{
    "count": 21,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 3028,
            "url": "https://svs.gsfc.nasa.gov/3028/",
            "result_type": "Visualization",
            "release_date": "2005-01-12T12:00:00-05:00",
            "title": "A 3-Dimensional Model of the Magnetosphere (WMS)",
            "description": "The earth's magnetosphere protects the earth from high-energy charged particles coming from the sun. Some charged particles are deflected by the magnetosphere, while others become trapped and produce the aurora. This presentation shows a 3-dimensional model of the magnetosphere. The features that it highlights are flat ribbons representing the paths of charged particles deflected by the magnetosphere, triangular ribbons representing magnetic field lines, and colored surfaces representing constant values of magnetic force. The original model is in Open Inventor format, and is available here. || ",
            "hits": 126
        },
        {
            "id": 2924,
            "url": "https://svs.gsfc.nasa.gov/2924/",
            "result_type": "Visualization",
            "release_date": "2004-06-28T12:00:00-04:00",
            "title": "Sun vs. Mission to Mars",
            "description": "Spacecraft (green trajectory) on their way from the Earth (blue orbit) to Mars (red orbit) risk being hit by energetic events from the Sun, such as X-rays, energetic protons (blue streaks), and material from Coronal Mass Ejections (CMEs) (red blobs).  The spiral lines from the Sun represent the magnetic field lines 'frozen' into the solar wind. || ",
            "hits": 42
        },
        {
            "id": 2676,
            "url": "https://svs.gsfc.nasa.gov/2676/",
            "result_type": "Visualization",
            "release_date": "2003-03-18T12:00:00-05:00",
            "title": "Tour of the Magnetosphere",
            "description": "Tour of the Earth's magnetosphere generated for 'Live from the Aurora'.  This viz pulls out from the Earth and fades in components of the magnetosphere. || ",
            "hits": 29
        },
        {
            "id": 2391,
            "url": "https://svs.gsfc.nasa.gov/2391/",
            "result_type": "Visualization",
            "release_date": "2002-03-01T12:00:00-05:00",
            "title": "Magnetosphere II: The Solar Wind Strikes Back!",
            "description": "A view of a computer-generated model of the Earth's magnetosphere.  Semi-transparent surfaces represent particle density (red is high, blue is low), the silvery tube represent magnetic field lines and the yellow ribbons represent the paths of charged solar wind particles.  In this particular model, the solar wind has an ambient density of 8.35 particles/cm^3.  The isosurfaces are then red (> 17 particles/cm^3), yellow (> 12 particles/cm^3), green (> 8.6 particles/cm^3) and blue (< 1.0 particle/cm^3). || ",
            "hits": 120
        },
        {
            "id": 2387,
            "url": "https://svs.gsfc.nasa.gov/2387/",
            "result_type": "Visualization",
            "release_date": "2002-02-28T12:00:00-05:00",
            "title": "The Magnetosphere: Earth Raises its Shields",
            "description": "A view of a computer-generated model of the Earth's magnetosphere. Semi-transparent surfaces represent particle density (red is high, blue is low) and silvery tubes represent the magnetic field lines. In this particular model, the solar wind has an ambient density of 8.35 particles/cm^3. The isosurfaces are then red (> 17 particles/cm^3), yellow (> 12 particles/cm^3), green (> 8.6 particles/cm^3) and blue (< 1.0 particle/cm^3). || ",
            "hits": 208
        },
        {
            "id": 803,
            "url": "https://svs.gsfc.nasa.gov/803/",
            "result_type": "Visualization",
            "release_date": "1999-11-12T12:00:00-05:00",
            "title": "Digital Earth Workbench: The Earth's Magnetic Field",
            "description": "The Digital Earth Workbench is an interactive application that runs on a SGI Onyx Infinite Reality system and is controlled by an Immersive Workbench, tracked stereo glasses, and a tracked wand. The application allows an unprecedented freedom to roam georeferenced data sets at multiple resolutions and timescales. This animation is one of a series of direct screen captures of the application in operation. The occasional menu appearance denotes direct intervention by the operator to add or delete data or to activate a new control option. || ",
            "hits": 110
        },
        {
            "id": 804,
            "url": "https://svs.gsfc.nasa.gov/804/",
            "result_type": "Visualization",
            "release_date": "1999-11-12T12:00:00-05:00",
            "title": "Digital Earth Workbench: Magnetospheric Density",
            "description": "The Digital Earth Workbench is an interactive application that runs on a SGI Onyx Infinite Reality system and is controlled by an Immersive Workbench, tracked stereo glasses, and a tracked wand. The application allows an unprecedented freedom to roam georeferenced data sets at multiple resolutions and timescales. This animation is one of a series of direct screen captures of the application in operation. The occasional menu appearance denotes direct intervention by the operator to add or delete data or to activate a new control option. || ",
            "hits": 101
        },
        {
            "id": 805,
            "url": "https://svs.gsfc.nasa.gov/805/",
            "result_type": "Visualization",
            "release_date": "1999-11-12T12:00:00-05:00",
            "title": "Digital Earth Workbench: Magnetospheric Pressure",
            "description": "The Digital Earth Workbench is an interactive application that runs on a SGI Onyx Infinite Reality system and is controlled by an Immersive Workbench, tracked stereo glasses, and a tracked wand. The application allows an unprecedented freedom to roam georeferenced data sets at multiple resolutions and timescales. This animation is one of a series of direct screen captures of the application in operation. The occasional menu appearance denotes direct intervention by the operator to add or delete data or to activate a new control option. || ",
            "hits": 39
        },
        {
            "id": 111,
            "url": "https://svs.gsfc.nasa.gov/111/",
            "result_type": "Visualization",
            "release_date": "1996-12-12T12:00:00-05:00",
            "title": "Numerical Simulation of Magnetic Flux Emerging Through a Model Solar Atmosphere: Density",
            "description": "This animation is one of a series depicting the results of a two-dimensional ideal magnetohydrodynamic simulation of magnetic flux emerging through a solar atmosphere.  The simulation has a resolution of 300x500 cells and a length scale of 16 Mm x 6.8 Mm.  The simulation depicts 1730 seconds in the evolution of the model. || ",
            "hits": 74
        },
        {
            "id": 112,
            "url": "https://svs.gsfc.nasa.gov/112/",
            "result_type": "Visualization",
            "release_date": "1996-12-12T12:00:00-05:00",
            "title": "Numerical Simulation of Magnetic Flux Emerging Through a Model Solar Atmosphere: Density Gradient",
            "description": "This animation is one of a series depicting the results of a two-dimensional ideal magnetohydrodynamic simulation of magnetic flux emerging through a solar atmosphere.  The simulation has a resolution of 300x500 cells and a length scale of 16 Mm x 6.8 Mm.  The simulation depicts 1730 seconds in the evolution of the model. || ",
            "hits": 39
        },
        {
            "id": 113,
            "url": "https://svs.gsfc.nasa.gov/113/",
            "result_type": "Visualization",
            "release_date": "1996-12-12T12:00:00-05:00",
            "title": "Numerical Simulation of Magnetic Flux Emerging Through a Model Solar Atmosphere: Density, Magnetic Field, and Mach Number",
            "description": "This animation is one of a series depicting the results of a two-dimensional ideal magnetohydrodynamic simulation of magnetic flux emerging through a solar atmosphere.  The simulation has a resolution of 300x500 cells and a length scale of 16 Mm x 6.8 Mm.  The simulation depicts 1730 seconds in the evolution of the model. || ",
            "hits": 20
        },
        {
            "id": 114,
            "url": "https://svs.gsfc.nasa.gov/114/",
            "result_type": "Visualization",
            "release_date": "1996-12-12T12:00:00-05:00",
            "title": "Numerical Simulation of Magnetic Flux Emerging Through a Model Solar Atmosphere: Density Gradient, Magnetic Field, and Mach Number",
            "description": "This animation is one of a series depicting the results of a two-dimensional ideal magnetohydrodynamic simulation of magnetic flux emerging through a solar atmosphere.  The simulation has a resolution of 300x500 cells and a length scale of 16 Mm x 6.8 Mm.  The simulation depicts 1730 seconds in the evolution of the model. || ",
            "hits": 46
        },
        {
            "id": 115,
            "url": "https://svs.gsfc.nasa.gov/115/",
            "result_type": "Visualization",
            "release_date": "1996-12-12T12:00:00-05:00",
            "title": "Numerical Simulation of Magnetic Flux Emerging Through a Model Solar Atmosphere: Density Gradient and Velocities",
            "description": "This animation is one of a series depicting the results of a two-dimensional ideal magnetohydrodynamic simulation of magnetic flux emerging through a solar atmosphere.  The simulation has a resolution of 300x500 cells and a length scale of 16 Mm x 6.8 Mm.  The simulation depicts 1730 seconds in the evolution of the model. || ",
            "hits": 47
        },
        {
            "id": 117,
            "url": "https://svs.gsfc.nasa.gov/117/",
            "result_type": "Visualization",
            "release_date": "1996-12-12T12:00:00-05:00",
            "title": "Global Hybrid Versus MHD Modeling of the Magnetosphere: Magnetic Potential",
            "description": "This series of animations compares a two-dimensional global hybrid simulation with an magnetohydrodynamic model of the interaction of the solar wind with the Earth's magnetosphere. || ",
            "hits": 16
        },
        {
            "id": 1393,
            "url": "https://svs.gsfc.nasa.gov/1393/",
            "result_type": "Visualization",
            "release_date": "1996-12-12T12:00:00-05:00",
            "title": "Global Hybrid Versus MHD Modeling of the Magnetosphere: Density and Magnetic Field",
            "description": "This series of animations compares a two-dimensional global hybrid simulation with an magnetohydrodynamic model of the interaction of the solar wind with the Earth's magnetosphere. || ",
            "hits": 30
        },
        {
            "id": 107,
            "url": "https://svs.gsfc.nasa.gov/107/",
            "result_type": "Visualization",
            "release_date": "1996-05-21T12:00:00-04:00",
            "title": "High Resolution 2-D Numerical Simulation of Emergence of Magnetic Flux Through the Solar Atmosphere",
            "description": "This series of animations (animations 107, 1416, 1417, and 1418) show sheets of magnetic flux undergoing velocity perturbations. The conditions for each simulation are outlined within the video. || ",
            "hits": 42
        },
        {
            "id": 1416,
            "url": "https://svs.gsfc.nasa.gov/1416/",
            "result_type": "Visualization",
            "release_date": "1996-05-21T12:00:00-04:00",
            "title": "High Resolution 2-D Numerical Simulation of Emergence of Magnetic Flux Through the Solar Atmosphere",
            "description": "This series of animations (animations 107, 1416, 1417, and 1418) show sheets of magnetic flux undergoing velocity perturbations. The conditions for each simulation are outlined within the video. || ",
            "hits": 14
        },
        {
            "id": 1417,
            "url": "https://svs.gsfc.nasa.gov/1417/",
            "result_type": "Visualization",
            "release_date": "1996-05-21T12:00:00-04:00",
            "title": "High Resolution 2-D Numerical Simulation of Emergence of Magnetic Flux Through the Solar Atmosphere",
            "description": "This series of animations (animations 107, 1416, 1417, and 1418) show sheets of magnetic flux undergoing velocity perturbations. The conditions for each simulation are outlined within the video. || ",
            "hits": 5
        },
        {
            "id": 1418,
            "url": "https://svs.gsfc.nasa.gov/1418/",
            "result_type": "Visualization",
            "release_date": "1996-05-21T12:00:00-04:00",
            "title": "High Resolution 2-D Numerical Simulation of Emergence of Magnetic Flux Through the Solar Atmosphere",
            "description": "This series of animations (animations 107, 1416, 1417, and 1418) show sheets of magnetic flux undergoing velocity perturbations. The conditions for each simulation are outlined within the video. || ",
            "hits": 8
        },
        {
            "id": 86,
            "url": "https://svs.gsfc.nasa.gov/86/",
            "result_type": "Visualization",
            "release_date": "1995-12-19T12:00:00-05:00",
            "title": "2-D Unstructured Mesh Particle-MHD Solar Wind Flow Over the Earth: Magnetic Potential",
            "description": "This series of animations shows a two-dimensional unstructured mesh particle-magnetohydrodynamic solar wind flow simulation of the interaction of the solar wind with the Earth's magnetosphere. || ",
            "hits": 10
        },
        {
            "id": 87,
            "url": "https://svs.gsfc.nasa.gov/87/",
            "result_type": "Visualization",
            "release_date": "1995-12-19T12:00:00-05:00",
            "title": "2-D Unstructured Mesh Particle-MHD Solar Wind Flow Over the Earth:Density and Magnetic Field",
            "description": "This series of animations shows a two-dimensional unstructured mesh particle-magnetohydrodynamic solar wind flow simulation of the interaction of the solar wind with the Earth's magnetosphere. || ",
            "hits": 38
        }
    ]
}