{"as_of":"2026-08-18T15:42:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:181069817ae8f33b653df040fce777750294646ab39c1284be5d8533896fa055","coverage":[{"denominator":54,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":54,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-11T11:50:26.030339Z","state":"measured"},{"denominator":54,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":54,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-18T06:34:40.430872+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/2607.07004/citation-record","integrity":"/paper/2607.07004/integrity","json":"/paper/2607.07004/citation-record.json","paper":"/paper/2607.07004"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"2201.05620","last_updated":"2022-03-15T16:48:47Z","snapshot_observed_at":"2026-08-16T17:28:16.654637Z","submitted_at":"2022-01-14T19:00:04Z","title":"The Magnetic Field versus Density relation in Star-Forming Molecular Clouds","version":2},"cited_work":{"arxiv_id":"2201.05620","doi":"10.3847/2041-8213/ac5a5a","metadata_source":"pith","pith_arxiv_id":"2201.05620","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"The Magnetic Field versus Density relation in Star-Forming Molecular Clouds","venue":"astro-ph.GA","work_id":"5ad883e4-5ea7-49ae-b9d8-6abb3ddcd8c2","year":2022},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2201.05620","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:d4d0f09ce7ee721137a91602de5b4504a0ad7a3943cee9f0793410904b8f7a96","observation_id":"e7e6fe55-ae04-48f2-b5a8-3b5980af48d8","resolution":{"observed_at":"2026-07-09T22:06:35.052749Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2109.10470","last_updated":"2022-10-15T19:53:47Z","snapshot_observed_at":"2026-08-16T17:54:59.818754Z","submitted_at":"2021-09-22T01:20:18Z","title":"The density distribution and physical origins of intermittency in supersonic, highly magnetised turbulence with diverse modes of driving","version":3},"cited_work":{"arxiv_id":"2109.10470","doi":null,"metadata_source":"pith","pith_arxiv_id":"2109.10470","snapshot_observed_at":"2026-07-09T22:06:35.107378Z","title":"The density distribution and physical origins of intermittency in supersonic, highly magnetised turbulence with diverse modes of driving","venue":"astro-ph.GA","work_id":"f9c6d382-1a3e-4a9a-8c72-fe8df9ae10fe","year":2021},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2109.10470","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:800a122ee1e48140f4d19713ab382d4a1cccb40e216fcd78761eb73c1fa73af3","observation_id":"918b71ef-d5a7-4bf5-bb2c-726be9dd173c","resolution":{"observed_at":"2026-07-09T22:06:35.108889Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2007.13937","last_updated":"2020-07-29T03:19:50Z","snapshot_observed_at":"2026-07-06T09:42:20.131155Z","submitted_at":"2020-07-28T01:38:59Z","title":"Magnetic field fluctuations in anisotropic, supersonic turbulence","version":2},"cited_work":{"arxiv_id":"2007.13937","doi":null,"metadata_source":"pith","pith_arxiv_id":"2007.13937","snapshot_observed_at":"2026-07-09T22:06:35.077169Z","title":"Magnetic field fluctuations in anisotropic, supersonic turbulence","venue":"astro-ph.GA","work_id":"5ed3172c-a047-4e9f-9de1-dd5499bbe26a","year":2020},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2007.13937","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:bfb950774f2a93fbc1107ad57c3b14c5680304da83f4c931b0b78afa09b0ffe8","observation_id":"b3939b2f-f1b6-423b-b20c-4ad84fe5eae0","resolution":{"observed_at":"2026-07-09T22:06:35.078605Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"physics/0105058","last_updated":"2001-05-18T11:35:45Z","snapshot_observed_at":"2026-07-07T06:45:41.622820Z","submitted_at":"2001-05-18T11:35:45Z","title":"On the small-scale statistics of Lagrangian turbulence","version":1},"cited_work":{"arxiv_id":"physics/0105058","doi":"10.1016/s0375-9601(01)00483-2","metadata_source":"pith","pith_arxiv_id":"physics/0105058","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"On the small-scale statistics of Lagrangian turbulence","venue":"physics.flu-dyn","work_id":"46d21a30-3e4b-4ecf-b5f3-5a89be926c05","year":2001},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/physics/0105058","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:859c57a6ddeab6ff7c6391ffc816105604d642f1c566f9f4e0bda58a26a92a82","observation_id":"95a8a254-860a-4645-8e8f-62237e19d7bf","resolution":{"observed_at":"2026-07-09T22:06:35.039223Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"cond-mat/0105374","last_updated":"2001-05-18T16:05:18Z","snapshot_observed_at":"2026-07-07T01:42:40.055725Z","submitted_at":"2001-05-18T16:05:18Z","title":"Dynamical foundations of nonextensive statistical mechanics","version":1},"cited_work":{"arxiv_id":"cond-mat/0105374","doi":null,"metadata_source":"pith","pith_arxiv_id":"cond-mat/0105374","snapshot_observed_at":"2026-07-09T22:06:35.088456Z","title":"Dynamical foundations of nonextensive statistical mechanics","venue":"cond-mat.stat-mech","work_id":"475bc097-dcdb-4c81-a2a6-02fbcacb7ed9","year":2001},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/cond-mat/0105374","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:9270dd81d4e163ab9286f854bc397ee063d20d69356de80d6b234f1b2bbaf69f","observation_id":"404795a3-85f6-47ba-8458-77a164125e8a","resolution":{"observed_at":"2026-07-09T22:06:35.090287Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2112.03838","last_updated":"2022-03-14T11:01:54Z","snapshot_observed_at":"2026-08-18T00:06:48.018949Z","submitted_at":"2021-12-07T17:23:43Z","title":"Dynamo effect in unstirred self-gravitating turbulence","version":3},"cited_work":{"arxiv_id":"2112.03838","doi":null,"metadata_source":"pith","pith_arxiv_id":"2112.03838","snapshot_observed_at":"2026-07-09T22:06:35.058203Z","title":"Dynamo effect in unstirred self-gravitating turbulence","venue":"astro-ph.GA","work_id":"2eddba51-993b-4aba-9460-a063157d82a2","year":2021},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2112.03838","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:474df8855670c97e414772f19d3bd328516944a1c186b53e835f6af7ac7c7121","observation_id":"d675a2a5-bcf6-43c0-b3d5-d03bc8513783","resolution":{"observed_at":"2026-07-09T22:06:35.062004Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2010.11227","last_updated":"2020-10-21T18:09:20Z","snapshot_observed_at":"2026-08-16T19:11:41.282174Z","submitted_at":"2020-10-21T18:09:20Z","title":"The Catalogue for Astrophysical Turbulence Simulations (CATS)","version":1},"cited_work":{"arxiv_id":"2010.11227","doi":null,"metadata_source":"pith","pith_arxiv_id":"2010.11227","snapshot_observed_at":"2026-07-09T22:06:35.066945Z","title":"The Catalogue for Astrophysical Turbulence Simulations (CATS)","venue":"astro-ph.GA","work_id":"f216aa34-f061-4403-985a-9e576bf6531a","year":2020},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2010.11227","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:268979a79ee05143fc63e31cecafd4314197962bffa92865b56175fc50a221c4","observation_id":"2517b25c-2a62-4faf-8767-96d63172b2ab","resolution":{"observed_at":"2026-07-09T22:06:35.068523Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0811.0822","last_updated":"2008-11-05T21:24:15Z","snapshot_observed_at":"2026-08-15T10:02:40.393253Z","submitted_at":"2008-11-05T21:24:15Z","title":"Density Studies of MHD Interstellar Turbulence: Statistical Moments, Correlations and Bispectrum","version":1},"cited_work":{"arxiv_id":"0811.0822","doi":null,"metadata_source":"pith","pith_arxiv_id":"0811.0822","snapshot_observed_at":"2026-07-09T22:06:35.031819Z","title":"Density Studies of MHD Interstellar Turbulence: Statistical Moments, Correlations and Bispectrum","venue":"astro-ph","work_id":"937cf23c-3fa7-4792-954c-bd7a286e9ca8","year":2008},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/0811.0822","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:81ffdfd46daaae5e8252c1fbd296042a189a32ec1667ccf320af6af917aa39cc","observation_id":"f8b61fd6-eb1a-43f0-8f43-fb54e4b66d30","resolution":{"observed_at":"2026-07-09T22:06:35.034273Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"8711.2003","doi":"10.1046/j.1365-8711.2003","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Jiang, F","venue":null,"work_id":"7159653d-74d0-44ca-b473-c338d9a8cd44","year":2003},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-07-09T21:57:49.151864Z"},"links":{"citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:e2f6a84bddbbb845d87a55b871dffde6610c4c032012b27ad505a99e0e12d65b","observation_id":"82a7866b-7984-4358-a5be-f2c0f8628a81","resolution":{"observed_at":"2026-07-09T22:06:35.055906Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1146/annurev-astro-081811-125514","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"doi:10.1146/annurev-astro-081811-125514 , journal =","venue":"Annual Review of Astronomy and Astrophysics","work_id":"a1d029b0-30ec-49d3-ad68-2f453c66fa45","year":2012},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-07-09T21:57:49.151864Z"},"links":{"citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:dff7a9bafda6f7f41e7e891d610a406a1def7855e0597110f02ea9d4a35818be","observation_id":"8e8c0a9b-0f81-4015-a74c-2605ecf0b219","resolution":{"observed_at":"2026-07-09T22:06:35.014141Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-17T19:38:17.373277+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-17T19:38:17.373277+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/248.1.1","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"MNRAS248, 1–13 (1991) https://doi.org/10.1093/mnras/248.1.1","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"3214ed7a-bccb-445e-b8e2-09ad7b4e5dad","year":1991},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-07-09T21:57:49.151864Z"},"links":{"citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:aa2a87636d93199f7ac02802b4b2c97dc6bd98477119047c7ef9f5a92070853b","observation_id":"3f3815e1-04c1-437a-aec0-1ef38ae41a7c","resolution":{"observed_at":"2026-07-09T22:06:35.012965Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1802.09485","last_updated":"2018-02-26T18:07:04Z","snapshot_observed_at":"2026-08-14T19:42:00.509719Z","submitted_at":"2018-02-26T18:07:04Z","title":"Thermodynamics and dynamics of two-dimensional systems with dipole-like repulsive interactions","version":1},"cited_work":{"arxiv_id":"1802.09485","doi":"10.1146/annurev.astro.41.011802.094856","metadata_source":"pith","pith_arxiv_id":"1802.09485","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Thermodynamics and dynamics of two-dimensional systems with dipole-like repulsive interactions","venue":"cond-mat.soft","work_id":"b7355e60-f402-4e0f-9ef3-6668fcfdd8d6","year":2018},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1802.09485","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:cc077b1ac9e80881819d235dc328a40bcf3c4feac324f35adb4ee98732193802","observation_id":"b52f1e0c-9c74-4cb8-a23a-af7328000ba1","resolution":{"observed_at":"2026-07-09T22:06:35.087299Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0808.0605","last_updated":"2008-11-06T15:37:41Z","snapshot_observed_at":"2026-08-15T10:09:31.074733Z","submitted_at":"2008-08-05T10:07:09Z","title":"The Density Probability Distribution in Compressible Isothermal Turbulence: Solenoidal versus Compressive Forcing","version":2},"cited_work":{"arxiv_id":"0808.0605","doi":null,"metadata_source":"pith","pith_arxiv_id":"0808.0605","snapshot_observed_at":"2026-07-09T22:06:35.061674Z","title":"The Density Probability Distribution in Compressible Isothermal Turbulence: Solenoidal versus Compressive Forcing","venue":"astro-ph","work_id":"06c7a603-bdb0-4558-a4d8-e79d4f8d4c15","year":2008},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/0808.0605","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:9993872aa6b9291e8f55a195ba85251c6009f1303c65bcac60d98c69af5ef442","observation_id":"0b6247cb-6060-4eaf-8882-39cfdfa594d0","resolution":{"observed_at":"2026-07-09T22:06:35.063184Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0905.1060","last_updated":"2010-04-13T19:01:47Z","snapshot_observed_at":"2026-08-15T05:48:57.816588Z","submitted_at":"2009-05-07T16:56:01Z","title":"Comparing the statistics of interstellar turbulence in simulations and observations: Solenoidal versus compressive turbulence forcing","version":4},"cited_work":{"arxiv_id":"0905.1060","doi":null,"metadata_source":"pith","pith_arxiv_id":"0905.1060","snapshot_observed_at":"2026-07-09T22:06:34.996566Z","title":"Comparing the statistics of interstellar turbulence in simulations and observations: Solenoidal versus compressive turbulence forcing","venue":"astro-ph.SR","work_id":"1425e34d-239c-442c-9cea-3b739c90daea","year":2009},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/0905.1060","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:47dc42fcf867831db555e5e28a60df7774fca92439ee953dc3d6040381db03b5","observation_id":"04981ea8-af69-456f-86c4-5d88ea23b21d","resolution":{"observed_at":"2026-07-09T22:06:34.999520Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1017/cbo9781139170666","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"doi: 10.1017/cbo9781139170666","venue":"Cambridge University Press eBooks","work_id":"d27816eb-73d7-491c-8f13-92bb4b56b0fe","year":1995},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-07-09T21:57:49.151864Z"},"links":{"citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:a5b1c6b59f6092c60d5e9cebe2872576d7013f01c3775a70e2ad214726098bc0","observation_id":"4be694ea-f276-46ed-a447-459c51787dd5","resolution":{"observed_at":"2026-07-09T22:06:35.089504Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-08T04:08:16.032343+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-08T04:08:16.032343+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0607230","last_updated":"2006-07-11T15:12:04Z","snapshot_observed_at":"2026-08-15T11:09:17.861932Z","submitted_at":"2006-07-11T15:12:04Z","title":"A High Order Godunov Scheme with Constrained Transport and Adaptive Mesh Refinement for Astrophysical MHD","version":1},"cited_work":{"arxiv_id":"astro-ph/0607230","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0607230","snapshot_observed_at":"2026-07-09T22:06:35.111441Z","title":"A High Order Godunov Scheme with Constrained Transport and Adaptive Mesh Refinement for Astrophysical MHD","venue":"astro-ph","work_id":"e359a523-5108-480d-8f6e-d37cff5a20f7","year":2006},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/astro-ph/0607230","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:f9c9eff928c9967da153e9ea7e4ac9653258c41a950b1db392c4ad5c618b4cd3","observation_id":"50bada41-c9cb-4bdb-8321-f6210682fc3a","resolution":{"observed_at":"2026-07-09T22:06:35.112886Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/317361","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T01:57:45.460968Z","title":"Fryxell, et al., Astrophys","venue":"The Astrophysical Journal Supplement Series","work_id":"ae0f4f84-8c0b-4c65-ba8a-f3c1efb19d03","year":2000},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-07-09T21:57:49.151864Z"},"links":{"citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:1f26651bb951fc9ce25af8546c164bb974fc29d6915bf792091f4e59dcde3d8f","observation_id":"64902760-87d1-4be6-b738-f90ce51eef09","resolution":{"observed_at":"2026-07-09T22:06:34.980843Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-17T19:08:12.896112+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-17T19:08:12.896112+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-09T22:06:35.959687Z","title":null,"venue":null,"work_id":"6041adcc-99b0-4b8b-a8aa-76e3903985ae","year":null},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-07-09T21:57:49.151864Z"},"links":{"citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:06be942941d8c33bd9dc2b12b53b50326a88d510afc7a7b2d644a2a9cac8c338","observation_id":"763cda60-8c4c-4110-8972-d38d23fa1030","resolution":{"observed_at":"2026-07-09T22:06:35.960873Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1063/1.857773","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Physics of Fluids A , keywords =","venue":"Physics of Fluids A Fluid Dynamics","work_id":"1a8fa11a-80c7-4556-b64b-68bdf937c8a7","year":null},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-07-09T21:57:49.151864Z"},"links":{"citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:62cae8066f1f27e6b8877da582e84546ce2038ec9705c442d5541480c2d94cd7","observation_id":"c005e435-bf0b-43c5-88a1-fce27510b958","resolution":{"observed_at":"2026-07-09T22:06:35.117655Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2005.06472","last_updated":"2020-05-13T18:00:00Z","snapshot_observed_at":"2026-08-17T13:53:23.011477Z","submitted_at":"2020-05-13T18:00:00Z","title":"Physical Processes in Star Formation","version":1},"cited_work":{"arxiv_id":"2005.06472","doi":null,"metadata_source":"pith","pith_arxiv_id":"2005.06472","snapshot_observed_at":"2026-07-09T22:06:35.063751Z","title":"Physical Processes in Star Formation","venue":"astro-ph.GA","work_id":"6d678c55-e08b-4e2d-ac2f-c80c226b8bd3","year":2020},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2005.06472","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:0ccf3f3e8e0c33023d40e09d25707f277ac0b20db4772948265cf1fef5f9f16d","observation_id":"30d6a119-3c9a-43b7-969d-43a27e01d88f","resolution":{"observed_at":"2026-07-09T22:06:35.065675Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0605121","last_updated":"2007-01-12T10:42:07Z","snapshot_observed_at":"2026-07-07T01:00:09.607410Z","submitted_at":"2006-05-04T10:13:09Z","title":"Simulating the formation of molecular clouds. II. Rapid formation from turbulent initial conditions","version":2},"cited_work":{"arxiv_id":"astro-ph/0605121","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0605121","snapshot_observed_at":"2026-07-09T22:06:35.097435Z","title":"Simulating the formation of molecular clouds. II. Rapid formation from turbulent initial conditions","venue":"astro-ph","work_id":"af6b9079-29f5-4a84-ae5c-f509fb3ea157","year":2006},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/astro-ph/0605121","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:48068458f099bb3346d6b8a6e86150531e9e12c9a8dcfd2caf4dd79e57fbca21","observation_id":"da08d3fc-d0a2-4a5f-a02d-86eb88a8875a","resolution":{"observed_at":"2026-07-09T22:06:35.098830Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2019.00005","doi":"10.1109/sp.2019.00005","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Frontiers in Astronomy and Space Sciences , keywords =","venue":null,"work_id":"832699c0-692d-4025-8993-ab1475ee4530","year":2019},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-07-09T21:57:49.151864Z"},"links":{"citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:739d366f95bc66230f99fb3067083b44004189424e03c765862b83ac98b4aad0","observation_id":"5a6a13ed-b960-42cc-a8b6-927c7697e958","resolution":{"observed_at":"2026-07-09T22:06:35.094157Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1211.0637","last_updated":"2012-11-03T21:26:40Z","snapshot_observed_at":"2026-08-15T00:40:36.349371Z","submitted_at":"2012-11-03T21:26:40Z","title":"Turbulent molecular clouds","version":1},"cited_work":{"arxiv_id":"1211.0637","doi":null,"metadata_source":"pith","pith_arxiv_id":"1211.0637","snapshot_observed_at":"2026-07-09T22:06:35.076328Z","title":"Turbulent molecular clouds","venue":"astro-ph.GA","work_id":"6976e0cb-d63e-460d-9a0f-93d757df2518","year":2012},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1211.0637","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:728cb5d90804a2f6d3e83c51558f91b3e4d1a9d46bd7718086731cc2896a9cbf","observation_id":"533cc63d-3133-44cd-aaf8-c2f71c2db916","resolution":{"observed_at":"2026-07-09T22:06:35.078287Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1211.3119","last_updated":"2013-07-01T09:47:36Z","snapshot_observed_at":"2026-08-15T00:39:28.473476Z","submitted_at":"2012-11-13T21:00:02Z","title":"A Model for (Non-Lognormal) Density Distributions in Isothermal Turbulence","version":2},"cited_work":{"arxiv_id":"1211.3119","doi":null,"metadata_source":"pith","pith_arxiv_id":"1211.3119","snapshot_observed_at":"2026-07-09T22:06:35.082708Z","title":"A Model for (Non-Lognormal) Density Distributions in Isothermal Turbulence","venue":"astro-ph.GA","work_id":"d0420c2f-70a3-4255-8359-3adaa8d51a56","year":2012},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1211.3119","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:c82336873a0ffd78c9ee8115bc896d70d5194cfcf594c6422a55b142be774806","observation_id":"945514f7-ce28-4b93-8011-1fad4582bbcf","resolution":{"observed_at":"2026-07-09T22:06:35.084342Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2402.10268","last_updated":"2024-02-19T19:00:01Z","snapshot_observed_at":"2026-08-16T14:18:11.122567Z","submitted_at":"2024-02-15T19:00:01Z","title":"Time evolution of the galactic $B- \\rho$ relation: the impact of the magnetic field morphology","version":2},"cited_work":{"arxiv_id":"2402.10268","doi":null,"metadata_source":"pith","pith_arxiv_id":"2402.10268","snapshot_observed_at":"2026-07-09T22:06:35.039512Z","title":"Time evolution of the galactic $B- \\rho$ relation: the impact of the magnetic field morphology","venue":"astro-ph.GA","work_id":"1e8f855e-e1ea-4aeb-87ee-d2c610286654","year":2024},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2402.10268","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:cd3b796de8f09e66afc5af19212612ee83af56636c87a4a19824468f905dbe32","observation_id":"74381d18-8056-4fbe-b452-c970d621208e","resolution":{"observed_at":"2026-07-09T22:06:35.041033Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0608051","last_updated":"2007-02-12T21:40:49Z","snapshot_observed_at":"2026-07-07T01:02:02.430757Z","submitted_at":"2006-08-02T06:20:11Z","title":"Density Fluctuations in MHD Turbulence: Spectra, Intermittency and Topology","version":2},"cited_work":{"arxiv_id":"astro-ph/0608051","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0608051","snapshot_observed_at":"2026-07-09T22:06:35.042297Z","title":"Density Fluctuations in MHD Turbulence: Spectra, Intermittency and Topology","venue":"astro-ph","work_id":"85f0ecda-9c70-4e66-ae22-60ab92144ed7","year":2006},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/astro-ph/0608051","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:092be6631f0f5cebf5d0dfbc266b2dfd4db9c6f1fa41ea0d4ca74cb0305794b5","observation_id":"ba96cc71-5974-4814-815b-18483b3ef373","resolution":{"observed_at":"2026-07-09T22:06:35.043638Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physreve.59.5457","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":", keywords =","venue":"Journal de Physique et le Radium (France)     Changed to J. Phys. (Orsay, Fr.)","work_id":"c5e8f899-70a5-4fa1-b2a1-c7a706e9b96c","year":null},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-07-09T21:57:49.151864Z"},"links":{"citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:14e880abc7586e0b96e61f82871523eef9d95a636d30c272996353f78b63ded7","observation_id":"8be417ed-e409-4839-bcc8-d547f8eac378","resolution":{"observed_at":"2026-07-09T22:06:35.036188Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1608.02050","last_updated":"2016-08-06T01:54:23Z","snapshot_observed_at":"2026-08-14T21:45:12.633855Z","submitted_at":"2016-08-06T01:54:23Z","title":"SHOCKFIND - An algorithm to identify magnetohydrodynamic shock waves in turbulent clouds","version":1},"cited_work":{"arxiv_id":"1608.02050","doi":"10.1093/mnras/stw2015","metadata_source":"pith","pith_arxiv_id":"1608.02050","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"SHOCKFIND - An algorithm to identify magnetohydrodynamic shock waves in turbulent clouds","venue":"astro-ph.GA","work_id":"d7e44d41-c5c1-403d-84aa-9660a294489d","year":2016},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1608.02050","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:401ed1cdb53e7bb750e8252dddbf72a5f67a578acf96142e6d4b183077b28bb7","observation_id":"c9366782-a702-4a50-9d8c-cff8a1f6f5cd","resolution":{"observed_at":"2026-07-09T22:06:35.120659Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0410734","last_updated":"2005-01-27T19:04:08Z","snapshot_observed_at":"2026-07-07T00:45:45.012448Z","submitted_at":"2004-10-29T13:28:44Z","title":"The Distribution of Pressures in a Supernova-Driven Interstellar Medium. I. Magnetized Medium","version":2},"cited_work":{"arxiv_id":"astro-ph/0410734","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0410734","snapshot_observed_at":"2026-07-09T22:06:35.113292Z","title":"The Distribution of Pressures in a Supernova-Driven Interstellar Medium. I. Magnetized Medium","venue":"astro-ph","work_id":"06cff1ca-d5a2-42e3-b925-580321de6cea","year":2004},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/astro-ph/0410734","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:6bbb09f9714dabbb846ebd97936608cb11ac116ad3a04ab362779decbdb0b96e","observation_id":"f6f45353-8ae1-46ff-a0a6-68fd1de8c183","resolution":{"observed_at":"2026-07-09T22:06:35.114659Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0301093","last_updated":"2003-09-10T12:57:06Z","snapshot_observed_at":"2026-07-07T00:30:33.951336Z","submitted_at":"2003-01-06T22:54:18Z","title":"Control of star formation by supersonic turbulence","version":2},"cited_work":{"arxiv_id":"astro-ph/0301093","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0301093","snapshot_observed_at":"2026-07-09T22:06:35.118867Z","title":"Control of star formation by supersonic turbulence","venue":"astro-ph","work_id":"1cecb28a-0b98-453e-b54e-ae23d8144232","year":2003},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/astro-ph/0301093","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:0f1d3628a026b159dc5a0b6e28ab2a97c6add782e9ec751c5ca97fe4b0026d20","observation_id":"d3a2863d-2a9b-4f8a-a185-8ca780d49885","resolution":{"observed_at":"2026-07-09T22:06:35.120520Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1206.2476","last_updated":"2015-10-21T11:57:23Z","snapshot_observed_at":"2026-08-15T00:57:10.344068Z","submitted_at":"2012-06-12T09:51:17Z","title":"Incorporating Ambipolar and Ohmic Diffusion in the AMR MHD code RAMSES","version":2},"cited_work":{"arxiv_id":"1206.2476","doi":null,"metadata_source":"pith","pith_arxiv_id":"1206.2476","snapshot_observed_at":"2026-07-09T22:06:35.067140Z","title":"Incorporating Ambipolar and Ohmic Diffusion in the AMR MHD code RAMSES","venue":"astro-ph.SR","work_id":"b03f9b06-2ffa-4cac-99b7-d5c5501f0854","year":2012},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1206.2476","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:5205c67ec9b6ca08b204348b437425a73b96f10f9e6af7ba052dc0ec32d3bf9c","observation_id":"e0937af5-a175-4bb2-b531-f2d67e0316ba","resolution":{"observed_at":"2026-07-09T22:06:35.069332Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-09T22:06:35.957652Z","title":", year = 1965, month = jun, volume =","venue":null,"work_id":"4d2344c2-7e04-448a-ac4a-2dde140fb9bb","year":1965},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-07-09T21:57:49.151864Z"},"links":{"citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:e5ebc9a6e495c47986731c772c7da56389705eef7a8a8eb7c62c9d7609dcd661","observation_id":"3d18a0ea-2ba3-49cc-a6d6-44535cca8a85","resolution":{"observed_at":"2026-07-09T22:06:35.959116Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1908.00544","last_updated":"2019-10-06T14:01:52Z","snapshot_observed_at":"2026-08-14T15:46:04.270361Z","submitted_at":"2019-08-01T18:00:00Z","title":"A Markov model for non-lognormal density distributions in compressive isothermal turbulence","version":2},"cited_work":{"arxiv_id":"1908.00544","doi":null,"metadata_source":"pith","pith_arxiv_id":"1908.00544","snapshot_observed_at":"2026-07-09T22:06:35.122338Z","title":"A Markov model for non-lognormal density distributions in compressive isothermal turbulence","venue":"astro-ph.GA","work_id":"285321ff-bc91-4716-a2f7-083488123ae2","year":2019},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1908.00544","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:81bc49d1e38bbfd5d4665280ee8e50ee8e59cbb5a2c3c5f7c50380ef5ba7b412","observation_id":"09dc6f34-be9a-4faf-a48b-b6221985cb00","resolution":{"observed_at":"2026-07-09T22:06:35.123643Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/154835","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"keywords =","venue":"The Astrophysical Journal","work_id":"8d676642-cac4-4834-ae19-54df8b2c9708","year":1976},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-07-09T21:57:49.151864Z"},"links":{"citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:1ec17cf9f1a625930a2b8b6c0cf58bcc13c0549fb4ed01f42735e3f1ae728fcc","observation_id":"63779c71-99d2-4dde-ae78-5cbce6397dca","resolution":{"observed_at":"2026-07-09T22:06:35.029846Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:49:20.393686+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:49:20.393686+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2409.16699","last_updated":"2024-09-25T07:45:20Z","snapshot_observed_at":"2026-08-16T13:15:36.295677Z","submitted_at":"2024-09-25T07:45:20Z","title":"Strong turbulence and magnetic coherent structures in the interstellar medium","version":1},"cited_work":{"arxiv_id":"2409.16699","doi":null,"metadata_source":"pith","pith_arxiv_id":"2409.16699","snapshot_observed_at":"2026-07-09T22:06:35.102624Z","title":"Strong turbulence and magnetic coherent structures in the interstellar medium","venue":"astro-ph.GA","work_id":"8c55e545-3129-45a3-92c7-c65ffc459d20","year":2024},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2409.16699","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:3b64184b1981468fa7587c3788981114b3c0524ff8c2f835c60a7f79ea28be4e","observation_id":"99886413-699c-442d-893d-9899d7db2584","resolution":{"observed_at":"2026-07-09T22:06:35.104092Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"physics/9802019","last_updated":"1998-02-10T19:14:30Z","snapshot_observed_at":"2026-07-07T06:58:38.987532Z","submitted_at":"1998-02-10T19:14:30Z","title":"Density probability distribution in one-dimensional polytropic gas dynamics","version":1},"cited_work":{"arxiv_id":"physics/9802019","doi":null,"metadata_source":"pith","pith_arxiv_id":"physics/9802019","snapshot_observed_at":"2026-07-09T22:06:35.052937Z","title":"Density probability distribution in one-dimensional polytropic gas dynamics","venue":"physics.flu-dyn","work_id":"8e1bc424-9cc4-4417-ae22-0e28e51729db","year":1998},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/physics/9802019","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:485e54ca012ebe37ef4a8d867acb4546b69f2e1158d84a61daebfc4630810b25","observation_id":"f61decd8-04fd-4b1b-a837-3599419aa910","resolution":{"observed_at":"2026-07-09T22:06:35.054563Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9603061","last_updated":"1996-03-14T02:10:38Z","snapshot_observed_at":"2026-07-07T01:13:02.642541Z","submitted_at":"1996-03-14T02:10:38Z","title":"Supersonic turbulence in the ISM: stellar extinction determinations as probes of the structure and dynamics of dark clouds","version":1},"cited_work":{"arxiv_id":"astro-ph/9603061","doi":"10.1086/303482","metadata_source":"pith","pith_arxiv_id":"astro-ph/9603061","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Supersonic turbulence in the ISM: stellar extinction determinations as probes of the structure and dynamics of dark clouds","venue":"astro-ph","work_id":"3ee0bfe2-19fb-4bef-98e3-7541f258da27","year":1996},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/astro-ph/9603061","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:f960064dd40b99b6fc1d7bcb5bd3f40bf1ca6978c3dcc97d50333842955606d1","observation_id":"77bfd88e-3942-4596-8232-9843e47b725a","resolution":{"observed_at":"2026-07-09T22:06:35.127364Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-05-24T10:23:26.328053+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-24T10:23:26.328053+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0907.0248","last_updated":"2010-12-11T12:43:06Z","snapshot_observed_at":"2026-08-15T05:44:38.602140Z","submitted_at":"2009-07-01T21:40:55Z","title":"The Star Formation Rate of Supersonic MHD Turbulence","version":4},"cited_work":{"arxiv_id":"0907.0248","doi":null,"metadata_source":"pith","pith_arxiv_id":"0907.0248","snapshot_observed_at":"2026-07-09T22:06:35.095666Z","title":"The Star Formation Rate of Supersonic MHD Turbulence","venue":"astro-ph.GA","work_id":"14438e1c-544f-44b7-96a9-0080a29cb059","year":2009},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/0907.0248","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:236b38af99264c20cc86716aba4398c8bb313b6e859ea5b37efc6977adb6c30e","observation_id":"c770f38c-0df1-4441-a32e-de5aa1d3b1e4","resolution":{"observed_at":"2026-07-09T22:06:35.097232Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2203.11179","last_updated":"2022-03-21T17:56:34Z","snapshot_observed_at":"2026-08-16T17:12:55.414945Z","submitted_at":"2022-03-21T17:56:34Z","title":"Magnetic fields in star formation: from clouds to cores","version":1},"cited_work":{"arxiv_id":"2203.11179","doi":"10.48550/arxiv.2203.11179","metadata_source":"pith","pith_arxiv_id":"2203.11179","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Magnetic fields in star formation: from clouds to cores","venue":"astro-ph.GA","work_id":"f1d5c4f2-ead0-4518-884d-e84bf6ea8aae","year":2022},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-07-09T21:57:49.151864Z"},"links":{"cited_paper":"/paper/2203.11179","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:92147f7bf0918da4f4e5d04a94a1c4639f25c7320a542466583b5284efb21a6a","observation_id":"b88592f7-f397-473e-a66a-28fa203bd204","resolution":{"observed_at":"2026-07-09T22:06:35.115711Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:49:46.000223+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:49:46.000223+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2307.04876","last_updated":"2023-07-10T19:54:38Z","snapshot_observed_at":"2026-08-16T15:17:19.432164Z","submitted_at":"2023-07-10T19:54:38Z","title":"Density and Velocity Correlations in Isothermal Supersonic Turbulence","version":1},"cited_work":{"arxiv_id":"2307.04876","doi":"10.1093/mnras/stad2195","metadata_source":"pith","pith_arxiv_id":"2307.04876","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Density and Velocity Correlations in Isothermal Supersonic Turbulence","venue":"astro-ph.GA","work_id":"0ae77879-cfd8-40af-bdb0-9716c05daa2e","year":2023},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2307.04876","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:d68dea7b2f6a6f0a7489160106ccdcc2202a9917b08cd3bd14966d7e8ba9d4a7","observation_id":"fc1dc1b3-f2d8-4cab-ba26-b556d97fc9dd","resolution":{"observed_at":"2026-07-09T22:06:35.092167Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.22408","last_updated":"2024-10-29T18:00:02Z","snapshot_observed_at":"2026-08-16T13:04:50.041975Z","submitted_at":"2024-10-29T18:00:02Z","title":"Understanding Density Fluctuations in Supersonic, Isothermal Turbulence","version":1},"cited_work":{"arxiv_id":"2410.22408","doi":"10.1126/sciadv.ado3958","metadata_source":"pith","pith_arxiv_id":"2410.22408","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Understanding Density Fluctuations in Supersonic, Isothermal Turbulence","venue":"astro-ph.GA","work_id":"ca669ea3-0620-4c8a-b2a6-f405ce7b1d9c","year":2024},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2410.22408","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:c355948943a34de0fa0a2cc9d63646e5ed2c6389c6d18ce7f8c1922bd31be3b7","observation_id":"0acf349a-62dd-4238-8e34-be5827a15319","resolution":{"observed_at":"2026-07-09T22:06:35.105920Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1809.07780","last_updated":"2018-09-20T18:00:23Z","snapshot_observed_at":"2026-08-14T18:25:42.379490Z","submitted_at":"2018-09-20T18:00:23Z","title":"Modeling Star Formation as a Markov Process in a Supersonic Gravoturbulent Medium","version":1},"cited_work":{"arxiv_id":"1809.07780","doi":"10.3847/2041-8213/aae1f9","metadata_source":"pith","pith_arxiv_id":"1809.07780","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Modeling Star Formation as a Markov Process in a Supersonic Gravoturbulent Medium","venue":"astro-ph.GA","work_id":"ab87f55b-bf6c-4640-b4c6-acba476830da","year":2018},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1809.07780","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:47381e2908f90e82497668eabdd3e6b758d663a54578455f131c38e2c888293f","observation_id":"5b0d5229-61ef-42f9-bf19-e1fc57a224d7","resolution":{"observed_at":"2026-07-09T22:06:35.111887Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0312046","last_updated":"2005-01-16T16:14:56Z","snapshot_observed_at":"2026-07-07T00:38:42.432535Z","submitted_at":"2003-12-01T22:27:01Z","title":"Simulations of small-scale turbulent dynamo","version":3},"cited_work":{"arxiv_id":"astro-ph/0312046","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0312046","snapshot_observed_at":"2026-07-09T22:06:34.982560Z","title":"Simulations of small-scale turbulent dynamo","venue":"astro-ph","work_id":"a606cc6c-e3e8-4ba0-b457-85f536037e9c","year":2003},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/astro-ph/0312046","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:610b58423e6c216d19ab96446c9656102a86762ccc5f7beaed17bc5ad3419610","observation_id":"6d8c7d1d-5692-410c-896b-8da1a9400b70","resolution":{"observed_at":"2026-07-09T22:06:34.984182Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2003.07997","last_updated":"2020-03-18T00:46:53Z","snapshot_observed_at":"2026-08-08T05:43:18.715579Z","submitted_at":"2020-03-18T00:46:53Z","title":"On the saturation mechanism of the fluctuation dynamo at ${\\text{Pr}_\\mathrm{M}} \\ge 1$","version":1},"cited_work":{"arxiv_id":"2003.07997","doi":null,"metadata_source":"pith","pith_arxiv_id":"2003.07997","snapshot_observed_at":"2026-07-09T22:06:35.105505Z","title":"On the saturation mechanism of the fluctuation dynamo at ${\\text{Pr}_\\mathrm{M}} \\ge 1$","venue":"astro-ph.GA","work_id":"bc896c6c-7e53-4a7b-9a54-4a1fe62203d7","year":2020},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2003.07997","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:432872e860a214796e41c3157012cdc5e3027250f54c10fcf3ebd3f35ded0f4c","observation_id":"dbeedaf8-779e-4639-b11b-168f329ebca7","resolution":{"observed_at":"2026-07-09T22:06:35.107102Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2109.11698","last_updated":"2021-09-24T00:38:45Z","snapshot_observed_at":"2026-08-16T17:54:25.640377Z","submitted_at":"2021-09-24T00:38:45Z","title":"Saturation mechanism of the fluctuation dynamo in supersonic turbulent plasmas","version":1},"cited_work":{"arxiv_id":"2109.11698","doi":null,"metadata_source":"pith","pith_arxiv_id":"2109.11698","snapshot_observed_at":"2026-07-09T22:06:35.024559Z","title":"Saturation mechanism of the fluctuation dynamo in supersonic turbulent plasmas","venue":"astro-ph.GA","work_id":"bbe89026-9aac-4414-8612-78802cce8565","year":2021},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2109.11698","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:6d0ebce66d6b097075fdcb3c7528ceace41011343ea6977732b7e39c66afe5aa","observation_id":"ae1503be-4704-4171-9153-aff5efcc6f28","resolution":{"observed_at":"2026-07-09T22:06:35.026905Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0008125","last_updated":"2000-08-08T15:13:20Z","snapshot_observed_at":"2026-07-07T00:12:28.123751Z","submitted_at":"2000-08-08T15:13:20Z","title":"The distribution of shock waves in driven supersonic turbulence","version":1},"cited_work":{"arxiv_id":"astro-ph/0008125","doi":"10.48550/arxiv.astro-ph/0008125","metadata_source":"pith","pith_arxiv_id":"astro-ph/0008125","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"The distribution of shock waves in driven supersonic turbulence","venue":"astro-ph","work_id":"cd379677-1f0b-4aae-b3a9-cbe1197080a7","year":2000},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-07-09T21:57:49.151864Z"},"links":{"cited_paper":"/paper/astro-ph/0008125","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:a067d8d4f3917292f25d86b00bba499253375a3804f7e95e1ddedc4f28665fbc","observation_id":"c018ea53-d52f-4831-b6c5-18000f4bffa1","resolution":{"observed_at":"2026-07-09T22:06:35.086910Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1702.07731","last_updated":"2017-02-24T19:09:35Z","snapshot_observed_at":"2026-08-15T16:30:01.269987Z","submitted_at":"2017-02-24T19:09:35Z","title":"The distribution of density in supersonic turbulence","version":1},"cited_work":{"arxiv_id":"1702.07731","doi":null,"metadata_source":"pith","pith_arxiv_id":"1702.07731","snapshot_observed_at":"2026-07-09T22:06:35.108466Z","title":"The distribution of density in supersonic turbulence","venue":"astro-ph.GA","work_id":"ed0f642b-a6ba-4062-be7d-eedf5727a1e3","year":2017},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1702.07731","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:2868aca64dba69186cc3121a863447e64809e776d6d58bba92eb81ed0f155386","observation_id":"aeb07dff-4bc2-44cd-842d-1129c5bcf80b","resolution":{"observed_at":"2026-07-09T22:06:35.109956Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2202.08324","last_updated":"2022-05-17T04:21:35Z","snapshot_observed_at":"2026-08-16T17:20:44.693179Z","submitted_at":"2022-02-16T20:41:28Z","title":"Turbulent dynamo in the two-phase interstellar medium","version":2},"cited_work":{"arxiv_id":"2202.08324","doi":"10.1093/mnras/stac1400","metadata_source":"pith","pith_arxiv_id":"2202.08324","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Turbulent dynamo in the two-phase interstellar medium","venue":"astro-ph.GA","work_id":"5579b5b4-2838-4991-af56-bdb6ef28b995","year":2022},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2202.08324","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:d0d1bb2fac84e8c8a0def564bb700f3b8235357f5c740d18ef41607549b96aec","observation_id":"48898d65-055e-4c49-a3f9-f4647e97d757","resolution":{"observed_at":"2026-07-09T22:06:35.117503Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0111367","last_updated":"2001-11-19T18:11:54Z","snapshot_observed_at":"2026-07-07T00:23:16.895347Z","submitted_at":"2001-11-19T18:11:54Z","title":"Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES","version":1},"cited_work":{"arxiv_id":"astro-ph/0111367","doi":"10.48550/arxiv.astro-ph/0111367","metadata_source":"pith","pith_arxiv_id":"astro-ph/0111367","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES","venue":"astro-ph","work_id":"fe2efa9c-1a59-4cfc-aa59-a0132a81ee4d","year":2001},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/astro-ph/0111367","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:20da9056ba66bb14dd63b21fee132ba43bfceff6f08e51966218d7195c2e6924","observation_id":"9b09c36e-1064-4e04-ab6b-fd3350ed21e3","resolution":{"observed_at":"2026-07-09T22:06:35.083086Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1007/bf01016429","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-09T22:06:35.020961Z","title":"Possible generalization of Boltzmann-Gibbs statistics , url =","venue":"Journal of Statistical Physics","work_id":"4628e251-6dd9-4d6f-ad9c-1ad9409de22a","year":1988},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-07-09T21:57:49.151864Z"},"links":{"citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:c9db11c788238b05c53421dfb8e9122145e39f74941305652607a7239a01caca","observation_id":"9c208256-470b-4eee-81aa-4ab87eedef70","resolution":{"observed_at":"2026-07-09T22:06:35.023050Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-07-31T22:51:24.710607+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-31T22:51:24.710607+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1505.05508","last_updated":"2015-05-20T20:00:34Z","snapshot_observed_at":"2026-08-14T22:47:45.457728Z","submitted_at":"2015-05-20T20:00:34Z","title":"Magnetic Field - Gas Density Relation and Observational Implications Revisited","version":1},"cited_work":{"arxiv_id":"1505.05508","doi":null,"metadata_source":"pith","pith_arxiv_id":"1505.05508","snapshot_observed_at":"2026-07-09T22:06:35.059106Z","title":"Magnetic Field - Gas Density Relation and Observational Implications Revisited","venue":"astro-ph.GA","work_id":"b41fbe07-0fa5-4f3d-9b87-59a02617744b","year":2015},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1505.05508","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:d2f150e9a692c0042b20f67d67d234d4af1e4ba93eccf72eaf1f94fe200f16ed","observation_id":"3cf8844c-e55f-44ae-bd25-a9913a1376a8","resolution":{"observed_at":"2026-07-09T22:06:35.060439Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-09T22:06:35.955498Z","title":"biburl =","venue":null,"work_id":"1dda9284-68f5-48b2-ad9d-38830a2a4277","year":null},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-07-09T21:57:49.151864Z"},"links":{"citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:96941ead758fae7f870940776d01d651a3fc552e0cd4470743a71dbd44d66ad7","observation_id":"bafd3227-057e-402d-8a63-e0daffb2651e","resolution":{"observed_at":"2026-07-09T22:06:35.956961Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/173847","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"The Astrophysical Journal , keywords =","venue":"The Astrophysical Journal","work_id":"db165f35-e370-4ca9-a191-9457926427dc","year":1994},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-07-09T21:57:49.151864Z"},"links":{"citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:91c2dca9f98468d15653d5b8032aed235e59e7b81ead905a0a11d3969308b38f","observation_id":"4aed0e07-0713-4d97-a36f-f74f2ce820a8","resolution":{"observed_at":"2026-07-09T22:06:35.065510Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-07-13T13:49:50.860217+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-13T13:49:50.860217+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.18293","last_updated":"2025-06-04T18:00:00Z","snapshot_observed_at":"2026-08-16T13:30:59.501801Z","submitted_at":"2024-07-25T18:00:00Z","title":"On the relation between magnetic field strength and gas density in the interstellar medium: A multiscale analysis","version":3},"cited_work":{"arxiv_id":"2407.18293","doi":"10.48550/arxiv.2407.18293","metadata_source":"pith","pith_arxiv_id":"2407.18293","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"J., Srinivasan, S., Pudritz, R","venue":"astro-ph.GA","work_id":"f54f282b-3eb9-495e-99f5-e63eebddb051","year":2024},"citing_paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2407.18293","citing_paper":"/paper/2607.07004"},"observation_digest":"sha256:5691d2cf4a3bece86a69eefc28bfe0984f3a1d036a7afca479b3ed885c57fe79","observation_id":"ac87ef5b-7c23-46b7-9993-afebd821db74","resolution":{"observed_at":"2026-07-09T22:06:35.075736Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2607.07004","last_updated":"2026-07-08T04:55:12Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-18T14:41:05.889129Z","submitted_at":"2026-07-08T04:55:12Z","title":"The dynamical origin of the magnetic field distributions in compressible turbulence"},"reference_resolution":{"displayed":54,"state_counts":{"malformed_identifier":0,"metadata_mismatch":12,"parse_uncertain":0,"unresolved":1,"verified_exact":39,"verified_fuzzy":2},"total_outbound_references":54},"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":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"thesis":"As of 18 August 2026, this Paper Citation Record lists 54 of 54 outbound references and 0 inbound Pith citation observations for arXiv:2607.07004."}