{
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    "results": [
        {
            "id": 5625,
            "url": "https://svs.gsfc.nasa.gov/5625/",
            "result_type": "Visualization",
            "release_date": "2026-03-25T00:00:00-04:00",
            "title": "GUARDIAN Warns Hawaii Early of Incoming Kamchatka Tsunami",
            "description": "GUARDIAN is a near-real-time ionospheric monitoring software that uses multi-GNSS total electron content time series to detect natural hazard signatures over the Pacific. Its AI-powered extension, GUARDIAN Scout, automates earthquake and tsunami detection. On July 29, 2025, GUARDIAN detected an incoming tsunami triggered by a magnitude 8.8 Kamchatka earthquake 32 minutes before the earliest tidal gauge detection, demonstrating its life-saving early warning potential.",
            "hits": 977
        },
        {
            "id": 5626,
            "url": "https://svs.gsfc.nasa.gov/5626/",
            "result_type": "Visualization",
            "release_date": "2026-03-25T00:00:00-04:00",
            "title": "GUARDIAN Warns Hawaii Early of Incoming Kamchatka Tsunami (Vertical version)",
            "description": "This data visualizaton show the Kamchatka earthquake, soon followed by GUARDIAN stations G027 and QSPP early warning detections. NOAA's MOST simulation then shows the progression of the tsunami waves across the Pacific Ocean. Guardian station KOKB (Hawaii) picks up the incoming tsunami wave followed by Hawaii's tidal gauge detectors.",
            "hits": 83
        },
        {
            "id": 13688,
            "url": "https://svs.gsfc.nasa.gov/13688/",
            "result_type": "Produced Video",
            "release_date": "2020-08-17T11:45:00-04:00",
            "title": "NASA Explores Earth's Magnetic \"Dent\"",
            "description": "Music: \"Now We Wait\" by Kamal David Kamruddin [PRS]This video can be freely shared and downloaded. While the video in its entirety can be shared without permission, some individual imagery provided by pond5.com and Artbeats is obtained through permission and may not be excised or remixed in other products. Specific details on stock footage may be found here. For more information on NASA’s media guidelines, visit https://www.nasa.gov/multimedia/guidelines/index.html.Complete transcript available. || South_Atlantic_Anomaly_Still_2.jpg (1920x1080) [346.0 KB] || South_Atlantic_Anomaly_Still_2_print.jpg (1024x576) [139.2 KB] || South_Atlantic_Anomaly_Still_2_searchweb.png (320x180) [43.0 KB] || South_Atlantic_Anomaly_Still_2_web.png (320x180) [43.0 KB] || South_Atlantic_Anomaly_Still_2_thm.png (80x40) [4.8 KB] || 13688_South_Atlantic_Anomaly_Fine.mov (1920x1080) [2.6 GB] || 13688_South_Atlantic_Anomaly_Fine.webm (960x540) [65.7 MB] || 13688_South_Atlantic_Anomaly_Fine.mp4 (1920x1080) [292.9 MB] || 13688_South_Atlantic_Anomaly_Fine_lowres.mp4 (1280x720) [52.3 MB] || SAA.en_US.srt [3.5 KB] || SAA.en_US.vtt [3.5 KB] || ",
            "hits": 162
        },
        {
            "id": 4840,
            "url": "https://svs.gsfc.nasa.gov/4840/",
            "result_type": "Visualization",
            "release_date": "2020-08-17T11:00:00-04:00",
            "title": "South Atlantic Anomaly: 2015 through 2025",
            "description": "South Atlantic Anomaly from 2015 through 2025 showing the geomagnetic intensity at the Earth's surface and the core-mantle boundary.  There are versions that include the dates and colorbars and versions without the date and colorbat.This video is also available on our YouTube channel. || saa_intensity_comp2160_p60.4898_print.jpg (1024x576) [58.0 KB] || saa_intensity_comp2160_p60.4898_print_searchweb.png (320x180) [49.9 KB] || saa_intensity_comp2160_p60.4898_print_thm.png (80x40) [3.8 KB] || saa_intensity_comp_1080p30.mp4 (1920x1080) [31.9 MB] || saa_intensity_comp_1080p60.mp4 (1920x1080) [34.4 MB] || saa_intensity_dataOnly_1080_p30.mp4 (1920x1080) [29.3 MB] || saa_intensity_dataOnly_1080_p60.mp4 (1920x1080) [31.3 MB] || saa_intensity_dataOnly_1080_p30.webm (1920x1080) [9.1 MB] || dataOnly (1920x1080) [0 Item(s)] || saa_intensity_comp2160_p30.mp4 (3840x2160) [86.1 MB] || saa_intensity_comp2160_p60.mp4 (3840x2160) [93.1 MB] || comp (3840x2160) [0 Item(s)] || captions_silent.29860.en_US.srt [43 bytes] || saa_intensity_dataOnly_1080_p30.mp4.hwshow [197 bytes] || ",
            "hits": 1437
        },
        {
            "id": 4773,
            "url": "https://svs.gsfc.nasa.gov/4773/",
            "result_type": "Visualization",
            "release_date": "2019-12-12T03:30:00-05:00",
            "title": "BedMachine: A high-precision map of Antarctic ice sheet bed topography",
            "description": "BedMachine is a new Antarctic bed topography product based on ice thickness data from 19 different research institutes dating back to 1967, encompassing nearly a million line-miles of radar soundings. BedMachine relies on the fundamental physics-based method of mass conservation to estimate what lies between the radar sounding lines, utilizing highly detailed information on ice flow motion from satellite data that dictates how ice moves. The dataset is available from the National Snow & Ice Data Center here. || ",
            "hits": 354
        },
        {
            "id": 13446,
            "url": "https://svs.gsfc.nasa.gov/13446/",
            "result_type": "Produced Video",
            "release_date": "2019-11-25T00:00:00-05:00",
            "title": "Operation IceBridge - Instrument Panels",
            "description": "NASA's P-3B and DC-8 airborne laboratories have been the workhorses of Operation IceBridge. These aircraft house several sophisticated instruments for measuring snow depth, ice elevation and thickness, surface temperature, bed topography and other characteristics of sea ice, ice sheets and glaciers.The airborne laboratories have been joined by other aircraft, such as NASA's C-130 Hercules, King Air B-200 and HU-25C Falcon, the Gulfstream G-V owned by the National Science Foundation and operated by NCAR’s Research Aviation Facility, the University of Texas Institute for Geophysics' (UTIG) chartered Kenn Borek Basler BT-67, and a variety of small planes used by researchers from the University of Alaska-Fairbanks (UAF). These aircraft increase the number of instruments IceBridge can field at one time, greatly expand the geographic area covered and add a higher-altitude perspective on polar ice. || ",
            "hits": 20
        },
        {
            "id": 4670,
            "url": "https://svs.gsfc.nasa.gov/4670/",
            "result_type": "Visualization",
            "release_date": "2018-08-01T09:00:00-04:00",
            "title": "Geothermal Heat Flux Reveals the Iceland Hotspot Track underneath Greenland",
            "description": "This visualization shows the Greenland geothermal heat flux map, the track of the Iceland hotspot through Greenland, and the plate tectonic motion of Greenland over the hotspot during the past 100 million years.This video is also on the NASA YouTube channel. || hotspot.0240_print.jpg (1024x576) [157.4 KB] || hotspot.0240_searchweb.png (320x180) [100.2 KB] || hotspot.0240_thm.png (80x40) [7.9 KB] || hotspot_1080p30.mp4 (1920x1080) [17.1 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || hotspot_720p30.mp4 (1280x720) [8.7 MB] || hotspot_720p30.webm (1280x720) [3.0 MB] || hotspot_360p30.mp4 (640x360) [3.4 MB] || hotspot_1080p30.mp4.hwshow [181 bytes] || ",
            "hits": 150
        },
        {
            "id": 13025,
            "url": "https://svs.gsfc.nasa.gov/13025/",
            "result_type": "Produced Video",
            "release_date": "2018-08-01T09:00:00-04:00",
            "title": "NASA Scientist Reveals Greenland's Geologic Past",
            "description": "A new map of Greenland's geothermal heat flux is helping to reveal the path of the North American tectonic plate over geologic time. Complete transcript available.Watch this video on the NASA Goddard YouTube channel.Music Provided by Killer Tracks: \"Valfri\" by James Alexander Dorman || FACEBOOK_720_13025_Greenland_Hotspot_MASTER_facebook_720.mp4 (1280x720) [173.9 MB] || Greenland_Tectonic_Preview_print.jpg (1024x576) [383.0 KB] || Greenland_Tectonic_Preview.jpg (3840x2160) [3.0 MB] || Greenland_Tectonic_Preview_searchweb.png (320x180) [136.6 KB] || Greenland_Tectonic_Preview_thm.png (80x40) [8.8 KB] || TWITTER_720_13025_Greenland_Hotspot_MASTER_twitter_720.mp4 (1280x720) [28.6 MB] || 13025_Greenland_Hotspot_MASTER.webm (960x540) [53.0 MB] || YOUTUBE_1080_13025_Greenland_Hotspot_MASTER_youtube_1080.mp4 (1920x1080) [228.2 MB] || YOUTUBE_1080_13025_Greenland_Hotspot_MASTER_youtube_1080_Output.en_US.srt [2.5 KB] || YOUTUBE_1080_13025_Greenland_Hotspot_MASTER_youtube_1080_Output.en_US.vtt [2.5 KB] || YOUTUBE_4K_13025_Greenland_Hotspot_MASTER_youtube_4k.mp4 (3840x2160) [543.3 MB] || 13025_Greenland_Hotspot_MASTER_youtube_hq.mov (3840x2160) [1.3 GB] || 13025_Greenland_Hotspot_MASTER.mov (3840x2160) [6.3 GB] || ",
            "hits": 71
        },
        {
            "id": 4634,
            "url": "https://svs.gsfc.nasa.gov/4634/",
            "result_type": "Visualization",
            "release_date": "2018-06-28T09:00:00-04:00",
            "title": "Global Fire Weather Database",
            "description": "The Global Fire WEather Database (GFWED) integrates different weather factors influencing the likelihood of a vegetation fire starting and spreading. It is based on the Fire Weather Index (FWI) System, which tracks the dryness of three general fuel classes, and the potential behavior of a fire if it were to start. Each day, FWI values are calculated from global weather data, including satellite rainfall data from the Global Precipitation Measurement (GPM) mission.The FWI System is the most widely used fire danger rating system in the world, and has been adopted for different boreal, temperate and tropical fire environments. GFWED provides a globally consistent fire weather dataset for fire researchers and managers to apply locally. The Fire Weather Index component is suitable as a general index of fire danger. Globally, shifts in continental-scale fire activity follow seasonal changes in the FWI. Over South America and Africa, regions of high FWI and active agricultural burning shift with the tropical rain belts, seen in the GPM precipitation overlay. Over North America and Eurasia, the FWI will ‘activate’ in the spring, and shows how week-to-week surges in fire activity can be driven by high FWI values. || ",
            "hits": 118
        },
        {
            "id": 12811,
            "url": "https://svs.gsfc.nasa.gov/12811/",
            "result_type": "Produced Video",
            "release_date": "2017-12-20T16:00:00-05:00",
            "title": "Our Home Planet (NASM 2017)",
            "description": "NASA explores. From the far reaches of the cosmos, to right here at home, NASA scientists are uncovering new insights that provide economic and societal benefits to the U.S. and the world.Since NASA was created nearly six decades ago, we have essentially \"discovered\" how Earth works as a system. It continues to be a fascinating exercise in fundamental science. And we are still discovering.Complete transcript available. || NASM_2017_Our_Home_Planet.00001_print.jpg (1024x576) [141.9 KB] || NASM_2017_Our_Home_Planet.00001_searchweb.png (320x180) [92.1 KB] || NASM_2017_Our_Home_Planet.00001_thm.png (80x40) [6.8 KB] || NASM_2017_Our_Home_Planet_prores.mov (1280x720) [35.3 GB] || NASM_2017_Our_Home_Planet_large.mp4 (1280x720) [2.5 GB] || NASM_2017_Our_Home_Planet.mp4 (1280x720) [4.9 GB] || NASM_2017_Our_Home_Planet_youtube_1080.mp4 (1920x1080) [4.1 GB] || NASM_2017_Our_Home_Planet_appletv.m4v (1280x720) [1.3 GB] || NASM_2017_Our_Home_Planet.webm (1280x720) [275.6 MB] || NASM-2017-captions-20180830.en_US.srt [47.1 KB] || NASM-2017-captions-20180830.en_US.vtt [47.1 KB] || ",
            "hits": 22
        },
        {
            "id": 12456,
            "url": "https://svs.gsfc.nasa.gov/12456/",
            "result_type": "Produced Video",
            "release_date": "2016-12-12T18:45:00-05:00",
            "title": "Tracking Ocean Heat With Magnetic Fields",
            "description": "As Earth warms, much of the extra heat is stored in the planet’s ocean – but monitoring the magnitude of that heat content is a difficult task. A surprising feature of the tides could help, however. Scientists at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, are developing a new way to use satellite observations of magnetic fields to measure heat stored in the ocean.Music: War Torn by Brad Smith [BMI] Complete transcript available.Watch this video on the NASA Goddard YouTube channel. || 12456-ocean-heat-AGU-web.jpg (1920x1080) [354.1 KB] || 12456-ocean-heat-AGU-web_searchweb.png (320x180) [122.0 KB] || 12456-ocean-heat-AGU-web_thm.png (80x40) [7.7 KB] || 12456-ocean-heat-APR_VX-680579_large.mp4 (1920x1080) [59.1 MB] || 12456-ocean-heat-APR_VX-680579_appletv.m4v (1280x720) [30.6 MB] || 12456-ocean-heat-AGU-720p.mp4 (1280x720) [59.5 MB] || 12456-ocean-heat-AGU.mp4 (1920x1080) [59.9 MB] || 12456-ocean-heat-APR_VX-680579.webm (960x540) [23.6 MB] || 12456-ocean-heat-APR_VX-680579_appletv_subtitles.m4v (1280x720) [30.7 MB] || 12456-ocean-heat-captions.en_US.srt [891 bytes] || 12456-ocean-heat-captions.en_US.vtt [904 bytes] || 12456-ocean-heat-APR_VX-680579_ipod_sm.mp4 (320x240) [10.9 MB] || 12456-ocean-heat-APR_VX-680579_prores.mov (1280x720) [791.2 MB] || 12456-ocean-heat-APR_VX-680579_youtube_hq.mov (1920x1080) [212.0 MB] || 12456-ocean-heat-APR_VX-680579.mpeg (1280x720) [196.6 MB] || ",
            "hits": 44
        },
        {
            "id": 12450,
            "url": "https://svs.gsfc.nasa.gov/12450/",
            "result_type": "Produced Video",
            "release_date": "2016-12-12T18:30:00-05:00",
            "title": "Ocean Tides and Magnetic Fields",
            "description": "Seawater is an electrical conductor, and therefore interacts with the magnetic field.  As the tides cycle around the ocean basins, the ocean water essentially tries to pull the geomagnetic field lines along.Because the salty water is a good, but not great, conductor, the interaction is relatively weak.  Scientists at NASA Goddard Space Flight Center are developing improved methods to isolate the signal from ocean tides and use that information to determine the heat content of the ocean.Music: \"Memory Of A Lifetime\" by J Ehrlich [SESAC], Jean-Christophe Beck [BMI]Complete transcript available.Watch this video on the NASA Goddard YouTube channel. || 12450-Tidal-Magnetic-Animation-APR_large.00545_print.jpg (1024x576) [189.1 KB] || 12450-Tidal-Magnetic-Animation-APR_large.00545_searchweb.png (320x180) [93.6 KB] || 12450-Tidal-Magnetic-Animation-APR_large.00545_thm.png (80x40) [5.8 KB] || 12450-Tidal-Magnetic-Animation-APR.webm (960x540) [26.5 MB] || 12450-Tidal-Magnetic-Animation-APR_prores.mov (1280x720) [989.0 MB] || 12450-Tidal-Magnetic-Animation-APR_large.mp4 (1920x1080) [66.1 MB] || 12450-Tidal-Magnetic-Animation-APR_youtube_hq.mov (1920x1080) [1.0 GB] || 12450-Tidal-Magnetic-Animation-APR_appletv.m4v (1280x720) [32.1 MB] || 12450-Tidal-Magnetic-Animation-APR_appletv_subtitles.m4v (1280x720) [32.2 MB] || 1920x1080_16x9_30p (1920x1080) [128.0 KB] || 12450-Tidal-Magnetic-Animation.en_US.srt [1.4 KB] || 12450-Tidal-Magnetic-Animation.en_US.vtt [1.4 KB] || 12450-Tidal-Magnetic-Animation-APR_ipod_sm.mp4 (320x240) [11.5 MB] || ",
            "hits": 324
        },
        {
            "id": 30476,
            "url": "https://svs.gsfc.nasa.gov/30476/",
            "result_type": "Hyperwall Visual",
            "release_date": "2013-11-01T15:00:00-04:00",
            "title": "Mount Etna",
            "description": "Twin volcanic plumes—one of ash, one of gas—rose from Sicily’s Mount Etna on the morning of October 26, 2013. L’Istituto Nazionale di Geofisica e Vulcanologia (INGV) Osservatorio Etneo (National Institute of Geophysics and Volcanology Etna Observatory) reported that Etna was experiencing its first paroxysm in six months. Multiple eruption columns are common at Etna, a result of complex plumbing within the volcano. The Northeast Crater, one of several on Etna’s summit, was emitting the ash column, while the New Southeast Crater was simultaneously venting mostly gas.This natural-color image collected by Landsat 8 shows the view from space at 11:38 a.m. local time. The towering, gas-rich plume cast a dark shadow over the lower, ash-rich plume and Etna’s northwestern flank. Relatively fresh lava flows (less than a century or so old) are dark gray; vegetation is green; and the tile-roofed buildings of Bronte and Biancavilla lend the towns an ochre hue. || ",
            "hits": 128
        },
        {
            "id": 11274,
            "url": "https://svs.gsfc.nasa.gov/11274/",
            "result_type": "Produced Video",
            "release_date": "2013-06-20T00:00:00-04:00",
            "title": "Antarctica Exposed",
            "description": "Our understanding of what lies beneath the world's biggest ice sheet has taken another leap forward. Thanks to work led by the British Antarctic Survey, scientists have a new 3D map of Antarctica’s ice and bedrock. The map, called Bedmap2, incorporates millions of new measurements, including data collected by NASA's ICESat satellite and airborne Operation IceBridge mission. The result is a virtual reconstruction of the continent’s bedrock topography and ice layers captured in never-before-seen detail. Antarctica plays a large role in the global climate system. The melting and emptying of its ice into the sea influences ocean currents and the rate of sea level rise. By having a precise map of Antarctica’s mountains, ridges, slopes and valleys—all of which affect how fast the continent's ice travels across the ice sheet—scientists can better predict future rates of ice flow. Watch the video to learn more. || ",
            "hits": 296
        },
        {
            "id": 4060,
            "url": "https://svs.gsfc.nasa.gov/4060/",
            "result_type": "Visualization",
            "release_date": "2013-06-04T10:00:00-04:00",
            "title": "Antarctic Bedrock",
            "description": "<!——><!—Above: Move bar to compare the bedrock topography (left) to the ice sheet surface (right).Download HTML to embed this in your web page.The topography of the bedrock under the Antarctic Ice Sheet is critical to understanding the dynamic motion of the ice sheet, its thickness and its influence on the surrounding ocean and global climate. In 2001, the British Antarctic Survey (BAS) released a map of the bed under the Antarctic Ice Sheet and the seabed extending out on to the continental shelf derived from data collected by an international consortium of scientists over the prior fifty years. The resulting dataset was called BEDMAP (or BEDMAP1).In 2013, BAS released an update of the topographic dataset called BEDMAP2 that incorporates twenty-five million measurements taken over the past two decades from the ground, air and space. This visualization compares the new BEDMAP2 dataset to the original BEDMAP1 dataset showing the improvements in resolution and coverage. <!——><!—Above: Move bar to compare the Bedmap1 topography (left) to the Bedmap2 topography (right). Download HTML to embed this in your web page.Since 2009, NASA's mission Operation IceBridge (OIB) has flown aircraft over the Antarctic Ice Sheet carrying laser and ice-penetrating radar instruments to collect data about the surface height, bedrock topography and ice thickness. This visualization highlights the contribution that OIB has made to this important dataset.The topography in this visualization is exaggerated to emphasize the topographic relief. The amount of exaggeration varies based on the viewpoint, from twenty times in distant views down to nine times when near the Pine Island Bay. || ",
            "hits": 241
        },
        {
            "id": 3886,
            "url": "https://svs.gsfc.nasa.gov/3886/",
            "result_type": "Visualization",
            "release_date": "2013-05-16T14:00:00-04:00",
            "title": "Regional Rates of Glacier Loss for 2003 to 2009",
            "description": "In the image below, global glacial mass loss and area are summarized by regions. The area of the red circles corresponds to the annual glacial mass loss from 2003 to 2009. Glacier mass change estimates are determined from a combination of satellite altimetry (ICESat), satellite gravimetry (GRACE) and in situ field observations as determined by Gardner et al. Light orange halos surrounding red circles show the 95% confidence interval in mass change estimates, but can only be seen in regions with large uncertainties.The area of the green/blue circles depicts total glacier area for each region with the tidewater basin fractions [TW] shown separately in blue. The geographic locations of all glaciers, evident primarily in mountainous regions and high latitudes, are shown in yellow with their area increased to improve visibility. || ",
            "hits": 41
        },
        {
            "id": 11060,
            "url": "https://svs.gsfc.nasa.gov/11060/",
            "result_type": "Produced Video",
            "release_date": "2012-08-30T00:00:00-04:00",
            "title": "Stuck In Neverland",
            "description": "Like the storybook character Peter Pan, Saturn's moon Phoebe may have a serious case of arrested development. One of 62 moons orbiting the ringed planet, Phoebe has some traits of what's called a planetesimal, a planetary building block. A team including NASA scientists took data from the Cassini spacecraft orbiting Saturn and plugged it into a model of Phoebe's chemistry, geology and geophysics to learn more about this intriguing object. They found that the moon most likely evolved actively for a time after it formed. This is unlike most asteroids and comets, which haven't changed much since the solar system's formation about 4.5 billion years ago. Scientists think that if Phoebe was born early enough in the solar system's history, its gravity could have pulled in radioactive material that would have produced enough heat to warm the interior and reshape the moon. Watch the video to learn more about Phoebe's lifetime. || ",
            "hits": 18
        },
        {
            "id": 3822,
            "url": "https://svs.gsfc.nasa.gov/3822/",
            "result_type": "Visualization",
            "release_date": "2011-02-14T00:00:00-05:00",
            "title": "Stereoscopic Magnetic Field Lines",
            "description": "This stereoscopic visualization shows a simple model of the Earth's magnetic field. The magnetic field partially shields the Earth from harmful charged particles emanating from the sun. The field is stretched back away from Sun by solar particle and radiation pressures.The geomagnetic field is generated (and regenerated) as the conducting fluid of the Earth's mantle and core, driven by convection of heat from deeper in the interior, induces an electromotive force (EMF) with the existing magnetic field.  This process is very similar to the way an electric generator generates a voltage.  That voltage then drives an induced current in the conducting fluid, which also produces a magnetic field.  This feedback mechanism helps maintain the field, continuously converting the thermal energy in the Earth into magnetic field energy.The magnetic field line data used in this visualization is from a simplified static model. More complex models deform the magnetic field over time as the Earth rotates and experiences solar pressures. Many of the field lines (particulary near the back, away from the Sun) should eventually connect (north and south poles), but the 3d model used in this visualization does not extend far enough to see this.The day/night terminator is aligned with the Sun and is therefore aligned with the magnetic field too. This visualization is based on a previous monoscopic visualizaton that included magnetic field line data. || ",
            "hits": 265
        },
        {
            "id": 3605,
            "url": "https://svs.gsfc.nasa.gov/3605/",
            "result_type": "Visualization",
            "release_date": "2009-07-06T00:00:00-04:00",
            "title": "Magnetospheric Multiscale Mission (MMS) Dayside Orbit Animation for the Preliminary Design Review (PDR)",
            "description": "This visualization uses simulated ephemerides to show the proposed orbits of the Magnetospheric Multiscale Mission (MMS) during the \"dayside magnetosheath/magnetopause\" orbit phase. The movie initially shows the general orientation of the orbit with respect to the Earth, Moon, and Sun. It then zooms in to \"ride\" along with the spacecraft. We then zoom in even closer to show that there are actually four spacecraft flying in a tetrahedral formation. Finally, we see how the 4 spacecraft skim the magnetosheath such that, occasionally, some of the spacecraft are inside (e.g., MMS #1) and some are outside (e.g., MMS #2, #3, and #4) of the magnetosheath boundary.This visualization was created in support of the MMS Preliminary Design Review (PDR) which was held May 4 - 7, 2009. || ",
            "hits": 35
        },
        {
            "id": 3606,
            "url": "https://svs.gsfc.nasa.gov/3606/",
            "result_type": "Visualization",
            "release_date": "2009-07-06T00:00:00-04:00",
            "title": "Magnetospheric Multiscale Mission (MMS) Nightside Orbit Animation for the Preliminary Design Review (PDR)",
            "description": "This visualization uses simulated ephemerides to show the proposed orbits of the Magnetospheric Multiscale Mission (MMS) during the \"nightside\" orbit phase. The movie initially shows the general orientation of the orbit with respect to the Earth, Moon, and Sun. It then moves in towards the Earth revealing Earth's magnetic field. The camera then moves down towards the dark side of the Earth showing how MMS will fly through the tail of the magnetosphereThis visualization was created in support of the MMS Preliminary Design Review (PDR) which was held May 4th through May 7th of 2009. || ",
            "hits": 30
        },
        {
            "id": 2970,
            "url": "https://svs.gsfc.nasa.gov/2970/",
            "result_type": "Visualization",
            "release_date": "2004-08-05T12:00:00-04:00",
            "title": "Volumetric Visualization of the Convection-generated Stresses in Earth",
            "description": "The fundamental problem of the deformation of the Earth involves stress conditions on the basis of the crust caused by the mantle convection. Based on decades of satellite gravity data, a harmonic analytical model of the convection flow has been developed at GSFC. The magnitudes and directions of the resultant stresses in the crust were obtained at 64,000 grid points for each of 18 layers from 150 km to 600 km under the Earth. In this project, we explored three dimensional volumetric visualization methods for the data. To overcome the typical volumetric visualization obstacles such as enormous amount of data and opacity of objects in the scene, we developed an interactive and transparent isosurface model to render the volumetric data. a) Animated isosurfaces of earth stress below Hawaii. The blue objects indicate the shape of the stress distribution and the yellow objects indicate the high stress areas. b) Interactive global earth stress. To view the model, please use the QuickTime Player (similarly, please select the QuickTime version of the movie). Hold the left button and drag the mouse horizontally to view areas on the earth at the same depth. Hold the left button and drag the mouse vertically to view the different layers of the stress distributions inside the earth, between 150 km to 600 km deep. || ",
            "hits": 30
        },
        {
            "id": 2891,
            "url": "https://svs.gsfc.nasa.gov/2891/",
            "result_type": "Visualization",
            "release_date": "2004-02-10T12:00:00-05:00",
            "title": "Aurora over the North Pole on April 17, 1999 (WMS)",
            "description": "When the charged particles flowing outward from the Sun (the solar wind) hit the Earth's magnetic field, they are channeled down the magnetic field lines to the ionosphere at the North and South Poles.  The impact of these particles on atmospheric molecules causes the molecules to emit light, which forms the visible aurora.  This visualization shows the development of the aurora over the North Pole for about three hours on April 17, 1999, as seen by the ultraviolet VIS Earth Camera on the POLAR spacecraft.  The two main features of these ultraviolet images are the very bright ultraviolet emission from the reflected solar radiation on the dayside of the Earth and the bright ring of the auroral oval circling the North Pole.  The aurora seen in this visualization is the diffuse aurora, a very large bright band that is actually too dim to be seen well from the ground by the human eye.  What we normally think of as the aurora are the even brighter curtains of light within the diffuse auroral caused by very energetic electrons.  These curtains are too small to be seen in this image.  The diffuse aurora appears as a ring around the pole rather than as a bright spot over the entire pole because the solar particles actually spend extended time wandering about within the Earth's magnetic field before traveling down a very select set of magnetic field lines to the Earth.  Near the end of this three hour period, the spacecraft was getting so close to the Earth that the edges of the globe were outside the camera's image, which accounts for the growing circular data gaps over Asia and the Pacific Ocean. || ",
            "hits": 41
        },
        {
            "id": 2675,
            "url": "https://svs.gsfc.nasa.gov/2675/",
            "result_type": "Visualization",
            "release_date": "2003-01-10T16:00:00-05:00",
            "title": "Haze over China",
            "description": "NASA satellite image of eastern Asia shows a dense blanket of polluted air over central eastern China — dense enough that the coastline around Shanghai virtually disappears. The 'Asian Brown Cloud' is a toxic mix of ash, acids and airborne particles from car and factory emissions, as well as from low-tech polluters like wood-burning stoves. || ",
            "hits": 23
        },
        {
            "id": 2699,
            "url": "https://svs.gsfc.nasa.gov/2699/",
            "result_type": "Visualization",
            "release_date": "2003-01-10T16:00:00-05:00",
            "title": "Haze over China, Shenzhen",
            "description": "NASA satellite image of eastern Asia shows a dense blanket of polluted air over central eastern China — dense enough that the coastline around Shanghai virtually disappears. The 'Asian Brown Cloud' is a toxic mix of ash, acids and airborne particles from car and factory emissions, as well as from low-tech polluters like wood-burning stoves. || ",
            "hits": 20
        },
        {
            "id": 2435,
            "url": "https://svs.gsfc.nasa.gov/2435/",
            "result_type": "Visualization",
            "release_date": "2002-05-09T12:00:00-04:00",
            "title": "IMAGE/LENA Observes Oxygen Atoms in the near-Earth Environment",
            "description": "Electrically charged oxygen atoms (green) are ejected into the magnetosphere due to heating in the ionosphere.  The red 'thermometer' displays the intensity of the solar wind (dynamic pressure) measured by the Geotail spacecraft.  The yellow 'thermometer' represents the source intensity or hydrogen counts as measured by IMAGE/LENA. || ",
            "hits": 18
        },
        {
            "id": 2444,
            "url": "https://svs.gsfc.nasa.gov/2444/",
            "result_type": "Visualization",
            "release_date": "2002-05-09T12:00:00-04:00",
            "title": "IMAGE/HENA Views Oxygen in the Magnetosphere (Rainbow Version)",
            "description": "IMAGE/HENA observes the oxygen ions, expelled from the Earth's atmosphere by the solar wind, return to the polar regions via the magnetic field. || Movie of IMAGE-HENA data using a rainbow color table for oxygen intensity. || a002444.00100_print.png (720x480) [373.3 KB] || HENArainbow_pre.jpg (320x288) [13.5 KB] || a002444.webmhd.webm (960x540) [8.1 MB] || a002444.dv (720x480) [112.3 MB] || HENArainbow.mpg (320x288) [942.9 KB] || ",
            "hits": 19
        },
        {
            "id": 2445,
            "url": "https://svs.gsfc.nasa.gov/2445/",
            "result_type": "Visualization",
            "release_date": "2002-05-09T12:00:00-04:00",
            "title": "IMAGE/HENA Views Oxygen in the Magnetosphere (Blue Version)",
            "description": "IMAGE/HENA observes the oxygen ions, expelled from the Earth's atmosphere by the solar wind, return to the polar regions via the magnetic field. || Movie of IMAGE-HENA data using a blue color table for oxygen intensity. || a002445.00010_print.png (720x480) [371.4 KB] || HENAblue_pre.jpg (320x320) [7.9 KB] || a002445.webmhd.webm (960x540) [8.1 MB] || a002445.dv (720x480) [153.6 MB] || HENAblue.mpg (320x320) [1.3 MB] || ",
            "hits": 18
        },
        {
            "id": 2410,
            "url": "https://svs.gsfc.nasa.gov/2410/",
            "result_type": "Visualization",
            "release_date": "2002-03-14T12:00:00-05:00",
            "title": "Farallon Plate Remnants",
            "description": "The Rockies are fifteen hundred kilometers, or one thousand miles, to the east. The cause must be the tectonic plate that built these mountains. Its name is Farallon. Farallon started off normally enough. It plunged beneath the North American Plate at a forty-five degree angle. This process sprouted volcanoes to form the Sierra Nevada in what is now California.  Next, mantle motions pulled North America westward over Farallon, and the plate scraped along the bottom of the continent - for fifteen hundred kilometers.  As North America continued its westward trek, Farallon settled to the bottom of the mantle.The image is output from a model run using the TERRA mantle software. To learn more about Bunge's work, visit his web site at: http://www.geophysik.uni-muenchen.de/Members/bunge. || ",
            "hits": 38
        },
        {
            "id": 2328,
            "url": "https://svs.gsfc.nasa.gov/2328/",
            "result_type": "Visualization",
            "release_date": "2001-12-12T12:00:00-05:00",
            "title": "Terra/CERES View of the Earth",
            "description": "Data sets from the Terra/CERES instrument || Outgoing Longwave Radiation (Average May 11-25, 2000) || ceres_olr_20010511_25_avg.jpg (1800x1098) [414.4 KB] || ceres_olr_20010511_25_avg_web.jpg (320x195) [12.7 KB] || ceres_olr_20010511_25_avg_thm.png (80x40) [5.5 KB] || ceres_olr_20010511_25_avg_web_searchweb.jpg (320x180) [89.5 KB] || ceres_olr_20010511_25_avg.tif (1800x1098) [941.4 KB] || ",
            "hits": 17
        },
        {
            "id": 2156,
            "url": "https://svs.gsfc.nasa.gov/2156/",
            "result_type": "Visualization",
            "release_date": "2001-06-20T12:00:00-04:00",
            "title": "One Year of Terra/CERES Data (Reflected Solar Radiation) Daily Data",
            "description": "This animation displays a little over one year of Terra/CERES data (March 1, 2000 to May 25, 2001) at one day resolution. The data are 2.5 degree resolution. The band is reflected solar radiation (often referred to as 'shortwave' in the literature). Bright areas correspond to cloud tops or snowcover. || ",
            "hits": 10
        },
        {
            "id": 2157,
            "url": "https://svs.gsfc.nasa.gov/2157/",
            "result_type": "Visualization",
            "release_date": "2001-06-20T12:00:00-04:00",
            "title": "One Year of Terra/CERES Data (Outgoing Longwave Radiation) Daily Data",
            "description": "This animation displays one year of Outgoing Longwave Radiation (OLR) Terra/CERES data (March 1, 2000 to May 25, 2001) at one day resolution. The data are 2.5 degree resolution. || Movie at one frame per day of Terra-CERES OLR data. || a002157.00005_print.png (720x480) [513.3 KB] || a002157_pre.jpg (320x242) [10.1 KB] || a002157.webmhd.webm (960x540) [22.4 MB] || a002157.dv (720x480) [432.9 MB] || a002157.mpg (352x240) [16.4 MB] || ",
            "hits": 19
        },
        {
            "id": 2158,
            "url": "https://svs.gsfc.nasa.gov/2158/",
            "result_type": "Visualization",
            "release_date": "2001-06-20T12:00:00-04:00",
            "title": "14-Day Boxcar Averaged Terra/CERES (Reflected Solar Radiation)",
            "description": "This animation displays one year of Reflected Solar Radiation (RSR) Terra/CERES data (March 1, 2000 to May 25, 2001) with a 14-day boxcar average. Endpoints have the average re-weighted for the smaller amount of data. The data are 2.5 degree resolution. || ",
            "hits": 8
        },
        {
            "id": 2159,
            "url": "https://svs.gsfc.nasa.gov/2159/",
            "result_type": "Visualization",
            "release_date": "2001-06-20T12:00:00-04:00",
            "title": "14-Day Boxcar Averaged Terra/CERES Data (Outgoing Longwave Radiation)",
            "description": "This animation displays one year of Outgoing Longwave Radiation (OLR) Terra/CERES data (March 1, 2000 to May 25, 2001) with a 14-day boxcar average. Endpoints have the average re-weighted for the smaller amount of data. The data are 2.5 degree resolution. || ",
            "hits": 7
        },
        {
            "id": 2167,
            "url": "https://svs.gsfc.nasa.gov/2167/",
            "result_type": "Visualization",
            "release_date": "2001-06-20T12:00:00-04:00",
            "title": "Terra/CERES on the American Southwest: May 2001",
            "description": "Terra/CERES views the American southwest during the heatwave of May 2001.  The animation is generated for outgoing longwave radiation (heat). || Movie of the American Southwest during a heatwave.  April-May 2001. || a002167.00005_print.png (720x480) [580.5 KB] || a002167_pre.jpg (320x242) [8.7 KB] || a002167.webmhd.webm (960x540) [1.9 MB] || a002167.dv (720x480) [55.5 MB] || a002167.mpg (352x240) [1.9 MB] || ",
            "hits": 7
        },
        {
            "id": 2168,
            "url": "https://svs.gsfc.nasa.gov/2168/",
            "result_type": "Visualization",
            "release_date": "2001-06-20T12:00:00-04:00",
            "title": "Terra/CERES Views the Americas in Reflected Solar Radiation - Daily Data",
            "description": "Terra/CERES views the Americas in Reflected Solar Radiation (March 1, 2000 to May 25, 2001). These are daily data. || Movie of the Americas in RSR - daily data. || a002168.00005_print.png (720x480) [623.8 KB] || a002168_pre.jpg (320x242) [11.4 KB] || a002168.webmhd.webm (960x540) [31.6 MB] || a002168.dv (720x480) [432.9 MB] || a002168.mpg (352x240) [16.6 MB] || ",
            "hits": 9
        },
        {
            "id": 2169,
            "url": "https://svs.gsfc.nasa.gov/2169/",
            "result_type": "Visualization",
            "release_date": "2001-06-20T12:00:00-04:00",
            "title": "Terra/CERES Views the Americas in Outgoing Longwave Radiation - Daily Data",
            "description": "Terra/CERES views the Americas in Outgoing Longwave Radiation (March 1, 2000 to May 25, 2001). These are daily data. || Movie of the Americas in OLR. || a002169.00005_print.png (720x480) [621.3 KB] || a002169_pre.jpg (320x242) [9.1 KB] || a002169.webmhd.webm (960x540) [22.3 MB] || a002169.dv (720x480) [432.7 MB] || a002169.mpg (352x240) [16.4 MB] || ",
            "hits": 20
        },
        {
            "id": 2170,
            "url": "https://svs.gsfc.nasa.gov/2170/",
            "result_type": "Visualization",
            "release_date": "2001-06-20T12:00:00-04:00",
            "title": "Terra/CERES Outgoing Longwave and Reflected Solar Radiation: Boxcar Averaged",
            "description": "Terra/CERES views the world in outgoing longwave radiation (left) and reflected solar radiation (right). This is a 14-day boxcar averaged datas ets from March 1, 2001 to May 25, 2001. || Side-by-side Earth views of 14-day boxcar averaged OLR & RSR data. || a002170.00005_print.png (720x480) [424.9 KB] || a002170_pre.jpg (320x240) [7.0 KB] || a002170.webmhd.webm (960x540) [2.5 MB] || a002170.dv (720x480) [72.0 MB] || a002170.mpg (320x240) [2.1 MB] || ",
            "hits": 7
        },
        {
            "id": 2171,
            "url": "https://svs.gsfc.nasa.gov/2171/",
            "result_type": "Visualization",
            "release_date": "2001-06-20T12:00:00-04:00",
            "title": "Terra/CERES Outgoing Longwave and Reflected Solar Radiation: Daily Data",
            "description": "Terra/CERES views the world in outgoing longwave radiation (left) and reflected solar radiation (right). This is daily data from March 1, 2000 to May 25, 2001. || Synchronized, side-by-side views of the Earth in RSR & OLR. || a002171.00005_print.png (720x480) [451.5 KB] || a002171_pre.jpg (320x238) [7.8 KB] || a002171.webmhd.webm (960x540) [24.2 MB] || a002171.dv (720x480) [432.9 MB] || a002171.mpg (352x240) [16.4 MB] || ",
            "hits": 62
        },
        {
            "id": 2172,
            "url": "https://svs.gsfc.nasa.gov/2172/",
            "result_type": "Visualization",
            "release_date": "2001-06-20T12:00:00-04:00",
            "title": "Terra/CERES Views the World in Reflected Solar Radiation - Daily Data",
            "description": "Terra/CERES views the world in Reflected Solar Radiation. These are daily data from March 1, 2000 to May 25, 2001. || Movie of the Earth in RSR. || a002172.00005_print.png (720x480) [390.8 KB] || a002172_pre.jpg (320x242) [6.8 KB] || a002172.webmhd.webm (960x540) [23.9 MB] || a002172.dv (720x480) [433.0 MB] || a002172.mpg (352x240) [16.5 MB] || ",
            "hits": 146
        },
        {
            "id": 2173,
            "url": "https://svs.gsfc.nasa.gov/2173/",
            "result_type": "Visualization",
            "release_date": "2001-06-20T12:00:00-04:00",
            "title": "Terra/CERES Views the World in Outgoing Longwave Radiation - Daily data",
            "description": "Terra/CERES views the world in outgoing longwave radiation. These are daily data from March 1, 2000 to May 25, 2001. || Movie of daily OLR data on a spinning Earth. || a002173.00005_print.png (720x480) [430.1 KB] || a002173_pre.jpg (320x242) [6.6 KB] || a002173.webmhd.webm (960x540) [19.8 MB] || a002173.dv (720x480) [433.0 MB] || a002173.mpg (352x240) [16.5 MB] || ",
            "hits": 122
        },
        {
            "id": 2174,
            "url": "https://svs.gsfc.nasa.gov/2174/",
            "result_type": "Visualization",
            "release_date": "2001-06-20T12:00:00-04:00",
            "title": "Terra/CERES Views the Pakistan Heat Wave: May 2001",
            "description": "Terra/CERES views the Pakistan heat wave. || Movie of OLR changes in May 2001 near Pakistan. || a002174.00005_print.png (720x480) [630.4 KB] || a002174_pre.jpg (320x242) [9.8 KB] || a002174.webmhd.webm (960x540) [2.4 MB] || a002174.dv (720x480) [55.5 MB] || a002174.mpg (352x240) [1.5 MB] || May 5, 2001 || PakistanOLR3445.jpg (2560x1920) [420.0 KB] || PakistanOLR3445_web.jpg (320x240) [14.8 KB] || PakistanOLR3445.tif (2560x1920) [2.9 MB] || ",
            "hits": 25
        },
        {
            "id": 2037,
            "url": "https://svs.gsfc.nasa.gov/2037/",
            "result_type": "Visualization",
            "release_date": "2000-11-15T12:00:00-05:00",
            "title": "Polar Visible Aurora Animation: July 16, 2000",
            "description": "An animation of the visible aurora in the northern hemisphere on July 16, 2000 as measured by Polar.  Text on preview image reads, \"Polar Visible Aurora July 16, 2000\". || a002037.00290_print.png (720x480) [499.6 KB] || a001326_pre.jpg (320x242) [8.3 KB] || a001326_thm.png (80x40) [5.0 KB] || a001326_pre_searchweb.jpg (320x180) [55.4 KB] || a002037.webmhd.webm (960x540) [3.3 MB] || a002037.dv (720x480) [50.9 MB] || a002037.mp4 (640x480) [2.7 MB] || a001326.mpg (352x240) [2.0 MB] || ",
            "hits": 13
        },
        {
            "id": 2038,
            "url": "https://svs.gsfc.nasa.gov/2038/",
            "result_type": "Visualization",
            "release_date": "2000-11-15T12:00:00-05:00",
            "title": "Stills of the Polar Visible Aurora from January 10, 1997",
            "description": "Polar Visible Aurora from January 10, 1997 || still_polar_hires.1997.Jan.10_1.jpg (2560x1920) [415.9 KB] || still_polar_hires.1997.Jan.10_1_web.jpg (320x240) [8.3 KB] || still_polar_hires.1997.Jan.10_1_thm.png (80x40) [6.5 KB] || still_polar_hires.1997.Jan.10_1_web_searchweb.jpg (320x180) [56.5 KB] || still_polar_hires.1997.Jan.10_1.tif (2560x1920) [2.6 MB] || ",
            "hits": 15
        },
        {
            "id": 2040,
            "url": "https://svs.gsfc.nasa.gov/2040/",
            "result_type": "Visualization",
            "release_date": "2000-11-15T12:00:00-05:00",
            "title": "Stills of the Polar Visible Aurora from October 22, 1999",
            "description": "Polar Visible Aurora from October 22, 1999 || still_polar_hires.1999.Oct.22_1_med.jpg (1536x1152) [115.1 KB] || still_polar_hires.1999.Oct.22_1_sm.jpg (512x384) [19.7 KB] || still_polar_hires.1999.Oct.22_1_thm.png (80x40) [3.4 KB] || still_polar_hires.1999.Oct.22_1_sm_searchweb.jpg (320x180) [61.1 KB] || still_polar_hires.1999.Oct.22_1.tif (2560x1920) [2.7 MB] || ",
            "hits": 16
        },
        {
            "id": 2043,
            "url": "https://svs.gsfc.nasa.gov/2043/",
            "result_type": "Visualization",
            "release_date": "2000-11-15T12:00:00-05:00",
            "title": "Stills of the Polar Visible Aurora from July 16, 2000",
            "description": "Polar Visible Aurora from July 16, 2000 || still_polar_hires2000.July.16_2.jpg (2560x1920) [477.8 KB] || still_polar_hires2000.July.16_2_web.jpg (320x240) [10.5 KB] || still_polar_hires2000.July.16_2_thm.png (80x40) [3.5 KB] || still_polar_hires2000.July.16_2_web_searchweb.jpg (180x320) [65.2 KB] || still_polar_hires2000.July.16_2.tif (2560x1920) [3.0 MB] || ",
            "hits": 8
        },
        {
            "id": 1210,
            "url": "https://svs.gsfc.nasa.gov/1210/",
            "result_type": "Visualization",
            "release_date": "2000-10-11T12:00:00-04:00",
            "title": "Polar Visible Aurora Animation: July 15, 2000",
            "description": "An animation of the visible aurora in the northern hemisphere on July 15, 2000 as measured by Polar || a001210.00010_print.png (720x480) [366.2 KB] || a001210_thm.png (80x40) [3.8 KB] || a001210_pre.jpg (320x242) [5.5 KB] || a001210_pre_searchweb.jpg (320x180) [34.4 KB] || a001210.webmhd.webm (960x540) [6.2 MB] || a001210.dv (720x480) [95.2 MB] || a001210.mp4 (640x480) [5.0 MB] || a001210.mpg (352x240) [3.8 MB] || ",
            "hits": 15
        },
        {
            "id": 1211,
            "url": "https://svs.gsfc.nasa.gov/1211/",
            "result_type": "Visualization",
            "release_date": "2000-10-11T12:00:00-04:00",
            "title": "Polar Visible Aurora Animation: July 13, 2000",
            "description": "An animation of the visible aurora in the northern hemisphere on July 13, 2000 as measured by Polar || a001211.00010_print.png (720x480) [376.4 KB] || a001211_thm.png (80x40) [3.8 KB] || a001211_pre.jpg (320x242) [5.5 KB] || a001211_pre_searchweb.jpg (320x180) [34.4 KB] || a001211.webmhd.webm (960x540) [4.9 MB] || a001211.dv (720x480) [92.5 MB] || a001211.mp4 (640x480) [4.8 MB] || a001211.mpg (352x240) [4.4 MB] || ",
            "hits": 13
        },
        {
            "id": 1206,
            "url": "https://svs.gsfc.nasa.gov/1206/",
            "result_type": "Visualization",
            "release_date": "2000-10-03T12:00:00-04:00",
            "title": "Polar Visible Aurora Animation: July 15, 2000 to July 16, 2000",
            "description": "An animation of the visible aurora in the northern hemisphere from July 15, 2000 to July 16, 2000 as measured by Polar || a001206.00005_print.png (720x480) [336.4 KB] || a001206_thm.png (80x40) [3.8 KB] || a001206_pre.jpg (320x242) [5.3 KB] || a001206_pre_searchweb.jpg (320x180) [33.8 KB] || a001206.webmhd.webm (960x540) [5.1 MB] || a001206.dv (720x480) [95.2 MB] || a001206.mp4 (640x480) [5.0 MB] || a001206.mpg (352x240) [3.8 MB] || ",
            "hits": 15
        },
        {
            "id": 1170,
            "url": "https://svs.gsfc.nasa.gov/1170/",
            "result_type": "Visualization",
            "release_date": "2000-05-24T12:00:00-04:00",
            "title": "Plasmasphere With Earth Inset in EUV",
            "description": "This version of IMAGE observing the Earth's plasmasphere includes an inset showing the size of the Earth. || The Earths plasmasphere, as seen by IMAGE-EUV. || a001170.00095_print.png (720x480) [418.1 KB] || a001170_thm.png (80x40) [4.9 KB] || a001170_pre.jpg (320x242) [6.1 KB] || a001170_pre_searchweb.jpg (320x180) [52.2 KB] || a001170.webmhd.webm (960x540) [694.1 KB] || a001170.dv (720x480) [54.7 MB] || a001170.mp4 (640x480) [2.9 MB] || a001170.mpg (352x240) [2.1 MB] || ",
            "hits": 17
        },
        {
            "id": 1171,
            "url": "https://svs.gsfc.nasa.gov/1171/",
            "result_type": "Visualization",
            "release_date": "2000-05-24T12:00:00-04:00",
            "title": "Aurora With Earth Inset",
            "description": "Earths aurora, as seen by IMAGE. || a001171.00005_print.png (720x480) [439.3 KB] || a001171_pre.jpg (320x242) [6.8 KB] || a001171_thm.png (80x40) [4.7 KB] || a001171_pre_searchweb.jpg (320x180) [54.4 KB] || a001171.webmhd.webm (960x540) [797.7 KB] || a001171.dv (720x480) [61.6 MB] || a001171.mp4 (640x480) [3.3 MB] || a001171.mpg (352x240) [2.3 MB] || ",
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            "id": 1172,
            "url": "https://svs.gsfc.nasa.gov/1172/",
            "result_type": "Visualization",
            "release_date": "2000-05-24T12:00:00-04:00",
            "title": "Plasmasphere Close-up With Earth Inset",
            "description": "The Earths plasmasphere, as seen by IMAGE-EUV. || a001172.00005_print.png (720x480) [549.0 KB] || a001172_thm.png (80x40) [5.8 KB] || a001172_pre.jpg (320x242) [8.9 KB] || a001172_pre_searchweb.jpg (320x180) [68.3 KB] || a001172.webmhd.webm (960x540) [944.5 KB] || a001172.dv (720x480) [54.7 MB] || a001172.mp4 (640x480) [2.9 MB] || a001172.mpg (352x240) [1.8 MB] || ",
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            "id": 1173,
            "url": "https://svs.gsfc.nasa.gov/1173/",
            "result_type": "Visualization",
            "release_date": "2000-05-24T12:00:00-04:00",
            "title": "Aurora Close-up With Earth Inset",
            "description": "Earths aurora, as seen by IMAGE. || a001173.00005_print.png (720x480) [480.6 KB] || a001173_thm.png (80x40) [5.0 KB] || a001173_pre.jpg (320x242) [7.7 KB] || a001173_pre_searchweb.jpg (320x180) [58.5 KB] || a001173.webmhd.webm (960x540) [908.0 KB] || a001173.dv (720x480) [61.6 MB] || a001173.mp4 (640x480) [3.3 MB] || a001173.mpg (352x240) [2.2 MB] || ",
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        {
            "id": 1174,
            "url": "https://svs.gsfc.nasa.gov/1174/",
            "result_type": "Visualization",
            "release_date": "2000-05-24T12:00:00-04:00",
            "title": "IMAGE Views the Plasmasphere in EUV",
            "description": "The IMAGE spacecraft views the Earth's plasmasphere. This animation has no earth inset || The Earths plasmasphere, as seen by IMAGE-EUV. || a001174.00005_print.png (720x480) [439.4 KB] || a001174_thm.png (80x40) [4.7 KB] || a001174_pre.jpg (320x242) [5.9 KB] || a001174_pre_searchweb.jpg (320x180) [51.3 KB] || a001174.webmhd.webm (960x540) [723.1 KB] || a001174.dv (720x480) [54.7 MB] || a001174.mp4 (640x480) [2.9 MB] || a001174.mpg (352x240) [2.1 MB] || ",
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            "id": 1175,
            "url": "https://svs.gsfc.nasa.gov/1175/",
            "result_type": "Visualization",
            "release_date": "2000-05-24T12:00:00-04:00",
            "title": "Aurora Without Earth Inset",
            "description": "A view of aurora from the IMAGE satellite without an earth inset || A movie of the Earths aurora, as seen by IMAGE. || a001175.00005_print.png (720x480) [422.7 KB] || a001175_thm.png (80x40) [4.5 KB] || a001175_pre.jpg (320x242) [6.4 KB] || a001175_pre_searchweb.jpg (320x180) [50.2 KB] || a001175.webmhd.webm (960x540) [725.0 KB] || a001175.dv (720x480) [61.6 MB] || a001175.mp4 (640x480) [3.3 MB] || a001175.mpg (352x240) [2.2 MB] || ",
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            "url": "https://svs.gsfc.nasa.gov/1176/",
            "result_type": "Visualization",
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            "title": "Plasmasphere with Earth Inset",
            "description": "May 16, 2000 || Plasmasphere movie, as seen by IMAGE-EUV || a001176.00005_print.png (720x480) [416.6 KB] || a001176_thm.png (80x40) [4.8 KB] || a001176_pre.jpg (320x242) [5.9 KB] || a001176_pre_searchweb.jpg (320x180) [52.2 KB] || a001176.webmhd.webm (960x540) [647.0 KB] || a001176.dv (720x480) [51.3 MB] || a001176.mp4 (640x480) [2.7 MB] || a001176.mpg (352x240) [2.1 MB] || ",
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            "id": 1177,
            "url": "https://svs.gsfc.nasa.gov/1177/",
            "result_type": "Visualization",
            "release_date": "2000-05-24T12:00:00-04:00",
            "title": "Plasmasphere Without Earth Inset",
            "description": "May 16, 2000 || Plasmasphere movie, as seen by IMAGE-EUV || a001177.00005_print.png (720x480) [404.8 KB] || a001177_thm.png (80x40) [4.7 KB] || a001177_pre.jpg (320x242) [5.7 KB] || a001177_pre_searchweb.jpg (320x180) [50.6 KB] || a001177.webmhd.webm (960x540) [606.7 KB] || a001177.dv (720x480) [51.3 MB] || a001177.mp4 (640x480) [2.8 MB] || a001177.mpg (352x240) [1.9 MB] || ",
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            "url": "https://svs.gsfc.nasa.gov/1136/",
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            "title": "CERES Globe",
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            "url": "https://svs.gsfc.nasa.gov/1137/",
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            "url": "https://svs.gsfc.nasa.gov/1139/",
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            "title": "Global Longwave from CERES",
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            "title": "Longwave Radiation from CERES Unwrapped",
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            "result_type": "Visualization",
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            "title": "Global Shortwave from CERES",
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            "title": "Shortwave from CERES Unwrapped",
            "description": "CERES stands for Clouds and the Earth's Radiant Energy System. More information about CERES can be found at (http://terra.nasa.gov/Brochure/Sect_4-3.html) and (http://ceres.larc.nasa.gov/ceres_brochure.php). || ",
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            "url": "https://svs.gsfc.nasa.gov/1143/",
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            "title": "Spinning Global Longwave from CERES",
            "description": "CERES stands for Clouds and the Earth's Radiant Energy System. More information about CERES can be found at (http://terra.nasa.gov/Brochure/Sect_4-3.html) and (http://ceres.larc.nasa.gov/ceres_brochure.php). || ",
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            "id": 1144,
            "url": "https://svs.gsfc.nasa.gov/1144/",
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            "title": "Spinning Global Shortwave from CERES",
            "description": "CERES stands for Clouds and the Earth's Radiant Energy System.  More information about CERES can be found at (http://terra.nasa.gov/Brochure/Sect_4-3.html) and (http://ceres.larc.nasa.gov/ceres_brochure.php). || ",
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            "id": 777,
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            "result_type": "Visualization",
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            "title": "Polar: PIXIE at Perigee on May 11, 1999 (North)",
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            "url": "https://svs.gsfc.nasa.gov/779/",
            "result_type": "Visualization",
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            "title": "Polar: PIXIE at Perigee 1 on May 11, 1999 (South)",
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            "url": "https://svs.gsfc.nasa.gov/780/",
            "result_type": "Visualization",
            "release_date": "1999-12-08T12:00:00-05:00",
            "title": "Polar: PIXIE at Perigee 2 on May 11, 1999 (South)",
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            "result_type": "Visualization",
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            "result_type": "Visualization",
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            "title": "Polar: PIXIE at T055798 on May 11, 1999 at 22:55",
            "description": "On May 11, 1999, the solar wind that blows constantly from the Sun virtually disappeared. Dropping to a small fraction of its normal density and to half its normal speed, the solar wind died down enough to allow physicists to observe particles flowing directly from the Sun's corona to Earth. This severe change in the solar wind also drastically changed the shape of Earth's magnetic field and produced a rare auroral display at Earth's North Pole. || ",
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            "result_type": "Visualization",
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            "result_type": "Visualization",
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            "url": "https://svs.gsfc.nasa.gov/788/",
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            "title": "Polar Visible Aurora: Normal Solar Wind Conditions on November 13, 1999 over the North Pole",
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            "result_type": "Visualization",
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            "id": 1338,
            "url": "https://svs.gsfc.nasa.gov/1338/",
            "result_type": "Visualization",
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            "title": "Iturralde Structure",
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        {
            "id": 1339,
            "url": "https://svs.gsfc.nasa.gov/1339/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Iturralde Structure Without Labels",
            "description": "Zooming in to the Iturralde structure, a suspected impact crater in northern Bolivia, from Landsat imagery taken in 1988. || a001339.00005_print.png (720x480) [431.4 KB] || a001339_thm.png (80x40) [4.8 KB] || a001339_pre.jpg (320x238) [7.6 KB] || a001339_pre_searchweb.jpg (320x180) [49.2 KB] || a001339.webmhd.webm (960x540) [2.5 MB] || a001339.dv (720x480) [53.3 MB] || a001339.mp4 (640x480) [2.8 MB] || a001339.mpg (352x240) [2.2 MB] || ",
            "hits": 15
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        {
            "id": 1340,
            "url": "https://svs.gsfc.nasa.gov/1340/",
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            "url": "https://svs.gsfc.nasa.gov/1341/",
            "result_type": "Visualization",
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            "id": 251,
            "url": "https://svs.gsfc.nasa.gov/251/",
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            "release_date": "1997-11-01T12:00:00-05:00",
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            "result_type": "Visualization",
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