-03T00:55:40Z","title":"Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling","version":1},"cited_work":{"arxiv_id":"2502.00974","doi":null,"metadata_source":"pith","pith_arxiv_id":"2502.00974","snapshot_observed_at":"2026-07-10T15:27:20.192934Z","title":"Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling","venue":"astro-ph.SR","work_id":"624d39aa-2327-44f8-9eed-f8a1babc9c08","year":2025},"citing_paper":{"arxiv_id":"2607.07925","last_updated":"2026-07-08T21:16:10Z","snapshot_observed_at":"2026-08-12T20:37:13.168260Z","submitted_at":"2026-07-08T21:16:10Z","title":"Cluster-Weighted Training of Deep Surrogate Models for Subgrid Turbulent Transport","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-07-10T15:20:03.307437Z"},"links":{"cited_paper":"/paper/2502.00974","citing_paper":"/paper/2607.07925"},"observation_digest":"sha256:e1c9247c29027dd27c9f2d1787fc92a6c502fd72d9e447e2ba62a6835a4fe9d6","observation_id":"b5ff9361-3f1f-4003-823f-b0178a05bea3","resolution":{"observed_at":"2026-07-10T15:27:20.194353Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2502.00974/citation-record","integrity":"/paper/2502.00974/integrity","json":"/paper/2502.00974/citation-record.json","paper":"/paper/2502.00974"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:06:16.704607Z","title":"2018, Diﬀere ntial Rotation in Solar-like Con- vective Envelopes: Inﬂuence of Overshoot and Magnetism","venue":null,"work_id":"7b34d46d-1980-4024-b1e5-25cd62799f7d","year":2018},"citing_paper":{"arxiv_id":"2502.00974","last_updated":"2025-02-03T00:55:40Z","snapshot_observed_at":"2026-08-13T11:34:41.622007Z","submitted_at":"2025-02-03T00:55:40Z","title":"Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-09T17:06:16.245771Z"},"links":{"citing_paper":"/paper/2502.00974"},"observation_digest":"sha256:cb79ff0f6c470c90c503d64b88cdc9edb02236347494ec3f6b303e14269659d9","observation_id":"b99851fc-a4c8-4b91-9e7f-043d9bb19498","resolution":{"observed_at":"2026-08-09T17:06:16.710078Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:06:16.445301Z","title":"Kitiashvili, Alan A","venue":null,"work_id":"65c8fd22-478b-4f96-bc6c-030ad239acea","year":2007},"citing_paper":{"arxiv_id":"2502.00974","last_updated":"2025-02-03T00:55:40Z","snapshot_observed_at":"2026-08-13T11:34:41.622007Z","submitted_at":"2025-02-03T00:55:40Z","title":"Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-09T17:06:16.327984Z"},"links":{"citing_paper":"/paper/2502.00974"},"observation_digest":"sha256:9416e911d5977e069cb1db4b5f983ffccc24d46b2b955c8e7041a3d4ee62a22a","observation_id":"69d7020e-f71e-43b9-9001-f08b5ab0536b","resolution":{"observed_at":"2026-08-09T17:06:16.450243Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:06:16.476751Z","title":"I., Hindman, B","venue":null,"work_id":"e2eae967-a755-415b-942f-740de106099b","year":2019},"citing_paper":{"arxiv_id":"2502.00974","last_updated":"2025-02-03T00:55:40Z","snapshot_observed_at":"2026-08-13T11:34:41.622007Z","submitted_at":"2025-02-03T00:55:40Z","title":"Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-09T17:06:16.317897Z"},"links":{"citing_paper":"/paper/2502.00974"},"observation_digest":"sha256:a39740b0e2f6b318a0a2567b67cb1a10434a57916977bcd65be343421bfb1095","observation_id":"66b34c46-77fe-4bbb-a839-b8a95c8a761c","resolution":{"observed_at":"2026-08-09T17:06:16.482073Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:06:16.551249Z","title":null,"venue":null,"work_id":"87125947-7f2b-4e2d-bc30-8955630b3091","year":2019},"citing_paper":{"arxiv_id":"2502.00974","last_updated":"2025-02-03T00:55:40Z","snapshot_observed_at":"2026-08-13T11:34:41.622007Z","submitted_at":"2025-02-03T00:55:40Z","title":"Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-09T17:06:16.293538Z"},"links":{"citing_paper":"/paper/2502.00974"},"observation_digest":"sha256:a071f3acf582bed45ad3e907821fc4b66421f7898add4ba4a26443949b9ad317","observation_id":"acc00f39-1c45-4b2a-b6cc-e0129097757b","resolution":{"observed_at":"2026-08-09T17:06:16.556485Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:06:16.599545Z","title":"2022, Generation of Sola r-like Diﬀerential Rotation","venue":null,"work_id":"e3d9988a-25eb-4fbe-97a0-6303cbaec4b6","year":2022},"citing_paper":{"arxiv_id":"2502.00974","last_updated":"2025-02-03T00:55:40Z","snapshot_observed_at":"2026-08-13T11:34:41.622007Z","submitted_at":"2025-02-03T00:55:40Z","title":"Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-09T17:06:16.279993Z"},"links":{"citing_paper":"/paper/2502.00974"},"observation_digest":"sha256:5db90b67d2179cc23e8443d592619e849286fcdf32aa2bf1e80dfa5b95fc2ad0","observation_id":"0d7c7e1b-64c6-4d16-b593-6a2a6c33a368","resolution":{"observed_at":"2026-08-09T17:06:16.604629Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:06:16.508516Z","title":"2021, Divergence and Vorticity of Subsurface Flows During Solar Cycles 23 and","venue":null,"work_id":"beefc0d4-5b26-4352-97b4-86484493143e","year":2021},"citing_paper":{"arxiv_id":"2502.00974","last_updated":"2025-02-03T00:55:40Z","snapshot_observed_at":"2026-08-13T11:34:41.622007Z","submitted_at":"2025-02-03T00:55:40Z","title":"Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-09T17:06:16.307207Z"},"links":{"citing_paper":"/paper/2502.00974"},"observation_digest":"sha256:6bd613e4904a1b96a61dfb09b2670be5cfd7faabbcbcaf6b5ba9ff3c94b495ab","observation_id":"d314a2d3-fbcc-40d2-b4a7-0e7425ed6cff","resolution":{"observed_at":"2026-08-09T17:06:16.513042Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:06:16.396350Z","title":null,"venue":null,"work_id":"c369cb7a-3083-41cf-bb44-5a6423b706f0","year":2001},"citing_paper":{"arxiv_id":"2502.00974","last_updated":"2025-02-03T00:55:40Z","snapshot_observed_at":"2026-08-13T11:34:41.622007Z","submitted_at":"2025-02-03T00:55:40Z","title":"Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-09T17:06:16.343159Z"},"links":{"citing_paper":"/paper/2502.00974"},"observation_digest":"sha256:0da5096ac83103c45afee00ccfb3325773a6f9f7232be1e8933a47d4b4ad8ee1","observation_id":"7eeb64b5-35b6-4f2f-a353-207d15116438","resolution":{"observed_at":"2026-08-09T17:06:16.402200Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:06:16.566636Z","title":"Jain, K., Tripathy, S","venue":null,"work_id":"a5579152-645e-42c5-a43b-b80010563ca2","year":1935},"citing_paper":{"arxiv_id":"2502.00974","last_updated":"2025-02-03T00:55:40Z","snapshot_observed_at":"2026-08-13T11:34:41.622007Z","submitted_at":"2025-02-03T00:55:40Z","title":"Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-09T17:06:16.289088Z"},"links":{"citing_paper":"/paper/2502.00974"},"observation_digest":"sha256:d1a612f5f88d482a9be026ac57f2003dd0adc624374ad6346aae63d0b017ae94","observation_id":"32effa7e-8521-4461-b8cf-6126a92b76d0","resolution":{"observed_at":"2026-08-09T17:06:16.571927Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1507.07999","last_updated":"2015-07-29T01:24:45Z","snapshot_observed_at":"2026-08-14T07:15:10.128026Z","submitted_at":"2015-07-29T01:24:45Z","title":"Simulations of Stellar Magnetoconvection using the Radiative MHD Code `StellarBox'","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1507.07999","snapshot_observed_at":"2026-08-09T17:06:16.348118Z","title":"& K¨ apyl¨ a, M","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.00974","last_updated":"2025-02-03T00:55:40Z","snapshot_observed_at":"2026-08-13T11:34:41.622007Z","submitted_at":"2025-02-03T00:55:40Z","title":"Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-09T17:06:16.348118Z"},"links":{"cited_paper":"/paper/1507.07999","citing_paper":"/paper/2502.00974"},"observation_digest":"sha256:91e44ee24a47a395ec619dd59a49c6ec4f1f1aa398deeb2fc606e582eafb54fb","observation_id":"b1fd4d36-35b2-4909-aafe-5b5250656b59","resolution":{"observed_at":"2026-08-09T17:06:16.348118Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:06:16.523007Z","title":"N., Kosovichev, A","venue":null,"work_id":"04dca10a-0f86-4726-8819-bd44e08666dc","year":2010},"citing_paper":{"arxiv_id":"2502.00974","last_updated":"2025-02-03T00:55:40Z","snapshot_observed_at":"2026-08-13T11:34:41.622007Z","submitted_at":"2025-02-03T00:55:40Z","title":"Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-09T17:06:16.302775Z"},"links":{"citing_paper":"/paper/2502.00974"},"observation_digest":"sha256:48632287bc7bb0f3464ed150ce1d81b849502957c10ccceb8faafb978e04b464","observation_id":"778895a2-d4b1-47d5-92cd-37739a90705b","resolution":{"observed_at":"2026-08-09T17:06:16.527260Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:06:16.645014Z","title":"A dynamic subgrid- scale eddy viscosity model","venue":null,"work_id":"223e8620-aa6d-4b39-959c-cdfd09c7ba01","year":1991},"citing_paper":{"arxiv_id":"2502.00974","last_updated":"2025-02-03T00:55:40Z","snapshot_observed_at":"2026-08-13T11:34:41.622007Z","submitted_at":"2025-02-03T00:55:40Z","title":"Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-09T17:06:16.266253Z"},"links":{"citing_paper":"/paper/2502.00974"},"observation_digest":"sha256:9d6799a7f4e963cf2f47ae1474200433fda12dbd75ad8129b5a30d74236521ec","observation_id":"7e06b9d7-57ed-45e8-aeed-4a600ac7ff50","resolution":{"observed_at":"2026-08-09T17:06:16.650126Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:06:16.536495Z","title":"N., Kosovichev, A","venue":null,"work_id":"9ec13350-7e6b-498d-8255-04332863b53a","year":2019},"citing_paper":{"arxiv_id":"2502.00974","last_updated":"2025-02-03T00:55:40Z","snapshot_observed_at":"2026-08-13T11:34:41.622007Z","submitted_at":"2025-02-03T00:55:40Z","title":"Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-09T17:06:16.297783Z"},"links":{"citing_paper":"/paper/2502.00974"},"observation_digest":"sha256:960bc8a46825e72783d39e4bcd1bcb5762760149bfb4ed1e353ee9d0dce437e5","observation_id":"9ebf40b3-7f47-49cb-ae5c-aead67414871","resolution":{"observed_at":"2026-08-09T17:06:16.540798Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:06:16.689322Z","title":"P., Leenaarts, J., Rempel, M., Cheung, M","venue":null,"work_id":"c8236423-46a8-41f1-84db-0418448bbaca","year":2019},"citing_paper":{"arxiv_id":"2502.00974","last_updated":"2025-02-03T00:55:40Z","snapshot_observed_at":"2026-08-13T11:34:41.622007Z","submitted_at":"2025-02-03T00:55:40Z","title":"Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-09T17:06:16.251288Z"},"links":{"citing_paper":"/paper/2502.00974"},"observation_digest":"sha256:9663a167cd665fec1ab0c19cb60e3ee745a17bf7d7147bb31bd2dc715c261036","observation_id":"3afb9950-be03-4e44-a3f9-ad3795a1dfd1","resolution":{"observed_at":"2026-08-09T17:06:16.694104Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:06:16.493395Z","title":null,"venue":null,"work_id":"bc3495cf-7031-4b31-9d08-11f48a169964","year":2011},"citing_paper":{"arxiv_id":"2502.00974","last_updated":"2025-02-03T00:55:40Z","snapshot_observed_at":"2026-08-13T11:34:41.622007Z","submitted_at":"2025-02-03T00:55:40Z","title":"Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-09T17:06:16.312665Z"},"links":{"citing_paper":"/paper/2502.00974"},"observation_digest":"sha256:e1f9fcc8b5f6f51e2ca170e0143b27b19c26289771409fe135f43f0750edf11a","observation_id":"a86a28cf-9676-47e3-854e-287578215fdd","resolution":{"observed_at":"2026-08-09T17:06:16.497737Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:06:16.413101Z","title":null,"venue":null,"work_id":"00050ebf-cfb7-4e3c-824a-824cc56a66bf","year":2023},"citing_paper":{"arxiv_id":"2502.00974","last_updated":"2025-02-03T00:55:40Z","snapshot_observed_at":"2026-08-13T11:34:41.622007Z","submitted_at":"2025-02-03T00:55:40Z","title":"Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling","version":1},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-09T17:06:16.338014Z"},"links":{"citing_paper":"/paper/2502.00974"},"observation_digest":"sha256:4f0a1e107588e7dfae3967a57cb9f7f6271beb9502c97481685cc007a48dbe52","observation_id":"8255f779-1f7d-438e-89b7-b72251f9f49c","resolution":{"observed_at":"2026-08-09T17:06:16.418122Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:06:16.674121Z","title":null,"venue":null,"work_id":"e2993316-dbe3-416f-b62a-017894adff74","year":2024},"citing_paper":{"arxiv_id":"2502.00974","last_updated":"2025-02-03T00:55:40Z","snapshot_observed_at":"2026-08-13T11:34:41.622007Z","submitted_at":"2025-02-03T00:55:40Z","title":"Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling","version":1},"reference_index":108,"source":"pdf_text","source_observed_at":"2026-08-09T17:06:16.256427Z"},"links":{"citing_paper":"/paper/2502.00974"},"observation_digest":"sha256:ed75ddc95013946aea72241a57c29602664fb7ade761e2cea39e6de548d42a6d","observation_id":"cf4da986-eda3-4038-b49d-987cedd9d171","resolution":{"observed_at":"2026-08-09T17:06:16.678877Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:06:16.428921Z","title":"2009, Radiative M agnetohydrodynamic Simulation of Sunspot Structure","venue":null,"work_id":"68609bb8-f89c-475f-b9ab-549dc05071f6","year":2009},"citing_paper":{"arxiv_id":"2502.00974","last_updated":"2025-02-03T00:55:40Z","snapshot_observed_at":"2026-08-13T11:34:41.622007Z","submitted_at":"2025-02-03T00:55:40Z","title":"Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling","version":1},"reference_index":143,"source":"pdf_text","source_observed_at":"2026-08-09T17:06:16.333011Z"},"links":{"citing_paper":"/paper/2502.00974"},"observation_digest":"sha256:0f59fdf45dd169e3023af1fb60222107d8af979b35ceda46dbcc4d06da5963ac","observation_id":"5a25e1a0-e0ec-433c-8b3d-8e466c7ea6aa","resolution":{"observed_at":"2026-08-09T17:06:16.434700Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:06:16.660065Z","title":"2023, Eruption of a Magnetic Fl ux Rope in a Comprehensive Radiative Magnetohydrodynamic Simulation of Flare-produ ctive Active Regions","venue":null,"work_id":"0b60bcc2-1302-4763-a454-97f290dc084a","year":2023},"citing_paper":{"arxiv_id":"2502.00974","last_updated":"2025-02-03T00:55:40Z","snapshot_observed_at":"2026-08-13T11:34:41.622007Z","submitted_at":"2025-02-03T00:55:40Z","title":"Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling","version":1},"reference_index":160,"source":"pdf_text","source_observed_at":"2026-08-09T17:06:16.261637Z"},"links":{"citing_paper":"/paper/2502.00974"},"observation_digest":"sha256:896b9a53e96cd0ce2070cbf45fe68eb0eab019dad8b6603bcbfb7490613f79ba","observation_id":"1957a045-cfe8-449b-9cf7-f25d722cf7c4","resolution":{"observed_at":"2026-08-09T17:06:16.664725Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:06:16.630229Z","title":null,"venue":null,"work_id":"15aaf8d4-9be7-4306-820e-bc3ee1ca9620","year":2023},"citing_paper":{"arxiv_id":"2502.00974","last_updated":"2025-02-03T00:55:40Z","snapshot_observed_at":"2026-08-13T11:34:41.622007Z","submitted_at":"2025-02-03T00:55:40Z","title":"Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling","version":1},"reference_index":176,"source":"pdf_text","source_observed_at":"2026-08-09T17:06:16.270572Z"},"links":{"citing_paper":"/paper/2502.00974"},"observation_digest":"sha256:6c1735e2b0a5181d366d9b9a93ae30c1dcb835b5379fa6d56073e0c21548ff13","observation_id":"f323c5d3-f17e-4f74-ba52-b1ea846e0547","resolution":{"observed_at":"2026-08-09T17:06:16.635131Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:06:16.583562Z","title":"R., Chaplin, W","venue":null,"work_id":"27a67727-9d67-4e05-b76f-5d3ca6d937ed","year":2017},"citing_paper":{"arxiv_id":"2502.00974","last_updated":"2025-02-03T00:55:40Z","snapshot_observed_at":"2026-08-13T11:34:41.622007Z","submitted_at":"2025-02-03T00:55:40Z","title":"Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling","version":1},"reference_index":199,"source":"pdf_text","source_observed_at":"2026-08-09T17:06:16.284444Z"},"links":{"citing_paper":"/paper/2502.00974"},"observation_digest":"sha256:fb17078d1d317d1dd5d30a752d1702420c82b49238ccb23c781fe7a6e40de516","observation_id":"672b2ef7-9dac-442f-bc3b-8d08336c47ac","resolution":{"observed_at":"2026-08-09T17:06:16.588896Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:06:16.460573Z","title":"1991, A dynamic sub grid-scale model for compressible turbulence and scalar transport","venue":null,"work_id":"059745e2-c621-4d21-b880-fa4e02e4ec62","year":1991},"citing_paper":{"arxiv_id":"2502.00974","last_updated":"2025-02-03T00:55:40Z","snapshot_observed_at":"2026-08-13T11:34:41.622007Z","submitted_at":"2025-02-03T00:55:40Z","title":"Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling","version":1},"reference_index":217,"source":"pdf_text","source_observed_at":"2026-08-09T17:06:16.322990Z"},"links":{"citing_paper":"/paper/2502.00974"},"observation_digest":"sha256:7090338d49f270a5d18c7477656b568214b45315812c01443f0d07b741e95a90","observation_id":"f371b3d9-433d-41d9-855b-7663d1a05ea8","resolution":{"observed_at":"2026-08-09T17:06:16.465767Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:06:16.614714Z","title":null,"venue":null,"work_id":"21829a52-37bb-4169-8be0-c0de03bd2d8f","year":2021},"citing_paper":{"arxiv_id":"2502.00974","last_updated":"2025-02-03T00:55:40Z","snapshot_observed_at":"2026-08-13T11:34:41.622007Z","submitted_at":"2025-02-03T00:55:40Z","title":"Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling","version":1},"reference_index":288,"source":"pdf_text","source_observed_at":"2026-08-09T17:06:16.275418Z"},"links":{"citing_paper":"/paper/2502.00974"},"observation_digest":"sha256:c4d0e247280a07bb0bc2d9309676a298259d4e0f6f9461aa71663baae880a257","observation_id":"174a980d-eadd-4b00-ae50-5b0a3d7238c5","resolution":{"observed_at":"2026-08-09T17:06:16.619575Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2502.00974","last_updated":"2025-02-03T00:55:40Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-13T11:34:41.622007Z","submitted_at":"2025-02-03T00:55:40Z","title":"Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling"},"reference_resolution":{"displayed":22,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":8,"verified_exact":0,"verified_fuzzy":14},"total_outbound_references":22},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 14 August 2026, this Paper Citation Record lists 22 of 22 outbound references and 2 inbound Pith citation observations for arXiv:2502.00974."}