Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Radiative MHD simulation of sunspot structure
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:0808.3294.
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 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T21:17:49.462365Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-03T05:27:39.498216Z
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 9c07f22e-9d51-4b3f-a8a9-9ebbb62d98a2 · inbound
Connecting mean-field theory with dynamo simulations cites this paper.
Connecting mean-field theory with dynamo simulations Radiative MHD simulation of sunspot structure
Reference 268
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T21:17:49.462365Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 699329c9-51a1-4675-b9d3-3f3452b3faf3 · inbound
Research Progress on Solar Small-Scale Dynamo cites this paper.
Research Progress on Solar Small-Scale Dynamo Radiative MHD simulation of sunspot structure
Reference 246
- Resolution
- verified exact
- local_arxiv, observed 2026-07-03T05:27:39.499340Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation c19df0c1-ecab-40b6-8136-8262dd8bd0df · inbound
Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models cites this paper.
Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models Radiative MHD simulation of sunspot structure
Reference 73
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T19:35:43.463187Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.