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SUMMARY:Local\, global\, and locally global models of radial convection in
  protoplanetary disks
DTSTART;VALUE=DATE-TIME:20260610T060000Z
DTEND;VALUE=DATE-TIME:20260610T080000Z
DTSTAMP;VALUE=DATE-TIME:20260701T124700Z
UID:indico-event-5106@indico-tdli.sjtu.edu.cn
DESCRIPTION:Speakers: Min-Kai Lin\n\nHost: Dong LaiLocation: TDLI\, Open A
 rea (4F-SW)Join Tencent Meeting：https://meeting.tencent.com/dm/RCv78Lx24
 biUMeeting ID: 904672573 (no password） Abstract:Hydrodynamic processes 
 in protoplanetary disks influence a number of key stages in planet format
 ion and evolution. One candidate\, the Convective Overstability may operat
 e in planet-forming disk regions. I will present our group’s recent effo
 rts in modeling the COS using a variety of frameworks to test its robustn
 ess and explore its implications for planetesimal formation and planet mig
 ration. This includes the local Boussinesq approximation\, global compress
 ible  simulations\, with and without dust\, an ongoing “locally global
 ” setup\, and extensions to magnetized gas. I will discuss the advantage
 s and caveats of each approach\, and suggest future directions.  Biogra
 phy:Dr. Min-Kai Lin is an Associate Research Fellow at the Academia Sinica
  Institute of Astronomy and Astrophysics. He completed his PhD in 2011 at 
 the University of Cambridge\, followed by a postdoctoral fellowship at the
  Canadian Institute for Theoretical Astrophysics from 2011 to 2014\, and w
 as a Steward Theory Fellow at the University of Arizona from 2014 to 2016\
 , before taking up his current faculty position at ASIAA. Dr. Lin's primar
 y expertise is astrophysical fluid dynamics applied to theories of planet 
 formation and evolution. \n\nhttps://indico-tdli.sjtu.edu.cn/event/5106/
LOCATION:Tsung-Dao Lee Institute
URL:https://indico-tdli.sjtu.edu.cn/event/5106/
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