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Paper Citation Record · LEDGER

Modeling the Saturation of the Bell Instability using Hybrid Simulations

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2210.08072.

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

pith.paper-citation-record.v1
2210.08072 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T11:06:44.403478Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-12T11:06:45.128165Z

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 b0ccabff-fcd4-4dd5-8589-af778af4c74f · inbound

Nonthermal Signatures of Radiative Supernova Remnants II: The Impact of Cosmic Rays and Magnetic Fields cites this paper.

Nonthermal Signatures of Radiative Supernova Remnants II: The Impact of Cosmic Rays and Magnetic Fields Modeling the Saturation of the Bell Instability using Hybrid Simulations

Reference 85

Resolution
metadata mismatch
local_arxiv, observed 2026-08-12T11:06:45.133641Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-12T11:06:44.403478Z digest=sha256:a4ff890ad13167433882c3df6b415ce2e1a038438d57b4f456a3e102125b8380

Observation 2aed91bc-e87a-4087-8f5b-f70d3296687c · inbound

Self-confinement of relativistic pair beams in magnetized interstellar plasmas: the case of pulsar X-ray filaments cites this paper.

Self-confinement of relativistic pair beams in magnetized interstellar plasmas: the case of pulsar X-ray filaments Modeling the Saturation of the Bell Instability using Hybrid Simulations

Reference 40

Resolution
unresolved
no resolver link, observed 2026-08-03T15:48:52.245353Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T15:48:52.245353Z digest=sha256:9014be5c70d32e2defcfe50132bb37d95480e15d11bb3d2a46c5d399246a63ee

Observation 10f5a11d-1f78-4b63-b5ef-0dccd140a421 · inbound

CRESCENDO II: Spectral cosmic rays with improved energy losses and realistic supernova seeding cites this paper.

CRESCENDO II: Spectral cosmic rays with improved energy losses and realistic supernova seeding Modeling the Saturation of the Bell Instability using Hybrid Simulations

Reference 194

Resolution
unresolved
no resolver link, observed 2026-08-02T02:26:52.953788Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T02:26:52.953788Z digest=sha256:d1f6979a55bc2010a9d716ae5e29f75c944043d8e5513a325e9a88b76281daf7