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    "results": [
        {
            "id": 31308,
            "url": "https://svs.gsfc.nasa.gov/31308/",
            "result_type": "Hyperwall Visual",
            "release_date": "2024-09-12T00:00:00-04:00",
            "title": "SWOT’s Sea Surface Height Anomaly",
            "description": "SWOT Sea Surface Height Anomaly  This visualization illustrates global Sea Surface Height Anomaly (SSHA) over the oceans and Water Surface Elevation (WSE) on land, as observed by the Surface Water and Ocean Topography (SWOT) satellite during its inaugural science orbit. The SSHA displayed in the animation is derived from along-track high-pass-filtered SWOT SSH data, which effectively removes long-wavelength errors and large-scale ocean signals. SWOT provides detailed measurements of water elevations across various global water bodies, including open and coastal oceans, rivers, and lakes, making it a true global all-water mission. The data gathered will enhance our understanding of small-scale ocean circulations, the ocean's role in Earth's climate, global hydrological circle, and freshwater management worldwide. || swot_oceans-rivers_00000_print.jpg (1024x576) [147.5 KB] || swot_oceans-rivers_00000.png (3840x2160) [3.8 MB] || swot_oceans-rivers_00000_searchweb.png (320x180) [53.8 KB] || swot_oceans-rivers_00000_thm.png (80x40) [4.3 KB] || swot_2024-06-06-A-HD.mp4 (1920x1080) [65.7 MB] || swot_2024-06-06-A-HD.webm (1920x1080) [14.3 MB] || swot_2024-06-06-A-4K.mp4 (3840x2160) [65.8 MB] || ",
            "hits": 181
        },
        {
            "id": 31265,
            "url": "https://svs.gsfc.nasa.gov/31265/",
            "result_type": "Hyperwall Visual",
            "release_date": "2023-11-24T00:00:00-05:00",
            "title": "Global sea surface height by the Surface Water and Ocean Topography (SWOT) mission – the first 21-day cycle",
            "description": "Rotating globe showing sea surface height anomaly || swot_2023-10-30-A.0001_print.jpg (1024x576) [150.8 KB] || swot_2023-10-30-A.0001_searchweb.png (320x180) [45.9 KB] || swot_2023-10-30-A.0001_thm.png (80x40) [4.2 KB] || swot_2023-10-30-A_1080p60.mp4 (1920x1080) [44.5 MB] || swot_2023-10-30-A_1080p60.webm (1920x1080) [8.1 MB] || swot_2023-10-30-A.0001.tif (5760x3240) [13.9 MB] || swot_2023-10-30-A_2160p60.mp4 (3840x2160) [113.5 MB] || swot_2023-10-30-A_1080p60.hwshow [91 bytes] || ",
            "hits": 185
        },
        {
            "id": 30169,
            "url": "https://svs.gsfc.nasa.gov/30169/",
            "result_type": "Hyperwall Visual",
            "release_date": "2013-10-17T12:00:00-04:00",
            "title": "Tropical Storm Leslie",
            "description": "CloudSat overpassed Tropical Storm Leslie in the Atlantic Ocean on August 31, 2012 at 1653 UTC. Leslie contained maximum sustained winds of 65 mph with a minimum central pressure of 999 mb. CloudSat overpassed directly over a developing cumulonimbus cloud with an overshooting cloud top near the center of the storm. This animation combines Cloudsat imagery with an animation of GOES weather satellite images.Tropical Storm Leslie was moving towards the NW and experiencing moderate shear from the NE (note the lack of cirrus canopy in NE portions of the storm). CloudSat overpassed an area of buoyant tropical convection associated with strong updrafts. The overpass reveals the overshooting cloud tops extending over 17 km into the atmosphere and penetrating the lower stratosphere. The CPR signal attenuates in areas of moderate and heavy rainfall, quite evident in the region of the overshooting cloud top. || ",
            "hits": 214
        },
        {
            "id": 30170,
            "url": "https://svs.gsfc.nasa.gov/30170/",
            "result_type": "Hyperwall Visual",
            "release_date": "2013-10-17T12:00:00-04:00",
            "title": "CloudSat's View of Hurricane Sandy",
            "description": "CloudSat passes over Hurricane Sandy || cloudsat_hurr_sandy_print.jpg (1024x576) [128.8 KB] || cloudsat_hurr_sandy_searchweb.png (320x180) [84.2 KB] || cloudsat_hurr_sandy_thm.png (80x40) [18.6 KB] || cloudsat_hurr_sandy_720p.mp4 (1280x720) [4.8 MB] || cloudsat_hurr_sandy_1080p.mp4 (1920x1080) [9.3 MB] || cloudsat_hurr_sandy_720p.webm (1280x720) [4.9 MB] || cloudsat_hurr_sandy_2304p.mp4 (4096x2304) [40.0 MB] || cloudsat_hurr_sandy.tif (4096x2304) [7.6 MB] || ",
            "hits": 117
        },
        {
            "id": 3794,
            "url": "https://svs.gsfc.nasa.gov/3794/",
            "result_type": "Visualization",
            "release_date": "2010-11-09T00:00:00-05:00",
            "title": "STEREO in Stereo: April 8, 2007",
            "description": "Full Disk View: Image sequences taken April 8-9, 2007 by the EUVI telescopes on the two STEREO spacecraft (STEREO-B, left eye; STEREO-A, right eye). At this time the spacecraft were about 3.7 degrees apart. These images show the Sun in extreme ultraviolet light at a wavelength of 171 angstroms, highlighting parts of the Sun's atmosphere (the corona) at about one million degrees C. Note the bright active regions near the Sun's equator and the dark \"coronal holes\" at the north and south poles. These are features of the Sun's magnetic field. Coronal holes are areas where the magnetic field opens out to allow material to flow out into the solar system, while active regions are made up of strong, closed fields which bottle up hot plasma (ionized gas) close to the surface. This image was taken near the minimum in solar activity, so there are few active regions.Closeup View: Image sequences taken April 8-9, 2007 by the EUVI telescopes in the SECCHI imaging suites on the two STEREO spacecraft (STEREO-B, left eye; STEREO-A, right eye). At this time the spacecraft were about 3.7 degrees apart. Here we see a close up of solar magnetic active regions, flickering as they rotate out of sight around the sun. These are areas where the Sun's strong magnetic field bottles up million degree C plasma (ionized gas) low in the corona (the Sun's outer atmosphere). These images are taken at a wavelength of 171 angstroms (0.00000171 cm) in the extreme ultraviolet.Note for Large Displays: These movies are produced using images from STEREO where the angle between the spacecraft is getting larger than the optimum angle for stereo separation. While they work well on small displays, large-screens and projection systems can introduce significant distortions in the stereo effect which the audience may find uncomfortable. When doing large-screen projection, you may need to adjust the left-right image alignment for optimum viewing. However, this does not guarantee a distortion-free result. || ",
            "hits": 42
        },
        {
            "id": 3423,
            "url": "https://svs.gsfc.nasa.gov/3423/",
            "result_type": "Visualization",
            "release_date": "2007-04-25T12:00:00-04:00",
            "title": "First 3-D Stereo from STEREO: EUVI 171 Angstroms (Full Disk View)",
            "description": "This movie shows the Sun from the two STEREO spacecraft using the 171 || ",
            "hits": 111
        },
        {
            "id": 3424,
            "url": "https://svs.gsfc.nasa.gov/3424/",
            "result_type": "Visualization",
            "release_date": "2007-04-25T12:00:00-04:00",
            "title": "First 3-D Stereo from STEREO: 284 Angstroms (Active Region)",
            "description": "This movie shows the Sun from the two STEREO spacecraft using the 284 angstrom filter in the Extreme UltraViolet Imager (EUVI). This filter reveals ionized iron (Fe+14=Fe XV), which forms at temperatures above 2x106K, and flows along the magnetic field lines of the solar active regions. New regions come into view as the Sun rotates. || ",
            "hits": 41
        },
        {
            "id": 3425,
            "url": "https://svs.gsfc.nasa.gov/3425/",
            "result_type": "Visualization",
            "release_date": "2007-04-25T12:00:00-04:00",
            "title": "First 3-D Stereo from STEREO: EUVI 284 Angstroms (Full Disk View)",
            "description": "This movie shows the Sun from the two STEREO spacecraft using the 284 angstrom filter in the Extreme UltraViolet Imager (EUVI). This filter reveals ionized iron (Fe+14=Fe XV), which forms at temperatures above 2x106K, and flows along the magnetic field lines of the solar active regions. New active regions come into view as the Sun rotates. || ",
            "hits": 21
        },
        {
            "id": 3426,
            "url": "https://svs.gsfc.nasa.gov/3426/",
            "result_type": "Visualization",
            "release_date": "2007-04-25T12:00:00-04:00",
            "title": "First 3-D Stereo from STEREO: 304 Angstroms (South Pole View)",
            "description": "This movie shows the Sun from the two STEREO spacecraft using the 304 || ",
            "hits": 26
        },
        {
            "id": 3427,
            "url": "https://svs.gsfc.nasa.gov/3427/",
            "result_type": "Visualization",
            "release_date": "2007-04-25T12:00:00-04:00",
            "title": "First 3-D Stereo from STEREO: EUVI 171 Angstroms (South Pole View)",
            "description": "This movie shows the south pole of the Sun from the two STEREO spacecraft using the 171 angstrom filter in the Extreme UltraViolet Imager (EUVI). This filter reveals ionized iron (Fe+8=Fe IX, Fe+9=Fe X) which forms at temperatures above 1.3x106K, and flows along the magnetic field lines of the solar active regions. New active regions come into view as the Sun rotates. || ",
            "hits": 15
        },
        {
            "id": 3428,
            "url": "https://svs.gsfc.nasa.gov/3428/",
            "result_type": "Visualization",
            "release_date": "2007-04-25T12:00:00-04:00",
            "title": "First 3-D Stereo from STEREO: EUVI 195 Angstroms (Full Disk View)",
            "description": "This movie shows the Sun from the two STEREO spacecraft using the 195 || ",
            "hits": 36
        },
        {
            "id": 3421,
            "url": "https://svs.gsfc.nasa.gov/3421/",
            "result_type": "Visualization",
            "release_date": "2007-04-23T00:00:00-04:00",
            "title": "First 3-D stereo from STEREO: EUVI 171 Ångströms (Active Region)",
            "description": "This movie shows the Sun from the two STEREO spacecraft using the 171 ? filter in the Extreme UltraViolet Imager (EUVI). This filter reveals ionized iron (Fe+8=Fe IX, Fe+9=Fe X) which forms at temperatures above 1.3x106K, and flows along the magnetic field lines of the solar active regions. New regions of solar activity come into view as the Sun rotates left to right. || ",
            "hits": 16
        },
        {
            "id": 3422,
            "url": "https://svs.gsfc.nasa.gov/3422/",
            "result_type": "Visualization",
            "release_date": "2007-04-23T00:00:00-04:00",
            "title": "First 3-D stereo from STEREO: EUVI 304",
            "description": "This movie shows the Sun from the two STEREO spacecraft using the 304 || ",
            "hits": 25
        },
        {
            "id": 558,
            "url": "https://svs.gsfc.nasa.gov/558/",
            "result_type": "Visualization",
            "release_date": "1999-01-21T12:00:00-05:00",
            "title": "Asteroid Castalia Impact Simulation",
            "description": "This visualization shows Castalia, a larger-than-average asteroid, being hit by a house-sized rock traveling at 5 kilometers per second.  Lasting merely a second, the collision approximates the force of the Hiroshima atomic bomb. Using nuclear weapons has been proposed for breaking up, or at least diverting, asteroids headed towards Earth.  Simulations show that such an impact will fracture a solid asteroid, but, later, gravity will reassemble the pieces. || ",
            "hits": 109
        },
        {
            "id": 329,
            "url": "https://svs.gsfc.nasa.gov/329/",
            "result_type": "Visualization",
            "release_date": "1998-10-23T12:00:00-04:00",
            "title": "Images of Earth and Space II",
            "description": "This videotape tours the Solar System and outer space using scientific visualizations from Goddard Space Flight Center, Jet Propulsion Laboratory, and the HPCC Earth and Space Sciences Project. At the Sun, simulations investigate processes that create magnetic field and release energetic particles. Earth science begins with the Pacific Ocean, studying the 1997-98 El Niño and Cyclone Susan. Crossing the globe, visualizations trace North America's East Coast and ocean currents in the North Atlantic Ocean. The lights of the world's cities then show human impact. Next, two models probe nearby-space phenomena, fluid behavior in microgravity conditions and an asteroid collision. A jaunt to Mars explores the mountains and trenches of its dry, rocky exterior. The video concludes at a binary neutron star system, where two city-sized objects with the Sun's mass merge in a titanic explosion. || ",
            "hits": 184
        }
    ]
}