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SUMMARY:Constraining the Radial Turbulence Parameter $\\alpha$ from the Di
 stribution of Water and Refractory species in an Evolving Solar Nebula
DTSTART;VALUE=DATE-TIME:20200511T121500Z
DTEND;VALUE=DATE-TIME:20200511T123500Z
DTSTAMP;VALUE=DATE-TIME:20240704T115618Z
UID:indico-contribution-53@meetings.aip.de
DESCRIPTION:Speakers: Anusha Kalyaan (Clemson University)\nThe overall str
 ucture of the evolving protoplanetary disk is set by the interaction of ac
 cretion and dispersal processes such as turbulence\, winds and photoevapor
 ation (Ercolano & Pascucci 2017)\, with finer structural details (as gaps\
 , cavities\, spirals and warps) in the disk provided by planet formation (
 eg. Van der Marel et al. 2015). Recent meteoritic evidence from Kruijer et
  al. (2017) strongly suggest the presence of two distinct isotopic reservo
 irs in the \n\nhttps://meetings.aip.de/event/1/contributions/53/
LOCATION:Leibniz Institute for Astrophysics Potsdam (AIP) Lecture Hall
URL:https://meetings.aip.de/event/1/contributions/53/
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