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            "id": 2395,
            "url": "https://svs.gsfc.nasa.gov/2395/",
            "result_type": "Visualization",
            "release_date": "2002-03-05T12:00:00-05:00",
            "title": "Pulse of the Planet",
            "description": "Akin to a living creature, Earth's land, air, oceans, ice, and life fit together into a complex, interlocking system.  Space affords a unique vantage point from which to observe the daily, seasonal, and annual changes in Earth's systems. Using data from advanced satellites, NASA visualizations portray a majestic, and sometimes violent, natural world and also capture the influences humans have on the planet.Over 80 NASA-related earth science animations created over the past 8 years implementing realtime and non-realtime techniques have been used on this visual journey.  Tools used included IDL, Lightwave3D, Final Cut Pro, Performer, Vis5D, and custom software. || ",
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        {
            "id": 251,
            "url": "https://svs.gsfc.nasa.gov/251/",
            "result_type": "Visualization",
            "release_date": "1997-11-01T12:00:00-05:00",
            "title": "Images of Earth and Space: SC97 Edition",
            "description": "The entire narrated Images video made for Supercomputing 97 || a000251_pre.jpg (320x238) [8.0 KB] || a000251_thm.png (80x40) [3.8 KB] || a000251_pre_searchweb.jpg (320x180) [45.9 KB] || preview_made_from_dv.00450_print.png (352x240) [104.0 KB] || a000251.webmhd.webm (960x540) [63.8 MB] || a000251.mpg (352x240) [156.0 MB] || ",
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            "url": "https://svs.gsfc.nasa.gov/111/",
            "result_type": "Visualization",
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            "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. || ",
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            "url": "https://svs.gsfc.nasa.gov/112/",
            "result_type": "Visualization",
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            "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. || ",
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            "result_type": "Visualization",
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            "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. || ",
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            "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. || ",
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            "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. || ",
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            "url": "https://svs.gsfc.nasa.gov/117/",
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            "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. || ",
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            "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. || ",
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            "url": "https://svs.gsfc.nasa.gov/116/",
            "result_type": "Visualization",
            "release_date": "1996-10-25T12:00:00-04:00",
            "title": "The HoloGlobe Project (Version 2)",
            "description": "This animation was produced for the Smithsonian Institution's HoloGlobe Exhibit which opened to the public on August 10, 1996. The various orthographic data sets showing progressive global change were mapped onto a rotating globe and projected into space to create a holographic image of the Earth. Showing Earthandapos;s atmosphere, hydrosphere, geosphere, and biosphere are dynamic, changing on timescales of days, minutes, or even seconds. This animation is a revised version of Animation #96 [The HoloGlobe Project (Version 1)]. || ",
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            "url": "https://svs.gsfc.nasa.gov/96/",
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            "title": "The HoloGlobe Project (Version 1)",
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            "url": "https://svs.gsfc.nasa.gov/155/",
            "result_type": "Visualization",
            "release_date": "1996-08-01T12:00:00-04:00",
            "title": "The HoloGlobe Project (Version 3)",
            "description": "These animations were produced for the Smithsonian Institution's HoloGlobe Exhibit which opened to the public on August 10, 1996 at the Museum of Natural History in Washington, DC. The various data sets show progressive global change mapped onto a rotating globe and projected into space to create a holographic image of the Earth. The exhibit shows that Earth's atmosphere, hydrosphere, geosphere, and biosphere are dynamic, changing on timescales of days, minutes, or even seconds. The exhibit has since been relocated to the west coast. This is a revised version from Animation #116 [The HoloGlobe Project (version 2)]. || ",
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            "url": "https://svs.gsfc.nasa.gov/107/",
            "result_type": "Visualization",
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            "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": 46
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            "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. || ",
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            "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": 14
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            "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. || ",
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            "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": 23
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        {
            "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": 24
        },
        {
            "id": 88,
            "url": "https://svs.gsfc.nasa.gov/88/",
            "result_type": "Visualization",
            "release_date": "1995-12-07T12:00:00-05:00",
            "title": "Magnetic Cloud Event: October 18-20, 1995",
            "description": "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. || a000088.00095_web.png (720x480) [357.3 KB] || a000088_thm.png (80x40) [3.9 KB] || a000088_pre.jpg (320x238) [11.4 KB] || a000088_pre_searchweb.jpg (320x180) [49.4 KB] || a000088.webmhd.webm (960x540) [14.4 MB] || a000088.dv (720x480) [186.0 MB] || a000088.mp4 (640x480) [10.5 MB] || a000088.mpg (352x240) [7.8 MB] || ",
            "hits": 40
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        {
            "id": 90,
            "url": "https://svs.gsfc.nasa.gov/90/",
            "result_type": "Visualization",
            "release_date": "1995-11-07T12:00:00-05:00",
            "title": "SAMPEX - Yohkoh: Solar Modification of Relativistic Electrons in the Earth's Radiation Belts",
            "description": "The Solar Anomalous and Magnetospheric Particle Explorer, SAMPEX, measures fluxes of energetic particles from the sun, the Earth's magnetosphere, and cosmic ray sources over a broad range of energies. The four instruments aboard SAMPEX are the Low-Energy Ion Analyzer (LEICA), The Heavy Ion Large Telescope (HILT), The Mass Spectrometer Telescope (MAST), and the Proton-Electron Telescope (PET). The Soft X-ray Telescope on the Yohkoh satellite takes daily full-disk soft X-ray images of the Sun. Comparing data sets from the two satellites allows correlation of electron fluxes in the Earth's radiation belts with solar output. || ",
            "hits": 44
        },
        {
            "id": 81,
            "url": "https://svs.gsfc.nasa.gov/81/",
            "result_type": "Visualization",
            "release_date": "1995-01-11T12:00:00-05:00",
            "title": "Hurricane Florence with Inset of VR Operator",
            "description": "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. || a000081.00005_web.png (720x480) [481.0 KB] || a000081_pre.jpg (320x238) [11.7 KB] || a000081_thm.png (80x40) [6.5 KB] || a000081_pre_searchweb.jpg (320x180) [66.8 KB] || a000081.webmhd.webm (960x540) [26.6 MB] || a000081.dv (720x480) [402.9 MB] || a000081.mp4 (640x480) [22.6 MB] || a000081.mpg (352x240) [12.5 MB] || ",
            "hits": 52
        },
        {
            "id": 82,
            "url": "https://svs.gsfc.nasa.gov/82/",
            "result_type": "Visualization",
            "release_date": "1995-01-11T12:00:00-05:00",
            "title": "Hurricane Florence",
            "description": "An interactive exploration of a computational model of Hurricane Florence using an immersive environment controlled by a boom || a000082.00005_web.png (720x480) [414.0 KB] || a000082_thm.png (80x40) [6.1 KB] || a000082_pre.jpg (320x238) [10.5 KB] || a000082_pre_searchweb.jpg (320x180) [63.9 KB] || a000082.webmhd.webm (960x540) [25.8 MB] || a000082.dv (720x480) [382.5 MB] || a000082.mp4 (640x480) [21.8 MB] || a000082.mpg (352x240) [12.5 MB] || ",
            "hits": 50
        },
        {
            "id": 83,
            "url": "https://svs.gsfc.nasa.gov/83/",
            "result_type": "Visualization",
            "release_date": "1995-01-11T12:00:00-05:00",
            "title": "VR Operator",
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            "hits": 47
        }
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}