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DTSTART;TZID=America/New_York:20191101T140000
DTEND;TZID=America/New_York:20191101T150000
DTSTAMP:20260408T094106
CREATED:20190909T184651Z
LAST-MODIFIED:20190909T184651Z
UID:1951-1572616800-1572620400@seasevents.nmsdev7.com
SUMMARY:PICS Seminar: "High-order Spectral Difference Method for Studying Marine Hydrodynamics and Thermal Convection and Magneto-hydrodynamics for the Sun"
DESCRIPTION:Abstract\nTwo recent advancements of high-order spectral difference (SD) method for computational fluid dynamics on unstructured meshes will be presented. The first progress is our contribution to a new curved sliding-mesh approach to the SD method for simulating flapping and rotary wing aerodynamics.  The second elevation of the SD method is our recent successful design of a massively parallel code\, namely CHORUS\, for predicting thermal convection in the Sun.  Recently\, we have also built a simulation capability for predicting magnetohydrodynamics of the Sun.
URL:https://seasevents.nmsdev7.com/event/pics-seminar-high-order-spectral-difference-method-for-studying-marine-hydrodynamics-and-thermal-convection-and-magneto-hydrodynamics-for-the-sun/
LOCATION:PICS Conference Room 534 – A Wing \, 5th Floor\, 3401 Walnut Street\, Philadelphia\, PA\, 19104\, United States
CATEGORIES:Colloquium
ORGANIZER;CN="Penn Institute for Computational Science (PICS)":MAILTO:dkparks@seas.upenn.edu
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