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Paper Citation Record · LEDGER

The Sun's Global Photospheric and Coronal Magnetic Fields: Observations and Models

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1211.6545.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
1211.6545 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T22:10:01.811714Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: cited_works

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 f999ebf5-ee23-4a6f-bea3-aedf161fd542 · inbound

Solar Cycle Variation of the Distribution of Photospheric Magnetic Flux Features cites this paper.

Solar Cycle Variation of the Distribution of Photospheric Magnetic Flux Features The Sun's Global Photospheric and Coronal Magnetic Fields: Observations and Models

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-01T22:10:01.811714Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T22:10:01.811714Z digest=sha256:dea12a17c9a7716b06a5c32e543c2c2092f657e64c73228bb9d37640c34fdd92

Observation 68baca47-2ae8-42aa-baa2-f05d21e9661b · 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 The Sun's Global Photospheric and Coronal Magnetic Fields: Observations and Models

Reference 78

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:43.856157Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:43.856157Z digest=sha256:fb1ddddaf319a1cbabf6dba3b961828f4ae969d80ab74187db21925564df8513