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Paper Citation Record · LEDGER

Three-dimensional modeling of the Ca II H&K lines in the solar atmosphere

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:1712.01045.

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

pith.paper-citation-record.v1
1712.01045 v1

Coverage vector

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 2026-08-17T06:30:58.91139+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T04:19:29.170180Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-11T04:27:48.151216Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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Outbound references

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Pith citing papers

Observation e56f86a3-2e11-499e-b2ef-e32cb4dfd4c3 · inbound

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet cites this paper.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Three-dimensional modeling of the Ca II H&K lines in the solar atmosphere

Reference 22

Resolution
verified exact
local_arxiv, observed 2026-07-11T04:27:48.154879Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:bf0f84bd898adfd1633b49d23fe65cb2cbc0f22141c0725ffd3b9d7eb3a002b2