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Paper Citation Record · LEDGER

Helicity Balance and Steady-State Strength of the Dynamo Generated Galactic Magnetic Field

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/0205266.

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

pith.paper-citation-record.v1
astro-ph/0205266 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T19:47:10.253020Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-10T05:30:23.456663Z

Reference resolution

0 of 0 outbound references displayed

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

External citation measurements

32
pith, observed 2026-08-10T05:30:23.456663Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation edee4fd6-c5db-4da9-9ad5-41c9ca4e5989 · inbound

Forecast of solar activity based on mean-field dynamo model and neural network cites this paper.

Forecast of solar activity based on mean-field dynamo model and neural network Helicity Balance and Steady-State Strength of the Dynamo Generated Galactic Magnetic Field

Reference 27

Resolution
unresolved
no resolver link, observed 2026-08-12T19:47:10.253020Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-12T19:47:10.253020Z digest=sha256:c1140e1282e6512132ec66c51ce0622b9a4416add0d36081b652f7c2587ed77d

Observation 05cba9f0-78cb-4761-95a5-ac53e2ff01f2 · inbound

Magnetic helicity fluxes in dynamos from rotating inhomogeneous turbulence cites this paper.

Magnetic helicity fluxes in dynamos from rotating inhomogeneous turbulence Helicity Balance and Steady-State Strength of the Dynamo Generated Galactic Magnetic Field

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-11T05:32:32.511187Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T05:32:32.511187Z digest=sha256:577c6e08c7007001352f31d9904492da617e09e4afea94273c7a1677979dfe6d

Observation 62c66feb-93f8-479b-afe8-8f01792ac3e6 · inbound

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

Connecting mean-field theory with dynamo simulations Helicity Balance and Steady-State Strength of the Dynamo Generated Galactic Magnetic Field

Reference 192

Resolution
verified exact
local_arxiv, observed 2026-08-06T21:17:54.537713Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=arxiv_source observed=2026-08-06T21:17:40.179545Z digest=sha256:4b2ac0e3cbbe46887b4f0fd81f23bfaa1d534aac4e4f1be3d5d7832aadb7ec75