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            "id": 12948,
            "url": "https://svs.gsfc.nasa.gov/12948/",
            "result_type": "Produced Video",
            "release_date": "2018-06-18T12:00:00-04:00",
            "title": "Dropped into a Hurricane",
            "description": "Learn one of the ways scientists drop in to study hurricanes. || hs3_33_4k_alt.0344_1024x576.jpg (1024x576) [60.4 KB] || hs3_33_4k_alt.0344.jpg (3840x2160) [895.2 KB] || hs3_33_4k_alt.0344_thm.png (80x40) [5.1 KB] || hs3_33_4k_alt.0344_searchweb.png (320x180) [48.8 KB] || ",
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            "id": 12821,
            "url": "https://svs.gsfc.nasa.gov/12821/",
            "result_type": "Produced Video",
            "release_date": "2018-05-31T09:50:00-04:00",
            "title": "NASA Studies Hurricane Edouard in HS3 Mission (2014)",
            "description": "NASA's Global Hawk in 2014 traveled to the middle of the Atlantic and flew over Hurricane Edouard. Remote sensing nstruments on the plane measured temperature, relative humidity, wind speed, wind direction as well as other data. Along with measurements from the aircraft, NASA scientists also collected data from dropsondes that parachuted down through the hurricane.Complete transcript available.Music: Who Done It? by Robert Leslie Bennett [ASCAP]Watch this video on the NASA Goddard YouTube channel. || 12821_HS3_dropsondes_youtube_1080.00555_print.jpg (1024x576) [53.6 KB] || 12821_HS3_dropsondes_youtube_1080.00555_searchweb.png (320x180) [43.1 KB] || 12821_HS3_dropsondes_youtube_1080.00555_thm.png (80x40) [4.2 KB] || 12821_HS3_dropsondes_1920.mov (1920x1080) [2.7 GB] || 12821_HS3_dropsondes_1920_large.mp4 (1920x1080) [101.8 MB] || 12821_HS3_dropsondes_youtube_1080.mp4 (1920x1080) [152.1 MB] || 12821_HS3_dropsondes_facebook_720.mp4 (1280x720) [112.6 MB] || 12821_HS3_dropsondes.webm (960x540) [40.3 MB] || 12821_HS3_dropsondes_UHD.mov (3840x2160) [11.0 GB] || 12821_HS3_dropsondes_youtube_4k.mp4 (3840x2160) [377.0 MB] || 12821_HS3_dropsondes-captions.en_US.srt [2.1 KB] || 12821_HS3_dropsondes-captions.en_US.vtt [2.1 KB] || ",
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            "id": 4456,
            "url": "https://svs.gsfc.nasa.gov/4456/",
            "result_type": "Visualization",
            "release_date": "2017-08-10T00:00:00-04:00",
            "title": "Global Hawk aircraft observes Hurricane Edouard",
            "description": "This animation shows how NASA scientists used an unmanned Global Hawk aircraft to study Hurricane Edouard. Dropsonde data is compared to SHIS curtain data as the aircraft flies back and forth over the storm.  Relative humidity is displayed with blue representing dry air and red representing moist air.  Additionally, dropsonde wind vector data is displayed using white arrows.  This video is also available on our YouTube channel. || hs3_Eduardo_0650_print.jpg (1024x576) [93.2 KB] || hs3_Eduardo_0650_searchweb.png (320x180) [71.6 KB] || hs3_Eduardo_0650_thm.png (80x40) [6.7 KB] || hs3_Eduardo_1080p30.mp4 (1920x1080) [45.6 MB] || hs3_Eduardo_1080p30.webm (1920x1080) [4.4 MB] || hs3_edouard (3840x2160) [0 Item(s)] || hs3_Eduardo_2160p30.mp4 (3840x2160) [464.2 MB] || hs3_Eduardo_1080p30.mp4.hwshow [185 bytes] || ",
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            "id": 40036,
            "url": "https://svs.gsfc.nasa.gov/gallery/2002hurricane-season/",
            "result_type": "Gallery",
            "release_date": "2010-03-08T00:00:00-05:00",
            "title": "2002 Hurricane Season",
            "description": "No description available.",
            "hits": 37
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            "id": 3536,
            "url": "https://svs.gsfc.nasa.gov/3536/",
            "result_type": "Visualization",
            "release_date": "2008-08-11T12:00:00-04:00",
            "title": "Tropical Storm Edouard",
            "description": "NASA's TRMM spacecraft observed this view of Tropical Storm Edouard on August 5, 2008 as it made landfall in Texas. At this time the storm sustained winds of 55 knots (63 mph). The cloud cover is taken by TRMM's Visible and Infrared Scanner(VIRS) and the GOES spacecraft. The rain structure is taken by TRMM's Tropical Microwave Imager (TMI) and TRMM's Precitation Radar(PR) instruments. TRMM looks underneath of the storm's clouds to reveal the underlying rain structure. Blue represents areas with at least 0.25 inches of rain per hour. Green shows at least 0.5 inches of rain per hour. Yellow is at least 1.0 inches of rain and red is at least 2.0 inches of rain per hour. || ",
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            "id": 2654,
            "url": "https://svs.gsfc.nasa.gov/2654/",
            "result_type": "Visualization",
            "release_date": "2002-12-04T12:00:00-05:00",
            "title": "Tropical Storm Edouard",
            "description": "Closer view of Tropical Storm Edouard off the coast of Florida on September 3, 2002. || edouard_closer.jpg (2560x1920) [1.3 MB] || edouard_closer_web.jpg (320x240) [22.5 KB] || edouard_closer_thm.png (80x40) [7.5 KB] || edouard_closer_web_searchweb.jpg (320x180) [117.8 KB] || edouard_closer.tif (2560x1920) [7.6 MB] || ",
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            "id": 97,
            "url": "https://svs.gsfc.nasa.gov/97/",
            "result_type": "Visualization",
            "release_date": "1996-02-08T12:00:00-05:00",
            "title": "Images of Earth and Space: The Role of Visualization in NASA Science",
            "description": "This compilation video contains visualizations of Earth and Space Sciences resulting from supercomputer models. The excerpted visualizations include: Ocean Planet, El Niño, Ozone 1991, Clouds, Changes in Glacier Bay, Alaska, Biosphere, Lunar Topography from the Clementine Mission, Musculoskeletal Modeling Dynamic Simulations, Simulations of the Breakup and Dynamical Evolution of Comet Shoemaker-Levy 9, Convective Penetration in Stellar Interiors, Topological Features of a Compressible Plasma Vortex Sheet: A Model for the Outer Heliospheric Solar Wind, R-Aquarii Jet, The Evolution of Distorted Black Holes, Rayleigh-Taylor Instability in a Supernova, Galaxy Harassment, N-Body Simulation of the Cold Dark Matter Cosmology. || ",
            "hits": 168
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        {
            "id": 8,
            "url": "https://svs.gsfc.nasa.gov/8/",
            "result_type": "Visualization",
            "release_date": "1993-12-17T12:00:00-05:00",
            "title": "Topological Features of a Compressible Plasma Vortex Sheet: 6 Cases",
            "description": "The Voyager and Pioneer Spacecraft have detected large-scale quasi-periodic plasma fluctuations in the outer heliosphere beyond 20 AU. A plasma vortex sheet model can explain these fluctuations and the observed correlations between various physical variables. The large scale outer heliosphere is modeled by solving the 3-D compressible magnetohydrodynamic equations involving three interacting shear layers.Computations were done on a Cray computer at the NASA Center for Computational Sciences.Six cases are animated: Weak magnetic field and strong magnetic field, each at three values of tau, the vortex street characteristic time. Contours of density are shown as dark transparent 'tubes'. Critical points of the velocity field are represented by 'Glyphs'. Vortex cores are shown in orange and blue. || ",
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            "id": 9,
            "url": "https://svs.gsfc.nasa.gov/9/",
            "result_type": "Visualization",
            "release_date": "1993-12-17T12:00:00-05:00",
            "title": "Topological Features of a Compressible Plasma Vortex Sheet - a Model of the Outer Heliospheric Wind",
            "description": "The Voyager and Pioneer Spacecraft have detected large-scale quasi-periodic plasma fluctuations in the outer heliosphere beyond 20 AU. A plasma vortex sheet model can explain these fluctuations and the observed correlations between various physical variables. The large scale outer heliosphere is modeled by solving the 3-D compressible magnetohydrodynamic equations involving three interacting shear layers. Computations were done on a Cray computer at the NASA Center for Computational Sciences. Six cases are animated: Weak magnetic field and strong magnetic field, each at three values of tau, the vortex street characteristic time. Contours of densityare shown as dark transparent 'tubes'. Critical points of the velocity field are represented by 'Glyphs'. Vortex cores are shown in orange and blue. || ",
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}