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DTSTAMP:20190719T085754Z
LOCATION:HG E 1.1
DTSTART;TZID=Europe/Stockholm:20190612T153000
DTEND;TZID=Europe/Stockholm:20190612T173000
UID:submissions.pasc-conference.org_PASC19_sess162@linklings.com
SUMMARY:MS11 - Multidimensional Stellar Evolution: Bridging the Modelling 
 and Computational Challenges
DESCRIPTION:Minisymposium\nComputer Science and Applied Mathematics, Physi
 cs\n\nHigh-Order Well-Balanced FVM for the Euler Equations with Gravity an
 d Astrophysical Applications\n\nGrosheintz\n\nTBD.\n\n--------------------
 -\nComputational Challenges of Numerical Simulations of Convection inside 
 Stars\n\nKupka\n\nNumerical simulations of convection have become a widely
  used tool in stellar astrophysics to investigate the interaction of conve
 ction with stellar pulsation, energy transfer, mixing, and the generation 
 of magnetic fields inside stars. Such simulations have to account for phys
 ical processes which o...\n\n---------------------\nAspects of Multi-Dimen
 sional Radiation Transfer in Stellar Atmospheres\n\nSteiner\n\nRadiative t
 ransfer (RT) computations are the bread and butter of astrophysical resear
 ch. One can arguably divide RT tasks into three categories. First, RT occu
 rs as part of the energy equation in numerical simulations of stellar atmo
 sphere. In this case, details of the spectrum are less important th...\n\n
 ---------------------\nMulti-Dimensional Fully Compressible, Time Implicit
   Simulations of Hydrodynamical Processes in Stars\n\nBaraffe\n\nI will pr
 esent the recent development of a multi-dimensional, fully compressible hy
 drodynamical time implicit code MUSIC devoted to stellar and planetary int
 eriors. I will discuss the main challenges in the computation of multi-dim
 ensional stellar structures and some of the advantages of our approac...\n
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