Paper Citation Record · LEDGER

The Axisymmetric Pulsar Magnetosphere

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:astro-ph/9903049.

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

pith.paper-citation-record.v1
astro-ph/9903049 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T12:52:22.633985Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-28T22:02:41.342927Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
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 553cb630-42fb-46fc-bafd-94d6552b0c3e · inbound

Inductive acceleration of ions in Poynting-flux dominated outflows cites this paper.

Inductive acceleration of ions in Poynting-flux dominated outflows The Axisymmetric Pulsar Magnetosphere

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-14T12:52:22.633985Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8e56fa5e-6ce4-487d-8854-0a210049b5dc · inbound

General-relativistic resistive-magnetohydrodynamics simulations of self-consistent magnetized rotating neutron stars cites this paper.

General-relativistic resistive-magnetohydrodynamics simulations of self-consistent magnetized rotating neutron stars The Axisymmetric Pulsar Magnetosphere

Reference 14

Resolution: verified exact; arxiv_id, observed 2026-05-09T04:41:38.050084Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 158f9426-f562-4da3-a27c-01a283d7b726 · inbound

Tearing of charged current layers cites this paper.

Tearing of charged current layers The Axisymmetric Pulsar Magnetosphere

Reference 21

Resolution: verified exact; arxiv_id, observed 2026-05-11T21:11:19.823100Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 731e444e-8c91-46e9-9768-1d73cc66280f · inbound

A synchro-curvature treatment of gamma-ray luminosity trends in pulsars cites this paper.

A synchro-curvature treatment of gamma-ray luminosity trends in pulsars The Axisymmetric Pulsar Magnetosphere

Reference 23

Resolution: verified exact; local_arxiv, observed 2026-06-28T22:02:41.346819Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.