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Paper Citation Record · LEDGER

The crucial role of surface magnetic fields for the solar dynamo

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1503.08469.

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

pith.paper-citation-record.v1
1503.08469 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 2026-08-01T19:35:39.202865Z

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

189
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 054f6faa-70b2-44d0-9e4d-814df2209235 · inbound

Towards inertial-mode helioseismology: Direct sensing of solar rotation at 75 deg latitude and 0.8 Rsun cites this paper.

Towards inertial-mode helioseismology: Direct sensing of solar rotation at 75 deg latitude and 0.8 Rsun The crucial role of surface magnetic fields for the solar dynamo

Reference 146

Resolution
metadata mismatch
local_arxiv, observed 2026-05-20T02:47:58.700380Z

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.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:5dd5ec770c724b6103bf6d15db834b9137359cdb2657d1e4a3653152459fd7bb

Observation 39da63cd-16f4-4a45-bcae-fe03518ed245 · 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 crucial role of surface magnetic fields for the solar dynamo

Reference 29

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:39.202865Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:39.202865Z digest=sha256:5f48861e7052c6f938c0e8505c7d1c154add94fb206a0532bb75a89ec8f04e1e