{
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    "next": null,
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    "results": [
        {
            "id": 30726,
            "url": "https://svs.gsfc.nasa.gov/30726/",
            "result_type": "Hyperwall Visual",
            "release_date": "2015-11-19T09:00:00-05:00",
            "title": "NuSTAR Stares at the Sun",
            "description": "Blue-White areas in composite image with NuSTAR data show most energetic spots. || nustar_sun_PIA19821_print.jpg (1024x576) [80.4 KB] || nustar_sun_PIA19821_searchweb.png (180x320) [45.4 KB] || nustar_sun_PIA19821_thm.png (80x40) [9.5 KB] || nustar_sun_PIA19821.tif (5760x3240) [10.8 MB] || nustar_sun_30726.key [13.4 MB] || nustar_sun_30726.pptx [10.8 MB] || nustar_sun_PIA19821.hwshow [206 bytes] || ",
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        {
            "id": 2917,
            "url": "https://svs.gsfc.nasa.gov/2917/",
            "result_type": "Visualization",
            "release_date": "2004-02-20T12:00:00-05:00",
            "title": "SORCE Monitors Solar Variability during Record Solar Flares",
            "description": "The SORCE mission monitors solar variability to determine its impact on the Earth's climate. The X-ray photometer aboard SORCE observes the record-breaking solar flares in the Fall of 2003. The line graph shows the photometer's measured solar radiation flux in the 1-7 nanometer wavelength band (x-ray) measured in milliwatts per square meter. The ultraviolet (195 angstrom) imagery from SOHO/EIT (green) illustrates where the flares (the bright white spots) are located on the solar disk. || ",
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            "id": 2918,
            "url": "https://svs.gsfc.nasa.gov/2918/",
            "result_type": "Visualization",
            "release_date": "2004-02-20T12:00:00-05:00",
            "title": "SORCE Monitors Solar Variability during Record Solar Flares - Video version",
            "description": "The SORCE mission monitors solar variability to determine its impact on the Earth's climate. The X-ray photometer aboard SORCE observes the record-breaking solar flares in the Fall of 2003. The line graph shows the photometer's measured solar radiation flux in the 1-7 nanometer wavelength band (x-ray) measured in milliwatts per square meter. The ultraviolet (195 angstrom) imagery from SOHO/EIT (green) illustrates where the flares (the bright white spots) are located on the solar disk. This version has the contents slightly smaller for use in video. || ",
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}