{
    "count": 15,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 11498,
            "url": "https://svs.gsfc.nasa.gov/11498/",
            "result_type": "Produced Video",
            "release_date": "2014-03-05T09:00:00-05:00",
            "title": "MAVEN Particles & Fields Package",
            "description": "To planetary scientists, the Martian atmosphere presents an intriguing mystery: today it's a thin, cold wisp of carbon dioxide with just one percent the pressure of Earth's atmosphere, but long ago it was thick and warm enough to support lakes and rivers on the Martian surface. How did Mars lose so much of its early atmosphere? Scientists think that the solar wind may be responsible, and NASA's Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft is designed to find out. The instruments of MAVEN's Particles & Fields package will study the interaction of the solar wind with Mars's upper atmosphere, helping scientists to better understand how Mars became the freeze-dried planet that we see today. || ",
            "hits": 78
        },
        {
            "id": 3159,
            "url": "https://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": 45
        },
        {
            "id": 3160,
            "url": "https://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": 52
        },
        {
            "id": 3161,
            "url": "https://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": 41
        },
        {
            "id": 3162,
            "url": "https://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": 23
        },
        {
            "id": 2750,
            "url": "https://svs.gsfc.nasa.gov/2750/",
            "result_type": "Visualization",
            "release_date": "2003-09-02T12:00:00-04:00",
            "title": "RHESSI Observes 2.2 MeV Line Emission from a Solar Flare",
            "description": "The solar flare at Active Region 10039 on July 23, 2002 exhibits many exceptional high-energy phenomena including the 2.223 MeV neutron capture line and the 511 keV electron-positron (antimatter) annihilation line. In the animation, the RHESSI low-energy channels (12-25 keV) are represented in red and appears predominantly in coronal loops. The high-energy flux appears as blue at the footpoints of the coronal loops. Violet is used to indicate the location and relative intensity of the 2.2MeV emission. || ",
            "hits": 30
        },
        {
            "id": 2458,
            "url": "https://svs.gsfc.nasa.gov/2458/",
            "result_type": "Visualization",
            "release_date": "2002-06-05T12:00:00-04:00",
            "title": "RHESSI Observes the Flare over AR9906 - Time Tagged",
            "description": "Close-up view of the solar active region AR9906 on April 21, 2002 with TRACE and RHESSI data. RHESSI observes x-rays from this flare. The red contours represent the 12-25 keV photon energy range and the blue contours represent 50-100 keV. || ",
            "hits": 9
        },
        {
            "id": 2459,
            "url": "https://svs.gsfc.nasa.gov/2459/",
            "result_type": "Visualization",
            "release_date": "2002-06-05T12:00:00-04:00",
            "title": "RHESSI Observes the Flare over AR9906 - No time tags",
            "description": "Close-up view of the solar active region AR9906 on April 21, 2002 with TRACE data and RHESSI. RHESSI observes x-rays from this flare. The red contours represent the 12-25 keV photon energy range and the blue contours represent 50-100 keV. || ",
            "hits": 9
        },
        {
            "id": 2460,
            "url": "https://svs.gsfc.nasa.gov/2460/",
            "result_type": "Visualization",
            "release_date": "2002-06-05T12:00:00-04:00",
            "title": "RHESSI Observes the Flare over AR9906 - zoom with times",
            "description": "Zoom in to solar active region AR9906 on April 21, 2002 with SOHO/EIT, TRACE and RHESSI data. RHESSI observes x-rays from this flare. The red contours represent the 12-25 keV photon energy range and the blue contours represent 50-100 keV. || Movie of RHESSI and TRACE data. || a002460.00100_print.png (720x480) [447.6 KB] || ar9906-zoom-dates_pre.jpg (320x240) [6.9 KB] || a002460.webmhd.webm (960x540) [6.9 MB] || ar9906-zoom-dates.mpg (640x480) [15.0 MB] || a002460.dv (720x480) [118.8 MB] || ",
            "hits": 12
        },
        {
            "id": 2461,
            "url": "https://svs.gsfc.nasa.gov/2461/",
            "result_type": "Visualization",
            "release_date": "2002-06-05T12:00:00-04:00",
            "title": "RHESSI Observes the Flare over AR9906 - zoom without times",
            "description": "Zoom in to solar active region AR9906 on April 21, 2002 with SOHO/EIT, TRACE and RHESSI data. RHESSI observes x-rays from this flare. The red contours represent the 12-25 keV photon energy range and the blue contours represent 50-100 keV. || ",
            "hits": 9
        },
        {
            "id": 2462,
            "url": "https://svs.gsfc.nasa.gov/2462/",
            "result_type": "Visualization",
            "release_date": "2002-06-05T12:00:00-04:00",
            "title": "RHESSI Observes the Flare over AR9906 - rotate view with times",
            "description": "Zoom in (with rotation) to solar active region AR9906 on April 21, 2002 with SOHO/EIT,TRACE and RHESSI data. RHESSI observes x-rays from this flare. The red contours represent the 12-25 keV photon energy range and the blue contours represent 50-100 keV. || ",
            "hits": 11
        },
        {
            "id": 2463,
            "url": "https://svs.gsfc.nasa.gov/2463/",
            "result_type": "Visualization",
            "release_date": "2002-06-05T12:00:00-04:00",
            "title": "RHESSI Observes the Flare over AR9906 - Rotate View Without Times",
            "description": "Zoom in (with rotation) to solar active region AR9906 on April 21, 2002 with SOHO/EIT, TRACE and RHESSI data. RHESSI observes x-rays from this flare. The red contours represent the 12-25 keV photon energy range and the blue contours represent 50-100 keV. || ",
            "hits": 10
        },
        {
            "id": 2402,
            "url": "https://svs.gsfc.nasa.gov/2402/",
            "result_type": "Visualization",
            "release_date": "2002-03-20T12:00:00-05:00",
            "title": "First Flare movie for the RHESSI Instrument (Speed 105x Normal)",
            "description": "An animation of an M-class flare viewed by the RHESSI instrument on February 20, 2002. On tape, this version plays at the maximum speed of one frame corresponding to 3.5 seconds of data collection time. The flare was located at -17.8 degrees South, 9.8 degrees West (heliographic coordinates) in NOAA active region number 9830. || ",
            "hits": 14
        },
        {
            "id": 2403,
            "url": "https://svs.gsfc.nasa.gov/2403/",
            "result_type": "Visualization",
            "release_date": "2002-03-20T12:00:00-05:00",
            "title": "First Flare Movie for the RHESSI Instrument (Speed 52x Normal)",
            "description": "An animation of an M-class flare viewed by the RHESSI instrument on February 20, 2002. On tape, this version plays at a speed of two video frames corresponding to 3.5 seconds of data collection time. The flare was located at -17.8 degrees South, 9.8 degrees West (heliographic coordinates) in NOAA active region number 9830. || ",
            "hits": 7
        },
        {
            "id": 2404,
            "url": "https://svs.gsfc.nasa.gov/2404/",
            "result_type": "Visualization",
            "release_date": "2002-03-20T12:00:00-05:00",
            "title": "First Flare Movie for the RHESSI Instrument (Speed 26x Normal)",
            "description": "An animation of an M-class flare viewed by the RHESSI instrument on February 20, 2002. On tape, this version plays at a speed of four video frames corresponding to 3.75 seconds of data collection time. The flare was located at -17.8 degrees South, 9.8 degrees West (heliographic coordinates) in NOAA active region number 9830. || ",
            "hits": 17
        }
    ]
}