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...
Saved in:
Published in | Monthly notices of the Royal Astronomical Society Vol. 507; no. 1; pp. 1106 - 1126 |
---|---|
Main Authors | , |
Format | Journal Article |
Language | English |
Published |
London
Oxford University Press
01.10.2021
|
Subjects | |
Online Access | Get full text |
Cover
Loading…
Be the first to leave a comment!