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SUMMARY:Magnetic flux transport in protoplanetary discs
DTSTART;VALUE=DATE-TIME:20200511T110000Z
DTEND;VALUE=DATE-TIME:20200511T112000Z
DTSTAMP;VALUE=DATE-TIME:20240704T115617Z
UID:indico-contribution-27@meetings.aip.de
DESCRIPTION:Speakers: Philip Leung ()\nMagnetic effects are important for 
 accretion disc dynamics. In PPDs\, much still needs to be understood in ho
 w non-ideal MHD effects (Ohmic\, Hall and ambipolar diffusion)\, which are
  relevant because of the low ionisation levels found in much of the disc\,
  affect the radial accumulation and retention of magnetic flux needed for 
 processes such as the launching of a magnetic disc wind. I aim to present 
 results from semi-analytic local models incorporating all three non-ideal 
 effects\, and how they inform our understanding of the flux transport prob
 lem. I will also be presenting some recent numerical simulations exploring
  the interplay of these non-ideal effects with the magnetic field geometry
 \, and the resulting implications on the flux transport process.\n\nhttps:
 //meetings.aip.de/event/1/contributions/27/
LOCATION:Leibniz Institute for Astrophysics Potsdam (AIP) Lecture Hall
URL:https://meetings.aip.de/event/1/contributions/27/
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