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        {
            "id": 4601,
            "url": "https://svs.gsfc.nasa.gov/4601/",
            "result_type": "Visualization",
            "release_date": "2017-12-18T11:00:00-05:00",
            "title": "Jupiter Quasi-Quadrennial Oscillation",
            "description": "Climate patterns on Jupiter can have striking similarities to those on Earth, making the gas giant a natural laboratory for understanding planetary atmospheres. Complete transcript available.Watch this video on the NASA Goddard YouTube channel.Music provided by Killer Tracks: \"Lights,\" \"Times Waits,\" \"The Space Between\" || JupiterQQOpreview.jpg (1920x1080) [456.5 KB] || TWITTER_720_4601_Jupiter_QQO_Master_APR_twitter_720.mp4 (1280x720) [37.7 MB] || 4601_Jupiter_QQO_Master.webm (960x540) [72.7 MB] || FACEBOOK_720_4601_Jupiter_QQO_Master_APR_facebook_720.mp4 (1280x720) [218.0 MB] || YOUTUBE_HQ_4601_Jupiter_QQO_Master_APR_youtube_hq.mov (1920x1080) [875.9 MB] || 4601_Jupiter_QQO_Master_APR_Output.en_US.srt [3.8 KB] || 4601_Jupiter_QQO_Master_APR_Output.en_US.vtt [3.8 KB] || 4601_Jupiter_QQO_Master_APR.mov (1920x1080) [2.4 GB] || ",
            "hits": 64
        },
        {
            "id": 4469,
            "url": "https://svs.gsfc.nasa.gov/4469/",
            "result_type": "Visualization",
            "release_date": "2016-06-16T15:00:00-04:00",
            "title": "Dynamic Earth-A New Beginning",
            "description": "The visualization 'Excerpt from \"Dynamic Earth\"' has been one of the most popular visualizations that the Scientific Visualization Studio has ever created.  It's often used in presentations and Hyperwall shows to illustrate the connections between the Earth and the Sun, as well as the power of computer simulation in understanding those connections.There is one part of this visualization, however, that has always seemed a little clumsy to us.  The opening shot is a pullback from the limb of the sun, where the sun is represented by a movie of 304 Angstrom images from the Solar Dynamics Observatory (SDO).  It is difficult to pull back from the limb of a flat sun image and make the sun look spherical, and the problem was made more difficult because the original sun images were in a spherical dome show format.  As a result, the pullback from the sun showed some odd reprojection artifacts.The best solution to this issue was to replace the existing pullout with a new one, one which pulled directly out from the center of the solar disk.  For the new beginning, we chose a series of SDO images in the 171 Angstrom channel that show a visible coronal mass ejection (CME) in the lower right corner of the solar disk.  Although this is not the specific CME that is seen affecting Venus and Earth later in this visualization, its presence links the SDO animation  thematically to the later solar storm.  The SDO images were also brightened considerably and tinted yellow to match the common perception of the Sun as a bright yellow object (even though it is actually white).Please go to the original version of this visualization to see the complete credits and additional details. || ",
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        },
        {
            "id": 11906,
            "url": "https://svs.gsfc.nasa.gov/11906/",
            "result_type": "Produced Video",
            "release_date": "2015-06-24T12:00:00-04:00",
            "title": "NASA On Air: NASA Aids European Space Agency In Measuring Upper Air Arctic Winds (6/24/2015)",
            "description": "LEAD: In 2016 the European Space Agency, ESA, will launch a ‘first-of-its-kind' satellite to measure key elements in the earth's wind fields.1. The Aeolus satellite, named after the mythical Greek god of the winds, will measure worldwide upper level winds to help improve weather and climate forecasts.2. NASA recently helped ESA calibrate its new wind instrument by taking simultaneous wind measurements with two Doppler lidars aboard its DC-8 aircraft.TAG: The flights focused over the Arctic since this area holds particular interest due to the continued rise in Arctic temperatures. || WC_Aeolus-1920-MASTER_iPad_1920x0180_print.jpg (1024x576) [101.4 KB] || WC_Aeolus-1920-MASTER_iPad_1920x0180_searchweb.png (320x180) [68.2 KB] || WC_Aeolus-1920-MASTER_iPad_1920x0180_web.png (320x180) [68.2 KB] || WC_Aeolus-1920-MASTER_iPad_1920x0180_thm.png (80x40) [5.7 KB] || WC_Aeolus-1920-MASTER_1920x1080.mov (1920x1080) [625.6 MB] || WC_Aeolus-1920-MASTER_1280x720.mov (1280x720) [711.7 MB] || WC_Aeolus-1920-MASTER_NBC_Today.mov (1920x1080) [269.7 MB] || WC_Aeolus-1920-MASTER_WEA_CEN.wmv (1280x720) [16.1 MB] || WC_Aeolus_converted.avi (1280x720) [16.8 MB] || WC_Aeolus-1920-MASTER_baron.mp4 (1920x1080) [12.6 MB] || WC_Aeolus-1920-MASTER_prores.mov (1920x1080) [435.3 MB] || WC_Aeolus-1920-MASTER_iPad_960x540.m4v (960x540) [80.1 MB] || WC_Aeolus-1920-MASTER_iPad_1280x720.m4v (1280x720) [134.5 MB] || WC_Aeolus-1920-MASTER_iPad_1920x0180.m4v (1920x1080) [269.7 MB] || WC_Aeolus-1920-MASTER_iPad_1920x0180.webm (1920x1080) [3.1 MB] || ",
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        {
            "id": 4171,
            "url": "https://svs.gsfc.nasa.gov/4171/",
            "result_type": "Visualization",
            "release_date": "2014-05-20T00:00:00-04:00",
            "title": "European Jet Stream",
            "description": "Meandering around the planet like a rollicking roller coaster in the sky, the Northern Hemisphere's polar jet stream is a fast-moving belt of westerly winds that traverses the lower layers of the atmosphere. The jet is created by the convergence of cold air masses descending from the Arctic and rising warm air from the tropics. Deep troughs and steep ridges emerge as the denser cold air sinks and deflects warm air regions north, giving the jet stream its wavy appearance. This pattern propagates across the mid-latitudes of North America, Europe and Asia, as pockets of cold air sporadically creep down from the Arctic—creating contrasting waves and flows that accelerate eastward due to Earth's rotation. This visualization uses weather and climate observations from NASA's MERRA data model. || ",
            "hits": 387
        },
        {
            "id": 4148,
            "url": "https://svs.gsfc.nasa.gov/4148/",
            "result_type": "Visualization",
            "release_date": "2014-02-25T00:00:00-05:00",
            "title": "The Polar Jet Stream Over Asia, 2010",
            "description": "Meandering around the planet like a rollicking roller coaster in the sky, the Northern Hemisphere's polar jet stream is a fast-moving belt of westerly winds that traverses the lower layers of the atmosphere. The jet is created by the convergence of cold air masses descending from the Arctic and rising warm air from the tropics. Deep troughs and steep ridges emerge as the denser cold air sinks and deflects warm air regions north, giving the jet stream its wavy appearance. This pattern propagates across the mid-latitudes of North America, Europe and Asia, as pockets of cold air sporadically creep down from the Arctic—creating contrasting waves and flows that accelerate eastward due to Earth's rotation. This visualization was adapted from The Polar Jet Stream (#3864) by special request, using weather and climate observations from NASA's MERRA data model from 2010 for the period of the floods in Russia and the droughts in Pakistan. || ",
            "hits": 88
        },
        {
            "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": 56
        },
        {
            "id": 3864,
            "url": "https://svs.gsfc.nasa.gov/3864/",
            "result_type": "Visualization",
            "release_date": "2011-10-03T00:00:00-04:00",
            "title": "The Polar Jet Stream",
            "description": "Meandering around the planet like a rollicking roller coaster in the sky, the Northern Hemisphere's polar jet stream is a fast-moving belt of westerly winds that traverses the lower layers of the atmosphere. The jet is created by the convergence of cold air masses descending from the Arctic and rising warm air from the tropics. Deep troughs and steep ridges emerge as the denser cold air sinks and deflects warm air regions north, giving the jet stream its wavy appearance. This pattern propagates across the mid-latitudes of North America, Europe and Asia, as pockets of cold air sporadically creep down from the Arctic - creating contrasting waves and flows that accelerate eastward due to Earth's rotation. Running from June 10 to July 8 of 1988, the visualization below uses weather and climate observations from NASA's MERRA dataset to model nearly a month of the jet stream's whirling journey over North America. || ",
            "hits": 1037
        }
    ]
}