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Paper Citation Record · LEDGER

Grand Minima and Equatorward Propagation in a Cycling Stellar Convective Dynamo

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1410.6547.

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

pith.paper-citation-record.v1
1410.6547 v3

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 2026-08-06T21:17:16.320735Z

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

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  • verified fuzzy0
  • unresolved0
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  • malformed identifier0
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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 6b4f2fc6-eb62-4452-a818-6d57e1c244a8 · inbound

Connecting mean-field theory with dynamo simulations cites this paper.

Connecting mean-field theory with dynamo simulations Grand Minima and Equatorward Propagation in a Cycling Stellar Convective Dynamo

Reference 2

Resolution
unresolved
no resolver link, observed 2026-08-06T21:17:16.320735Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T21:17:16.320735Z digest=sha256:469d594452b6ed9a5c2a9880b10bebffe03620e6fd6d30e96da0421b13835c10

Observation 8b0407e9-7875-46db-9936-74c068327869 · 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 Grand Minima and Equatorward Propagation in a Cycling Stellar Convective Dynamo

Reference 107

Resolution
unresolved
no resolver link, observed 2026-08-01T19:35:46.827622Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:35:46.827622Z digest=sha256:fe4fbc58caf7022f58304fff82ab594e770a081f496087612ecd913c711b8a3f