Paper Citation Record · LEDGER

Simulations of Stellar Magnetoconvection using the Radiative MHD Code `StellarBox'

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1507.07999.

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

pith.paper-citation-record.v1
1507.07999 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 2026-08-16T06:30:59.297886+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T17:06:16.348118Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T15:27:20.195798Z

Reference resolution

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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 b1fd4d36-35b2-4909-aafe-5b5250656b59 · inbound

Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling cites this paper.

Revisiting turbulent properties of solar convection with 3D radiative hydrodynamic modeling Simulations of Stellar Magnetoconvection using the Radiative MHD Code `StellarBox'

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-09T17:06:16.348118Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7d09c92b-e87a-432d-83cb-a5745b8ec0df · inbound

Properties of Turbulent Convection and Large-Scale Flows in a Rotating F-type Star Revealed by 3D Realistic Radiative Hydrodynamic Simulations cites this paper.

Properties of Turbulent Convection and Large-Scale Flows in a Rotating F-type Star Revealed by 3D Realistic Radiative Hydrodynamic Simulations Simulations of Stellar Magnetoconvection using the Radiative MHD Code `StellarBox'

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-08T14:10:22.083759Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c5954d5f-4deb-4521-bce5-f804bce29485 · inbound

Cluster-Weighted Training of Deep Surrogate Models for Subgrid Turbulent Transport cites this paper.

Cluster-Weighted Training of Deep Surrogate Models for Subgrid Turbulent Transport Simulations of Stellar Magnetoconvection using the Radiative MHD Code `StellarBox'

Reference 5

Resolution: verified exact; local_arxiv, observed 2026-07-10T15:27:20.197225Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation fb4351e4-3c27-43b0-b891-35f7d32bb165 · inbound

Developing Machine Learning Models of Subgrid Turbulent Transport for Quiet Sun 3D Radiative Hydrodynamic Simulations cites this paper.

Developing Machine Learning Models of Subgrid Turbulent Transport for Quiet Sun 3D Radiative Hydrodynamic Simulations Simulations of Stellar Magnetoconvection using the Radiative MHD Code `StellarBox'

Reference 37

Resolution: unresolved; no resolver link, observed 2026-07-13T05:25:47.083510Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.