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Liam Krauss



Movie   ID   Roles   Title
SeaWiFS Biosphere data symbolizing the heartbeat of our planet.   2395 Animator
  Pulse of the Planet
The entire narrated Images video made for Supercomputing 97   251 Animator
  Images of Earth and Space: SC97 Edition
A animation of the evolution of the density in the solar atmosphere model   111 Animator
  Numerical Simulation of Magnetic Flux Emerging Through a Model Solar Atmosphere: Density
A animation of the evolution of the density gradient in the solar atmosphere model   112 Animator
  Numerical Simulation of Magnetic Flux Emerging Through a Model Solar Atmosphere: Density Gradient
A animation of the evolution of the density, the magnetic field, and the mach number in the solar atmosphere model.  Magnetic field contours are shown in black and mach number contours are shown in green.   113 Animator
  Numerical Simulation of Magnetic Flux Emerging Through a Model Solar Atmosphere: Density, Magnetic Field, and Mach Number
A animation of the evolution of the density gradient, the magnetic field, and the mach number in the solar atmosphere model.  Magnetic field contours are shown in magenta and mach number contours are shown in green.   114 Animator
  Numerical Simulation of Magnetic Flux Emerging Through a Model Solar Atmosphere: Density Gradient, Magnetic Field, and Mach Number
A animation of the evolution of the density gradient and velocities in the solar atmosphere model.  The three velocities shown are the velocity normalized to the fast magnetosonic speed and the velocities parallel and perpendicular to the magnetic field.  Mach number contours are shown in green.   115 Animator
  Numerical Simulation of Magnetic Flux Emerging Through a Model Solar Atmosphere: Density Gradient and Velocities
Contour lines of the z-component of the magnetic potential are compared for a 2D global hybrid simulation and a magnetohydrodynamic model of the solar wind-magnetosphere interaction   117 Animator
  Global Hybrid Versus MHD Modeling of the Magnetosphere: Magnetic Potential
Magnetic field lines superimposed over density are compared for a 2D global hybrid simulation and a magnetohydrodynamic model of the solar wind-magnetosphere interaction   1393 Animator
  Global Hybrid Versus MHD Modeling of the Magnetosphere: Density and Magnetic Field
Narrated Hologlobe (version 2)   116 Animator
  The HoloGlobe Project (Version 2)
Hologlobe (version 1)   96 Animator
  The HoloGlobe Project (Version 1)
This image represents a one month sample (October 1983) of composite images from cloud cover data collected from a suite of U.S., European, and Japanese geostationary satellites and U.S. polar orbiting meteorological satellites.   155 Animator
  The HoloGlobe Project (Version 3)
Density and magnetic flux surfaces from a simulation of magnetic flux in the solar atmosphere undergoing velocity perturbations.  This run has a vertical scale height of 4.8 million meters.   107 Animator
  High Resolution 2-D Numerical Simulation of Emergence of Magnetic Flux Through the Solar Atmosphere
Various quantities from a simulation of magnetic flux in the solar atmosphere undergoing velocity perturbations.  This run has a vertical scale height of 4.8 million meters.   1416 Animator
  High Resolution 2-D Numerical Simulation of Emergence of Magnetic Flux Through the Solar Atmosphere
Various quantities from a simulation of magnetic flux in the solar atmosphere undergoing velocity perturbations.  This run has a vertical scale height of 6.8 million meters.   1417 Animator
  High Resolution 2-D Numerical Simulation of Emergence of Magnetic Flux Through the Solar Atmosphere
Density and magnetic flux surfaces from a simulation of magnetic flux in the solar atmosphere undergoing velocity perturbations.  This run has a vertical scale height of 6.8 million meters.   1418 Animator
  High Resolution 2-D Numerical Simulation of Emergence of Magnetic Flux Through the Solar Atmosphere
Contour lines of the z-component of the magnetic potential for a 2D simulation of the solar wind-magnetosphere interaction   86 Animator
  2-D Unstructured Mesh Particle-MHD Solar Wind Flow Over the Earth: Magnetic Potential
Magnetic field lines superimposed over density for a 2D simulation of the solar wind-magnetosphere interaction   87 Animator
  2-D Unstructured Mesh Particle-MHD Solar Wind Flow Over the Earth:Density and Magnetic Field
This animation presents correlated measurements and model data for an impact of a magnetic cloud originating from the Sun on the Earths magnetosphere on October 18-20, 1995.   88 Animator
  Magnetic Cloud Event: October 18-20, 1995
A comparison of energetic electron fluxes (> 0.4 MeV) over the North Pole from the PET P1 solid state detector during the period 7-19-1993 through 8-6-1994 with soft X-ray images from Yohkoh   90 Animator
  SAMPEX - Yohkoh: Solar Modification of Relativistic Electrons in the Earth's Radiation Belts
An interactive exploration of a computational model of Hurricane Florence using an immersive environment controlled by a boom, with an inset of the boom operator.   81 Animator
  Hurricane Florence with Inset of VR Operator
An interactive exploration of a computational model of Hurricane Florence using an immersive environment controlled by a boom   82 Animator
  Hurricane Florence
Video of an operator using a boom to control an immersive application   83 Animator
  VR Operator
An interactive exploration of a computational model of Hurricane Florence using an immersive environment controlled by a boom, with an inset of the boom operator.   122 Animator
  Hurricane Florence Mesoscale Simulation Results Using Virtual Reality


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