{
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    "results": [
        {
            "id": 10692,
            "url": "http://svs.gsfc.nasa.gov/10692/",
            "result_type": "Produced Video",
            "release_date": "2010-11-15T12:00:00-05:00",
            "title": "IceBridge Antarctic 2010 Video File",
            "description": "Operation IceBridge video file for the Antarctic 2010 campaign. || ",
            "hits": 35
        },
        {
            "id": 3159,
            "url": "http://svs.gsfc.nasa.gov/3159/",
            "result_type": "Visualization",
            "release_date": "2005-05-24T12:00:00-04:00",
            "title": "SOHO/LASCO View of January 2005 Solar Events",
            "description": "The January 20 flare began just before 2 a.m. ET. A storm of energetic protons impacted Earth just 15 minutes later. These views of the flare are from the Solar and Heliospheric Observatory (SOHO). The proton storm near Earth causes `snow' in the images, obscuring the Sun as radiation swamps the cameras. The structure at the 1:30 position in the SOHO/LASCO/C3 data is the occulting disk pylon. || ",
            "hits": 73
        },
        {
            "id": 3160,
            "url": "http://svs.gsfc.nasa.gov/3160/",
            "result_type": "Visualization",
            "release_date": "2005-05-24T12:00:00-04:00",
            "title": "January 2005 Solar Flares from SOHO/EIT",
            "description": "SOHO/EIT's view of the Sun in late January 2005. || fast_eit.0000.jpg (720x480) [44.6 KB] || fast_eit_320x240_pre.jpg (320x240) [8.1 KB] || fast_eit_NTSC.webmhd.webm (960x540) [4.1 MB] || fast_eit_640x480.mpg (640x480) [15.0 MB] || fast_eit_NTSC.m2v (720x480) [24.0 MB] || 720x480_4x3_30 (720x480) [32.0 KB] || a003160_fast_eit_NTSC.mp4 (640x480) [4.8 MB] || fast_eit_320x240.mpg (320x240) [3.9 MB] || ",
            "hits": 41
        },
        {
            "id": 3161,
            "url": "http://svs.gsfc.nasa.gov/3161/",
            "result_type": "Visualization",
            "release_date": "2005-05-24T12:00:00-04:00",
            "title": "TRACE Ultraviolet View of January 20, 2005 Solar Flare",
            "description": "AR 10720 in the TRACE 1600 angstrom band. || fast_trace.0000.jpg (720x480) [59.4 KB] || fast_trace_320x240_pre.jpg (320x240) [9.6 KB] || fast_trace_NTSC.webmhd.webm (960x540) [7.1 MB] || fast_trace_640x480.mpg (640x480) [12.2 MB] || fast_trace_NTSC.m2v (720x480) [19.5 MB] || 720x480_4x3_30 (720x480) [32.0 KB] || a003161_fast_trace_NTSC.mp4 (640x480) [3.9 MB] || fast_trace_320x240.mpg (320x240) [3.1 MB] || ",
            "hits": 25
        },
        {
            "id": 3162,
            "url": "http://svs.gsfc.nasa.gov/3162/",
            "result_type": "Visualization",
            "release_date": "2005-05-24T12:00:00-04:00",
            "title": "RHESSI and TRACE View of January 20, 2005 Solar Flare",
            "description": "RHESSI spacecraft images of gamma-rays (blue) and X-rays (red) thrown off by the hottest part of the flare are shown with UV images from the TRACE spacecraft. The gamma rays are made by energetic protons at the Sun. Scientists were surprised that the gamma rays matched the energy spectrum of protons at Earth: the proton storm may have come directly from the Sun and not from the CME as anticipated. || ",
            "hits": 31
        },
        {
            "id": 90,
            "url": "http://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": 64
        },
        {
            "id": 89,
            "url": "http://svs.gsfc.nasa.gov/89/",
            "result_type": "Visualization",
            "release_date": "1995-01-01T12:00:00-05:00",
            "title": "SAMPEX - A Synoptic View of Earth's Electron Radiation Belts: North Pole Energetic Fluxes from HILT",
            "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). || ",
            "hits": 70
        },
        {
            "id": 1385,
            "url": "http://svs.gsfc.nasa.gov/1385/",
            "result_type": "Visualization",
            "release_date": "1995-01-01T12:00:00-05:00",
            "title": "SAMPEX - A Synoptic View of Earth's Electron Radiation Belts: South Pole Energetic Fluxes from HILT",
            "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). || ",
            "hits": 31
        },
        {
            "id": 1386,
            "url": "http://svs.gsfc.nasa.gov/1386/",
            "result_type": "Visualization",
            "release_date": "1995-01-01T12:00:00-05:00",
            "title": "SAMPEX - A Synoptic View of Earth's Electron Radiation Belts: North Pole Energetic Fluxes from PET",
            "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). || ",
            "hits": 1458
        },
        {
            "id": 1387,
            "url": "http://svs.gsfc.nasa.gov/1387/",
            "result_type": "Visualization",
            "release_date": "1995-01-01T12:00:00-05:00",
            "title": "SAMPEX - A Synoptic View of Earth's Electron Radiation Belts: South Pole Energetic Fluxes from PET",
            "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). || ",
            "hits": 28
        }
    ]
}