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Paper Citation Record · LEDGER

Comparing the statistics of interstellar turbulence in simulations and observations: Solenoidal versus compressive turbulence forcing

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:0905.1060.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
0905.1060 v4

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measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 11 of 11 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 11 of 11 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T11:31:37.861325Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-07-09T22:06:34.996566Z

Reference resolution

0 of 0 outbound references displayed

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External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 2423148c-ab11-49a1-b5d8-982d26d86b61 · inbound

The Formation of Globular Clusters cites this paper.

The Formation of Globular Clusters Comparing the statistics of interstellar turbulence in simulations and observations: Solenoidal versus compressive turbulence forcing

Reference 89

Resolution
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no resolver link, observed 2026-08-10T13:20:41.211891Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation e1d4fc5c-6111-44fa-837e-1e1a66e9eed7 · inbound

Local relaxation and scale-dependent alignment in compressible, magnetized turbulence cites this paper.

Local relaxation and scale-dependent alignment in compressible, magnetized turbulence Comparing the statistics of interstellar turbulence in simulations and observations: Solenoidal versus compressive turbulence forcing

Reference 33

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malformed identifier
no resolver link, observed 2026-08-16T11:31:37.861325Z

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Observation 17030dda-f02f-4a1c-9f5e-127638419f60 · inbound

Cosmic ray and plasma coupling for isothermal supersonic turbulence in the magnetized interstellar medium cites this paper.

Cosmic ray and plasma coupling for isothermal supersonic turbulence in the magnetized interstellar medium Comparing the statistics of interstellar turbulence in simulations and observations: Solenoidal versus compressive turbulence forcing

Reference 41

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unresolved
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Observation e9fb4146-fd1d-4340-b240-c15d03c284e3 · inbound

Grain alignment and dust evolution physics with polarisation (GRADE-POL). II. On the physical basis of Serkowski and super-Serkowski polarisation spectra cites this paper.

Grain alignment and dust evolution physics with polarisation (GRADE-POL). II. On the physical basis of Serkowski and super-Serkowski polarisation spectra Comparing the statistics of interstellar turbulence in simulations and observations: Solenoidal versus compressive turbulence forcing

Reference 163

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verified exact
local_arxiv, observed 2026-06-27T06:50:39.954205Z

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source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:ccf986e4423fef985884d1ee9b428c3f97cc16dcd318d32581284f8ec2cb6a2f

Observation 0955f660-aeeb-4db3-955f-409ba338e3fd · inbound

The evolution of the galaxy gas-phase mass-metallicity relation from $z=15$ to $z=0$ in the COLIBRE cosmological simulations cites this paper.

The evolution of the galaxy gas-phase mass-metallicity relation from $z=15$ to $z=0$ in the COLIBRE cosmological simulations Comparing the statistics of interstellar turbulence in simulations and observations: Solenoidal versus compressive turbulence forcing

Reference 18

Resolution
verified exact
local_arxiv, observed 2026-06-25T19:58:18.746284Z

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.

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Observation 5d788450-fc6f-4e9a-b4cf-a6cbb7c5c5d0 · inbound

Kolmogorov turbulence across multi-fractal gas in Polaris Flare cites this paper.

Kolmogorov turbulence across multi-fractal gas in Polaris Flare Comparing the statistics of interstellar turbulence in simulations and observations: Solenoidal versus compressive turbulence forcing

Reference 12

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verified exact
local_arxiv, observed 2026-07-02T09:06:48.271724Z

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.

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Observation 7ee09783-d132-4570-bb3c-0102487b494d · inbound

Jet--ISM Interactions in Gaseous Disks: Simulating Kinetic Feedback in the Radio Galaxy 3C 326 N cites this paper.

Jet--ISM Interactions in Gaseous Disks: Simulating Kinetic Feedback in the Radio Galaxy 3C 326 N Comparing the statistics of interstellar turbulence in simulations and observations: Solenoidal versus compressive turbulence forcing

Reference 64

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation dc5a35c1-78ae-4b18-aeba-3dad4a57d7d3 · inbound

ALMA observations of Magnetic Fields in the Massive Star-forming Region IRAS 18360-0537 cites this paper.

ALMA observations of Magnetic Fields in the Massive Star-forming Region IRAS 18360-0537 Comparing the statistics of interstellar turbulence in simulations and observations: Solenoidal versus compressive turbulence forcing

Reference 172

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 04981ea8-af69-456f-86c4-5d88ea23b21d · inbound

The dynamical origin of the magnetic field distributions in compressible turbulence cites this paper.

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.

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Observation 7ff14c3f-f180-42ed-bc91-8496e76f8daf · inbound

The first three-dimensional map of thermal phases in the local interstellar medium cites this paper.

The first three-dimensional map of thermal phases in the local interstellar medium Comparing the statistics of interstellar turbulence in simulations and observations: Solenoidal versus compressive turbulence forcing

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-01T23:40:46.115651Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation cce9fe80-f0a7-42ce-985e-a33d79df5f05 · inbound

Bipolar HII regions Produced by Cloud-Cloud Collisions cites this paper.

Bipolar HII regions Produced by Cloud-Cloud Collisions Comparing the statistics of interstellar turbulence in simulations and observations: Solenoidal versus compressive turbulence forcing

Reference 35

Resolution
unresolved
no resolver link, observed 2026-07-31T15:39:28.059161Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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