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Paper Citation Record · LEDGER

Simulating the Solar Corona with Multiple Solar Photospheric Magnetic Maps during the 8 April 2024 Total Solar Eclipse

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2503.10974.

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

pith.paper-citation-record.v1
2503.10974 v2

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 2026-08-07T06:34:17.273281+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T11:24:27.888594Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

0
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation b7aaa0e2-e740-4f2d-b848-3f53afb4b55c · inbound

The Role of Far-side Magnetic Structures in Modeling 2024 Solar Eclipse cites this paper.

The Role of Far-side Magnetic Structures in Modeling 2024 Solar Eclipse Simulating the Solar Corona with Multiple Solar Photospheric Magnetic Maps during the 8 April 2024 Total Solar Eclipse

Reference 30

Resolution
unresolved
no resolver link, observed 2026-08-05T11:24:27.888594Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T11:24:27.888594Z digest=sha256:49acf901005ab5bff8ce8f957c6655c28842cccea10e560b51238fda9a6ee1f2

Observation 416334f1-8914-452b-804a-19bdd542a80a · inbound

A Non-Spherical Model for the Solar Coronal Magnetic Field cites this paper.

A Non-Spherical Model for the Solar Coronal Magnetic Field Simulating the Solar Corona with Multiple Solar Photospheric Magnetic Maps during the 8 April 2024 Total Solar Eclipse

Reference 34

Resolution
verified exact
local_arxiv, observed 2026-08-02T17:03:25.427329Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-08-02T17:00:18.492316Z digest=sha256:3b06a8886ed507fa2f5cacada747961e9f486c44ac00f1d33908de675d6e52f0