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    "results": [
        {
            "id": 4557,
            "url": "https://svs.gsfc.nasa.gov/4557/",
            "result_type": "Visualization",
            "release_date": "2017-03-15T10:00:00-04:00",
            "title": "Leaky Radiation Belts",
            "description": "This visualization opens with a full view of the radiation belt of trapped electrons circling Earth.  We open a slice of the belts, to display a cross-section for clarity and move the camera to a more equatorial view.  Earth rotation and solar motion have been turned off for this visualization to reduce distracting additional motions. || LeakyBelts_FullData_ObliqueIntro.slate_CRTT.HD1080i.0600_print.jpg (1024x576) [113.8 KB] || LeakyBelts_FullData_ObliqueIntro.slate_CRTT.HD1080i.0600_searchweb.png (180x320) [83.0 KB] || LeakyBelts_FullData_ObliqueIntro.slate_CRTT.HD1080i.0600_thm.png (80x40) [6.0 KB] || ObliqueIntro (1920x1080) [0 Item(s)] || LeakyBelts_FullData_ObliqueIntro.HD1080i_p30.mp4 (1920x1080) [77.0 MB] || LeakyBelts_FullData_ObliqueIntro.HD1080i_p30.webm (1920x1080) [5.5 MB] || ObliqueIntro (3840x2160) [0 Item(s)] || LeakyBelts_FullData_ObliqueIntro.UHD2160_p30.mp4 (3840x2160) [279.0 MB] || LeakyBelts_FullData_ObliqueIntro.HD1080i_p30.mp4.hwshow [210 bytes] || ",
            "hits": 52
        },
        {
            "id": 4241,
            "url": "https://svs.gsfc.nasa.gov/4241/",
            "result_type": "Visualization",
            "release_date": "2014-11-26T13:00:00-05:00",
            "title": "Radiation Belts & Plasmapause",
            "description": "Visualization of the radiation belts with confined charged particles (blue & yellow) and plasmapause boundary (blue-green surface) || Earth_BeltsPlasmapauseParticles_Oblique.noslate_GSEmove.HD1080i.0400_print.jpg (1024x576) [136.6 KB] || Earth_BeltsPlasmapauseParticles_Oblique.noslate_GSEmove.HD1080i.0400_web.png (320x180) [96.2 KB] || Earth_BeltsPlasmapauseParticles_Oblique.noslate_GSEmove.HD1080i.0400_searchweb.png (320x180) [96.2 KB] || Earth_BeltsPlasmapauseParticles_Oblique.noslate_GSEmove.HD1080i.0400_thm.png (80x40) [6.9 KB] || BeltsPlasmapauseParticles_HD1080.mov (1920x1080) [28.3 MB] || Earth_BeltsPlasmapauseParticles_Oblique_HD1080.mp4 (1920x1080) [16.6 MB] || BeltsPlasmapauseParticles_HD720.mov (1280x720) [10.6 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || Earth_BeltsPlasmapauseParticles_Oblique_HD1080.webm (960x540) [2.3 MB] || BeltsPlasmapauseParticles_iPod.m4v (640x360) [3.7 MB] || radiation-belts--plasmapause.hwshow [342 bytes] || ",
            "hits": 127
        },
        {
            "id": 3478,
            "url": "https://svs.gsfc.nasa.gov/3478/",
            "result_type": "Visualization",
            "release_date": "2007-12-11T00:00:00-05:00",
            "title": "THEMIS Explores the Earth's Bow Shock",
            "description": "The solar wind's first contact with the Earth's magnetic field creates a region known as the bow shock, much like the bow wave of a boat moving through the water. This region can also create additional turbulence which generates bursts of explosion-like currents. In this visualization, the orbits of the THEMIS fleet are combined with a 2-D slice from a hybrid magnetosphere simulation which illustrates these turbulent regions in the bow shock. This hybrid magnetosphere simulation treats the slow-moving ions by particle-in-cell computational methods and the faster electrons as a massless fluid. These simulations more accurately represent the magnetospheric physics, enabling a view of turbulent non-linear processes not visible in the simpler magnetohydrodynamic models. In this simulation, the color table is somewhat unusual. In order of increasing density, the colors run from white through violet, blue, green to black. || ",
            "hits": 70
        },
        {
            "id": 3310,
            "url": "https://svs.gsfc.nasa.gov/3310/",
            "result_type": "Visualization",
            "release_date": "2005-12-05T00:00:00-05:00",
            "title": "Ionosphere Total Electron Content - April 2001",
            "description": "A view of the ionospheric Total Electron Content (TEC) measured over North America during a storm in April 2001.  Red is high electron counts, blue is low, gray where there is no data.  From the pre-storm state, we see relatively low electron counts.  As the storm intensity increases, so do the number of electrons.  The increase will generate more interference for communications systems, GPS, etc. || ",
            "hits": 59
        },
        {
            "id": 3311,
            "url": "https://svs.gsfc.nasa.gov/3311/",
            "result_type": "Visualization",
            "release_date": "2005-12-05T00:00:00-05:00",
            "title": "Zoom-in to plasmapause-induced TEC enhancement - April 2001",
            "description": "Space weather events which disturb the plasmapause (displayed here as a green surface enclosing the Earth) can propagate down to the Earth's ionosphere.  There they enhance the ionosphere electron content which can disrupt radio signals from satellites.NOTE:  This visualization shows the Earth's magnetic dipole field lines rotating rigidly with the Earth.  Technically, this is inaccurate.  Ions and electrons in the lower atmosphere can create currents which can make these lines 'drag' with Earth's rotation, but this will occur mostly near the Earth and not higher up.  More details on this process can be found in the FAQ at the The Exploration of the Earth's Magnetosphere web site, Does the Earth's magnetic field rotate?. || ",
            "hits": 14
        },
        {
            "id": 3312,
            "url": "https://svs.gsfc.nasa.gov/3312/",
            "result_type": "Visualization",
            "release_date": "2005-12-05T00:00:00-05:00",
            "title": "The 'Big Picture' View of the Plasmapause and Ionospheric Electron Content - April 2001",
            "description": "This visualization presents a wide-angle overview of the plasmapause-Earth system.  Electron content data is mapped to the sphere of the Earth.  As the space storm progresses, the structure of the plasmapause becomes distorted but is still constrained by the structure of the Earth's dipolar magnetic field. || ",
            "hits": 17
        },
        {
            "id": 3313,
            "url": "https://svs.gsfc.nasa.gov/3313/",
            "result_type": "Visualization",
            "release_date": "2005-12-05T00:00:00-05:00",
            "title": "Ionosphere Total Electron Content - November 2003",
            "description": "This movie displays plume formation for a space weather event in November 2003.  In this visualization, the observer is fixed between the Sun and the Earth (slightly off the center line for better perspective).  Blue represents low ionospheric electron counts, dark red is high electron counts. || ",
            "hits": 21
        },
        {
            "id": 3314,
            "url": "https://svs.gsfc.nasa.gov/3314/",
            "result_type": "Visualization",
            "release_date": "2005-12-05T00:00:00-05:00",
            "title": "Time-varying Plasmapause and Electron data - April 2001",
            "description": "This is another view of the plasmapause and electron content data for the April 11, 2001 time frame (similar to ID 3312).  This point of view is shifted slightly to the sunlit side of the Earth to present a better view of the plume formation. || ",
            "hits": 17
        },
        {
            "id": 3316,
            "url": "https://svs.gsfc.nasa.gov/3316/",
            "result_type": "Visualization",
            "release_date": "2005-12-05T00:00:00-05:00",
            "title": "Zoom-in to Plasmapause-Induced TEC Enhancement - April 2001 (Version 2)",
            "description": "Space weather events which disturb the plasmapause (displayed here as a green surface enclosing the Earth) can propagate down to the Earth's ionosphere. There they enhance the ionosphere electron content which can disrupt radio signals from satellites. This movie is a variation on animation ID 3311 with slightly different camera motions. NOTE: This visualization shows the Earth's magnetic dipole field lines rotating rigidly with the Earth. Technically, this is inaccurate. Ions and electrons in the lower atmosphere can create currents which can make these lines 'drag' with Earth's rotation, but this will occur mostly near the Earth and not higher up. More details on this process can be found in the FAQ at the The Exploration of the Earth's Magnetosphere web site, Does the Earth's magnetic field rotate?. || ",
            "hits": 22
        },
        {
            "id": 3317,
            "url": "https://svs.gsfc.nasa.gov/3317/",
            "result_type": "Visualization",
            "release_date": "2005-12-05T00:00:00-05:00",
            "title": "Zoom-in to plasmapause-induced TEC enhancement - April 2001",
            "description": "Space weather events which disturb the plasmapause can propagate down to the Earth's ionosphere.  There they enhance the ionosphere electron content which can disrupt radio signals from satellites.  This is a re-timed version of ID 3311.  This version is designed to play synchronously with ID 3310, ID 3312, and ID 3314.NOTE:  This visualization shows the Earth's magnetic dipole field lines rotating rigidly with the Earth.  Technically, this is inaccurate.  Ions and electrons in the lower atmosphere can create currents which can make these lines 'drag' with Earth's rotation, but this will occur mostly near the Earth and not higher up.  More details on this process can be found in the FAQ at the The Exploration of the Earth's Magnetosphere web site, Does the Earth's magnetic field rotate?. || ",
            "hits": 10
        }
    ]
}