Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z
Paper Citation Record · LEDGER
The dynamical origin of the magnetic field distributions in compressible turbulence
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.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
54 of 54 outbound references displayed
- verified exact39
- verified fuzzy2
- unresolved1
- parse uncertain0
- malformed identifier0
- metadata mismatch12
External citation measurements
No source-named external measurement is stored.
Outbound references
Observation e7e6fe55-ae04-48f2-b5a8-3b5980af48d8 · outbound
This paper cites The Magnetic Field versus Density relation in Star-Forming Molecular Clouds.
The dynamical origin of the magnetic field distributions in compressible turbulence The Magnetic Field versus Density relation in Star-Forming Molecular Clouds
Reference 1
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.052749Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 918b71ef-d5a7-4bf5-bb2c-726be9dd173c · outbound
This paper cites The density distribution and physical origins of intermittency in supersonic, highly magnetised turbulence with diverse modes of driving.
The dynamical origin of the magnetic field distributions in compressible turbulence The density distribution and physical origins of intermittency in supersonic, highly magnetised turbulence with diverse modes of driving
Reference 2
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.108889Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation b3939b2f-f1b6-423b-b20c-4ad84fe5eae0 · outbound
This paper cites Magnetic field fluctuations in anisotropic, supersonic turbulence.
The dynamical origin of the magnetic field distributions in compressible turbulence Magnetic field fluctuations in anisotropic, supersonic turbulence
Reference 3
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.078605Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 95a8a254-860a-4645-8e8f-62237e19d7bf · outbound
This paper cites On the small-scale statistics of Lagrangian turbulence.
The dynamical origin of the magnetic field distributions in compressible turbulence On the small-scale statistics of Lagrangian turbulence
Reference 4
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-07-09T22:06:35.039223Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 404795a3-85f6-47ba-8458-77a164125e8a · outbound
This paper cites Dynamical foundations of nonextensive statistical mechanics.
The dynamical origin of the magnetic field distributions in compressible turbulence Dynamical foundations of nonextensive statistical mechanics
Reference 5
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.090287Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation d675a2a5-bcf6-43c0-b3d5-d03bc8513783 · outbound
This paper cites Dynamo effect in unstirred self-gravitating turbulence.
The dynamical origin of the magnetic field distributions in compressible turbulence Dynamo effect in unstirred self-gravitating turbulence
Reference 6
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.062004Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 2517b25c-2a62-4faf-8767-96d63172b2ab · outbound
This paper cites The Catalogue for Astrophysical Turbulence Simulations (CATS).
The dynamical origin of the magnetic field distributions in compressible turbulence The Catalogue for Astrophysical Turbulence Simulations (CATS)
Reference 7
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.068523Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation f8b61fd6-eb1a-43f0-8f43-fb54e4b66d30 · outbound
This paper cites Density Studies of MHD Interstellar Turbulence: Statistical Moments, Correlations and Bispectrum.
The dynamical origin of the magnetic field distributions in compressible turbulence Density Studies of MHD Interstellar Turbulence: Statistical Moments, Correlations and Bispectrum
Reference 8
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.034273Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 82a7866b-7984-4358-a5be-f2c0f8628a81 · outbound
This paper cites Jiang, F.
The dynamical origin of the magnetic field distributions in compressible turbulence Jiang, F
Reference 9
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-07-09T22:06:35.055906Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 8e8c0a9b-0f81-4015-a74c-2605ecf0b219 · outbound
This paper cites doi:10.1146/annurev-astro-081811-125514 , journal =.
The dynamical origin of the magnetic field distributions in compressible turbulence doi:10.1146/annurev-astro-081811-125514 , journal =
Reference 10
- Resolution
- metadata mismatch
- doi, observed 2026-07-09T22:06:35.014141Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 3f3815e1-04c1-437a-aec0-1ef38ae41a7c · outbound
This paper cites MNRAS248, 1–13 (1991) https://doi.org/10.1093/mnras/248.1.1.
The dynamical origin of the magnetic field distributions in compressible turbulence MNRAS248, 1–13 (1991) https://doi.org/10.1093/mnras/248.1.1
Reference 11
- Resolution
- verified exact
- doi, observed 2026-07-09T22:06:35.012965Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation b52f1e0c-9c74-4cb8-a23a-af7328000ba1 · outbound
This paper cites Thermodynamics and dynamics of two-dimensional systems with dipole-like repulsive interactions.
The dynamical origin of the magnetic field distributions in compressible turbulence Thermodynamics and dynamics of two-dimensional systems with dipole-like repulsive interactions
Reference 12
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-07-09T22:06:35.087299Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 0b6247cb-6060-4eaf-8882-39cfdfa594d0 · outbound
This paper cites The Density Probability Distribution in Compressible Isothermal Turbulence: Solenoidal versus Compressive Forcing.
The dynamical origin of the magnetic field distributions in compressible turbulence The Density Probability Distribution in Compressible Isothermal Turbulence: Solenoidal versus Compressive Forcing
Reference 13
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.063184Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 04981ea8-af69-456f-86c4-5d88ea23b21d · outbound
This paper cites Comparing the statistics of interstellar turbulence in simulations and observations: Solenoidal versus compressive turbulence forcing.
The dynamical origin of the magnetic field distributions in compressible turbulence Comparing the statistics of interstellar turbulence in simulations and observations: Solenoidal versus compressive turbulence forcing
Reference 14
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:34.999520Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 4be694ea-f276-46ed-a447-459c51787dd5 · outbound
This paper cites doi: 10.1017/cbo9781139170666.
The dynamical origin of the magnetic field distributions in compressible turbulence doi: 10.1017/cbo9781139170666
Reference 15
- Resolution
- verified exact
- doi, observed 2026-07-09T22:06:35.089504Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 50bada41-c9cb-4bdb-8321-f6210682fc3a · outbound
This paper cites A High Order Godunov Scheme with Constrained Transport and Adaptive Mesh Refinement for Astrophysical MHD.
The dynamical origin of the magnetic field distributions in compressible turbulence A High Order Godunov Scheme with Constrained Transport and Adaptive Mesh Refinement for Astrophysical MHD
Reference 16
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.112886Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 64902760-87d1-4be6-b738-f90ce51eef09 · outbound
This paper cites Fryxell, et al., Astrophys.
The dynamical origin of the magnetic field distributions in compressible turbulence Fryxell, et al., Astrophys
Reference 17
- Resolution
- verified exact
- doi, observed 2026-07-09T22:06:34.980843Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 763cda60-8c4c-4110-8972-d38d23fa1030 · outbound
This paper cites an unresolved cited work.
The dynamical origin of the magnetic field distributions in compressible turbulence Unresolved cited work
Reference 18
- Resolution
- unresolved
- raw_fallback, observed 2026-07-09T22:06:35.960873Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation c005e435-bf0b-43c5-88a1-fce27510b958 · outbound
This paper cites Physics of Fluids A , keywords =.
The dynamical origin of the magnetic field distributions in compressible turbulence Physics of Fluids A , keywords =
Reference 19
- Resolution
- verified exact
- doi, observed 2026-07-09T22:06:35.117655Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 30d6a119-3c9a-43b7-969d-43a27e01d88f · outbound
This paper cites Physical Processes in Star Formation.
The dynamical origin of the magnetic field distributions in compressible turbulence Physical Processes in Star Formation
Reference 20
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.065675Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation da08d3fc-d0a2-4a5f-a02d-86eb88a8875a · outbound
This paper cites Simulating the formation of molecular clouds. II. Rapid formation from turbulent initial conditions.
The dynamical origin of the magnetic field distributions in compressible turbulence Simulating the formation of molecular clouds. II. Rapid formation from turbulent initial conditions
Reference 21
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.098830Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 5a6a13ed-b960-42cc-a8b6-927c7697e958 · outbound
This paper cites Frontiers in Astronomy and Space Sciences , keywords =.
The dynamical origin of the magnetic field distributions in compressible turbulence Frontiers in Astronomy and Space Sciences , keywords =
Reference 22
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-07-09T22:06:35.094157Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 533cc63d-3133-44cd-aaf8-c2f71c2db916 · outbound
This paper cites Turbulent molecular clouds.
The dynamical origin of the magnetic field distributions in compressible turbulence Turbulent molecular clouds
Reference 23
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.078287Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 945514f7-ce28-4b93-8011-1fad4582bbcf · outbound
This paper cites A Model for (Non-Lognormal) Density Distributions in Isothermal Turbulence.
The dynamical origin of the magnetic field distributions in compressible turbulence A Model for (Non-Lognormal) Density Distributions in Isothermal Turbulence
Reference 24
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.084342Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 74381d18-8056-4fbe-b452-c970d621208e · outbound
This paper cites Time evolution of the galactic $B- \rho$ relation: the impact of the magnetic field morphology.
The dynamical origin of the magnetic field distributions in compressible turbulence Time evolution of the galactic $B- \rho$ relation: the impact of the magnetic field morphology
Reference 25
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.041033Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation ba96cc71-5974-4814-815b-18483b3ef373 · outbound
This paper cites Density Fluctuations in MHD Turbulence: Spectra, Intermittency and Topology.
The dynamical origin of the magnetic field distributions in compressible turbulence Density Fluctuations in MHD Turbulence: Spectra, Intermittency and Topology
Reference 26
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.043638Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 8be417ed-e409-4839-bcc8-d547f8eac378 · outbound
This paper cites , keywords =.
The dynamical origin of the magnetic field distributions in compressible turbulence , keywords =
Reference 27
- Resolution
- verified exact
- doi, observed 2026-07-09T22:06:35.036188Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation c9366782-a702-4a50-9d8c-cff8a1f6f5cd · outbound
This paper cites SHOCKFIND - An algorithm to identify magnetohydrodynamic shock waves in turbulent clouds.
The dynamical origin of the magnetic field distributions in compressible turbulence SHOCKFIND - An algorithm to identify magnetohydrodynamic shock waves in turbulent clouds
Reference 28
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.120659Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation f6f45353-8ae1-46ff-a0a6-68fd1de8c183 · outbound
This paper cites The Distribution of Pressures in a Supernova-Driven Interstellar Medium. I. Magnetized Medium.
The dynamical origin of the magnetic field distributions in compressible turbulence The Distribution of Pressures in a Supernova-Driven Interstellar Medium. I. Magnetized Medium
Reference 29
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.114659Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation d3a2863d-2a9b-4f8a-a185-8ca780d49885 · outbound
This paper cites Control of star formation by supersonic turbulence.
The dynamical origin of the magnetic field distributions in compressible turbulence Control of star formation by supersonic turbulence
Reference 30
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-07-09T22:06:35.120520Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation e0937af5-a175-4bb2-b531-f2d67e0316ba · outbound
This paper cites Incorporating Ambipolar and Ohmic Diffusion in the AMR MHD code RAMSES.
The dynamical origin of the magnetic field distributions in compressible turbulence Incorporating Ambipolar and Ohmic Diffusion in the AMR MHD code RAMSES
Reference 31
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.069332Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 3d18a0ea-2ba3-49cc-a6d6-44535cca8a85 · outbound
This paper cites , year = 1965, month = jun, volume =.
The dynamical origin of the magnetic field distributions in compressible turbulence , year = 1965, month = jun, volume =
Reference 32
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-07-09T22:06:35.959116Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 09dc6f34-be9a-4faf-a48b-b6221985cb00 · outbound
This paper cites A Markov model for non-lognormal density distributions in compressive isothermal turbulence.
The dynamical origin of the magnetic field distributions in compressible turbulence A Markov model for non-lognormal density distributions in compressive isothermal turbulence
Reference 33
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.123643Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 63779c71-99d2-4dde-ae78-5cbce6397dca · outbound
This paper cites keywords =.
The dynamical origin of the magnetic field distributions in compressible turbulence keywords =
Reference 34
- Resolution
- verified exact
- doi, observed 2026-07-09T22:06:35.029846Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 99886413-699c-442d-893d-9899d7db2584 · outbound
This paper cites Strong turbulence and magnetic coherent structures in the interstellar medium.
The dynamical origin of the magnetic field distributions in compressible turbulence Strong turbulence and magnetic coherent structures in the interstellar medium
Reference 35
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.104092Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation f61decd8-04fd-4b1b-a837-3599419aa910 · outbound
This paper cites Density probability distribution in one-dimensional polytropic gas dynamics.
The dynamical origin of the magnetic field distributions in compressible turbulence Density probability distribution in one-dimensional polytropic gas dynamics
Reference 36
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.054563Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 77bfd88e-3942-4596-8232-9843e47b725a · outbound
This paper cites Supersonic turbulence in the ISM: stellar extinction determinations as probes of the structure and dynamics of dark clouds.
The dynamical origin of the magnetic field distributions in compressible turbulence Supersonic turbulence in the ISM: stellar extinction determinations as probes of the structure and dynamics of dark clouds
Reference 37
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.127364Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation c770f38c-0df1-4441-a32e-de5aa1d3b1e4 · outbound
This paper cites The Star Formation Rate of Supersonic MHD Turbulence.
The dynamical origin of the magnetic field distributions in compressible turbulence The Star Formation Rate of Supersonic MHD Turbulence
Reference 38
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.097232Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation b88592f7-f397-473e-a66a-28fa203bd204 · outbound
This paper cites Magnetic fields in star formation: from clouds to cores.
The dynamical origin of the magnetic field distributions in compressible turbulence Magnetic fields in star formation: from clouds to cores
Reference 39
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-07-09T22:06:35.115711Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation fc1dc1b3-f2d8-4cab-ba26-b556d97fc9dd · outbound
This paper cites Density and Velocity Correlations in Isothermal Supersonic Turbulence.
The dynamical origin of the magnetic field distributions in compressible turbulence Density and Velocity Correlations in Isothermal Supersonic Turbulence
Reference 40
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.092167Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 0acf349a-62dd-4238-8e34-be5827a15319 · outbound
This paper cites Understanding Density Fluctuations in Supersonic, Isothermal Turbulence.
The dynamical origin of the magnetic field distributions in compressible turbulence Understanding Density Fluctuations in Supersonic, Isothermal Turbulence
Reference 41
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-07-09T22:06:35.105920Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 5b0d5229-61ef-42f9-bf19-e1fc57a224d7 · outbound
This paper cites Modeling Star Formation as a Markov Process in a Supersonic Gravoturbulent Medium.
The dynamical origin of the magnetic field distributions in compressible turbulence Modeling Star Formation as a Markov Process in a Supersonic Gravoturbulent Medium
Reference 42
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.111887Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 6d8c7d1d-5692-410c-896b-8da1a9400b70 · outbound
This paper cites Simulations of small-scale turbulent dynamo.
The dynamical origin of the magnetic field distributions in compressible turbulence Simulations of small-scale turbulent dynamo
Reference 43
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:34.984182Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation dbeedaf8-779e-4639-b11b-168f329ebca7 · outbound
This paper cites On the saturation mechanism of the fluctuation dynamo at ${\text{Pr}_\mathrm{M}} \ge 1$.
The dynamical origin of the magnetic field distributions in compressible turbulence On the saturation mechanism of the fluctuation dynamo at ${\text{Pr}_\mathrm{M}} \ge 1$
Reference 44
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-07-09T22:06:35.107102Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation ae1503be-4704-4171-9153-aff5efcc6f28 · outbound
This paper cites Saturation mechanism of the fluctuation dynamo in supersonic turbulent plasmas.
The dynamical origin of the magnetic field distributions in compressible turbulence Saturation mechanism of the fluctuation dynamo in supersonic turbulent plasmas
Reference 45
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-07-09T22:06:35.026905Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation c018ea53-d52f-4831-b6c5-18000f4bffa1 · outbound
This paper cites The distribution of shock waves in driven supersonic turbulence.
The dynamical origin of the magnetic field distributions in compressible turbulence The distribution of shock waves in driven supersonic turbulence
Reference 46
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.086910Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation aeb07dff-4bc2-44cd-842d-1129c5bcf80b · outbound
This paper cites The distribution of density in supersonic turbulence.
The dynamical origin of the magnetic field distributions in compressible turbulence The distribution of density in supersonic turbulence
Reference 47
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.109956Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 48898d65-055e-4c49-a3f9-f4647e97d757 · outbound
This paper cites Turbulent dynamo in the two-phase interstellar medium.
The dynamical origin of the magnetic field distributions in compressible turbulence Turbulent dynamo in the two-phase interstellar medium
Reference 48
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.117503Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 9b09c36e-1064-4e04-ab6b-fd3350ed21e3 · outbound
This paper cites Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES.
The dynamical origin of the magnetic field distributions in compressible turbulence Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES
Reference 49
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-07-09T22:06:35.083086Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 9c208256-470b-4eee-81aa-4ab87eedef70 · outbound
This paper cites Possible generalization of Boltzmann-Gibbs statistics , url =.
The dynamical origin of the magnetic field distributions in compressible turbulence Possible generalization of Boltzmann-Gibbs statistics , url =
Reference 50
- Resolution
- verified exact
- doi, observed 2026-07-09T22:06:35.023050Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 3cf8844c-e55f-44ae-bd25-a9913a1376a8 · outbound
This paper cites Magnetic Field - Gas Density Relation and Observational Implications Revisited.
The dynamical origin of the magnetic field distributions in compressible turbulence Magnetic Field - Gas Density Relation and Observational Implications Revisited
Reference 51
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T22:06:35.060439Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation bafd3227-057e-402d-8a63-e0daffb2651e · outbound
This paper cites biburl =.
The dynamical origin of the magnetic field distributions in compressible turbulence biburl =
Reference 52
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-07-09T22:06:35.956961Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 4aed0e07-0713-4d97-a36f-f74f2ce820a8 · outbound
This paper cites The Astrophysical Journal , keywords =.
The dynamical origin of the magnetic field distributions in compressible turbulence The Astrophysical Journal , keywords =
Reference 53
- Resolution
- verified exact
- doi, observed 2026-07-09T22:06:35.065510Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation ac87ef5b-7c23-46b7-9993-afebd821db74 · outbound
This paper cites On the relation between magnetic field strength and gas density in the interstellar medium: A multiscale analysis.
The dynamical origin of the magnetic field distributions in compressible turbulence On the relation between magnetic field strength and gas density in the interstellar medium: A multiscale analysis
Reference 54
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-07-09T22:06:35.075736Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Pith citing papers
No inbound Pith citation observations are available.