University of Cambridge > > DAMTP Astro Mondays > Non-ideal magnetohydrodynamics in protoplanetary disks

Non-ideal magnetohydrodynamics in protoplanetary disks

Add to your list(s) Download to your calendar using vCal

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 Astro Mondays series.

Tell a friend about this talk:

This talk is included in these lists:

Note that ex-directory lists are not shown.


© 2006-2022, University of Cambridge. Contact Us | Help and Documentation | Privacy and Publicity