{
    "count": 36,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 30706,
            "url": "https://svs.gsfc.nasa.gov/30706/",
            "result_type": "Hyperwall Visual",
            "release_date": "2015-10-28T12:00:00-04:00",
            "title": "Io in Motion",
            "description": "Io a moon of Jupiter in motion || io_in_motion_grid_1280x720_print.jpg (1024x576) [42.0 KB] || io_in_motion_grid_1280x720_searchweb.png (180x320) [31.9 KB] || io_in_motion_grid_1280x720_web.png (320x180) [31.9 KB] || io_in_motion_grid_1280x720_thm.png (80x40) [3.0 KB] || io_in_motion_grid_1280x720.mp4 (1280x720) [2.2 MB] || io_in_motion_grid_1280x720.webm (1280x720) [1.7 MB] || io_in_motion_grid_4096x2304.mp4 (4104x2304) [15.3 MB] || 4104x2304_16x9_30p (4104x2304) [0 Item(s)] || io_in_motion_grid.key [4.3 MB] || io_in_motion_grid.pptx [2.8 MB] || ",
            "hits": 86
        },
        {
            "id": 4306,
            "url": "https://svs.gsfc.nasa.gov/4306/",
            "result_type": "Visualization",
            "release_date": "2015-06-25T00:00:00-04:00",
            "title": "FROZEN: The Full Story",
            "description": "On March 27, 2009, NASA released FROZEN, a twelve-minute show about the Earth's frozen regions designed for Science On a Sphere.  Science On a Sphere was created by NOAA and displays movies on a spherical screen, which is ideal for a show about the Earth or the planets.  The audience can view the show from any side of the sphere and can see any part of the Earth.  Making a movie for this system is challenging, and FROZEN was an exciting project to create.  Until now, only the \"trailer\" for FROZEN has been available for viewing from our site.  Here, for the first time, is an on-line version of the complete show, presented in several different formats that show different aspects of the movie. || ",
            "hits": 49
        },
        {
            "id": 11204,
            "url": "https://svs.gsfc.nasa.gov/11204/",
            "result_type": "Produced Video",
            "release_date": "2013-03-14T14:30:00-04:00",
            "title": "Jupiter's Hot Spots",
            "description": "Jupiter's bright Equatorial Zone swirls with dark patches, dubbed \"hot spots\" for their infrared glow. These holes in the ammonia clouds at the top of the atmosphere allow a glimpse into Jupiter's darker, hotter layers below. In 1995 NASA's Galileo spacecraft dropped a probe directly into a hot spot, taking the first and only in situ measurements of Jupiter's atmosphere. Now, movies recorded by NASA's Cassini spacecraft reveal that hot spots are not just local weather phenomena, but are in fact linked to much larger-scale atmospheric structures called Rossby waves. || ",
            "hits": 53
        },
        {
            "id": 3619,
            "url": "https://svs.gsfc.nasa.gov/3619/",
            "result_type": "Visualization",
            "release_date": "2009-09-01T18:00:00-04:00",
            "title": "A Tour of the Cryosphere 2009",
            "description": "The cryosphere consists of those parts of the Earth's surface where water is found in solid form, including areas of snow, sea ice, glaciers, permafrost, ice sheets, and icebergs. In these regions, surface temperatures remain below freezing for a portion of each year. Since ice and snow exist relatively close to their melting point, they frequently change from solid to liquid and back again due to fluctuations in surface temperature. Although direct measurements of the cryosphere can be difficult to obtain due to the remote locations of many of these areas, using satellite observations scientists monitor changes in the global and regional climate by observing how regions of the Earth's cryosphere shrink and expand.This animation portrays fluctuations in the cryosphere through observations collected from a variety of satellite-based sensors. The animation begins in Antarctica, showing some unique features of the Antarctic landscape found nowhere else on earth. Ice shelves, ice streams, glaciers, and the formation of massive icebergs can be seen clearly in the flyover of the Landsat Image Mosaic of Antarctica. A time series shows the movement of iceberg B15A, an iceberg 295 kilometers in length which broke off of the Ross Ice Shelf in 2000. Moving farther along the coastline, a time series of the Larsen ice shelf shows the collapse of over 3,200 square kilometers ice since January 2002. As we depart from the Antarctic, we see the seasonal change of sea ice and how it nearly doubles the apparent area of the continent during the winter.From Antarctica, the animation travels over South America showing glacier locations on this mostly tropical continent. We then move further north to observe daily changes in snow cover over the North American continent. The clouds show winter storms moving across the United States and Canada, leaving trails of snow cover behind. In a close-up view of the western US, we compare the difference in land cover between two years: 2003 when the region received a normal amount of snow and 2002 when little snow was accumulated. The difference in the surrounding vegetation due to the lack of spring melt water from the mountain snow pack is evident.As the animation moves from the western US to the Arctic region, the areas affected by permafrost are visible. As time marches forward from March to September, the daily snow and sea ice recede and reveal the vast areas of permafrost surrounding the Arctic Ocean.The animation shows a one-year cycle of Arctic sea ice followed by the mean September minimum sea ice for each year from 1979 through 2008. The superimposed graph of the area of Arctic sea ice at this minimum clearly shows the dramatic decrease in Artic sea ice over the last few years.While moving from the Arctic to Greenland, the animation shows the constant motion of the Arctic polar ice using daily measures of sea ice activity. Sea ice flows from the Arctic into Baffin Bay as the seasonal ice expands southward. As we draw close to the Greenland coast, the animation shows the recent changes in the Jakobshavn glacier. Although Jakobshavn receded only slightly from 1964 to 2001, the animation shows significant recession from 2001 through 2009. As the animation pulls out from Jakobshavn, the effect of the increased flow rate of Greenland costal glaciers is shown by the thinning ice shelf regions near the Greenland coast.This animation shows a wealth of data collected from satellite observations of the cryosphere and the impact that recent cryospheric changes are making on our planet.For more information on the data sets used in this visualization, visit NASA's EOS DAAC website.Note: This animation is an update of the animation 'A Short Tour of the Cryosphere', which is itself an abridged version of the animation 'A Tour of the Cryosphere'. The popularity of the earlier animations and their continuing relevance prompted us to update the datasets in parts of the animation and to remake it in high definition. In certain cases, our experiences in using the earlier work have led us to tweak the presentation of some of the material to make it clearer. Our thanks to Dr. Robert Bindschadler for suggesting and supporting this remake. || ",
            "hits": 50
        },
        {
            "id": 10403,
            "url": "https://svs.gsfc.nasa.gov/10403/",
            "result_type": "Produced Video",
            "release_date": "2009-03-12T12:00:00-04:00",
            "title": "FROZEN: A Spherical Movie About the Cryosphere",
            "description": "NASA's home for spherical films on Magic Planet.  Download the Magic Planet-ready movie file here.Released on March 27, 2009, FROZEN is NASA's second major production for the Science On a Sphere platform, a novel cinema-in-the-round technology developed by the Space Agency's sibling NOAA. Viewers see the Earth suspended in darkness as if it were floating in space. Moving across the planet's face, viewers see the undulating wisps of clouds, the ephemeral sweep of fallen snow, the churning crash of shifting ice, and more.FROZEN brings the Earth alive. Turning in space, the sphere becomes a portal onto a virtual planet, complete with churning, swirling depictions of huge natural forces moving below. FROZEN features the global cryosphere, those places on Earth where the temperature doesn't generally rise above water's freezing point. As one of the most directly observable climate gauges, the changing cryosphere serves as a proxy for larger themes.But just as thrilling as this unusual—and unusually realistic—look at the planet's structure and behavior is the sheer fun and fascination of looking at a spherically shaped movie. FROZEN bends the rules of cinema, revealing new ways to tell exciting, valuable stories of all kinds. The movie may be FROZEN, but the experience itself rockets along. || ",
            "hits": 43
        },
        {
            "id": 3355,
            "url": "https://svs.gsfc.nasa.gov/3355/",
            "result_type": "Visualization",
            "release_date": "2006-05-20T23:55:00-04:00",
            "title": "A Short Tour of the Cryosphere",
            "description": "A newer version of this animation is available here.This narrated, 5-minute animation shows a wealth of data collected from satellite observations of the cryosphere and the impact that recent cryospheric changes are making on our planet. This is a shorter version of a narrated, 7 1/2 minute animation entitled  'A Tour of the Cryosphere'.See the above link for a detailed description of the full animation.Two sections have been removed from the original animation: one showing a flyby of the South Pole station and glaciers feeding the Ross Ice Shelf and one showing solar data related to the Earth's energy balance.For more information on the data sets used in this visualization, visit NASA's EOS DAAC website. || ",
            "hits": 34
        },
        {
            "id": 2946,
            "url": "https://svs.gsfc.nasa.gov/2946/",
            "result_type": "Visualization",
            "release_date": "2006-05-15T12:00:00-04:00",
            "title": "Europa's Synthetic Subsurface Heat Transport (Version 2)",
            "description": "Encounters with Jupiter's moon Europa by the Voyager and Galileo spacecraft indicated that a liquid salty ocean might exist below a layer of surface ice that is up to 10 kilometers thick. An ocean general circulation model developed to study the earth's oceans was used to investigate the tidally-forced ocean circulations on Europa. The orbit of Europa is 'gravity locked' so that the same side of Europa always faces Jupiter as is the case with the earth's moon. The icy surface of Europa heaves up and down 50 meters due to the strong tidal forces. This visualization shows the temperature changes induced from the flow fields calculated for a European ocean 50 kilometers deep. The warmest temperatures tend to be near the equator, not because of heating by the sun, but because the currents in the European ocean move the warmest waters to that location. Understanding the thermal and flow fields from these model runs will help to interpret observations from future missions to Europa such as the Jupiter's Icy Moons Orbiter mission proposed for launch in 2012. || ",
            "hits": 61
        },
        {
            "id": 2947,
            "url": "https://svs.gsfc.nasa.gov/2947/",
            "result_type": "Visualization",
            "release_date": "2006-05-15T12:00:00-04:00",
            "title": "Europa's Synthetic Subsurface Heat Transport (Version 1)",
            "description": "Under Europa's icy surface are vast extraterrestrial oceans.  This conceptual animation depicts simulated heat transport of these subsurface oceans.  Please note that the simulated heat transport in this animation is only conceptual and a more accurate representation can be found at animation #2946. || ",
            "hits": 24
        },
        {
            "id": 3181,
            "url": "https://svs.gsfc.nasa.gov/3181/",
            "result_type": "Visualization",
            "release_date": "2005-12-04T23:55:00-05:00",
            "title": "A Tour of the Cryosphere",
            "description": "A new HD version of this animation is available here.Click here to go to the media download section.The cryosphere consists of those parts of the Earth's surface where water is found in solid form, including areas of snow, sea ice, glaciers, permafrost, ice sheets, and icebergs. In these regions, surface temperatures remain below freezing for a portion of each year. Since ice and snow exist relatively close to their melting point, they frequently change from solid to liquid and back again due to fluctuations in surface temperature. Although direct measurements of the cryosphere can be difficult to obtain due to the remote locations of many of these areas, using satellite observations scientists monitor changes in the global and regional climate by observing how regions of the Earth's cryosphere shrink and expand.This animation portrays fluctuations in the cryosphere through observations collected from a variety of satellite-based sensors. The animation begins in Antarctica, showing ice thickness ranging from 2.7 to 4.8 kilometers thick along with swaths of polar stratospheric clouds. In a tour of this frozen continent, the animation shows some unique features of the Antarctic landscape found nowhere else on earth. Ice shelves, ice streams, glaciers, and the formation of massive icebergs can be seen. A time series shows the movement of iceberg B15A, an iceberg 295 kilometers in length which broke off of the Ross Ice Shelf in 2000. Moving farther along the coastline, a time series of the Larsen ice shelf shows the collapse of over 3,200 square kilometers ice since January 2002. As we depart from the Antarctic, we see the seasonal change of sea ice and how it nearly doubles the size of the continent during the winter.From Antarctica, the animation travels over South America showing areas of permafrost over this mostly tropical continent. We then move further north to observe daily changes in snow cover over the North American continent. The clouds show winter storms moving across the United States and Canada, leaving trails of snow cover behind. In a close-up view of the western US, we compare the difference in land cover between two years: 2003 when the region received a normal amount of snow and 2002 when little snow was accumulated. The difference in the surrounding vegetation due to the lack of spring melt water from the mountain snow pack is evident.As the animation moves from the western US to the Arctic region, the areas effected by permafrost are visible. In December, we see how the incoming solar radiation primarily heats the Southern Hemisphere. As time marches forward from December to June, the daily snow and sea ice recede as the incoming solar radiation moves northward to warm the Northern Hemisphere.Using satellite swaths that wrap the globe, the animation shows three types of instantaneous measurements of solar radiation observed on June 20, 2003: shortwave (reflected) radiation, longwave (thermal) radiation and net flux (showing areas of heating and cooling). Correlation between reflected radiation and clouds are evident. When the animation fades to show the monthly global average net flux, we see that the polar regions serve to cool the global climate by radiating solar energy back into space throughout the year.The animation shows a one-year cycle of the monthly average Arctic sea ice concentration followed by the mean September minimum sea ice for each year from 1979 through 2004. A red outline indicates the mean sea ice extent for September over 22 years, from 1979 to 2002. The minimum Arctic sea ice animation clearly shows how over the last 5 years the quantity of polar ice has decreased by 10 - 14% from the 22 year average.While moving from the Arctic to Greenland, the animation shows the constant motion of the Arctic polar ice using daily measures of sea ice activity. Sea ice flows from the Arctic into Baffin Bay as the seasonal ice expands southward. As we draw close to the Greenland coast, the animation shows the recent changes in the Jakobshavn glacier. Although Jakobshavn receded only slightly from 1042 to 2001, the animation shows significant recession over the past three years, from 2002 through 2004.This animation shows a wealth of data collected from satellite observations of the cryosphere and the impact that recent cryospheric changes are making on our planet.For more information on the data sets used in this visualization, visit NASA's EOS DAAC website. || ",
            "hits": 123
        },
        {
            "id": 3041,
            "url": "https://svs.gsfc.nasa.gov/3041/",
            "result_type": "Visualization",
            "release_date": "2004-11-01T12:00:00-05:00",
            "title": "Lunar Fly By and Earth Approach",
            "description": "This is an animation flying over the surface of the moon then approaching the earth. It was created in support of a presentation at the National Air and Space Museum (NASM) in October 2004. Scales are not accurate in this visualization. The Earth is about 3 times larger than it would actually appear. The source of the moon texture is unknown; it is thought to be a composite from several missions. The Earth texture was captured as the Galileo spacecraft swung by the Earth in 1990 for a gravity assist on its way to Jupiter. || ",
            "hits": 22
        },
        {
            "id": 3042,
            "url": "https://svs.gsfc.nasa.gov/3042/",
            "result_type": "Visualization",
            "release_date": "2004-11-01T12:00:00-05:00",
            "title": "Lunar Beauty Shot",
            "description": "This is a beauty shot animation flying over the surface of the moon created in support of a series of live interviews about the 2004 lunar eclipse.Scales are not accurate in this visualization.  The Earth is about 3 times larger than it would actually appear.  The source of the moon texture is unknown; it is thought to be a composite from several missions.  The Earth texture was captured as the Galileo spacecraft swung by the Earth in 1990 for a gravity assist on its way to Jupiter. || ",
            "hits": 18
        },
        {
            "id": 3044,
            "url": "https://svs.gsfc.nasa.gov/3044/",
            "result_type": "Visualization",
            "release_date": "2004-11-01T12:00:00-05:00",
            "title": "Apollo Lunar Landing Sites",
            "description": "This visualization shows a fly by of the lunar surface highlighting each Apollo lunar landing site. || ",
            "hits": 209
        },
        {
            "id": 2933,
            "url": "https://svs.gsfc.nasa.gov/2933/",
            "result_type": "Visualization",
            "release_date": "2004-10-01T12:00:00-04:00",
            "title": "Mission Proposal: Polar GOES-like spacecraft (beauty shot)",
            "description": "This visualization was created to support a mission proposal led by Lars Peter Riishojgaard. This mission would fly a GOES-like spacecraft in a polar elliptical orbit around the Earth providing a large percentage of observing time for northern polar regions. This version of the visualization is a beauty shot first showing the orbit from afar, then moving into the orbital plane and riding the orbit as the spacecraft would. || ",
            "hits": 19
        },
        {
            "id": 2934,
            "url": "https://svs.gsfc.nasa.gov/2934/",
            "result_type": "Visualization",
            "release_date": "2004-10-01T12:00:00-04:00",
            "title": "Mission Proposal: Polar GOES-like Spacecraft (Riding the Spacecraft - Animated Clouds)",
            "description": "This visualization was created to support a mission proposal led by Lars Peter Riishojgaard. This mission would fly a GOES-like spacecraft in a polar elliptical orbit around the Earth providing a large percentage of observing time for northern polar regions. This version of the visualization has the camera riding the orbit as the spacecraft would with GOES clouds animating on the Earth. The clouds are constantly lit so as to provide an infra-red (IR) type of view. || ",
            "hits": 22
        },
        {
            "id": 2935,
            "url": "https://svs.gsfc.nasa.gov/2935/",
            "result_type": "Visualization",
            "release_date": "2004-10-01T12:00:00-04:00",
            "title": "Mission Proposal: Polar GOES-like Spacecraft (Riding the Spacecraft - Animated Swaths)",
            "description": "This visualization was created to support a mission proposal led by Lars Peter Riishojgaard. This mission would fly a GOES-like spacecraft in a polar elliptical orbit around the Earth providing a large percentage of observing time for northern polar regions. This version of the visualization has the camera riding the orbit as the spacecraft would with a MODIS swath and GOES footprint animating. The MODIS swath is colored red, and the GOES footprint is colored light gray. This shows how this proposal would provide more continuous coverage of north polar regions than MODIS and GOES can provide. || ",
            "hits": 18
        },
        {
            "id": 2971,
            "url": "https://svs.gsfc.nasa.gov/2971/",
            "result_type": "Visualization",
            "release_date": "2004-08-13T12:00:00-04:00",
            "title": "Galileo Earth Views (WMS)",
            "description": "The Galileo spacecraft was launched from the Space Shuttle Atlantis on October 18, 1989 on a six-year trip to Jupiter. On the way, the trajectory of the spacecraft took it past Venus once and Earth twice. Galileo took the Earth images in this animation just after the first flyby of the Earth, on December 11 and 12, 1990. This six-hour sequence of images taken two minutes apart clearly shows how the Earth looks from space and how fast (or slow) the cloud features change when looked at from a distance. The path of the sun can be seen crossing Australia by its reflection in the nearby ocean, and the terminator region between night and day can be seen moving across the Indian Ocean. In the original images, the Earth's rotation is so dominant that cloud movement is hard to see, but these images have been mapped to the Earth is such a way that a viewer can watch just the clouds move in the ocean around Antarctica or across the Australian land mass. In this animation, New Zealand can ony be seen as a stationary disturbance under a moving cloud bank. The black area with the sharp boundary to the north and east of Australia is the side of the Earth that could not be seen from Galileo's position. || ",
            "hits": 89
        },
        {
            "id": 2924,
            "url": "https://svs.gsfc.nasa.gov/2924/",
            "result_type": "Visualization",
            "release_date": "2004-06-28T12:00:00-04:00",
            "title": "Sun vs. Mission to Mars",
            "description": "Spacecraft (green trajectory) on their way from the Earth (blue orbit) to Mars (red orbit) risk being hit by energetic events from the Sun, such as X-rays, energetic protons (blue streaks), and material from Coronal Mass Ejections (CMEs) (red blobs).  The spiral lines from the Sun represent the magnetic field lines 'frozen' into the solar wind. || ",
            "hits": 25
        },
        {
            "id": 2948,
            "url": "https://svs.gsfc.nasa.gov/2948/",
            "result_type": "Visualization",
            "release_date": "2004-05-17T12:00:00-04:00",
            "title": "Simulated Aura/OMI Data Collection",
            "description": "On June 19, 2004, NASA launches Aura, a next generation Earth-observing satellite. One of several instruments on the Aura satellite is the Ozone Monitoring Instrument (OMI). OMI is a contribution of the Netherland's Agency for Aerospace Programs (NIVR) along with the Finnish Meteorological Institute (FMI). OMI will continue the TOMS record for total ozone and other atmospheric parameters related to ozone chemistry and climate. (For more information on the Aura project, please visit http://aura.gsfc.nasa.gov/)Note: The size of the satellite model in the following animation and stills has been exaggerated for aesthetic purposes. || ",
            "hits": 48
        },
        {
            "id": 1011,
            "url": "https://svs.gsfc.nasa.gov/1011/",
            "result_type": "Visualization",
            "release_date": "1999-11-10T12:00:00-05:00",
            "title": "Nine Datasets on a Single Globe with Wipe Between Different Datasets",
            "description": "Single globe with wipe between different data sets. Sequence: Galileo, radiant energy, vegetation index anomalies, temperature, fires, aerosols, clouds, methane, water vapor, biosphere, Galileo || ",
            "hits": 17
        },
        {
            "id": 1012,
            "url": "https://svs.gsfc.nasa.gov/1012/",
            "result_type": "Visualization",
            "release_date": "1999-11-10T12:00:00-05:00",
            "title": "Nine Datasets on a Single Globe with Wipe Between Different Datasets Run as a Continuous Two Minute Loop",
            "description": "Single globe with wipe between different data sets run as a continuous 2 minute loop. Sequence: Galileo, radiant energy (Globe), vegetation index anomalies, temperature (globe), fires, aerosols (TOMS), clouds (GOES 9 and 10, Meteosat, and GMS-5), methane (UARS), water vapor (GOES 9 and 10, Meteosat, and GMS-5), biosphere (SeaStar/SeaWiFS), Galileo || ",
            "hits": 18
        },
        {
            "id": 1013,
            "url": "https://svs.gsfc.nasa.gov/1013/",
            "result_type": "Visualization",
            "release_date": "1999-11-10T12:00:00-05:00",
            "title": "Six Annotated Datasets Pull Away from a Single Globe",
            "description": "Six globes showing data (biosphere, aerosols, radiant energy, air pollution, temperature, and water vapor) pull away from a single globe, to illustrate the measurements taken by the instruments on Terra || a001013.00005_print.png (720x480) [451.7 KB] || a001013_thm.png (80x40) [4.8 KB] || a001013_pre.jpg (320x238) [6.8 KB] || a001013_pre_searchweb.jpg (320x180) [49.5 KB] || a001013.webmhd.webm (960x540) [6.7 MB] || a001013.dv (720x480) [124.2 MB] || a001013.mpg (352x240) [4.5 MB] || ",
            "hits": 23
        },
        {
            "id": 1024,
            "url": "https://svs.gsfc.nasa.gov/1024/",
            "result_type": "Visualization",
            "release_date": "1999-11-10T12:00:00-05:00",
            "title": "Single Globe Galileo Dataset",
            "description": "A rotating Earth, using a composite image derived from the flyby of Galileo in December, 1990 || a001024.00005_print.png (720x480) [494.9 KB] || a001024_thm.png (80x40) [5.4 KB] || a001024_pre.jpg (320x242) [8.8 KB] || a001024_pre_searchweb.jpg (320x180) [59.9 KB] || a001024.webmhd.webm (960x540) [6.6 MB] || a001024.dv (720x480) [186.7 MB] || a001024.mpg (352x240) [7.5 MB] || ",
            "hits": 35
        },
        {
            "id": 328,
            "url": "https://svs.gsfc.nasa.gov/328/",
            "result_type": "Visualization",
            "release_date": "1998-10-20T12:00:00-04:00",
            "title": "Earth Today 1998 Countdown",
            "description": "The ability to see Earth from space has forever changed our view of the planet. We are now able to look at the Earth as a whole, and observe how its atmosphere, oceans, land masses, and life interact as global systems. Earth's atmosphere, hydrosphere, geosphere, and biosphere are dynamic, changing on timescales of days, minutes, or even seconds. Monitoring the Earth in near real time allows us to get an up to date picture of conditions on our planet. More SVS visualizations for the Earth Today exhibit are in animation ids 1401 and 1402. || ",
            "hits": 50
        },
        {
            "id": 1401,
            "url": "https://svs.gsfc.nasa.gov/1401/",
            "result_type": "Visualization",
            "release_date": "1998-10-20T12:00:00-04:00",
            "title": "Earth Today 1998 Introduction",
            "description": "The ability to see Earth from space has forever changed our view of the planet. We are now able to look at the Earth as a whole, and observe how its atmosphere, oceans, land masses, and life interact as global systems. Earth's atmosphere, hydrosphere, geosphere, and biosphere are dynamic, changing on timescales of days, minutes, or even seconds. Monitoring the Earth in near real time allows us to get an up to date picture of conditions on our planet. More SVS visualizations for the Earth Today exhibit can be found in animation ids 328 and 1402. || ",
            "hits": 45
        },
        {
            "id": 1402,
            "url": "https://svs.gsfc.nasa.gov/1402/",
            "result_type": "Visualization",
            "release_date": "1998-10-20T12:00:00-04:00",
            "title": "Earth Today 1998",
            "description": "The ability to see Earth from space has forever changed our view of the planet. We are now able to look at the Earth as a whole, and observe how its atmosphere, oceans, land masses, and life interact as global systems. Earth's atmosphere, hydrosphere, geosphere, and biosphere are dynamic, changing on timescales of days, minutes, or even seconds. Monitoring the Earth in near real time allows us to get an up to date picture of conditions on our planet. More SVS visualizations for the Earth Today exhibit can be found in animation ids 328 and 1401. || ",
            "hits": 67
        },
        {
            "id": 1371,
            "url": "https://svs.gsfc.nasa.gov/1371/",
            "result_type": "Visualization",
            "release_date": "1998-09-01T12:00:00-04:00",
            "title": "Earth Rotation from Galileo Imagery: 1 x Real-Time",
            "description": "This animation is one in a series created to show an accurate representation of the Earth's rotation at different temporal resolutions.  The animation is created from images taken by the Galileo spacecraft during a close pass of the Earth on December 11-12, 1990.  The animations range from real-time, in which no rotation can be perceived, to 3600 times real-time, in which both the Earth's rotation and cloud motion can bee seen.  The series also includes an animation in which the Earth's rotation has been 'halted' so that cloud motion is easier to see and an animation showing the specific amount of rotation that takes place in three minutes. || ",
            "hits": 54
        },
        {
            "id": 1372,
            "url": "https://svs.gsfc.nasa.gov/1372/",
            "result_type": "Visualization",
            "release_date": "1998-09-01T12:00:00-04:00",
            "title": "Earth Rotation from Galileo Imagery: 10 x Real-Time",
            "description": "This animation is one in a series created to show an accurate representation of the Earth's rotation at different temporal resolutions. The animation is created from images taken by the Galileo spacecraft during a close pass of the Earth on December 11-12, 1990. The animations range from real-time, in which no rotation can be perceived, to 3600 times real-time, in which both the Earth's rotation and cloud motion can bee seen. The series also includes an animation in which the Earth's rotation has been 'halted' so that cloud motion is easier to see and an animation showing the specific amount of rotation that takes place in three minutes. || ",
            "hits": 32
        },
        {
            "id": 1373,
            "url": "https://svs.gsfc.nasa.gov/1373/",
            "result_type": "Visualization",
            "release_date": "1998-09-01T12:00:00-04:00",
            "title": "Earth Rotation from Galileo Imagery: 100 x Real-Time",
            "description": "This animation is one in a series created to show an accurate representation of the Earth's rotation at different temporal resolutions. The animation is created from images taken by the Galileo spacecraft during a close pass of the Earth on December 11-12, 1990. The animations range from real-time, in which no rotation can be perceived, to 3600 times real-time, in which both the Earth's rotation and cloud motion can bee seen. The series also includes an animation in which the Earth's rotation has been 'halted' so that cloud motion is easier to see and an animation showing the specific amount of rotation that takes place in three minutes. || ",
            "hits": 240
        },
        {
            "id": 1374,
            "url": "https://svs.gsfc.nasa.gov/1374/",
            "result_type": "Visualization",
            "release_date": "1998-09-01T12:00:00-04:00",
            "title": "Earth Rotation from Galileo Imagery: 600 x Real-Time",
            "description": "This animation is one in a series created to show an accurate representation of the Earth's rotation at different temporal resolutions. The animation is created from images taken by the Galileo spacecraft during a close pass of the Earth on December 11-12, 1990. The animations range from real-time, in which no rotation can be perceived, to 3600 times real-time, in which both the Earth's rotation and cloud motion can bee seen. The series also includes an animation in which the Earth's rotation has been 'halted' so that cloud motion is easier to see and an animation showing the specific amount of rotation that takes place in three minutes. || ",
            "hits": 42
        },
        {
            "id": 1375,
            "url": "https://svs.gsfc.nasa.gov/1375/",
            "result_type": "Visualization",
            "release_date": "1998-09-01T12:00:00-04:00",
            "title": "Earth Rotation from Galileo Imagery: 3600 x Real-Time",
            "description": "This animation is one in a series created to show an accurate representation of the Earth's rotation at different temporal resolutions. The animation is created from images taken by the Galileo spacecraft during a close pass of the Earth on December 11-12, 1990. The animations range from real-time, in which no rotation can be perceived, to 3600 times real-time, in which both the Earth's rotation and cloud motion can bee seen. The series also includes an animation in which the Earth's rotation has been 'halted' so that cloud motion is easier to see and an animation showing the specific amount of rotation that takes place in three minutes. || ",
            "hits": 410
        },
        {
            "id": 1376,
            "url": "https://svs.gsfc.nasa.gov/1376/",
            "result_type": "Visualization",
            "release_date": "1998-09-01T12:00:00-04:00",
            "title": "Earth Rotation from Galileo Imagery: 3600 x Real-Time (no rotation)",
            "description": "This animation is one in a series created to show an accurate representation of the Earth's rotation at different temporal resolutions. The animation is created from images taken by the Galileo spacecraft during a close pass of the Earth on December 11-12, 1990. The animations range from real-time, in which no rotation can be perceived, to 3600 times real-time, in which both the Earth's rotation and cloud motion can bee seen. The series also includes an animation in which the Earth's rotation has been 'halted' so that cloud motion is easier to see and an animation showing the specific amount of rotation that takes place in three minutes. || ",
            "hits": 25
        },
        {
            "id": 1377,
            "url": "https://svs.gsfc.nasa.gov/1377/",
            "result_type": "Visualization",
            "release_date": "1998-09-01T12:00:00-04:00",
            "title": "Earth Rotation from Galileo Imagery: 3-Minute Interval",
            "description": "This animation is one in a series created to show an accurate representation of the Earth's rotation at different temporal resolutions. The animation is created from images taken by the Galileo spacecraft during a close pass of the Earth on December 11-12, 1990. The animations range from real-time, in which no rotation can be perceived, to 3600 times real-time, in which both the Earth's rotation and cloud motion can bee seen. The series also includes an animation in which the Earth's rotation has been 'halted' so that cloud motion is easier to see and an animation showing the specific amount of rotation that takes place in three minutes. || ",
            "hits": 90
        },
        {
            "id": 116,
            "url": "https://svs.gsfc.nasa.gov/116/",
            "result_type": "Visualization",
            "release_date": "1996-10-25T12:00:00-04:00",
            "title": "The HoloGlobe Project (Version 2)",
            "description": "This animation was produced for the Smithsonian Institution's HoloGlobe Exhibit which opened to the public on August 10, 1996. The various orthographic data sets showing progressive global change were mapped onto a rotating globe and projected into space to create a holographic image of the Earth. Showing Earthandapos;s atmosphere, hydrosphere, geosphere, and biosphere are dynamic, changing on timescales of days, minutes, or even seconds. This animation is a revised version of Animation #96 [The HoloGlobe Project (Version 1)]. || ",
            "hits": 64
        },
        {
            "id": 1319,
            "url": "https://svs.gsfc.nasa.gov/1319/",
            "result_type": "Visualization",
            "release_date": "1996-08-10T12:00:00-04:00",
            "title": "HoloGlobe: Galileo Earth",
            "description": "This is one of a series of animations that were produced to be part of the narrated video shown in the HoloGlobe exhibit at the Smithsonian Museum of Natural History and the Earth Today exhibit at the Smithsonian Air and Space Museum. || ",
            "hits": 90
        },
        {
            "id": 96,
            "url": "https://svs.gsfc.nasa.gov/96/",
            "result_type": "Visualization",
            "release_date": "1996-08-01T12:00:00-04:00",
            "title": "The HoloGlobe Project (Version 1)",
            "description": "This animation was originally produced for the Smithsonian Institution's HoloGlobe Exhibit which opened to the public on August 10, 1996 at the Museum of Natural History in Washington, DC.  These various data sets showing progressive global change were mapped onto a rotating globe and projected into space to create a holographic image of the Earth. Showing Earth's atmosphere, hydrosphere, geosphere, and biosphere are dynamic, changing on timescales of days, minutes, or even seconds. || ",
            "hits": 59
        },
        {
            "id": 155,
            "url": "https://svs.gsfc.nasa.gov/155/",
            "result_type": "Visualization",
            "release_date": "1996-08-01T12:00:00-04:00",
            "title": "The HoloGlobe Project (Version 3)",
            "description": "These animations were produced for the Smithsonian Institution's HoloGlobe Exhibit which opened to the public on August 10, 1996 at the Museum of Natural History in Washington, DC. The various data sets show progressive global change mapped onto a rotating globe and projected into space to create a holographic image of the Earth. The exhibit shows that Earth's atmosphere, hydrosphere, geosphere, and biosphere are dynamic, changing on timescales of days, minutes, or even seconds. The exhibit has since been relocated to the west coast. This is a revised version from Animation #116 [The HoloGlobe Project (version 2)]. || ",
            "hits": 77
        }
    ]
}