SC25 Home
Close

Presentation

Magnetic Field of a Star Formation Simulation
SessionArt of HPC Gallery
DescriptionThis star formation simulation data shows how the rotating gas winds up the magnetic field around a forming protostar. All protostellar systems have angular momentum/rotation—this is how accretion disks/planetary systems form. Various details of the magnetic field geometry visualized here in response to this rotation are interesting in protostar research.
Authors
Greg Foss
Texas Advanced Computing Center (TACC)
The University of Texas at Austin
Dave Semeraro
Texas Advanced Computing Center (TACC)
The University of Texas at Austin
Stella Soffner
Oden Institute for Computational Engineering and Sciences
The University of Texas at Austin
Nina Flippova
Oden Institute for Computational Engineering and Sciences
The University of Texas at Austin
Sean Cunningham
Texas Advanced Computing Center (TACC)
The University of Texas at Austin
Event Type
Art of HPC
TimeFriday, 21 November 20258:00am - 12:00pm CST
LocationArt of HPC - Plaza Lobby
Tags
Art of HPC
Next PresentationNext Presentation
Machine Dreaming
Similar Presentations
The First Star-by-Star $N$-body/Hydrodynamics Simulation of Our Galaxy Coupling with a Surrogate Model