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Paper Citation Record · LEDGER

Acceleration and propagation of Solar Energetic Particles

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1705.07274.

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

pith.paper-citation-record.v1
1705.07274 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 2026-08-13T06:32:02.005865+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T17:08:09.354849Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-03T01:57:31.773769Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • 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 7cd0dd9b-d8d8-4cd5-ac71-d8854412231a · inbound

Nonthermal line broadening at solar flare footpoints is primarily field-aligned cites this paper.

Nonthermal line broadening at solar flare footpoints is primarily field-aligned Acceleration and propagation of Solar Energetic Particles

Reference 24

Resolution
malformed identifier
local_arxiv, observed 2026-07-02T15:47:06.834306Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-06-27T23:21:08.521919Z digest=sha256:1bfbe17927370a34c7a39f8576a82787b393361227763300f46abcd270835250

Observation b075ae8e-55c9-4207-b5e1-e8c5ab7e50bf · inbound

Time-dependent cosmic-ray escape from wind bubbles: hard spectra formation cites this paper.

Time-dependent cosmic-ray escape from wind bubbles: hard spectra formation Acceleration and propagation of Solar Energetic Particles

Reference 262

Resolution
verified exact
local_arxiv, observed 2026-06-27T08:40:45.643018Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:42a12030ea2e83a52018e193940a360c08a76e8fcee01a1503cb07f44af8fe22

Observation e88fabe0-9f2e-424c-938b-5463f4d58020 · inbound

Energetic particle-mediated interplanetary shocks observed by Solar Orbiter cites this paper.

Energetic particle-mediated interplanetary shocks observed by Solar Orbiter Acceleration and propagation of Solar Energetic Particles

Reference 249

Resolution
verified exact
local_arxiv, observed 2026-07-03T01:57:31.775445Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:3f28d818e4f7fcc421ab7e8b7040ec5d160b8a2bed503b8a21a1da5f23f6dccd

Observation c2ee8459-d93c-4efa-9688-8a23f6f57181 · inbound

A new methodology for inferring the plasma conditions in solar flare energetic electron source regions from in situ electron energy spectra cites this paper.

A new methodology for inferring the plasma conditions in solar flare energetic electron source regions from in situ electron energy spectra Acceleration and propagation of Solar Energetic Particles

Reference 22

Resolution
unresolved
no resolver link, observed 2026-08-04T17:08:09.354849Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T17:08:09.354849Z digest=sha256:65b6ae9ef15ba28935f9e71d06ea14c02bba1f6d338f14ce921a6c40b91e7332