{
    "count": 6,
    "next": null,
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    "results": [
        {
            "id": 4715,
            "url": "https://svs.gsfc.nasa.gov/4715/",
            "result_type": "Visualization",
            "release_date": "2019-06-07T00:00:00-04:00",
            "title": "Swedish Solar Telescope: Solar Closeups",
            "description": "Close-up of Active Region 12593 through the 400 nm filter of the Swedish Solar Telescope.  SDO/HMI provides the background image. || Sept2016_CHROMIS4000A_stand.HD1080i.00100_print.jpg (1024x576) [200.8 KB] || Sept2016_CHROMIS4000A_stand.HD1080i.00100_searchweb.png (180x320) [136.4 KB] || Sept2016_CHROMIS4000A_stand.HD1080i.00100_thm.png (80x40) [9.1 KB] || SwedishST (1920x1080) [0 Item(s)] || Sept2016_CHROMIS4000A.HD1080i_p30.mp4 (1920x1080) [19.4 MB] || Sept2016_CHROMIS4000A.HD1080i_p30.webm (1920x1080) [1.5 MB] || SwedishST (3840x2160) [0 Item(s)] || Sept2016_CHROMIS4000A.UHD3840_2160p30.mp4 (3840x2160) [50.6 MB] || Sept2016_CHROMIS4000A.HD1080i_p30.mp4.hwshow [199 bytes] || ",
            "hits": 129
        },
        {
            "id": 4133,
            "url": "https://svs.gsfc.nasa.gov/4133/",
            "result_type": "Visualization",
            "release_date": "2014-02-11T10:00:00-05:00",
            "title": "February 2013: The Busy Sun",
            "description": "Even near solar maximum, with sunspots dotting the photosphere, the Sun can look tranquil and serene in visible light. In the case of these images from the HMI instrument on the Solar Dynamics Observatory, the only obvious changes are the constant shimmering of the solar disk due to the bubbling of solar granulation.But in ultraviolet light, in particular the 30.4 nanometer line of the helium ion, we see much more activity. Dark, wispy lines of cooler solar filaments (the term used for solar prominences when seen against the disk) stretch across the disk. The same structures, seen against the fainter glow of the solar corona, resemble slowly evolving flames on the limb of the Sun. Solar active regions surrounding the sunspots, appear bright in ultraviolet light. || ",
            "hits": 38
        },
        {
            "id": 3898,
            "url": "https://svs.gsfc.nasa.gov/3898/",
            "result_type": "Visualization",
            "release_date": "2012-01-27T00:00:00-05:00",
            "title": "Growing Sunspots - Tracking Closeup: February 2011",
            "description": "This visualization tracks the emergence and evolution of a sunspot group as seen by SDO/HMI starting in early February 2011 and continuing for two weeks. Images are sampled one hour apart.In this version, the camera tracks the movement of the solar rotation.At this scale, a 'shimmer' of the solar surface is visible, created by the turnover of convection cells. A higher-resolution view of these convection cells can be seen in Hinode imagery (see entry #3412, Hinode's High-resolution view of solar granulation).For a full-disk view of the Sun, covering the same time frame, see entry #3897, Growing Sunspots - A Full Disk View: February 2011. || ",
            "hits": 23
        },
        {
            "id": 3411,
            "url": "https://svs.gsfc.nasa.gov/3411/",
            "result_type": "Visualization",
            "release_date": "2007-03-22T00:00:00-04:00",
            "title": "Hinode's High-Resolution View of the Sun",
            "description": "A  new sunspot collided with an existing sunspot which built up a  highly sheared magnetic configuration.  This resulted in a solar flare on December 13, 2006. || ",
            "hits": 30
        },
        {
            "id": 3412,
            "url": "https://svs.gsfc.nasa.gov/3412/",
            "result_type": "Visualization",
            "release_date": "2007-03-22T00:00:00-04:00",
            "title": "Hinode's High-resolution view of solar granulation",
            "description": "This zoom-in from a full view of the Hinode Solar Optical Telescope (SOT) (the same as in animation 3411) shows details of solar granulation and how rapidly it changes. || ",
            "hits": 155
        },
        {
            "id": 20075,
            "url": "https://svs.gsfc.nasa.gov/20075/",
            "result_type": "Animation",
            "release_date": "2003-03-26T12:00:00-05:00",
            "title": "Wave",
            "description": "Like fans doing the wave at a stadium, large cell-like features called supergranules are moving in a vertical motion, giving the illusion of the solar surface rotating faster than the Sun. || ",
            "hits": 24
        }
    ]
}