{
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    "next": null,
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    "results": [
        {
            "id": 12179,
            "url": "http://svs.gsfc.nasa.gov/12179/",
            "result_type": "Produced Video",
            "release_date": "2017-07-25T09:30:00-04:00",
            "title": "NASA Jets Chase The Total Solar Eclipse",
            "description": "For most viewers, the Aug. 21, 2017, total solar eclipse will last less than two and half minutes. But for one team of NASA-funded scientists, the eclipse will last over seven minutes. Their secret? Following the shadow of the Moon in two retrofitted WB-57F jet planes. Amir Caspi of the Southwest Research Institute in Boulder, Colorado, and his team will use two of NASA’s WB-57F research jets to chase the darkness across America on Aug. 21. Taking observations from twin telescopes mounted on the noses of the planes, Caspi will capture the clearest images of the Sun’s outer atmosphere — the corona — to date and the first-ever thermal images of Mercury, revealing how temperature varies across the planet’s surface. || ",
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        {
            "id": 2717,
            "url": "http://svs.gsfc.nasa.gov/2717/",
            "result_type": "Visualization",
            "release_date": "2003-04-11T12:00:00-04:00",
            "title": "Closeup of Solar 'Tadpoles' with time tags",
            "description": "Here is a close-up view of dark 'tentacles' or 'tadpoles' moving towards the solar surface in this solar flare of April 21, 2002 seen by TRACE.  One theory proposed in this press release is that they are due to voids created by magnetic reconnection in the flare.  This version of the visualization displays the instrument clock time tags. || ",
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        {
            "id": 2718,
            "url": "http://svs.gsfc.nasa.gov/2718/",
            "result_type": "Visualization",
            "release_date": "2003-04-11T12:00:00-04:00",
            "title": "Closeup of Solar 'Tadpoles' without time tags",
            "description": "Here is a close-up view of dark 'tentacles' or 'tadpoles' moving towards the solar surface in this solar flare of April 21, 2002 seen by TRACE.  One theory proposed in this press release is that they are due to voids created by magnetic reconnection in the flare.  This version of the visualization does not display the instrument clock time tags. || ",
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        {
            "id": 2655,
            "url": "http://svs.gsfc.nasa.gov/2655/",
            "result_type": "Visualization",
            "release_date": "2002-12-06T12:00:00-05:00",
            "title": "Solar Eclipse: December 4, 2002",
            "description": "A composite of red continuum with SOHO/EIT near totality.  The red image was taken in Ceduna, South Australia.  The images are co-registered so one can install smooth dissolves between them. || Solar eclipse in red continuum || eclipse0002.jpg (1280x960) [46.6 KB] || eclipse0002_web.jpg (320x240) [3.9 KB] || eclipse0002.tif (1280x960) [208.4 KB] || ",
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