Magnetically Driven Turbulence in the Inner Regions of Protoplanetary Disks

Given the important role turbulence plays in the settling and growth of dust grains in protoplanetary disks, it is crucial that we determine whether these disks are turbulent and to what extent. Protoplanetary disks are weakly ionized near the midplane, which has led to a paradigm in which largely l...

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Hlavní autoři:	David G. Rea, Jacob B. Simon, Daniel Carrera, Geoffroy Lesur, Wladimir Lyra, Debanjan Sengupta, Chao-Chin Yang, Andrew N. Youdin
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	IOP Publishing 2024-01-01
Edice:	The Astrophysical Journal
Témata:	Planet formation Magnetohydrodynamics Accretion Protoplanetary disks Magnetohydrodynamical simulations
On-line přístup:	https://doi.org/10.3847/1538-4357/ad57c5
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