{
    "count": 9,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 14516,
            "url": "https://svs.gsfc.nasa.gov/14516/",
            "result_type": "Produced Video",
            "release_date": "2024-02-01T10:00:00-05:00",
            "title": "NASA to Study Effects of Radio Noise on Lunar Science",
            "description": "Watch this video on the NASA Goddard YouTube channel.Music is \"Black Hole\" by Sergey Azbel. || ROLSES_thumb_final.jpg (1280x720) [261.8 KB] || 14516_ROLSES.00886_searchweb.png (320x180) [97.2 KB] || 14516_ROLSES.00886_thm.png (80x40) [7.6 KB] || 14516_ROLSES.mp4 (1440x1080) [156.5 MB] || ROLSES_SOCIAL.en_US.srt [2.2 KB] || ROLSES_SOCIAL.en_US.vtt [2.1 KB] || ",
            "hits": 23
        },
        {
            "id": 13715,
            "url": "https://svs.gsfc.nasa.gov/13715/",
            "result_type": "Produced Video",
            "release_date": "2020-09-15T13:00:00-04:00",
            "title": "How To Track The Solar Cycle",
            "description": "A new solar cycle comes roughly every 11 years. Over the course of each cycle, the Sun transitions from relatively calm to active and stormy, and then quiet again; at its peak, the Sun’s magnetic poles flip. Now that the star has passed solar minimum, scientists expect the Sun will grow increasingly active in the months and years to come.Understanding the Sun’s behavior is an important part of life in our solar system. The Sun’s outbursts—including eruptions known as solar flares and coronal mass ejections—can disturb the satellites and communications signals traveling around Earth, or one day, Artemis astronauts exploring distant worlds. Scientists study the solar cycle so we can better predict solar activity. As of 2020, the Sun has begun to shake off the sleep of minimum, which occurred in December 2019, and Solar Cycle 25 is underway. Scientists use several indicators to track solar cycle progress. || ",
            "hits": 306
        },
        {
            "id": 13291,
            "url": "https://svs.gsfc.nasa.gov/13291/",
            "result_type": "Produced Video",
            "release_date": "2019-08-23T11:30:00-04:00",
            "title": "NASA’s New Solar Scope Is Ready For Balloon Flight",
            "description": "NASA and the Korea Astronomy and Space Science Institute, or KASI, are getting ready to test a new way to see the Sun, high over the New Mexico desert. A pearlescent balloon — large enough to hug a football field — is scheduled to take flight no earlier than Aug. 26, 2019, carrying beneath it a solar scope called BITSE. BITSE is a coronagraph, a kind of telescope that blocks the Sun’s bright face in order to reveal its dimmer atmosphere, called the corona. Short for Balloon-borne Investigation of Temperature and Speed of Electrons in the corona, BITSE seeks to explain how the Sun spits out the solar wind. || ",
            "hits": 79
        },
        {
            "id": 12704,
            "url": "https://svs.gsfc.nasa.gov/12704/",
            "result_type": "Produced Video",
            "release_date": "2017-08-31T12:00:00-04:00",
            "title": "NASA Eclipse Imagery",
            "description": "As millions of people across the United States experienced a total eclipse as the umbra, or Moon’s shadow passed over them, only six people witnessed the umbra from space. Viewing the eclipse from orbit were NASA’s Randy Bresnik, Jack Fischer and Peggy Whitson, ESA (European Space Agency’s) Paolo Nespoli, and Roscosmos’ Commander Fyodor Yurchikhin and Sergey Ryazanskiy. The space station crossed the path of the eclipse three times as it orbited above the continental United States at an altitude of 250 miles. Credit: NASA || iss052e056122.jpg (4928x3280) [844.0 KB] || ",
            "hits": 1240
        },
        {
            "id": 12636,
            "url": "https://svs.gsfc.nasa.gov/12636/",
            "result_type": "Produced Video",
            "release_date": "2017-08-07T00:00:00-04:00",
            "title": "2 Minutes, 6 Hands, 1 Chance",
            "description": "Watch this video on the NASA Goddard YouTube channel.Complete transcript available.Music credit: Patisserie Pressure by Benjamin James Parsons || LARGE_MP4-12636_2Minutes6Hands1ChanceV6_large.02184_print.jpg (1024x576) [159.7 KB] || LARGE_MP4-12636_2Minutes6Hands1ChanceV6_large.02184_searchweb.png (320x180) [112.1 KB] || LARGE_MP4-12636_2Minutes6Hands1ChanceV6_large.02184_thm.png (80x40) [7.9 KB] || APPLE_TV-12636_2Minutes6Hands1ChanceV6_appletv.m4v (1280x720) [86.9 MB] || LARGE_MP4-12636_2Minutes6Hands1ChanceV6_large.webm (1920x1080) [16.4 MB] || APPLE_TV-12636_2Minutes6Hands1ChanceV6_appletv_subtitles.m4v (1280x720) [86.9 MB] || LARGE_MP4-12636_2Minutes6Hands1ChanceV6_large.mp4 (1920x1080) [152.5 MB] || YOUTUBE_1080-12636_2Minutes6Hands1ChanceV6_youtube_1080.mp4 (1920x1080) [244.6 MB] || NASA_TV-12636_2Minutes6Hands1ChanceV6.mpeg (1280x720) [507.3 MB] || YOUTUBE_HQ-12636_2Minutes6Hands1ChanceV6_youtube_hq.mov (1920x1080) [672.4 MB] || NASA_PODCAST-12636_2Minutes6Hands1ChanceV6_ipod_sm.en_US.srt [2.6 KB] || NASA_PODCAST-12636_2Minutes6Hands1ChanceV6_ipod_sm.en_US.vtt [2.6 KB] || NASA_PODCAST-12636_2Minutes6Hands1ChanceV6_ipod_sm.mp4 (320x240) [26.4 MB] || PRORES_B-ROLL-12636_2Minutes6Hands1ChanceV6_prores.mov (1280x720) [2.1 GB] || 12636_2Minutes6Hands1ChanceV6.mov (1920x1080) [4.0 GB] || ",
            "hits": 197
        },
        {
            "id": 12147,
            "url": "https://svs.gsfc.nasa.gov/12147/",
            "result_type": "Produced Video",
            "release_date": "2016-03-03T10:00:00-05:00",
            "title": "2016 Eclipse",
            "description": "Solar scientists Natchimuthuk Gopalswamy, Nelson Reginal, Eric Christian, and Sarah Jaeggli discuss the 2016 eclipse and how it is great preparation for the 2017 eclipse.Complete transcript available. || eclipse_promo_thumb.jpg (1280x720) [53.1 KB] || eclipse_promo_thumb_searchweb.png (320x180) [69.9 KB] || eclipse_promo_thumb_thm.png (80x40) [12.8 KB] || YOUTUBE_HQ_12147_2016.eclipse_promo_V2_youtube_hq.mov (1920x1080) [534.5 MB] || PRORES_B-ROLL_12147_2016.eclipse_promo_V2_prores.mov (1280x720) [1.5 GB] || APPLE_TV_12147_2016.eclipse_promo_V2_appletv.m4v (1280x720) [63.3 MB] || NASA_TV_12147_2016.eclipse_promo_V2.mpeg (1280x720) [383.5 MB] || 12147_2016.eclipse_promo_V2.mov (1920x1080) [2.7 GB] || YOUTUBE_HQ_12147_2016.eclipse_promo_V2_youtube_hq.webm (1920x1080) [11.6 MB] || APPLE_TV_12147_2016.eclipse_promo_V2_appletv_subtitles.m4v (1280x720) [63.4 MB] || 12147_2016_eclipse_PROMO.en_US.srt [2.0 KB] || 12147_2016_eclipse_PROMO.en_US.vtt [2.0 KB] || NASA_PODCAST_12147_2016.eclipse_promo_V2_ipod_sm.mp4 (320x240) [21.4 MB] || ",
            "hits": 292
        },
        {
            "id": 3431,
            "url": "https://svs.gsfc.nasa.gov/3431/",
            "result_type": "Visualization",
            "release_date": "2007-05-29T00:00:00-04:00",
            "title": "Coronal Mass Ejections (CME): Radio Quiet Variety",
            "description": "This is a simple comparison of SOHO/LASCO/C3 difference images (left side) combined with radio data from Wind/WAVES (right side).The LASCO difference images are produced from a time series of images by subtracting the previous image from the current image. Moving material therefore appears white on the leading edge and dark behind it. The WAVES spectrograph shows the variation of radio intensity (black is low, violet is high) in frequency (vertical axis) and time(horizontal axis). A vertical white bar marks the time of the LASCO image.This CME shows no radio-loud emission between 0.2-1.0 MHz. || ",
            "hits": 16
        },
        {
            "id": 3432,
            "url": "https://svs.gsfc.nasa.gov/3432/",
            "result_type": "Visualization",
            "release_date": "2007-05-29T00:00:00-04:00",
            "title": "Coronal Mass Ejections (CME): Radio Loud Variety",
            "description": "This is a simple comparison of SOHO/LASCO/C3 difference images (left side) combined with radio data from Wind/WAVES (right side).The LASCO difference images are produced from a time series of images by subtracting the previous image from the current image.  Moving material therefore appears white on the leading edge and dark behind it.  The WAVES spectrograph shows the variation of radio intensity (black is low, violet is high) in frequency (vertical axis) and time(horizontal axis).  A vertical white bar marks the time of the LASCO image.The radio-loud emission of the CME is the yellow-orange band between 0.2-1.0 MHz. || ",
            "hits": 140
        },
        {
            "id": 2936,
            "url": "https://svs.gsfc.nasa.gov/2936/",
            "result_type": "Visualization",
            "release_date": "2004-05-23T12:00:00-04:00",
            "title": "The fastest CME of Cycle 23 overtakes another fast CME",
            "description": "On November 4, 2003, the Sun produced its fastest coronal mass ejection (CME) for cycle 23 out of the active region 0486 located near the southwest limb of the Sun. The CME was expelled with a speed of approximately 2700 km/s. At the time of the launch of this CME, there was another ejection in progress from the same region. The previous ejection started about 7 hours earlier with a speed of about 1000 km/s. The fastest CME overtook the previous one within 2 hours and produced a spectacular radio radiation detected by the Wind, Ulysses and Cassini spacecraft. The movie shows the radio emission and the two interacting CMEs as observed by the SOHO spacecraft. || ",
            "hits": 389
        }
    ]
}