Skip all navigation and jump to content Jump to site navigation Jump to section navigation.
NASA Logo - Goddard Space Flight Center + Visit NASA.gov
HOME PROJECTS RESOURCES SEARCH MAP

+ Advanced Search
Home
Home
View Most Recently Released Imagery
View Gallery of Imagery: A topical collection of SVS Imagery
Search Imagery by the keywords assigned to it
Search Imagery by the instruments that supplied data for a visualization product
Search Imagery by the series of visualizations that have been produced
Search Imagery by the scientist providing the data used in a visualization product
Search Imagery by the animator that created the product
Search Imagery by the identification number assigned to the visualization product
See other search options
Learn about the SVS Image Server
  + About the Server
  + Animation List
  + How to Use the Server


  + RSS Feeds
blank image

Dan Spicer
Movie   ID   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   A 3-Dimensional Model of the Magnetosphere (WMS)
Movie of spacecraft on an Earth-to-Mars trajectory.   2924   Sun vs. Mission to Mars
A brief flight through the magnetotail   2676   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   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   The Magnetosphere - Earth Raises its Shields
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   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   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   High Resolution 2-D Numerical Simulation of Emergence of Magnetic Flux Through the Solar Atmosphere
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   Global Hybrid Versus MHD Modeling of the Magnetosphere: Density and Magnetic Field
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   Digital Earth Workbench: Magnetospheric Pressure
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   Digital Earth Workbench: Magnetospheric Density
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   Digital Earth Workbench: The Earth's Magnetic Field
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   Global Hybrid Versus MHD Modeling of the Magnetosphere: Magnetic Potential
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   Numerical Simulation of Magnetic Flux Emerging Through a Model Solar Atmosphere: Density Gradient and Velocities
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   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, 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   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 in the solar atmosphere model   112   Numerical Simulation of Magnetic Flux Emerging Through a Model Solar Atmosphere: Density Gradient
A animation of the evolution of the density in the solar atmosphere model   111   Numerical Simulation of Magnetic Flux Emerging Through a Model Solar Atmosphere: Density
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   High Resolution 2-D Numerical Simulation of Emergence of Magnetic Flux Through the Solar Atmosphere
Magnetic field lines superimposed over density for a 2D simulation of the solar wind-magnetosphere interaction   87   2-D Unstructured Mesh Particle-MHD Solar Wind Flow Over the Earth:Density and Magnetic Field
Contour lines of the z-component of the magnetic potential for a 2D simulation of the solar wind-magnetosphere interaction   86   2-D Unstructured Mesh Particle-MHD Solar Wind Flow Over the Earth: Magnetic Potential


Back to Top

USA.gov logo - the U.S. Government's official Web portal. + Privacy Policy and Important Notices
+ Reproduction Guidelines 		NASA NASA Official:
SVS Contact:
Curator: