Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The magnetic field vector of the Sun-as-a-star
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1603.09226.
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 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-01T19:35:43.350693Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
61
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 6d871e55-7be6-4042-ab0c-db4b81d5bdec · inbound
Upper Limits on Planet-Induced GHz Radio Emission from Inactive M Dwarfs cites this paper.
Upper Limits on Planet-Induced GHz Radio Emission from Inactive M Dwarfs The magnetic field vector of the Sun-as-a-star
Reference 128
- Resolution
- verified exact
- local_arxiv, observed 2026-06-26T16:39:35.975013Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation a0161a16-d28b-421f-8dec-cf0b0401a841 · inbound
Magnetic activity in cool stars: manifestations and relevance to exoplanets cites this paper.
Magnetic activity in cool stars: manifestations and relevance to exoplanets The magnetic field vector of the Sun-as-a-star
Reference 131
- Resolution
- verified exact
- local_arxiv, observed 2026-07-01T03:05:19.505381Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation aa94fb5f-2350-427d-9c0a-6a3988b2edad · inbound
Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models cites this paper.
Constraining the radial decay timescale of solar surface magnetic field through a comparative study of data-assimilative 2D surface flux transport and 3D dynamo models The magnetic field vector of the Sun-as-a-star
Reference 72
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T19:35:43.350693Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.