Pith. sign in

Paper Citation Record · LEDGER

30 to 100-kG magnetic fields in the cores of red giant stars

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2208.09487.

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

pith.paper-citation-record.v1
2208.09487 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 2026-08-10T06:31:04.303077+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T12:59:21.335070Z

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

  • 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 12c88394-566f-4576-9c38-f1b43590d9ce · inbound

Transport of angular momentum and chemical elements by the MRI dynamo in stellar radiative zones cites this paper.

Transport of angular momentum and chemical elements by the MRI dynamo in stellar radiative zones 30 to 100-kG magnetic fields in the cores of red giant stars

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-01T08:39:48.501152Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T08:39:48.501152Z digest=sha256:761b08f3df5fea01fc6d2f7075fa3d679a6359585ab43f18fd07d04f341187c8

Observation 2414940f-6e15-4c75-8a2e-380e64df4608 · inbound

Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations cites this paper.

Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations 30 to 100-kG magnetic fields in the cores of red giant stars

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-03T12:59:21.335070Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-03T12:59:21.335070Z digest=sha256:9d430b2163a0d2579d880ae29bdef3dd6f585589f737ea494288ab5e13b4c1c3