Magnetorotational instability in protoplanetary discs: the effect of dust grains
We investigate the linear growth and vertical structure of the magnetorotational instability (MRI) in weakly ionized, stratified protoplanetary discs. The magnetic field is initially vertical and dust grains are assumed to be well mixed with the gas over
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|Source:||Monthly Notices of the Royal Astronomical Society|
|01_Salmeron_Magnetorotational_instability_2008.pdf||734.63 kB||Adobe PDF||Request a copy|
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