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    "results": [
        {
            "id": 10395,
            "url": "https://svs.gsfc.nasa.gov/10395/",
            "result_type": "Produced Video",
            "release_date": "2009-02-19T00:00:00-05:00",
            "title": "Earth's Energy Budget Animations: Global View and Budget Breakout",
            "description": "Total solar irradiance (TSI) is the dominant driver of the Earth's climate. The global temperature of the Earth is almost completely determined by the balance between the intensity of the incident solar radiation and the response of the Earth's atmosphere via absorption, reflection, and re-radiation. Roughly 30 percent of the TSI that strikes the Earth is reflected back into space by clouds, atmospheric aerosols, snow, ice, desert sand, rooftops, and even ocean surf. The remaining 70 percent of the TSI is absorbed by the land, ocean, and atmosphere. In addition, different layers of the Earth's atmosphere absorb different wavelengths of light. Changes in either the TSI or in the composition of the atmosphere can cause climate change. Two conceptual science animations provide two different perspectives that both illustrate Earth's energy budget. || ",
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        {
            "id": 10198,
            "url": "https://svs.gsfc.nasa.gov/10198/",
            "result_type": "Produced Video",
            "release_date": "2008-05-07T00:00:00-04:00",
            "title": "Striking a Solar Balance",
            "description": "This short film explores the vital connection between the Earth and the Sun.  NASA's Glory mission and the Total Irradiance Monitor will continue nearly three decades of solar irradiance measurments.  This crucial data will contribute to the long-term climate record.For complete transcript, click here. || Striking_a_Solar_Balance_640x48001227_print.jpg (1024x768) [110.2 KB] || Striking_a_Solar_Balance_640x480_web.png (320x240) [213.2 KB] || Striking_a_Solar_Balance_640x480_thm.png (80x40) [13.1 KB] || Striking_a_Solar_Balance_640x480_searchweb.png (320x180) [84.5 KB] || Striking_a_Solar_Balance_720x486_ProRes.webmhd.webm (960x540) [44.9 MB] || Striking_a_Solar_Balance_640x480.mpg (640x480) [118.9 MB] || Striking_a_Solar_Balance_720x486_ProRes.mov (720x486) [972.5 MB] || Striking_a_Solar_Balance_640x480_H264.mov (720x486) [171.0 MB] || Striking_a_Solar_Balance_640x480.m4v (640x480) [39.9 MB] || Striking_a_Solar_Balance_320x240.mp4 (320x240) [17.5 MB] || Striking_a_Solar_Balance.wmv (346x260) [30.4 MB] || ",
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        {
            "id": 2644,
            "url": "https://svs.gsfc.nasa.gov/2644/",
            "result_type": "Visualization",
            "release_date": "2003-01-02T12:00:00-05:00",
            "title": "The Solar 'Constant' - Faculae vs. Sunspots",
            "description": "Three views of the Sun showing different levels of solar activity. The color table has been altered to enhance the appearance of the faculae (white regions) which are hotter than sunspots (red-black regions) and whose greater total area contribute to increasing the solar flux reaching the Earth. || Low solar activity - October 28, 1998 || activity-01-low.jpg (2048x2048) [437.9 KB] || activity-01-low_web.jpg (320x320) [21.2 KB] || activity-01-low.tif (2048x2048) [1.7 MB] || ",
            "hits": 106
        },
        {
            "id": 2656,
            "url": "https://svs.gsfc.nasa.gov/2656/",
            "result_type": "Visualization",
            "release_date": "2003-01-02T12:00:00-05:00",
            "title": "Zoom-out from the Sun",
            "description": "A close-up view of a sunspot group with faculae and pull-out to show the entire Sun. || ",
            "hits": 41
        }
    ]
}