{
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    "url": "https://svs.gsfc.nasa.gov/10733/",
    "page_type": "Produced Video",
    "title": "SDO First Light Media",
    "description": "A compilation of some of the videos and stills used during the SDO First Light press conference.There are more video and stills available. || ",
    "release_date": "2011-03-03T16:00:00-05:00",
    "update_date": "2023-05-03T13:53:52.565287-04:00",
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        "filename": "10733_SDO_First_Light_Movies_prores_1280x720_29.97.mov",
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    "main_credits": {},
    "progress": "Complete",
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            "description": "This EVE image is showing the raw spectral irradiance data. The ridges are summed to give the actual spectrum. The top part covers wavelengths from 20 to 5 nm (left to right) and the bottom from 37 to 17 nm (left to right. The overlap between 17 and 20 nm is used to better measure that part of the spectrum. In the lower left is a pinhole camera image of the Sun in X-rays with wavelengths between 0.1-7 nm. Credit: NASA/SDO/EVE",
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                        "alt_text": "The Flare that Started the Wave.  Movies of the small (B 3.7) flare that started the wave. In a series of temperature, the start of the wave and the heating of the flare. Credit: NASA/GSFC/SDO/AIA",
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            "title": "SDO Resolution Comparison Resource Page",
            "description": "Ultra High Definition, or 4k, TV has four times as many pixels as a high definition 1080 TV.  NASA's Solar Dynamics Observatory (SDO). Its Atmospheric Imaging Assembly (AIA) and Helioseismic Magnetic Imager (HMI) instruments together capture an image almost once a second that is twice again as large as what the ultra high-def screens can display. Such detailed pictures show features on the sun that are as small as 200 miles across, helping researchers observe such things as what causes giant eruptions on the sun known as coronal mass ejections (CME) that can travel toward Earth and interfere with our satellites. || ",
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