Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
MHD simulations of the magnetorotational instability in a shearing box with zero net flux. II. The effect of transport coefficients
As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:0705.3622.
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 2026-08-21T06:32:19.484+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-01T08:39:44.941348Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-11T17:11:06.296256Z
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 706854f3-a3ea-42d6-81ea-3291980b2e07 · 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 MHD simulations of the magnetorotational instability in a shearing box with zero net flux. II. The effect of transport coefficients
Reference 23
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T17:03:57.719103Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation eb23726e-ad23-492e-8919-ddecf2ad1273 · 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 MHD simulations of the magnetorotational instability in a shearing box with zero net flux. II. The effect of transport coefficients
Reference 22
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T17:03:57.719103Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation e692d9c5-ee03-4e9f-89ba-45e44bc9c503 · 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 MHD simulations of the magnetorotational instability in a shearing box with zero net flux. II. The effect of transport coefficients
Reference 34
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T08:39:44.941348Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.