{ "count": 182, "next": "https://svs.gsfc.nasa.gov/api/search/?limit=100&offset=100&search=%22Equatorial%22", "previous": null, "results": [ { "id": 14884, "url": "https://svs.gsfc.nasa.gov/14884/", "result_type": "Produced Video", "release_date": "2026-01-29T11:00:00-05:00", "title": "NASA Supercomputer Probes Tangled Magnetospheres of Merging Neutron Stars", "description": "New supercomputer simulations explore the tangled magnetic structures around merging neutron stars. These structures, called magnetospheres, interact as the city-sized stars enter their final orbits. Magnetic field lines can connect both stars, break, and reconnect, while currents surge through surrounding plasma moving at nearly the speed of light. The simulations show that these systems may produce X-rays and gamma rays that future observatories should be able to detect. Credit: NASA’s Goddard Space Flight CenterAlt text: Narrated video introducing simulations of merging neutron star magnetospheresMusic: “A Theory Develops,” Pip Heywood [PRS], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || NS_Binary_Sim_Still.jpg (5760x3240) [1.4 MB] || NS_Binary_Sim_Still_searchweb.png (320x180) [67.6 KB] || NS_Binary_Sim_Still_thm.png (80x40) [5.2 KB] || 14884_NeutronStarBinarySim2_good.mp4 (1920x1080) [220.4 MB] || 14884_NeutronStarBinarySim2_best.mp4 (1920x1080) [363.9 MB] || NeutronStarBinarySimulationCaptions.en_US.srt [2.4 KB] || NeutronStarBinarySimulationCaptions.en_US.vtt [2.2 KB] || 14884_NeutronStarBinarySim2_ProRes_1920x1080_2997.mov (1920x1080) [1.7 GB] || ", "hits": 434 }, { "id": 14943, "url": "https://svs.gsfc.nasa.gov/14943/", "result_type": "Produced Video", "release_date": "2026-01-20T11:00:00-05:00", "title": "Far and Wide: Additional Graphics", "description": "This page houses animation clips from the Far and Wide video series, which may be useful in presentations or other video products. || ", "hits": 110 }, { "id": 14892, "url": "https://svs.gsfc.nasa.gov/14892/", "result_type": "Produced Video", "release_date": "2025-08-29T16:00:00-04:00", "title": "Solar Wind Animations", "description": "The Sun releases a constant stream of charged particles, called the solar wind. The solar wind originates in the outermost layer of the Sun’s atmosphere, the corona, when plasma is heated to a point that the Sun’s gravity can’t hold it down. When this plasma escapes – often reaching speeds of over one million miles per hour – it drags the Sun’s magnetic out across the solar system. When the solar wind encounters Earth, it is deflected by our planet's magnetic shield, causing most of the solar wind's energetic particles to flow around and beyond us. However, some of these high-energy particles can sneak past Earth’s natural magnetic defenses and produce hazardous conditions for satellites and astronauts, as well as power grids and infrastructure on Earth.Learn more about the solar wind: https://science.nasa.gov/sun/what-is-the-solar-wind/ || ", "hits": 896 }, { "id": 5535, "url": "https://svs.gsfc.nasa.gov/5535/", "result_type": "Visualization", "release_date": "2025-08-15T09:05:00-04:00", "title": "What Apollo Saw in Sunlight While in Orbit", "description": "A map showing the sunlit parts of the lunar surface that the Apollo astronauts could see from orbit. The darkened parts of the map were either never in sunlight or were beyond the horizon of the spacecraft.", "hits": 5410 }, { "id": 5394, "url": "https://svs.gsfc.nasa.gov/5394/", "result_type": "Visualization", "release_date": "2024-11-27T00:00:00-05:00", "title": "How much does the Gulf of Mexico Contribute to the Gulf Stream?", "description": "Animation 1: Lagrangian particles colored by temperature viewed from above with fixed camera. || GM_experiment22_2024-11-01_1336_final_flatT.01638_print.jpg (1024x576) [232.7 KB] || GM_experiment22_2024-11-01_1336_final_flatT.01638_searchweb.png (320x180) [103.9 KB] || GM_experiment22_2024-11-01_1336_final_flatT.01638_thm.png (80x40) [6.5 KB] || GM_experiment_flatT_1080p30.mp4 (1920x1080) [58.9 MB] || flatT [0 Item(s)] || GM_experiment22_final_flatT.mp4 (3840x2160) [196.8 MB] || GM_experiment22_final_flatT.mp4.hwshow [193 bytes] || ", "hits": 174 }, { "id": 5344, "url": "https://svs.gsfc.nasa.gov/5344/", "result_type": "Visualization", "release_date": "2024-10-15T14:00:00-04:00", "title": "Solar Cycle 25 - the Solar Magnetic Field from Solar Minimum to Pole Flip", "description": "One advantage of long-lived missions like Solar Dynamics Observatory (SDO) is the ability to see slow but significant changes over long periods of time.This view from SDO's Helioseismic and Magnetic Imager (HMI) shows the evolution of sunspots on the solar disk starting from solar minimum (around December 2019) and into the maximum solar activity phase. The video ends in September 2024, however this maximum phase is expected to continue into 2025.", "hits": 561 }, { "id": 14700, "url": "https://svs.gsfc.nasa.gov/14700/", "result_type": "Produced Video", "release_date": "2024-10-08T10:00:00-04:00", "title": "NASA + The Smithsonian: Biodiversity", "description": "Biodiverse ecosystems need protection. Through fieldwork, coordination with local partners, and satellite observations, NASA and the Smithsonian are working hard to protect them. Using NASA Earth science satellite and other data, the Goodall Institute puts imagery and data into the hands of local communities to drive conservation efforts. The Scimitar-horned oryx went from extinct in the wild to endangered in the wild thanks to the Smithsonian’s work with partners to re-introduce the species.", "hits": 72 }, { "id": 5298, "url": "https://svs.gsfc.nasa.gov/5298/", "result_type": "Visualization", "release_date": "2024-09-30T00:00:00-04:00", "title": "July mean Sargassum in the Atlantic: 2010 - 2023", "description": "This visualization shows the July mean Sargassum observed in the Atlantic Ocean by the MODIS instruments on NASA's TERRA and AQUA satellites from 2010 to 2023. Each square box of color represents an area 0.5 x 0.5 degrees, roughly 3025 square kilometers in size. The color represents the mean amount of Sargassum observed in that box during the month of July. Blue shades indicate that this area had on average less than 3 square kilomenters of Sargassum, while red indicates that the region had an average of 9 square kilometers or more. || sargassum_v28_JulyMean_4k_2024-05-28_1650.01775_print.jpg (1024x576) [156.7 KB] || sargassum_v28_JulyMean_4k_2024-05-28_1650.01775_searchweb.png (320x180) [77.0 KB] || sargassum_v28_JulyMean_4k_2024-05-28_1650.01775_thm.png (80x40) [6.5 KB] || sargassum_v28_JulyMean_4k_2024-05-28_1650_30p_1080p30.mp4 (1920x1080) [6.4 MB] || sargassum_v28_JulyMean_4k_2024-05-28_1650_30p_2160p30.mp4 (3840x2160) [21.4 MB] || sargassum_v28_JulyMean_4k_2024-05-28_1650_2160p60.mp4 (3840x2160) [18.9 MB] || composite [0 Item(s)] || composite [0 Item(s)] || ", "hits": 134 }, { "id": 5299, "url": "https://svs.gsfc.nasa.gov/5299/", "result_type": "Visualization", "release_date": "2024-09-30T00:00:00-04:00", "title": "Monthly mean Sargassum in the Atlantic: Jan 2018 - Dec 2023", "description": "This visualization shows the monthly mean Sargassum observed in the Atlantic Ocean by the MODIS instruments on NASA's TERRA and AQUA satellites from January 2018 through December 2023. Each square box of color represents an area 0.5 x 0.5 degrees, roughly 3025 square kilometers in size. The color represents the mean amount of Sargassum observed in that box during the month of July. Blue shades indicate that this area had on average less than 3 square kilomenters of Sargassum, while red indicates that the region had an average of 9 square kilometers or more. || sargassum_v30_monthly_4k_2024-05-28_1632.02876_print.jpg (1024x576) [152.7 KB] || sargassum_v30_monthly_4k_2024-05-28_1632.02876_searchweb.png (320x180) [75.7 KB] || sargassum_v30_monthly_4k_2024-05-28_1632.02876_thm.png (80x40) [6.4 KB] || sargassum_v30_monthly_4k_2024-05-28_1632_p30_1080p30.mp4 (1920x1080) [10.8 MB] || composite [0 Item(s)] || composite [0 Item(s)] || sargassum_v30_monthly_4k_2024-05-28_1632_p30_2160p30.mp4 (3840x2160) [31.5 MB] || sargassum_v30_monthly_4k_2024-05-28_1632_2160p60.mp4 (3840x2160) [31.8 MB] || ", "hits": 44 }, { "id": 5300, "url": "https://svs.gsfc.nasa.gov/5300/", "result_type": "Visualization", "release_date": "2024-09-30T00:00:00-04:00", "title": "Winds over the Sargasso Sea: December 2009 - March 2010", "description": "This visualization of MERRA-2 surface winds over the Atlantic Ocean and Sargasso Sea shows some unusually strong westerly winds during the winter of 2009-2010. Here the slower winds are shown in blue while the faster winds are shown in shades of red. The blue oval shows the nominal area of the Sargasso Sea while the yellow rectangle marks the 20–40°N, 80–10°W geographic box. || sargassum_v24_winds_2024-05-29_1627.03090_print.jpg (1024x576) [365.2 KB] || sargassum_v24_winds_2024-05-29_1627.03090_searchweb.png (320x180) [130.0 KB] || sargassum_v24_winds_2024-05-29_1627.03090_thm.png (80x40) [7.8 KB] || sargassum_v24_winds_2024-05-29_1627_p30_1080p30.mp4 (1920x1080) [297.3 MB] || composite [0 Item(s)] || composite [0 Item(s)] || sargassum_v24_winds_2024-05-29_1627_p30_2160p30.mp4 (3840x2160) [682.8 MB] || sargassum_v24_winds_2024-05-29_1627_2160p60.mp4 (3840x2160) [770.7 MB] || ", "hits": 56 }, { "id": 5301, "url": "https://svs.gsfc.nasa.gov/5301/", "result_type": "Visualization", "release_date": "2024-09-30T00:00:00-04:00", "title": "Atlantic Ocean Surface Drift Patterns from the Caribbean in 2010 and 2011", "description": "Simulated particle backtrack with windage and timelineThis visualization shows simulated particles released during 2010 and 2011 traced back in time to show their path based on the ocean surface velocities from Global HYCOM model with 1% windage applied. Simulated particles were released between December through April and tracked back in time. The gold balls under the timeline indicate the months when particles were released. Flow lines represent the movement of a particle over a 20-day period. Particles that venture above the 23 degree north latitude line (shown in red) during their lifespan are colored gold while particles that stayed south of it are colored green. || sargassum_rev3_v54_w_Timeline_w_wind_2024-08-14_1619.02999_print.jpg (1024x576) [193.3 KB] || sargassum_rev3_v54_w_Timeline_w_wind_2024-08-14_1619.02999_searchweb.png (320x180) [76.7 KB] || sargassum_rev3_v54_w_Timeline_w_wind_2024-08-14_1619.02999_thm.png (80x40) [6.2 KB] || sargassum_rev3_v54_w_Timeline_w_wind_2024-08-14_1619_1080p60.mp4 (1920x1080) [52.6 MB] || sargassum_rev3_v54_w_Timeline_w_wind_2024-08-14_1619_p30_1080p30.mp4 (1920x1080) [54.0 MB] || composite_wWind [0 Item(s)] || composite_wWind [0 Item(s)] || sargassum_rev3_v54_w_Timeline_w_wind_2024-08-14_1619_2160p60.mp4 (3840x2160) [151.2 MB] || sargassum_rev3_v54_w_Timeline_w_wind_2024-08-14_1619_p30_2160p30.mp4 (3840x2160) [158.8 MB] || sargassum_rev3_v54_w_Timeline_w_wind_2024-08-14_1619_2160p60.mp4.hwshow [226 bytes] || ", "hits": 43 }, { "id": 5213, "url": "https://svs.gsfc.nasa.gov/5213/", "result_type": "Visualization", "release_date": "2024-08-14T15:00:00-04:00", "title": "Changes in the Atmosphere and Ocean During a Transition From La Niña to El Niño", "description": "This is the final version of the ENSO visualization with narration. There are HD and 4k versions available as mp4s. There is also a high quality 4k version which is very large (3.8 Gbytes). Other non-narrated formats including individual frames are available below this entry.This movie is also available on youtube here:https://youtu.be/jK20dl3g9R8?si=38LHf1e0iIzrfhRQlink || ENSO_99_final_4k.01200_print.jpg (1024x576) [82.0 KB] || ENSO_Locked_Final_1080.mp4 (1920x1080) [155.7 MB] || ENSO_Final_Audio.en_US.srt [8.6 KB] || ENSO_Final_Audio.en_US.vtt [8.7 KB] || ENSO_Locked_Final_2160.mp4 (3840x2160) [184.8 MB] || ENSO_Locked_Final_2160_HIGH_QUAL.mp4 (3840x2160) [3.7 GB] || ENSO_Locked_Final_2160.mp4.hwshow [188 bytes] || ", "hits": 292 }, { "id": 5238, "url": "https://svs.gsfc.nasa.gov/5238/", "result_type": "Visualization", "release_date": "2024-06-27T11:00:00-04:00", "title": "Our Active Ionosphere", "description": "In this view of Earth on October 7, 2019, just past sunset, GOLD observed an X-shaped structure in the equatorial ionization anomaly. || GOLD_O5S_20191007.00034_print.jpg (1024x576) [76.3 KB] || GOLD_O5S_20191007 [0 Item(s)] || GOLD_O5S_20191007_1080p4.mp4 (1920x1080) [1.8 MB] || ", "hits": 154 }, { "id": 14507, "url": "https://svs.gsfc.nasa.gov/14507/", "result_type": "Produced Video", "release_date": "2024-04-18T08:40:00-04:00", "title": "NASA Joins the Jane Goodall Institute to Conserve Chimpanzee Habitat, Earth Information Center Videos", "description": "After years of forest loss, chimpanzee habitats are recovering. This is, in part, due to a collaboration between NASA and the Jane Goodall Institute (JGI). Using NASA Earth science satellite and other data, the Goodall Institute puts data into the hands of local communities to drive conservation across Africa’s equatorial forest belt.", "hits": 57 }, { "id": 14542, "url": "https://svs.gsfc.nasa.gov/14542/", "result_type": "Produced Video", "release_date": "2024-03-05T10:00:00-05:00", "title": "EZIE – Electrojet Zeeman Imaging Explorer", "description": "Slated to launch in 2025, NASA’s Electrojet Zeeman Imaging Explorer (EZIE) will be the first mission to image the magnetic fingerprint of the auroral electrojets — intense electric currents flowing high above Earth’s poles that are central to the electrical circuit coupling the planet’s magnetosphere to its atmosphere.Led by the Johns Hopkins Applied Physics Laboratory (APL), EZIE will use a trio of small satellites to characterize and record the electrojets’ structure over space and time. It will fill gaps in our understanding of this space weather phenomenon and provide findings that scientists can apply to other magnetized planets, both within and outside our solar system.Learn more:https://science.nasa.gov/mission/ezie/ || ", "hits": 99 }, { "id": 31232, "url": "https://svs.gsfc.nasa.gov/31232/", "result_type": "Hyperwall Visual", "release_date": "2024-02-26T00:00:00-05:00", "title": "Sea Surface Height Anomaly, 2022-2024", "description": "Animation of Sea Surface Height Anomaly in the Pacific starting January 1, 2022. || nrt_global_allsat_phy_l4_20240207_print.jpg (1024x576) [184.6 KB] || nrt_global_allsat_phy_l4_20240207_searchweb.png (320x180) [63.1 KB] || nrt_global_allsat_phy_l4_20240207_thm.png (80x40) [13.1 KB] || nrt_global_allsat_phy_l4_20220101-20240207_1080p30.mp4 (1920x1080) [35.8 MB] || nrt_global_allsat_phy_l4_20220101-20240207_1080p30.webm (1920x1080) [3.1 MB] || nrt_global_allsat_phy_l4 (3840x2160) [0 Item(s)] || nrt_global_allsat_phy_l4_20220101-20240207_2160p30.mp4 (3840x2160) [91.4 MB] || nrt_global_allsat_phy_l4_20240207.tif (3840x2160) [4.2 MB] || nrt_global_allsat_phy_l4_2022-2024.hwshow [133 bytes] || ", "hits": 248 }, { "id": 14410, "url": "https://svs.gsfc.nasa.gov/14410/", "result_type": "Produced Video", "release_date": "2023-09-13T10:00:00-04:00", "title": "NASA Joins Jane Goodall to Conserve Chimp Habitats", "description": "Complete transcript available. || Jane_Goodall_fullvideo_FINAL.00001_print.jpg (1024x576) [225.0 KB] || Jane_Goodall_fullvideo_FINAL.00001_searchweb.png (320x180) [123.8 KB] || Jane_Goodall_fullvideo_FINAL.00001_web.png (320x180) [123.8 KB] || Jane_Goodall_fullvideo_FINAL.00001_thm.png (80x40) [8.1 KB] || Jane_Goodall_fullvideo_FINAL.en_US.srt [10.7 KB] || Jane_Goodall_fullvideo_FINAL.en_US.vtt [10.2 KB] || Jane_Goodall_fullvideo_FINAL.mp4 (3840x2160) [4.3 GB] || ", "hits": 37 }, { "id": 5112, "url": "https://svs.gsfc.nasa.gov/5112/", "result_type": "Visualization", "release_date": "2023-07-12T11:00:00-04:00", "title": "Landsat Next Planned Orbits and Swath Coverage (version 2)", "description": "Lansdat Next trio of satellites orbiting and revealing data. It takes Landsat Next 6 days to get full coverage of the earth (aside from areas near the poles). This visualization shows two full cycles of coverage. || landsat_next.048.02000_print.jpg (1024x576) [68.5 KB] || landsat_next.048.02000_searchweb.png (320x180) [38.0 KB] || landsat_next.048.02000_thm.png (80x40) [3.6 KB] || landsat_next.048_1080p59.94.mp4 (1920x1080) [29.2 MB] || landsat_next.048_2160p59.94.mp4 (3840x2160) [84.5 MB] || landsat_next_hyperwall_preview.mp4 (2400x810) [35.4 MB] || landsat_next (3840x2160) [256.0 KB] || landsat_next (9600x3240) [256.0 KB] || ", "hits": 73 }, { "id": 14362, "url": "https://svs.gsfc.nasa.gov/14362/", "result_type": "Produced Video", "release_date": "2023-06-13T12:00:00-04:00", "title": "High Above Down Under Series", "description": "Around a different star, Earth may never have developed life at all. So what makes a star friendly to life? We joined two rocket teams as they traveled to the remote Northern Territory of Australia to capture light from our closest stellar neighbors to help reveal the answer. Follow their journey in the 6-part video series High Above Down Under. Episodes released weekly starting June 27, 2023. || ", "hits": 91 }, { "id": 14326, "url": "https://svs.gsfc.nasa.gov/14326/", "result_type": "Produced Video", "release_date": "2023-06-10T09:55:00-04:00", "title": "Hubble’s Inside The Image: Eta Carinae", "description": "The Hubble Space Telescope has taken over 1.5 million observations over the years. One of them is the breathtaking image of Eta Carinae.Eta Carinae was the site of a giant outburst about 150 years ago, when it became one of the brightest stars in the southern sky. Though the star released as much visible light as a supernova explosion, it survived the outburst. Somehow, the explosion produced two polar lobes and a large thin equatorial disk, all moving outward at about 1.5 million miles per hour.In this video, Dr. Keith Noll explains this breathtaking image and explains how important Hubble is to exploring the mysteries of the universe.For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Producer & Director: James LeighEditor: Lucy LundDirector of Photography: James BallAdditional Editing & Photography: Matthew DuncanExecutive Producers: James Leigh & Matthew DuncanProduction & Post: Origin Films Music Credit:\"Transcode\" by Lee Groves [PRS], and Peter George Marett [PRS] via Universal Production Music“Night Call” by Timothy Paul Handels [SABAM] via Pedigree Cuts [PRS] and Universal Production Music || ", "hits": 37 }, { "id": 5003, "url": "https://svs.gsfc.nasa.gov/5003/", "result_type": "Visualization", "release_date": "2022-12-21T00:00:00-05:00", "title": "Landsat Next Planned Orbits and Swath Coverage", "description": "Landsat Next observatories viewed from near the equator || landsat_next_equatorialView_withElapsed.01968_print.jpg (1024x576) [51.0 KB] || landsat_next_equatorialView_withElapsed_1080p59.94.mp4 (1920x1080) [17.0 MB] || landsat_next_equatorialView_withoutDates_1080p59.94.mp4 (1920x1080) [14.0 MB] || landsat_next_equatorialView_withoutDates_1080p59.94.webm (1920x1080) [6.2 MB] || landsat_next_equatorialView_withElapsed_1080p59.94.webm (1920x1080) [6.8 MB] || landsat_next_equatorialView_withoutDates_2160p59.94.mp4 (3840x2160) [39.1 MB] || landsat_next_equatorialView_withElapsed_2160p59.94.mp4 (3840x2160) [53.4 MB] || without_dates (3840x2160) [256.0 KB] || with_elapsed (3840x2160) [256.0 KB] || ", "hits": 44 }, { "id": 5019, "url": "https://svs.gsfc.nasa.gov/5019/", "result_type": "Visualization", "release_date": "2022-10-14T11:00:00-04:00", "title": "PACE orbit with swaths and instrument fields of view", "description": "PACE orbiting the Earth showing OCI, HARP2, and SPEXone instument fields of view followed by instrument ground swath patterns || pace_orbit_swath.42_FINAL_HD.09000_print.jpg (1024x576) [110.6 KB] || pace_orbit_swath.42_FINAL_HD.09000.png (1920x1080) [10.1 MB] || pace_orbit_swath.42_FINAL_HD.09000_searchweb.png (320x180) [72.6 KB] || pace_orbit_swath.42_FINAL_HD.09000_thm.png (80x40) [4.6 KB] || pace_orbit_swath.42_FINAL_HD_1080p59.94.mp4 (1920x1080) [70.0 MB] || 1920x1080_16x9_60p (1920x1080) [0 Item(s)] || pace_orbit_swath.42_FINAL_HD_1080p59.94.webm (1920x1080) [20.3 MB] || 3840x2160_16x9_60p (3840x2160) [0 Item(s)] || 9600x3240_16x9_30p (9600x3240) [0 Item(s)] || pace_orbit_swath.42_FINAL_4K_2160p59.94.mp4 (3840x2160) [269.9 MB] || ", "hits": 131 }, { "id": 14164, "url": "https://svs.gsfc.nasa.gov/14164/", "result_type": "Produced Video", "release_date": "2022-06-07T19:00:00-04:00", "title": "Australia Sounding Rocket Campaign Press Kit", "description": "NASA will launch three suborbital sounding rockets in June and July 2022 from the Arnhem Space Center in Australia’s Northern Territory to conduct astrophysics studies that can only be done from the Southern Hemisphere. The three missions will focus on α Centauri A and B, two of the three-star α Centauri system that are the closest stars to our Sun, and X-rays emanating from the interstellar medium, clouds of gases and particles between stars.The three sounding rocket night-time missions will be launched between June 26 and July 12 on two-stage Black Brant IX sounding rockets, from the Arnhem Space Center, which is owned and operated by Equatorial Launch Australia or ELA. The Arnhem Space Center is a commercial space launch facility, located on the Dhupuma Plateau near Nhulunbuy. The NASA missions will be the first launches from Arnhem.Learn more: Australia Sounding Rocket Fact SheetWatch more: Sounding Rockets: Cutting Edge Science, 15 Minutes at a TimeWhat Is a Sounding Rocket?Riding Along with a NASA Sounding Rocket || ", "hits": 69 }, { "id": 4983, "url": "https://svs.gsfc.nasa.gov/4983/", "result_type": "Visualization", "release_date": "2022-04-11T12:00:00-04:00", "title": "Global Carbon Dioxide 2020-2021 for Hyperwalls", "description": "This webpage provides a wide aspect ratio version of: Global Carbon Dioxide 2020-2021, released on November 2, 2021. This version has been created for wide aspect ratio display systems with resolution up to 9600x3240. It is recommended to use content from this version for display systems with 16:9 aspect ratio. || ", "hits": 72 }, { "id": 4917, "url": "https://svs.gsfc.nasa.gov/4917/", "result_type": "Visualization", "release_date": "2021-11-29T11:00:00-05:00", "title": "ICON Snaps a Peek at the Ionospheric Dynamo", "description": "Visualization of ICON in Earth orbit, camera ahead of the spacecraft looking back on spacecraft and limb of Earth. Magenta curves are lines of Earth's geomagnetic field. Field-of-view (FOV) of MIGHTI imagers (green frustums) and the longitudinal wind vectors (green arrows) it measures are shown. MIGHTI imagers FOV eventually fades out. Vertical plasma speed (red arrows) is measured at the spacecraft. Magnetic field lines turn yellow as measurements of winds by MIGHT provide a connection to influence the plasma velocity measured at the spacecraft, redirecting the plasma flow from upward to downward. || ICONDataView.ICONSyncView+x_.clockSlate_CRTT.HD1080i.000750_print.jpg (1024x576) [135.0 KB] || ICONDataView.ICONSyncView+x_.clockSlate_CRTT.HD1080i.000750_searchweb.png (320x180) [79.4 KB] || ICONDataView.ICONSyncView+x_.clockSlate_CRTT.HD1080i.000750_thm.png (80x40) [5.7 KB] || ICONSyncView+x (1920x1080) [0 Item(s)] || ICONDataView.ICONSyncView+x.HD1080i_p30.mp4 (1920x1080) [36.4 MB] || ICONDataView.ICONSyncView+x.HD1080i_p30.webm (1920x1080) [5.1 MB] || ICONSyncView+x (3840x2160) [0 Item(s)] || ICONDataView.ICONSyncView+x.2160p30.mp4 (3840x2160) [114.3 MB] || ICONDataView.ICONSyncView+x.HD1080i_p30.mp4.hwshow || ", "hits": 52 }, { "id": 14015, "url": "https://svs.gsfc.nasa.gov/14015/", "result_type": "Produced Video", "release_date": "2021-11-19T09:00:00-05:00", "title": "Terra Orbital Drift Video", "description": "\"From Small Beginnings,\" by Jay Price [PRS]; Universal Production Music || 14015_4938_TerraDrift_FINAL.02577_print.jpg (1024x576) [113.6 KB] || 14015_4938_TerraDrift_FINAL.02577_searchweb.png (320x180) [53.9 KB] || 14015_4938_TerraDrift_FINAL.02577_thm.png (80x40) [5.2 KB] || 14015_4938_TerraDrift_FINAL.mov (1920x1080) [2.8 GB] || 14015_4938_TerraDrift_FINAL_lowres.mp4 (1280x720) [39.6 MB] || 14015_YOUTUBE_1080_4938_TerraDrift_FINAL_youtube_1080.mp4 (1920x1080) [181.1 MB] || 4938_TerraDrift_FINAL.webm (960x540) [41.8 MB] || 14015_FACEBOOK_720_4938_TerraDrift_FINAL_facebook_720.mp4 (1280x720) [153.7 MB] || 14015_YOUTUBE_4K_4938_TerraDrift_FINAL_youtube_4k.mp4 (3840x2160) [899.2 MB] || 14015_4938_TerraDrift_FINAL.en_US.srt [2.8 KB] || 14015_4938_TerraDrift_FINAL.en_US.vtt [2.7 KB] || ", "hits": 138 }, { "id": 4949, "url": "https://svs.gsfc.nasa.gov/4949/", "result_type": "Visualization", "release_date": "2021-11-02T00:00:00-04:00", "title": "Global Carbon Dioxide 2020-2021", "description": "Data visualization featuring volumetric carbon dioxide on a global scale for the period June 1, 2020 - July 31, 2021.Coming soon to our YouTube channel. || CO2Volumetric_1024x576_02582_print.jpg (1024x576) [90.6 KB] || CO2Volumetric_1024x576_02582.png (1024x576) [569.1 KB] || CO2Volumetric_1024x576_02582_searchweb.png (180x320) [60.0 KB] || CO2Volumetric_1024x576_02582_thm.png (80x40) [5.1 KB] || CO2Volumetric_1920x1080p30.mp4 (1920x1080) [65.3 MB] || CO2Volumetric_1920x1080p30.webm (1920x1080) [13.3 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || CO2Volumetric_3840x2160_30fps_02582.exr (3840x2160) [63.3 MB] || CO2Volumetric_3840x2160_30fps_02582.tif (3840x2160) [44.5 MB] || captions_silent.31831.en_US.srt [43 bytes] || CO2Volumetric_3840x2160p30.mp4 (3840x2160) [931.2 MB] || ", "hits": 114 }, { "id": 20347, "url": "https://svs.gsfc.nasa.gov/20347/", "result_type": "Animation", "release_date": "2021-09-28T00:00:00-04:00", "title": "Fast and Slow Solar Wind", "description": "These animations show how Earth’s magnetosphere responds as it encounters the slow and fast solar wind.The solar wind is a plasma made of ions and electrons that have escaped the Sun. The solar wind streams outwards in all directions, filling the spaces between the planets and carrying with it the Sun’s magnetic field. When the solar wind reaches Earth’s magnetosphere, the region of space surrounding our planet where Earth’s magnetic field is dominant, the magnetosphere can respond differently depending on the speed of the solar wind, as demonstrated here. || ", "hits": 318 }, { "id": 4938, "url": "https://svs.gsfc.nasa.gov/4938/", "result_type": "Visualization", "release_date": "2021-09-24T15:00:00-04:00", "title": "Terra Orbit Drift", "description": "This visualization illustrates the milestones of Terra’s drift in orbit and showcases its impacts to shadow length and swath width from the change in crossing time. || terra_orbit_drift_comp_4685_print.jpg (1024x576) [115.6 KB] || terra_orbit_drift_comp_4685_searchweb.png (320x180) [55.9 KB] || terra_orbit_drift_comp_4685_thm.png (80x40) [5.5 KB] || terra_orbit_drift_comp_1080p60.mp4 (1920x1080) [20.0 MB] || terra_orbit_drift_comp_1080p60.webm (1920x1080) [9.5 MB] || terra_orbit_drift_comp (3840x2160) [512.0 KB] || terra_orbit_drift_comp_2160p60.mp4 (3840x2160) [56.9 MB] || ", "hits": 136 }, { "id": 4914, "url": "https://svs.gsfc.nasa.gov/4914/", "result_type": "Visualization", "release_date": "2021-09-01T00:00:00-04:00", "title": "Impact of Climate Change on Global Wheat Yields", "description": "Data visualization of predicted Wheat yields through the end of this centaury based on an ensemble of crop and climate models. || WheatMapFuture.01000_print.jpg (1024x576) [123.1 KB] || WheatMapFuture.01000_searchweb.png (320x180) [54.6 KB] || WheatMapFuture.01000_web.png (320x180) [54.6 KB] || WheatMapFuture.01000_thm.png (80x40) [5.4 KB] || WheatMapFuture_1080p.mp4 (1920x1080) [21.7 MB] || WheatMapFuture.mp4 (3840x2160) [79.7 MB] || WheatMapFuture.webm (3840x2160) [6.4 MB] ||", "hits": 132 }, { "id": 4929, "url": "https://svs.gsfc.nasa.gov/4929/", "result_type": "Visualization", "release_date": "2021-08-30T14:00:00-04:00", "title": "Comparing Atomic Oxygen Emission Observed by GOLD with Ionospheric Total Electron Content (TEC)", "description": "At 23:00UTC on November 19, 2018, we see the maxima of TEC values (red dots) closely aligned with the maxima of OI 135.6nm emission (black dots) || GOLD_TEC_anomalies_inset.00034_print.jpg (1024x576) [121.4 KB] || ", "hits": 33 }, { "id": 13715, "url": "https://svs.gsfc.nasa.gov/13715/", "result_type": "Produced Video", "release_date": "2020-09-15T13:00:00-04:00", "title": "How To Track The Solar Cycle", "description": "A new solar cycle comes roughly every 11 years. Over the course of each cycle, the Sun transitions from relatively calm to active and stormy, and then quiet again; at its peak, the Sun’s magnetic poles flip. Now that the star has passed solar minimum, scientists expect the Sun will grow increasingly active in the months and years to come.Understanding the Sun’s behavior is an important part of life in our solar system. The Sun’s outbursts—including eruptions known as solar flares and coronal mass ejections—can disturb the satellites and communications signals traveling around Earth, or one day, Artemis astronauts exploring distant worlds. Scientists study the solar cycle so we can better predict solar activity. As of 2020, the Sun has begun to shake off the sleep of minimum, which occurred in December 2019, and Solar Cycle 25 is underway. Scientists use several indicators to track solar cycle progress. || ", "hits": 246 }, { "id": 13687, "url": "https://svs.gsfc.nasa.gov/13687/", "result_type": "Produced Video", "release_date": "2020-08-14T10:00:00-04:00", "title": "NASA Spacecraft Uncover Mystery Behind Auroral Beads", "description": "A special type of aurora, draped east-west across the night sky like a glowing pearl necklace, is helping scientists better understand the science of auroras and their powerful drivers out in space. Known as auroral beads, these lights often show up just before large auroral displays, which are caused by electrical storms in space called substorms. Until now, scientists weren’t sure if auroral beads are somehow connected to other auroral displays as a phenomenon in space that precedes substorms, or if they are caused by disturbances closer to Earth’s atmosphere.But powerful new computer models, combined with observations from NASA’s Time History of Events and Macroscale Interactions during Substorms – THEMIS – mission, have provided the first direct evidence of the events in space that lead to the appearance of these beads, and demonstrated the important role they play in our local space environment. || ", "hits": 80 }, { "id": 13664, "url": "https://svs.gsfc.nasa.gov/13664/", "result_type": "Produced Video", "release_date": "2020-07-16T08:00:00-04:00", "title": "ESA and NASA Release First Images From Solar Orbiter Mission", "description": "Scientists from ESA (European Space Agency) and NASA will present the first images captured by Solar Orbiter, the joint ESA/NASA mission to study the Sun, during an online news briefing at 8 a.m. EDT Thursday, July 16. Launched on Feb. 9, 2020, Solar Orbiter turned on all 10 of its instruments together for the first time in mid-June as it made its first close pass of the Sun. The flyby captured the closest images ever taken of the Sun. During the briefing, mission experts will discuss what these closeup images reveal about our star, including what we can learn from Solar Orbiter’s new measurements of particles and magnetic fields flowing from the Sun.The briefing will stream live at:https://www.nasa.gov/solarorbiterfirstlight/Participants in the call include:•Daniel Müller – Solar Orbiter Project Scientist at ESA•Holly R. Gilbert – Solar Orbiter Project Scientist at NASA•José Luis Pellón Bailón – Solar Orbiter Deputy Spacecraft Operations Manager at ESA•David Berghmans – Principal investigator of the Extreme Ultraviolet Imager (EUI) at the Royal Observatory of Belgium•Sami Solanki – Principal investigator of the Polarimetric and Helioseismic Imager (PHI) and director of the Max Planck Institute for Solar System Research•Christopher J. Owen – Principal investigator of the Solar Wind Analyser (SWA) at Mullard Space Science Laboratory, University College London•ESA’s first light images•ESA press release •NASA feature story || ", "hits": 208 }, { "id": 13635, "url": "https://svs.gsfc.nasa.gov/13635/", "result_type": "Produced Video", "release_date": "2020-06-30T10:50:00-04:00", "title": "NASA’s TESS Provides New Insights Into an Ultrahot World", "description": "Explore KELT-9 b, one of the hottest planets known. Observations from NASA's Transiting Exoplanet Survey Satellite (TESS) have revealed new details about the planet’s environment. The planet follows a close, polar orbit around a squashed star with different surface temperatures, factors that make peculiar seasons for KELT-9 b. Credit: NASA's Goddard Space Flight CenterMusic: \"Migrating Species\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Kelt9b_Still.jpg (1920x1080) [711.8 KB] || Kelt9b_Still_searchweb.png (320x180) [77.8 KB] || Kelt9b_Still_thm.png (80x40) [6.0 KB] || 13635_KELT-9b_1080.mp4 (1920x1080) [146.6 MB] || 13635_KELT-9b_Best_1080.mp4 (1920x1080) [418.4 MB] || 13635_KELT-9b_ProRes_1920x1080_2997.mov (1920x1080) [1.9 GB] || 13635_KELT-9b_1080.webm (1920x1080) [15.9 MB] || 13635_KELT-9b_SRT_Captions.en_US.srt [2.7 KB] || 13635_KELT-9b_SRT_Captions.en_US.vtt [2.7 KB] || ", "hits": 111 }, { "id": 4782, "url": "https://svs.gsfc.nasa.gov/4782/", "result_type": "Visualization", "release_date": "2020-03-04T00:00:00-05:00", "title": "Vegetation Index Anomalies and Rift Valley fever (RVF) outbreaks in South Africa region: 2008-2011", "description": "This visualization with corresponding data dashboard shows the relationship between vegetation index anomalies and outbreaks of Rift Valley fever (RVF) during 2008 and 2011 in the South Africa region. The sequence starts in 2007 looking at the entire continent of Africa and zooms in the region of South Africa to take a closer look at the patterns between ENSO events (El Niño and La Niña), above normal vegetaion over land (green) and RVF outbreak locations (orange pins). || NDVI_RVF_SAfrica_Composite_3840x2160_2657_print.jpg (1024x576) [102.7 KB] || NDVI_RVF_SAfrica_Composite_3840x2160_2657_searchweb.png (320x180) [57.8 KB] || NDVI_RVF_SAfrica_Composite_3840x2160_2657_thm.png (80x40) [5.0 KB] || NDVI_RVF_SAfrica_Composite_1920x1080p30.mp4 (1920x1080) [35.6 MB] || NDVI_RVF_SAfrica_Composite_1920x1080p30.webm (1920x1080) [7.1 MB] || Composite (3840x2160) [0 Item(s)] || Composite (3840x2160) [0 Item(s)] || NDVI_RVF_SAfrica_Composite_3840x2160_p30.mp4 (3840x2160) [72.6 MB] || NDVI_RVF_SAfrica_Composite_3840x2160_2657.tif (3840x2160) [31.6 MB] || ", "hits": 38 }, { "id": 4783, "url": "https://svs.gsfc.nasa.gov/4783/", "result_type": "Visualization", "release_date": "2020-02-27T00:00:00-05:00", "title": "Precipitation Anomaly and Rift Valley fever (RVF) outbreaks in South Africa: 2008-2011", "description": "This visualization with corresponding data dashboard shows the relationship between precipitation anomalies and outbreaks of Rift Valley fever (RVF) during 2008 and 2011 in the South Africa region. The sequence starts in 2007 looking at the entire continent of Africa and zooms in the region of South Africa to take a closer look at the patterns between ENSO events (El Niño and La Niña), above normal precipitation over land (blue) and RVF outbreak locations (orange pins). || PrecipRVF_SAfrica_Composite_3840x2160_3422_print.jpg (1024x576) [97.8 KB] || PrecipRVF_SAfrica_Composite_3840x2160_3422_searchweb.png (320x180) [57.6 KB] || PrecipRVF_SAfrica_Composite_3840x2160_3422_thm.png (80x40) [5.2 KB] || PrecipRVF_SAfrica_Composite_1920x1080p30.mp4 (1920x1080) [31.5 MB] || Composite (3840x2160) [0 Item(s)] || Composite (3840x2160) [0 Item(s)] || PrecipRVF_SAfrica_Composite_3840x2160_p30.mp4 (3840x2160) [68.2 MB] || PrecipRVF_SAfrica_Composite_3840x2160_3422.tif (3840x2160) [4.0 MB] || PrecipRVF_SAfrica_Composite_3840x2160_p30.webm (3840x2160) [14.1 MB] || ", "hits": 26 }, { "id": 4795, "url": "https://svs.gsfc.nasa.gov/4795/", "result_type": "Animation", "release_date": "2020-02-26T16:00:00-05:00", "title": "OSIRIS-REx – Global Model of Asteroid Bennu", "description": "Looping animation of asteroid Bennu rotating. This 3D model of Bennu was created using 20cm resolution laser altimetry data and imagery taken by OSIRIS-REx. || Bennu_spin_full_20cm.1000_print.jpg (1024x576) [82.7 KB] || Bennu_spin_full_20cm.1000_searchweb.png (320x180) [17.4 KB] || Bennu_spin_full_20cm.1000_thm.png (80x40) [1.5 KB] || Bennu_spin_full_20cm_1080p30.webm (1920x1080) [14.4 MB] || Bennu_spin_full_20cm_1080p30.mp4 (1920x1080) [111.9 MB] || Bennu_GlobalSpin_20cm (3840x2160) [0 Item(s)] || Bennu_spin_full_20cm_2160p30.mp4 (3840x2160) [351.8 MB] || 4771_20cm_Bennu_Global_Spin.mov (3840x2160) [8.1 GB] || Bennu_spin_full_20cm_1080p30.mp4.hwshow [194 bytes] || ", "hits": 100 }, { "id": 4724, "url": "https://svs.gsfc.nasa.gov/4724/", "result_type": "Visualization", "release_date": "2020-02-21T00:00:00-05:00", "title": "Vegetation index anomalies and Rift Valley fever (RVF) outbreaks in Africa and Middle East during 2000-2018", "description": "Data visualization featuring vegetation index anomalies over Africa and Middle East and locations of Rift Valley Fever (RVF) outbreaks (orange pins) during the period of 2000-2018. Frames are provided in 4K resolution. || Africa_NDVIRVF_2000_2018_3840x2160_2430_print.jpg (1024x576) [78.8 KB] || Africa_NDVIRVF_2000_2018_3840x2160_2430_searchweb.png (320x180) [48.8 KB] || Africa_NDVIRVF_2000_2018_3840x2160_2430_thm.png (80x40) [4.4 KB] || Africa_NDVIRVFComposite_2000_2018_3840x2160_1080p30.mp4 (1920x1080) [88.7 MB] || Africa_NDVIRVFComposite_2000_2018_3840x2160_1080p30.webm (1920x1080) [25.5 MB] || Africa_NDVIRVF_2000_2018_Composite (3840x2160) [0 Item(s)] || Africa_NDVIRVF_2000_2018_3840x2160_2430.tif (3840x2160) [6.0 MB] || Africa_NDVIRVFComposite_2000_2018_3840x2160_p30.mp4 (3840x2160) [283.2 MB] || ", "hits": 37 }, { "id": 4747, "url": "https://svs.gsfc.nasa.gov/4747/", "result_type": "Visualization", "release_date": "2020-02-21T00:00:00-05:00", "title": "Vegetation index anomalies and Rift Valley fever (RVF) outbreaks in South Africa during 2009-2011", "description": "This visualization shows the relationship between vegetation index anomalies (Normalized Difference Vegetation Index - NDVI) data and outbreak locations of Rift Valley fever (RVf) during 2008 and 2011. The sequence starts in 2007 looking at the entire continent of Africa and zooms in the region of South Africa slowly to take a closer look at the above normal vegetation (green) and RVF outbreak locations (orange pins). Frames are provided in 4K resolution. || SAfrica_NDVIRVFwDates_3840x2160_1263_print.jpg (1024x576) [86.2 KB] || SAfrica_NDVIRVFwDates_3840x2160_1263_searchweb.png (320x180) [56.0 KB] || SAfrica_NDVIRVFwDates_3840x2160_1263_thm.png (80x40) [4.5 KB] || SAfrica_NDVIRVFComposite_1080p30.mp4 (1920x1080) [31.6 MB] || SAfrica_NDVIRVFComposite_1080p30.webm (1920x1080) [7.0 MB] || Composite (3840x2160) [0 Item(s)] || SAfrica_NDVIRVFwDates_3840x2160_1263.tif (3840x2160) [7.6 MB] || SAfrica_NDVIRVFComposite_3840x2160_p30.mp4 (3840x2160) [96.4 MB] || ", "hits": 35 }, { "id": 4784, "url": "https://svs.gsfc.nasa.gov/4784/", "result_type": "Visualization", "release_date": "2020-02-21T00:00:00-05:00", "title": "ENSO Teleconnections and Rift Valley fever (RVF) Outbreaks", "description": "During the 2008-2011 period, ENSO events brought changes to weather conditions across the globe that triggered infectious disease outbreaks, such as mosquito-borne Rift Valley fever (RVF) in South Africa. This visualization with corresponding data dashboard shows how Sea Surface Temperature (SST) anomalies in the equatorial Pacific Ocean (left) gave rise to Precipitation (center) and Vegetation (right) Index Anomalies in South Africa. During La Niña events, Southern Africa receives persistent and above normal rainfall, which floods habitats of RVF mosquito vectors triggering hatching of RVF virus infected eggs. The above-normal rainfall is followed by an increase in vegetation creating appropriate habitats for the mosquito vectors setting the stage for RVF outbreak activity, which in simple terms means an uptick in mosquito populations that cause infections of domestic livestock and human populations with the RVF virus. However, in rare cases there is a departure from this canonical response, as we can observe in 2009-2010, when a mild El Niño event resulted in above normal vegetaton and a large RVF outbreak in South Africa. || ENSO_TeleconnectionsRVF_2008_2011_3840x2160_2960_print.jpg (1024x576) [107.8 KB] || ENSO_TeleconnectionsRVF_2008_2011_3840x2160_3525_searchweb.png (320x180) [63.0 KB] || ENSO_TeleconnectionsRVF_2008_2011_3840x2160_3525_thm.png (80x40) [6.5 KB] || ENSO_Teleconnections (1920x1080) [0 Item(s)] || SST_Precip_NDVI_Dashboard_2008_2011_1920x1080_p30.mp4 (1920x1080) [22.7 MB] || ENSO_Teleconnections (3840x2160) [0 Item(s)] || ENSO_Teleconnections (3840x2160) [0 Item(s)] || ENSO_TeleconnectionsRVF_2008_2011_3840x2160_p30.mp4 (3840x2160) [56.0 MB] || ENSO_TeleconnectionsRVF_2008_2011_3840x2160_p30.webm (3840x2160) [10.2 MB] || ENSO_TeleconnectionsRVF_2008_2011_3840x2160_2960.tif (3840x2160) [3.4 MB] || ENSO_TeleconnectionsRVF_2008_2011_3840x2160_3525.tif (3840x2160) [3.4 MB] || ", "hits": 32 }, { "id": 4788, "url": "https://svs.gsfc.nasa.gov/4788/", "result_type": "Visualization", "release_date": "2020-02-04T12:00:00-05:00", "title": "The Solar Polar Magnetic Field", "description": "From our single vantage point of Earth, our view of the Sun is never complete. While the far-side of the Sun eventually rotates into view, coverage of the Sun's polar regions is never satisfactory as perspective effects either completely block our view or create a distorted view. We must often resort to computer modeling of these solar polar regions.This visualization presents the Potential Field Source Surface (PFSS) magnetic field model based on solar observations covering the years 2017-2019. One version also presents the 'hole' in our measurements of the solar polar region. The region oscillates in size over the course of the year due to the changing perspective created by the tilt of Earth's orbital plane with the solar equator. In this region, researchers must resort to approximations to build a more complete view of the solar magnetic field.Why is the solar magnetic field in this region important? Because the combined with the outgoing flow of the solar wind, the magnetic field lines from the polar regions curve up, and then back down to near the Sun's equatorial plane, which is still fairly close to the orbital plane of Earth and other planets in our solar system. This gives the Sun's polar magnetic field a significant influence on the space weather impacting Earth and crewed and uncrewed assets around the solar system. || ", "hits": 56 }, { "id": 4785, "url": "https://svs.gsfc.nasa.gov/4785/", "result_type": "Visualization", "release_date": "2020-01-09T00:00:00-05:00", "title": "Sea Surface Temperature Anomalies and Patterns of Global Disease Outbreaks: 2009-2018 (4K version)", "description": "This webpage provides the 4K version of: Sea Surface Temperature anomalies and patterns of Global Disease Outbreaks: 2009-2018 (updated), released on January 6, 2020.Content has been created for 4K display systems that can handle finer resolution and details. It is recommended to use content from this version for HD (1920x1080) and lower resolutions. || ", "hits": 69 }, { "id": 4781, "url": "https://svs.gsfc.nasa.gov/4781/", "result_type": "Visualization", "release_date": "2020-01-06T00:00:00-05:00", "title": "Sea Surface Temperature anomalies and patterns of Global Disease Outbreaks: 2009-2018 (updated)", "description": "This visualization shows the variability in global sea surface temperature anomalies, the associated ENSO index timeline and locations of infectious disease outbreaks over the global land surface. || CompositeWLabel_2009_2018_1920x108060fps_1705_print.jpg (1024x576) [135.9 KB] || CompositeWLabel_2009_2018_1920x108060fps_1705_searchweb.png (320x180) [82.6 KB] || CompositeWLabel_2009_2018_1920x108060fps_1705_thm.png (80x40) [7.1 KB] || Composite_StrongElNino (1920x1080) [0 Item(s)] || Composite_StrongElNino (1920x1080) [0 Item(s)] || CompositeWLabel_2009_2018_1920x1080_p30.mp4 (1920x1080) [22.1 MB] || CompositeWLabel_2009_2018_1920x108060fps_1705.tif (1920x1080) [1.3 MB] || CompositeWLabel_2009_2018_1920x1080_p30.webm (1920x1080) [4.6 MB] || CompositeWLabel_2009_2018_1920x1080_p30.mp4.hwshow [205 bytes] || ", "hits": 83 }, { "id": 4771, "url": "https://svs.gsfc.nasa.gov/4771/", "result_type": "Animation", "release_date": "2019-12-12T13:15:00-05:00", "title": "OSIRIS-REx – Asteroid Bennu Sample Site Flyovers", "description": "Global view of asteroid Bennu with insets of the four candidate sample collection sites. This animation is available in Hyperwall resolution (5760x3240).This video is also available on our YouTube channel. || bennu_sites_agu_4k_04_0750_print.jpg (1024x576) [155.8 KB] || bennu_sites_agu_4k_04_0750_searchweb.png (320x180) [64.4 KB] || bennu_sites_agu_4k_04_0750_thm.png (80x40) [5.1 KB] || bennu_sites_1080p30.mp4 (1920x1080) [82.9 MB] || bennu_sites_1080p30.webm (1920x1080) [9.3 MB] || Bennu_SampleSites (5760x3240) [0 Item(s)] || Bennu_SampleSites (3840x2160) [0 Item(s)] || captions_silent.28627.en_US.srt [43 bytes] || bennu_sites_2160p30.mp4 (3840x2160) [218.3 MB] || 4771_Bennu_Sites_3D_Clean.mov (3840x2160) [4.9 GB] || bennu_sites_1080p30.mp4.hwshow [185 bytes] || ", "hits": 83 }, { "id": 4765, "url": "https://svs.gsfc.nasa.gov/4765/", "result_type": "Visualization", "release_date": "2019-12-10T00:00:00-05:00", "title": "Sea Surface Temperature anomalies and patterns of Global Disease Outbreaks: 2009-2018", "description": "El Niño is an irregularly recurring climate pattern characterized by warmer than usual ocean temperatures in the equatorial Pacific, which creates a ripple effect of anticipated weather changes in far-spread regions. This visualization captures monthly Sea Surface Temperature (SST) anomalies around the world from 2009-2018, along with locations of global disease outbreaks and a corresponding timeline showcasing the Niño 3.4 Index. The Niño 3.4 Index represents average equatorial sea surface temperatures in the Pacific Ocean from about the International Date Line to the coast of South America. Highlighted in the timeline are the above average El Niño years, in which sea surface temperature anomalies peaked during 2015-2016. || SSTENSO_Diseases_Comp_2009_2018_1920x1080_0769_print.jpg (1024x576) [130.6 KB] || SSTENSO_Diseases_Comp_2009_2018_1920x1080_0769_searchweb.png (320x180) [79.7 KB] || SSTENSO_Diseases_Comp_2009_2018_1920x1080_0769_thm.png (80x40) [7.0 KB] || Composite (1920x1080) [0 Item(s)] || Composite (1920x1080) [0 Item(s)] || SSTENSO_Diseases_Comp_2009_2018_1920x1080_p30.mp4 (1920x1080) [23.0 MB] || SSTENSO_Diseases_Comp_2009_2018_1920x1080_0769.tif (1920x1080) [1.3 MB] || SSTENSO_Diseases_Comp_2009_2018_1920x1080_p30.webm (1920x1080) [4.7 MB] || SSTENSO_Diseases_Comp_2009_2018_1920x1080_p30.mp4.hwshow [211 bytes] || ", "hits": 106 }, { "id": 40388, "url": "https://svs.gsfc.nasa.gov/gallery/nasaearth-science/", "result_type": "Gallery", "release_date": "2019-09-13T10:53:37-04:00", "title": "NASA Earth Science", "description": "NASA’s Earth Science Division (ESD) missions help us to understand our planet’s interconnected systems, from a global scale down to minute processes. Working in concert with a satellite network of international partners, ESD can measure precipitation around the world, and it can employ its own constellation of small satellites to look into the eye of a hurricane. ESD technology can track dust storms across continents and mosquito habitats across cities.\n\nFor more information:\nhttps://science.nasa.gov/earth-science", "hits": 209 }, { "id": 4720, "url": "https://svs.gsfc.nasa.gov/4720/", "result_type": "Visualization", "release_date": "2019-09-06T10:00:00-04:00", "title": "CGI Moon Kit", "description": "These color and elevation maps are designed for use in 3D rendering software. They are created from data assembled by the Lunar Reconnaissance Orbiter camera and laser altimeter instrument teams.", "hits": 42712 }, { "id": 4744, "url": "https://svs.gsfc.nasa.gov/4744/", "result_type": "Animation", "release_date": "2019-08-12T14:00:00-04:00", "title": "OSIRIS-REx - Asteroid Bennu Sample Site Finalists", "description": "The visualization begins with a rotating 3D model representation of the asteroid Bennu, created using data from the OSIRIS-REx Laser Altimeter (OLA) instrument. Four candidate sample sites (with labels) are highlighted with PolyCam images.Watch this video on the NASA Goddard YouTube channel. || bennu_callouts_05_labels_4k_60fps_1349_print.jpg (1024x576) [149.3 KB] || bennu_callouts_05_labels_4k_60fps_1349_thm.png (80x40) [5.6 KB] || bennu_callouts_05_labels_4k_60fps_1349_print_searchweb.png (320x180) [56.8 KB] || bennu_callouts_05_labels_4k_60fps_1080p60.mp4 (1920x1080) [30.4 MB] || bennu_callouts_05_labels_4k_60fps_1080p60.webm (1920x1080) [4.3 MB] || Bennu_SampleSiteCallouts_wLabels (3840x2160) [0 Item(s)] || bennu_callouts_05_labels_4k_60fps_2160p30.mp4 (3840x2160) [70.5 MB] || 4744_Bennu_4_Sites_Output.en_US.srt [47 bytes] || 4744_Bennu_4_Sites_Output.en_US.vtt [60 bytes] || 4744_Bennu_4_Candidate_Sites.mov (3840x2160) [3.1 GB] || bennu_callouts.hwshow [68 bytes] || ", "hits": 45 }, { "id": 4737, "url": "https://svs.gsfc.nasa.gov/4737/", "result_type": "Visualization", "release_date": "2019-07-17T11:00:00-04:00", "title": "Observing Earth's Ionosphere with GOLD", "description": "A visualization of GOLD data observing Earth's ionosphere in ultraviolet light around the wavelength of an atomic oxygen emission. || GOLDData201903.GOLDview_O5S.clockSlate_CRTT.UHD3840.000267_print.jpg (1024x576) [70.4 KB] || GOLD_March2019_animated.gif (1042x586) [5.5 MB] || GOLDData201903.GOLDview_O5S.clockSlate_CRTT.UHD3840.000267_searchweb.png (320x180) [72.3 KB] || GOLDData201903.GOLDview_O5S.clockSlate_CRTT.UHD3840.000267_thm.png (80x40) [5.4 KB] || GOLDData201903.GOLDview_O5S.HD1080i_p10.mp4 (1920x1080) [24.0 MB] || basic (1920x1080) [0 Item(s)] || GOLDData201903.GOLDview_O5S.HD1080i_p10.webm (1920x1080) [3.1 MB] || basic (3840x2160) [0 Item(s)] || GOLDData201903.GOLDview_O5S_2160p10.mp4 (3840x2160) [72.0 MB] || ", "hits": 45 }, { "id": 13188, "url": "https://svs.gsfc.nasa.gov/13188/", "result_type": "Produced Video", "release_date": "2019-04-19T11:00:00-04:00", "title": "Earth from Orbit 2019: How NASA Satellites #PictureEarth", "description": "Music: After the Sun by Andrew Michael Britton [PRS], David Stephen Goldsmith [PRS], Andrew Skeet [PRS]Complete transcript available. || Still_print.jpg (1024x574) [166.3 KB] || Still.png (3022x1696) [8.0 MB] || Still_searchweb.png (320x180) [119.3 KB] || Still_thm.png (80x40) [7.5 KB] || 13188_Earth_From_Orbit_2019_Final_Text.webm (960x540) [49.7 MB] || FACEBOOK_720_13188_Earth_From_Orbit_2019_Final_Text_facebook_720.mp4 (1280x720) [139.2 MB] || YOUTUBE_1080_13188_Earth_From_Orbit_2019_Final_Text_youtube_1080.mp4 (1920x1080) [193.3 MB] || 13188_Earth_From_Orbit_2019_Final_Text.en_US.srt [1.2 KB] || 13188_Earth_From_Orbit_2019_Final_Text.en_US.vtt [1.2 KB] || ", "hits": 98 }, { "id": 13152, "url": "https://svs.gsfc.nasa.gov/13152/", "result_type": "Produced Video", "release_date": "2019-02-28T12:30:00-05:00", "title": "2015-2016 El Niño Triggered Disease Outbreaks Across the Globe", "description": "Music: Under Offer by Peter Keith Yelland-BrownComplete transcript available. || ENSO_Dengue_Thumbnail.png (1920x1080) [3.2 MB] || ENSO_Dengue_Thumbnail_print.jpg (1024x576) [143.5 KB] || ENSO_Dengue_Thumbnail_searchweb.png (320x180) [88.1 KB] || ENSO_Dengue_Thumbnail_thm.png (80x40) [6.2 KB] || ENSO_Dengue_FINAL_lowres.mp4 (1280x720) [39.4 MB] || ENSO_Dengue_FINAL_lowres.webm (1280x720) [16.2 MB] || ENSO_Dengue_Captions.en_US.srt [2.6 KB] || ENSO_Dengue_Captions.en_US.vtt [2.6 KB] || ENSO_Dengue_FINAL.mov (1920x1080) [3.9 GB] || ", "hits": 62 }, { "id": 4695, "url": "https://svs.gsfc.nasa.gov/4695/", "result_type": "Visualization", "release_date": "2019-02-28T09:00:00-05:00", "title": "Niño 3.4 Index and Sea Surface Temperature Anomaly Timeline: 1982-2017", "description": "This visualization captures Sea Surface Temperature (SST) anomalies around the world from 1982 to 2017, along with a corresponding timeplot graph focusing on the Niño 3.4 SST Index region (5N-5S, 120W-170W), which represents average equatorial sea surface temperatures in the Pacific Ocean from about the International Date Line to the coast of South America. Highlighted in the timeline are the El Niño years, in which sea surface temperature anomalies peaked: 1982-1983, 1997-1998, and 2015-2016. || NINO3.4SST_FlatMapComposite_1920x1080_00932_print.jpg (1024x576) [104.9 KB] || NINO3.4SST_FlatMapComposite_1920x1080_00932_searchweb.png (320x180) [72.1 KB] || NINO3.4SST_FlatMapComposite_1920x1080_00932_thm.png (80x40) [6.8 KB] || SST_Nino3.4Index_1982_2017_Composite (1920x1080) [0 Item(s)] || NINO3.4SST_FlatMapComposite_1920x1080_p30.mp4 (1920x1080) [57.2 MB] || NINO3.4SST_FlatMapComposite_1920x1080_00932.tif (1920x1080) [1.4 MB] || NINO3.4SST_FlatMapComposite_1920x1080_p30.webm (1920x1080) [9.3 MB] || SSTNino3.4Index_1982_2017_Composite (3840x2160) [0 Item(s)] || ", "hits": 351 }, { "id": 4697, "url": "https://svs.gsfc.nasa.gov/4697/", "result_type": "Visualization", "release_date": "2019-02-28T09:00:00-05:00", "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] || SST_Precip_LST_Plot_Composite (1920x1080) [0 Item(s)] || 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] || TeleconnectionsSEAsia (3840x2160) [0 Item(s)] || SST_LST_Precip_2014_2016_Comp_1080p30.mp4.hwshow [203 bytes] || ", "hits": 80 }, { "id": 20287, "url": "https://svs.gsfc.nasa.gov/20287/", "result_type": "Animation", "release_date": "2018-11-30T09:00:00-05:00", "title": "OSIRIS-REx Mission Design: Site Selection Campaign", "description": "Baseball Diamond Left || Shot19_422.00001_print.jpg (1024x576) [82.5 KB] || Shot19_422.00001_searchweb.png (320x180) [67.6 KB] || Shot19_422.00001_thm.png (80x40) [4.5 KB] || Shot19_h264.mov (3840x2160) [47.1 MB] || Shot19 (3840x2160) [64.0 KB] || Shot19_422.webm (3840x2160) [4.4 MB] || Shot19_422.mov (3840x2160) [1.3 GB] || ", "hits": 26 }, { "id": 30978, "url": "https://svs.gsfc.nasa.gov/30978/", "result_type": "Hyperwall Visual", "release_date": "2018-07-20T00:00:00-04:00", "title": "Seeing Titan with Infrared Eyes", "description": "Six infrared views of Saturn's moon Titan. || titan_infrared_eyes_PIA21923_print.jpg (1024x576) [89.4 KB] || titan_infrared_eyes_PIA21923.png (5760x3240) [9.4 MB] || titan_infrared_eyes_PIA21923_searchweb.png (320x180) [65.1 KB] || titan_infrared_eyes_PIA21923_thm.png (80x40) [6.1 KB] || titan_infrared_eyes_PIA21923.hwshow [218 bytes] || ", "hits": 102 }, { "id": 30975, "url": "https://svs.gsfc.nasa.gov/30975/", "result_type": "Hyperwall Visual", "release_date": "2018-07-12T00:00:00-04:00", "title": "Sea Surface Height Anomaly, 2014-2016", "description": "Animation of Sea Surface Height Anomaly in the Pacific for 2014 through 2016. || duacs_rep_global_merged_allsat_phy_20161231_adj_color_print.jpg (1024x576) [98.3 KB] || duacs_rep_global_merged_allsat_phy_20161231_adj_color_searchweb.png (320x180) [55.8 KB] || duacs_rep_global_merged_allsat_phy_20161231_adj_color_thm.png (80x40) [5.0 KB] || duacs_rep_global_merged_allsat_phy_2014-2016_libx264_1080p.mp4 (1920x1080) [32.2 MB] || duacs_rep_global_merged_allsat_phy_2014-2016_libx264_720p.mp4 (1280x720) [20.3 MB] || duacs_rep_global_merged_allsat_phy_2014-2016_libx264_720p.webm (1280x720) [4.6 MB] || duacs_rep_global_merged_allsat_phy_2014-2016_libx264_2160p.mp4 (3840x2160) [69.1 MB] || duacs_rep_global_merged_allsat_phy_20161231_adj_color.tif (3840x2160) [6.8 MB] || ", "hits": 28 }, { "id": 12718, "url": "https://svs.gsfc.nasa.gov/12718/", "result_type": "Produced Video", "release_date": "2018-04-16T12:00:00-04:00", "title": "Tracking El Niño", "description": "Follow changes in sea surface temperature and ocean currents during El Niño. || GMAO_elNino_oceanTemperatureAnomaly_currents__0191_1024x576.jpg (1024x576) [115.4 KB] || GMAO_elNino_oceanTemperatureAnomaly_currents__0191_1920x1080.jpg (1920x1080) [360.7 KB] || GMAO_elNino_oceanTemperatureAnomaly_currents__0191_searchweb.png (320x180) [78.9 KB] || GMAO_elNino_oceanTemperatureAnomaly_currents__0191_thm.png (80x40) [6.2 KB] || GMAO_elNino_oceanTemperatureAnomaly_currents__0191.tif (3840x2160) [23.7 MB] || ", "hits": 120 }, { "id": 40346, "url": "https://svs.gsfc.nasa.gov/gallery/icon/", "result_type": "Gallery", "release_date": "2018-03-27T00:00:00-04:00", "title": "ICON", "description": "The Ionospheric Connection Explorer, or ICON, is a low-Earth orbiting satellite that will give us new information about how Earth’s atmosphere interacts with near-Earth space — a give-and-take that plays a major role in the safety of our satellites and reliability of communications signals. \n\nSpecifically, ICON investigates the connections between the neutral atmosphere — which extends from near Earth’s surface to far above us, at the edge of space— and the electrically charged part of the atmosphere, called the ionosphere. The particles of the ionosphere carry electrical charge that can disrupt communications signals, cause satellites in low-Earth orbit to become electrically charged, and, in extreme cases, cause power outages on the ground.", "hits": 144 }, { "id": 4617, "url": "https://svs.gsfc.nasa.gov/4617/", "result_type": "Visualization", "release_date": "2018-01-31T14:00:00-05:00", "title": "Interface to Space: The Equatorial Fountain", "description": "Visualization illustrating the Fountain Effect of ions in the near-Earth electric and magnetic fields. || IRIConceptual.Limb2PullOut_OionFountainIGRF.noslate_CRTT.HD1080i.000660_print.jpg (1024x576) [114.5 KB] || IRIConceptual.Limb2PullOut_OionFountainIGRF.noslate_CRTT.HD1080i.000660_searchweb.png (320x180) [87.8 KB] || IRIConceptual.Limb2PullOut_OionFountainIGRF.noslate_CRTT.HD1080i.000660_thm.png (80x40) [7.2 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || IRIConceptual.Limb2PullOut_OionFountainIGRF.HD1080i_p30.mp4 (1920x1080) [32.1 MB] || IRIConceptual.Limb2PullOut_OionFountainIGRF.HD1080i_p30.webm (1920x1080) [4.2 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || IRIConceptual.Limb2PullOut_OionFountainIGRF_2160p30.mp4 (3840x2160) [96.1 MB] || IRIConceptual.Limb2PullOut_OionFountainIGRF.HD1080i_p30.mp4.hwshow [221 bytes] || ", "hits": 85 }, { "id": 4618, "url": "https://svs.gsfc.nasa.gov/4618/", "result_type": "Visualization", "release_date": "2018-01-31T00:00:00-05:00", "title": "Geostationary Operational Environmental Satellite (GOES) East and West", "description": "This animation depicts the areas of the Earth viewed by GOES-East and GOES-West from their vantage point 22,236 miles above the equator.This video is also available on our YouTube channel. || goes_EastWest.000945_print.jpg (1024x576) [50.9 KB] || goes_EastWest.000945_searchweb.png (320x180) [48.6 KB] || goes_EastWest.000945_thm.png (80x40) [2.9 KB] || goes_EastWest (1920x1080) [0 Item(s)] || goes_EastWest_1080p30.mp4 (1920x1080) [48.2 MB] || goes_EastWest_1080p30.webm (1920x1080) [6.5 MB] || goes_EastWest_1080p30.mp4.hwshow [187 bytes] || ", "hits": 179 }, { "id": 4601, "url": "https://svs.gsfc.nasa.gov/4601/", "result_type": "Visualization", "release_date": "2017-12-18T11:00:00-05:00", "title": "Jupiter Quasi-Quadrennial Oscillation", "description": "Climate patterns on Jupiter can have striking similarities to those on Earth, making the gas giant a natural laboratory for understanding planetary atmospheres. Complete transcript available.Watch this video on the NASA Goddard YouTube channel.Music provided by Killer Tracks: \"Lights,\" \"Times Waits,\" \"The Space Between\" || JupiterQQOpreview.jpg (1920x1080) [456.5 KB] || TWITTER_720_4601_Jupiter_QQO_Master_APR_twitter_720.mp4 (1280x720) [37.7 MB] || 4601_Jupiter_QQO_Master.webm (960x540) [72.7 MB] || FACEBOOK_720_4601_Jupiter_QQO_Master_APR_facebook_720.mp4 (1280x720) [218.0 MB] || YOUTUBE_HQ_4601_Jupiter_QQO_Master_APR_youtube_hq.mov (1920x1080) [875.9 MB] || 4601_Jupiter_QQO_Master_APR_Output.en_US.srt [3.8 KB] || 4601_Jupiter_QQO_Master_APR_Output.en_US.vtt [3.8 KB] || 4601_Jupiter_QQO_Master_APR.mov (1920x1080) [2.4 GB] || ", "hits": 58 }, { "id": 12777, "url": "https://svs.gsfc.nasa.gov/12777/", "result_type": "Produced Video", "release_date": "2017-11-13T13:00:00-05:00", "title": "Our Living Planet From Space", "description": "Life. It's the one thing that, so far, makes Earth unique among the thousands of other planets we've discovered. Since the fall of 1997, NASA satellites have continuously and globally observed all plant life at the surface of the land and ocean. Earth is still the only planet we know of with life - with that in mind, our habitable home world seems evermore fragile and beautiful when considering the vastness of unlivable space. || ", "hits": 106 }, { "id": 4594, "url": "https://svs.gsfc.nasa.gov/4594/", "result_type": "Visualization", "release_date": "2017-10-31T10:00:00-04:00", "title": "ICON Scans the Ionosphere", "description": "ICON orbits Earth at 575 kilometers altitude, measuring the composition and motions of the ionosphere. || IRIDaily.limbwICON_OionHwindIGRF.clockSlate_CRTT.HD1080i.000870_print.jpg (1024x576) [105.7 KB] || IRIDaily.limbwICON_OionHwindIGRF.clockSlate_CRTT.HD1080i.000870_searchweb.png (320x180) [63.8 KB] || IRIDaily.limbwICON_OionHwindIGRF.clockSlate_CRTT.HD1080i.000870_thm.png (80x40) [5.0 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || IRIDaily.limbwICON_OionHwindIGRF.HD1080i_p30.mp4 (1920x1080) [76.4 MB] || IRIDaily.limbwICON_OionHwindIGRF.HD1080i_p30.webm (1920x1080) [10.9 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || IRIDaily.limbwICON_OionHwindIGRF.UHD3840_2160p30.mp4 (3840x2160) [217.4 MB] || IRIDaily.limbwICON_OionHwindIGRF.HD1080i_p30.mp4.hwshow [210 bytes] || ", "hits": 102 }, { "id": 30907, "url": "https://svs.gsfc.nasa.gov/30907/", "result_type": "Hyperwall Visual", "release_date": "2017-10-03T00:00:00-04:00", "title": "Jupiter Storm of the High North", "description": "A storm on Jupiter || PIA21776_print.jpg (1024x1193) [247.1 KB] || PIA21776_searchweb.png (320x180) [87.9 KB] || PIA21776_thm.png (80x40) [5.9 KB] || PIA21776.tif (2119x2470) [11.9 MB] || -jupiter-storm-of-the-high-north.hwshow [208 bytes] || ", "hits": 45 }, { "id": 12732, "url": "https://svs.gsfc.nasa.gov/12732/", "result_type": "Produced Video", "release_date": "2017-09-25T00:00:00-04:00", "title": "Waves and Changes in Jupiter's Atmosphere", "description": "The movement of Jupiter’s clouds can be seen when comparing these two global maps, in which Jupiter’s cloud bands are laid out as a flat projection. Scientists produced these maps of Jupiter using Hubble Space Telescope observations for the Outer Planet Atmospheres Legacy program taken on January 19, 2015, from 2:00 UT to 12:30 UT and from 15:00 UT to 23:40 UT. In Jupiter’s North Equatorial Belt, Hubble imaged an elusive wave that had been spotted on the planet only once before, decades earlier, by Voyager 2. In Voyager’s images, the wave is barely visible, and nothing like it was seen again until the recent Hubble observations. In the Hubble images, the wave appears as nearly vertical lines passing through the top of the dark, central cloud belt. The wave was found traveling in a region dotted with cyclones and anticyclones. Similar waves—called baroclinic waves—sometimes appear in Earth’s atmosphere where cyclones are forming. The wave may originate in a clear layer beneath the clouds, only becoming visible when it propagates up into the cloud deck. || JupiterBlink6.00001_print.jpg (1024x576) [109.1 KB] || JupiterBlink6.00001_searchweb.png (320x180) [86.8 KB] || JupiterBlink6.00001_thm.png (80x40) [5.5 KB] || JupiterBlink6.mp4 (1920x1080) [14.7 MB] || JupiterBlink6.webm (1920x1080) [840.9 KB] || ", "hits": 63 }, { "id": 11937, "url": "https://svs.gsfc.nasa.gov/11937/", "result_type": "Produced Video", "release_date": "2017-07-20T08:00:00-04:00", "title": "Earth's Energy Budget", "description": "Earth's energy budget is a metaphor for the delicate equilibrium between energy received from the Sun versus energy radiated back out in to space. Research into precise details of Earth's energy budget is vital for understanding how the planet's climate may be changing, as well as variabilities in solar energy output. NASA’s (The Clouds and the Earth's Radiant Energy System) CERES and NASA's Total and Spectral solar Irradiance Sensor (TSIS-1), missions play key roles in our continued understanding of Earth’s Energy Budget.NASA’s TSIS helps scientists keep a close watch on the sun’s energy input to Earth. Various satellites have captured a continuous record of this solar energy input since 1978. TSIS-1 sensors advance previous measurements, enabling scientists to study the sun's natural influence on Earth's ozone layer, atmospheric circulation, clouds, and ecosystems. These observations are essential for a scientific understanding of the effects of solar variability on the Earth system. TSIS-1 makes two key measurements: total solar irradiance, or TSI, the sun's total energy input into Earth, and solar spectral irradiance (SSI), the distribution of the sun's energy input across ultraviolet, visible, and infrared wavelengths of light. TSI measurements are needed to quantify the solar variations in the total amount of energy input to the Earth. SSI measurements are also vital because different wavelengths of light are absorbed by different parts of the atmosphere.For more than 20 years, NASA Langley's CERES (System) instruments have measured the solar energy reflected by Earth, the heat the planet emits, and the role of clouds in that process. The final CERES Flight Model, CERES FM6 launched aboard NOAA’s JPSS-1 in Fall 2017. CERES FM6 contributes to an already extensive CERES dataset that helps scientists validate models that calculate the effect of clouds on planetary heating and cooling. The same data can also be helpful for improving near-term, seasonal forecasts influenced by weather events such as El Niño and La Niña. El Niño and La Niña are weather patterns that develop when ocean temperatures fluctuate between warm and cool phases in the Equatorial Pacific Ocean. Built by Northrop Grumman and managed by Langley, CERES FM6 joins five other CERES instruments orbiting the planet on three other satellites.NASA Goddard Space Flight Center manages the TSIS-1 project. The University of Colorado's Laboratory for Atmospheric and Space Physics (LASP) built both instruments and provides mission operations. The International Space Station carries TSIS-1.Earth's energy budget is a metaphor for the delicate equilibrium between energy received from the Sun versus energy radiated back out in to space. Research into precise details of Earth's energy budget is vital for understanding how the planet's climate may be changing, as well as variabilities in solar energy output. NASA’s (The Clouds and the Earth's Radiant Energy System) CERES and NASA's Total and Spectral solar Irradiance Sensor (TSIS-1), missions play key roles in our continued understanding of Earth’s Energy Budget.NASA’s TSIS helps scientists keep a close watch on the sun’s energy input to Earth. Various satellites have captured a continuous record of this solar energy input since 1978. TSIS-1 sensors advance previous measurements, enabling scientists to study the sun's natural influence on Earth's ozone layer, atmospheric circulation, clouds, and ecosystems. These observations are essential for a scientific understanding of the effects of solar variability on the Earth system. TSIS-1 makes two key measurements: total solar irradiance, or TSI, the sun's total energy input into Earth, and solar spectral irradiance (SSI), the distribution of the sun's energy input across ultraviolet, visible, and infrared wavelengths of light. TSI measurements are needed to quantify the solar variations in the total amount of energy input to the Earth. SSI measurements are also vital because different wavelengths of light are absorbed by different parts of the atmosphere.For more than 20 years, NASA Langley's CERES (System) instruments have measured the solar energy reflected by Earth, the heat the planet emits, and the role of clouds in that process. The final CERES Flight Model, CERES FM6 launched aboard NOAA’s JPSS-1 in Fall 2017. CERES FM6 contributes to an already extensive CERES dataset that helps scientists validate models that calculate the effect of clouds on planetary heating and cooling. The same data can also be helpful for improving near-term, seasonal forecasts influenced by weather events such as El Niño and La Niña. El Niño and La Niña are weather patterns that develop when ocean temperatures fluctuate between warm and cool phases in the Equatorial Pacific Ocean. Built by Northrop Grumman and managed by Langley, CERES FM6 joins five other CERES instruments orbiting the planet on three other satellites.NASA Goddard Space Flight Center manages the TSIS-1 project. The University of Colorado's Laboratory for Atmospheric and Space Physics (LASP) built both instruments and provides mission operations. The International Space Station carries TSIS-1. || ", "hits": 158 }, { "id": 40335, "url": "https://svs.gsfc.nasa.gov/gallery/interfaceto-space/", "result_type": "Gallery", "release_date": "2017-06-23T00:00:00-04:00", "title": "Interface to Space", "description": "The ionosphere is layer of the upper atmosphere (60-1000 km up) where the neutral atoms and molecules of the lower atmosphere transition to the plasma of space.", "hits": 99 }, { "id": 4544, "url": "https://svs.gsfc.nasa.gov/4544/", "result_type": "Visualization", "release_date": "2017-05-26T10:30:00-04:00", "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.webm (1920x1080) [163.5 KB] || with_colorbar (3840x2160) [256.0 KB] || GMAO_elNino_oceanTemperatureAnomaly_currents_1080p.mp4 (1920x1080) [159.4 MB] || GMAO_oceanTemperatureAnomaly_withColorbar.mp4 (3840x2160) [166.0 MB] || ", "hits": 64 }, { "id": 12601, "url": "https://svs.gsfc.nasa.gov/12601/", "result_type": "Produced Video", "release_date": "2017-05-26T10:30:00-04:00", "title": "A 3D Look at the 2015 El Niño", "description": "Scientists at NASA's Goddard Space Flight Center have combined ocean measurements with cutting-edge supercomputer simulations to analyze the 2015-2016 El Niño in three dimensions. This visualization looks at the top 225 meters of the ocean, showing warmer than normal water in red, colder than normal water in blue. In the second half, current information is included, with east-flowing currents in yellow and west-flowing currents in white.Music: Bourrée from Handel's Water MusicWatch this video on the NASA Goddard YouTube channel. || 12601-El-Nino-3D-print.jpg (3840x2160) [2.7 MB] || 12601-El-Nino-3D-print_searchweb.png (320x180) [93.3 KB] || 12601-El-Nino-3D-print_thm.png (80x40) [7.1 KB] || 12601-El-Nino-3D-UHD.mp4 (3840x2160) [381.6 MB] || 12601-El-Nino-3D-captions.en_US.srt [1.7 KB] || 12601-El-Nino-3D-captions.en_US.vtt [1.7 KB] || 12601-El-Nino-3D-UHD.webm (3840x2160) [24.9 MB] || ", "hits": 50 }, { "id": 4557, "url": "https://svs.gsfc.nasa.gov/4557/", "result_type": "Visualization", "release_date": "2017-03-15T10:00:00-04:00", "title": "Leaky Radiation Belts", "description": "This visualization opens with a full view of the radiation belt of trapped electrons circling Earth. We open a slice of the belts, to display a cross-section for clarity and move the camera to a more equatorial view. Earth rotation and solar motion have been turned off for this visualization to reduce distracting additional motions. || LeakyBelts_FullData_ObliqueIntro.slate_CRTT.HD1080i.0600_print.jpg (1024x576) [113.8 KB] || LeakyBelts_FullData_ObliqueIntro.slate_CRTT.HD1080i.0600_searchweb.png (180x320) [83.0 KB] || LeakyBelts_FullData_ObliqueIntro.slate_CRTT.HD1080i.0600_thm.png (80x40) [6.0 KB] || ObliqueIntro (1920x1080) [0 Item(s)] || LeakyBelts_FullData_ObliqueIntro.HD1080i_p30.mp4 (1920x1080) [77.0 MB] || LeakyBelts_FullData_ObliqueIntro.HD1080i_p30.webm (1920x1080) [5.5 MB] || ObliqueIntro (3840x2160) [0 Item(s)] || LeakyBelts_FullData_ObliqueIntro.UHD2160_p30.mp4 (3840x2160) [279.0 MB] || LeakyBelts_FullData_ObliqueIntro.HD1080i_p30.mp4.hwshow [210 bytes] || ", "hits": 106 }, { "id": 30855, "url": "https://svs.gsfc.nasa.gov/30855/", "result_type": "Hyperwall Visual", "release_date": "2017-02-27T15:00:00-05:00", "title": "The Sombrero Galaxy from Hubble", "description": "The majestic Sombrero Galaxy as observed by Hubble || sombrero-hst-c169-5760x3240_print.jpg (1024x576) [91.8 KB] || sombrero-hst-c169-5760x3240.png (5760x3240) [26.0 MB] || sombrero-hst-c169-5760x3240_searchweb.png (320x180) [66.7 KB] || sombrero-hst-c169-5760x3240_thm.png (80x40) [4.8 KB] || sombrero-hst-c169-30855.key [505.6 KB] || sombrero-hst-c169-30855.pptx [178.2 KB] || the-majestic-sombrero-galaxy-from-hubble-max.hwshow || ", "hits": 193 }, { "id": 4539, "url": "https://svs.gsfc.nasa.gov/4539/", "result_type": "Visualization", "release_date": "2017-01-13T10:00:00-05:00", "title": "Exploring Earth's Ionosphere: Limb view with approach", "description": "Oxygen ion enhancements at 350km altitude, ionospheric winds at altitudes of 100 km (white) and 350 km (violet) and the low-latitude geomagnetic field. || IRIDaily.zoom2limb_OionHwindIGRF.clockSlate_CRTT.HD1080i.000400_print.jpg (1024x576) [92.1 KB] || IRIDaily.zoom2limb_OionHwindIGRF.clockSlate_CRTT.HD1080i.000400_searchweb.png (320x180) [58.1 KB] || IRIDaily.zoom2limb_OionHwindIGRF.clockSlate_CRTT.HD1080i.000400_thm.png (80x40) [4.9 KB] || IRIDaily.zoom2limb_OionHwindIGRF.HD1080i_p30.mp4 (1920x1080) [89.8 MB] || OionHwindIGRF (1920x1080) [0 Item(s)] || IRIDaily.zoom2limb_OionHwindIGRF.HD1080i_p30.webm (1920x1080) [8.6 MB] || OionHwindIGRF (3840x2160) [0 Item(s)] || IRIDaily.zoom2limb_OionHwindIGRF.2160p30.mp4 (3840x2160) [274.0 MB] || IRIDaily.zoom2limb_OionHwindIGRF.HD1080i_p30.mp4.hwshow [210 bytes] || ", "hits": 78 }, { "id": 4540, "url": "https://svs.gsfc.nasa.gov/4540/", "result_type": "Visualization", "release_date": "2017-01-13T10:00:00-05:00", "title": "Exploring Earth's Ionosphere: Limb view", "description": "This visualization presents data on the concentration of the singly-ionized oxygen atom (rainbow color table, red is highest concentration), the low-latitude geomagnetic field (gold field lines) and the ionospheric winds at two altitude levels, 100km (white) and 350 km (violet). || IRIDaily.limb_OionHwindIGRF.clockSlate_CRTT.HD1080i.000750_print.jpg (1024x576) [101.4 KB] || IRIDaily.limb_OionHwindIGRF.clockSlate_CRTT.HD1080i.000750_thm.png (80x40) [5.0 KB] || IRIDaily.limb_OionHwindIGRF.clockSlate_CRTT.HD1080i.000750_searchweb.png (320x180) [62.5 KB] || IRIDaily.limb_OionHwindIGRF.HD1080i_p30.mp4 (1920x1080) [88.3 MB] || OionHwindIGRF (1920x1080) [0 Item(s)] || OionHwindIGRF (3840x2160) [0 Item(s)] || IRIDaily.limb_OionHwindIGRF.2160p30.webm (3840x2160) [12.4 MB] || IRIDaily.limb_OionHwindIGRF.2160p30.mp4 (3840x2160) [274.0 MB] || IRIDaily.limb_OionHwindIGRF.HD1080i_p30.mp4.hwshow [205 bytes] || ", "hits": 77 }, { "id": 12399, "url": "https://svs.gsfc.nasa.gov/12399/", "result_type": "Produced Video", "release_date": "2016-10-27T12:55:00-04:00", "title": "NASA's Kepler, Swift Missions Harvest ‘Pumpkin’ Stars", "description": "Dive into the Kepler field and learn more about the origins of these rapidly spinning stars.Credit: NASA's Goddard Space Flight CenterMusic: \"Electric Cosmos\" from Killer TracksWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || Pumpkin_Star_Still.png (1920x1080) [10.8 MB] || Pumpkin_Star_Still_print.jpg (1024x576) [85.7 KB] || Pumpkin_Star_Still_searchweb.png (320x180) [66.5 KB] || Pumpkin_Star_Still_thm.png (80x40) [4.4 KB] || 12399_Swift_Pumpkin_Star2_ProRes_1920x1080_2997.mov (1920x1080) [2.0 GB] || 12399_Swift_Pumpkin_Star_FINAL2_youtube_hq.mov (1920x1080) [1.2 GB] || 12399_Swift_Pumpkin_Star2_H264_1080.mov (1920x1080) [221.8 MB] || 12399_Swift_Pumpkin_Star2_1080_Good.m4v (1920x1080) [147.1 MB] || 12399_Swift_Pumpkin_Star2_1080_Most_Compatible.m4v (960x540) [59.7 MB] || 12399_Swift_Pumpkin_Star_FINAL2_HD.wmv (1920x1080) [332.6 MB] || 12399_Swift_Pumpkin_Star2_ProRes_1920x1080_2997.webm (1920x1080) [17.0 MB] || 12399_Swift_Pumpkin_Star_SRT_Captions.en_US.srt [2.3 KB] || 12399_Swift_Pumpkin_Star_SRT_Captions.en_US.vtt [2.3 KB] || 12399_Swift_Pumpkin_Star_FINAL2_ipod_sm.mp4 (320x240) [26.8 MB] || ", "hits": 103 }, { "id": 4482, "url": "https://svs.gsfc.nasa.gov/4482/", "result_type": "Animation", "release_date": "2016-10-04T00:00:00-04:00", "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. || ", "hits": 135 }, { "id": 12370, "url": "https://svs.gsfc.nasa.gov/12370/", "result_type": "Produced Video", "release_date": "2016-09-13T11:00:00-04:00", "title": "Return To Normal in 2016, After Strong El Niño in 2015", "description": "Scientists at the Global Modeling and Assimilation Office of NASA's Goddard Space Flight Center regulary produce a forecast of sea surface temperatures in the equatorial Pacific ocean. The temperatures in this area are used to determine the conditions known as El Niño and La Niña. For several months, the NASA forecast has indicated the temperatures will be neutral over the next nine months. This indicates there will be no La Niña in 2016-2017, after the previous year's very strong El Niño.Music: Find The Answer, by Klangraum. Composers: Bernhard Hering [GEMA], Matthias Kruger [GEMA]Complete transcript available. || 12370_La_Nada_2016_MASTER_large.00090_print.jpg (1024x576) [106.7 KB] || 12370_La_Nada_2016_MASTER_large.00090_searchweb.png (320x180) [66.2 KB] || 12370_La_Nada_2016_MASTER_large.00090_thm.png (80x40) [5.0 KB] || 12370_La_Nada_2016_MASTER_V2_prores.mov (1280x720) [970.6 MB] || 12370_La_Nada_2016_MASTER_V2_youtube_hq.mov (1280x720) [196.0 MB] || 12370_La_Nada_2016_MASTER_V2_large.mp4 (1280x720) [70.8 MB] || 12370_La_Nada_2016_MASTER_V2_appletv.m4v (1280x720) [33.1 MB] || 12370_La_Nada_2016_MASTER_V2_appletv_subtitles.m4v (1280x720) [33.1 MB] || 12370_La_Nada_2016-captions.en_US.srt [970 bytes] || 12370_La_Nada_2016-captions.en_US.vtt [983 bytes] || 12370_La_Nada_2016_MASTER_V2_ipod_sm.mp4 (320x240) [11.2 MB] || 12370_La_Nada_2016_MASTER_V2_prores.webm [0 bytes] || ", "hits": 46 }, { "id": 12367, "url": "https://svs.gsfc.nasa.gov/12367/", "result_type": "Produced Video", "release_date": "2016-09-08T11:00:00-04:00", "title": "Seeing Jupiter Up Close", "description": "NASA’s Juno spacecraft beams back new images of the solar system’s largest planet. || c-1024.jpg (1024x576) [103.3 KB] || c-1280.jpg (1280x720) [135.3 KB] || c-1024_print.jpg (1024x576) [107.0 KB] || c-1024_searchweb.png (320x180) [57.0 KB] || c-1024_web.png (320x180) [57.0 KB] || c-1024_thm.png (80x40) [5.0 KB] || ", "hits": 160 }, { "id": 12320, "url": "https://svs.gsfc.nasa.gov/12320/", "result_type": "Produced Video", "release_date": "2016-07-21T11:00:00-04:00", "title": "A Viking On Mars", "description": "July 20 marked the 40th anniversary of NASA’s historic first Mars landing. || c-1024.jpg (1024x576) [232.0 KB] || c-1280.jpg (1280x720) [307.8 KB] || c-1024_print.jpg (1024x576) [244.0 KB] || c-1024_searchweb.png (320x180) [93.4 KB] || c-1024_web.png (320x180) [93.4 KB] || c-1024_thm.png (80x40) [5.8 KB] || ", "hits": 83 }, { "id": 12199, "url": "https://svs.gsfc.nasa.gov/12199/", "result_type": "Produced Video", "release_date": "2016-05-12T14:00:00-04:00", "title": "Evolution of Pacific Ocean Temperatures", "description": "Every two to seven years, an unusually warm pool of water—sometimes two to three degrees Celsius higher than normal—develops across the eastern equatorial Pacific Ocean. This warm condition, known as El Niño, can disrupt marine ecosystems and spur extreme weather patterns around the world. To predict when an El Niño is coming, NASA scientists use computer models that simulate ocean temperatures in the Pacific. Changes in ocean temperatures typical of an El Niño occur on the sea surface and up to 1,000 feet deep. With inputs from ocean buoys, satellite data and other sources, the models show what ocean temperatures might look like months into the future. The information not only helps scientists estimate the strength of an El Niño, but also study its evolution. || ", "hits": 32 }, { "id": 12242, "url": "https://svs.gsfc.nasa.gov/12242/", "result_type": "Produced Video", "release_date": "2016-05-05T20:22:00-04:00", "title": "El Niño Evolution", "description": "Computer models help scientists see El Niño unfold in the Pacific. || c-1024.jpg (1024x576) [238.4 KB] || c-1280.jpg (1280x720) [351.4 KB] || c-1920.jpg (1920x1080) [605.7 KB] || c-1024_print.jpg (1024x576) [252.3 KB] || c-1024_searchweb.png (320x180) [100.5 KB] || c-1024_web.png (320x180) [100.5 KB] || c-1024_thm.png (80x40) [17.1 KB] || ", "hits": 98 }, { "id": 30766, "url": "https://svs.gsfc.nasa.gov/30766/", "result_type": "Hyperwall Visual", "release_date": "2016-04-18T08:00:00-04:00", "title": "El Niño Precipitation Anomaly", "description": "El Nino precipitation anomaly || from_hal_2_1080p.00001_print.jpg (1024x576) [320.6 KB] || from_hal_2_1080p.00001_searchweb.png (320x180) [131.9 KB] || from_hal_2_1080p.00001_thm.png (80x40) [8.2 KB] || el_nino_precip_anom_720p.webm (1280x720) [22.6 MB] || el_nino_precip_anom_360p.mp4 (640x360) [50.9 MB] || 4104x2304_16x9_30p (4104x2304) [256.0 KB] || el_nino_precip_anom_1080p.mp4 (1920x1080) [264.2 MB] || el_nino_precip_anom_720p.mp4 (1280x720) [149.1 MB] || el_nino_precip_anom_2304p.mp4 (4096x2304) [809.4 MB] || El_Nino_Precipitation_Anomaly_30766.key [182.5 MB] || El_Nino_Precipitation_Anomaly_30766.pptx [180.2 MB] || the-earth-observing-fleet-by-theme-precipitation.hwshow [1.2 KB] || ", "hits": 56 }, { "id": 12193, "url": "https://svs.gsfc.nasa.gov/12193/", "result_type": "Produced Video", "release_date": "2016-04-07T17:16:00-04:00", "title": "What's Next After El Niño?", "description": "Following a strong El Niño winter, scientists see Pacific Ocean temperatures return to normal. || NewCoverName-1024.jpg (1024x576) [371.3 KB] || NewCoverName-1024_print.jpg (1024x576) [378.7 KB] || NewCoverName-1024_searchweb.png (320x180) [92.3 KB] || NewCoverName-1024_web.png (320x180) [92.3 KB] || NewCoverName-1024_thm.png (80x40) [7.7 KB] || ", "hits": 16 }, { "id": 30762, "url": "https://svs.gsfc.nasa.gov/30762/", "result_type": "Hyperwall Visual", "release_date": "2016-03-25T00:00:00-04:00", "title": "Jason-3 Begins Mapping the Ocean", "description": "Launched on January 17, 2016, Jason-3 is a partnership that includes NOAA, NASA, CNES, and EUMETSAT. After launch, Jason-3 was maneuvered into orbit about 80 seconds behind Jason-2, where it collected data at essentially the same time and place. It will stay in this tandem orbit for about six months while scientists and engineers take a careful look at any differences between Jason-2 and Jason-3. The map shown here was generated using sea surface height measurements from the first 10 days (February 12-20, 2016) of data collected once Jason-3 reached its operational orbit of 830 miles (1336 kilometers). The map corresponds well to data from its predecessor, Jason-2. Higher-than-normal sea levels are red; lower-than-normal sea levels are blue. El Niño is visible as the red blob in the eastern equatorial Pacific. After that, Jason-2 will move to an interleaved orbit (ground tracks halfway between those of Jason-3) where the two missions collectively will provide double the observational coverage of the global ocean. Extending the timeline of ocean surface topography measurements begun by the Topex/Poseidon and Jason-1 and Jason-2 satellites; Jason-3 will make highly detailed measurements of sea-level on Earth to monitor climate change and track phenomena like El Niño. It will also enable more accurate weather, ocean, and climate forecasts, including helping global weather and environmental agencies more accurately forecast the strength of tropical cyclones. || ", "hits": 19 }, { "id": 30756, "url": "https://svs.gsfc.nasa.gov/30756/", "result_type": "Hyperwall Visual", "release_date": "2016-03-08T00:00:00-05:00", "title": "Sea Surface Height Anomaly", "description": "Sea Surface Height Anomaly during the 2015-2016 El Niño || aviso_ssha_20160101_print.jpg (1024x574) [113.0 KB] || aviso_ssha_20160101_searchweb.png (320x180) [54.8 KB] || aviso_ssha_20160101_thm.png (80x40) [4.8 KB] || aviso_ssha_2015-2016_1080p.mp4 (1920x1080) [20.8 MB] || aviso_ssha_2015-2016_720p.mp4 (1280x720) [13.5 MB] || aviso_ssha_2015-2016_720p.webm (1280x720) [6.0 MB] || aviso_ssha_20160101.tif (4104x2304) [4.9 MB] || aviso_ssha_2015-2016_2304p.mp4 (4096x2304) [18.2 MB] || ", "hits": 54 }, { "id": 4433, "url": "https://svs.gsfc.nasa.gov/4433/", "result_type": "Visualization", "release_date": "2016-02-25T20:00:00-05:00", "title": "El Niño: GMAO Daily Sea Surface Temperature Anomaly from 1997/1998 and 2015/2016", "description": "This visualization shows how the Sea Surface Temperature Anomaly (SSTA) data and subsurface Temperature Anomaly from the 1997 El Nino year compares to the 2015 El Nino year. The visualization shows how the 1997 event started from colder-than-average sea surface temperatures – but the 2015 event started with warmer-than-average temperatures not only in the Pacific but also in in the Atlantic and Indian Oceans.This video is also available on our YouTube channel. || SSTcompare1997_2015_0000_print.jpg (1024x576) [87.4 KB] || SSTcompare1997_2015_0000_searchweb.png (320x180) [53.0 KB] || SSTcompare1997_2015_0000_thm.png (80x40) [5.6 KB] || Compare1997_2015_SSTA.mp4 (1920x1080) [28.7 MB] || compare (1920x1080) [0 Item(s)] || Compare1997_2015_SSTA.webm (1920x1080) [1.5 MB] || Compare1997_2015_SSTA.m4v (640x360) [2.5 MB] || Compare1997_2015_SSTA.mp4.hwshow [187 bytes] || ", "hits": 85 }, { "id": 30753, "url": "https://svs.gsfc.nasa.gov/30753/", "result_type": "Hyperwall Visual", "release_date": "2016-02-18T03:00:00-05:00", "title": "Sea Surface Temperature Anomaly Time Series", "description": "Sea Surface Temperature Anomaly February 2015-February 2016 || ssta_flat_1080p_print.jpg (1024x576) [186.0 KB] || ssta_flat_1080p_searchweb.png (320x180) [112.3 KB] || ssta_flat_1080p_thm.png (80x40) [7.9 KB] || ssta_flat_1080p.mp4 (1920x1080) [43.3 MB] || ssta_flat_720p.mp4 (1280x720) [23.2 MB] || ssta_flat_720p.webm (1280x720) [5.5 MB] || ssta_flat_360p.mp4 (640x360) [7.7 MB] || flat (4104x2304) [0 Item(s)] || omniglobe (4104x2052) [0 Item(s)] || ssta_flat_2304p.mp4 (4096x2304) [140.8 MB] || ", "hits": 35 }, { "id": 12143, "url": "https://svs.gsfc.nasa.gov/12143/", "result_type": "Produced Video", "release_date": "2016-02-05T11:00:00-05:00", "title": "NASA On Air: NASA's Global Hawk Flies Over El Niño Storms (2/5/2016)", "description": "LEAD: This month government scientists are making special research flights into and over the Pacific El Niño storms.1. NASA's remotely piloted Global Hawk aircraft will complete a series of high-level flights near 60,000 feet to measure the rainfall and upper level winds of the El Niño storms.2. This special research project is probing how the current El Niño’s unusually warm ocean temperatures in the equatorial Pacific are producing extreme precipitation on the West Coast, thousands of miles away.TAG: The goal of the research is help provide better warnings for the extreme weather that can accompany El Niño related storms. || IPAD_DELIVERABLES_NASAOnAir-Global_Hawk_iPad_1920x1080_print.jpg (1024x576) [94.2 KB] || IPAD_DELIVERABLES_NASAOnAir-Global_Hawk_iPad_1920x1080_searchweb.png (320x180) [70.2 KB] || IPAD_DELIVERABLES_NASAOnAir-Global_Hawk_iPad_1920x1080_thm.png (80x40) [4.5 KB] || WSI_WEATHER_CHANNEL_NASAOnAir-Global_Hawk_1280x720.mov (1280x720) [499.3 MB] || WSI_WEATHER_CHANNEL_NASAOnAir-Global_Hawk_1920x1080.mov (1920x1080) [430.3 MB] || NBC_TODAY_NASAOnAir-Global_Hawk_NBC_Today.mov (1920x1080) [36.9 MB] || Weather_Channel_NASAOnAir-Global_Hawk_Weather_Channel.wmv (1280x720) [5.2 MB] || Accuweather_NASAOnAir-Global_Hawk_Accuweather.avi (1280x720) [4.3 MB] || BARON_SERVICE_NASAOnAir-Global_Hawk_baron.mp4 (1920x1080) [17.0 MB] || WC_PRORES_422_NASAOnAir-Global_Hawk_prores.mov (1920x1080) [322.9 MB] || IPAD_DELIVERABLES_NASAOnAir-Global_Hawk_iPad_960x540.m4v (960x540) [19.6 MB] || IPAD_DELIVERABLES_NASAOnAir-Global_Hawk_iPad_1280x720.m4v (1280x720) [34.5 MB] || IPAD_DELIVERABLES_NASAOnAir-Global_Hawk_iPad_1920x1080.m4v (1920x1080) [55.0 MB] || WEBM_NASAOnAir-Global_Hawk.webm (960x540) [10.4 MB] || ", "hits": 19 }, { "id": 30748, "url": "https://svs.gsfc.nasa.gov/30748/", "result_type": "Hyperwall Visual", "release_date": "2016-02-01T00:00:00-05:00", "title": "Sea Surface Temperature and Temperature Anomaly 2015-2016", "description": "El Niño is characterized by unusually warm ocean temperatures in the eastern equatorial Pacific. Sea surface temperature is the temperature of the top millimeter of the ocean's surface. A sea surface temperature anomaly (SSTA) represents how different the ocean temperature, at a particular location and time, is from the normal (or average) temperature for that place and time. These maps, showing sea surface temperature and sea surface temperature anomalies, reveal the progression of the strong 2015-16 El Nino event from January 1, 2015 to January 2, 2016. The sea surface temperature data are seven-day averages calculated using daily thermal data from the Moderate Resolution Imaging Spectroradiometer (MODIS) instrument. Missing data have been filled with monthly-average data. The sea surface temperature anomaly data are seven-day averages calculated using the 5-kilometer Coral Reef Watch product produced by the National Oceanic and Atmospheric Administration. The data are based on observations from geostationary and polar-orbiting satellites. || ", "hits": 148 }, { "id": 30747, "url": "https://svs.gsfc.nasa.gov/30747/", "result_type": "Hyperwall Visual", "release_date": "2016-01-29T10:00:00-05:00", "title": "2015 El Niño Disrupts Ocean Chlorophyll", "description": "Sea Surface Temperature Anomaly & Ocean Color variations during El Nino vs. La Nina, using the rainbow colorbar for Ocean Color || ocean_color_ssta_swipe_new_rainbow_1080p.00001_print.jpg (1024x576) [116.9 KB] || ocean_color_ssta_swipe_new_rainbow_1080p.mp4 (1920x1080) [2.4 MB] || ocean_color_ssta_swipe_new_rainbow_720p.mp4 (1280x720) [1.4 MB] || ocean_color_ssta_swipe_new_rainbow_720p.webm (1280x720) [3.8 MB] || ocean_color_ssta_swipe_new_rainbow_2304p.mp4 (4096x2304) [7.5 MB] || ocean_color_ssta_swipe_new_rainbow_360p.mp4 (640x360) [530.1 KB] || ", "hits": 65 }, { "id": 12114, "url": "https://svs.gsfc.nasa.gov/12114/", "result_type": "Produced Video", "release_date": "2016-01-05T11:00:00-05:00", "title": "Observing El Niño", "description": "Explore how NASA will see this year’s El Niño from the vantage of space. || cf-1024.jpg (1024x576) [105.8 KB] || cf-1024_print.jpg (1024x576) [108.0 KB] || cf-1024_searchweb.png (320x180) [56.5 KB] || cf-1024_web.png (320x180) [56.5 KB] || cf-1024_thm.png (80x40) [17.9 KB] || ", "hits": 39 }, { "id": 30629, "url": "https://svs.gsfc.nasa.gov/30629/", "result_type": "Hyperwall Visual", "release_date": "2015-12-27T16:00:00-05:00", "title": "El Niño Watch 2015", "description": "Animation of Sea Surface Height Anomaly for 2015 compared to 1997 || ssha_1997vs2015_print.jpg (1024x574) [142.6 KB] || ssha_1997vs2015_searchweb.png (180x320) [71.4 KB] || ssha_1997vs2015_thm.png (80x40) [7.0 KB] || ssha_1997vs2015_720p.webm (1280x720) [2.4 MB] || ssha_1997vs2015_720p.mp4 (1280x720) [4.0 MB] || ssha_1997vs2015_1080p.mp4 (1920x1080) [5.1 MB] || ssha_1997vs2015_2304p.mp4 (4096x2304) [15.3 MB] || ssha_1997vs2015_360p.mp4 (640x360) [1.7 MB] || ssha_1997vs2015.tif (4104x2304) [4.3 MB] || ssha_1997vs2015_30629.key [7.5 MB] || ssha_1997vs2015_30629.pptx [4.9 MB] || el_nino_1997vs2015_recent_still.hwshow [230 bytes] || ", "hits": 46 }, { "id": 12098, "url": "https://svs.gsfc.nasa.gov/12098/", "result_type": "Produced Video", "release_date": "2015-12-14T14:30:00-05:00", "title": "Observing the 2015 El Niño", "description": "For complete transcript, click here. || 12098-MASTER_youtube_hq_print.jpg (1024x576) [116.7 KB] || 12098-MASTER_youtube_hq_searchweb.png (320x180) [77.2 KB] || 12098-MASTER_youtube_hq_web.png (320x180) [77.2 KB] || 12098-MASTER_youtube_hq_thm.png (80x40) [5.6 KB] || 12098-MASTER.mov (1920x1080) [1.2 GB] || 12098-MASTER_prores.mov (1280x720) [662.4 MB] || 12098-MASTER_youtube_hq.mov (1920x1080) [438.1 MB] || 12098-MASTER_appletv.m4v (1280x720) [46.0 MB] || 12098-MASTER.mpeg (1280x720) [322.5 MB] || 12098-MASTER_youtube_hq.webm (1920x1080) [10.3 MB] || 12098-MASTER_appletv_subtitles.m4v (1280x720) [46.1 MB] || 2015_El_Nino.en_US.srt [1.8 KB] || 2015_El_Nino.en_US.vtt [1.8 KB] || 12098-MASTER_ipod_sm.mp4 (320x240) [16.8 MB] || ", "hits": 33 }, { "id": 12032, "url": "https://svs.gsfc.nasa.gov/12032/", "result_type": "Produced Video", "release_date": "2015-10-27T11:00:00-04:00", "title": "Antarctic Sea Ice Update", "description": "This year’s Antarctic sea ice maximum extent is the lowest since 2008. || c-1920.jpg (1920x1080) [234.6 KB] || c-1280.jpg (1280x720) [161.1 KB] || c-1024.jpg (1024x576) [118.4 KB] || c-1024_print.jpg (1024x576) [124.0 KB] || c-1024_searchweb.png (320x180) [73.7 KB] || c-1024_web.png (320x180) [73.7 KB] || c-1024_thm.png (80x40) [17.0 KB] || ", "hits": 32 }, { "id": 12021, "url": "https://svs.gsfc.nasa.gov/12021/", "result_type": "Produced Video", "release_date": "2015-10-13T13:00:00-04:00", "title": "Hubble Maps Jupiter in 4k Ultra HD", "description": "New imagery from the Hubble Space Telescope is revealing details never before seen on Jupiter. Hubble’s new Jupiter maps were used to create this Ultra HD animation.Watch this video on the NASA Explorer YouTube channel. || JupiterThumbnailSmall.png (2160x1215) [1.4 MB] || G2015-085_Jupiter720_MASTER_appletv_appletv_subtitles.m4v (1280x720) [39.0 MB] || G2015-085_Jupiter720_MASTER_appletv.m4v (1280x720) [39.0 MB] || WEBM_G2015-085_Jupiter4k_MASTER_YouTube.webm (960x540) [28.5 MB] || G2015-085_Jupiter720_MASTER.mp4 (1280x720) [98.9 MB] || G2015-085_Jupiter720_MASTER_nasa_tv.mpeg (1280x720) [249.3 MB] || G2015-085_Jupiter720_MASTER_prores.mov (1280x720) [917.9 MB] || G2015-085_Jupiter720_MASTER.en_US.srt [98 bytes] || G2015-085_Jupiter720_MASTER.en_US.vtt [111 bytes] || G2015-085_Jupiter720_.key [41.8 MB] || G2015-085_Jupiter720_.pptx [39.3 MB] || G2015-085_Jupiter720_MASTER_12021.key [41.7 MB] || G2015-085_Jupiter720_MASTER_12021.pptx [39.3 MB] || G2015-085_Jupiter4k_MASTER_YouTube.mp4 (3840x2160) [495.9 MB] || G2015-085_Jupiter4k_MASTER.mov (3840x2160) [4.5 GB] || G2015-085_Jupiter4k_MASTER_YouTube.hwshow [94 bytes] || G2015-085_Jupiter720_MASTER_appletv.m4v.hwshow [88 bytes] || ", "hits": 1037 }, { "id": 11921, "url": "https://svs.gsfc.nasa.gov/11921/", "result_type": "Produced Video", "release_date": "2015-10-13T11:00:00-04:00", "title": "Planetary Portrait", "description": "The Hubble Space Telescope provides new maps of Jupiter. || c-1920.jpg (1920x1080) [171.1 KB] || c-1280.jpg (1280x720) [116.9 KB] || c-1024.jpg (1024x576) [89.3 KB] || c-1024_print.jpg (1024x576) [94.5 KB] || c-1024_searchweb.png (320x180) [34.8 KB] || c-1024_web.png (320x180) [34.8 KB] || c-1024_thm.png (80x40) [3.3 KB] || ", "hits": 76 }, { "id": 12012, "url": "https://svs.gsfc.nasa.gov/12012/", "result_type": "Produced Video", "release_date": "2015-09-23T14:00:00-04:00", "title": "Instagram: Earth’s Oceans Show Decline In Microscopic Plant Life", "description": "The world's oceans have seen significant declines in certain types of microscopic plant-life at the base of the marine food chain, according to a new NASA study. The research is the first to look at global, long-term phytoplankton community trends based on a model driven by NASA satellite data. Diatoms, the largest type of phytoplankton algae, have declined more than 1 percent per year from 1998 to 2012 globally, with significant losses occurring in the North Pacific, North Indian and Equatorial Indian oceans. The reduction in population may have an impact on the amount of carbon dioxide drawn out of the atmosphere and transferred to the deep ocean for long-term storage. || ", "hits": 11 }, { "id": 12009, "url": "https://svs.gsfc.nasa.gov/12009/", "result_type": "Produced Video", "release_date": "2015-09-23T09:30:00-04:00", "title": "Earth’s Oceans Show Decline In Microscopic Plant Life", "description": "The world's oceans have seen significant declines in certain types of microscopic plant-life at the base of the marine food chain, according to a new NASA study. The research is the first to look at global, long-term phytoplankton community trends based on a model driven by NASA satellite data. Diatoms, the largest type of phytoplankton algae, have declined more than 1 percent per year from 1998 to 2012 globally, with significant losses occurring in the North Pacific, North Indian and Equatorial Indian oceans. The reduction in population may have an impact on the amount of carbon dioxide drawn out of the atmosphere and transferred to the deep ocean for long-term storage. || ", "hits": 50 }, { "id": 30645, "url": "https://svs.gsfc.nasa.gov/30645/", "result_type": "Hyperwall Visual", "release_date": "2015-09-23T00:00:00-04:00", "title": "ENSO Sea Surface Temperature Anomalies: 2015-2016", "description": "Animation of Sea Surface Temperature Animaly from Dec 31, 2013 to present. || enso_ssta_2014-2016_print.jpg (1024x574) [225.9 KB] || enso_ssta_2014-2016.png (4104x2304) [6.5 MB] || enso_ssta_2014-2016_searchweb.png (320x180) [112.5 KB] || enso_ssta_2014-2016_thm.png (80x40) [8.0 KB] || enso_ssta_20131201-20160217_720p15.webm (1280x720) [28.8 MB] || enso_ssta_20131201-20160217_720p15.mp4 (1280x720) [221.0 MB] || enso_ssta_20131201-20160217_1080p15.mp4 (1920x1080) [360.9 MB] || enso_ssta_20131201-20160217_30645.key [223.5 MB] || enso_ssta_20131201-20160217_30645.pptx [221.1 MB] || enso_ssta_20131201-20160217_2304p15.mp4 (4104x2304) [896.9 MB] || ", "hits": 128 }, { "id": 4350, "url": "https://svs.gsfc.nasa.gov/4350/", "result_type": "Visualization", "release_date": "2015-09-08T00:00:00-04:00", "title": "Phytoplankton Decline", "description": "Diatom Concentration, Equirectangular Projection || dia_diff_time_series.0001_print.jpg (1024x576) [115.8 KB] || dia_diff_time_series.0001_searchweb.png (320x180) [84.0 KB] || dia_diff_time_series.0001_thm.png (80x40) [7.4 KB] || dia_diff_time_series_1080p30.mp4 (1920x1080) [11.4 MB] || rectangular (1920x1080) [0 Item(s)] || dia_diff_time_series_1080p30.webm (1920x1080) [2.4 MB] || dia_diff_time_series_1080p30.mp4.hwshow [194 bytes] || ", "hits": 90 } ] }