Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
MRI turbulence in accretion discs at large magnetic Prandtl numbers
As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2206.00497.
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 2026-08-18T06:34:40.430872+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-01T08:39:40.226035Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-11T17:11:06.961897Z
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 615e6c6b-257f-438b-b715-eb11b07e7d1c · inbound
Wave interference as the origin of the cyclic magnetorotational dynamo in accretion disks: insights from weakly nonlinear theory and local shearing box simulations cites this paper.
Wave interference as the origin of the cyclic magnetorotational dynamo in accretion disks: insights from weakly nonlinear theory and local shearing box simulations MRI turbulence in accretion discs at large magnetic Prandtl numbers
Reference 66
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T17:11:06.987225Z
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.
Observation 7c2bf4fd-92e6-4b15-bd85-d3b39073083a · inbound
Wave interference as the origin of the cyclic magnetorotational dynamo in accretion disks: insights from weakly nonlinear theory and local shearing box simulations cites this paper.
Wave interference as the origin of the cyclic magnetorotational dynamo in accretion disks: insights from weakly nonlinear theory and local shearing box simulations MRI turbulence in accretion discs at large magnetic Prandtl numbers
Reference 68
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T05:06:04.561602Z
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.
Observation 55e192b0-791e-4110-9405-74f389bd6f36 · inbound
Transport of angular momentum and chemical elements by the MRI dynamo in stellar radiative zones cites this paper.
Transport of angular momentum and chemical elements by the MRI dynamo in stellar radiative zones MRI turbulence in accretion discs at large magnetic Prandtl numbers
Reference 1
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T08:39:40.226035Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.