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"result_type": "Visualization",
"release_date": "2025-04-25T07:00:59-04:00",
"title": "Airborne Aerosol Wind Profiler (AWP) Measurements",
"description": "This is a visualization of Aerosol Wind Profiler (AWP) data aboard the NASA Gulfstream-III for a flight on 15 October 2024 that originated from NASA/Langley Research Center (LaRC) in Hampton, Virginia.",
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"url": "https://svs.gsfc.nasa.gov/31296/",
"result_type": "Hyperwall Visual",
"release_date": "2024-06-21T00:00:00-04:00",
"title": "Coming in Hot — NASA’s Chandra Checks Habitability of Exoplanets",
"description": "Credits:Movie: Cal Poly Pomona/B. Binder; Illustration: NASA/CXC/M.Weiss || chandra-exoplanets.00001_print.jpg (1024x576) [195.6 KB] || chandra-exoplanets.00001_searchweb.png (320x180) [78.4 KB] || chandra-exoplanets.00001_thm.png (80x40) [5.7 KB] || chandra-exoplanets.mp4 (1280x720) [63.9 MB] || chandra-exoplanets.webm (1280x720) [7.0 MB] || coming-in-hot-nasas-chandra-checks-habitability-of-exoplanets.hwshow [319 bytes] || ",
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"result_type": "Visualization",
"release_date": "2024-05-30T14:00:00-04:00",
"title": "NASA’s TEMPO Instrument Air Quality Data Now Publicly Available",
"description": "The TEMPO instrument measured elevated levels of nitrogen dioxide (NO2) from a number of different areas and emission sources throughout the daytime on March 28, 2024. Yellow, red, purple, and black clusters represent increased levels of pollutants from TEMPO’s data and show drift over time. || TEMPO_3_28_2024_CONUS.0500_print.jpg (1024x576) [289.5 KB] || TEMPO_3_28_2024_CONUS.0500_searchweb.png (320x180) [103.2 KB] || TEMPO_3_28_2024_CONUS.0500_thm.png (80x40) [6.9 KB] || TEMPO_3_28_2024_CONUS [0 Item(s)] || TEMPO_3_28_2024_CONUS_1080p30.mp4 (1920x1080) [29.3 MB] || TEMPO_3_28_2024_CONUS (3840x2160) [1000 Item(s)] || TEMPO_3_28_2024_CONUS_2160p30.mp4 (3840x2160) [111.7 MB] || TEMPO_3_28_2024_CONUS_1080p30.mp4.hwshow || ",
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"result_type": "Visualization",
"release_date": "2023-09-22T00:00:00-04:00",
"title": "Sea Surface Salinity Near The Maritime Continent",
"description": "This animation of sea surface salinity shows the flow of freshwater from the Pacific into the Indian Ocean. The flow of freshwater (low salinity, blue color in 30-32 range) through narrow gaps of the maritime continent is known as Indonesian Throughflow. || sss.2020110117_print.jpg (1024x576) [172.0 KB] || sss.2020110117.png (5760x3240) [3.0 MB] || sss.2020110117_searchweb.png (320x180) [94.3 KB] || sss.2020110117_thm.png (80x40) [8.5 KB] || fixed_sss_1080p60_h265.mp4 (1920x1080) [88.2 MB] || 5760x3240_16x9_30p (5760x3240) [1.0 MB] || 3840x2160_16x9_30p (3840x2160) [1.0 MB] || fixed_sss_2160p60.mp4 (3840x2160) [482.0 MB] || ",
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"release_date": "2023-05-01T00:00:00-04:00",
"title": "Cosmic Cycles 3 Earth as Art",
"description": "Starting in 1972, nine Landsat satellites have orbited Earth, taking images of the surface. This unprecedented coverage has been tremendously useful to the scientific community, but it has also produced thousands of beautiful high-resolution images of the complex patterns of our world. From the fractal patterns of mountain ranges and river deltas to the precise geometry of agriculture, Landsat has rendered Earth as a work of art.",
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"release_date": "2022-04-13T10:00:00-04:00",
"title": "Seaflow Search for Prochlorococcus",
"description": "Overview of data collected from research ship paths through the north Pacific Ocean measuring the phytoplankton species Prochlorococcus with an instrument called Seaflow. Additionally, results from the Darwin global ocean ecosystem computer model show interactions between Prochlorococcus, a copiotrophic heterotrophic bacteria and a shared grazer that limits the poleward extent of Prochlorococcus. || cruise_2-25-2022b_2022-02-25_1746.01500_print.jpg (1024x576) [71.2 KB] || cruise_2-25-2022b_2022-02-25_1746.01500_searchweb.png (320x180) [34.3 KB] || cruise_2-25-2022b_2022-02-25_1746.01500_thm.png (80x40) [3.4 KB] || cruise_2-25-2022b_2022-02-25_1746.webm (1920x1080) [12.8 MB] || annotated (1920x1080) [256.0 KB] || withAnnotation (3840x2160) [256.0 KB] || cruise_2-25-2022b_2022-02-25_1746.mp4 (1920x1080) [179.4 MB] || seaflowCruise_4k_3-31-2022b_2022-03-31_1056_2160p30.mp4 (3840x2160) [531.2 MB] || cruise_2-25-2022b_2022-02-25_1746.mp4.hwshow [238 bytes] || ",
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"release_date": "2022-04-13T10:00:00-04:00",
"title": "Darwin Model of Ocean Microbes Updated",
"description": "Left: Older Darwin model of global ocean microbiome showing no drop-off of Prochlorococcus populations in arctic regions.Right: New Darwin model, updated to show interactions between heterotrophic bacteria and shared grazer, which prevents Prochlorococcus habitat extending poleward. || seaflow_x4_2-26d_comp.01620_print.jpg (1024x576) [259.0 KB] || seaflow_x4_2-26d_comp.01620_searchweb.png (320x180) [79.6 KB] || seaflow_x4_2-26d_comp.01620_thm.png (80x40) [5.6 KB] || seaflow_x4_2-26d_comp.webm (1920x1080) [12.7 MB] || 1920x1080_16x9_30p (1920x1080) [256.0 KB] || 3840x2160_16x9_30p (3840x2160) [256.0 KB] || seaflow_x4_2-26d_comp.mp4 (1920x1080) [407.3 MB] || seaflowOverviewCOMP_4k_4-5-2022a_2160p30.mp4 (3840x2160) [863.7 MB] || seaflow_x4_2-26d_comp.mp4.hwshow [214 bytes] || ",
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"release_date": "2021-03-12T11:00:00-05:00",
"title": "Scientists Build a Detailed Image of U Mon Binary",
"description": "Two stars orbit each other within an enormous dusty disk in the U Monocerotis system, illustrated here. When the stars are farthest from each other, they funnel material from the disk’s inner edge. At this time, the primary star is slightly obscured by the disk from our perspective. The primary star, a yellow supergiant, expands and contracts. The smaller secondary star is thought to maintain its own disk of material, which likely powers an outflow of gas that emits X-rays.This listing includes Spanish-language and music-free versions.Credit: NASA’s Goddard Space Flight Center/Chris Smith (USRA/GESTAR)Music: \"Moving in Thought\" from Universal Production MusicNote: While this video in its entirety can be shared without permission, its music has been licensed and may not be excised or remixed in other products. || u_mon_full_edit_still.jpg (1920x1080) [707.8 KB] || u_mon_full_edit_still_print.jpg (1024x576) [294.6 KB] || u_mon_full_edit_still_searchweb.png (320x180) [80.8 KB] || u_mon_full_edit_still_web.png (320x180) [80.8 KB] || u_mon_full_edit_still_thm.png (80x40) [6.4 KB] || u_mon_full_edit_w_music_spanish_LQ.mp4 (1920x1080) [47.5 MB] || u_mon_full_edit_HQ.mp4 (1920x1080) [90.3 MB] || u_mon_full_edit_w_music_LQ.mp4 (1920x1080) [47.5 MB] || u_mon_full_edit_w_music_SVS_preview.webm (1280x720) [5.5 MB] || u_mon_full_edit_w_music_spanish_prores.mov (1920x1080) [526.2 MB] || u_mon_full_edit_w_music_spanish_HQ.mp4 (1920x1080) [96.6 MB] || u_mon_full_edit_w_music_prores.mov (1920x1080) [526.5 MB] || u_mon_full_edit_w_music_SVS_preview.mp4 (1280x720) [30.0 MB] || u_mon_full_edit_w_music_HQ.mp4 (1920x1080) [96.6 MB] || u_mon_full_edit_spanish_prores.mov (1920x1080) [488.5 MB] || u_mon_full_edit_prores.mov (1920x1080) [488.8 MB] || u_mon_full_edit_LQ.mp4 (1920x1080) [48.6 MB] || u_mon_full_edit_captions.en_US.vtt [536 bytes] || u_mon_full_edit_captions.en_US.srt [581 bytes] || ",
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"url": "https://svs.gsfc.nasa.gov/13267/",
"result_type": "Produced Video",
"release_date": "2019-11-05T13:00:00-05:00",
"title": "TESS Southern Hemisphere Sector Images",
"description": "Sector 1.The Transiting Exoplanet Survey Satellite (TESS) observed this strip of stars and galaxies in the southern sky from July 25, 2018, to August 22, 2018. TESS captured this individual image during one 30-minute period on 2018-08-07 at 04:59:42 UTC. The Large and Small Magellanic Clouds appear on the right-hand side. || TESS_Sector_1.png (16774x4272) [75.1 MB] || TESS_Sector_1.jpeg (16774x4272) [27.6 MB] || TESS_Sector_1_halfsize.jpeg (8387x2136) [9.7 MB] || TESS_Sector_1_halfsize.png (8387x2136) [9.7 MB] || ",
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"url": "https://svs.gsfc.nasa.gov/13248/",
"result_type": "Produced Video",
"release_date": "2019-07-25T06:00:00-04:00",
"title": "NASA’s Newest Planet Hunter To Reveal New Results From Its First Year In Orbit Live Shots",
"description": "B-roll and canned interviews to be added by 7:00 p.m. EDT July 24 || Screen_Shot_2019-07-03_at_10.56.17_AM.png (2980x462) [1.9 MB] || Screen_Shot_2019-07-03_at_10.56.17_AM_print.jpg (1024x158) [41.8 KB] || Screen_Shot_2019-07-03_at_10.56.17_AM_searchweb.png (180x320) [80.8 KB] || Screen_Shot_2019-07-03_at_10.56.17_AM_thm.png (80x40) [6.5 KB] || ",
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"url": "https://svs.gsfc.nasa.gov/13201/",
"result_type": "Produced Video",
"release_date": "2019-05-03T08:00:00-04:00",
"title": "The Story of Robert Goddard, Father of Modern Rocketry",
"description": "Dr. Robert Hutchings Goddard (1882-1945) is considered the father of modern rocket propulsion. It is in his memory that NASA’s Goddard Space Flight Center in Greenbelt, Maryland, was established on May 1, 1959.Music Credits: “Suburban Waltz” by Philip Guyler and “Unchartered Territories” by Phil Stevens Complete transcript available.Watch this video on the NASA Goddard YouTube channel. || RobertGoddard.03500_print.jpg (1024x576) [139.0 KB] || RobertGoddard.03500_searchweb.png (320x180) [69.4 KB] || RobertGoddard.03500_thm.png (80x40) [5.6 KB] || RobertGoddard.mp4 (1920x1080) [198.2 MB] || RobertGoddard.webm (1920x1080) [27.7 MB] || RobertGoddard.en_US.srt [3.2 KB] || ",
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"url": "https://svs.gsfc.nasa.gov/12916/",
"result_type": "Produced Video",
"release_date": "2018-12-11T14:00:00-05:00",
"title": "50th Anniversary of NASA's OAO 2 Mission",
"description": "“Seas of Infinity” (1968), full-length version scanned from 16mm color film and color corrected; run time 14:25. Original description: The film opens with an explanation of the electromagnetic spectrum. The limited capabilities of skyhook balloons and sounding rockets are used to illustrate the need for orbiting observatories. Reviews the planning, development, launching and function of the Orbiting Astronomical Observatory, a series of orbiting telescopes which are being used to study our solar system and the stars beyond. Features comments by the following leading scientists on the potential of this advancement in astronomy: Dr. Arthur Code, Wisconsin telescopes; Dr. James Kupperian, Goddard Flight Center using Cassegrain designs; Dr. Fred Whipple on the ultraviolet light sky mapping project; and Dr. Donald Morton on the Princeton OAO ultraviolet spectroscopy project. The film has scenes of the assembly of the OAO. The OAO will be launched by an Atlas-Centaur. Credit: NASAComplete transcript available. || Seas_Of_Infinity_OAO2_Color_Corrected.22261_print.jpg (1024x768) [40.5 KB] || Seas_Of_Infinity_OAO2_Color_Corrected.22261_searchweb.png (320x180) [42.3 KB] || Seas_Of_Infinity_OAO2_Color_Corrected.22261_thm.png (80x40) [4.5 KB] || Seas_Of_Infinity_OAO2_Color_Corrected.mp4 (640x480) [136.1 MB] || Seas_Of_Infinity_OAO2_SRT_Captions.en_US.srt [16.6 KB] || Seas_Of_Infinity_OAO2_SRT_Captions.en_US.vtt [16.6 KB] || Seas_Of_Infinity_OAO2_Color_Corrected.webm (640x480) [110.9 MB] || ",
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"url": "https://svs.gsfc.nasa.gov/13069/",
"result_type": "Produced Video",
"release_date": "2018-09-17T13:00:00-04:00",
"title": "NASA’s TESS Releases First Science Image",
"description": "The Transiting Exoplanet Survey Satellite (TESS) took this snapshot of the Large Magellanic Cloud (right) and the bright star R Doradus (left) with just a single detector of one of its cameras on Tuesday, Aug. 7. The frame is part of a swath of the southern sky TESS captured in its “first light” science image as part of its initial round of data collection.Credit: NASA/MIT/TESS || TESSFLleadimagefeature.jpg (987x1019) [839.4 KB] || ",
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"result_type": "Produced Video",
"release_date": "2018-08-08T16:00:00-04:00",
"title": "Parker Solar Probe Instruments",
"description": "SWEAPThe Solar Wind Electrons Alphas and Protons investigation, or SWEAP, gathers observations using two complementary instruments: the Solar Probe Cup, or SPC, and the Solar Probe Analyzers, or SPAN. The instruments count the most abundant particles in the solar wind — electrons, protons and helium ions — and measure such properties as velocity, density, and temperature to improve our understanding of the solar wind and coronal plasma. SWEAP was built mainly at the Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, and at the Space Sciences Laboratory at the University of California, Berkeley. The institutions jointly operate the instrument. The principal investigator is Justin Kasper from the University of Michigan. || SWEAP.00001_print.jpg (1024x581) [151.9 KB] || SWEAP_thumb.png (2560x1448) [4.7 MB] || SWEAP.00001_searchweb.png (320x180) [86.1 KB] || SWEAP.00001_web.png (320x181) [86.8 KB] || SWEAP.00001_thm.png (80x40) [5.6 KB] || SWEAP.webm (1902x1080) [21.8 MB] || SWEAP.mp4 (1902x1080) [195.4 MB] || SWEAP.en_US.srt [3.8 KB] || SWEAP.en_US.vtt [3.8 KB] || ",
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"url": "https://svs.gsfc.nasa.gov/13030/",
"result_type": "Produced Video",
"release_date": "2018-08-06T10:00:00-04:00",
"title": "NASA's Planet-Hunting TESS Catches a Comet Before Starting Science",
"description": "This video is compiled from a series of images taken on July 25 by the Transiting Exoplanet Survey Satellite. The angular extent of the widest field of view is six degrees. Visible in the images are the comet C/2018 N1, asteroids, variable stars, asteroids and reflected light from Mars. TESS is expected to find thousands of planets around other nearby stars. Credit: Massachusetts Institute of Technology/NASA’s Goddard Space Flight CenterWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || TESS_Comet_Still.jpg (1920x1080) [409.0 KB] || TESS_Comet_Still_print.jpg (1024x576) [112.2 KB] || TESS_Comet_Still_searchweb.png (320x180) [50.8 KB] || TESS_Comet_Still_thm.png (80x40) [3.8 KB] || 13030_TESS_Comet_ProRes_1080_2997.mov (1920x1080) [1.7 GB] || 13030_TESS_Comet_1080.mp4 (1920x1080) [118.6 MB] || 13030_TESS_Comet_H264_1080_Best.mov (1920x1080) [173.0 MB] || 13030_TESS_Comet_H264_1080_Good.m4v (1920x1080) [114.8 MB] || 13030_TESS_Comet_ProRes_1080_2997.webm (1920x1080) [10.8 MB] || 13030_TESS_Comet_SRT_Captions.en_US.srt [1.3 KB] || 13030_TESS_Comet_SRT_Captions.en_US.vtt [1.3 KB] || ",
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"url": "https://svs.gsfc.nasa.gov/12576/",
"result_type": "Produced Video",
"release_date": "2017-04-10T11:00:00-04:00",
"title": "NASA Catches April 1 Nor'easter over New England",
"description": "The Global Precipitation Measurement mission catches the April 1, 2017, Nor'easter over New England.Music: \"Flowing with Time,\" Philippe Lhommet, KOKA MediaComplete transcript available. || 12576_April1Noreaster.00038_print.jpg (1024x576) [194.0 KB] || 12576_April1Noreaster.00038_searchweb.png (320x180) [115.8 KB] || 12576_April1Noreaster.00038_thm.png (80x40) [7.5 KB] || 12576_April1Noreaster.mp4 (1920x1080) [84.3 MB] || 12576_April1Noreaster.en_US.srt [1.3 KB] || 12576_April1Noreaster.en_US.vtt [1.3 KB] || 12576_April1Noreaster_prores.mov (1920x1080) [1.0 GB] || ",
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"release_date": "2017-03-10T00:00:00-05:00",
"title": "NICER Mission B-roll Footage",
"description": "The Neutron star Interior Composition Explorer (NICER) mission was built and tested at NASA's Goddard Space Flight Center in Greenbelt, Maryland.In addition to NASA Goddard scientists and engineers, the mission team includes the Massachusetts Institute of Technology and commercial partners, who provided spaceflight hardware. || ",
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"result_type": "Produced Video",
"release_date": "2016-11-07T13:45:00-05:00",
"title": "Small Satellites for Earth Science",
"description": "NASA has embraced the revolution in small spacecraft and satellites, from CubeSats you can hold in your hand to microsatellites the size of a small washing machine. The technology helps advance scientific and human exploration, reduces the cost of new missions, and expands access to space. The briefing will discuss NASA's overall program, technology development initiatives, and new Earth-observing missions that use individual and constellations of small satellites to study climate change, hurricanes and clouds.Briefing PanelistsEllen Stofan, chief scientists at NASA Headquarters in WashingtonThomas Zurbuchen, associate administrator for the Science Mission Directorate at NASA HeadquartersSteve Jurczyk, associate administrator for the Science Mission Directorate at NASA HeadquartersMichael Freilich, director of the Earth Science Division at NASA HeadquartersAaron Ridley, mission constellation scientist for NASA's Cyclone Global Navigation Satellite System (CYGNSS) at the University of Michigan in Ann ArborBill Swartz, CubeSat principal investigator for the Radiometer Assessment using Vertically Aligned Nanotubes (RAVAN) project at Johns Hopkins University Applied Physics Laboratory in Laurel, MarylandWilliam Blackwell, principal investigator for the Time-Resolved Observations of Precipitation structure and storm Intensity with a Constellation of Smallsat (TROPICS) mission at the Massachusetts Institute of Technology Lincoln Laboratory, Lexington, Mass.More information is available. || ",
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{
"id": 4499,
"url": "https://svs.gsfc.nasa.gov/4499/",
"result_type": "Visualization",
"release_date": "2016-10-21T00:00:00-04:00",
"title": "Orientale Impact Basin for the Cover of Science",
"description": "This print-resolution still image was created for the cover of the October 28, 2016 issue of Science. It features a free-air gravity map of the Orientale impact basin based on data returned by the Gravity Recovery and Interior Laboratory (GRAIL) mission.Orientale is about 930 kilometers wide and lies on the western limb of the Moon as viewed from Earth. It's the Moon's youngest and best-preserved large impact basin, formed about 3.8 billion years ago at the end of the conjectured Late Heavy Bombardment. A paper in Science by Maria Zuber et al. uses the GRAIL data to shed new light on the basin's geology, while a second paper by Brandon Johnson et al. describes a computer simulation of the basin's formation constrained by that data.The shaded relief in this image is not a photograph. It's a very accurate computer rendering based on a digital model of the terrain. The model is derived from a digital elevation map called SLDEM2015. This map combines data from the laser altimeter (LOLA) on NASA's Lunar Reconnaissance Orbiter (LRO) with stereo imagery from the Terrain Camera on the Japan Space Agency's SELENE spacecraft.The angle of the virtual Sun was chosen to throw Orientale's terrain into high relief — it's just after sunrise at Orientale, about a day past full Moon. The camera is on the western terminator (day/night line) looking north.The colorful part is the gravity anomaly based on measurements by GRAIL. Red indicates areas of higher gravity, or excess mass, and blue indicates lower gravity or areas of mass deficits. The GRAIL data reveals the structure of the basin beneath the surface. The red in the center of the basin, for example, shows that the crust is particularly thin there, and that denser mantle material is closer to the surface. || ",
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},
{
"id": 12181,
"url": "https://svs.gsfc.nasa.gov/12181/",
"result_type": "Produced Video",
"release_date": "2016-03-22T16:56:00-04:00",
"title": "Mars Gravity Map",
"description": "Scientists have used small fluctuations in the orbits of three NASA spacecraft to map the gravity field of Mars. || c-1024.jpg (1024x576) [238.0 KB] || c-1280.jpg (1280x720) [324.9 KB] || c-1920.jpg (1920x1080) [504.9 KB] || c-1024_print.jpg (1024x576) [251.2 KB] || c-1024_searchweb.png (320x180) [97.5 KB] || c-1024_web.png (320x180) [97.5 KB] || c-1024_thm.png (80x40) [7.0 KB] || ",
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{
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"url": "https://svs.gsfc.nasa.gov/4436/",
"result_type": "Visualization",
"release_date": "2016-03-21T12:30:00-04:00",
"title": "GMM-3 Mars Gravity Map",
"description": "Scientists have used small fluctuations in the orbits of three NASA spacecraft to map the gravity field of Mars.Watch this video on the NASA Goddard YouTube channel.Complete transcript available.This video is also available on our YouTube channel. || MarsGravityMapYouTube.png (1920x1080) [7.9 MB] || MarsGravityMapYouTube.jpg (1920x1080) [706.6 KB] || APPLE_TV_G2016-003_Mars_Gravity_Map_MASTER_appletv.m4v (1280x720) [51.0 MB] || WEBM_G2016-003_Mars_Gravity_Map_MASTER.webm (960x540) [43.4 MB] || APPLE_TV_G2016-003_Mars_Gravity_Map_MASTER_appletv_appletv_subtitles.m4v (1280x720) [15.5 MB] || LARGE_MP4_G2016-003_Mars_Gravity_Map_MASTER_large.mp4 (1920x1080) [109.0 MB] || NASA_TV_G2016-003_Mars_Gravity_Map_MASTER.mpeg (1280x720) [362.0 MB] || G2016-003_Mars_Gravity_Map_MASTER_GoogOut.en_US.srt [1.8 KB] || G2016-003_Mars_Gravity_Map_MASTER_GoogOut.en_US.vtt [1.9 KB] || G2016-003_Mars_Gravity_Map_MASTER.mov (1920x1080) [2.9 GB] || ",
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"url": "https://svs.gsfc.nasa.gov/gallery/live-shots-gallery/",
"result_type": "Gallery",
"release_date": "2015-11-27T00:00:00-05:00",
"title": "Live Shots Gallery Collection",
"description": "Collection of live shot pages of b-roll and interviews!",
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"url": "https://svs.gsfc.nasa.gov/4398/",
"result_type": "Visualization",
"release_date": "2015-11-18T00:00:00-05:00",
"title": "Ocean Surface CO2 Flux with Wind Stress",
"description": "This animation shows the ocean surface CO2 flux between 1/1/2009 and 12/31/2010. Blue colors indicate uptake and orange-red colors indicate outgassing of ocean carbon. The pathlines indicate surface wind stress. || CO2flux_windStress.00480_print.jpg (1024x576) [213.6 KB] || CO2flux_windStress.00480_searchweb.png (180x320) [97.8 KB] || CO2flux_windStress.00480_thm.png (80x40) [7.2 KB] || CO2flux_windStress_1080p30.webm (1920x1080) [23.4 MB] || 3840x2160_16x9_30p (3840x2160) [512.0 KB] || 5760x3240_16x9_30p (5760x3240) [512.0 KB] || CO2flux_windStress_1080p30.mp4 (1920x1080) [673.7 MB] || CO2flux_windStress_2160p30.mp4 (3840x2160) [1.7 GB] || CO2flux_windStress_4398.key [679.6 MB] || CO2flux_windStress_4398.pptx [677.0 MB] || CO2flux_windStress_1080p30.mp4.hwshow [201 bytes] || ",
"hits": 55
},
{
"id": 4377,
"url": "https://svs.gsfc.nasa.gov/4377/",
"result_type": "Visualization",
"release_date": "2015-10-02T16:00:00-04:00",
"title": "A 3-D Look at Weather, Clouds, and Aerosols",
"description": "This gallery was created for Earth Science Week 2015 and beyond. It includes a quick start guide for educators and first-hand stories (blogs) for learners of all ages by NASA visualizers, scientists and educators. We hope that your understanding and use of NASA's visualizations will only increase as your appreciation grows for the beauty of the science they portray, and the communicative power they hold. Read all the blogs and find educational resources for all ages at: The Earth Science Week 2015 page.I've always been fascinated by our atmosphere. Think about it: even though we don't see it, above us is a great aerial ocean! Over time my fascination has grown from weather maps and pondering the origins of storms, to learning all about the physics that surround our everyday lives. From as early as grade school I was also very interested in computers: diagnosing errors, developing programming skills and learning all about hardware and operating systems. So you might say my interests naturally led me to a career as a NASA scientist, where I create visualizations to study the underlying factors that drive weather patterns. Visualizations help us to see the world differently and actively.Many of you have no doubt seen your homes from space using a program called Google Earth™. But did you know you could do a lot more with the right data? In fact I often use it to map atmospheric data in three-dimensions (3-D) around the globe. But one of the challenges I often face is that data comes from many different sources, such as NASA and NOAA satellites or ground-observation stations. This means the data is stored on computer disks all over the country and are named and organized according to different standards, requiring us to customize techniques for producing accurate visualizations in one, 3-D display of the Earth. We do this in order to analyze atmospheric relationships more easily because many weather phenomena arise from physical interactions, both horizontally and vertically, in the global circulation.A big part of atmospheric research relies on using computer models to simulate what our atmosphere will do under different conditions. A great example of this is the data used to prepare the daily weather forecast. This data originates from weather forecasting models that calculate atmospheric motions using the world’s fastest supercomputers. But how do we know these forecasts are accurate? Researchers can verify a model's performance by visualizing one of the variables such as temperature, humidity, wind speed, wind direction, or air pressure and then using color shading, contour curves, and wind \"barbs\" to graph that data. Then they overlay the observations from NASA satellites such as cloud-top imagery, cloud-top temperature, and vertical distributions of clouds and aerosols, with the graph (it can be challenging to synchronize the data display as these times usually don't match). After this process, the display confirms the model's accuracy. This method is used to study many atmospheric events, such as timing of a storm system, precipitation, or the direction of dust or smoke transport. || ",
"hits": 147
},
{
"id": 30669,
"url": "https://svs.gsfc.nasa.gov/30669/",
"result_type": "Hyperwall Visual",
"release_date": "2015-09-30T18:00:00-04:00",
"title": "Modeled Phytoplankton Communities in the Global Ocean",
"description": "Phytoplankton are the base of the marine food web and are crucial players in the Earth's carbon cycle. They are also incredibly diverse. This visualization shows dominant phytoplankton types from 1994-1998 generated by the Darwin Project using a high-resolution ocean and ecosystem model. The model contains flow fields from 1994-1998 (generated by the ECCO2 model), inorganic nutrients, 78 species of phytoplankton, zooplankton, as well as particulate and dissolved organic matter. Colors represent the most dominant type of phytoplankton at a given location based on their size and ability to uptake nutrients. Red represents diatoms (big phytoplankton, which need silica), yellow represents flagellates (other big phytoplankton), green represents prochlorococcus (small phytoplankton that cannot use nitrate), and cyan represents synechococcus (other small phytoplankton). Opacity indicates concentration of the carbon biomass.A key part of the Darwin Project is developing theoretical and numerical models of the marine ecosystems. The data shown here are from a simulation of the Darwin model in a physical run of the Massachusetts Institute of Technology general circulation model by the Estimating the Circulation and Climate of the Ocean (ECCO) group. The model provides a laboratory to explore the controls on biodiversity and the biogeography of different phytoplankton species. In particular, the role of the swirls and filaments (mesoscale features) appear important in maintaining high biodiversity in the ocean. || ",
"hits": 126
},
{
"id": 11833,
"url": "https://svs.gsfc.nasa.gov/11833/",
"result_type": "Produced Video",
"release_date": "2015-04-07T11:30:00-04:00",
"title": "Portrait Of An Asteroid",
"description": "Scientists use lasers to create a 3-D model of asteroid Eros. || c-1280.jpg (1280x720) [118.7 KB] || c-1024.jpg (1024x576) [82.2 KB] || c-1024_print.jpg (1024x576) [77.5 KB] || c-1024_searchweb.png (320x180) [40.5 KB] || c-1024_print_thm.png (80x40) [10.2 KB] || ",
"hits": 70
},
{
"id": 4258,
"url": "https://svs.gsfc.nasa.gov/4258/",
"result_type": "Visualization",
"release_date": "2015-02-06T00:00:00-05:00",
"title": "Mercury Mascons for the Cover of JGR Planets",
"description": "A gravity map of Mercury shows mass concentrations (red) centered on the Caloris basin (center) and the Sobkou region (right limb). || mercury_jgr_print.jpg (1024x1280) [170.5 KB] || mercury_jgr_print_ipad_poster_frame.jpg (1024x576) [113.1 KB] || mercury_jgr_web.jpg (320x400) [19.5 KB] || mercury_jgr_searchweb.png (320x180) [71.9 KB] || mercury_jgr_thm.png (80x40) [5.2 KB] || mercury_jgr.tif (2400x3000) [5.7 MB] || ",
"hits": 44
},
{
"id": 4266,
"url": "https://svs.gsfc.nasa.gov/4266/",
"result_type": "Visualization",
"release_date": "2015-01-28T00:00:00-05:00",
"title": "GPM Sees 2015 Nor'easter Dump Snow on New England",
"description": "Animation of the Nor'easter as it develops and moves east of the New England coast and then stops on January 26 at 5:06pm EST while GPM takes a snapshot of the storm. Slicing through the volumetric precipitation data shows the low lying nature of this storm as well as the intense precipitation amounts at it's center. The massive potentional for precipitation can be seen in the underlying GMI ground precipitation data. Had the center of the storm parked over New England, it could have generated massive amounts of snowfall. Luckily, it quickly moved out over the warmer ocean water and only the outer bands affected New England, still generating considerable snowfall, but not the historical totals that had been anticipated. || juno1080p.0300_print.jpg (1024x576) [166.7 KB] || juno720p.webm (1280x720) [5.1 MB] || juno1080p.mp4 (1920x1080) [21.3 MB] || juno720p.mp4 (1280x720) [11.2 MB] || 1920x1080_16x9_30p (1920x1080) [64.0 KB] || juno1080p_4266.pptx [23.0 MB] || juno1080p_4266.key [25.6 MB] || juno1080p.mp4.hwshow [190 bytes] || ",
"hits": 42
},
{
"id": 11587,
"url": "https://svs.gsfc.nasa.gov/11587/",
"result_type": "Produced Video",
"release_date": "2014-07-17T11:00:00-04:00",
"title": "The Moving Shoreline",
"description": "Beaches are dynamic, living landscapes, and the prime example of their evolution is the coastal barrier. These islands and spits run parallel to the mainland and protect it from the full force of ocean winds and waves. More than 2,100 barriers front about 10 percent of the world’s continental shorelines. These sandy barriers are constantly raised up, shifted, and torn down by the natural ebb and flow of waves, currents, winds, and tides. Hooks form, inlets open and close, and beaches slowly march across their back bays and lagoons toward the mainland. This process allows them to naturally move ever upwards as sea levels rise. Since 1984, USGS-NASA Landsat satellites have observed coastline changes off of Chatham, Massachusetts, on the southeastern elbow of Cape Cod. Over the past 30 years, three major breaches opened, and barrier islands connected to the coastline and to each other. Watch the video to see the changes unfold. || ",
"hits": 48
},
{
"id": 4175,
"url": "https://svs.gsfc.nasa.gov/4175/",
"result_type": "Visualization",
"release_date": "2014-06-17T00:00:00-04:00",
"title": "GRAIL Gravity Map for the Cover of Geophysical Research Letters",
"description": "This print-resolution still image was created for the cover of the May 28, 2014 issue of Geophysical Research Letters. It features a free-air gravity map of the Moon's southern latitudes developed by S. Goossens et al. from data returned by the Gravity Recovery and Interior Laboratory (GRAIL) mission.If the Moon were a perfectly smooth sphere of uniform density, the gravity map would be a single, featureless color, indicating that the force of gravity at a given elevation was the same everywhere. But like other rocky bodies in the solar system, including Earth, the Moon has both a bumpy surface and a lumpy interior. Spacecraft in orbit around the Moon experience slight variations in gravity caused by both of these irregularities.The free-air gravity map shows deviations from the mean gravity that a cueball Moon would have. The deviations are measured in milliGals, a unit of acceleration. On the map, purple is at the low end of the range, at around -400 mGals, and red is at the high end near +400 mGals. Yellow denotes the mean.The map shown here extends from the south pole of the Moon up to 50°S and reveals the gravity for that region in even finer detail than the global gravity maps published previously. The image illustrates the very good correlation between the gravity map and topographic features such as peaks and craters, as well as the mass concentration lying beneath the large Schrödinger basin in the center of the frame. The terrain in the image is based on Lunar Reconnaissance Orbiter (LRO) altimeter and camera data. || ",
"hits": 212
},
{
"id": 30494,
"url": "https://svs.gsfc.nasa.gov/30494/",
"result_type": "Hyperwall Visual",
"release_date": "2014-03-01T00:00:00-05:00",
"title": "Simulated Sea Surface Speeds",
"description": "This simulation shows sea surface speed in ultra-high resolution. Several oceanic characteristics are included in the simulation and are visible in its output; including tides, atmospheric pressure forcing, diurnal cycles, and dynamic/thermodynamic sea ice . The model has a .75 to 2.2 km horizontal grid spacing and 90 vertical levels, with 1-m vertical levels near the surface. The full 3D grid is output at hourly intervals.Yellow shades represent relatively fast sea surface speeds, while red shades represent slower speeds. The simulation was carried out using the Massachusetts Institute of Technology general circulation model (mitgcm.org) by the Estimating the Circulation and Climate of the Ocean (ECCO) group. Credits: C. Hill, G. Forget (MIT)C. Henze, B. Nelson, B. Ciotti (Ames)D. Menemenlis (JPL)A. Chaudhuri (AER)MITgcm/ECCO developers and usersSGI and NAS computer scientists and engineers || ",
"hits": 30
},
{
"id": 11186,
"url": "https://svs.gsfc.nasa.gov/11186/",
"result_type": "Produced Video",
"release_date": "2013-02-12T00:00:00-05:00",
"title": "Final Orbit",
"description": "On December 17, 2012, two NASA spacecraft slammed into a ridge near the moon's north pole. The collisions marked the planned end to NASA's GRAIL (Gravity Recovery and Interior Laboratory) mission. Flying in formation, the twin, washing machine-sized probes, named Ebb and Flow, spent 351 days in lunar orbit mapping the moon's gravitational field. The maps revealed features of the lunar surface and interior in incredible detail, providing scientists with new information about the moon's craggy topography and lumpy crust. Using these maps, researchers will be able to peer back at the moon's early history and better understand its origin and development, along with that of Earth and the other rocky bodies in the solar system. The visualization shows the two spacecraft's final three orbits and their mission-ending crash. || ",
"hits": 33
},
{
"id": 4041,
"url": "https://svs.gsfc.nasa.gov/4041/",
"result_type": "Visualization",
"release_date": "2013-02-08T00:00:00-05:00",
"title": "GRAIL Free-Air Gravity Map for the Cover of Science",
"description": "These print-resolution stills were created for the cover of the February 8, 2013 issue of Science. They show the free-air gravity map developed by the Gravity Recovery and Interior Laboratory (GRAIL) mission.If the Moon were a perfectly smooth sphere of uniform density, the gravity map would be a single, featureless color, indicating that the force of gravity at a given elevation was the same everywhere. But like other rocky bodies in the solar system, including Earth, the Moon has both a bumpy surface and a lumpy interior. Spacecraft in orbit around the Moon experience slight variations in gravity caused by both of these irregularities.The free-air gravity map shows deviations from the mean, the gravity that a cueball Moon would have. The deviations are measured in milliGals, a unit of acceleration. On the map, dark purple is at the low end of the range, at around -400 mGals, and red is at the high end near +400 mGals. Yellow denotes the mean.These views show a part of the Moon's surface that's never visible from Earth. They are centered on lunar coordinates 29°N 142°E. The large, multi-ringed impact feature near the center is Mare Moscoviense. The crater Mendeleev is south of this. The digital elevation model for the terrain is from the Lunar Reconnaissance Orbiter laser altimeter (LOLA). Merely for plausibility, the sun angle and starry background are accurate for specific dates (December 21, 2012, 0:00 UT and January 8, 2013, 14:00 UT, respectively). || ",
"hits": 71
},
{
"id": 11184,
"url": "https://svs.gsfc.nasa.gov/11184/",
"result_type": "Produced Video",
"release_date": "2013-02-05T00:00:00-05:00",
"title": "Mercury's Ice Lockers",
"description": "Mercury, the closest planet to the sun, sits in the hot seat, with temperatures soaring up to 800 degrees Fahrenheit. Certain spots at the planet's north and south poles, however, remain extremely cold—so cold, in fact, that scientists long suspected this sun-scorched planet of harboring ice. Sure enough, in 2012 NASA's MESSENGER (MErcury Surface, Space ENvironment, GEochemistry, and Ranging) mission reported finding deposits of ice and frozen chemicals at Mercury's north pole. Granted, Mercury doesn't have the same kind of ice cap Earth does. But if all the deposits were added up, there would be enough ice to bury Washington, D.C., under a layer two miles thick. Watch the animation to see just how bone-chillingly dark Mercury's north pole can be, especially in deep craters, where the sun may never shine. || ",
"hits": 334
},
{
"id": 4023,
"url": "https://svs.gsfc.nasa.gov/4023/",
"result_type": "Visualization",
"release_date": "2012-12-17T09:00:00-05:00",
"title": "GRAIL Impacts the Moon",
"description": "The Gravity Recovery and Interior Laboratory (GRAIL) mission comprises a pair of satellites launched in September, 2011 and placed in orbit around the Moon in January, 2012. The two satellites, named Ebb and Flow, used radio signals to precisely measure their separation as they flew in formation, one following the other in the same nearly circular polar orbit. These measurements allowed mission scientists to build up an accurate and detailed gravity map of the Moon.GRAIL ends its successful mission by impacting the Moon on December 17, 2012 at approximately 5:27 p.m. EST (22:27 UT). The two spacecraft were placed in an orbit that takes them within a kilometer of the surface, so low that they will hit the side of an unnamed mountain that lies between Mouchez and Philolaus craters, near the north pole at 75°45'N, 26°11'W. Ebb strikes first, followed 24 seconds later by Flow.This animation shows the last three orbits of the two spacecraft, with views of the impact site. The impact occurs on the night side of a waxing crescent Moon, so the view shifts from a natural color Moon to a false-color elevation map. || ",
"hits": 55
},
{
"id": 4014,
"url": "https://svs.gsfc.nasa.gov/4014/",
"result_type": "Visualization",
"release_date": "2012-12-05T12:00:00-05:00",
"title": "GRAIL Primary Mission Gravity Maps (AGU 2012)",
"description": "The Gravity Recovery and Interior Laboratory (GRAIL) mission comprises a pair of satellites launched in September, 2011 and placed in orbit around the Moon in January, 2012. The two satellites, named Ebb and Flow, used radio signals to precisely measure their separation as they flew in formation, one following the other in the same nearly circular polar orbit. These measurements allowed mission scientists to build up an accurate and detailed gravity map of the Moon.If the Moon were a perfectly smooth sphere of uniform density, the gravity experienced by the spacecraft would be exactly the same everywhere. But like other rocky bodies in the solar system, including the Earth, the Moon has both a bumpy surface and a lumpy interior. As the spacecraft fly in their orbits, they experience slight variations in gravity caused by both of these irregularities, variations which show up as small changes in the separation of the two spacecraft.The free-air gravity map shows these variations directly. (Free-air is a historical term; there is, of course, no air on the Moon.) The Bouguer gravity map subtracts the effect of the bumpy surface to show the lumpiness underneath. The elevation maps from the laser altimeter on Lunar Reconnaissance Orbiter (LRO) were used to create a model of what the gravity would be if the Moon were bumpy but not lumpy. This model was then subtracted from the free-air map to produce the Bouguer map. (Note: The Bouguer map shown here was filtered to emphasize smaller features; harmonic degrees 1 to 6 were excluded.)The crustal thickness map is inferred from the Bouguer map: If the density of the crust is assumed to be uniform, then the gravity anomalies visible in the Bouguer gravity map can be explained by variations in the thickness of the crust. Highs in gravity indicate places where the denser mantle is closer to the surface, and hence where the crust is thinner.While aiding navigation for future lunar missions, GRAIL's gravity measurements reveal information about the internal structure of the Moon, improving our understanding of the origin and development of not just the Moon, but also the Earth and the rest of the inner solar system. || ",
"hits": 164
},
{
"id": 30020,
"url": "https://svs.gsfc.nasa.gov/30020/",
"result_type": "Hyperwall Visual",
"release_date": "2012-11-21T00:00:00-05:00",
"title": "The Not-So \"Milky\" Milky Way",
"description": "Bound together by gravity, galaxies are large collections of stars and stellar remnants that coexist with interstellar gas and dust (as well as dark matter). On a clear night, our galaxy—the Milky Way—can be seen by the naked eye, but because our eyes cannot distinguish the individual stars that make up the glowing band of light, it appears “milky.” Infrared telescopes, however, see with different “eyes,” capable of detecting various wavelengths (outside the visible range) that provide unprecedented views of our Galaxy and beyond. This not-so-milky image of the Milky Way—nearly free of the obscuring effects of interstellar dust—was made with data from two highly automated 1.3 m ground-based telescopes used during the Two Micron All Sky Survey (2MASS) project. 2MASS is a joint project of the University of Massachusetts in Amherst and the Infrared Processing and Analysis Center at the California Institute of Technology. 2MASS has uniformly scanned the entire sky in three near-infrared bands, using two highly-automated 1.3-meter telescopes, one at a northern hemisphere facility and the other in a southern hemisphere facility. Images such as this, allow scientists to gain a better understanding of the structure of our Galaxy and the universe. || ",
"hits": 602
},
{
"id": 11076,
"url": "https://svs.gsfc.nasa.gov/11076/",
"result_type": "Produced Video",
"release_date": "2012-09-06T00:00:00-04:00",
"title": "America On Fire",
"description": "For more than a decade, NASA satellites have monitored fires around the world. The data that is collected provides scientists with information about the location of fires, how much land is burned and how fires are responding to changes in climate. Dry conditions, for example, fueled a number of wildfires in the United States in recent years. From 2009 to 2011, more than 200,000 fires burned 18 million acres, or roughly all of Massachusetts, Vermont, New Hampshire, Delaware and Rhode Island. Exacerbated by ongoing drought conditions in the South, the state of Texas experienced an extreme wildfire season in 2011 that consumed more than 2.7 million acres. The visualization shows fires detected in the United States from July 2002 through July 2011 by the MODIS instrument aboard NASA's Aqua and Terra satellites. Look for fires that reliably burn each year in western states and across the Southeast. || ",
"hits": 41
},
{
"id": 11050,
"url": "https://svs.gsfc.nasa.gov/11050/",
"result_type": "Produced Video",
"release_date": "2012-07-18T00:00:00-04:00",
"title": "Landsat 40th Liveshot City Images",
"description": "The following are U.S. cities imaged by Landsat over its 40 year span. Multiple years of selected cities are grouped together with specific years in parentheses. || Atlanta, Georgia || Atlanta_crop_321_1920x1080.jpg (1920x1080) [3.8 MB] || Atlanta_crop_321_1920x1080_web.png (320x180) [347.9 KB] || landsat_us_city_image.hwshow [65 bytes] || ",
"hits": 73
},
{
"id": 4716,
"url": "https://svs.gsfc.nasa.gov/4716/",
"result_type": "Visualization",
"release_date": "2012-06-21T00:00:00-04:00",
"title": "Visualizing Shackleton Crater",
"description": "A visualization of Shackleton crater. The near (Earth-facing) side of the Moon is to the right. In the false-color elevation on the left, red is higher and blue is lower. || shackleton_split_final_print.jpg (1024x1024) [280.9 KB] || shackleton_split_final_searchweb.png (320x180) [87.2 KB] || shackleton_split_final_thm.png (80x40) [7.1 KB] || shackleton_split_final.tif (3600x3600) [12.8 MB] || ",
"hits": 568
},
{
"id": 10835,
"url": "https://svs.gsfc.nasa.gov/10835/",
"result_type": "Produced Video",
"release_date": "2011-10-13T00:00:00-04:00",
"title": "Space Lasers",
"description": "While most satellites work like digital cameras and passively record a narrow spectrum of emitted or reflected radiation—visible light, in a camera's case—those equipped with lidar (Light Detection And Ranging) instruments use rapidly pulsating laser beams to actively detect specific features. Measurements made with lidar in recent years have provided detailed information about the topography of Earth's surface and characteristics of its atmosphere. ICESat, a NASA laser altimetry mission launched in 2003, monitored the changing elevation of Arctic and Antarctic ice sheets and created 3-D maps of forest canopies throughout the world. Since 2006 NASA's CALIPSO satellite has detected clouds and airborne particles that reflect or absorb heat and help drive global climate. Watch the video below to learn how this advanced technology is used to study the contours of ice, clouds, trees, and even the cratered terrain of the moon. || ",
"hits": 61
},
{
"id": 10757,
"url": "https://svs.gsfc.nasa.gov/10757/",
"result_type": "Produced Video",
"release_date": "2011-04-14T00:00:00-04:00",
"title": "Intro to LIDAR 3D",
"description": "Want to know the 3D shape of terrain on another planet? Want to study the height and density of Earth's forests? An amazing tool called LIDAR can help. Learn more in this video!This video is presented in stereoscopic 3D for those who can view it. We've included left and right eye clips, a side-by-side version, and an anaglyph (red/blue) version. Download any of them below! || ",
"hits": 151
},
{
"id": 2778,
"url": "https://svs.gsfc.nasa.gov/2778/",
"result_type": "Visualization",
"release_date": "2003-07-03T12:00:00-04:00",
"title": "Mars Odyssey: Mars' Northern Hemisphere",
"description": "NASA's Mars Odyssey detected water ice in the northern hemisphere. During the winter months, the icy soil is covered by a thick layer of carbon dioxide ('dry ice') frost obscuring the water ice signature. This animation is match-framed to animation 2779 and animation 2780. Its purpose is to establish a frame of reference using a true color data set. In this case, that data is from Viking. || ",
"hits": 37
},
{
"id": 2779,
"url": "https://svs.gsfc.nasa.gov/2779/",
"result_type": "Visualization",
"release_date": "2003-07-03T12:00:00-04:00",
"title": "Mars Odyssey: Water Ice/Winter Observations",
"description": "NASA's Mars Odyssey detected water ice in the northern hemisphere. During the winter months, the icy soil is covered by a thick layer of carbon dioxide ('dry ice') frost obscuring the water ice signature.This animation is match-framed to animation #2778 and animation #2780. It shows the areas of ice during a martian winter. || ",
"hits": 109
},
{
"id": 2780,
"url": "https://svs.gsfc.nasa.gov/2780/",
"result_type": "Visualization",
"release_date": "2003-07-03T12:00:00-04:00",
"title": "Mars Odyssey: Water Ice/Summer Observations",
"description": "NASA's Mars Odyssey detected water ice in the northern hemisphere. During the winter months, the icy soil is covered by a thick layer of carbon dioxide ('dry ice') frost obscuring the water ice signature.This animation is match-framed to #2778 and #2779. It shows the areas of ice during a martian summer. || ",
"hits": 45
},
{
"id": 2702,
"url": "https://svs.gsfc.nasa.gov/2702/",
"result_type": "Visualization",
"release_date": "2003-02-21T15:00:00-05:00",
"title": "Snow Covers Northeastern United States on February 20, 2003",
"description": "Snow cover left from a storm front that came through from February 16 to February 17, 2003. || ",
"hits": 15
},
{
"id": 2672,
"url": "https://svs.gsfc.nasa.gov/2672/",
"result_type": "Visualization",
"release_date": "2003-01-14T12:00:00-05:00",
"title": "Great Zoom into Boston, MA: Park Plaza Hotel",
"description": "Using data from different spacecraft and some powerful computer technology, visualizers at the Goddard Space Flight Center present you with a collection of American cities in a way you have never seen them before. Starting with our camera high above the Earth, we rush in towards the surface at what would be an impossible speed for any known vehicle. Passing though layers of atmosphere, the colors of our destinations shimmer with their own unique characteristics, and suddenly we find ourselves floating in virtual space just above the ground.This zoom was created to support a paper given at IEEE Vis 2002. || ",
"hits": 16
},
{
"id": 2673,
"url": "https://svs.gsfc.nasa.gov/2673/",
"result_type": "Visualization",
"release_date": "2003-01-14T12:00:00-05:00",
"title": "Great Zoom out from Boston, MA: Park Plaza Hotel",
"description": "Using data from different spacecraft and some powerful computer technology, visualizers at the Goddard Space Flight Center present you with a collection of American cities in a way you have never seen them before. Starting with our camera high above the Earth, we rush in towards the surface at what would be an impossible speed for any known vehicle. Passing though layers of atmosphere, the colors of our destinations shimmer with their own unique characteristics, and suddenly we find ourselves floating in virtual space just above the ground.This zoom was created to support a paper given at IEEE Vis 2002. || ",
"hits": 13
},
{
"id": 2324,
"url": "https://svs.gsfc.nasa.gov/2324/",
"result_type": "Visualization",
"release_date": "2001-12-11T12:00:00-05:00",
"title": "MOLA: Seasonal Snow Variations on Mars: Polar Images",
"description": "Print resolution still images in support of the MOLA: Seasonal Snow Variation story || The north pole of Mars shown colored by elevation || marsNPoleFalseCol.jpg (2730x2048) [791.2 KB] || marsNPoleFalseCola_web.png (320x240) [83.6 KB] || marsNPoleFalseCola_thm.png (80x40) [5.0 KB] || marsNPoleFalseCola_searchweb.png (320x180) [62.0 KB] || marsNPoleFalseCol.tif (2730x2048) [6.1 MB] || marsNPoleFalseCol.tif.hwshow [189 bytes] || ",
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{
"id": 2292,
"url": "https://svs.gsfc.nasa.gov/2292/",
"result_type": "Visualization",
"release_date": "2001-12-06T12:00:00-05:00",
"title": "MOLA: Seasonal Snow Variations on Mars, Zoom to Martian North Pole: True Color",
"description": "This is a visualization of the topography near the Martian north pole as measured with the MOLA instrument. This particular animation shows a short zoom to an overhead view of the rotating north pole in true color. || ",
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{
"id": 2293,
"url": "https://svs.gsfc.nasa.gov/2293/",
"result_type": "Visualization",
"release_date": "2001-12-06T12:00:00-05:00",
"title": "MOLA: Seasonal Snow Variations on Mars: Fast Zoom to Martian North Pole: False Color",
"description": "This is a visualization of the topography near the Martian north pole as measured with the MOLA instrument. This particular animation shows a fast zoom to the surface of the pole. The surface color is based on the elevation of the topography. || ",
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{
"id": 2294,
"url": "https://svs.gsfc.nasa.gov/2294/",
"result_type": "Visualization",
"release_date": "2001-12-06T12:00:00-05:00",
"title": "MOLA: Seasonal Snow Variations on Mars, Fast Zoom out from Martian South Pole: False Color",
"description": "This is a visualization of the topography near the Martian south pole as measured with the MOLA instrument. This particular animation shows a fast zoom out from the surface of the pole. The surface color is based on the elevation of the topography. || ",
"hits": 13
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{
"id": 2295,
"url": "https://svs.gsfc.nasa.gov/2295/",
"result_type": "Visualization",
"release_date": "2001-12-06T12:00:00-05:00",
"title": "MOLA: Seasonal Snow Variations on Mars: Medium Zoom to Martian North Pole: False Color",
"description": "This is a visualization of the topography near the Martian north pole as measured with the MOLA instrument. This particular animation shows a medium speed zoom to the surface of the pole. The surface color is based on the elevation of the topography. || ",
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{
"id": 2296,
"url": "https://svs.gsfc.nasa.gov/2296/",
"result_type": "Visualization",
"release_date": "2001-12-06T12:00:00-05:00",
"title": "MOLA: Seasonal Snow Variations on Mars, Medium Zoom out from Martian South Pole: False Color",
"description": "This is a visualization of the topography near the Martian south pole as measured with the MOLA instrument. This particular animation shows a medium zoom out from the surface of the pole. The surface color is based on the elevation of the topography. || ",
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{
"id": 2297,
"url": "https://svs.gsfc.nasa.gov/2297/",
"result_type": "Visualization",
"release_date": "2001-12-06T12:00:00-05:00",
"title": "MOLA: Seasonal Snow Variations on Mars: Slow Flyover of the Martian North Pole: False Color",
"description": "This is a visualization of the topography near the Martian north pole as measured with the MOLA instrument. This particular animation shows a slow zoom to the surface of the pole, a flyover of the polar cap and a slow zoom out. The surface color is based on the elevation of the topography. || ",
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{
"id": 2298,
"url": "https://svs.gsfc.nasa.gov/2298/",
"result_type": "Visualization",
"release_date": "2001-12-06T12:00:00-05:00",
"title": "MOLA: Seasonal Snow Variations on Mars: Slow Zoom out from the Martian North Pole: True Color",
"description": "This is a true color visualization of the topography near the Martian north pole as measured with the MOLA instrument. This particular animation shows a slow zoom out from the surface of the pole and is a frame-accurate match to the end of animation id #2297. || ",
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{
"id": 2299,
"url": "https://svs.gsfc.nasa.gov/2299/",
"result_type": "Visualization",
"release_date": "2001-12-06T12:00:00-05:00",
"title": "MOLA: Seasonal Snow Variations on Mars: Slow Flyover of the Martian South Pole: False Color",
"description": "This is a visualization of the topography near the Martian south pole as measured with the MOLA instrument. This particular animation shows a slow zoom to the surface of the pole, a flyover of the polar cap and a slow zoom out. The surface color is based on the elevation of the topography. || ",
"hits": 33
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{
"id": 2300,
"url": "https://svs.gsfc.nasa.gov/2300/",
"result_type": "Visualization",
"release_date": "2001-12-06T12:00:00-05:00",
"title": "MOLA: Seasonal Snow Variations on Mars: Slow Zoom to the Martian South Pole: True Color",
"description": "This is a true color visualization of the topography near the Martian south pole as measured with the MOLA instrument. This particular animation shows a slow zoom to the surface of the pole and is a frame-accurate match to the beginning ofanimation id #2299. || ",
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{
"id": 2301,
"url": "https://svs.gsfc.nasa.gov/2301/",
"result_type": "Visualization",
"release_date": "2001-12-06T12:00:00-05:00",
"title": "MOLA: Seasonal Snow Variations on Mars: Slow Zoom to the Martian North Pole: True Color",
"description": "This is a true color visualization of the topography near the Martian north pole as measured with the MOLA instrument. This particular animation shows a slow zoom to the surface of the pole and is a frame-accurate match to the beginning of animation id #2297. || ",
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{
"id": 2302,
"url": "https://svs.gsfc.nasa.gov/2302/",
"result_type": "Visualization",
"release_date": "2001-12-06T12:00:00-05:00",
"title": "MOLA: Seasonal Snow Variations on Mars: Slow Zoom Out from the Martian North Pole: True Color",
"description": "This is a true color visualization of the topography near the Martian north pole as measured with the MOLA instrument. This particular animation shows a slow zoom out from the surface of the pole and is a frame-accurate match to the end of animation id #2297. || ",
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{
"id": 2303,
"url": "https://svs.gsfc.nasa.gov/2303/",
"result_type": "Visualization",
"release_date": "2001-12-06T12:00:00-05:00",
"title": "MOLA: Seasonal Snow Variations on Mars: Flyover and Slow Zoom out from Martian S. Pole: True Color",
"description": "This is a true color visualization of the topography near the Martian south pole as measured with the MOLA instrument. This particular animation shows a flyover and slow zoom out from the surface of the pole and is a frame-accurate match to the end of animation id #2299. || ",
"hits": 18
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{
"id": 2306,
"url": "https://svs.gsfc.nasa.gov/2306/",
"result_type": "Visualization",
"release_date": "2001-12-06T12:00:00-05:00",
"title": "MOLA: Seasonal Snow Variations on Mars, Graph Showing Snow Variations at Both Poles, With Dates",
"description": "This is a visualization of a series of graphs showing the seasonal changes in the Martian polar caps. This particular version includes both poles and the Martian year timestamp. || Seasonal Mars snow variations graph (with dates) showing both poles || a002306.00100_print.png (720x480) [269.8 KB] || mola_graph_pre.jpg (320x240) [6.5 KB] || a002306.webmhd.webm (960x540) [2.8 MB] || a002306.dv (720x480) [142.8 MB] || a002306.mp4 (640x480) [8.1 MB] || mola_graph.mpg (320x240) [220.3 KB] || ",
"hits": 35
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{
"id": 2307,
"url": "https://svs.gsfc.nasa.gov/2307/",
"result_type": "Visualization",
"release_date": "2001-12-06T12:00:00-05:00",
"title": "MOLA: Seasonal Snow Variations on Mars, graph showing snow variations at both poles, without dates",
"description": "This is a visualization of a series of graphs showing the seasonal changes in the Martian polar caps. This particular version includes both poles and no Martian year timestamp. || ",
"hits": 18
},
{
"id": 2308,
"url": "https://svs.gsfc.nasa.gov/2308/",
"result_type": "Visualization",
"release_date": "2001-12-06T12:00:00-05:00",
"title": "MOLA: Seasonal Snow Variations on Mars, graph showing snow variations at north pole, with dates",
"description": "This is a visualization of a series of graphs showing the seasonal changes in the Martian polar caps. This particular version includes just the north pole and the Martian year timestamp. || ",
"hits": 25
},
{
"id": 2309,
"url": "https://svs.gsfc.nasa.gov/2309/",
"result_type": "Visualization",
"release_date": "2001-12-06T12:00:00-05:00",
"title": "MOLA: Seasonal Snow Variations on Mars, graph showing snow variations at north pole, without dates",
"description": "This is a visualization of a series of graphs showing the seasonal changes in the Martian polar caps. This particular version includes just the north pole without the Martian year timestamp. || ",
"hits": 14
},
{
"id": 2310,
"url": "https://svs.gsfc.nasa.gov/2310/",
"result_type": "Visualization",
"release_date": "2001-12-06T12:00:00-05:00",
"title": "MOLA: Seasonal Snow Variations on Mars, clouds at both poles, with dates, without contours",
"description": "This is a visualization of the clouds near the Marian polar caps measured using the MOLA instrument. This particular animation shows both poles, with dates, and without contours. || ",
"hits": 13
},
{
"id": 2311,
"url": "https://svs.gsfc.nasa.gov/2311/",
"result_type": "Visualization",
"release_date": "2001-12-06T12:00:00-05:00",
"title": "MOLA: Seasonal Snow Variations on Mars, clouds at both poles, with dates, with contours",
"description": "This is a visualization of the clouds near the Marian polar caps measured using the MOLA instrument. This particular animation shows both poles, with dates, and with contours. || ",
"hits": 23
},
{
"id": 2312,
"url": "https://svs.gsfc.nasa.gov/2312/",
"result_type": "Visualization",
"release_date": "2001-12-06T12:00:00-05:00",
"title": "MOLA: Seasonal Snow Variations on Mars, clouds at north pole, with dates, without contours",
"description": "This is a visualization of the clouds near the Marian polar caps measured using the MOLA instrument. This particular animation shows just the north pole, with dates, and without contours. || ",
"hits": 15
},
{
"id": 2313,
"url": "https://svs.gsfc.nasa.gov/2313/",
"result_type": "Visualization",
"release_date": "2001-12-06T12:00:00-05:00",
"title": "MOLA: Seasonal Snow Variations on Mars, Clouds at North Pole, With Dates and Contours",
"description": "This is a visualization of the clouds near the Marian polar caps measured using the MOLA instrument. This particular animation shows just the north pole, with dates, and with contours. || ",
"hits": 17
},
{
"id": 2326,
"url": "https://svs.gsfc.nasa.gov/2326/",
"result_type": "Visualization",
"release_date": "2001-12-01T12:00:00-05:00",
"title": "MOLA Stills for possible cover of 'Nature'",
"description": "These are draft renders of Mars using MOLA data for Topography and Viking data (true color) for the surface texture. One of these was picked and used by Nature on the cover of 'Insight' on 12 July 2001. The same image was used on the cover of the Planetary Report July/August 2001. || Mars MOLA true color image of Kasei Valles looking west to east (vertical exaggeration 3x, shading 6x) || mola_nature_3x6x0.2s.0001_tc.jpg (425x550) [24.7 KB] || ",
"hits": 16
},
{
"id": 2327,
"url": "https://svs.gsfc.nasa.gov/2327/",
"result_type": "Visualization",
"release_date": "2001-12-01T12:00:00-05:00",
"title": "MOLA Stills for possible cover of 'Science'",
"description": "These stills were generated as possible cover images for Science. Science did not select one of these - instead they selected a MOC image. || Mars MOLA true color image of the north pole || science2_fixed_true.0000.jpg (425x550) [27.3 KB] || Mars MOLA false color image of the north and south poles || science.0000_false_northAndSouth.jpg (425x550) [31.4 KB] || Mars MOLA false color image of the north pole || science.0007_false.jpg (425x550) [24.2 KB] || ",
"hits": 21
},
{
"id": 2189,
"url": "https://svs.gsfc.nasa.gov/2189/",
"result_type": "Visualization",
"release_date": "2001-06-15T12:00:00-04:00",
"title": "Great Zoom into Cambridge, MA: Massachusetts Institute of Technology Kresge Auditorium",
"description": "Using data from different spacecraft and some powerful computer technology, visualizers at the Goddard Space Flight Center present you with a collection of American cities in a way you have never seen them before. Starting with our camera high above the Earth, we rush in towards the surface at what would be an impossible speed for any known vehicle. Passing though layers of atmosphere, the colors of our destinations shimmer with their own unique characteristics, and suddenly we find ourselves floating in virtual space just above the ground. || ",
"hits": 8
},
{
"id": 2190,
"url": "https://svs.gsfc.nasa.gov/2190/",
"result_type": "Visualization",
"release_date": "2001-06-15T12:00:00-04:00",
"title": "Great Zoom out of Cambridge, MA: Massachusetts Institute of Technology Kresge Auditorium",
"description": "Using data from different spacecraft and some powerful computer technology, visualizers at the Goddard Space Flight Center present you with a collection of American cities in a way you have never seen them before. Starting with our camera high above the Earth, we rush in towards the surface at what would be an impossible speed for any known vehicle. Passing though layers of atmosphere, the colors of our destinations shimmer with their own unique characteristics, and suddenly we find ourselves floating in virtual space just above the ground. || ",
"hits": 19
},
{
"id": 2121,
"url": "https://svs.gsfc.nasa.gov/2121/",
"result_type": "Visualization",
"release_date": "2001-04-13T12:00:00-04:00",
"title": "Great Zoom into Boston, MA: The Bunker Hill Monument",
"description": "Using data from different spacecraft and some powerful computer technology, visualizers at the Goddard Space Flight Center present you with a collection of American cities in a way you have never seen them before. Starting with our camera high above the Earth, we rush in towards the surface at what would be an impossible speed for any known vehicle. Passing though layers of atmosphere, the colors of our destinations shimmer with their own unique characteristics, and suddenly we find ourselves floating in virtual space just above the ground. || ",
"hits": 25
},
{
"id": 2130,
"url": "https://svs.gsfc.nasa.gov/2130/",
"result_type": "Visualization",
"release_date": "2001-04-13T12:00:00-04:00",
"title": "Great Zoom out of Boston, MA: The Bunker Hill Monument",
"description": "Using data from different spacecraft and some powerful computer technology, visualizers at the Goddard Space Flight Center present you with a collection of American cities in a way you have never seen them before. Starting with our camera high above the Earth, we rush in towards the surface at what would be an impossible speed for any known vehicle. Passing though layers of atmosphere, the colors of our destinations shimmer with their own unique characteristics, and suddenly we find ourselves floating in virtual space just above the ground. || ",
"hits": 21
},
{
"id": 2060,
"url": "https://svs.gsfc.nasa.gov/2060/",
"result_type": "Visualization",
"release_date": "2001-01-29T12:00:00-05:00",
"title": "NEAR Views the Asteroid Eros (Gravity Slope)",
"description": "Views of the asteroid Eros generated by data from the laser rangefinder. This false color image shows the 'gravity slope' at various regions on the object. The gravity slope is the angle between the local gravitation field (computed assuming a constant density for the asteroid) and the normal to the surface. Blue is low slope, red is high slope. || ",
"hits": 29
},
{
"id": 2061,
"url": "https://svs.gsfc.nasa.gov/2061/",
"result_type": "Visualization",
"release_date": "2001-01-29T12:00:00-05:00",
"title": "NEAR Views the Asteroid Eros ('True' Color)",
"description": "Views of the asteroid Eros generated by data from the laser rangefinder. The 3-D model was generated from laser rangefinder data and the color was applied based on color images. || ",
"hits": 85
},
{
"id": 1335,
"url": "https://svs.gsfc.nasa.gov/1335/",
"result_type": "Visualization",
"release_date": "2000-12-31T12:00:00-05:00",
"title": "Mars Flyover Based on MOLA Data for the Carl Sagan Lecture",
"description": "This visualization of the topography of Mars was created for Maria Zuber's Carl Sagan Lecture. The camera flies over several areas of interest. The south pole, Tharsis Rise, the north pole, and Valles Marineris. This animation was created using Maya and Renderman, using MOLA Topography data. The colors represent height - dark blue is about 8km deep and white is over 14km high (as measured from an arbitrary location picked as 'sea-level'). || ",
"hits": 48
},
{
"id": 1213,
"url": "https://svs.gsfc.nasa.gov/1213/",
"result_type": "Visualization",
"release_date": "2000-06-14T12:00:00-04:00",
"title": "Cape Cod",
"description": "Zoom into and pan around Cape Cod, Massachusetts. || a001213.00010_print.png (720x480) [703.4 KB] || a001213_pre.jpg (320x242) [16.0 KB] || a001213_thm.png (80x40) [6.8 KB] || a001213_pre_searchweb.jpg (320x180) [91.1 KB] || a001213.webmhd.webm (960x540) [18.5 MB] || a001213.dv (720x480) [492.0 MB] || a001213.mp4 (640x480) [26.5 MB] || a001213.mpg (352x240) [19.7 MB] || Video slate image reads, \"Cape Cod\". || a001213_slate.jpg (720x528) [28.8 KB] || a001213_slate_web.png (320x234) [16.5 KB] || ",
"hits": 16
},
{
"id": 968,
"url": "https://svs.gsfc.nasa.gov/968/",
"result_type": "Visualization",
"release_date": "1999-08-14T12:00:00-04:00",
"title": "Cape Cod Flyby",
"description": "This animation of Cape Cod, Massachusetts, was done as part of a series of animations showing Landsat's view of our National Parks. || ",
"hits": 50
},
{
"id": 647,
"url": "https://svs.gsfc.nasa.gov/647/",
"result_type": "Visualization",
"release_date": "1999-05-24T12:00:00-04:00",
"title": "Onion Skin of Un-named Martian Crater",
"description": "Onion skin of Martian crater || a000647.00005_print.png (720x480) [352.1 KB] || a000647_pre.jpg (320x242) [9.5 KB] || a000647.webmhd.webm (960x540) [1.9 MB] || a000647.mp4 (640x480) [5.0 MB] || a000647.dv (720x480) [92.6 MB] || a000647.mpg (352x240) [3.4 MB] || Seepage regions in an un-named Martian crater (draft render) || seepage.jpg (720x486) [102.5 KB] || seepage_web.jpg (320x216) [5.7 KB] || seepage_thm.png (80x40) [3.8 KB] || seepage_web_searchweb.jpg (320x180) [29.6 KB] || ",
"hits": 51
},
{
"id": 648,
"url": "https://svs.gsfc.nasa.gov/648/",
"result_type": "Visualization",
"release_date": "1999-05-24T12:00:00-04:00",
"title": "Polar Lander Landing Site (Curved Box) (False Color)",
"description": "Flyover of Mars Polar Lander landing site with false color texture || a000648.00010_print.png (720x480) [497.8 KB] || a000648_thm.png (80x40) [4.1 KB] || a000648_pre.jpg (320x238) [7.6 KB] || a000648_pre_searchweb.jpg (320x180) [59.1 KB] || a000648.webmhd.webm (960x540) [2.7 MB] || a000648.dv (720x480) [51.5 MB] || a000648.mp4 (640x480) [2.9 MB] || a000648.mpg (352x240) [1.7 MB] || ",
"hits": 47
},
{
"id": 649,
"url": "https://svs.gsfc.nasa.gov/649/",
"result_type": "Visualization",
"release_date": "1999-05-24T12:00:00-04:00",
"title": "Polar Lander Landing Site (Rect. Box) (False Color)",
"description": "Mars global topography view rotating and zooming into Polar Lander landing site || a000649.00010_print.png (720x480) [495.3 KB] || a000649_thm.png (80x40) [4.1 KB] || a000649_pre.jpg (320x238) [7.6 KB] || a000649_pre_searchweb.jpg (320x180) [58.6 KB] || a000649.webmhd.webm (960x540) [2.9 MB] || a000649.dv (720x480) [54.9 MB] || a000649.mp4 (640x480) [3.0 MB] || a000649.mpg (352x240) [1.8 MB] || ",
"hits": 47
},
{
"id": 650,
"url": "https://svs.gsfc.nasa.gov/650/",
"result_type": "Visualization",
"release_date": "1999-05-24T12:00:00-04:00",
"title": "Viewing North and South Poles of Mars (False Color)",
"description": "Mars topography globe flyover of polar regions using false color texture || a000650.00010_print.png (720x480) [490.2 KB] || a000650_thm.png (80x40) [4.2 KB] || a000650_pre.jpg (320x238) [7.8 KB] || a000650_pre_searchweb.jpg (320x180) [59.8 KB] || a000650.webmhd.webm (960x540) [11.4 MB] || a000650.dv (720x480) [226.5 MB] || a000650.mp4 (640x480) [12.2 MB] || a000650.mpg (352x240) [8.8 MB] || ",
"hits": 70
},
{
"id": 651,
"url": "https://svs.gsfc.nasa.gov/651/",
"result_type": "Visualization",
"release_date": "1999-05-24T12:00:00-04:00",
"title": "MOLA-based Flyover of Valles Marineris (False Color)",
"description": "Flyover of Valles Marineris on Mars topography globe with false color texture || a000651.00010_print.png (720x480) [531.7 KB] || a000651_thm.png (80x40) [4.1 KB] || a000651_pre.jpg (320x242) [8.0 KB] || a000651_pre_searchweb.jpg (320x180) [58.3 KB] || a000651.webmhd.webm (960x540) [6.5 MB] || a000651.m2v (720x480) [31.1 MB] || a000651.dv (720x480) [145.6 MB] || a000651.mp4 (640x480) [7.4 MB] || a000651.mpg (352x240) [5.4 MB] || ",
"hits": 22
},
{
"id": 652,
"url": "https://svs.gsfc.nasa.gov/652/",
"result_type": "Visualization",
"release_date": "1999-05-24T12:00:00-04:00",
"title": "Flyover of Mars' Valles Marineris (True Color)",
"description": "The height is based on MOLA data. || Flyover of Valles Marineris on Mars topography globe with true color texture || a000652.00010_print.png (720x480) [434.2 KB] || a000652_thm.png (80x40) [3.7 KB] || a000652_pre.jpg (320x242) [6.7 KB] || a000652_pre_searchweb.jpg (320x180) [50.2 KB] || a000652.webmhd.webm (960x540) [4.8 MB] || a000652.dv (720x480) [144.2 MB] || a000652.mp4 (640x480) [7.8 MB] || a000652.mpg (352x240) [5.4 MB] || ",
"hits": 102
},
{
"id": 653,
"url": "https://svs.gsfc.nasa.gov/653/",
"result_type": "Visualization",
"release_date": "1999-05-24T12:00:00-04:00",
"title": "Mars Hellas Crater - Flat Spin (False Color)",
"description": "Hellas Crater Flat Spin (False Color) || Mars flat topographic map flyover and spin over Hellas Crater with false color texture || a000653.00010_print.png (720x480) [576.8 KB] || a000653_thm.png (80x40) [6.7 KB] || a000653_pre.jpg (320x242) [12.4 KB] || a000653_pre_searchweb.jpg (320x180) [92.9 KB] || a000653.webmhd.webm (960x540) [14.0 MB] || a000653.dv (720x480) [192.3 MB] || a000653.mp4 (640x480) [10.7 MB] || a000653.mpg (352x240) [7.1 MB] || ",
"hits": 50
},
{
"id": 654,
"url": "https://svs.gsfc.nasa.gov/654/",
"result_type": "Visualization",
"release_date": "1999-05-24T12:00:00-04:00",
"title": "Tharsis Rise (True Color)",
"description": "Flyover of Mars topography globe in Tharsis region with true color texture || a000654.00010_print.png (720x480) [453.9 KB] || a000654_thm.png (80x40) [3.7 KB] || a000654_pre.jpg (320x238) [6.5 KB] || a000654_pre_searchweb.jpg (320x180) [51.1 KB] || a000654.webmhd.webm (960x540) [12.4 MB] || a000654.dv (720x480) [192.3 MB] || a000654.mp4 (640x480) [10.3 MB] || a000654.mpg (352x240) [7.2 MB] || ",
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{
"id": 655,
"url": "https://svs.gsfc.nasa.gov/655/",
"result_type": "Visualization",
"release_date": "1999-05-24T12:00:00-04:00",
"title": "Tharsis Rise (False Color)",
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"hits": 50
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{
"id": 656,
"url": "https://svs.gsfc.nasa.gov/656/",
"result_type": "Visualization",
"release_date": "1999-05-24T12:00:00-04:00",
"title": "Mars Topography: Downhill Showing a Gradient Slope (False Color)",
"description": "Flat map of Mars topography tipped on its side to show cross section sloping downhill from South to North || a000656.00010_print.png (720x480) [550.4 KB] || a000656_thm.png (80x40) [6.3 KB] || a000656_pre.jpg (320x238) [9.9 KB] || a000656_pre_searchweb.jpg (320x180) [77.1 KB] || a000656.webmhd.webm (960x540) [3.3 MB] || a000656.m2v (720x480) [19.2 MB] || a000656.dv (720x480) [89.4 MB] || a000656.mp4 (640x480) [4.4 MB] || a000656.mpg (352x240) [2.6 MB] || ",
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{
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"url": "https://svs.gsfc.nasa.gov/657/",
"result_type": "Visualization",
"release_date": "1999-05-24T12:00:00-04:00",
"title": "Mars Hellas Crater Flat Flyover (False Color)",
"description": "Based on MOLA data. || Flyover flat map of Mars topography of Hellas Crater with false color texture || a000657.00010_print.png (720x480) [540.8 KB] || a000657_thm.png (80x40) [6.2 KB] || a000657_pre.jpg (320x238) [9.9 KB] || a000657_pre_searchweb.jpg (320x180) [79.9 KB] || a000657.webmhd.webm (960x540) [5.8 MB] || a000657.dv (720x480) [121.3 MB] || a000657.mp4 (640x480) [6.6 MB] || a000657.mpg (352x240) [4.4 MB] || ",
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{
"id": 658,
"url": "https://svs.gsfc.nasa.gov/658/",
"result_type": "Visualization",
"release_date": "1999-05-24T12:00:00-04:00",
"title": "Hellas Crater Flat Flyover (True Color)",
"description": "Flyover flat map of Mars topography of Hellas Crater with true color texture || a000658.00010_print.png (720x480) [448.5 KB] || a000658_thm.png (80x40) [5.2 KB] || a000658_pre.jpg (320x238) [8.5 KB] || a000658_pre_searchweb.jpg (320x180) [69.6 KB] || a000658.webmhd.webm (960x540) [4.2 MB] || a000658.dv (720x480) [121.3 MB] || a000658.mp4 (640x480) [6.7 MB] || a000658.mpg (352x240) [4.3 MB] || ",
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{
"id": 659,
"url": "https://svs.gsfc.nasa.gov/659/",
"result_type": "Visualization",
"release_date": "1999-05-24T12:00:00-04:00",
"title": "Mars Rotate (True Color)",
"description": "Rotating Mars with MOLAi topography and a true color Viking texure || a000659.00010_print.png (720x480) [422.9 KB] || a000659_thm.png (80x40) [3.5 KB] || a000659_pre.jpg (320x238) [5.7 KB] || a000659_pre_searchweb.jpg (320x180) [44.7 KB] || a000659.webmhd.webm (960x540) [6.5 MB] || a000659.dv (720x480) [233.3 MB] || a000659.mp4 (640x480) [12.8 MB] || a000659.mpg (352x240) [8.8 MB] || ",
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{
"id": 660,
"url": "https://svs.gsfc.nasa.gov/660/",
"result_type": "Visualization",
"release_date": "1999-05-24T12:00:00-04:00",
"title": "Mars Rotate (False Color)",
"description": "Rotating Mars with false color MOLA topography || a000660.00010_print.png (720x480) [507.8 KB] || a000660_thm.png (80x40) [4.3 KB] || a000660_pre.jpg (320x238) [8.5 KB] || a000660_pre_searchweb.jpg (320x180) [63.1 KB] || a000660.webmhd.webm (960x540) [16.3 MB] || a000660.dv (720x480) [223.6 MB] || a000660.mp4 (640x480) [11.8 MB] || a000660.mpg (352x240) [8.6 MB] || ",
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{
"id": 661,
"url": "https://svs.gsfc.nasa.gov/661/",
"result_type": "Visualization",
"release_date": "1999-05-24T12:00:00-04:00",
"title": "Rotating around the Tharsis Rise (True Color)",
"description": "Push in and spin around Tharsis rise on a flat map of Mars MOLA topography with Viking true color || a000661.00010_print.png (720x480) [449.7 KB] || a000661_thm.png (80x40) [5.2 KB] || a000661_pre.jpg (320x238) [8.6 KB] || a000661_pre_searchweb.jpg (320x180) [70.6 KB] || a000661.webmhd.webm (960x540) [11.8 MB] || a000661.dv (720x480) [192.3 MB] || a000661.mp4 (640x480) [10.6 MB] || a000661.mpg (352x240) [7.3 MB] || ",
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},
{
"id": 662,
"url": "https://svs.gsfc.nasa.gov/662/",
"result_type": "Visualization",
"release_date": "1999-05-24T12:00:00-04:00",
"title": "Rotating Around the Tharsis Rise (False Color)",
"description": "Push in and spin around Tharsis rise on a flat map of Mars MOLA topography with false color || a000662.00010_print.png (720x480) [537.4 KB] || a000662_thm.png (80x40) [6.4 KB] || a000662_pre.jpg (320x240) [11.0 KB] || a000662_pre_searchweb.jpg (320x180) [86.5 KB] || a000662.webmhd.webm (960x540) [13.7 MB] || a000662.dv (720x480) [192.1 MB] || a000662.mp4 (640x480) [10.6 MB] || a000662.mpg (352x240) [7.6 MB] || ",
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},
{
"id": 848,
"url": "https://svs.gsfc.nasa.gov/848/",
"result_type": "Visualization",
"release_date": "1999-04-09T12:00:00-04:00",
"title": "Boston Flyby",
"description": "This scene shows Landsat Thematic Mapper data from the shortwave infrared (TM band 5), infrared (TM band 4), and visible green (TM band 2) channels of Boston. Logan Airport is visible in the foreground, while high resolution images show the highway network running around the city. || ",
"hits": 51
},
{
"id": 404,
"url": "https://svs.gsfc.nasa.gov/404/",
"result_type": "Visualization",
"release_date": "1998-11-30T12:00:00-05:00",
"title": "Zoom Down to Boston and Nantucket Shoals - October 6th 1997",
"description": "A zoom down to Boston and the Nantucket Shoals, from SeaWiFS imagery || a000404.00095_print.png (720x480) [716.5 KB] || a000404_thm.png (80x40) [7.8 KB] || a000404_pre.jpg (320x238) [16.7 KB] || a000404_pre_searchweb.jpg (320x180) [95.6 KB] || a000404.webmhd.webm (960x540) [3.0 MB] || a000404.dv (720x480) [43.4 MB] || a000404.mp4 (640x480) [2.5 MB] || a000404.mpg (352x240) [1.1 MB] || ",
"hits": 39
},
{
"id": 97,
"url": "https://svs.gsfc.nasa.gov/97/",
"result_type": "Visualization",
"release_date": "1996-02-08T12:00:00-05:00",
"title": "Images of Earth and Space: The Role of Visualization in NASA Science",
"description": "This compilation video contains visualizations of Earth and Space Sciences resulting from supercomputer models. The excerpted visualizations include: Ocean Planet, El Niño, Ozone 1991, Clouds, Changes in Glacier Bay, Alaska, Biosphere, Lunar Topography from the Clementine Mission, Musculoskeletal Modeling Dynamic Simulations, Simulations of the Breakup and Dynamical Evolution of Comet Shoemaker-Levy 9, Convective Penetration in Stellar Interiors, Topological Features of a Compressible Plasma Vortex Sheet: A Model for the Outer Heliospheric Solar Wind, R-Aquarii Jet, The Evolution of Distorted Black Holes, Rayleigh-Taylor Instability in a Supernova, Galaxy Harassment, N-Body Simulation of the Cold Dark Matter Cosmology. || ",
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},
{
"id": 79,
"url": "https://svs.gsfc.nasa.gov/79/",
"result_type": "Visualization",
"release_date": "1995-06-09T12:00:00-04:00",
"title": "Lunar Rotation and Flyby from Clementine Data (with route map)",
"description": "Clementine was a joint project between the Strategic Defense Initiative Organization and NASA. The objective of the mission was to test sensors and spacecraft components under extended exposure to the space environment and to make scientific observations of the Moon and the near-Earth asteroid 1620 Geographos. Clementine was launched on 25 January 1994 at 16:34 UTC (12:34 PM EDT) from Vandenberg AFB aboard a Titan II G rocket. After two Earth flybys, lunar insertion was achieved on February 21. Lunar mapping took place over approximately two months, in two parts. The first part consisted of a 5 hour elliptical polar orbit with a perilune of about 400 km at 28 degrees S latitude. After one month of mapping the orbit was rotated to a perilune of 29 degrees N latitude, where it remained for one more month. This allowed global imaging as well as altimetry coverage from 60 degrees S to 60 degrees N. || ",
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}
]
}