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Paper Citation Record · LEDGER

Global-Scale Turbulent Convection and Magnetic Dynamo Action in the Solar Envelope

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0610073.

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

pith.paper-citation-record.v1
astro-ph/0610073 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 2026-08-07T06:34:17.273281+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T21:17:24.136496Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-20T02:47:58.821835Z

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 b7b118e8-2f39-4aea-995c-c76dc5f3944d · inbound

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

Connecting mean-field theory with dynamo simulations Global-Scale Turbulent Convection and Magnetic Dynamo Action in the Solar Envelope

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-06T21:17:24.136496Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T21:17:24.136496Z digest=sha256:7cdee662db5d9389731e8b5b456078690d6f36706efaa701439a64696e6b15f9

Observation 3273b6a5-a830-427c-87e0-5aff3c175f41 · 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 Global-Scale Turbulent Convection and Magnetic Dynamo Action in the Solar Envelope

Reference 134

Resolution
verified exact
local_arxiv, observed 2026-05-20T02:47:58.824229Z

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=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:7923ea4b2bfa03deb5ef94a2a4b670cea0baceb79b10ca0a4bc4bcc083e5912e