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Dan Spicer
Movie   ID   Roles   Title
A rendering of the model of the Earths magnetosphere. The flat ribbons represent charged particles entering the influence of the magnetosphere and being deflected. The curved lines visible to the right represent the magnetic field lines extending out from the Earth. The force from the sun pushes these lines into a distinctive tail-like shape. Finally, the green surface represents a constant value for the magnetic field strength.   3028 Scientist
  A 3-Dimensional Model of the Magnetosphere (WMS)
Movie of spacecraft on an Earth-to-Mars trajectory.   2924 Scientist
  Sun vs. Mission to Mars
A brief flight through the magnetotail   2676 Scientist
  Tour of the Magnetosphere
A profile view of the magnetosphere. The Sun would be located to the left. Lines from the Earths magnetic field are stretched out behind the Earth to form the magnetotail.   2391 Scientist
  Magnetosphere II: The Solar Wind Strikes Back!
A profile view of the magnetosphere. The Sun would be located to the left. Lines from the Earth's magnetic field are stretched out behind the Earth to form the magnetotail.   2387 Scientist
  The Magnetosphere - Earth Raises its Shields
Zooming out from the surface of the Earth to a view of the Earths magnetic field as represented by selected field lines. A representation of the Sun is also added.   803 Scientist
  Digital Earth Workbench: The Earth's Magnetic Field
Starting with a view of the magnetic field of the Earth, a surface of constant plasma density is added. The basket shape of the surface depicts the compression in front of the Earth caused by solar wind pressure and the handle behind the Earth due to the magnetotail current   804 Scientist
  Digital Earth Workbench: Magnetospheric Density
Starting with a view of the magnetosphere of the Earth, a surface of constant plasma pressure is added showing a shield-like configuration due to the pressure from the solar wind   805 Scientist
  Digital Earth Workbench: Magnetospheric Pressure
A animation of the evolution of the density in the solar atmosphere model   111 Scientist
  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 Scientist
  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 Scientist
  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 Scientist
  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 Scientist
  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 Scientist
  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 Scientist
  Global Hybrid Versus MHD Modeling of the Magnetosphere: Density and Magnetic Field
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 Scientist
  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 Scientist
  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 Scientist
  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 Scientist
  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 Scientist
  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 Scientist
  2-D Unstructured Mesh Particle-MHD Solar Wind Flow Over the Earth:Density and Magnetic Field


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