{
    "count": 6,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 20056,
            "url": "https://svs.gsfc.nasa.gov/20056/",
            "result_type": "Animation",
            "release_date": "2005-03-30T12:00:00-05:00",
            "title": "Earth's Magnetic Field to Aurora",
            "description": "Join a ride with electrons along the Earth's magnetic field line to the formation site of the aurora. || ",
            "hits": 128
        },
        {
            "id": 20057,
            "url": "https://svs.gsfc.nasa.gov/20057/",
            "result_type": "Animation",
            "release_date": "2005-03-30T12:00:00-05:00",
            "title": "A CME Generates Reconnection in Earth's Magnetic Field",
            "description": "A burst of fast material from the Sun generates magnetic reconnection events in the Earth's magnetic field. This eventually sends high-speed electrons and protons into the Earth's upper atmosphere to form aurora. || ",
            "hits": 57
        },
        {
            "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": 118
        },
        {
            "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": 92
        },
        {
            "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": 49
        },
        {
            "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": 50
        }
    ]
}