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Paper Citation Record · LEDGER

Numerical Simulations of MHD Turbulence in Accretion Disks

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0203353.

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

pith.paper-citation-record.v1
astro-ph/0203353 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T21:12:50.730972Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-15T18:46:28.687771Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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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 dbbeada1-5eda-48eb-bce5-0d63074ed1bd · inbound

AGN star dynamics under the Influence of Outflow-Ambient Interactions cites this paper.

AGN star dynamics under the Influence of Outflow-Ambient Interactions Numerical Simulations of MHD Turbulence in Accretion Disks

Reference 3

Resolution
unresolved
no resolver link, observed 2026-08-15T21:12:50.730972Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T21:12:50.730972Z digest=sha256:85d9dff024bc3e8706a99539703996f35c60a9ba1039351bc4b3ee2c6da63e3b

Observation ca17cfa6-c774-4a6f-aebe-39a13f8b1c96 · inbound

Revisiting the Perseus Cluster III: Role of Aspherical Explosions on its Chemical Composition and Extension to Metal-Poor Stars and Galaxies cites this paper.

Revisiting the Perseus Cluster III: Role of Aspherical Explosions on its Chemical Composition and Extension to Metal-Poor Stars and Galaxies Numerical Simulations of MHD Turbulence in Accretion Disks

Reference 1

Resolution
verified exact
local_arxiv, observed 2026-05-15T18:46:28.694305Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=pdf_text observed=2026-07-11T11:50:26.030339Z digest=sha256:0cbb5e66df8b17e4a4806f521fe2a6e4f7543d18283388779775a8c72b3e15cf