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BEGIN:VEVENT
DTSTAMP:20260202T201256Z
LOCATION:Art of HPC - Plaza Lobby
DTSTART;TZID=America/Chicago:20251121T080000
DTEND;TZID=America/Chicago:20251121T120000
UID:submissions.supercomputing.org_SC25_sess608_art116@linklings.com
SUMMARY:Magnetic Field of a Star Formation Simulation
DESCRIPTION:Greg Foss and Dave Semeraro (Texas Advanced Computing Center (
 TACC), The University of Texas at Austin); Stella Soffner and Nina Flippov
 a (Oden Institute for Computational Engineering and Sciences, The Universi
 ty of Texas at Austin); and Sean Cunningham (Texas Advanced Computing Cent
 er (TACC), The University of Texas at Austin)\n\nThis star formation simul
 ation data shows how the rotating gas winds up the magnetic field around a
  forming protostar. All protostellar systems have angular momentum/rotatio
 n—this is how accretion disks/planetary systems form. Various details of t
 he magnetic field geometry visualized here in response to this rotation ar
 e interesting in protostar research.\n\nTag: Art of HPC\n\nRecording: Not 
 Livestreamed, Not Recorded\n\nRegistration Category: Technical Program Reg
  Pass, Workshop Reg Pass, Tutorial Reg Pass, Exhibits Reg Pass\n\n
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