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Paper Citation Record · LEDGER

Generalized Squashing Factors for Covariant Description of Magnetic Connectivity in the Solar Corona

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0703671.

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

pith.paper-citation-record.v1
astro-ph/0703671 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 2026-08-17T06:30:58.91139+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T15:06:43.732247Z

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 6e64d3cf-db1b-442f-8c50-f89fc468a4b3 · inbound

Coronal dimmings and what they tell us about solar and stellar coronal mass ejections cites this paper.

Coronal dimmings and what they tell us about solar and stellar coronal mass ejections Generalized Squashing Factors for Covariant Description of Magnetic Connectivity in the Solar Corona

Reference 284

Resolution
unresolved
no resolver link, observed 2026-08-07T14:22:02.607042Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T14:22:02.607042Z digest=sha256:dbc98816e9d0cde95e01d2f6049a110d9f77a347306c6e5ef21b7368cf729d45

Observation 9df3a436-7e30-4749-9ab3-a680017c70bd · inbound

The location and propagation of fine structures in type II solar radio bursts cites this paper.

The location and propagation of fine structures in type II solar radio bursts Generalized Squashing Factors for Covariant Description of Magnetic Connectivity in the Solar Corona

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-15T15:06:43.732247Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:06:43.732247Z digest=sha256:691de45e6dbd2c0903a8e6bae639fdbfc644df207378ff36a7143c8e12a3e500