Global three-dimensional simulations of outer protoplanetary discs with ambipolar diffusion

ABSTRACT The structure and evolution of protoplanetary discs (PPDs) are largely governed by disc angular momentum transport, mediated by magnetic fields. In the most observable outer disc, ambipolar diffusion is the primary non-ideal magnetohydrodynamic (MHD) effect. In this work, we study the gas d...

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Bibliographic Details
Published inMonthly notices of the Royal Astronomical Society Vol. 507; no. 1; pp. 1106 - 1126
Main Authors Cui, Can, Bai, Xue-Ning
Format Journal Article
LanguageEnglish
Published London Oxford University Press 01.10.2021
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