{ "id": 4742, "url": "https://svs.gsfc.nasa.gov/4742/", "page_type": "Visualization", "title": "SVS Demo Reel", "description": "This is the SVS Demo Reel presented at SIGGRAPH 2019 in Los Angeles, CA. || svs_siggraphreel2019_print.jpg (1920x1080) [319.8 KB] || svs_siggraphreel2019_print_searchweb.png (320x180) [36.2 KB] || svs_siggraphreel2019_print_thm.png (80x40) [3.3 KB] || svs_siggraphreel2019.mp4 (1920x1080) [298.4 MB] || svs_siggraphreel2019.webm (1920x1080) [18.6 MB] || svs_siggraphreel2019.en_US.srt [38 bytes] || svs_siggraphreel2019.en_US.vtt [51 bytes] || ", "release_date": "2019-07-25T15:00:00-04:00", "update_date": "2023-05-03T13:45:46.534851-04:00", "main_image": { "id": 394300, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004700/a004742/svs_siggraphreel2019_print.jpg", "filename": "svs_siggraphreel2019_print.jpg", "media_type": "Image", "alt_text": "This is the SVS Demo Reel presented at SIGGRAPH 2019 in Los Angeles, CA.", "width": 1920, "height": 1080, "pixels": 2073600 }, "main_video": { "id": 394299, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004700/a004742/svs_siggraphreel2019.mp4", "filename": "svs_siggraphreel2019.mp4", "media_type": "Movie", "alt_text": "This is the SVS Demo Reel presented at SIGGRAPH 2019 in Los Angeles, CA.", "width": 1920, "height": 1080, "pixels": 2073600 }, "progress": "Complete", "media_groups": [ { "id": 323110, "url": "https://svs.gsfc.nasa.gov/4742/#media_group_323110", "widget": "Video player", "title": "", "caption": "", "description": "This is the SVS Demo Reel presented at SIGGRAPH 2019 in Los Angeles, CA.", "items": [ { "id": 237950, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 394300, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004700/a004742/svs_siggraphreel2019_print.jpg", "filename": "svs_siggraphreel2019_print.jpg", "media_type": "Image", "alt_text": "This is the SVS Demo Reel presented at SIGGRAPH 2019 in Los Angeles, CA.", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 237951, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 394301, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004700/a004742/svs_siggraphreel2019_print_searchweb.png", "filename": "svs_siggraphreel2019_print_searchweb.png", "media_type": "Image", "alt_text": "This is the SVS Demo Reel presented at SIGGRAPH 2019 in Los Angeles, CA.", "width": 320, "height": 180, "pixels": 57600 } }, { "id": 237952, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 394302, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004700/a004742/svs_siggraphreel2019_print_thm.png", "filename": "svs_siggraphreel2019_print_thm.png", "media_type": "Image", "alt_text": "This is the SVS Demo Reel presented at SIGGRAPH 2019 in Los Angeles, CA.", "width": 80, "height": 40, "pixels": 3200 } }, { "id": 237949, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 394299, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004700/a004742/svs_siggraphreel2019.mp4", "filename": "svs_siggraphreel2019.mp4", "media_type": "Movie", "alt_text": "This is the SVS Demo Reel presented at SIGGRAPH 2019 in Los Angeles, CA.", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 237953, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 394303, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004700/a004742/svs_siggraphreel2019.webm", "filename": "svs_siggraphreel2019.webm", "media_type": "Movie", "alt_text": "This is the SVS Demo Reel presented at SIGGRAPH 2019 in Los Angeles, CA.", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 237954, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 850191, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004700/a004742/svs_siggraphreel2019.en_US.srt", "filename": "svs_siggraphreel2019.en_US.srt", "media_type": "Captions", "alt_text": "This is the SVS Demo Reel presented at SIGGRAPH 2019 in Los Angeles, CA.", "label": "English", "language_code": "" } }, { "id": 237955, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 850192, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004700/a004742/svs_siggraphreel2019.en_US.vtt", "filename": "svs_siggraphreel2019.en_US.vtt", "media_type": "Captions", "alt_text": "This is the SVS Demo Reel presented at SIGGRAPH 2019 in Los Angeles, CA.", "label": "English", "language_code": "" } } ], "extra_data": {} } ], "studio": "SVS", "funding_sources": [ "ESE" ], "credits": [ { "role": "Producer", "people": [ { "name": "Devika Elakara", "employer": "GSFC Interns" } ] }, { "role": "Visualizer", "people": [ { "name": "Lori Perkins", "employer": "NASA/GSFC" }, { "name": "Greg Shirah", "employer": "NASA/GSFC" }, { "name": "Alex Kekesi", "employer": "Global Science and Technology, Inc." }, { "name": "Ernie Wright", "employer": "USRA" }, { "name": "Trent L. Schindler", "employer": "USRA" }, { "name": "Helen-Nicole Kostis", "employer": "USRA" }, { "name": "Cindy Starr", "employer": "Global Science and Technology, Inc." }, { "name": "Kel Elkins", "employer": "USRA" }, { "name": "Horace Mitchell", "employer": "NASA/GSFC" }, { "name": "Tom Bridgman", "employer": "Global Science and Technology, Inc." } ] }, { "role": "Technical support", "people": [ { "name": "Leann Johnson", "employer": "Global Science and Technology, Inc." } ] } ], "missions": [], "series": [], "tapes": [], "papers": [], "datasets": [], "nasa_science_categories": [ "Earth", "Planets & Moons", "Sun", "Universe" ], "keywords": [ "SIGGRAPH", "Sizzle Reel" ], "recommended_pages": [], "related": [ { "id": 13814, "url": "https://svs.gsfc.nasa.gov/13814/", "page_type": "Produced Video", "title": "SVS Demo Reel 2020", "description": "This is the SVS Demo Reel submitted to SIGGRAPH 2021.Coming soon to our YouTube channel. || SVS_2020.File.1080p.00250_print.jpg (1024x576) [129.8 KB] || SVS_2020.File.1080p.00250_thm.png (80x40) [3.1 KB] || SVS_2020.File.1080p.00250_searchweb.png (320x180) [60.0 KB] || SVS_2020.File.1080p.mp4 (1920x1080) [367.7 MB] || captions_silent.30842.en_US.srt [42 bytes] || SVS_2020.File.720p.mp4 (720x404) [62.6 MB] || SVS_2020.file.2160pp.mp4 (3840x2160) [1.4 GB] || SVS_2020.file.2160pp.webm (3840x2160) [78.3 MB] || ", "release_date": "2021-02-18T00:00:00-05:00", "update_date": "2023-05-03T13:44:20.561761-04:00", "main_image": { "id": 379755, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a013800/a013814/SVS_2020.File.1080p.00250_print.jpg", "filename": "SVS_2020.File.1080p.00250_print.jpg", "media_type": "Image", "alt_text": "This is the SVS Demo Reel submitted to SIGGRAPH 2021.Coming soon to our YouTube channel.", "width": 1024, "height": 576, "pixels": 589824 } } ], "sources": [ { "id": 4905, "url": "https://svs.gsfc.nasa.gov/4905/", "page_type": "Animation", "title": "A Web Around Asteroid Bennu – Visualizations", "description": "This visualization depicts the OSIRIS-REx spacecraft’s trajectory around the asteroid Bennu from the initial arrival in Dec 2018 through the final departure in April 2021. The trajectory is presented in a Sun Bennu North reference frame. Several mission segments are highlighted in white, leading up to the TAG sample collection maneuver on Oct 20, 2020. || web_around_bennu-orbits_bennu_stars.15100_print.jpg (1024x576) [105.4 KB] || web_around_bennu-orbits_bennu_stars.15100_searchweb.png (320x180) [55.9 KB] || web_around_bennu-orbits_bennu_stars.15100_thm.png (80x40) [3.5 KB] || web_around_bennu-orbits_bennu_stars (3840x2160) [1.0 MB] || web_around_bennu-orbits_bennu_stars_2160p60.mp4 (3840x2160) [759.1 MB] || web_around_bennu-orbits_bennu_stars_2160p60.webm (3840x2160) [133.2 MB] || ", "release_date": "2021-05-10T16:00:00-04:00", "update_date": "2024-04-24T00:16:13.181649-04:00", "main_image": { "id": 419630, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004900/a004905/web_around_bennu-orbits_bennu_stars.15100_print.jpg", "filename": "web_around_bennu-orbits_bennu_stars.15100_print.jpg", "media_type": "Image", "alt_text": "This visualization depicts the OSIRIS-REx spacecraft’s trajectory around the asteroid Bennu from the initial arrival in Dec 2018 through the final departure in April 2021. The trajectory is presented in a Sun Bennu North reference frame. Several mission segments are highlighted in white, leading up to the TAG sample collection maneuver on Oct 20, 2020. ", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 4722, "url": "https://svs.gsfc.nasa.gov/4722/", "page_type": "Visualization", "title": "Jakobshavn Regional View of Three Simulated Greenland Ice Sheet Response Scenarios: 2008 - 2300", "description": "The Greenland Ice Sheet holds enough water to raise the world’s sea level by over 7 meters (23 feet). Rising atmosphere and ocean temperatures have led to an ice loss equivalent to over a centimeter increase in global mean sea-level between 1991 and 2015. Large outlet glaciers, rivers of ice moving to the sea, drain the ice from the interior of Greenland and cause the outer margins of the ice sheet to recede. Improvements in measuring the ice thickness in ice sheets is enabling better simulation of the flow in outlet glaciers, which is key to predicting the retreat of ice sheets into the future.Recently, a simulation of the effects of outlet glacier flow on ice sheet thickness coupled with improved data and comprehensive climate modeling for differing future climate scenarios has been used to estimate Greenland’s contribution to sea-level over the next millennium. Greenland could contribute 5–34 cm (2-13 inches) to sea-level by 2100 and 11–162 cm (4-64 inches) by 2200, with outlet glaciers contributing 19–40 % of the total mass loss. The analysis shows that uncertainties in projecting mass loss are dominated by uncertainties in climate scenarios and surface processes, followed by ice dynamics. Uncertainties in ocean conditions play a minor role, particularly in the long term. Greenland will very likely become ice-free within a millennium without significant reductions in greenhouse gas emissions.Three visualizations of the evolution of the Jakobshavn region of the Greenland Ice Sheet between 2008 and 2300 based on three different climate scenarios are shown below. Each scenario is described briefly in the caption under each visualization. Each of the three visualizations are provided with a date, colorbar and a distance scale as well as without. The regions shown in a violet color are exposed areas of the Greenland bed that were covered by the ice sheet in 2008.The data sets used for these animations are the control (“CTRL”) simulations and were produced with the open-source Parallel Ice Sheet Model (www.pism-docs.org). All data sets for this study are publicly available at https://arcticdata.io (doi:10.18739/A2Z60C21V). || ", "release_date": "2019-06-19T14:00:00-04:00", "update_date": "2024-05-17T00:13:16.489416-04:00", "main_image": { "id": 395093, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004700/a004722/Jakobshavn_RCP_26_2008_2300_comp.0282_print.jpg", "filename": "Jakobshavn_RCP_26_2008_2300_comp.0282_print.jpg", "media_type": "Image", "alt_text": "Above is a visualization of the Jakobshavn region of the Greenland Ice Sheet from 2008 to 2300 based on the Representative Concentration Pathway (RCP) 2.6 climate scenario. This is the best case scenario for limiting greenhouse gasses and assumes that emissions will peak by mid-century and decline thereafter.This video is also available on our YouTube channel.", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 4697, "url": "https://svs.gsfc.nasa.gov/4697/", "page_type": "Visualization", "title": "ENSO teleconnections in South East Asia for the period of 2015-2016", "description": "The 2015-2016 strong El Niño event brought changes to weather conditions across the globe that triggered regional infectious disease outbreaks, including mosquito-borne dengue fever in South East Asia. This visualization with corresponding multi-plot graph shows how Sea Surface Temperature anomalies in the equatorial Pacific Ocean (left), resulted in anomalous drought conditions (center) and increase in land surface temperatures (right) in South East Asia. During the 2015-2016 El Niño event, the South East Asia region received below than normal precipitation resulting in drier and warner than normal conditions, which increased the populations of mosquito vectors in urban areas, where there are open water storage containers providing ideal habitats for mosquito production. In addition, the higher than normal temperature on land shortens the maturation time of larvae to adult mosquitos and induces frequent blood feeding/biting of humans by mosquito vectors resulting in the amplification of dengue disease outbreaks over the South East Asia region. || SST_LST_Precip_2014_2016_Comp_print.jpg (1024x576) [82.9 KB] || SST_LST_Precip_2014_2016_Comp_searchweb.png (320x180) [51.5 KB] || SST_LST_Precip_2014_2016_Comp_thm.png (80x40) [6.0 KB] || frames/1920x1080_16x9_30p/SST_Precip_LST_Plot_Composite/ (1920x1080) [128.0 KB] || SST_LST_Precip_2014_2016_Comp_1080p30.mp4 (1920x1080) [9.7 MB] || SST_LST_Precip_2014_2016_Comp.tif (1920x1080) [1.1 MB] || SST_LST_Precip_2014_2016_Comp_1080p30.webm (1920x1080) [4.2 MB] || frames/3840x2160_16x9_30p/TeleconnectionsSEAsia/ (3840x2160) [128.0 KB] || ", "release_date": "2019-02-28T09:00:00-05:00", "update_date": "2023-11-15T00:12:33.075123-05:00", "main_image": { "id": 398276, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004600/a004697/SST_LST_Precip_2014_2016_Comp_print.jpg", "filename": "SST_LST_Precip_2014_2016_Comp_print.jpg", "media_type": "Image", "alt_text": "The 2015-2016 strong El Niño event brought changes to weather conditions across the globe that triggered regional infectious disease outbreaks, including mosquito-borne dengue fever in South East Asia. This visualization with corresponding multi-plot graph shows how Sea Surface Temperature anomalies in the equatorial Pacific Ocean (left), resulted in anomalous drought conditions (center) and increase in land surface temperatures (right) in South East Asia. During the 2015-2016 El Niño event, the South East Asia region received below than normal precipitation resulting in drier and warner than normal conditions, which increased the populations of mosquito vectors in urban areas, where there are open water storage containers providing ideal habitats for mosquito production. In addition, the higher than normal temperature on land shortens the maturation time of larvae to adult mosquitos and induces frequent blood feeding/biting of humans by mosquito vectors resulting in the amplification of dengue disease outbreaks over the South East Asia region.", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 4593, "url": "https://svs.gsfc.nasa.gov/4593/", "page_type": "Visualization", "title": "Earthrise in 4K", "description": "On December 24, 1968, Apollo 8 astronauts Frank Borman, Jim Lovell, and Bill Anders became the first humans to witness the Earth rising above the moon's barren surface. Now we can relive the astronauts' experience, thanks to data from NASA's Lunar Reconnaissance Orbiter. Complete transcript available.Watch this video on the NASA Goddard YouTube channel. || YOUTUBE_1080_G2018_Earthrise_Master_VX-300368_youtube_1080.mp4 (1920x1080) [882.1 MB] || earthrise_print.jpg (3840x2160) [515.7 KB] || earthrise_print_searchweb.png (320x180) [52.8 KB] || earthrise_print_thm.png (80x40) [4.6 KB] || YOUTUBE_720_G2018_Earthrise_Master_VX-300368_youtube_720.mp4 (1280x720) [832.1 MB] || FACEBOOK_720_G2018_Earthrise_Master_VX-300368_facebook_720.mp4 (1280x720) [641.1 MB] || TWITTER_720_G2018_Earthrise_Master_VX-300368_twitter_720.mp4 (1280x720) [114.9 MB] || G2018_Earthrise_Master.mov (3840x2160) [19.6 GB] || G2018_Earthrise_Master.mp4 (3840x2160) [500.2 MB] || G2018_Earthrise_Master_Output.en_US.srt [6.8 KB] || G2018_Earthrise_Master_Output.en_US.vtt [6.7 KB] || G2018_Earthrise_Master.webm (3840x2160) [107.0 MB] || ", "release_date": "2018-12-21T09:00:00-05:00", "update_date": "2023-05-03T13:46:09.882116-04:00", "main_image": { "id": 397745, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004500/a004593/earthrise_print.jpg", "filename": "earthrise_print.jpg", "media_type": "Image", "alt_text": "On December 24, 1968, Apollo 8 astronauts Frank Borman, Jim Lovell, and Bill Anders became the first humans to witness the Earth rising above the moon's barren surface. Now we can relive the astronauts' experience, thanks to data from NASA's Lunar Reconnaissance Orbiter. Complete transcript available.Watch this video on the NASA Goddard YouTube channel.", "width": 3840, "height": 2160, "pixels": 8294400 } }, { "id": 4654, "url": "https://svs.gsfc.nasa.gov/4654/", "page_type": "Visualization", "title": "Evolution of the Meteorological Observing System in the MERRA-2 Reanalysis", "description": "Meteorological Observing Systems, 1980 and 2018. Data is revealed within a moving 1.5 hour window centered on the time shown. || gmao_HW.00300_print.jpg (1024x345) [102.7 KB] || gmao_HW.00300_searchweb.png (320x180) [93.0 KB] || gmao_HW.00300_thm.png (80x40) [6.4 KB] || gmao_HW_1920_648p30.mp4 (1920x648) [134.3 MB] || gmao_HW_1920_648p30.webm (1920x648) [11.9 MB] || frames/9600x3240_80x27_30p/ (9600x3240) [128.0 KB] || ", "release_date": "2018-12-14T12:00:00-05:00", "update_date": "2023-11-15T00:12:01.066508-05:00", "main_image": { "id": 397860, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004600/a004654/gmao_2018_HW.0300_print.jpg", "filename": "gmao_2018_HW.0300_print.jpg", "media_type": "Image", "alt_text": "Meteorological Observing Systems, 2018. Data is revealed within a moving 1.5 hour window centered on the time shown.", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 4624, "url": "https://svs.gsfc.nasa.gov/4624/", "page_type": "Visualization", "title": "El Yunque National Forest, Puerto Rico Canopy Change from Afar (2017-2018)", "description": "Sample Composite that split screens the lidar swath over the El Yunque National Forest, Puerto Rico. During the split screen, 2017 data is on the upper left and 2018 data on the bottom right. As the camera moves northwest, the viewer can see patches of ground becoming visible in the 2018 data. This is due to the vast numbers of trees that were stripped or fell during Hurricane Maria in September 2017. || el_verde_comp.0190_print.jpg (1024x576) [368.1 KB] || el_verde_comp.0800.png (1920x1080) [3.0 MB] || el_verde_comp.0190_searchweb.png (320x180) [115.9 KB] || el_verde_comp.0190_thm.png (80x40) [6.0 KB] || el_verde_comp_1080p30.mp4 (1920x1080) [247.1 MB] || frames/1920x1080_16x9_30p/Sample_Composite/ (1920x1080) [256.0 KB] || el_verde_comp_1080p30.webm (1920x1080) [11.9 MB] || el_verde_comp.0800.tif (1920x1080) [5.9 MB] || ", "release_date": "2018-12-10T12:00:00-05:00", "update_date": "2023-11-15T00:11:32.432920-05:00", "main_image": { "id": 855523, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004600/a004624/el_verde_comp.0800.png", "filename": "el_verde_comp.0800.png", "media_type": "Image", "alt_text": "Sample Composite that split screens the lidar swath over the El Yunque National Forest, Puerto Rico. During the split screen, 2017 data is on the upper left and 2018 data on the bottom right. As the camera moves northwest, the viewer can see patches of ground becoming visible in the 2018 data. This is due to the vast numbers of trees that were stripped or fell during Hurricane Maria in September 2017.", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 4658, "url": "https://svs.gsfc.nasa.gov/4658/", "page_type": "Visualization", "title": "NASA's Black Marble night lights used to examine disaster recovery in Puerto Rico", "description": "At night, Earth is lit up in bright strings of roads dotted with pearl-like cities and towns as human-made artificial light takes center stage. During Hurricane Maria, Puerto Rico's lights went out.In the days, weeks, and months that followed, research physical scientist Miguel Román at NASA's Goddard Space Flight Center in Greenbelt, Maryland, and his colleagues combined NASA's Black Marble night lights data product from the NASA/NOAA Suomi National Polar-orbiting Partnership satellite with USGS-NASA Landsat data and Google's OpenStreetMap to develop a neighborhood-scale map of energy use in communities across Puerto Rico as the electricity grid was slowly restored. They then analyzed the relationship between restoration rates in terms of days without electricity and the remoteness of communities from major cities. || ", "release_date": "2018-12-09T00:00:00-05:00", "update_date": "2023-11-15T00:12:05.543017-05:00", "main_image": { "id": 398084, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004600/a004658/bmhd_11_0940_print.jpg", "filename": "bmhd_11_0940_print.jpg", "media_type": "Image", "alt_text": "This visualization starts with a global view of hurricane Maria hitting Puerto Rico. We then zoom in to Puerto Rico to compare the standard night lights dataset to a new, high definition version of nights lights. After the hurricane passes over the island, we see a massive drop in night light intensity due to loss of power. After showing night light levels over several stages of hurricane recovery, we transition to a 'Days Without Power' dataset. The camera then zooms in to several locations around the island to examine each stage of recovery in more detail. ", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 4700, "url": "https://svs.gsfc.nasa.gov/4700/", "page_type": "Visualization", "title": "PACE - Studying Plankton, Aerosols, Clouds, and the Ocean Ecosystem", "description": "The visualization starts close on the PACE spacecraft. A representative data swath is shown, depicting biosphere plankton data. The camera then pulls out to show the spacecraft's polar orbit. Complete global coverage is achieved after approximately two days of orbits. Over time, the data swath cycles between biosphere, aerosol, and cloud data, representing PACE's collective mission to study Earth's ocean and atmosphere. This version end with animated biosphere data. || pace_v2_4k_0245_print.jpg (1024x576) [36.4 KB] || pace_v2_4k_0245_searchweb.png (320x180) [39.7 KB] || pace_v2_4k_0245_thm.png (80x40) [3.7 KB] || pace_v3_1080p30.mp4 (1920x1080) [30.0 MB] || frames/3840x2160_16x9_30p/pace_comp3_animated-biosphere/ (3840x2160) [128.0 KB] || pace_v3_2160p30.mp4 (3840x2160) [94.4 MB] || pace_v3_2160p30.webm (3840x2160) [19.1 MB] || ", "release_date": "2018-12-05T09:00:00-05:00", "update_date": "2024-01-21T00:10:36.321044-05:00", "main_image": { "id": 399098, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004700/a004700/pace_v2_4k_0245_print.jpg", "filename": "pace_v2_4k_0245_print.jpg", "media_type": "Image", "alt_text": "The visualization starts close on the PACE spacecraft. A representative data swath is shown, depicting biosphere plankton data. The camera then pulls out to show the spacecraft's polar orbit. Complete global coverage is achieved after approximately two days of orbits. Over time, the data swath cycles between biosphere, aerosol, and cloud data, representing PACE's collective mission to study Earth's ocean and atmosphere. This version end with animated biosphere data. ", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 4572, "url": "https://svs.gsfc.nasa.gov/4572/", "page_type": "Visualization", "title": "The Hiawatha Impact Crater", "description": "The series of visualizations below are derived from satellite imagery and radar sounding. They portray both the location and size of the 31-kilometer-wide impact crater beneath Hiawatha Glacier. They also portray the structure of the glacier ice that flows into and fills the crater.The Hiawatha impact crater was first suspected to exist in the summer of 2015, from examination of a compilation of Greenland's sub-ice topography radar measurements made by NASA over two decades. The visualizations of the subsurface shown below are derived from a spring 2016 airborne survey by Germany's Alfred Wegener Institute, using a new ultrawideband radar sounder developed by the Center for Remote Sensing of Ice Sheets at The University of Kansas. Subsequent helicopter visits to the deglaciated terrain in front of Hiawatha Glacier by scientists from the Natural History Museum in Denmark recovered sediment samples from the main river that discharges water from beneath Hiawatha Glacier, through the northwestern rim breach. Laboratory examination revealed that these sediment samples contained shocked quartz and elevated platinum-group-element concentrations, both signs that the sediment records evidence of the impact of an iron asteroid more than one kilometer wide. The Hiawatha impact crater is potentially one of the youngest large impact craters on Earth.In the visualizations below, the elevation of the topography of the bed, the ice surface and the radar curtains have been exaggerated ten times in order to better illustrate their structure. || ", "release_date": "2018-11-14T14:00:00-05:00", "update_date": "2023-11-15T00:10:56.164476-05:00", "main_image": { "id": 413123, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004500/a004572/Hiawatha_v45_scene1_4k_5mtopo.1665_print.jpg", "filename": "Hiawatha_v45_scene1_4k_5mtopo.1665_print.jpg", "media_type": "Image", "alt_text": "A still image showing the Greenland Ice Sheet and the Hiawatha Glacier.", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 13058, "url": "https://svs.gsfc.nasa.gov/13058/", "page_type": "Produced Video", "title": "Simulations Create New Insights Into Pulsars", "description": "Explore a new “pulsar in a box” computer simulation that tracks the fate of electrons (blue) and their antimatter kin, positrons (red), as they interact with powerful magnetic and electric fields around a neutron star. Lighter colors indicate higher particle energies. Each particle seen in this visualization actually represents trillions of electrons or positrons. Better knowledge of the particle environment around neutron stars will help astronomers understand how they produce precisely timed radio and gamma-ray pulses.Credit: NASA’s Goddard Space Flight CenterMusic: \"Reaching for the Horizon\" and \"Leaving Earth\" from Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Pulsar_Still_1_print.jpg (1024x576) [436.1 KB] || Pulsar_Still_1.jpg (3840x2160) [4.5 MB] || Pulsar_Still_1_searchweb.png (320x180) [134.5 KB] || Pulsar_Still_1_thm.png (80x40) [9.1 KB] || 13058_Pulsar_Particle_Simulation_H264_1080.mov (1920x1080) [313.3 MB] || 13058_Pulsar_Particle_Simulation_1080.mp4 (1920x1080) [208.0 MB] || 13058_Pulsar_Particle_Simulation_1080.webm (1920x1080) [25.8 MB] || 13058_Pulsar_Particle_Simulation_ProRes_3840x2160_2997.mov (3840x2160) [10.6 GB] || 13058_Pulsar_Particle_Simulation_2160.mp4 (3840x2160) [523.3 MB] || 13058_Pulsar_Particle_Simulation_SRT_Captions.en_US.srt [3.7 KB] || 13058_Pulsar_Particle_Simulation_SRT_Captions.en_US.vtt [3.6 KB] || ", "release_date": "2018-10-10T11:00:00-04:00", "update_date": "2023-05-03T13:46:21.643447-04:00", "main_image": { "id": 400729, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a013000/a013058/Pulsar_Still_1_print.jpg", "filename": "Pulsar_Still_1_print.jpg", "media_type": "Image", "alt_text": "Explore a new “pulsar in a box” computer simulation that tracks the fate of electrons (blue) and their antimatter kin, positrons (red), as they interact with powerful magnetic and electric fields around a neutron star. Lighter colors indicate higher particle energies. Each particle seen in this visualization actually represents trillions of electrons or positrons. Better knowledge of the particle environment around neutron stars will help astronomers understand how they produce precisely timed radio and gamma-ray pulses.Credit: NASA’s Goddard Space Flight CenterMusic: \"Reaching for the Horizon\" and \"Leaving Earth\" from Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available.", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 4683, "url": "https://svs.gsfc.nasa.gov/4683/", "page_type": "Visualization", "title": "NASA Scientists see Gravity Waves in Concentric Rings", "description": "NASA scientists have tracked gravity waves traveling thousands of miles across our atmosphere in concentric rings. Large storms can create these waves, which grow and spread upward hundreds of miles above Earth's surface. The AIRS instrument on NASA's Aqua satellite detected gravity waves in the troposphere and stratosphere 12 hours before a deadly EF5 tornado in Moore, Oklahoma, in 2013. On the instrument's next pass 11 hours later, it detected even stronger waves.We pull up 250 miles to the ionosphere, where the waves can be observed by GPS satellites. Here gravity waves are shown in greens and yellows, like ripples in a pond. The waves and tornado were both produced by a long-lived storm system.Understanding the spread of gravity waves improves global weather forecasting and space weather forecasting.Complete transcript available.This video is also available on our YouTube channel. || GravityWavesBeforeAfterMooreTornado_0740_print.jpg (1024x576) [131.1 KB] || GravityWavesBeforeAfterMooreTornado_0740_searchweb.png (320x180) [102.9 KB] || GravityWavesBeforeAfterMooreTornado_0740_thm.png (80x40) [8.3 KB] || GravityWavesMooreOK-SameWordsDifferentOrder.mp4 (1920x1080) [117.1 MB] || GravityWavesBeforeAfterMooreTornado_0740.tif (1920x1080) [3.2 MB] || GravityWavesMooreOK-SameWordsDifferentOrder.webm (1920x1080) [7.4 MB] || GWfacebook-AIRS-TEC-GOES-4k-audio.mp4 (1920x1080) [76.1 MB] || GW4k-AIRS-TEC-GOES-4k-audio-youtube.mp4 (3840x2160) [240.0 MB] || frames/3840x2160_16x9_30p/composite/ (3849x2160) [128.0 KB] || GW4k-AIRS-TEC-GOES-4k-audio-youtube.en_US.srt [1.2 KB] || GW4k-AIRS-TEC-GOES-4k-audio-youtube.en_US.vtt [1.2 KB] || ", "release_date": "2018-10-10T00:00:00-04:00", "update_date": "2024-02-22T00:10:03.557161-05:00", "main_image": { "id": 400206, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004600/a004683/GravityWavesBeforeAfterMooreTornado_0740_print.jpg", "filename": "GravityWavesBeforeAfterMooreTornado_0740_print.jpg", "media_type": "Image", "alt_text": "NASA scientists have tracked gravity waves traveling thousands of miles across our atmosphere in concentric rings. Large storms can create these waves, which grow and spread upward hundreds of miles above Earth's surface. \rThe AIRS instrument on NASA's Aqua satellite detected gravity waves in the troposphere and stratosphere 12 hours before a deadly EF5 tornado in Moore, Oklahoma, in 2013. On the instrument's next pass 11 hours later, it detected even stronger waves.\r\rWe pull up 250 miles to the ionosphere, where the waves can be observed by GPS satellites. Here gravity waves are shown in greens and yellows, like ripples in a pond. \r The waves and tornado were both produced by a long-lived storm system.\rUnderstanding the spread of gravity waves improves global weather forecasting and space weather forecasting.\rComplete transcript available.This video is also available on our YouTube channel.", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 4685, "url": "https://svs.gsfc.nasa.gov/4685/", "page_type": "Visualization", "title": "Inside Hurricane Maria in 360°", "description": "Tour Hurricane Maria in a whole new way! Late on September 17, 2017 (10:08 p.m. EDT) Category 1 Hurricane Maria was strengthening in the Atlantic Ocean when the Global Precipitation Measurement (GPM) mission's Core Observatory flew over it. The Dual Frequency Precipitation Radar, measuring in a narrow band over the storm center, shows 3-D estimates of rain, with snow at higher altitudes. The tall \"hot towers\" characteristic of deepening hurricanes are actually topped by snow! Surface rainfall rates estimated by the GPM Microwave Imager paint the surface over a wider swath. During the tour, you'll see the radar-observed rain intensities displayed three different ways in various parts of the storm. Then, for the first time you'll see estimates of the precipitation particle sizes, which the GPM DPR is uniquely capable of showing, and which provide important insights into storm processes.GPM is a joint mission between NASA and the Japanese space agency JAXA. || ", "release_date": "2018-10-04T09:55:00-04:00", "update_date": "2023-06-16T10:10:37.515918-04:00", "main_image": { "id": 400488, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004600/a004685/maria360.112_4k.7300_print.jpg", "filename": "maria360.112_4k.7300_print.jpg", "media_type": "Image", "alt_text": "Visualization of Hurricane Maria. These are full 360 degree frames. These fames appear warped because they include the entire 360 degree view.This video is also available on our YouTube channel.", "width": 1024, "height": 512, "pixels": 524288 } }, { "id": 4664, "url": "https://svs.gsfc.nasa.gov/4664/", "page_type": "Visualization", "title": "Jupiter's Magnetosphere", "description": "Jupiter's magnetosphere - a basic view. || Jupiter_JupiterBasic_Dayside.slate_BaseRig.HD1080i.1000_print.jpg (1024x576) [245.3 KB] || Jupiter_JupiterBasic_Dayside.slate_BaseRig.HD1080i.1000_searchweb.png (320x180) [132.5 KB] || Jupiter_JupiterBasic_Dayside.slate_BaseRig.HD1080i.1000_thm.png (80x40) [8.3 KB] || frames/1920x1080_16x9_30p/JupiterBasic-noglyph/ (1920x1080) [512.0 KB] || Jupiter_JupiterBasic_Dayside.HD1080i_p30.mp4 (1920x1080) [406.6 MB] || Jupiter_JupiterBasic_Dayside.HD1080i_p30.webm (1920x1080) [32.8 MB] || frames/3840x2160_16x9_30p/JupiterBasic-noglyph/ (3840x2160) [512.0 KB] || Jupiter_JupiterBasic_Dayside_2160p30.mp4 (3840x2160) [984.8 MB] || ", "release_date": "2018-07-27T00:00:00-04:00", "update_date": "2023-11-15T00:12:12.373473-05:00", "main_image": { "id": 402095, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004600/a004664/Jupiter_JupiterBasic_Dayside.slate_BaseRig.HD1080i.1000_print.jpg", "filename": "Jupiter_JupiterBasic_Dayside.slate_BaseRig.HD1080i.1000_print.jpg", "media_type": "Image", "alt_text": "Jupiter's magnetosphere - a basic view.", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 4639, "url": "https://svs.gsfc.nasa.gov/4639/", "page_type": "Visualization", "title": "MMS Sees a New Type of Reconnection", "description": "The Magnetospheric Multiscale (MMS) mission consists of four identical satellites that traverse various regions of Earth's magnetosphere measuring the particles and electric and magnetic field which influence them.In the turbulent plasma between Earth's magnetopause and bow shock, a region called the magnetosheath, the MMS satellite constellation has measured multiple jets of energetic electrons between magnetic bubbles. This appears to be a new 'flavor' of magnetic reconnection based on electrons and occuring on smaller time and spatial scales than the standard model of magnetic reconnection with ions.In these data visualizations, the arrows represent the data collected by the spacecraft. To better comprehend changes as the spacecraft moves along, the data are allowed to 'echo' along the spacecraft trail. The length of the vectors represent the relative magnitude of the vector. However, the electron and proton vectors are scaled so equal velocities correspond to vectors of equal magnitude.Magenta represents the direction and magnitude of the magnetic field at the spacecraft position.Green represents the direction and magnitude of the net electric current created by the motion of the electrons and ions measured at the spacecraft position.The four MMS spacecraft are represented by colored spheres, corresponding to the plotted data lines in the lower graphicMMS1MMS2MMS3MMS4The clocks on MMS are synchronized for the TAI (International Atomic Time) system provided through the Global Positioning System (GPS) satellites. It provides a high-precision time reference for comparing MMS measurements to other datasets. || ", "release_date": "2018-05-09T13:00:00-04:00", "update_date": "2023-11-15T00:11:48.742291-05:00", "main_image": { "id": 404491, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004600/a004639/PhanNewReconnect_Fly2Pursuit2Drift_Dec09DataShort_RE_MMS.slate_CRTT.HD1080i.3000_print.jpg", "filename": "PhanNewReconnect_Fly2Pursuit2Drift_Dec09DataShort_RE_MMS.slate_CRTT.HD1080i.3000_print.jpg", "media_type": "Image", "alt_text": "From a wide view of the MMS orbit, this visualization zooms down to the four spacecraft as they move between the magnetopause and bow shock. Along the track of each spacecraft we see the measured magnetic field vectors (magenta arrows) and the measured current vectors (green arrows). The energetic event of interest occurs at clock time of 09:03:54.3 TAI.", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 4629, "url": "https://svs.gsfc.nasa.gov/4629/", "page_type": "Visualization", "title": "Snowflakes Melting Simulation Over Turntable", "description": "Clockwise rotating turntable of a cluster of melting snowflakes. || turntable_v39.0000_print.jpg (1024x576) [69.2 KB] || turntable_v39.0000_searchweb.png (320x180) [34.1 KB] || turntable_v39.0000_thm.png (80x40) [3.4 KB] || turntable_v39_1080p30.mp4 (1920x1080) [13.2 MB] || frames/1920x1080_16x9_30p/ (1920x1080) [64.0 KB] || turntable_v39_1080p30.webm (1920x1080) [2.7 MB] || ", "release_date": "2018-03-29T00:00:00-04:00", "update_date": "2024-03-17T00:09:14.525932-04:00", "main_image": { "id": 405806, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004600/a004629/turntable_v39.0000_print.jpg", "filename": "turntable_v39.0000_print.jpg", "media_type": "Image", "alt_text": "Clockwise rotating turntable of a cluster of melting snowflakes.", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 4602, "url": "https://svs.gsfc.nasa.gov/4602/", "page_type": "Visualization", "title": "New island forms in Tonga", "description": "This visualization shows the change in the island of Hunga Tonga Hunga Ha'apa between January 2015 and September 2017.This video is also available on our YouTube channel. || Tonga_v60_vis.0780_print.jpg (1024x576) [123.5 KB] || Tonga_v60_vis.0780_searchweb.png (320x180) [76.8 KB] || Tonga_v60_vis.0780_thm.png (80x40) [6.0 KB] || frames/1920x1080_16x9_30p/new_island_vis/ (1920x1080) [128.0 KB] || Tonga_v60_vis_1080p30.mp4 (1920x1080) [33.3 MB] || Tonga_v60_vis_1080p30.webm (1920x1080) [5.1 MB] || Tonga_4k_final2_1080p30.mp4 (1920x1080) [34.3 MB] || frames/3840x2160_16x9_30p/new_island_vis/ (3840x2160) [128.0 KB] || Tonga_4k_final2_2160p30.mp4 (3840x2160) [52.0 MB] || ", "release_date": "2017-12-11T10:00:00-05:00", "update_date": "2023-11-15T00:11:21.704660-05:00", "main_image": { "id": 408449, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004600/a004602/Tonga_v60_vis.0780_print.jpg", "filename": "Tonga_v60_vis.0780_print.jpg", "media_type": "Image", "alt_text": "This visualization shows the change in the island of Hunga Tonga Hunga Ha'apa between January 2015 and September 2017.This video is also available on our YouTube channel.", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 4373, "url": "https://svs.gsfc.nasa.gov/4373/", "page_type": "Visualization", "title": "ICESat-2 Orbit", "description": "ICESat-2 orbiting Earth: starting with global view building up ground track, then riding the satellite view, then back to a global view with full ground track || icesat2_orbit26.2100_print.jpg (1024x576) [114.4 KB] || icesat2_orbit26.2100_searchweb.png (320x180) [77.7 KB] || icesat2_orbit26.2100_thm.png (80x40) [5.2 KB] || icesat2_orbit_long_1080p30.mp4 (1920x1080) [104.5 MB] || icesat2_orbit_long_720p30.mp4 (1280x720) [42.8 MB] || long (1920x1080) [512.0 KB] || long (1280x720) [512.0 KB] || icesat2_orbit_long_1080p30.webm (1920x1080) [18.2 MB] || icesat2_orbit_long_2160p30.mp4 (3840x2160) [406.6 MB] || icesat2_orbit_long_360p30.m4v (640x360) [27.8 MB] || long (3840x2160) [512.0 KB] || ", "release_date": "2017-11-03T15:00:00-04:00", "update_date": "2024-04-28T00:07:07.253706-04:00", "main_image": { "id": 412022, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004300/a004373/icesat2_orbit26.2100_print.jpg", "filename": "icesat2_orbit26.2100_print.jpg", "media_type": "Image", "alt_text": "ICESat-2 orbiting Earth: starting with global view building up ground track, then riding the satellite view, then back to a global view with full ground track", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 4571, "url": "https://svs.gsfc.nasa.gov/4571/", "page_type": "Visualization", "title": "Global Surface- and Upper-Level Winds", "description": "This entry compiles a series of animations created for the use of WGBH in an educational webside. The animations visualize data from the MERRA reanalysis product, showing winds at both the 850 mb and 250 mb levels. The upper level is rainbow-colored, the lower level is white. Both color and opacity of each level are being driven by windspeed. || ", "release_date": "2017-08-29T00:00:00-04:00", "update_date": "2023-12-03T22:49:10.556580-05:00", "main_image": { "id": 411703, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004500/a004571/test2.0001_print.jpg", "filename": "test2.0001_print.jpg", "media_type": "Image", "alt_text": "850 mb and 250 mb levels", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 4201, "url": "https://svs.gsfc.nasa.gov/4201/", "page_type": "Visualization", "title": "Tracking Data Relay Satellite (TDRS) Orbital Fleet Communicating with User Spacecraft 2017 - 360 video", "description": "Visualization depicting TDRS satellites communicating with customer satellites. White lines represent periods of communication between satellites. Constant contact between TDRS satellites and ground stations is also displayed using grey lines. || tdrs_access_1080_60fps_03.14100_print.jpg (1024x576) [106.7 KB] || tdrs_access_1080_60fps_03.14100_searchweb.png (320x180) [64.2 KB] || tdrs_access_1080_60fps_03.14100_thm.png (80x40) [4.2 KB] || frames/1920x1080_16x9_60p/ (1920x1080) [512.0 KB] || tdrs_access_1080_60fps_03_p60.mp4 (1920x1080) [106.1 MB] || tdrs_access_1080_60fps_03_p60.webm (1920x1080) [13.9 MB] || frames/3840x2160_16x9_60p/ (3840x2160) [512.0 KB] || tdrs_access_4k_60fps_10_2160p30.mp4 (3840x2160) [298.3 MB] || tdrs_access_4k_60fps_10_2160p60.mp4 (3840x2160) [295.9 MB] || tdrs_access_4k_60fps_APR.mov (3840x2160) [15.2 GB] || tdrs_access_4k_60fps_APRLite.mov (3840x2160) [4.3 GB] || tdrs_access_4k_60fps_YT4K.mp4 (3840x2160) [1.1 GB] || ", "release_date": "2017-08-16T00:00:00-04:00", "update_date": "2023-05-03T13:47:26.776005-04:00", "main_image": { "id": 412607, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004200/a004201/tdrs_access_1080_60fps_03.14100_print.jpg", "filename": "tdrs_access_1080_60fps_03.14100_print.jpg", "media_type": "Image", "alt_text": "Visualization depicting TDRS satellites communicating with customer satellites. White lines represent periods of communication between satellites. Constant contact between TDRS satellites and ground stations is also displayed using grey lines. ", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 12635, "url": "https://svs.gsfc.nasa.gov/12635/", "page_type": "Produced Video", "title": "A New Multi-dimensional View of a Hurricane", "description": "Music: \"Buoys,\" Donn Wilkerson, Killer Tracks; \"Late Night Drive,\" Donn Wilkerson, Killer Tracks.Complete transcript available. || Matthew_screengrab_print.jpg (1024x574) [158.4 KB] || Matthew_screengrab_searchweb.png (320x180) [114.3 KB] || Matthew_screengrab_thm.png (80x40) [8.1 KB] || 12635_Hurricane_Matthew_prores.mov (1920x1080) [3.0 GB] || 12635_Hurricane_Matthew.mp4 (1920x1080) [236.9 MB] || 12635_Hurricane_Matthew_prores.webm (1920x1080) [25.4 MB] || 12635_Hurricane_Matthew_facebook_720.mp4 (1280x720) [271.2 MB] || 12635_Hurricane_Matthew_prores_youtube_720.mp4 (1280x720) [362.8 MB] || 12635_Hurricane_Matthew_twitter_720.mp4 (1280x720) [49.8 MB] || 12635_Hurricane_Matthew_youtube_1080.mp4 (1920x1080) [362.9 MB] || 12635_Hurricane_Matthew.en_US.srt [4.1 KB] || 12635_Hurricane_Matthew.en_US.vtt [4.1 KB] || ", "release_date": "2017-07-25T00:00:00-04:00", "update_date": "2023-05-03T13:47:32.041851-04:00", "main_image": { "id": 413617, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012600/a012635/Matthew_screengrab_print.jpg", "filename": "Matthew_screengrab_print.jpg", "media_type": "Image", "alt_text": "Music: \"Buoys,\" Donn Wilkerson, Killer Tracks; \"Late Night Drive,\" Donn Wilkerson, Killer Tracks.Complete transcript available.", "width": 1024, "height": 574, "pixels": 587776 } }, { "id": 4544, "url": "https://svs.gsfc.nasa.gov/4544/", "page_type": "Visualization", "title": "2015-2016 El Niño: Daily Sea Surface Temperature Anomaly and Ocean Currents", "description": "This visualization shows 2015-2016 El Nino through changes in sea surface temperature and ocean currents. Blue regions represent colder temperatures and red regions represent warmer temperatures when compared with normal conditions. Yellow arrows illustrate eastward currents and white arrows are westward currents. || GMAO_elNino_oceanTemperatureAnomaly_currents__1300_print.jpg (1024x576) [175.5 KB] || GMAO_elNino_oceanTemperatureAnomaly_currents__1300_searchweb.png (320x180) [97.1 KB] || GMAO_elNino_oceanTemperatureAnomaly_currents__1300_thm.png (80x40) [6.7 KB] || GMAO_elNino_oceanTemperatureAnomaly_currents_1080p.mp4 (1920x1080) [159.4 MB] || GMAO_elNino_oceanTemperatureAnomaly_currents_1080p.webm (1920x1080) [163.5 KB] || GMAO_oceanTemperatureAnomaly_withColorbar.mp4 (3840x2160) [166.0 MB] || frames/3840x2160_16x9_30p/with_colorbar/ (3840x2160) [256.0 KB] || ", "release_date": "2017-05-26T10:30:00-04:00", "update_date": "2023-11-15T00:10:24.170256-05:00", "main_image": { "id": 426723, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004500/a004544/GMAO_elNino_oceanTemperatureAnomaly_currents__1300_print.jpg", "filename": "GMAO_elNino_oceanTemperatureAnomaly_currents__1300_print.jpg", "media_type": "Image", "alt_text": "This visualization shows 2015-2016 El Nino through changes in sea surface temperature and ocean currents. Blue regions represent colder temperatures and red regions represent warmer temperatures when compared with normal conditions. Yellow arrows illustrate eastward currents and white arrows are westward currents.", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 3899, "url": "https://svs.gsfc.nasa.gov/3899/", "page_type": "Visualization", "title": "Seasonal sea ice and snow cover visualizations", "description": "Seasonal snow cover and sea ice across the globe from September 2010 to August 2011 || FlatMap_1920x108060fps_0000_print.jpg (1024x576) [99.4 KB] || FlatMap_1920x108060fps_0000_searchweb.png (320x180) [65.9 KB] || FlatMap_1920x108060fps_0000_web.png (320x180) [65.9 KB] || FlatMap_1920x108060fps_0000_thm.png (80x40) [5.8 KB] || frames/1920x1080_16x9_60p/Global/ (1920x1080) [256.0 KB] || frames/1920x1080_16x9_30p/Global/ (1920x1080) [128.0 KB] || frames/1280x720_16x9_30p/Global/ (1280x720) [128.0 KB] || FlatMap_1920x1080_p30.mp4 (1920x1080) [13.3 MB] || FlatMap_1280x720_p30.mp4 (1280x720) [8.2 MB] || FlatMap_1280x720_p30.webm (1280x720) [3.6 MB] || ", "release_date": "2017-01-04T00:00:00-05:00", "update_date": "2023-11-14T00:01:45.256516-05:00", "main_image": { "id": 488382, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a003800/a003899/FlatMap_1920x108060fps_0000_print.jpg", "filename": "FlatMap_1920x108060fps_0000_print.jpg", "media_type": "Image", "alt_text": "Seasonal snow cover and sea ice across the globe from September 2010 to August 2011", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 4514, "url": "https://svs.gsfc.nasa.gov/4514/", "page_type": "Visualization", "title": "Carbon Dioxide from GMAO using Assimilated OCO-2 Data", "description": "Carbon Dioxide from the GEOS-5 modelThis video is also available on our YouTube channel. || co2_30.with_labels.2000_print.jpg (1024x576) [90.1 KB] || co2_30.with_labels.2000_searchweb.png (320x180) [64.0 KB] || co2_30.with_labels.2000_thm.png (80x40) [5.9 KB] || co2_30.with_labels_1080p30.mp4 (1920x1080) [75.6 MB] || co2_30.with_labels_1080p30.webm (1920x1080) [11.3 MB] || co2_30.with_labels_2160p30.mp4 (3840x2160) [306.7 MB] || co2_30.with_labels_360p30.mp4 (640x360) [12.2 MB] || frames/3840x2160_16x9_30p/final_no_dates/ (3840x2160) [256.0 KB] || frames/3840x2160_16x9_30p/final_with_labels/ (3840x2160) [256.0 KB] || co2_30.with_labels.key [77.8 MB] || co2_30.with_labels.pptx [77.4 MB] || ", "release_date": "2016-12-13T14:00:00-05:00", "update_date": "2023-11-14T00:08:19.384767-05:00", "main_image": { "id": 418954, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004500/a004514/co2_30.with_labels.2000_print.jpg", "filename": "co2_30.with_labels.2000_print.jpg", "media_type": "Image", "alt_text": "Carbon Dioxide from the GEOS-5 modelThis video is also available on our YouTube channel.", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 4516, "url": "https://svs.gsfc.nasa.gov/4516/", "page_type": "Visualization", "title": "2017 Path of Totality: Oblique View", "description": "This animation closely follows the Moon's umbra shadow as it passes over the United States during the August 21, 2017 total solar eclipse. Through the use of a number of NASA datasets, notably the global elevation maps from Lunar Reconnaissance Orbiter, the shape and location of the shadow is depicted with unprecedented accuracy. || usa_oblique.4044_print.jpg (1024x576) [307.4 KB] || usa_oblique.4044_searchweb.png (320x180) [115.3 KB] || usa_oblique.4044_thm.png (80x40) [6.7 KB] || totpathoblq2017_1080p30.mp4 (1920x1080) [207.3 MB] || totpathoblq2017_720p30.mp4 (1280x720) [117.9 MB] || totpathoblq2017_720p30.webm (1280x720) [22.6 MB] || totpathoblq2017_2160p30.mp4 (3840x2160) [499.6 MB] || totpathoblq2017_360p30.mp4 (640x360) [39.7 MB] || frames/3840x2160_16x9_30p/ (3840x2160) [512.0 KB] || totpathoblq2017_4516.key [120.0 MB] || totpathoblq2017_4516.pptx [119.6 MB] || ", "release_date": "2016-12-13T00:00:00-05:00", "update_date": "2024-01-25T00:07:54.342033-05:00", "main_image": { "id": 418904, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004500/a004516/usa_oblique.4044_print.jpg", "filename": "usa_oblique.4044_print.jpg", "media_type": "Image", "alt_text": "This animation closely follows the Moon's umbra shadow as it passes over the United States during the August 21, 2017 total solar eclipse. Through the use of a number of NASA datasets, notably the global elevation maps from Lunar Reconnaissance Orbiter, the shape and location of the shadow is depicted with unprecedented accuracy.", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 4482, "url": "https://svs.gsfc.nasa.gov/4482/", "page_type": "Animation", "title": "OSIRIS-REx orbits, maneuvers, and mapping", "description": "The Origins Spectral Interpretation Resource Identification Security - Regolith Explorer spacecraft will travel to a near-Earth asteroid, called Bennu (formerly 1999 RQ36), and bring at least a 2.1-ounce sample back to Earth for study. The mission will help scientists investigate how planets formed and how life began, as well as improve our understanding of asteroids that could impact Earth.OSIRIS-REx launched on Sept. 8, 2016, at 7:05 p.m. EDT. As planned, the spacecraft will reach its target asteroid in 2018 and return a sample to Earth in 2023. These animations depict the journey of OSIRIS-REx to Bennu and back, including the complex maneuvers that the spacecraft will perform in the asteroid's low-gravity environment. The animations are presented in chronological order. || ", "release_date": "2016-10-04T00:00:00-04:00", "update_date": "2024-04-24T00:08:41.359894-04:00", "main_image": { "id": 419432, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004400/a004482/orex_Outbound_GravityAssist_0790_print.jpg", "filename": "orex_Outbound_GravityAssist_0790_print.jpg", "media_type": "Image", "alt_text": "OSIRIS-REx outbound orbit to asteroid Bennu, including an Earth-gravity assist approximately one year after launch. The gravity assist will adjust the spacecraft’s orbit, putting it in the same inclination as the orbit of Bennu.", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 4469, "url": "https://svs.gsfc.nasa.gov/4469/", "page_type": "Visualization", "title": "Dynamic Earth-A New Beginning", "description": "The visualization 'Excerpt from \"Dynamic Earth\"' has been one of the most popular visualizations that the Scientific Visualization Studio has ever created. It's often used in presentations and Hyperwall shows to illustrate the connections between the Earth and the Sun, as well as the power of computer simulation in understanding those connections.There is one part of this visualization, however, that has always seemed a little clumsy to us. The opening shot is a pullback from the limb of the sun, where the sun is represented by a movie of 304 Angstrom images from the Solar Dynamics Observatory (SDO). It is difficult to pull back from the limb of a flat sun image and make the sun look spherical, and the problem was made more difficult because the original sun images were in a spherical dome show format. As a result, the pullback from the sun showed some odd reprojection artifacts.The best solution to this issue was to replace the existing pullout with a new one, one which pulled directly out from the center of the solar disk. For the new beginning, we chose a series of SDO images in the 171 Angstrom channel that show a visible coronal mass ejection (CME) in the lower right corner of the solar disk. Although this is not the specific CME that is seen affecting Venus and Earth later in this visualization, its presence links the SDO animation thematically to the later solar storm. The SDO images were also brightened considerably and tinted yellow to match the common perception of the Sun as a bright yellow object (even though it is actually white).Please go to the original version of this visualization to see the complete credits and additional details. || ", "release_date": "2016-06-16T15:00:00-04:00", "update_date": "2024-01-14T22:39:41.665871-05:00", "main_image": { "id": 423901, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004400/a004469/newsun.00000_print.jpg", "filename": "newsun.00000_print.jpg", "media_type": "Image", "alt_text": "This is the complete Dynamic Earth excerpt with a new beginning at 1080p and 4K resolution.This video is also available on our YouTube channel.", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 4370, "url": "https://svs.gsfc.nasa.gov/4370/", "page_type": "Visualization", "title": "Solar Wind Strips the Martian Atmosphere", "description": "Scientists have long suspected the solar wind of stripping the Martian upper atmosphere into space, turning Mars from a blue world to a red one. Now, NASA's MAVEN orbiter is observing this process in action, providing significant data on solar wind erosion at Mars.Watch this video on the NASA Goddard YouTube channel.Complete transcript available.This video is also available on our YouTube channel. || MarsAtmoLossExplainPreview.jpg (1920x1080) [993.6 KB] || APPLE_TV_4370_MAVEN_Mars_Atmo_Loss_appletv_subtitles.m4v (1280x720) [53.7 MB] || WEBM_4370_MAVEN_Mars_Atmo_Loss_APR.webm (960x540) [44.7 MB] || 4370_MAVEN_Mars_Atmo_Loss_appletv.m4v (1280x720) [53.7 MB] || 4370_MAVEN_Mars_Atmo_Loss_APR_Output.en_US.srt [2.3 KB] || 4370_MAVEN_Mars_Atmo_Loss_APR_Output.en_US.vtt [2.3 KB] || NASA_TV_4370_MAVEN_Mars_Atmo_Loss.mpeg (1280x720) [369.5 MB] || 4370_MAVEN_Mars_Atmo_Loss_APR.mov (3840x2160) [5.9 GB] || YOUTUBE_HQ_4370_MAVEN_Mars_Atmo_Loss_youtube_hq.mov (3840x2160) [2.2 GB] || LARGE_MP4_4370_MAVEN_Mars_Atmo_Loss_large.mp4 (3840x2160) [111.3 MB] || ", "release_date": "2015-11-05T14:00:00-05:00", "update_date": "2024-05-29T00:06:18.253192-04:00", "main_image": { "id": 439148, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004300/a004370/final_ions01.4300_print.jpg", "filename": "final_ions01.4300_print.jpg", "media_type": "Image", "alt_text": "Movie without music and titles. Available for download in up to 4k resolution.", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 4253, "url": "https://svs.gsfc.nasa.gov/4253/", "page_type": "Visualization", "title": "Moon Phase and Libration, from the Other Side", "description": "This narrated video introduces two views of the Moon's far side. Transcript.This video is also available on our YouTube channel. || opposite.0820_print.jpg (1024x576) [158.8 KB] || opposite.0820_thm.png (80x40) [5.8 KB] || G2015-013_ViewfromOtherSide_MASTER_youtube_hq.mov (1280x720) [75.4 MB] || G2015-013_ViewfromOtherSide_MASTER_1280x720.wmv (1280x720) [50.7 MB] || G2015-013_ViewfromOtherSide_MASTER_prores.mov (1280x720) [1.5 GB] || G2015-013_ViewfromOtherSide_MASTER_appletv.m4v (960x540) [43.3 MB] || G2015-013_ViewfromOtherSide_MASTER_appletv.webm (960x540) [13.8 MB] || G2015-013_ViewfromOtherSide_MASTER_appletv_subtitles.m4v (960x540) [43.2 MB] || G2015-013_ViewfromOtherSide_MASTER_nasaportal.mov (640x360) [34.9 MB] || G2015-013_ViewfromOtherSide_MASTER_ipod_lg.m4v (640x360) [19.0 MB] || G2015-013_ViewfromOtherSide.en_US.srt [2.0 KB] || G2015-013_ViewfromOtherSide.en_US.vtt [2.0 KB] || G2015-013_ViewfromOtherSide_MASTER_ipod_sm.mp4 (320x240) [9.0 MB] || ", "release_date": "2015-02-04T09:00:00-05:00", "update_date": "2023-05-03T13:50:03.382564-04:00", "main_image": { "id": 447486, "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004200/a004253/opposite.1170_print.jpg", "filename": "opposite.1170_print.jpg", "media_type": "Image", "alt_text": "The SIGGRAPH conference is widely recognized as the most prestigious forum for the publication of computer graphics research. The conference provides an interdisciplinary educational experience highlighting outstanding achievements in time-based art, scientific visualization, visual effects, real-time graphics, and narrative shorts. Below are contributions to the conference made by members of NASA Goddard's Scientific Visualization Studio.", "width": 576, "height": 1024, "pixels": 589824 } }, { "id": 11670, "url": "https://svs.gsfc.nasa.gov/11670/", "page_type": "Produced Video", "title": "Sun Emits Mid-Level Flare on October 2, 2014", "description": "The sun emitted a mid-level solar flare, peaking at 3:01 p.m. EDT on Oct. 2, 2014. NASA's Solar Dynamics Observatory, which watches the sun 24-hours a day, captured images of the flare. Solar flares are powerful bursts of radiation. Harmful radiation from a flare cannot pass through Earth's atmosphere to physically affect humans on the ground, however — when intense enough — they can disturb the atmosphere in the layer where GPS and communications signals travel.This flare is classified as an M7.3 flare. M-class flares are one-tenth as powerful as the most powerful flares, which are designated X-class flares. || ", "release_date": "2014-10-03T15:00:00-04:00", "update_date": "2023-05-03T13:50:29.586105-04:00", "main_image": { "id": 450865, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011600/a011670/Oct_2_Blend_Still.jpg", "filename": "Oct_2_Blend_Still.jpg", "media_type": "Image", "alt_text": "Video of flare and eruption in several wavelengths. It begins with 304 angstrom, then 171, and finally a blend of 304, 171 and 131, which shows the hottest flaring regions.Music: \"No Comment Before Sunset\" by Lars Leonhard, courtesy of the artist and BineMusic.Watch this video on the NASA Goddard YouTube channel.For complete transcript, click here.", "width": 1920, "height": 1080, "pixels": 2073600 } } ], "products": [], "newer_versions": [], "older_versions": [], "alternate_versions": [] }