Paper Citation Record · LEDGER

On the saturation mechanism of the fluctuation dynamo at ${\text{Pr}_\mathrm{M}} \ge 1$

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2003.07997.

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

pith.paper-citation-record.v1
2003.07997 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

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

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-09T22:06:35.105505Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

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 c77e4b82-e322-4d59-91a7-a470a45176ef · inbound

The universal growth of magnetic energy during the nonlinear phase of subsonic and supersonic small-scale dynamos cites this paper.

The universal growth of magnetic energy during the nonlinear phase of subsonic and supersonic small-scale dynamos On the saturation mechanism of the fluctuation dynamo at ${\text{Pr}_\mathrm{M}} \ge 1$

Reference 44

Resolution: verified exact; arxiv_id, observed 2026-05-18T18:21:43.695711Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 133b1028-f12d-416b-ab2d-1b800614a6e6 · inbound

Understanding the non-Gaussian nature of Galactic foreground emissions towards small scales cites this paper.

Understanding the non-Gaussian nature of Galactic foreground emissions towards small scales On the saturation mechanism of the fluctuation dynamo at ${\text{Pr}_\mathrm{M}} \ge 1$

Reference 49

Resolution: verified exact; arxiv_id, observed 2026-07-04T09:39:46.226801Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation ba41c5f0-9be9-46dd-9b24-1682a98f9964 · inbound

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM cites this paper.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM On the saturation mechanism of the fluctuation dynamo at ${\text{Pr}_\mathrm{M}} \ge 1$

Reference 76

Resolution: metadata mismatch; local_arxiv, observed 2026-07-08T09:14:46.928540Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation dbeedaf8-779e-4639-b11b-168f329ebca7 · 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 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 2026-08-19T06:32:44.657259+00:00.