Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Tidal dissipation due to inertial waves can explain the circularization periods of solar-type binaries
As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2203.03950.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-03T12:59:20.081045Z
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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- malformed identifier0
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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 bdfd9db6-d723-49e4-b252-c9093bad4559 · 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 Tidal dissipation due to inertial waves can explain the circularization periods of solar-type binaries
Reference 39
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T12:59:20.081045Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.