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    "results": [
        {
            "id": 13939,
            "url": "https://svs.gsfc.nasa.gov/13939/",
            "result_type": "Produced Video",
            "release_date": "2021-09-27T09:55:00-04:00",
            "title": "Hubble Observes Jupiter’s Great Red Spot Changing",
            "description": "Like the speed of an advancing race car driver, the winds in the outermost “lane” of Jupiter’s Great Red Spot are accelerating – a discovery only made possible by NASA’s Hubble Space Telescope, which has monitored the planet for more than a decade. Researchers analyzing Hubble’s regular “storm reports” found that the average wind speed just within the boundaries of the storm, known as a high-speed ring, has increased by up to 8 percent from 2009 to 2020. In contrast, the winds near the red spot’s innermost region are moving significantly more slowly, like someone cruising lazily on a sunny Sunday afternoon. For more information, visit https://nasa.gov/hubble. Music Credits: \"Underneath the same Moon\" by JC Lemay [SACEM] via Koka Media [SACEM], Universal Production Music France [SACEM], and Universal Production Music. || ",
            "hits": 159
        },
        {
            "id": 13279,
            "url": "https://svs.gsfc.nasa.gov/13279/",
            "result_type": "Produced Video",
            "release_date": "2019-08-08T09:55:00-04:00",
            "title": "Hubble’s Brand New Image of Jupiter",
            "description": "This new Hubble Space Telescope view of Jupiter, taken on June 27, 2019, reveals the giant planet's trademark Great Red Spot, and a more intense color palette in the clouds swirling in Jupiter's turbulent atmosphere than seen in previous years. The colors, and their changes, provide important clues to ongoing processes in planetary atmospheres. For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center/Paul Morris/Tracy VogelMusic credits: \"Solaris\" by Axel Tenner [GEMA], Michael Schluecker [GEMA] and Raphael Schalz [GEMA]; Killer Tracks Production Music || ",
            "hits": 60
        },
        {
            "id": 12878,
            "url": "https://svs.gsfc.nasa.gov/12878/",
            "result_type": "Produced Video",
            "release_date": "2018-03-13T13:00:00-04:00",
            "title": "Jupiter's Great Red Spot Shrinks and Grows",
            "description": "NASA scientists have found that not only is Jupiter's Great Red Spot shrinking, but it is actually growing taller and its color is deepening.Music provided by Killer Tracks: \"Moon Leaving\" by Maksim Tyutmanov and Victoria BeitsWatch this video on the NASA.gov Video YouTube channel. || 12878GRSthumbnail_print.jpg (1024x576) [38.9 KB] || 12878GRSthumbnail_searchweb.png (320x180) [29.5 KB] || 12878GRSthumbnail_thm.png (80x40) [3.1 KB] || 12878_GreatRedSpot_YouTubeHD.mp4 (1920x1080) [227.1 MB] || 12878_GreatRedSpot_MASTER.mov (1920x1080) [1.7 GB] || 12878_GreatRedSpot_FacebookHD.mp4 (1920x1080) [182.6 MB] || 12878_GreatRedSpot-Twitter.mp4 (1280x720) [32.9 MB] || 12878_GreatRedSpot_YouTubeHD.webm (1920x1080) [17.1 MB] || 12878GRSthumbnail.tiff (1920x1080) [5.9 MB] || 12878_GreatRedSpot_Captions.en_US.srt [2.5 KB] || 12878_GreatRedSpot_Captions.en_US.vtt [2.5 KB] || ",
            "hits": 131
        },
        {
            "id": 10927,
            "url": "https://svs.gsfc.nasa.gov/10927/",
            "result_type": "Produced Video",
            "release_date": "2012-03-13T13:00:00-04:00",
            "title": "RATTLING JET STREAM ON JUPITER",
            "description": "New movies of Jupiter are the first to catch an invisible wave shaking up one of the giant planet's jet streams, an interaction that also takes place in Earth's atmosphere and influences the weather.For complete transcript, click here. || G2012-013_Jupiter_Weather_portal.00752_print.jpg (1024x576) [69.0 KB] || G2012-013_Jupiter_Weather_portal_web.png (320x180) [190.6 KB] || G2012-013_Jupiter_Weather_portal_thm.png (80x40) [16.5 KB] || G2012-013_Jupiter_Weather.wmv (1280x720) [62.8 MB] || G2012-013_Jupiter_Weather_youtube_hq.mov (1280x720) [70.4 MB] || G2012-013_Jupiter_Weather_appletv.m4v (960x540) [56.5 MB] || G2012-013_Jupiter_Weather_appletv.webmhd.webm (960x540) [27.4 MB] || G2012-013_Jupiter_Weather_portal.mov (640x360) [53.2 MB] || G2012-013_Jupiter_Weather_ipod_lg.m4v (640x360) [22.3 MB] || GSFC_20120313_Jupiter_m10927_Weather.en_US.vtt [2.7 KB] || G2012-013_Jupiter_Weather_prores.mov (1280x720) [1.9 GB] || G2012-013_Jupiter_Weather_ipod_sm.mp4 (320x240) [11.7 MB] || ",
            "hits": 50
        },
        {
            "id": 3636,
            "url": "https://svs.gsfc.nasa.gov/3636/",
            "result_type": "Visualization",
            "release_date": "2009-09-25T00:00:00-04:00",
            "title": "Hubble Space Telescope Observes the Comet P/Shoemaker-Levy 9 Collision with Jupiter",
            "description": "From July 16 through July 22, 1994, pieces of an object designated as Comet P/Shoemaker-Levy 9 collided with Jupiter. This is the first collision of two solar system bodies ever to be observed, and the effects of the comet impacts on Jupiter's atmosphere have been simply spectacular and beyond expectations. Comet Shoemaker-Levy 9 consisted of at least 21 discernable fragments with diameters estimated at up to 2 kilometers. IMPORTANT NOTE: These images are for visualization purposes only. They are not suitable for scientific analysis. || ",
            "hits": 58
        },
        {
            "id": 3520,
            "url": "https://svs.gsfc.nasa.gov/3520/",
            "result_type": "Visualization",
            "release_date": "2009-09-21T00:00:00-04:00",
            "title": "Flow Field Representation of Jupiter's Great Red Spot",
            "description": "This visualization shows a simple simulated flow field representation of Jupiter's Great Red Spot. The flow field is static (i.e., the wind directions don't change over time). This visualization was created in support of the Science On a Sphere film called \"Largest\" which is about Jupiter. These frames were rendered \"flat\" and are intended to be duplicated several times around the sphere. || ",
            "hits": 38
        },
        {
            "id": 3610,
            "url": "https://svs.gsfc.nasa.gov/3610/",
            "result_type": "Visualization",
            "release_date": "2009-09-21T00:00:00-04:00",
            "title": "Jupiter Cloud Sequence from Cassini",
            "description": "When the Cassini mission flew by the planet Jupiter in late 2000, a sequence of full disk images were taken of the planet. Assembled with proper spatial and temporal registration, the sequence could produce fourteen distinct images suitable for wrapping around a sphere.But the time steps between images were large and exhibited significant jumping. The solution was to create additional images between the existing set by interpolation. But simple interpolation would not work due to significant changes between the images.To solve this, we interpolated between the images using the velocity vector field of the cloud images. The velocity vector field was computed by performing a 2-dimensional cross-correlation (Wikipedia: Cross-correlation) between the images. This velocity field was checked against Jupiter velocity profiles from the scientific literature and agreement was excellent. With the addition of a simple vortex flow at the location of the Great Red Spot, the interpolation process was used to generate intermediate images, increasing the total number of images from 14 to 220 and resulting in a smoother animation.  The elapsed time between each interpolated frame corresponds to about 1 hour.  More info on the image sequence is available at Jupiter Mosaics and Movies - Rings, Satellites, AtmosphereIMPORTANT NOTE: These images are for visualization purposes only. They are not suitable for scientific analysis. || ",
            "hits": 119
        },
        {
            "id": 3611,
            "url": "https://svs.gsfc.nasa.gov/3611/",
            "result_type": "Visualization",
            "release_date": "2009-09-21T00:00:00-04:00",
            "title": "Jupiter Cloud Sequence from Voyager 1",
            "description": "When the Voyager 1 mission flew by the planet Jupiter in March of 1979, a sequence of full disk images were taken of the planet. Assembled with proper spatial and temporal registration, the sequence could produce fourteen distinct images suitable for wrapping around a sphere.But the time steps between images were large and exhibited significant jumping and data gaps. The solution was to create additional images between the existing set by interpolation. But simple interpolation would not work due to significant changes between the images.To solve this, we interpolated between the images using the velocity vector field of the cloud images. The velocity vector field was computed by performing a 2-dimensional cross-correlation (Wikipedia: Cross-correlation) between the images. This velocity field was checked against Jupiter velocity profiles from the scientific literature and agreement was excellent. With the addition of a simple vortex flow at the location of the Great Red Spot, the interpolation process was used to generate intermediate images, increasing the total number of images from 14 to 220 and resulting in a smoother animation.IMPORTANT NOTE: These images are for visualization purposes only. They are not suitable for scientific analysis. || ",
            "hits": 75
        },
        {
            "id": 3614,
            "url": "https://svs.gsfc.nasa.gov/3614/",
            "result_type": "Visualization",
            "release_date": "2009-09-21T00:00:00-04:00",
            "title": "Jupiter Cloud Sequence from Voyager 2",
            "description": "When the Voyager 2 mission flew by the planet Jupiter in July of 1979, a sequence of full disk images were taken of the planet. Assembled with proper spatial and temporal registration, the sequence could produce fourteen distinct images suitable for wrapping around a sphere.But the time steps between images were large and exhibited significant jumping and data gaps. The solution was to create additional images between the existing set by interpolation. But simple interpolation would not work due to significant changes between the images.To solve this, we interpolated between the images using the velocity vector field of the cloud images. The velocity vector field was computed by performing a 2-dimensional cross-correlation (Wikipedia: Cross-correlation) between the images. This velocity field was checked against Jupiter velocity profiles from the scientific literature and agreement was excellent. With the addition of a simple vortex flow at the location of the Great Red Spot, the interpolation process was used to generate intermediate images, increasing the total number of images from 14 to 220 and resulting in a smoother animation.IMPORTANT NOTE: These images are for visualization purposes only. They are not suitable for scientific analysis. || ",
            "hits": 74
        }
    ]
}