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Integrity report for Three-dimensional simulations of near-surface convection in main-sequence stars. III. The structure of small-scale magnetic flux concentrations

A machine-verified record of the checks Pith has run against this paper: detector runs, findings, signed bundle events, and canonical identifiers.

arXiv:1505.04739 · pith:2015:KLOQ35PVVPQ3NUI6TIMPFKATH7

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Paper page arXiv integrity.json bundle.json

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Signed record

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