Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Cosmic ray diffusion in magnetic fields amplified by nonlinear turbulent dynamo
As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2406.03542.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T21:29:05.925755Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
0
arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation a1e22e89-76b9-4f4d-b32a-b8c28ee340d3 · inbound
Anisotropic diffusion of high-energy cosmic rays in magnetohydrodynamic turbulence cites this paper.
Anisotropic diffusion of high-energy cosmic rays in magnetohydrodynamic turbulence Cosmic ray diffusion in magnetic fields amplified by nonlinear turbulent dynamo
Reference 86
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T21:29:05.925755Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 059f3c49-cf25-46f5-9225-4613742c36ea · inbound
Studying the mirror acceleration via kinetic simulations of relativistic plasma turbulence cites this paper.
Studying the mirror acceleration via kinetic simulations of relativistic plasma turbulence Cosmic ray diffusion in magnetic fields amplified by nonlinear turbulent dynamo
Reference 42
- Resolution
- verified exact
- arxiv_id, observed 2026-05-09T02:33:42.986026Z
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 1a22587d-4a3e-4190-890d-705a00b32f72 · inbound
Clumps in a Cocoon: Geometry and Mixing Set the Universal X-ray to H$\alpha$ Surface Brightness Ratio cites this paper.
Clumps in a Cocoon: Geometry and Mixing Set the Universal X-ray to H$\alpha$ Surface Brightness Ratio Cosmic ray diffusion in magnetic fields amplified by nonlinear turbulent dynamo
Reference 103
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-06-27T22:01:21.588925Z
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.