{
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    "next": null,
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    "results": [
        {
            "id": 5649,
            "url": "https://svs.gsfc.nasa.gov/5649/",
            "result_type": "Visualization",
            "release_date": "2026-06-10T08:00:00-04:00",
            "title": "Four Days of Solar Dynamics in 16 Minutes",
            "description": "The Solar Dynamics Observatory (SDO) is a satellite that orbits Earth and always looks directly at the Sun. It observes the Sun in many wavelengths, which are all helpful in studying different aspects of solar science. In this 16-minute video, we watch the Sun evolve from midnight of February 1, 2026, all the way through 11:59 p.m. on February 4.",
            "hits": 559
        },
        {
            "id": 5577,
            "url": "https://svs.gsfc.nasa.gov/5577/",
            "result_type": "Animation",
            "release_date": "2025-11-20T09:00:00-05:00",
            "title": "SDO Sun This Week",
            "description": "This visualization shows SDO AIA-304 imagery from the past 7 days with a color table and image processing applied. Archive folders are provided in the Download menu.",
            "hits": 404
        },
        {
            "id": 14126,
            "url": "https://svs.gsfc.nasa.gov/14126/",
            "result_type": "Produced Video",
            "release_date": "2022-04-01T00:00:00-04:00",
            "title": "SDO Video Toolkit",
            "description": "The Trebuchet eruption (upper left) as seen in the SDO AIA 304 angstrom filter. This is probably one of the more popular views of the event.4k source files || New_Trebuchet_mkII.00300_print.jpg (1024x576) [336.5 KB] || New_Trebuchet_mkII.00300_print_searchweb.png (320x180) [95.4 KB] || New_Trebuchet_mkII.00300_print_thm.png (80x40) [6.2 KB] || New_Trebuchet_mkII.mp4 (1920x1080) [32.4 MB] || New_Trebuchet_mkII.webm (1920x1080) [3.7 MB] || New_Trebuchet_mkII.mov (1920x1080) [443.3 MB] || New_Trebuchet_mkII.mp4.hwshow [115 bytes] || ",
            "hits": 1061
        },
        {
            "id": 13778,
            "url": "https://svs.gsfc.nasa.gov/13778/",
            "result_type": "Produced Video",
            "release_date": "2020-12-03T17:00:00-05:00",
            "title": "Solar Activity Continues to Rise with 'Anemone' Eruption",
            "description": "Short video showing the solar flare and subsequent prominence eruption and \"arcade\" of loops.Credit: NASA/GSFC/SDOMusic: \"Beautiful Awesome\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Anemone_Eruption_131-171_Blend.jpg (1920x1080) [281.9 KB] || Anemone_Eruption_131-171_Blend_searchweb.png (180x320) [78.6 KB] || Anemone_Eruption_131-171_Blend_thm.png (80x40) [6.6 KB] || 13778_Anemone_Eruption_ProRes_1920x1080_2997.mov (1920x1080) [2.0 GB] || 13778_Anemone_Eruption_Best_1080.mp4 (1920x1080) [718.2 MB] || 13778_Anemone_Eruption_1080.mp4 (1920x1080) [220.6 MB] || 13778_Anemone_Eruption_Best_1080.webm (1920x1080) [16.0 MB] || AnemoneEruption_SRT_Captions.en_US.srt [500 bytes] || AnemoneEruption_SRT_Captions.en_US.vtt [513 bytes] || ",
            "hits": 48
        },
        {
            "id": 4089,
            "url": "https://svs.gsfc.nasa.gov/4089/",
            "result_type": "Visualization",
            "release_date": "2014-02-11T10:00:00-05:00",
            "title": "June 2013's 'Busy Sun'",
            "description": "June of 2013, near the maximum of solar cycle 24, while not extremely active from a solar flare perspective, presented a range of diverse phenomena. We have a couple of solar 'tornadoes' (the twisted protrusions off the limb of the Sun in upper and lower left quadrants), which we eventually see erupt material into space. There are also a number of coronal loops in active regions which are incredibly stable but still exhibit much fine detail. || ",
            "hits": 32
        },
        {
            "id": 4132,
            "url": "https://svs.gsfc.nasa.gov/4132/",
            "result_type": "Visualization",
            "release_date": "2014-02-11T10:00:00-05:00",
            "title": "May 2013: 'Light bulb'-shaped prominence",
            "description": "The active region on the solar limb (left side) generates a large bulb-shaped prominence before demonstrating more energetic activity. See SDO View of a May 2013 Solar Flare. || ",
            "hits": 12
        },
        {
            "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": 37
        }
    ]
}