{"as_of":"2026-08-10T19:09:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:42019ab1fb1be0f32323a33932560a776df35783ab92b92f68dd4a91c51b92d4","coverage":[{"denominator":295,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T21:17:29.884502Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2507.00632/citation-record","integrity":"/paper/2507.00632/integrity","json":"/paper/2507.00632/citation-record.json","paper":"/paper/2507.00632"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:17:16.224174Z","title":"Living Rev Sol Phys 17(1):1","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:16.224174Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:4c88fd3aed239bc5df64a4b6e61b1cffd876642dd0e63c9877a817deb323b951","observation_id":"3941840f-6a91-472f-9fa6-d870682e5b22","resolution":{"observed_at":"2026-08-06T21:17:16.224174Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1410.6547","last_updated":"2015-07-10T05:03:17Z","snapshot_observed_at":"2026-08-05T15:34:00.736154Z","submitted_at":"2014-10-24T02:33:07Z","title":"Grand Minima and Equatorward Propagation in a Cycling Stellar Convective Dynamo","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1410.6547","snapshot_observed_at":"2026-08-06T21:17:16.320735Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:16.320735Z"},"links":{"cited_paper":"/paper/1410.6547","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:469d594452b6ed9a5c2a9880b10bebffe03620e6fd6d30e96da0421b13835c10","observation_id":"6b4f2fc6-eb62-4452-a818-6d57e1c244a8","resolution":{"observed_at":"2026-08-06T21:17:16.320735Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:17:16.465340Z","title":null,"venue":null,"work_id":null,"year":1991},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:16.465340Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:2973fc3694ef6bc940173990c0437db5bcd2bc5ce2d831df05f27299d33ffcf8","observation_id":"820115d0-caff-439c-8d40-075bee07e7be","resolution":{"observed_at":"2026-08-06T21:17:16.465340Z","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":"10.1063/1.873263","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Physics of Plasmas 6(1):89--99","venue":"Physics of Plasmas","work_id":"2f4b1900-f709-413a-9fdd-86759422cba4","year":1999},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:16.615236Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:cab8a837d6c46a95282cf6bc2da249bc903af0bbe4ce408aaa429e1bdec19590","observation_id":"abbdc2c9-c5ae-4874-bb1b-615d266b16ff","resolution":{"observed_at":"2026-08-06T21:17:58.601909Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2012.06343","last_updated":"2020-12-10T14:45:33Z","snapshot_observed_at":"2026-08-10T02:00:27.320972Z","submitted_at":"2020-12-10T14:45:33Z","title":"Generation of mean flows in rotating anisotropic turbulence: The case of solar near-surface shear layer","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.06343","snapshot_observed_at":"2026-08-06T21:17:16.777929Z","title":"a pyl \\\"a MJ, K \\","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:16.777929Z"},"links":{"cited_paper":"/paper/2012.06343","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:a935d2a71ad3254dc5ccfe00548eb1eba282c03146aa1a17ea50f77c2d0e55d9","observation_id":"dceae0d2-dd9b-4f60-9621-f418a193ab12","resolution":{"observed_at":"2026-08-06T21:17:16.777929Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:17:16.930760Z","title":"AN 308:89--100","venue":null,"work_id":null,"year":1987},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:16.930760Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:14d65bfb19d3c7aeb0fc386b2889de08eb8d29c7923f6b3ec6abdd6b793404a9","observation_id":"bc169d06-1f7d-4ef5-91d9-d7a01891938a","resolution":{"observed_at":"2026-08-06T21:17:16.930760Z","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":"10.3847/0004-637x/826/2/138","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"826(2):138","venue":"The Astrophysical Journal","work_id":"e6273d51-b3f8-4b58-954f-d4634daf0476","year":2016},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:17.014681Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:8582abc497691d327bcf0b35b12f4a41484cc60b2305de66c618cfc502fa185c","observation_id":"a766b273-1a39-4507-9292-42125b2e68f3","resolution":{"observed_at":"2026-08-06T21:17:58.414285Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1510.04178","last_updated":"2015-10-14T15:59:38Z","snapshot_observed_at":"2026-07-06T04:33:06.251304Z","submitted_at":"2015-10-14T15:59:38Z","title":"Dynamo saturation in direct simulations of the multi-phase turbulent interstellar medium","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.04178","snapshot_observed_at":"2026-08-06T21:17:17.191899Z","title":"Astron Nachr 336(10):991","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:17.191899Z"},"links":{"cited_paper":"/paper/1510.04178","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:2cdb047e7f782bb3d7c16bf6ff53b77055ccb915b2795718df26790b60d2fb3a","observation_id":"9b5ff6cf-060a-424e-9321-f87d6c05cf1f","resolution":{"observed_at":"2026-08-06T21:17:17.191899Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:17:17.354749Z","title":"Living Rev Sol Phys 2:8","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:17.354749Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:cc309c9c417b5441a82676969f5718fb53be5ac6ceacd4dde20fb9ef7f1f3f97","observation_id":"a9a63226-cdfd-42ca-8731-399777005d35","resolution":{"observed_at":"2026-08-06T21:17:17.354749Z","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":"10.1086/176094","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":null,"venue":"The Astrophysical Journal","work_id":"41c888b9-4e1e-4091-9c0c-c10e6ca7c725","year":1995},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:17.477528Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:76746bb231bd639dfe37ffc8aab2ec40eae1e8e07109604fe72e2f7ebbae81d4","observation_id":"a61c8273-1b84-4278-a4e0-8dc773a6dbba","resolution":{"observed_at":"2026-08-06T21:17:58.165171Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/acac78","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"947(1):36","venue":"The Astrophysical Journal","work_id":"37d4f718-4e1c-4335-9c5a-3c2d27ff4e77","year":2023},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:17.645609Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:5fe9ba98fa778880f5e1763d4ebe3fb60ad15dafdc0ac0c1ea52edc7a63b5106","observation_id":"e7f9dda8-c92f-4db9-a84c-161c1b77d0d4","resolution":{"observed_at":"2026-08-06T21:17:57.911507Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:17:17.794870Z","title":"U ber den Ursprung der Magnetfelder auf Sternen und im interstellaren Raum (miteinem Anhang von A. Schl \\","venue":null,"work_id":null,"year":1950},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:17.794870Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:16aa34f8dc0ca17e646e97e3bac4014b7593b3e3eaa7f76bf4fd47ce0bc00a3a","observation_id":"45db14b0-8db2-487f-addb-0a2050aa495a","resolution":{"observed_at":"2026-08-06T21:17:17.794870Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1607.05250","last_updated":"2016-07-18T19:33:51Z","snapshot_observed_at":"2026-07-06T05:04:00.852031Z","submitted_at":"2016-07-18T19:33:51Z","title":"A low upper limit on the subsurface rise speed of solar active regions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1607.05250","snapshot_observed_at":"2026-08-06T21:17:17.925077Z","title":"Science Advances 2:e1600557--e1600557","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:17.925077Z"},"links":{"cited_paper":"/paper/1607.05250","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:763991010c7ec211b6dd2ad961ffa609e16e7ced1cf417b018e0d023a95a80e4","observation_id":"3fe587d5-76d7-451f-9227-9e0923615b27","resolution":{"observed_at":"2026-08-06T21:17:17.925077Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:17:18.018570Z","title":"Physics of Fluids 36(11):117136","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:18.018570Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:90372523034480b92cc6ce2ffda7a9b28d83592eb84d29d3ffcaaae0a5b42e4a","observation_id":"1b96437f-524d-43d1-9759-cdc1ee76891b","resolution":{"observed_at":"2026-08-06T21:17:18.018570Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9903384","last_updated":"1999-12-24T08:37:07Z","snapshot_observed_at":"2026-07-07T01:25:17.432011Z","submitted_at":"1999-03-25T22:48:54Z","title":"Constraints on the magnitude of alpha in dynamo theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9903384","snapshot_observed_at":"2026-08-06T21:17:18.114729Z","title":"534(2):984--988","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:18.114729Z"},"links":{"cited_paper":"/paper/astro-ph/9903384","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:8b92eeae2c55802427d9cd246750f7e0a49aeff2393f18f66f5b92176cb1700c","observation_id":"4479d27f-ff2f-4bd8-96da-57f461bbaf6a","resolution":{"observed_at":"2026-08-06T21:17:18.114729Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0207435","last_updated":"2002-10-23T03:59:05Z","snapshot_observed_at":"2026-08-08T11:42:18.945236Z","submitted_at":"2002-07-22T17:50:27Z","title":"A New Dynamical Mean-Field Dynamo Theory and Closure Approach","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0207435","snapshot_observed_at":"2026-08-06T21:17:18.214750Z","title":"Physical Review Letters 89(26):265007","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:18.214750Z"},"links":{"cited_paper":"/paper/astro-ph/0207435","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:dcb10d42fad6fedf9e2b2cd877439c04240d963cd865b3e4e334fba1974e87da","observation_id":"54bd0fff-2ca1-47a1-9cbf-99435e74221b","resolution":{"observed_at":"2026-08-06T21:17:18.214750Z","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":"10.1080/03091929508228992","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Geophys Astrophys Fluid Dyn 79(1):1--97","venue":"Geophysical & Astrophysical Fluid Dynamics","work_id":"1373affa-6b33-4435-9b41-c310ff6e5db0","year":1995},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:18.296772Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:20a24ac03821618f0e6a00f9cb813d125ed59eaf3f880e0a989e094b381c307e","observation_id":"6f81c9fd-9417-4d0d-a15b-cfc876c7c225","resolution":{"observed_at":"2026-08-06T21:17:57.749861Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0006186","last_updated":"2000-12-07T20:15:18Z","snapshot_observed_at":"2026-07-07T00:11:41.387151Z","submitted_at":"2000-06-13T21:56:05Z","title":"The inverse cascade and nonlinear alpha-effect in simulations of isotropic helical hydromagnetic turbulence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0006186","snapshot_observed_at":"2026-08-06T21:17:18.425883Z","title":"550:824--840","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:18.425883Z"},"links":{"cited_paper":"/paper/astro-ph/0006186","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:85d7c2b3ef0e048dc11e9ce35e505801c6d7ff7adf9c0f0a97b02a4d8c14360a","observation_id":"cac6c178-919a-424b-813e-e9f728dc580e","resolution":{"observed_at":"2026-08-06T21:17:18.425883Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0502275","last_updated":"2005-02-15T20:34:13Z","snapshot_observed_at":"2026-07-07T00:48:07.933367Z","submitted_at":"2005-02-15T20:34:13Z","title":"The case for a distributed solar dynamo shaped by near-surface shear","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0502275","snapshot_observed_at":"2026-08-06T21:17:18.587962Z","title":"625:539--547","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:18.587962Z"},"links":{"cited_paper":"/paper/astro-ph/0502275","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:8f2a713ee668c95eecedfbede7963902a859ce450091ce47037908af8fbb8c6d","observation_id":"1a9e99ca-9bd1-4ca7-9022-0779c16561a8","resolution":{"observed_at":"2026-08-06T21:17:18.587962Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0510015","last_updated":"2005-10-01T08:43:23Z","snapshot_observed_at":"2026-07-07T00:54:32.887284Z","submitted_at":"2005-10-01T08:43:23Z","title":"Turbulence and its parameterization in accretion discs","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0510015","snapshot_observed_at":"2026-08-06T21:17:18.724235Z","title":"Astron Nachr 326(9):787--797","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:18.724235Z"},"links":{"cited_paper":"/paper/astro-ph/0510015","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:7b883e8ae2f0065739dc54aa5720aca5d02c5af47ff91b339c12efc71152e231","observation_id":"395eec45-36d3-45a5-a075-f66f7f1a45f5","resolution":{"observed_at":"2026-08-06T21:17:18.724235Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0808.0959","last_updated":"2008-08-07T06:42:56Z","snapshot_observed_at":"2026-07-06T01:41:37.318075Z","submitted_at":"2008-08-07T06:42:56Z","title":"The dual role of shear in large-scale dynamos","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0808.0959","snapshot_observed_at":"2026-08-06T21:17:18.844376Z","title":"Astron Nachr 329(7):725","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:18.844376Z"},"links":{"cited_paper":"/paper/0808.0959","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:d049deb89b46bac9f1ed1cbb2dfc6d93e6d22987e40a09bbad6ba88da053197c","observation_id":"322ca159-9818-49f4-9d8e-923e219f48af","resolution":{"observed_at":"2026-08-06T21:17:18.844376Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.03189","last_updated":"2016-10-24T04:29:26Z","snapshot_observed_at":"2026-07-06T04:14:49.530046Z","submitted_at":"2015-04-13T14:05:40Z","title":"Stellar mixing length theory with entropy rain","version":7},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.03189","snapshot_observed_at":"2026-08-06T21:17:18.974815Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:18.974815Z"},"links":{"cited_paper":"/paper/1504.03189","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:3f6daeba9d5ffb426c290a5827423901e18d989ba66bf0e1716bf955e663ac1f","observation_id":"41238b9d-cbc3-412f-8503-1972a2a37052","resolution":{"observed_at":"2026-08-06T21:17:18.974815Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.02671","last_updated":"2017-02-10T14:16:06Z","snapshot_observed_at":"2026-08-10T06:21:39.982228Z","submitted_at":"2016-11-08T19:50:08Z","title":"Analytic solution of an oscillatory migratory alpha^2 stellar dynamo","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.02671","snapshot_observed_at":"2026-08-06T21:17:19.075781Z","title":"598:A117","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:19.075781Z"},"links":{"cited_paper":"/paper/1611.02671","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:ecb5b4bde60e96b99eee40826475ceae6e05bd0a81fa76758887608d226731cd","observation_id":"823b8bd8-9294-4afd-b29e-74a393bb1944","resolution":{"observed_at":"2026-08-06T21:17:19.075781Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.05384","last_updated":"2018-07-09T13:03:31Z","snapshot_observed_at":"2026-07-06T06:18:56.456590Z","submitted_at":"2018-01-16T17:40:34Z","title":"Advances in mean-field dynamo theory and applications to astrophysical turbulence","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.05384","snapshot_observed_at":"2026-08-06T21:17:19.187420Z","title":"Journal of Plasma Physics 84(4):735840404","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:19.187420Z"},"links":{"cited_paper":"/paper/1801.05384","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:d3b08cf0273c3c81416e762f10e15619ebc6327a4f9e576ee7c91c1555a12af2","observation_id":"741287f8-c045-49a7-9fb0-ce9502ef6839","resolution":{"observed_at":"2026-08-06T21:17:19.187420Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:17:19.364743Z","title":"Astron Nachr 339(631):631--640","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:19.364743Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:f0913adafd353c67d2ab0d23c401255c27b48f2161f8063124e488d76d802e52","observation_id":"8a947a8c-8549-4e88-973a-5fd339012a0c","resolution":{"observed_at":"2026-08-06T21:17:19.364743Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.04231","last_updated":"2018-02-12T18:24:15Z","snapshot_observed_at":"2026-08-07T06:20:10.300815Z","submitted_at":"2018-02-12T18:24:15Z","title":"Strong nonlocality variations in a spherical mean-field dynamo","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.04231","snapshot_observed_at":"2026-08-06T21:17:19.450148Z","title":"Astron Nachr 339:118--126","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:19.450148Z"},"links":{"cited_paper":"/paper/1802.04231","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:6204274db5e1c1daabd2e026ca3805ed748c57219609f07869852556f8d9bf0f","observation_id":"15ae14d7-ae83-4f24-8f4b-09844ba6b38d","resolution":{"observed_at":"2026-08-06T21:17:19.450148Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0012472","last_updated":"2001-01-29T17:01:09Z","snapshot_observed_at":"2026-08-10T15:11:20.749979Z","submitted_at":"2000-12-22T02:02:25Z","title":"Large scale dynamos with helicity loss through boundaries","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0012472","snapshot_observed_at":"2026-08-06T21:17:19.564750Z","title":"369:329--338","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:19.564750Z"},"links":{"cited_paper":"/paper/astro-ph/0012472","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:dcd6093be87f8256c4f08b121b18d5fe2c1e7744ec53b6b24f74975d002b07d1","observation_id":"e8315e42-9130-4e5e-bf65-0382d3f0ce88","resolution":{"observed_at":"2026-08-06T21:17:19.564750Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0207393","last_updated":"2002-07-18T17:16:07Z","snapshot_observed_at":"2026-07-07T00:27:32.385154Z","submitted_at":"2002-07-18T17:16:07Z","title":"Solar and stellar dynamos -- latest developments","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0207393","snapshot_observed_at":"2026-08-06T21:17:19.734767Z","title":"Astron Nachr 323:411--416","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:19.734767Z"},"links":{"cited_paper":"/paper/astro-ph/0207393","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:2c0c7d1d4b6088cac45fe206b552a18fb6f83474096b4c349917d148ec31f401","observation_id":"d100fc3a-8fa6-4dd5-9115-ab2bb0b040c1","resolution":{"observed_at":"2026-08-06T21:17:19.734767Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0705.3507","last_updated":"2007-05-24T05:42:44Z","snapshot_observed_at":"2026-07-06T01:28:00.530675Z","submitted_at":"2007-05-24T05:42:44Z","title":"Magnetic helicity effects in astrophysical and laboratory dynamos","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0705.3507","snapshot_observed_at":"2026-08-06T21:17:19.884129Z","title":"New Journal of Physics 9(8):305","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:19.884129Z"},"links":{"cited_paper":"/paper/0705.3507","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:ee31ad44a88805d1d022a18337ed2fb84cfaf6bd0edb268fde326bc5bf5d92b6","observation_id":"32d68214-e684-43da-a3b3-e61969a1db56","resolution":{"observed_at":"2026-08-06T21:17:19.884129Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0111568","last_updated":"2002-08-07T06:39:48Z","snapshot_observed_at":"2026-07-07T00:23:30.022556Z","submitted_at":"2001-11-29T20:56:14Z","title":"Local and nonlocal magnetic diffusion and alpha-effect tensors in shear flow turbulence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0111568","snapshot_observed_at":"2026-08-06T21:17:20.205248Z","title":"Geophys Astrophys Fluid Dynam 96:319--344","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:20.205248Z"},"links":{"cited_paper":"/paper/astro-ph/0111568","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:5c8c1459f80b7460179563abf77e0dbd171222b19151750473384c9645647ee9","observation_id":"cacd17d0-ea43-4c07-8602-c73f795f0e83","resolution":{"observed_at":"2026-08-06T21:17:20.205248Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0405052","last_updated":"2005-06-16T13:43:57Z","snapshot_observed_at":"2026-07-07T00:42:14.601568Z","submitted_at":"2004-05-04T13:13:45Z","title":"Astrophysical magnetic fields and nonlinear dynamo theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0405052","snapshot_observed_at":"2026-08-06T21:17:20.290775Z","title":"417:1--209","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:20.290775Z"},"links":{"cited_paper":"/paper/astro-ph/0405052","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:a0d307e3150e82116f10c1f9175899d44526e034243d7cae5fc19944a74c0359","observation_id":"fd289a98-8043-4754-a06d-fe04aadca272","resolution":{"observed_at":"2026-08-06T21:17:20.290775Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0504222","last_updated":"2005-08-18T16:40:53Z","snapshot_observed_at":"2026-08-10T18:10:00.837267Z","submitted_at":"2005-04-10T01:38:44Z","title":"Minimal tau approximation and simulations of the alpha effect","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0504222","snapshot_observed_at":"2026-08-06T21:17:20.387199Z","title":"439:835--843","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:20.387199Z"},"links":{"cited_paper":"/paper/astro-ph/0504222","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:116d587f675143155db352beb5206d7797832a1311e0c0519c314bd8a0927e4c","observation_id":"ee87ce02-bcbe-4cf7-80a8-7fd2c4e95032","resolution":{"observed_at":"2026-08-06T21:17:20.387199Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0505457","last_updated":"2005-06-24T18:25:53Z","snapshot_observed_at":"2026-07-07T00:50:48.284065Z","submitted_at":"2005-05-23T19:41:59Z","title":"Strong mean field dynamos require supercritical helicity fluxes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0505457","snapshot_observed_at":"2026-08-06T21:17:20.534298Z","title":"Astron Nachr 326(6):400--408","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:20.534298Z"},"links":{"cited_paper":"/paper/astro-ph/0505457","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:e1d286cc16bc2df33c902292e1ec1df173f2e376f840c34d9d4381e137c351a4","observation_id":"e768a9aa-16c6-40fb-9ec8-7caaabb65780","resolution":{"observed_at":"2026-08-06T21:17:20.534298Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:17:20.674823Z","title":"In: Finnish Astronomical Society","venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:20.674823Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:322b4fa7ebf477f8cab6f55dd0c1a2eaf4fbf3689ff9c6ad81d47c9bc44263f0","observation_id":"a3bc8752-38d0-4e20-8980-cea220263e08","resolution":{"observed_at":"2026-08-06T21:17:20.674823Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:17:20.864146Z","title":"232:277--291","venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:20.864146Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:8e9441f0139584a3d08540939021d5d1ff897821d7405cd763a20f30cf0e33e2","observation_id":"d3789bdd-e68a-4d52-9e16-93eb9a316682","resolution":{"observed_at":"2026-08-06T21:17:20.864146Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:17:21.070728Z","title":"265:328--344","venue":null,"work_id":null,"year":1992},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:21.070728Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:7b804212e06a8f2388a1057b275d1166b7d862b087833af83c152b35659dca43","observation_id":"c8dc70c1-25a8-4a68-bbce-2d1b41905959","resolution":{"observed_at":"2026-08-06T21:17:21.070728Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:17:21.266194Z","title":null,"venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:21.266194Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:f887ca7330bbbcae1d5b6a065b06c04802c26c71b19c8f6dda9c75a565c9e624","observation_id":"81f88b00-2a07-4bc9-9031-136805f02684","resolution":{"observed_at":"2026-08-06T21:17:21.266194Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:17:21.504793Z","title":"J Fluid Mech 306:325--352","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:21.504793Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:6a2adcca03ee6fbf945d195efdf21655f6a4963e9994d644f2ddc0a1c98312e9","observation_id":"538df616-dbbe-4916-945e-28c7e0ba1512","resolution":{"observed_at":"2026-08-06T21:17:21.504793Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0111567","last_updated":"2002-04-30T17:59:38Z","snapshot_observed_at":"2026-07-07T00:23:30.022556Z","submitted_at":"2001-11-29T20:14:25Z","title":"Magnetic helicity in stellar dynamos: new numerical experiments","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0111567","snapshot_observed_at":"2026-08-06T21:17:21.616701Z","title":"Astron Nachr 323(2):99--122","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:21.616701Z"},"links":{"cited_paper":"/paper/astro-ph/0111567","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:2c333f25d3bf6629ce7e78e37d803a3272d466e0732fa1854848311beb41233b","observation_id":"23c4df83-0e4d-4e98-8fc7-daa997ffebbd","resolution":{"observed_at":"2026-08-06T21:17:21.616701Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0710.4059","last_updated":"2008-02-28T20:05:25Z","snapshot_observed_at":"2026-07-06T01:30:42.699461Z","submitted_at":"2007-10-22T19:55:28Z","title":"Magnetic diffusivity tensor and dynamo effects in rotating and shearing turbulence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0710.4059","snapshot_observed_at":"2026-08-06T21:17:21.713607Z","title":"a dler KH, Rheinhardt M, K \\","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:21.713607Z"},"links":{"cited_paper":"/paper/0710.4059","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:59f6dabda5168df68c5c32668169090a010b48bcf1261985b12a4557b7c49aee","observation_id":"0be8d3b7-0f45-471d-87b6-bc5fdb6b089f","resolution":{"observed_at":"2026-08-06T21:17:21.713607Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0805.1287","last_updated":"2008-10-14T05:41:08Z","snapshot_observed_at":"2026-07-06T01:37:54.420489Z","submitted_at":"2008-05-09T07:04:04Z","title":"Nonlinear magnetic diffusivity and alpha tensors in helical turbulence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0805.1287","snapshot_observed_at":"2026-08-06T21:17:21.846200Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:21.846200Z"},"links":{"cited_paper":"/paper/0805.1287","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:400cb2f5236f8f3bb6b92924dc593db750fed9b30a69a608228411535a4621fc","observation_id":"9327382b-eab2-436c-a0ee-fac996c9db88","resolution":{"observed_at":"2026-08-06T21:17:21.846200Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0801.1320","last_updated":"2008-01-08T21:55:53Z","snapshot_observed_at":"2026-07-06T01:34:39.909325Z","submitted_at":"2008-01-08T21:55:53Z","title":"Scale dependence of alpha effect and turbulent diffusivity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0801.1320","snapshot_observed_at":"2026-08-06T21:17:21.944847Z","title":"482:739--746","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:21.944847Z"},"links":{"cited_paper":"/paper/0801.1320","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:e1de43a5086d5bbb3866a97f7681aaac26e96b6ffaa557fb1023db3ada6a793a","observation_id":"952ba85e-1383-4b25-89bf-de770448ee76","resolution":{"observed_at":"2026-08-06T21:17:21.944847Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0910.1835","last_updated":"2009-10-12T19:53:16Z","snapshot_observed_at":"2026-08-02T10:33:07.210819Z","submitted_at":"2009-10-12T19:53:16Z","title":"Large-scale magnetic flux concentrations from turbulent stresses","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0910.1835","snapshot_observed_at":"2026-08-06T21:17:22.214748Z","title":"AN 331:5","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:22.214748Z"},"links":{"cited_paper":"/paper/0910.1835","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:2a271e0234cfc86bd00fa1a1753c7f6a828e3836fda7bc3c74a951c6029a257c","observation_id":"6e8050ad-b4f7-47a5-9062-98b97cd4c74c","resolution":{"observed_at":"2026-08-06T21:17:22.214748Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1109.1270","last_updated":"2011-10-04T08:02:18Z","snapshot_observed_at":"2026-07-06T02:33:34.446024Z","submitted_at":"2011-09-06T19:04:26Z","title":"Detection of negative effective magnetic pressure instability in turbulence simulations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1109.1270","snapshot_observed_at":"2026-08-06T21:17:22.374751Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:22.374751Z"},"links":{"cited_paper":"/paper/1109.1270","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:5d96e73276d2079755a68d0d6f11c70997b7c93bd25bc2c20d2c2410384ce7ae","observation_id":"44b5d970-e732-4ca6-9953-761553a45105","resolution":{"observed_at":"2026-08-06T21:17:22.374751Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1005.5700","last_updated":"2012-02-21T05:09:29Z","snapshot_observed_at":"2026-07-06T02:11:05.693136Z","submitted_at":"2010-05-31T15:50:10Z","title":"The negative effective magnetic pressure in stratified forced turbulence","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1005.5700","snapshot_observed_at":"2026-08-06T21:17:22.524823Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:22.524823Z"},"links":{"cited_paper":"/paper/1005.5700","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:75bf12d5ee472f7bde94cf27d995a2d1ff0f55c394cf77613eb6d7d318ef4bae","observation_id":"eed3978c-ee39-4267-8b5d-a5cfcef6ecc5","resolution":{"observed_at":"2026-08-06T21:17:22.524823Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1108.2264","last_updated":"2012-02-22T09:34:40Z","snapshot_observed_at":"2026-07-06T02:32:15.141728Z","submitted_at":"2011-08-10T19:54:04Z","title":"Mean-field transport in stratified and/or rotating turbulence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1108.2264","snapshot_observed_at":"2026-08-06T21:17:22.707756Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:22.707756Z"},"links":{"cited_paper":"/paper/1108.2264","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:d984b601fed5e5d8cd7d326874954bd7937569e43f3ed9cff1ce2456445f4e53","observation_id":"fcc01718-7383-427b-a275-2e0ba2a5c0bb","resolution":{"observed_at":"2026-08-06T21:17:22.707756Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1208.5004","last_updated":"2012-11-20T11:19:56Z","snapshot_observed_at":"2026-07-06T02:54:19.910336Z","submitted_at":"2012-08-24T16:34:06Z","title":"New scaling for the alpha effect in slowly rotating turbulence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1208.5004","snapshot_observed_at":"2026-08-06T21:17:22.830097Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:22.830097Z"},"links":{"cited_paper":"/paper/1208.5004","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:e90c8b81c59e30bf5ad01cdae3e6cb2de18988753cfa4597301dc75c408c6c15","observation_id":"3e6a25fa-7301-44e3-a9b7-0ede526b397f","resolution":{"observed_at":"2026-08-06T21:17:22.830097Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1306.4915","last_updated":"2013-10-01T15:02:59Z","snapshot_observed_at":"2026-07-06T03:16:25.257171Z","submitted_at":"2013-06-20T15:40:36Z","title":"Self-assembly of shallow magnetic spots through strongly stratified turbulence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1306.4915","snapshot_observed_at":"2026-08-06T21:17:22.968416Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:22.968416Z"},"links":{"cited_paper":"/paper/1306.4915","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:6d796c15d72224dd0bd658f3fb7d1248efd1d8456e5849bb64f5e1f017aad205","observation_id":"ebc60b41-c7ea-451e-bde7-a75cf9f624b8","resolution":{"observed_at":"2026-08-06T21:17:22.968416Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1704.09009","last_updated":"2017-08-17T16:57:27Z","snapshot_observed_at":"2026-07-06T05:39:49.934262Z","submitted_at":"2017-04-28T17:05:16Z","title":"Evolution of coexisting long and short period stellar activity cycles","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1704.09009","snapshot_observed_at":"2026-08-06T21:17:23.074854Z","title":"845(1):79","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:23.074854Z"},"links":{"cited_paper":"/paper/1704.09009","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:fa13bd89e8c530ecc47fe57dd3aea05e8db493f6429b6d6d05c137b7a1074c7a","observation_id":"3cf0d979-327e-4060-9ce1-0a9b766da319","resolution":{"observed_at":"2026-08-06T21:17:23.074854Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.03421","last_updated":"2017-08-24T16:04:05Z","snapshot_observed_at":"2026-08-07T19:16:25.001211Z","submitted_at":"2017-06-11T23:13:49Z","title":"The contribution of kinetic helicity to turbulent magnetic diffusivity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.03421","snapshot_observed_at":"2026-08-06T21:17:23.188850Z","title":"Astron Nachr 338(7):790--793","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:23.188850Z"},"links":{"cited_paper":"/paper/1706.03421","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:0d6f400e065533f1248a7a56b62a2e00ec19ede26e06f88b40de5375f36e65f7","observation_id":"ed465e63-50be-4e9d-b078-4e4877786ad2","resolution":{"observed_at":"2026-08-06T21:17:23.188850Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.12425","last_updated":"2023-11-22T04:03:19Z","snapshot_observed_at":"2026-07-06T15:06:34.661668Z","submitted_at":"2023-03-22T09:54:49Z","title":"Turbulent processes and mean-field dynamo","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.12425","snapshot_observed_at":"2026-08-06T21:17:23.356120Z","title":"219(7):55","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:23.356120Z"},"links":{"cited_paper":"/paper/2303.12425","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:ce8c5201cea65a88256d353e21ad5e2b2075479d69a10bb844f04a5effe8ab73","observation_id":"02d2a0bb-05df-448c-941d-ba1a7985607f","resolution":{"observed_at":"2026-08-06T21:17:23.356120Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.08879","last_updated":"2025-05-01T12:54:16Z","snapshot_observed_at":"2026-08-10T05:38:53.962166Z","submitted_at":"2025-01-15T15:50:52Z","title":"Helicity effect on turbulent passive and active scalar diffusivities","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.08879","snapshot_observed_at":"2026-08-06T21:17:23.476647Z","title":"984(1):88","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:23.476647Z"},"links":{"cited_paper":"/paper/2501.08879","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:edade69ae68fec517bb90293cd16a17b07bf39a0a73f0e85f6052a38b19147ce","observation_id":"36af88e0-5ff6-483c-9d9f-a6283b364a3c","resolution":{"observed_at":"2026-08-06T21:17:23.476647Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1102.1993","last_updated":"2011-02-09T22:05:30Z","snapshot_observed_at":"2026-07-06T02:23:18.045396Z","submitted_at":"2011-02-09T22:05:30Z","title":"Magnetic Cycles in a Convective Dynamo Simulation of a Young Solar-type Star","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1102.1993","snapshot_observed_at":"2026-08-06T21:17:23.684884Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:23.684884Z"},"links":{"cited_paper":"/paper/1102.1993","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:20ef0b6433d39e0de6fcdca33e9cebb2fbb1773afff870368a9c9423da001165","observation_id":"6b07ba4a-539a-4704-8d74-da9ce9b8e350","resolution":{"observed_at":"2026-08-06T21:17:23.684884Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:17:23.827069Z","title":"Liv Rev Sol Phys 14:4","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:23.827069Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:b92b91a29e4ac3e3c492741e434d25b5a37f5f01f3453168c836b4d3ee6ed8b1","observation_id":"899d9f94-4b41-4ad7-a66e-5d05e4b14def","resolution":{"observed_at":"2026-08-06T21:17:23.827069Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0206196","last_updated":"2002-06-12T19:42:44Z","snapshot_observed_at":"2026-07-07T00:26:54.739118Z","submitted_at":"2002-06-12T19:42:44Z","title":"Turbulent Convection Under the Influence of Rotation: Sustaining a Strong Differential Rotation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0206196","snapshot_observed_at":"2026-08-06T21:17:23.939606Z","title":"570:865--885","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:23.939606Z"},"links":{"cited_paper":"/paper/astro-ph/0206196","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:92a9b8f83f0e67423c544f483e1923823c467f350b02ec8b5d82a21749d3a8a2","observation_id":"411b5dbf-bde8-4c7e-93e6-8e91ed28257e","resolution":{"observed_at":"2026-08-06T21:17:23.939606Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0610073","last_updated":"2006-10-03T13:18:07Z","snapshot_observed_at":"2026-07-07T01:03:24.785292Z","submitted_at":"2006-10-03T13:18:07Z","title":"Global-Scale Turbulent Convection and Magnetic Dynamo Action in the Solar Envelope","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0610073","snapshot_observed_at":"2026-08-06T21:17:24.136496Z","title":"614:1073--1098","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:24.136496Z"},"links":{"cited_paper":"/paper/astro-ph/0610073","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:52ddd5ca8f5c7e0517c5ed1a9e8008f285c64a9f1f97e86e1452d6a7e0aea8b7","observation_id":"b7b118e8-2f39-4aea-995c-c76dc5f3944d","resolution":{"observed_at":"2026-08-06T21:17:24.136496Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.06598","last_updated":"2017-02-21T21:59:45Z","snapshot_observed_at":"2026-07-06T05:30:52.469538Z","submitted_at":"2017-02-21T21:59:45Z","title":"On differential rotation and overshooting in solar-like stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.06598","snapshot_observed_at":"2026-08-06T21:17:24.271789Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:24.271789Z"},"links":{"cited_paper":"/paper/1702.06598","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:12bc152d0b71b7d5fe9a7def30e7acbaaba0466789340ac20daf710b1a8c0bc7","observation_id":"abae97cf-81cd-452b-a6e7-0f2f58213719","resolution":{"observed_at":"2026-08-06T21:17:24.271789Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:17:24.439029Z","title":"926(1):21","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:24.439029Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:2db963887fc6ae1aa021528ac67b1dc97be047d099a9edd477c44c7cb5fb5631","observation_id":"864e7633-7323-4e1e-adb1-b2c2b14b8291","resolution":{"observed_at":"2026-08-06T21:17:24.439029Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.03174","last_updated":"2018-01-15T11:23:05Z","snapshot_observed_at":"2026-07-06T06:03:20.830767Z","submitted_at":"2017-10-09T16:20:09Z","title":"Large-scale dynamos in rapidly rotating plane layer convection","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.03174","snapshot_observed_at":"2026-08-06T21:17:24.628671Z","title":"a pyl \\\"a PJ, Masada Y, Brandenburg A, Favier B, Guervilly C, K \\","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:24.628671Z"},"links":{"cited_paper":"/paper/1710.03174","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:32ed5cfc5fd12a32331290bdcac962b36bc4cc6a3e49538ccb421103fbc1bc17","observation_id":"d5d63cd7-17ad-477b-8102-b58f780fb563","resolution":{"observed_at":"2026-08-06T21:17:24.628671Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0904.4293","last_updated":"2009-04-28T01:55:13Z","snapshot_observed_at":"2026-07-06T01:52:40.343271Z","submitted_at":"2009-04-28T01:55:13Z","title":"Parameter dependences of convection driven dynamos in rotating spherical fluid shells","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0904.4293","snapshot_observed_at":"2026-08-06T21:17:24.768940Z","title":"Geophys Astrophys Fluid Dynam 100:341--361","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:24.768940Z"},"links":{"cited_paper":"/paper/0904.4293","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:0ce81e84f8616ce614863cce74c6e5012c0369cce2c7ff46e957906aaeab89c8","observation_id":"7b959d3e-0e39-4ec1-8eb3-6097c6eeae64","resolution":{"observed_at":"2026-08-06T21:17:24.768940Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1208.4529","last_updated":"2013-11-15T17:54:55Z","snapshot_observed_at":"2026-07-06T02:54:11.039540Z","submitted_at":"2012-08-22T15:27:12Z","title":"The kinetic helicity needed to drive large-scale dynamos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1208.4529","snapshot_observed_at":"2026-08-06T21:17:24.879308Z","title":"87(4):043104","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:24.879308Z"},"links":{"cited_paper":"/paper/1208.4529","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:c050ed2cc5ca5275525a812870dda68c094ff975e4d8dc37aced8d916e6a8b77","observation_id":"9534aeba-800e-4344-bc8a-a23f17c89661","resolution":{"observed_at":"2026-08-06T21:17:24.879308Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:17:24.954748Z","title":"515:L39--L42","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:24.954748Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:c5b568be846bebcdbf56c8864fe9d21a84b19ca2185129c7e503a96e9529d008","observation_id":"ec224223-50b6-4ed6-8334-00c48acd09be","resolution":{"observed_at":"2026-08-06T21:17:24.954748Z","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":"10.1103/physreve.54.r4532","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":null,"venue":"Physical review. E, Statistical physics, plasmas, fluids, and related interdisciplinary topics","work_id":"5652f77b-2686-451c-af3a-0c459d793f76","year":1996},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:25.114749Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:2d80bf58541323d6359b03ec5ece6aa72b89ad48881c1871236f534977eb3bf6","observation_id":"c322dbf3-9d47-4430-87d1-72d53a04dc03","resolution":{"observed_at":"2026-08-06T21:17:57.537440Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1017/s0022112006009165","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"J Fluid Mech 553:401--418","venue":"Journal of Fluid Mechanics","work_id":"bbff8440-e330-4052-b9a0-6bbf1dfbdab3","year":2006},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:25.257457Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:dd938a45af989b407f8a9d260ec4579f7b4450790179441c981dd75777099ca7","observation_id":"b14d48ff-4349-4cb0-afea-b572b40cf7e7","resolution":{"observed_at":"2026-08-06T21:17:57.379820Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1405.3071","last_updated":"2014-05-13T08:58:49Z","snapshot_observed_at":"2026-08-01T16:19:24.840365Z","submitted_at":"2014-05-13T08:58:49Z","title":"On Large-Scale Dynamo Action at High Magnetic Reynolds Number","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.3071","snapshot_observed_at":"2026-08-06T21:17:25.334749Z","title":"789(1):70","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:25.334749Z"},"links":{"cited_paper":"/paper/1405.3071","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:198a63ea976b1f931f48bdaf27a0ebb10b874d4dc57f559555809e41b6625bda","observation_id":"30c0ecd7-03d9-4b02-afb0-2dada7b4769f","resolution":{"observed_at":"2026-08-06T21:17:25.334749Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:17:25.485222Z","title":"376:L21--L24","venue":null,"work_id":null,"year":1991},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:25.485222Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:a9b00f2b43c9d4eb94081060d981a99ab4cf53011b2d7a4945cd747bd30a0971","observation_id":"43ba96ef-d824-4da5-8ecc-7ee0ba68a680","resolution":{"observed_at":"2026-08-06T21:17:25.485222Z","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":"10.1002/asna.200710837","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Astron Nachr 328:1059","venue":"Astronomische Nachrichten","work_id":"b7ad0003-0f13-463a-b1c2-4ecafd4b48e2","year":2007},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:25.624755Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:f0b51f9972dd60a1064c1c28bb858f03b577b85eec171a3f874e925808e3ded1","observation_id":"30c40ab7-fb83-4c5a-b523-3bcca7094677","resolution":{"observed_at":"2026-08-06T21:17:57.194513Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1016/j.epsl.2013.03.046","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Earth and Planetary Science Letters 371:212--219","venue":"Earth and Planetary Science Letters","work_id":"23e03c1b-97ba-443f-99ba-b1cde19f918a","year":2013},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:25.724887Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:3d150fccdef7107121c656ed5f194d9b52455124fcd03290ce36079881267c3f","observation_id":"78984755-8221-4de5-b7a3-a6a83aac06a1","resolution":{"observed_at":"2026-08-06T21:17:56.950205Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:17:25.814751Z","title":"Living Rev Sol Phys 17(1):4","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:25.814751Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:66e40c18a656aefb473c9407a4d8e4ce9e9981d0cfe09860318065433a279c2e","observation_id":"f721b2f8-b85f-49d3-856b-f5672daa7663","resolution":{"observed_at":"2026-08-06T21:17:25.814751Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.16553","last_updated":"2023-05-26T00:41:35Z","snapshot_observed_at":"2026-08-08T22:28:24.294747Z","submitted_at":"2023-05-26T00:41:35Z","title":"Evolution of solar and stellar dynamo theory","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.16553","snapshot_observed_at":"2026-08-06T21:17:25.914881Z","title":"219(5):35","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:25.914881Z"},"links":{"cited_paper":"/paper/2305.16553","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:65ad25cf62ff463738f08494f4070bab21f9bfe6908949c5111efaea965ffea2","observation_id":"41360033-b324-4258-86da-c0ca0f13a5b1","resolution":{"observed_at":"2026-08-06T21:17:25.914881Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0405027","last_updated":"2004-05-03T14:06:39Z","snapshot_observed_at":"2026-08-03T06:57:17.000165Z","submitted_at":"2004-05-03T14:06:39Z","title":"Full--Sphere Simulations of a Circulation--Dominated Solar Dynamo: Exploring the Parity Issue","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0405027","snapshot_observed_at":"2026-08-06T21:17:25.974983Z","title":"427:1019--1030","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:25.974983Z"},"links":{"cited_paper":"/paper/astro-ph/0405027","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:e68e58b5660b83d54c72f948934a153bf18c2cb43d90557d4df3309ba2522819","observation_id":"6e5e8fb0-647e-4b1e-a0e4-3e1a5243ae2e","resolution":{"observed_at":"2026-08-06T21:17:25.974983Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1011.1218","last_updated":"2010-11-04T17:30:15Z","snapshot_observed_at":"2026-07-06T02:18:44.164256Z","submitted_at":"2010-11-04T17:30:15Z","title":"Alpha effect due to buoyancy instability of a magnetic layer","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1011.1218","snapshot_observed_at":"2026-08-06T21:17:26.033171Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:26.033171Z"},"links":{"cited_paper":"/paper/1011.1218","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:4db9a42a908dcea5ccbfe0b3c2ccff1659cdf873367627bc370cf47f31e7f801","observation_id":"d43d9e8a-c7d3-47d7-b0e9-bad82d51aafc","resolution":{"observed_at":"2026-08-06T21:17:26.033171Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:17:26.124749Z","title":"J Fluid Mech 470(1):115--133","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:26.124749Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:c729c464df17f9b4ce28398b964746018ec12d09bc23d2acedf12d2cc8ebb567","observation_id":"b618d0a0-7786-42dd-ba76-a21e6a89e295","resolution":{"observed_at":"2026-08-06T21:17:26.124749Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.03009","last_updated":"2020-06-04T16:56:47Z","snapshot_observed_at":"2026-08-06T04:58:50.423444Z","submitted_at":"2020-06-04T16:56:47Z","title":"List-three-coloring $ P_t $-free graphs with no induced 1-subdivision of $ K_{1,s} $","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.03009","snapshot_observed_at":"2026-08-06T21:17:26.235206Z","title":"Geophys J Int 166:97--114","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:26.235206Z"},"links":{"cited_paper":"/paper/2006.03009","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:2130ee94e4aac274225910d8f6f9906e82795d34301a597b334e4d4bd4a3e03e","observation_id":"6d11780d-f49f-4f19-ac05-cd69a9a77ab5","resolution":{"observed_at":"2026-08-06T21:17:26.235206Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1601.05246","last_updated":"2016-01-20T12:01:58Z","snapshot_observed_at":"2026-07-06T04:43:28.148921Z","submitted_at":"2016-01-20T12:01:58Z","title":"Robustness of oscillatory $\\alpha^2$ dynamos in spherical wedges","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.05246","snapshot_observed_at":"2026-08-06T21:17:26.494781Z","title":"a pyl \\\"a PJ, K \\","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:26.494781Z"},"links":{"cited_paper":"/paper/1601.05246","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:6cb07286162510713d3fda66ce7b422d32d72ff5216f183bf0dd05e4d5fcaf4e","observation_id":"ac24ad9a-a6dc-4a67-9f9a-4e9f77952a1e","resolution":{"observed_at":"2026-08-06T21:17:26.494781Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4398","last_updated":"2010-01-25T17:53:37Z","snapshot_observed_at":"2026-07-06T02:05:54.099875Z","submitted_at":"2010-01-25T17:53:37Z","title":"A Self-Consistent Treatment of the Electromotive Force in Magnetohydrodynamics for Large Diffusivities","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4398","snapshot_observed_at":"2026-08-06T21:17:26.654755Z","title":"Astron Nachr 331:667","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:26.654755Z"},"links":{"cited_paper":"/paper/1001.4398","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:e6f18434c89ebb89dce22b06c60ed57e4b3cb0740e0f06a5227e32ca73702a09","observation_id":"a0147f62-b388-436f-85f9-82be435f4ea8","resolution":{"observed_at":"2026-08-06T21:17:26.654755Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9709062","last_updated":"1997-09-08T17:03:11Z","snapshot_observed_at":"2026-07-07T01:18:17.177186Z","submitted_at":"1997-09-08T17:03:11Z","title":"Axisymmetric mean field dynamos with dynamic and algebraic $\\alpha$--quenchings","version":1},"cited_work":{"arxiv_id":"astro-ph/9709062","doi":"10.48550/arxiv.astro-ph/9709062","metadata_source":"pith","pith_arxiv_id":"astro-ph/9709062","snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Axisymmetric mean field dynamos with dynamic and algebraic $\\alpha$--quenchings","venue":"astro-ph","work_id":"7f0e5197-5fc8-4d26-898e-31a441c4f31a","year":1997},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:26.787590Z"},"links":{"cited_paper":"/paper/astro-ph/9709062","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:d93fc08128dd78c0530a2969191d7d317b5971967389fa92f4a273430f799cce","observation_id":"27552335-d25c-4c0b-80d1-1bddf05d8a73","resolution":{"observed_at":"2026-08-06T21:17:56.741736Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:17:26.934728Z","title":"94:39--48","venue":null,"work_id":null,"year":1933},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:26.934728Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:fafc4e0ff079275b7ff372644a717aeffae8a79d9d96cb28e840ef9b86f8396d","observation_id":"502e5b6d-9537-4171-a9aa-c0912b2f1e99","resolution":{"observed_at":"2026-08-06T21:17:26.934728Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:17:27.075591Z","title":"Cambridge Texts in Applied Mathematics, Cambridge University Press","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:27.075591Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:104964162fc2dda8cbeccf91d2380a85e30dd76b0bc2132086e978f84cf2484a","observation_id":"d2e05645-8836-44ae-9ca2-81b8caf04959","resolution":{"observed_at":"2026-08-06T21:17:27.075591Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1205.3502","last_updated":"2012-11-13T18:46:20Z","snapshot_observed_at":"2026-07-06T02:48:11.908123Z","submitted_at":"2012-05-15T20:13:56Z","title":"Turbulent dynamo with advective magnetic helicity flux","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1205.3502","snapshot_observed_at":"2026-08-06T21:17:27.228088Z","title":"429:1686--1694","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:27.228088Z"},"links":{"cited_paper":"/paper/1205.3502","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:ad79b683dba646156a2c82125882a2ddaa7c0bf795dfc58b313de1f93dd673d1","observation_id":"f74c95da-336e-44f8-b3b9-6bcf10e3e24f","resolution":{"observed_at":"2026-08-06T21:17:27.228088Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:17:27.371442Z","title":"518:508--520","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:27.371442Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:4e3e8f8db09e165b950413e039a804b67ce794692383232194ace1fcbc387f14","observation_id":"b04ded5f-2ca4-4415-96bc-cdc536eb3ad0","resolution":{"observed_at":"2026-08-06T21:17:27.371442Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0410645","last_updated":"2006-01-19T19:55:25Z","snapshot_observed_at":"2026-08-10T03:39:47.986513Z","submitted_at":"2004-10-27T16:30:24Z","title":"Magnetic field generation in fully convective rotating spheres","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0410645","snapshot_observed_at":"2026-08-06T21:17:27.487524Z","title":"638:336--347","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:27.487524Z"},"links":{"cited_paper":"/paper/astro-ph/0410645","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:47a82af901206e61c5b8d9b4f2a727a99d44ed0a857f6dabe4293a9c86763b43","observation_id":"cfc12cfd-e329-43fd-9bdf-1654426794fd","resolution":{"observed_at":"2026-08-06T21:17:27.487524Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0403321","last_updated":"2004-03-13T00:13:15Z","snapshot_observed_at":"2026-08-04T02:05:54.430561Z","submitted_at":"2004-03-13T00:13:15Z","title":"Magnetic activity in late-type giant stars: Numerical MHD simulations of non-linear dynamo action in Betelgeuse","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0403321","snapshot_observed_at":"2026-08-06T21:17:27.639576Z","title":"423:1101--1107","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:27.639576Z"},"links":{"cited_paper":"/paper/astro-ph/0403321","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:565b07aa73f103e6e989120299e492dc9f44b03831f3f380b458b07b3e20800c","observation_id":"be1b7973-f3f0-433b-bc0d-9b5b0999e794","resolution":{"observed_at":"2026-08-06T21:17:27.639576Z","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":"10.1051/0004-6361:20000141","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"365:562--570","venue":"Astronomy and Astrophysics","work_id":"f029995f-1716-4107-aa41-efd21b783f72","year":2001},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:27.836302Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:c385710c287c38d38052b2ef05ffbb16a28e5656a020939bae86fca861062952","observation_id":"284cce73-5491-47e8-9df1-1f84142dd673","resolution":{"observed_at":"2026-08-06T21:17:56.524780Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1511.05813","last_updated":"2015-12-03T17:06:46Z","snapshot_observed_at":"2026-07-06T04:36:56.674557Z","submitted_at":"2015-11-18T14:46:42Z","title":"Helicity inversion in spherical convection as a means for equatorward dynamo wave propagation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1511.05813","snapshot_observed_at":"2026-08-06T21:17:28.046468Z","title":"456:1708--1722","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:28.046468Z"},"links":{"cited_paper":"/paper/1511.05813","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:a3129808e1c0ff9b6e133c386059089ec451ede1b27e2158fed5d655e4622d3d","observation_id":"a593e52d-9023-409e-a073-2e8c0995ab29","resolution":{"observed_at":"2026-08-06T21:17:28.046468Z","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":"10.1088/0004-637x/775/1/69","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":null,"venue":"The Astrophysical Journal","work_id":"c8b7c82d-b320-4ecf-81a4-3398b146999f","year":2013},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:28.206752Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:5babe087e62e1f2bc61094ef6893612ea246adeac279f5f33fd06b677358554b","observation_id":"037e7d9f-ae45-4ecc-abab-bd8ab4c5f5d4","resolution":{"observed_at":"2026-08-06T21:17:56.284421Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/308643","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"533(1):546--556","venue":"The Astrophysical Journal","work_id":"3a832248-edb7-48fc-9ff0-9315fd5fc3fe","year":2000},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:28.325469Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:885cc55976d58b384f5bf5b6442ed875545ebed93ba2ba360a11304dd1f0f364","observation_id":"d1ce0254-bd7f-474b-8359-3202c47d9e52","resolution":{"observed_at":"2026-08-06T21:17:56.108161Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1405.3926","last_updated":"2014-05-15T18:13:06Z","snapshot_observed_at":"2026-07-06T03:43:48.973183Z","submitted_at":"2014-05-15T18:13:06Z","title":"A simulation of convective dynamo in the solar convective envelope: maintenance of the solar-like differential rotation and emerging flux","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.3926","snapshot_observed_at":"2026-08-06T21:17:28.437095Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:28.437095Z"},"links":{"cited_paper":"/paper/1405.3926","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:b0f578bb7866ec07bba1d6a83ec14a7f6e2cf363a5ad5df25742ae2a31ab96e3","observation_id":"cf8e541a-41da-4593-b352-88502b35ad54","resolution":{"observed_at":"2026-08-06T21:17:28.437095Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.04393","last_updated":"2015-04-16T21:50:49Z","snapshot_observed_at":"2026-08-01T16:17:21.136587Z","submitted_at":"2015-04-16T21:50:49Z","title":"$\\delta$-Sunspot Formation in Simulation of Active-Region-Scale Flux Emergence","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.04393","snapshot_observed_at":"2026-08-06T21:17:28.525476Z","title":"806(1):79","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:28.525476Z"},"links":{"cited_paper":"/paper/1504.04393","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:b290a76a74bb6dd27d9b5ce9f1d16fda665d6823d4ec65edbb5ec1bdf78c4efc","observation_id":"a54c1899-02d0-4e3b-8246-82d5e056f749","resolution":{"observed_at":"2026-08-06T21:17:28.525476Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1110.0374","last_updated":"2011-10-03T15:06:33Z","snapshot_observed_at":"2026-07-06T02:35:05.258609Z","submitted_at":"2011-10-03T15:06:33Z","title":"Small-scale dynamo action in rotating compressible convection","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1110.0374","snapshot_observed_at":"2026-08-06T21:17:28.658187Z","title":"J Fluid Mech 690:262--287","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:28.658187Z"},"links":{"cited_paper":"/paper/1110.0374","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:03c319887a852a4411b945641af20e26e075aac35e1e1cd0a0269df438b90b57","observation_id":"4d59c8bf-8776-4780-ac74-e65e7c2a7231","resolution":{"observed_at":"2026-08-06T21:17:28.658187Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0106133","last_updated":"2006-06-02T14:19:50Z","snapshot_observed_at":"2026-07-07T00:18:59.127380Z","submitted_at":"2001-06-07T15:01:50Z","title":"Tachocline Confinement by an Oscillatory Magnetic Field","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0106133","snapshot_observed_at":"2026-08-06T21:17:28.785508Z","title":"203(2):195--210","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:28.785508Z"},"links":{"cited_paper":"/paper/astro-ph/0106133","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:f4b4d8392081a31a161daf62ef6c04ef21d86bd773a056f000c09adad9490f4b","observation_id":"a42c28f5-8237-41c6-a36c-df648ad7386f","resolution":{"observed_at":"2026-08-06T21:17:28.785508Z","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":"10.1038/356691a0","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"356(6371):691--693","venue":"Nature","work_id":"1bed4e32-dc6c-419b-9252-5cd8d80c018a","year":1992},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:28.935132Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:b166437cdb96b1078b8c0fcc87f7669d89cb047193b3ff0b565ad892bbf63169","observation_id":"a4d4bb72-f23a-41e2-b4fc-c694ab1d80f1","resolution":{"observed_at":"2026-08-06T21:17:55.937748Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1208.6093","last_updated":"2012-08-30T07:25:24Z","snapshot_observed_at":"2026-08-10T03:15:06.422745Z","submitted_at":"2012-08-30T07:25:24Z","title":"Dipolar versus multipolar dynamos: the influence of the background density stratification","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1208.6093","snapshot_observed_at":"2026-08-06T21:17:29.065063Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:29.065063Z"},"links":{"cited_paper":"/paper/1208.6093","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:a2bc275ca8dbe8533e7105e59ddee971b22187813aa662418d61f5180c9510bf","observation_id":"7c43b5a4-b4f7-4cbc-9dcf-d24cf6e2bd0c","resolution":{"observed_at":"2026-08-06T21:17:29.065063Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1311.3047","last_updated":"2013-11-13T08:19:43Z","snapshot_observed_at":"2026-07-06T03:28:03.012593Z","submitted_at":"2013-11-13T08:19:43Z","title":"From solar-like to anti-solar differential rotation in cool stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1311.3047","snapshot_observed_at":"2026-08-06T21:17:29.186217Z","title":"438:L76--L80","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:29.186217Z"},"links":{"cited_paper":"/paper/1311.3047","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:96a3c9dd4a2154592c290d1b140e619bf5aa8face35a1da7578b668e30ca241d","observation_id":"89336ad5-4ec9-47b9-8614-626759905914","resolution":{"observed_at":"2026-08-06T21:17:29.186217Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1206.6784","last_updated":"2012-11-28T22:35:18Z","snapshot_observed_at":"2026-07-06T02:50:53.242072Z","submitted_at":"2012-06-28T18:07:08Z","title":"The supernova-regulated ISM. II. The mean magnetic field","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1206.6784","snapshot_observed_at":"2026-08-06T21:17:29.334832Z","title":"The mean magnetic field","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:29.334832Z"},"links":{"cited_paper":"/paper/1206.6784","citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:963cf5b51ebc320d0063b68d671236c9cb412fcd25a6a36fac607d5016c64eed","observation_id":"3ae5503d-11eb-4e7d-aae5-7ee82301bda9","resolution":{"observed_at":"2026-08-06T21:17:29.334832Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:17:29.490340Z","title":"715:L133--L137","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:29.490340Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:f3e81c33f1581f2b983401716a9d56d5ac8ce5e5f9ecb85e721fa6df7c478688","observation_id":"88476f62-9660-4670-adad-9a7320fa2c54","resolution":{"observed_at":"2026-08-06T21:17:29.490340Z","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":"10.1086/190891","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"II - Dynamos with cycles and strong feedbacks","venue":"The Astrophysical Journal Supplement Series","work_id":"471cd1c6-6508-48c5-a938-9806643ab6b0","year":1983},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:29.590350Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:9758f05783292b6626ddc9dc06d799b1153ea6afa1e8e5276c4af5d3f051e07a","observation_id":"b6c0f969-e355-477a-b377-996b1db6b52e","resolution":{"observed_at":"2026-08-06T21:17:55.765687Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/190743","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"46:211--238","venue":"The Astrophysical Journal Supplement Series","work_id":"b27230cf-9a16-4362-9427-ba6000ac9276","year":1981},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:29.688754Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:5bc17441f138c4163c1cf211ef38b6c457050bad595f33ed5dc52cd0fc18a773","observation_id":"654033d5-3f40-499f-a1e5-b49a77ffebea","resolution":{"observed_at":"2026-08-06T21:17:55.533600Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:17:29.767032Z","title":"Science 368(6498):1469--1472","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":101,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:29.767032Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:2e7813a9b7cc594b1c04fc8708a7fa520039713f44b4bd8f605b32098058b813","observation_id":"5c396f86-d0a2-44b3-bbc6-398dfb9d4d8c","resolution":{"observed_at":"2026-08-06T21:17:29.767032Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:17:29.884502Z","title":null,"venue":null,"work_id":null,"year":1984},"citing_paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations","version":1},"reference_index":102,"source":"arxiv_source","source_observed_at":"2026-08-06T21:17:29.884502Z"},"links":{"citing_paper":"/paper/2507.00632"},"observation_digest":"sha256:1e5c171220e1fd81f4f23e79568ccfb31832a3d0e5e593a8c0416fb7bddf358a","observation_id":"07663ff9-1d7f-46f9-87f0-a19e999f3fe5","resolution":{"observed_at":"2026-08-06T21:17:29.884502Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2507.00632","last_updated":"2025-07-01T10:24:43Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-10T18:25:42.461286Z","submitted_at":"2025-07-01T10:24:43Z","title":"Connecting mean-field theory with dynamo simulations"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":84,"verified_exact":16,"verified_fuzzy":0},"total_outbound_references":295},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 100 of 295 outbound references and 0 inbound Pith citation observations for arXiv:2507.00632."}