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Non-ideal magnetohydrodynamics in protoplanetary disks

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If you have a question about this talk, please contact Jean Teyssandier.

Observations of protoplanetary disks have provided signatures of accretion, ejection, and large-scale organisation. I will address these three points in the light of recent numerical simulations. In particular, I will review the outcome of the Magneto-Rotational Instability in the context of non-ideal magnetohydrodynamics, and the possibility of producing organised structures out of turbulence.

This talk is part of the DAMTP Astrophysics Seminars series.

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