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Paper Citation Record · LEDGER

Theory of solar oscillations in the inertial frequency range: Linear modes of the convection zone

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2203.04442.

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pith.paper-citation-record.v1
2203.04442 v1

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measured 0 of 0 reference resolution

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Source: paper_references, paper_reference_links

measured 1 of 1 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T12:59:15.612354Z

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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Pith citing papers

Observation 97251018-b1d1-45fe-a655-2748f2b2d833 · 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 Theory of solar oscillations in the inertial frequency range: Linear modes of the convection zone

Reference 7

Resolution
unresolved
no resolver link, observed 2026-08-03T12:59:15.612354Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-03T12:59:15.612354Z digest=sha256:fe1d6501feb3523248e37377c2fd41b83f5a427c266c70cd2dc0d23e9cb63b38