{
    "count": 6,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 14622,
            "url": "https://svs.gsfc.nasa.gov/14622/",
            "result_type": "Produced Video",
            "release_date": "2024-07-03T13:00:00-04:00",
            "title": "Annular Solar Eclipse Broadcast Packages",
            "description": "Watch NASA's live broadcast as a “ring of fire” eclipse travels across the United States on Oct. 14, 2023, from Oregon to Texas. This event occurs when the Moon passes directly in front of the Sun, but appears too small to completely cover the Sun’s surface – resulting in what appears as a ring of fire in the sky. It’s also known as an annular solar eclipse. Everyone in the contiguous 48 states had the opportunity to see at least a partial eclipse on Oct. 14, 2023.Below is the collection of packages created for NASA's annular eclipse broadcast. || ",
            "hits": 24
        },
        {
            "id": 13494,
            "url": "https://svs.gsfc.nasa.gov/13494/",
            "result_type": "Produced Video",
            "release_date": "2019-12-11T13:00:00-05:00",
            "title": "AGU 2019 - New Science from NASA's Parker Solar Probe Mission",
            "description": "Little more than a year into its mission, Parker Solar Probe has returned gigabytes of data on the Sun and its atmosphere. The very first science from the Parker mission is just beginning to be shared, and five researchers presented new findings from the mission at the fall meeting of the American Geophysical Union on Dec. 11, 2019. Their research hints at the processes behind both the Sun's continual outflow of material — the solar wind — and more infrequent solar storms that can disrupt technology and endanger astronauts, along with new insight into space dust that creates the Geminids meteor shower.Speakers:Nicholeen Viall - Research Astrophysicist, NASA's Goddard Space Flight CenterTim Horbury - Professor of Physics, Imperial College LondonKelly Korreck - Astrophysicist, Head of Science Operations for SWEAP Suite, Harvard and Smithsonian Center for AstrophysicsNathan Schwadron - Presidential Chair, Norman S. and Anna Marie Waite Professor, University of New HampshireKarl Battams - Computational Scientist, U.S. Naval Research Laboratory || ",
            "hits": 49
        },
        {
            "id": 12154,
            "url": "https://svs.gsfc.nasa.gov/12154/",
            "result_type": "Produced Video",
            "release_date": "2016-02-18T11:00:00-05:00",
            "title": "Sun Time-lapse",
            "description": "See a year in the life of the sun. || c-1024.jpg (1024x576) [155.9 KB] || c-1280.jpg (1280x720) [212.0 KB] || c-1920.jpg (1920x1080) [363.6 KB] || c-1024_print.jpg (1024x576) [160.5 KB] || c-1024_searchweb.png (320x180) [65.2 KB] || c-1024_web.png (320x180) [65.2 KB] || c-1024_thm.png (80x40) [19.4 KB] || ",
            "hits": 149
        },
        {
            "id": 12144,
            "url": "https://svs.gsfc.nasa.gov/12144/",
            "result_type": "Produced Video",
            "release_date": "2016-02-12T09:00:00-05:00",
            "title": "SDO: Year 6",
            "description": "This ultra-high definition (3840x2160) video shows the sun in the 171 angstrom wavelength of extreme ultraviolet light. It covers a time period of January 2, 2015 to January 28, 2016 at a cadence of one frame every hour, or 24 frames per day.  This timelapse is repeated with narration by solar scientist Nicholeen Viall and contains close-ups and annotations. 171 angstrom light highlights material around 600,000 Kelvin and shows features in the upper transition region and quiet corona of the sun. The video is available to download here at 59.94 frames per second, double the rate YouTube currently allows for UHD content.  The music is titled \"Tides\" and is from Killer Tracks.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || SDO_Year6_HCblend_HD.png (1920x1080) [5.3 MB] || SDO_Year6_HCblend_HD.jpg (1920x1080) [545.9 KB] || SDO_Year6_HCblend_HD_print.jpg (1024x576) [179.5 KB] || SDO_Year6_HCblend_UHD.png (3840x2160) [19.7 MB] || SDO_Year6_HCblend_UHD.jpg (3840x2160) [1.2 MB] || SDO_Year6_HCblend_HD_searchweb.png (180x320) [59.6 KB] || SDO_Year6_HCblend_HD_thm.png (80x40) [4.8 KB] || 12144_SDO_Year_6_appletv.webm (1280x720) [50.5 MB] || 12144_SDO_Year_6_appletv.m4v (1280x720) [241.9 MB] || 12144_SDO_Year_6_appletv_appletv_subtitles.m4v (1280x720) [242.1 MB] || SDO_Year_6_SRT_Captions.en_US.srt [6.3 KB] || SDO_Year_6_SRT_Captions.en_US.vtt [6.3 KB] || 12144_SDO_Year_6_H264_Good_1920x1080_2997.mov (1920x1080) [1.4 GB] || 12144_SDO_Year_6_H264_Good_3840x2160_2997.mov (3840x2160) [9.1 GB] || 12144_SDO_Year_6_H264_Good_3840x2160_5994.mov (3840x2160) [10.2 GB] || 12144_SDO_Year_6_ProRes_3840x2160_5994.mov (3840x2160) [50.3 GB] || ",
            "hits": 96
        },
        {
            "id": 11062,
            "url": "https://svs.gsfc.nasa.gov/11062/",
            "result_type": "Produced Video",
            "release_date": "2012-08-14T00:00:00-04:00",
            "title": "Van Gogh Sun",
            "description": "Why is the sun's atmosphere so much hotter than its surface? To help solve this mystery, a NASA scientist recently analyzed satellite images of the sun in a way that yielded colorful strokes reminiscent of a Van Gogh painting. But this is science, not art. Each processed, color-coded image shows how material in the sun's atmosphere changed temperature over a 24-hour period. Red, yellow and orange were chosen to represent areas that cooled, while blue and green highlight areas that warmed. Watch the videos to see a gallery of these scientific works of art and learn how they were made. || ",
            "hits": 15
        },
        {
            "id": 11046,
            "url": "https://svs.gsfc.nasa.gov/11046/",
            "result_type": "Produced Video",
            "release_date": "2012-07-19T10:00:00-04:00",
            "title": "Van Gogh Sun",
            "description": "A crucial, and often underappreciated, facet of science lies in deciding how to turn the raw numbers of data into useful, understandable information — often through graphs and images. Such visualization techniques are needed for everything from making a map of planetary orbits based on nightly measurements of where they are in the sky to colorizing normally invisible light such as X-rays to produce \"images\" of the sun.More information, of course, requires more complex visualizations and occasionally such images are not just informative, but beautiful too.Such is the case with a new technique created by Nicholeen Viall, a solar scientist at NASA's Goddard Space Flight Center in Greenbelt, Md. She creates images of the sun reminiscent of Van Gogh, with broad strokes of bright color splashed across a yellow background. But it's science, not art. The color of each pixel contains a wealth of information about the 12-hour history of cooling and heating at that particular spot on the sun. That heat history holds clues to the mechanisms that drive the temperature and movements of the sun's atmosphere, or corona.To look at the corona from a fresh perspective, Viall created a new kind of picture, making use of the high resolution provided by NASA's Solar Dynamics Observatory (SDO). SDO's Atmospheric Imaging Assembly (AIA) provides images of the sun in 10 different wavelengths, each approximately corresponding to a single temperature of material. Therefore, when one looks at the wavelength of 171 angstroms, for example, one sees all the material in the sun's atmosphere that is a million degrees Kelvin. By looking at an area of the sun in different wavelengths, one can get a sense of how different swaths of material change temperature. If an area seems bright in a wavelength that shows a hotter temperature an hour before it becomes bright in a wavelength that shows a cooler temperature, one can gather information about how that region has changed over time.Viall's images show a wealth of reds, oranges, and yellow, meaning that over a 12-hour period the material appear to be cooling. Obviously there must have been heating in the process as well, since the corona isn't on a one-way temperature slide down to zero degrees. Any kind of steady heating throughout the corona would have shown up in Viall's images, so she concludes that the heating must be quick and impulsive — so fast that it doesn't show up in her images. This lends credence to those theories that say numerous nanobursts of energy help heat the corona. || ",
            "hits": 32
        }
    ]
}