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Paper Citation Record · LEDGER

The dynamical origin of the magnetic field distributions in compressible turbulence

As of 20 August 2026, this Paper Citation Record lists 54 of 54 outbound references and 0 inbound Pith citation observations for arXiv:2607.07004.

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pith.paper-citation-record.v1
2607.07004 v1

Coverage vector

measured 54 of 54 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

measured 54 of 54 standing notices

One-hop event checks from named stored sources.

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measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

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measured 0 of 1 external citation measurements

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Source: cited_works

Reference resolution

54 of 54 outbound references displayed

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  • verified fuzzy2
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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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The dynamical origin of the magnetic field distributions in compressible turbulence Unresolved cited work

Reference 18

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Observation c005e435-bf0b-43c5-88a1-fce27510b958 · outbound

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The dynamical origin of the magnetic field distributions in compressible turbulence Physics of Fluids A , keywords =

Reference 19

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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

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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

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The dynamical origin of the magnetic field distributions in compressible turbulence Frontiers in Astronomy and Space Sciences , keywords =

Reference 22

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The dynamical origin of the magnetic field distributions in compressible turbulence Turbulent molecular clouds

Reference 23

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The dynamical origin of the magnetic field distributions in compressible turbulence A Model for (Non-Lognormal) Density Distributions in Isothermal Turbulence

Reference 24

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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

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The dynamical origin of the magnetic field distributions in compressible turbulence Density Fluctuations in MHD Turbulence: Spectra, Intermittency and Topology

Reference 26

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The dynamical origin of the magnetic field distributions in compressible turbulence , keywords =

Reference 27

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The dynamical origin of the magnetic field distributions in compressible turbulence SHOCKFIND - An algorithm to identify magnetohydrodynamic shock waves in turbulent clouds

Reference 28

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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

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The dynamical origin of the magnetic field distributions in compressible turbulence Control of star formation by supersonic turbulence

Reference 30

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The dynamical origin of the magnetic field distributions in compressible turbulence Incorporating Ambipolar and Ohmic Diffusion in the AMR MHD code RAMSES

Reference 31

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The dynamical origin of the magnetic field distributions in compressible turbulence , year = 1965, month = jun, volume =

Reference 32

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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

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The dynamical origin of the magnetic field distributions in compressible turbulence keywords =

Reference 34

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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

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verified exact
local_arxiv, observed 2026-07-09T22:06:35.104092Z

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No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:8ac7a4c3317da9e8fbea9a844648d0afee669fbc90f7999c890443dc103609f2

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 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:217f4ab04b41ac4f544c20eb1f5dd4304da2ebc4798a30b445cee4ecd0d77973

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

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verified exact
local_arxiv, observed 2026-07-09T22:06:35.127364Z

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No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:05014bdea7d78ca4a03893678dbca84b86bb2a329e3a511b7a88660bc8055f47

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

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No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:9cebbb45f2efba3df7d35382879e60f15d17b929e8b6769bf4523e1678a9c101

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
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local_arxiv, observed 2026-07-09T22:06:35.115711Z

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No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-09T21:57:49.151864Z digest=sha256:9b75374afa2bf7105c0a544a7ff8902bb89f384e0e5946e3309102d892edcc8d

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 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:9268ef7e913b1e550ddb8c8e977d845b8f4070ae034055eafb1e69f69591436b

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
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local_arxiv, observed 2026-07-09T22:06:35.105920Z

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No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:be8b0b9ae04a2051f7d40f65bb57372aeb25e71ac240ac253d9e8b96ac1090c2

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

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No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:5a9f03dc69fe62e70c8e784f4d033ba525ce1c4b9a174e35bcbfe50ce72ffa9d

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

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No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:239cbfc87f4bbc8aa2d3b3baa8fe4a4ab084c5a0b3228e879d5bba84ca7ad6ae

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

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local_arxiv, observed 2026-07-09T22:06:35.107102Z

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No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:b2e64a598af09e94756ceaa80687c6f16fac8e987cbaee5cb0dd3ab7494c0b6d

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
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local_arxiv, observed 2026-07-09T22:06:35.026905Z

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No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:c225b4fe077f7300c34d85dcf3262ed74a2a2f5d1ba560826082f71160f2d5ab

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

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No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-09T21:57:49.151864Z digest=sha256:b71c1df994dbb61b864e8905306e823f459ab1b84000c1ffee948c5b72066943

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 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:0c45e8d868e5915cbb0570fab7dabd5a4d8be893ce97dc6c70a2d1df5fb7be2d

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 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:18d754a68fb9c0690b4eb050d29a9a5bfe1465b7d2ff2097c28c9a7bbda3e665

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
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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 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:694e349c5ab26e859e71844ed1bbaaa7f8d217313150e31b8cd47959222cca0c

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

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No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-09T21:57:49.151864Z digest=sha256:13a9e7d633b2826ea1838efe38fd50cce5b2a0d0d630a9e6e0ca82ef17fc9aae

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

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No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:094e4375f6a6a4d462ca054ea138440d03f8a1aacdc7afed8f07ceef75c247b6

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 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-09T21:57:49.151864Z digest=sha256:6e723405b4e8446e83c513d1312a836a8dbed97bd8bcd5be8a984f2d773199e5

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 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-09T21:57:49.151864Z digest=sha256:9f9a88e3e1c28c7e47eb15cbc708e7ec4e71c1515340e6d9f98b4b3339cf2d14

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

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No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:50e9802cc10c5e11564227750e78d4ad8f85824372fe960a206d3a59b96326af

Pith citing papers

No inbound Pith citation observations are available.