{
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    "next": null,
    "previous": null,
    "results": [
        {
            "id": 3109,
            "url": "https://svs.gsfc.nasa.gov/3109/",
            "result_type": "Visualization",
            "release_date": "2005-02-01T12:00:00-05:00",
            "title": "Solar Irradiance (WMS)",
            "description": "The Earth's climate is determined by energy transfer from the sun to the Earth's land, oceans, and atmosphere.  As the Earth moves around the sun, the fact that the Earth's axis is tilted means that the sun's overhead position moves from the Northern Hemisphere to the Southern Hemisphere and back from one summer to the next.  This effect causes winters to be cold and summers warm in the Northern Hemisphere and the opposite in the Southern Hemisphere.  This animation shows the incoming solar irradiance on the Earth at noon on the Greenwich meridian during an entire year, illustrating this movement.  The magnitude of this irradiance comes from measurements by the TIM instrument on SORCE.  Since the Earth's orbit is elliptical, the magnitude of the solar irradiance at the Earth is least when the Earth is farthest from the sun and greatest when the earth is closest.  This 6 or 7 percent change can be seen in the animation by watching the dark bands move.  When the bands expand from the bright spot, the Earth is getting closer to the sun, from July through December, and when they contract the Earth is moving away, from January through June.  The sun's irradiance is also variable from day to day, but that effect is about ten times smaller than the effect of the earth's orbit. || ",
            "hits": 72
        },
        {
            "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. || ",
            "hits": 25
        },
        {
            "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. || ",
            "hits": 47
        },
        {
            "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": 98
        },
        {
            "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": 67
        }
    ]
}