Paper Citation Record · LEDGER

Full--Sphere Simulations of a Circulation--Dominated Solar Dynamo: Exploring the Parity Issue

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0405027.

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

pith.paper-citation-record.v1
astro-ph/0405027 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 2026-08-06T21:17:25.974983Z

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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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 6e5e8fb0-647e-4b1e-a0e4-3e1a5243ae2e · inbound

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

Connecting mean-field theory with dynamo simulations Full--Sphere Simulations of a Circulation--Dominated Solar Dynamo: Exploring the Parity Issue

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-06T21:17:25.974983Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bd047f58-5721-4ecd-82bc-7a4793dba327 · 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 Full--Sphere Simulations of a Circulation--Dominated Solar Dynamo: Exploring the Parity Issue

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-01T19:35:38.505521Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.