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DTSTART:19700308T020000
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DTSTAMP:20181221T160907Z
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DTSTART;TZID=America/Chicago:20181114T103000
DTEND;TZID=America/Chicago:20181114T120000
UID:submissions.supercomputing.org_SC18_sess338@linklings.com
SUMMARY:Scientific Visualization & Data Analytics Showcase
DESCRIPTION:Scientific Visualization & Data Analytics Showcase\nVisualizat
 ion, Tech Program Reg Pass\n\nVisualizing Outbursts of Massive Stars\n\nIn
 sley, Jiang, Cantiello, Bildsten, Quataert...\n\nMassive stars play an imp
 ortant role in many astrophysical environments such as star formation and 
 the structure of the interstellar medium in galaxies. However, the structu
 res and mass loss of massive stars, which are crucial to understand the ev
 olution and fate of massive stars, are still mysterie...\n\n--------------
 -------\nVisualization of Droplet Dynamics in Cloud Turbulence\n\nKumar, R
 ehme, Suresh\n\nThe study of droplet dynamics is a crucial part of cloud p
 hysics and involves investigation of each and every droplet’s properties. 
 It is difficult to carry out such investigations using field observations.
  Small scale simulation is one method to study such phenomena, and visuali
 zation of these proc...\n\n---------------------\nArctic Ocean-Sea Ice Int
 eractions\n\nFoss, Nguyen, Bigdeli, Ocaña, Bradshaw...\n\nThe Arctic Ocean
 , the smallest and shallowest of the five major oceans, is a unique physic
 al and ecological system. With the recent shifts in global climate, which 
 are amplified in the Arctic, this system is undergoing profound changes. S
 cientists are working to document these changes to provide a b...\n\n-----
 ----------------\nThe First Water in the Universe\n\nWiggins, Samsel, Hoch
 , Abram, Gagliano...\n\nRecent work in the chemistry of molecular clouds i
 n the early universe has found reactions that may create ancient water mol
 ecules that predate our Sun.   For these to take place, however, particula
 r conditions of molecular density and temperature must exist.  Water molec
 ules will be destroyed by ei...\n\n---------------------\nVolume Rendering
 s of Sheared Thermal Convection\n\nFavre, Blass\n\nOceans play a big role 
 in the nature of our planet.  About 70% of our earth is covered by water. 
  Strong currents are transporting warm water around the world and therefor
 e not only make life possible, but also allow us to harvest its power prod
 ucing energy.  But humanity tends to easily forget that...\n\n------------
 ---------\nProgrammable Interactive Visualization of a Core-Collapse Super
 nova Simulation\n\nHaas, Mösta, Roopa, Kuhn, Nienhaus\n\nCore-collapse sup
 ernovae (CCSN) are the birth places of neutron stars and black holes. They
  liberate the ashes of stellar evolution, seeding the interstellar gas wit
 h the elements from which planets form and life is made. Despite their imp
 ortance for much of astrophysics, our understanding of the su...\n
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