Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Magnetic Flux Transport at the Solar Surface
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1408.3186.
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 2026-08-06T21:17:34.681980Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-03T05:27:39.372619Z
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 c336e53d-00c1-4b8f-9f5a-d103ed3a381e · inbound
Connecting mean-field theory with dynamo simulations cites this paper.
Connecting mean-field theory with dynamo simulations Magnetic Flux Transport at the Solar Surface
Reference 145
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T21:17:34.681980Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 66274b3f-e130-4dd1-8119-c3a55844717d · inbound
Research Progress on Solar Small-Scale Dynamo cites this paper.
Research Progress on Solar Small-Scale Dynamo Magnetic Flux Transport at the Solar Surface
Reference 236
- Resolution
- verified exact
- local_arxiv, observed 2026-07-03T05:27:39.373904Z
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 91e78e7e-fa4d-47e0-aff6-b3d0950f789a · 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 Magnetic Flux Transport at the Solar Surface
Reference 46
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T19:35:40.689880Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.