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LOCATION:HG E 1.1
DTSTART;TZID=Europe/Stockholm:20190614T103000
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UID:submissions.pasc-conference.org_PASC19_sess116@linklings.com
SUMMARY:MS45 - Numerical Methods and HPC Challenges in Magneto Hydro Dynam
 ics (MHD) Modelling in Plasma Physics
DESCRIPTION:Minisymposium\nComputer Science and Applied Mathematics, Physi
 cs\n\nHighly Parallel Geometric Multigrid Solver Suitable for Adaptive Mes
 h Refinement (AMR) Grids in Plasma Simulations\n\nTeunissen\n\nLarge-scale
  3D simulations of plasma physics phenomena are computationally very expen
 sive. By using adaptive mesh refinement (AMR), the resolution of the numer
 ical grid can be reduced in smooth or uninteresting regions. Through paral
 lelization, computation times can be further reduced. However, the ...\n\n
 ---------------------\nA Multidimensional Analogue of the HLLI Riemann Sol
 ver for Conservative Hyperbolic Systems for Astrophysical Plasma Applicati
 ons\n\nNkonga, Balsara\n\nJust as the quality of a one-dimensional approxi
 mate Riemann solver is improved by the inclusion of internal sub-structure
 , the quality of a multidimensional Riemann solver is also similarly impro
 ved. Such multidimensional Riemann problems arise when multiple states com
 e together at the vertex of a ...\n\n---------------------\nChallenges in 
 MHD Modelling in Fusion Devices\n\nHuijsmans\n\nThe main goal of the ITER 
 project is to create plasmas producing about 500 MW of fusion power. Due t
 o its large size, the thermal energy (350MJ) of ITER plasmas will be much 
 larger than current experiments. Magnetohydrodynamic (MHD) instabilities c
 an cause fast losses of the thermal plasma energy. I...\n\n---------------
 ------\nOpen Discussion\n\nBecoulet, Huijsmans, Teunissen, Nkonga\n\nFollo
 wing the three talks the round table discussion will be focused on the fin
 ding out the common interests and possible synergy in numerical and HPC co
 mputing methods in presented different applications of MHD in plasma physi
 cs including astrophysics, hot magnetic fusion plasmas and cold plasmas. .
 ..\n
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