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Paper Citation Record · LEDGER

Saturation mechanism of the fluctuation dynamo in supersonic turbulent plasmas

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2109.11698.

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

pith.paper-citation-record.v1
2109.11698 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 2026-08-23T06:30:58.430688+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

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

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-09T22:06:35.024559Z

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 694f4c73-cf14-4ef5-b22c-bd48502a7893 · 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 Saturation mechanism of the fluctuation dynamo in supersonic turbulent plasmas

Reference 78

Resolution
metadata mismatch
local_arxiv, observed 2026-07-08T09:14:46.945402Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:8194f3b827b0c7705de2278b4b08a4d4c49591f15fcf303a17b9f98e376bafb1

Observation ae1503be-4704-4171-9153-aff5efcc6f28 · 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 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 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:e3423457885198952e04722fe83dca7b49a2a23df6fa7e7bcf4c14ec4a85d48e