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Integrity report for Dust Dynamics in Protoplanetary Disk Winds Driven by Magneto-Rotational Turbulence: A Mechanism for Floating Dust Grains with Characteristic Sizes

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

arXiv:1505.03704 · pith:2015:3Y26UN5627GMVGFZJFQ5QH5URE

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Paper page arXiv integrity.json bundle.json

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Signed record

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