{
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    "results": [
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            "id": 4501,
            "url": "https://svs.gsfc.nasa.gov/4501/",
            "result_type": "Visualization",
            "release_date": "2016-10-25T10:00:00-04:00",
            "title": "STEREO in stereo: Spring 2007 at 284 Ångstroms",
            "description": "Red/Cyan stereo glasses are required to view it properly. || 2007stereo_STEREO_RedCyan_010_EUVI284A_UHD3840.02000_print.jpg (1024x576) [59.2 KB] || RedCyan (3840x2160) [512.0 KB] || 2007stereo_RedCyan_010_EUVI284A_2160p30.mp4 (3840x2160) [506.4 MB] || 2007stereo_RedCyan_010_EUVI284A_2160p30.webm (3840x2160) [12.7 MB] || ",
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            "id": 3424,
            "url": "https://svs.gsfc.nasa.gov/3424/",
            "result_type": "Visualization",
            "release_date": "2007-04-25T12:00:00-04:00",
            "title": "First 3-D Stereo from STEREO: 284 Angstroms (Active Region)",
            "description": "This movie shows the Sun from the two STEREO spacecraft using the 284 angstrom filter in the Extreme UltraViolet Imager (EUVI). This filter reveals ionized iron (Fe+14=Fe XV), which forms at temperatures above 2x106K, and flows along the magnetic field lines of the solar active regions. New regions come into view as the Sun rotates. || ",
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            "url": "https://svs.gsfc.nasa.gov/3425/",
            "result_type": "Visualization",
            "release_date": "2007-04-25T12:00:00-04:00",
            "title": "First 3-D Stereo from STEREO: EUVI 284 Angstroms (Full Disk View)",
            "description": "This movie shows the Sun from the two STEREO spacecraft using the 284 angstrom filter in the Extreme UltraViolet Imager (EUVI). This filter reveals ionized iron (Fe+14=Fe XV), which forms at temperatures above 2x106K, and flows along the magnetic field lines of the solar active regions. New active regions come into view as the Sun rotates. || ",
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}