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Paper Citation Record · LEDGER

The solar dynamo begins near the surface

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2404.07740.

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

pith.paper-citation-record.v1
2404.07740 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 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 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T00:15:41.934182Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-11T17:06:06.168855Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • 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 71dcaf94-663a-4937-823a-7628bb5eec07 · inbound

Wave interference as the origin of the cyclic magnetorotational dynamo in accretion disks: insights from weakly nonlinear theory and local shearing box simulations cites this paper.

Wave interference as the origin of the cyclic magnetorotational dynamo in accretion disks: insights from weakly nonlinear theory and local shearing box simulations The solar dynamo begins near the surface

Reference 67

Resolution
verified exact
arxiv_id, observed 2026-05-11T17:06:06.173427Z

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=pdf_text observed=2026-05-08T17:52:18.691984Z digest=sha256:281684d733d93877f661eaa2c8bf5b15ccb0b144e84d6cc27671d2e175f43bb3

Observation a38da32b-3ec9-412d-8d4d-58f7ee8442fa · inbound

Wave interference as the origin of the cyclic magnetorotational dynamo in accretion disks: insights from weakly nonlinear theory and local shearing box simulations cites this paper.

Wave interference as the origin of the cyclic magnetorotational dynamo in accretion disks: insights from weakly nonlinear theory and local shearing box simulations The solar dynamo begins near the surface

Reference 69

Resolution
verified exact
arxiv_id, observed 2026-05-11T05:06:04.435306Z

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=pdf_text observed=2026-05-11T00:51:45.150373Z digest=sha256:dd09043c8a68ca0309efd63a8d19e7d46911c75bd274db1d920373dfe5a72d25

Observation 90e9e388-f0df-49ee-a510-b99be772c8a9 · inbound

Comparative Periodogram Analysis of 22 Years of Super-Kamiokande Solar $^{8}\mathrm{B}$ Neutrino Data: Classical, Phase-Based, and Information Theoretic Methods cites this paper.

Comparative Periodogram Analysis of 22 Years of Super-Kamiokande Solar $^{8}\mathrm{B}$ Neutrino Data: Classical, Phase-Based, and Information Theoretic Methods The solar dynamo begins near the surface

Reference 21

Resolution
unresolved
no resolver link, observed 2026-07-31T21:33:01.008319Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-31T21:33:01.008319Z digest=sha256:672dc4b74b4e488d8f3842b7e117ed3b3223be62ea50b314dccb1ad513982146

Observation 4398cb43-7331-4e2e-853f-37d93bd8e384 · inbound

Comparative Periodogram Analysis of 22 Years of Super-Kamiokande Solar $^{8}\mathrm{B}$ Neutrino Data: Classical, Phase-Based, and Information Theoretic Methods cites this paper.

Comparative Periodogram Analysis of 22 Years of Super-Kamiokande Solar $^{8}\mathrm{B}$ Neutrino Data: Classical, Phase-Based, and Information Theoretic Methods The solar dynamo begins near the surface

Reference 21

Resolution
unresolved
no resolver link, observed 2026-08-03T01:42:28.036510Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T01:42:28.036510Z digest=sha256:25e8d31974907f5d915d0a1e2763a8843e82796d4a6ed2a98e2c2bf8ff5d6f0c

Observation 0f9dc5da-98ff-4ec1-bf0d-c836ac05924d · inbound

Something new under the Sun: A magnetically driven CH/CN anti-correlation cites this paper.

Something new under the Sun: A magnetically driven CH/CN anti-correlation The solar dynamo begins near the surface

Reference 134

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:41.934182Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:41.934182Z digest=sha256:9ddde64c23b9905badf2d5474bb8ff020502f4ee0fe0a7664bc10d7786d8fddb