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P. Diamessis,
K. Nomura
UCSD
Mechanical and Aerospace Engineering Dept.
G. Johnson, N. Bordes
San
Diego Supercomputer Center
Volume visualization techniques highlight small-scale structures within
turbulent flow. The flow itself has been computed using Direct Numerical
Simulation (DNS) that computes a numerica solution of the exact 3D time-dependent
Navier-Stokes equations.
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R. Carson
UCSD Economics Dept.
G. Johnson
San Diego Supercomputer Center
N. Bordes, B. Pailthorpe
University of Sydney
Using archetype analysis, US economic data for the last 100 years was
summarized by plotting boom, stagflation, and depression
parameters. The resulting "snake" illustrates the ups and
downs of the US economy.
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M. Martone, S. Peltier
UCSD
NCMIR
A. DeCastro, D. Nadeau
San
Diego Supercomputer Center
A section of a rat cerebellum, scanned by a laser scanning confocal
microscope, is re-assembled into a wide thin volume data set. The data
set is then visualized to highlight nerve cells.
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J. Feramisco
UCSD
Cancer Center, Digital Imaging Shared Resource.
A. DeCastro, P. Fisher-Ogden, D. Nadeau
San
Diego Supercomputer Center
Collaboration between the SDSC Scientific Visualization group and the UCSD Cancer Center,
Digital Imaging Shared Resource.
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Volume Visualization of the Orion Nebula
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D. Nadeau, J. Genetti
San
Diego Supercomputer Center
C. Emmart, E. Wesselak, D. Davidson
Hayden
Planetarium
C.R. O'Dell, Zheng Wen
Rice
University
A 3D volumetric model visualizes the ionization front and proplyds
(proto stars) within the Orion Nebula, 1500 light years from Earth.
The model is based upon data derived from Hubble and ground-based observations.
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Volume Visualization of the Evolution of an Emission Nebula
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D. Nadeau, E. Engquist
San
Diego Supercomputer Center
A. Braun, C. Emmart, R. Wyatt, M. Mac Low
Hayden
Planetarium
2.5 terabytes of computer simulation data are used to visualize the
evolution of an emission nebula. Dust and gas condenses to form a star whose
bright light ionizes the nearby gas to create an eerie red and green glow.
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