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DTSTART;TZID=America/New_York:20241119T100000
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UID:submissions.supercomputing.org_SC24_sess553_art101@linklings.com
SUMMARY:Magnetized Bipolar Jet
DESCRIPTION:Michael Sandoval (Oak Ridge National Laboratory (ORNL)); Forre
 st Glines (NVIDIA Corporation); Philipp Grete (University of Hamburg, Germ
 any); Benjamin Wibking (Michigan State University); Deovrat Prasad (Cardif
 f University); and Brian O'Shea (Michigan State University)\n\nThe simulat
 ion data was produced using the AthenaPK code (https://github.com/partheno
 n-hpc-lab/athenapk) using the Frontier supercomputer at the Oak Ridge Lead
 ership Computing Facility (OLCF). The data is a time snapshot from the Ath
 enaPK simulation of a galaxy cluster with a virial mass of ~6.6e14 solar m
 asses and a central supermassive black hole of ~1.1e9 solar masses. The da
 ta was then visualized on the Andes cluster at OLCF using VisIt (https://g
 ithub.com/visit-dav/visit). VisIt was used to generate an isosurface of th
 e jet and the streamlines of the magnetic field. Both the isosurfaces and 
 streamlines were exported to OBJ files to then be further visualized on Fr
 ontier using Blender (https://www.blender.org/). Blender was used to impor
 t both OBJ files and make the final PNG render of the objects using the Cy
 cles render engine.\n\nRegistration Category: Tech Program Reg Pass, Works
 hop Reg Pass, Tutorial Reg Pass, Exhibits Reg Pass\n\n
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