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Paper Citation Record · LEDGER

Reduction of the downward energy flux of non-thermal electrons in the solar flare corona due to co-spatial return current losses

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2407.17955.

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

pith.paper-citation-record.v1
2407.17955 v1

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Source: paper_references, paper_reference_links

measured 1 of 1 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T17:08:09.254245Z

measured 0 of 1 external citation measurements

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Source: cited_works

Reference resolution

0 of 0 outbound references displayed

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Pith citing papers

Observation 79eefe32-790d-44f5-81ae-b9a813f35a6f · 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 Reduction of the downward energy flux of non-thermal electrons in the solar flare corona due to co-spatial return current losses

Reference 2

Resolution
unresolved
no resolver link, observed 2026-08-04T17:08:09.254245Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T17:08:09.254245Z digest=sha256:ae0cf33d8d812bc2a2f440e1c589c691107ef57a6a4e98ea8ee21575175ada64