{ "count": 457, "next": "https://svs.gsfc.nasa.gov/api/search/?limit=100&offset=100&search=%22Number%22", "previous": null, "results": [ { "id": 14979, "url": "https://svs.gsfc.nasa.gov/14979/", "result_type": "Produced Video", "release_date": "2026-03-26T14:00:00-04:00", "title": "Early Testing of Aerogel and Silicon Detectors for TIGERISS", "description": "Nick Cannady, an astrophysicist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, examines a block of silica aerogel in May 2025. Cannady uses the light weight material in detectors for the upcoming TIGERISS (Trans-Iron Galactic Element Recorder for the International Space Station) mission, which is designed to study high-speed charged particles called cosmic rays.Credit: NASA/Scott WiessingerAlt text: A man studies a transparent block of aerogel.Image description: A man with glasses wearing a blue checkered shirt examines a block of transparent material resting on a table. He is leaning and rests his right hand on the table. The block glows faintly blue. The table is gray with evenly spaced rows of holes. || Tigeriss-Aerogel__Nick_Cannady-3.jpg (6393x4718) [17.4 MB] || Tigeriss-AerogelNick_Cannady-3-small.jpg (3196x2359) [1.6 MB] || ", "hits": 194 }, { "id": 31361, "url": "https://svs.gsfc.nasa.gov/31361/", "result_type": "Hyperwall Visual", "release_date": "2026-01-09T06:59:59-05:00", "title": "Large Solar Flares Erupt From the Sun", "description": "NASA’s Solar Dynamics Observatory captured images of two solar flares on Nov. 14 and Nov. 30, 2025.", "hits": 351 }, { "id": 14930, "url": "https://svs.gsfc.nasa.gov/14930/", "result_type": "Infographic", "release_date": "2025-12-18T10:00:00-05:00", "title": "NASA’s Fermi Spots Young Star Cluster Blowing Gamma-Ray Bubbles", "description": "Artist's concepts and images of Westerlund 1 and its budding gamma-ray-emitting outflow. Includes a multiwavelength reel", "hits": 147 }, { "id": 5587, "url": "https://svs.gsfc.nasa.gov/5587/", "result_type": "Visualization", "release_date": "2025-12-11T12:00:00-05:00", "title": "Moon Phase and Libration, 2026", "description": "The animation archived on this page shows the geocentric phase, libration, position angle of the axis, and apparent diameter of the Moon throughout the year 2026, at hourly intervals.", "hits": 7694 }, { "id": 5588, "url": "https://svs.gsfc.nasa.gov/5588/", "result_type": "Visualization", "release_date": "2025-12-11T12:00:00-05:00", "title": "Moon Phase and Libration, 2026 South Up", "description": "The animation archived on this page shows the geocentric phase, libration, position angle of the axis, and apparent diameter of the Moon throughout the year 2026, at hourly intervals.", "hits": 796 }, { "id": 14931, "url": "https://svs.gsfc.nasa.gov/14931/", "result_type": "Infographic", "release_date": "2025-12-04T00:00:00-05:00", "title": "Roman By The Numbers Infographic", "description": "NASA's Nancy Grace Roman Space Telescope will survey vast swaths of sky during its five-year primary mission. During that time, scientists expect it to see an incredible number of new object, including stars, galaxies, black holes and planets outside our solar system, known as exoplanets. This infographic previews some of the discoveries scientists anticipate from Roman's data deluge. || Roman_ByTheNumbers_Infographic_half.jpg (2000x1125) [498.6 KB] || Roman_ByTheNumbers_Infographic_print.jpg (1024x576) [223.6 KB] || Roman_ByTheNumbers_Infographic.png (4000x2250) [2.0 MB] || Roman_ByTheNumbers_Infographic.jpg (4000x2250) [1.0 MB] || Roman_ByTheNumbers_Infographic_searchweb.png (320x180) [75.1 KB] || Roman_ByTheNumbers_Infographic_thm.png (80x40) [7.1 KB] || ", "hits": 238 }, { "id": 14928, "url": "https://svs.gsfc.nasa.gov/14928/", "result_type": "Produced Video", "release_date": "2025-11-20T10:00:00-05:00", "title": "TESS Triples Size of Pleiades Star Cluster", "description": "These young, hot blue stars are members of the Pleiades open star cluster and reside about 430 light-years away in the northern constellation Taurus. The brightest stars are visible to the unaided eye during evenings from October to April. A new study finds the cluster to be triple the size previously thought — and shows that its stars are scattered across the night sky. The Schmidt telescope at the Palomar Observatory in California captured this color-composite image. Credit: NASA, ESA, and AURA/CaltechAlt text: Members of the Pleiades shine in blue. Image description: The Pleiades are shown in this image. Six of the stars, all blue-white, are larger than the others and have diffraction spikes and faint blue circles around them. Other, smaller blue stars are also scattered across the image. Patches of swirling blue dust surround some of the stars. || STScI-01EVVEYWX1TA3MGBK5F6EFQVGQ.jpg (4877x3513) [1.1 MB] || ", "hits": 434 }, { "id": 14906, "url": "https://svs.gsfc.nasa.gov/14906/", "result_type": "Produced Video", "release_date": "2025-09-30T15:00:00-04:00", "title": "Evolution of a Sun-Like Star", "description": "As a star ages, its spin and the number and sizes of its spots decreases as shown in this animation of a Sun-like star. Star spots are tied to local magnetic fields that have been amplified by the star’s rotation, so the phenomena are connected.A version without labels is available for download.Credit: NASA’s Goddard Space Flight Center || ThreeStars_Still.jpg (3840x2160) [586.8 KB] || ThreeStars_Still.png (3840x2160) [3.4 MB] || ThreeStars_Still_searchweb.png (320x180) [65.9 KB] || ThreeStars_Still_thm.png (80x40) [6.3 KB] || 14906_ThreeStars_NoText_1080.mp4 (1920x1080) [53.6 MB] || 14906_ThreeStars_1080.mp4 (1920x1080) [53.8 MB] || 14906_ThreeStars_4k.mp4 (3840x2160) [178.6 MB] || 14906_ThreeStars_NoText_4k.mp4 (3840x2160) [178.3 MB] || 14906_ThreeStars_NoText_ProRes_3840x2160_2997.mov (3840x2160) [1.8 GB] || 14906_ThreeStars_ProRes_3840x2160_2997.mov (3840x2160) [1.9 GB] || ", "hits": 342 }, { "id": 14883, "url": "https://svs.gsfc.nasa.gov/14883/", "result_type": "Produced Video", "release_date": "2025-08-25T11:00:00-04:00", "title": "Mapping Stellar ‘Polka Dots’", "description": "Watch to learn how a new tool uses data from exoplanets, worlds beyond our solar system, to tell us about their polka-dotted stars.Credit: NASA’s Goddard Space Flight CenterMusic: “Whimsical Whirlwinds,” Claire Leona Batchelor [PRS], Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available.Get the vertical version of this video [here](https://svs.gsfc.nasa.gov/14797/){target=_blank}. || PolkaDotStars_Thumbnail.jpg (1920x1080) [145.7 KB] || PolkaDotStars_Thumbnail_print.jpg (1024x576) [59.8 KB] || PolkaDotStars_Thumbnail_searchweb.png (320x180) [33.1 KB] || PolkaDotStars_Thumbnail_thm.png (80x40) [3.1 KB] || 14883_MappingStellarPolkaDots_Low.mp4 (1920x1080) [74.2 MB] || 14883_MappingStellarPolkaDots.mp4 (1920x1080) [262.9 MB] || MappingStellarPolkaDotsCaptions.en_US.srt [1.4 KB] || 14883_MappingStellarPolkaDots_ProRes_1920x1080_2997.mov (1920x1080) [1.4 GB] || ", "hits": 125 }, { "id": 20409, "url": "https://svs.gsfc.nasa.gov/20409/", "result_type": "Animation", "release_date": "2025-08-22T09:00:00-04:00", "title": "The Heliosphere and Galactic Cosmic Rays", "description": "Surrounding our solar system is a giant protective bubble created by particles and magnetic fields from the Sun called the heliosphere. Every 11 years, the Sun’s activity ramps up and down in what’s known as the solar cycle. As the Sun reaches its peak activity level, called solar maximum, the heliosphere expands. During this time, the heliosphere’s protective shield is strengthened by the increase in particles and magnetic fields from the Sun. As a result, fewer damaging particles from the galaxy, such as galactic cosmic rays, are able to penetrate into the heliosphere. As the Sun ramps down into a low level of activity, called solar minimum, the heliosphere shrinks and more cosmic rays are able to enter the heliosphere. || ", "hits": 446 }, { "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": 5258, "url": "https://svs.gsfc.nasa.gov/5258/", "result_type": "Visualization", "release_date": "2025-06-16T00:00:00-04:00", "title": "Tracking Satellites and Space Debris in Earth Orbit (Feb 2024)", "description": "This series of visualizations illustrates the population of objects orbiting Earth as of February 2024.", "hits": 3275 }, { "id": 5543, "url": "https://svs.gsfc.nasa.gov/5543/", "result_type": "Visualization", "release_date": "2025-06-11T10:00:00-04:00", "title": "Solar Magnetic Field - from Solar Minimum to Solar Maximum", "description": "Visualizations of the solar magnetic field evolution as a potential-field-source-surface model (PFSS) from solar minimum (2019) to solar maximum (2025).", "hits": 185 }, { "id": 5407, "url": "https://svs.gsfc.nasa.gov/5407/", "result_type": "Visualization", "release_date": "2025-05-28T00:00:00-04:00", "title": "Solar Loops and Eruptions - October 8, 2024", "description": "A fourteen hour continuous observation of the Sun, showing the variety of eruptions.", "hits": 55 }, { "id": 14798, "url": "https://svs.gsfc.nasa.gov/14798/", "result_type": "Produced Video", "release_date": "2025-05-27T20:56:00-04:00", "title": "Astrophysics Multiwavelength Vertical Video", "description": "This page contains vertically-formatted Astrophysics videos that show multiwavelength content.", "hits": 175 }, { "id": 14799, "url": "https://svs.gsfc.nasa.gov/14799/", "result_type": "Produced Video", "release_date": "2025-05-27T20:54:00-04:00", "title": "Astrophysics: Observing the Universe Vertical Video", "description": "This page contains vertically-formatted Astrophysics videos related to general astrophysical imagery.", "hits": 436 }, { "id": 5510, "url": "https://svs.gsfc.nasa.gov/5510/", "result_type": "Visualization", "release_date": "2025-02-25T17:10:00-05:00", "title": "Map of the March 29, 2025 Partial Solar Eclipse", "description": "On Saturday, March 29, 2025, the Moon passes in front of the Sun, casting its shadow across the Atlantic Ocean. Observers in Europe, western Africa, and eastern Canada are positioned to see a partial eclipse.", "hits": 412 }, { "id": 5442, "url": "https://svs.gsfc.nasa.gov/5442/", "result_type": "Visualization", "release_date": "2025-01-29T12:00:00-05:00", "title": "Water Cycle Nonstationarity", "description": "The global water cycle is undergoing unprecedented shifts from climate change, intensified by human water and land management practices. These changes are evident in phenomena such as depleted groundwater, earlier snowmelt, and erratic fluctuations in floods and drought occurrences. To better understand these changes in terrestrial water storage, scientists have integrated multiple remote sensing datasets with NASA’s advanced land surface model through data assimilation, creating a global water storage reanalysis dataset. The results capture the complex patterns of global water cycle shifts in response to both climate and human activities. Using this new integrated dataset, scientists use statistical methods (time series analysis) to identify trends (TR), seasonal shifts (SS), and changes in extreme events (EFR), ultimately developing an index, the “Nonstationarity Index,” (NSI) that quantifies the degree of nonstationarity within the global water system. || ", "hits": 30 }, { "id": 14772, "url": "https://svs.gsfc.nasa.gov/14772/", "result_type": "B-Roll", "release_date": "2025-01-29T11:00:00-05:00", "title": "Discoveries from Asteroid Bennu: Media Briefing Graphics", "description": "OSIRIS-REx MISSION RECAPThis highlight reel recaps the OSIRIS-REx mission, from assembly and launch of the spacecraft in 2016, to arrival at asteroid Bennu in 2018, TAG sample collection in 2020, the delivery of the sample to Earth in 2023, and curation of the Bennu samples in 2024.Credit: NASA || OSIRIS-REx_Collier_Present_2024_Preview_print.jpg (1024x576) [180.7 KB] || OSIRIS-REx_Collier_Present_2024_Preview.png (3840x2160) [8.3 MB] || OSIRIS-REx_Collier_Present_2024_Preview_searchweb.png (320x180) [116.3 KB] || OSIRIS-REx_Collier_Present_2024_Preview_thm.png [9.7 KB] || OSIRIS-REx_Collier_Present_2024_V3_Small.mp4 (1920x1080) [179.0 MB] || OSIRIS-REx_Collier_Present_2024_V3_Medium.mp4 (3840x2160) [500.9 MB] || OSIRIS-REx_Collier_Present_2024_V3_Large.mp4 (3840x2160) [1.6 GB] || ", "hits": 474 }, { "id": 5447, "url": "https://svs.gsfc.nasa.gov/5447/", "result_type": "Visualization", "release_date": "2025-01-02T15:09:00-05:00", "title": "Atmospheric Carbon Dioxide Concentrations", "description": "A plot of global atmospheric carbon dioxide levels from the Mauna Loa Observatory and Antarctic Ice Cores. The visualization starts by showing the Mauna Loa data which begins in 1958. There is a seasonal variation (maximum in May and minimum in September) and a steady year over year rise. The graph transforms from the monthly view to a line plot (The Keeling Curve). Finally the graph zooms out to show the full 800,000 year record from the Antarcic Ice Cores.", "hits": 1011 }, { "id": 14679, "url": "https://svs.gsfc.nasa.gov/14679/", "result_type": "Produced Video", "release_date": "2024-12-13T00:00:00-05:00", "title": "NICER Caddy Preparation", "description": "In Spring 2024, scientists and engineers at NASA prepared and packed a patch kit for NICER (Neutron star Interior Composition Explorer), an X-ray telescope on the International Space Station.In May 2023, damage to thin thermal shields protecting NICER allowed sunlight to reach its sensitive X-ray detectors. This saturated sensors and interfered with NICER’s measurements during orbital daytime.The NICER team designed five wedge-shaped patches to cover the largest areas of damage. The plan calls for astronauts to insert these patches into the instrument’s sunshades and lock them in place. || ", "hits": 59 }, { "id": 14707, "url": "https://svs.gsfc.nasa.gov/14707/", "result_type": "Produced Video", "release_date": "2024-11-25T11:00:00-05:00", "title": "XRISM's Resolve Instrument Gazes into Cygnus X-3", "description": "Cygnus X-3 is a high-mass X-ray binary system consisting of a compact object (likely a black hole) and a Wolf-Rayet star. This artist's concept shows one interpretation of the system. High-resolution X-ray spectroscopy indicates two gas components: a heavy background outflow, or wind, produced by the massive star and a turbulent structure — perhaps a wake carved into the wind — located close to the orbiting companion. As shown here, a black hole's gravity captures some of the wind into an accretion disk around it, and the disk's orbital motion sculpts a path (yellow arc) through the streaming gas. During strong outbursts, the companion emits jets of particles moving near the speed of light, seen here extending above and below the black hole.Credit: NASA’s Goddard Space Flight CenterAlt text: Illustration of the Cygnus X-3 systemImage description: On a cloudy reddish background, a bright blue-white circle — a representation of a hot, bright, massive star — sits near the center. Wisps of blue-white border its edges, and many lines of similar color radiate from it. In the foreground at about 4 o’clock lies a yellowish ring with a black hole in its center. From the ring trails a diffuse yellow arc, sweeping from right to left and exiting at the bottom of the illustration. Extending above and below the black hole are two blue-white triangles representing particle jets. || Cyg_X-3_illustration_4K.jpg (3840x2160) [505.1 KB] || Cyg_X-3_illustration_4K_print.jpg (1024x576) [58.5 KB] || Cyg_X-3_illustration_4K_searchweb.png (320x180) [64.7 KB] || Cyg_X-3_illustration_4K_web.png (320x180) [64.7 KB] || Cyg_X-3_illustration_4K_thm.png (80x40) [6.1 KB] || ", "hits": 597 }, { "id": 5415, "url": "https://svs.gsfc.nasa.gov/5415/", "result_type": "Visualization", "release_date": "2024-11-22T09:00:00-05:00", "title": "Moon Phase and Libration, 2025", "description": "The geocentric phase, libration, position angle of the axis, and apparent diameter of the Moon throughout the year 2025, at hourly intervals.", "hits": 4546 }, { "id": 5416, "url": "https://svs.gsfc.nasa.gov/5416/", "result_type": "Visualization", "release_date": "2024-11-22T09:00:00-05:00", "title": "Moon Phase and Libration, 2025 South Up", "description": " || The data in the table for all of 2025 can be downloaded as a JSON file or as a text file. || ", "hits": 573 }, { "id": 14685, "url": "https://svs.gsfc.nasa.gov/14685/", "result_type": "Produced Video", "release_date": "2024-10-15T15:00:00-04:00", "title": "What is Solar Maximum?", "description": "The Sun is stirring from its latest slumber. As sunspots and flares bubble from the Sun’s surface, representatives from NASA, the National Oceanic and Atmospheric Agency (NOAA), and the Solar Cycle Prediction Panel announced on Tuesday, September 24, 2024, the Sun has reached its solar maximum period.The solar cycle is the natural cycle of the Sun as it transitions between low and high activity. During the most active part of the cycle, known as solar maximum, the Sun can unleash immense explosions of light, energy, and solar radiation — all of which create conditions known as space weather. Space weather can affect satellites and astronauts in space, as well as communications systems — such as radio and GPS — and power grids on Earth. || ", "hits": 321 }, { "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": 14683, "url": "https://svs.gsfc.nasa.gov/14683/", "result_type": "Produced Video", "release_date": "2024-10-15T13:30:00-04:00", "title": "NASA, NOAA Announce That the Sun Has Reached the Solar Maximum Period", "description": "In a teleconference with reporters on Tuesday, October 15, 2024, representatives from NASA, the National Oceanic and Atmospheric Agency (NOAA), and the Solar Cycle Prediction Panel announced the Sun has reached its solar maximum period.The solar cycle is the natural cycle of the Sun as it transitions between low and high activity. Roughly every 11 years, at the height of the solar cycle, the Sun’s magnetic poles flip — on Earth, that’d be like the North and South Poles swapping places every decade — and the Sun transitions from sluggish to active and stormy.During the most active part of the cycle, known as solar maximum, the Sun can unleash immense explosions of light, energy, and solar radiation — all of which create conditions known as space weather. Space weather can affect satellites and astronauts in space, as well as communications systems — such as radio and GPS — and power grids on Earth. When the Sun is most active, space weather events become more frequent. Solar activity, such as the storm in May 2024, has led to increased aurora visibility and impacts on satellites and infrastructure in recent months.Listen to the media telecon.Read NASA's article about the news. || ", "hits": 836 }, { "id": 14703, "url": "https://svs.gsfc.nasa.gov/14703/", "result_type": "Produced Video", "release_date": "2024-10-10T07:00:00-04:00", "title": "X1.8 Flare Erupts From Sun on October 8, 2024", "description": "NASA’s Solar Dynamics Observatory captured this imagery of an X1.8 solar flare – as seen in the bright flash in the center – on Oct. 08, 2024. The footage shows from 9:15 to 10:18 p.m. EDT in a blend of 171, 304, and 131 Angstrom light, subsets of extreme ultraviolet light. This cropped version is slowed to 1/3 speed. Credit: NASA/SDO || Video_Still.jpg (1920x1080) [570.8 KB] || Video_Still_searchweb.png (320x180) [106.4 KB] || Video_Still_thm.png (80x40) [7.7 KB] || SDO_10_09_24_X1pt8_131-171-304tpz.mp4 (1920x1080) [22.1 MB] || SDO_10_09_24_X1pt8_131-171-304tpz.mov (1920x1080) [154.8 MB] || ", "hits": 79 }, { "id": 5327, "url": "https://svs.gsfc.nasa.gov/5327/", "result_type": "Visualization", "release_date": "2024-07-17T06:00:00-04:00", "title": "Slow Reveal Graphs: Twelve consecutive months of global surface temperature records (June 2023 - May 2024)", "description": "Slow reveal graphs are an instructional routine using scaffolded visuals and discourse to help students (in K-12 and beyond) make sense of data. This is a slow reveal graph of the SVS visualization of Twelve consectutive months of global surface temperature records. || ", "hits": 57 }, { "id": 5305, "url": "https://svs.gsfc.nasa.gov/5305/", "result_type": "Visualization", "release_date": "2024-07-02T08:00:00-04:00", "title": "2023 Atlantic Hurricane Season", "description": "The 2023 Atlantic Hurricane Season from June 1st through October 31st. The colors over the ocean are Sea Surface Temperatures where reds are high temperatures and blues are low. The colors underneath the clouds are precipitation measurements, where red is high and greens are low. Each hurricane name tracks with it's corresponding storm and leaves behind category designations (TD=Tropical Depression; TS=Tropical Storm; and 1 through 5 are hurricane strengths) as each storm increases and decreases in strength. || hurr2023_v34_ALL_2024-06-26_1103.00001_print.jpg (1024x576) [234.5 KB] || hurr2023_v34_ALL_2024-06-26_1103.00001_searchweb.png (320x180) [101.0 KB] || hurr2023_v34_ALL_2024-06-26_1103.00001_thm.png (80x40) [6.8 KB] || hurr2023_v34_ALL_2024-06-26_1103_1080p30.webm (1920x1080) [44.7 MB] || All_Data_in_HD [0 Item(s)] || hurr2023_v34_ALL_2024-06-26_1103_1080p30.mp4 (1920x1080) [739.1 MB] || ALL_Data_in_UHD [0 Item(s)] || hurr2023_v34_ALL_4k.mp4 (3840x2160) [2.3 GB] || ", "hits": 48 }, { "id": 5312, "url": "https://svs.gsfc.nasa.gov/5312/", "result_type": "Visualization", "release_date": "2024-06-16T18:00:00-04:00", "title": "Slow Reveal Graphs: Global Mean Sea Level 1993-2023", "description": "Slow reveal graphs are an instructional routine using scaffolded visuals and discourse to help students (in K-12 and beyond) make sense of data. This is a slow reveal graph of the SVS visualization of rising Global Mean Sea Level. || ", "hits": 120 }, { "id": 5303, "url": "https://svs.gsfc.nasa.gov/5303/", "result_type": "Visualization", "release_date": "2024-05-30T14:00:00-04:00", "title": "NASA’s TEMPO Instrument Air Quality Data Now Publicly Available", "description": "The TEMPO instrument measured elevated levels of nitrogen dioxide (NO2) from a number of different areas and emission sources throughout the daytime on March 28, 2024. Yellow, red, purple, and black clusters represent increased levels of pollutants from TEMPO’s data and show drift over time. || TEMPO_3_28_2024_CONUS.0500_print.jpg (1024x576) [289.5 KB] || TEMPO_3_28_2024_CONUS.0500_searchweb.png (320x180) [103.2 KB] || TEMPO_3_28_2024_CONUS.0500_thm.png (80x40) [6.9 KB] || TEMPO_3_28_2024_CONUS [0 Item(s)] || TEMPO_3_28_2024_CONUS_1080p30.mp4 (1920x1080) [29.3 MB] || TEMPO_3_28_2024_CONUS (3840x2160) [1000 Item(s)] || TEMPO_3_28_2024_CONUS_2160p30.mp4 (3840x2160) [111.7 MB] || TEMPO_3_28_2024_CONUS_1080p30.mp4.hwshow || ", "hits": 68 }, { "id": 14597, "url": "https://svs.gsfc.nasa.gov/14597/", "result_type": "Produced Video", "release_date": "2024-05-28T16:00:00-04:00", "title": "Strong Solar Flare Erupts from Sun, May 27, 2024 and Another May 29th.", "description": "NASA’s Solar Dynamics Observatory captured this image of a solar flare seen as the bright flash on the limb of the Sun on May 27, 2024, with an inset image of Earth for scale. The image shows a blend of 171 and 304 angstrom extreme ultraviolet light that highlights the extremely hot material in flares and which is colorized in red and yellow. Credit: NASA/SDO || SDO_May_27_Flare0700UT_171-304_EarthScale.jpg (1500x1500) [568.4 KB] || SDO_May_27_Flare0700UT_171-304_EarthScale_searchweb.png (320x180) [97.9 KB] || SDO_May_27_Flare0700UT_171-304_EarthScale_thm.png (80x40) [7.3 KB] || ", "hits": 71 }, { "id": 14592, "url": "https://svs.gsfc.nasa.gov/14592/", "result_type": "Produced Video", "release_date": "2024-05-14T00:00:00-04:00", "title": "Largest Flare yet from Solar Cycle 25", "description": "On May 14, 2024, the Sun emitted a strong solar flare. This solar flare is the largest of Solar Cycle 25 and is classified as an X8.7 flare. X-class denotes the most intense flares, while the number provides more information about its strength.A solar flare is an intense burst of radiation, or light, on the Sun. Flares are our solar system’s most powerful explosive events. Light only takes about 8 minutes to travel from the Sun to Earth, so that’s how long it would take the energy from a flare to reach our planet. Stronger solar flares — those rated class M5 or above — can have impacts on technology that depends on Earth’s ionosphere (our electrically charged upper atmosphere), like high-frequency radio used for navigation and GPS.NASA’s Solar Dynamics Observatory (SDO) captured these images of the flare, which peaked at 12:51 p.m. ET on May 14. The X8.7 flare appears on the lower right edge of the Sun. (A small eruption appears afterward in the upper left.) SDO sees the Sun in more than 10 distinct wavelengths of light, showing solar material at different temperatures. Different wavelengths are shown in this video to highlight different features of the flare.Music credit: “Ethereal Mirrorscape” from the album Reflections written and produced by Lars LeonhardWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || X8pt7_flare_May_14_2024.00_00_40_22.Still001.jpg (3840x2160) [3.0 MB] || X8pt7_flare_May_14_2024.00_00_40_22.Still001_print.jpg (1024x576) [342.3 KB] || X8pt7_flare_May_14_2024.00_00_40_22.Still001_searchweb.png (320x180) [75.1 KB] || X8pt7_flare_May_14_2024.00_00_40_22.Still001_web.png (320x180) [75.1 KB] || X8pt7_flare_May_14_2024.00_00_40_22.Still001_thm.png (80x40) [6.1 KB] || 14592_SDO_X8pt7_flare_May_14_2024_ProRes_Outro.webm (3840x2160) [20.4 MB] || 14592_SDO_X8pt7_flare_May_14_2024_Good_Outro.mp4 (3840x2160) [175.9 MB] || 14592_SDO_X8pt7_flare_May_14_2024_YouTube_Outro.mp4 (3840x2160) [673.0 MB] || 14592_SDO_X8pt7_flare_May_14_2024_ProRes_Outro.mov (3840x2160) [4.2 GB] || ", "hits": 447 }, { "id": 5254, "url": "https://svs.gsfc.nasa.gov/5254/", "result_type": "Visualization", "release_date": "2024-03-29T09:00:00-04:00", "title": "IMERG Daily Precipitation Climatology (2001 - 2022)", "description": "Example composite showing the 30 day moving average daily precipitation climatology along with the date and colorbar.", "hits": 89 }, { "id": 5248, "url": "https://svs.gsfc.nasa.gov/5248/", "result_type": "Visualization", "release_date": "2024-03-25T13:30:00-04:00", "title": "Insolation during the 2024 Eclipse", "description": "Insolation (the amount of sunlight reaching the ground) is affected dramatically by the Moon's shadow during the April 8, 2024 total solar eclipse. || insol.0765_print.jpg (1024x576) [144.8 KB] || insol.0765_searchweb.png (320x180) [73.2 KB] || insol.0765_thm.png (80x40) [6.1 KB] || eclipse2024_insol_720p30.mp4 (1280x720) [10.4 MB] || eclipse2024_insol_1080p30.mp4 (1920x1080) [21.3 MB] || eclipse2024_insol_2160p30.mp4 (3840x2160) [66.1 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || eclipse2024_insol_360p30.mp4 (640x360) [3.2 MB] || ", "hits": 52 }, { "id": 5234, "url": "https://svs.gsfc.nasa.gov/5234/", "result_type": "Visualization", "release_date": "2024-03-12T00:00:00-04:00", "title": "AIRS Global Carbon Dioxide (CO₂) measurements (2002-October 2023)", "description": "Data visualization showing the global distribution and variation of the concentration of mid-tropospheric carbon dioxide observed by the Atmospheric Infrared Sounder (AIRS) on the NASA Aqua spacecraft over a 20 year timespan.", "hits": 165 }, { "id": 14535, "url": "https://svs.gsfc.nasa.gov/14535/", "result_type": "Produced Video", "release_date": "2024-02-23T11:00:00-05:00", "title": "Sun Emits X6.3 Flare on February 22, 2024", "description": "NASA’s Solar Dynamics Observatory captured this image of a solar flare – as seen in the bright flash on the upper left – on Feb. 22, 2024. The image shows a blend of 171 Angstrom, 193 Angstrom and 1600 Angstrom light, subsets of ultraviolet and extreme ultraviolet light. Credit: NASA/SDO || SDO_Feb_22_X6pt3_Flare2244UTC_4k_171-193-1600.jpg (4096x4096) [1.9 MB] || SDO_Feb_22_X6pt3_Flare2244UTC_4k_171-193-1600_searchweb.png (320x180) [94.8 KB] || SDO_Feb_22_X6pt3_Flare2244UTC_4k_171-193-1600_thm.png (80x40) [7.6 KB] || ", "hits": 68 }, { "id": 14533, "url": "https://svs.gsfc.nasa.gov/14533/", "result_type": "Produced Video", "release_date": "2024-02-22T15:00:00-05:00", "title": "Sun Releases Two Strong Flares on February 21 and 22.", "description": "NASA’s Solar Dynamics Observatory captured this imagery of two solar flares – as seen in the flashes from the bright region in the upper left of the Sun – on Feb. 21 and 22, 2024. The footage shows a subset of extreme ultraviolet light that highlights the extremely hot material in flares, and which is colorized in teal. Credit: NASA/SDO || February_22_Flare_Still.png (1124x1124) [1.4 MB] || February_22_Flare_Still_print.jpg (1024x1024) [203.7 KB] || SDO_Feb21-22_DoubleXFlare_131_1024.mp4 (1024x1024) [14.4 MB] || SDO_Feb21-22_DoubleXFlare_131_1024.webm (1024x1024) [538.9 KB] || SDO_Feb21-22_DoubleXFlare_131.mp4 (4096x4096) [69.7 MB] || ", "hits": 51 }, { "id": 5222, "url": "https://svs.gsfc.nasa.gov/5222/", "result_type": "Visualization", "release_date": "2024-02-20T12:07:00-05:00", "title": "5000 Years of Total Solar Eclipses", "description": "A heatmap showing the frequency of total solar eclipses over the 5000 years from 2000 BCE to 3000 CE. Includes versions without the color key and without the continent outlines. || eclipse_freq_heatmap_print.jpg (1024x512) [323.0 KB] || eclipse_freq_heatmap_searchweb.png (320x180) [120.8 KB] || eclipse_freq_heatmap_thm.png (80x40) [17.8 KB] || eclipse_freq_heatmap.tif (5400x2700) [14.9 MB] || eclipse_freq_heatmap_nocbar.tif (5400x2700) [14.9 MB] || eclipse_freq_heatmap_noland.tif (5400x2700) [17.0 MB] || ", "hits": 553 }, { "id": 14531, "url": "https://svs.gsfc.nasa.gov/14531/", "result_type": "Produced Video", "release_date": "2024-02-20T10:00:00-05:00", "title": "February 16, 2024 X2.5 Solar Flare", "description": "NASA’s Solar Dynamics Observatory captured these images of a solar flare – as seen in the bright flash on the right of each image – on Feb. 16, 2024. The images show three subsets of extreme ultraviolet light that highlight the extremely hot material in flares and which are colorized in teal, gold, and red. Credit: NASA/SDO || Feb_16_Flare_Video_multi_still.jpg (1920x1080) [389.3 KB] || Feb_16_Flare_Video_multi_still_searchweb.png (320x180) [85.5 KB] || Feb_16_Flare_Video_multi_still_thm.png (80x40) [7.1 KB] || Feb_16_Flare_Video_multi.mp4 (1920x1080) [53.9 MB] || Feb_16_Flare_Video_multi.mov (1920x1080) [379.3 MB] || ", "hits": 79 }, { "id": 14479, "url": "https://svs.gsfc.nasa.gov/14479/", "result_type": "Produced Video", "release_date": "2024-02-09T11:00:00-05:00", "title": "Sun Releases X3.3 Flare on February 9, 2024", "description": "NASA’s Solar Dynamics Observatory captured this image of a solar flare – as seen in the bright flash on the lower right – on Feb. 9, 2024. The image shows a blend of 171 Angstrom and 131 Angstrom light, subsets of extreme ultraviolet light that highlight the plasma loops in the corona and the extremely hot material in flares, respectively. Credit: NASA/SDO || SDO_Feb_9_Flare1314UTC_131-171.jpg (4096x4096) [2.8 MB] || SDO_Feb_9_Flare1314UTC_131-171_searchweb.png (320x180) [102.5 KB] || SDO_Feb_9_Flare1314UTC_131-171_thm.png (80x40) [8.1 KB] || ", "hits": 77 }, { "id": 14727, "url": "https://svs.gsfc.nasa.gov/14727/", "result_type": "Produced Video", "release_date": "2024-01-22T00:00:00-05:00", "title": "Fort Sumner, New Mexico: 2024 Drone Views", "description": "This clip contains various shots of the NASA payload processing facility at Fort Sumner as well as general views of the surrounding area, acquired Aug. 23, 2024. Credit: NASA/Francis ReddyVideo playback is at half speed (30 fps). 0:00 A slow, early morning approach to the staging facility as its doors open, revealing the EXCITE (EXoplanet Climate Infrared TElescope) payload. 0:45 The camera descends, with the rising sun moving behind the staging facility. 0:58 A closer, lower approach to the EXCITE payload. 1:10 A higher, more distant arc that starts by showing the low sun and the NASA sign on the staging facility, moving north. 1:41 A slow ascent looking toward EXCITE and the morning sun. 1:28 Hovering as the doors close on EXCITE. 03:20 Overview flying back across the airport revealing various vehicles and structures. 4:41 Similar, but at higher altitude and flying in a different direction. || Drone_Shots_of_EXCITE_at_Balloon_Launch_Facility.00001_print.jpg (1024x576) [139.0 KB] || Drone_Shots_of_EXCITE_at_Balloon_Launch_Facility.webm (3840x2160) [67.5 MB] || Drone_Shots_of_EXCITE_at_Balloon_Launch_Facility.mp4 (3840x2160) [2.9 GB] || Drone_Shots_of_EXCITE_at_Balloon_Launch_Facility_ProRes.mov (3840x2160) [22.1 GB] || ", "hits": 53 }, { "id": 5207, "url": "https://svs.gsfc.nasa.gov/5207/", "result_type": "Visualization", "release_date": "2024-01-12T11:00:00-05:00", "title": "Global Temperature Anomalies from 1880 to 2023", "description": "This color-coded map in Robinson projection displays a progression of changing global surface temperature anomalies. Normal temperatures are shown in white. Higher than normal temperatures are shown in red and lower than normal temperatures are shown in blue. Normal temperatures are calculated over the 30 year baseline period 1951-1980. The maps are averages over a running 24 month window. The final frame represents global temperature anomalies in 2023. || 2023GISTEMP_Map.00899_print.jpg (1024x576) [138.7 KB] || 2023GISTEMP_Map.00899_searchweb.png (320x180) [66.6 KB] || 2023GISTEMP_Map.00899_thm.png (80x40) [6.4 KB] || 2023GISTEMP_Map.00899_web.png (320x180) [65.9 KB] || 2023GISTEMP_Map_HD.mp4 (1920x1080) [57.2 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || 2023GISTEMP_Map.mp4 (3840x2160) [114.3 MB] || earth_observations_5x3.hwshow || ", "hits": 686 }, { "id": 5208, "url": "https://svs.gsfc.nasa.gov/5208/", "result_type": "Visualization", "release_date": "2024-01-12T11:00:00-05:00", "title": "2023 Temperature Measurements", "description": "The locations of the temperature measurements that were used in the 2023 GISS Surface Temperature Analysis (v4). The data on land comes from the weather stations that make up the Global Historical Climatology Network (GHCN). Over water temperature measurements come from International Comprehensive Ocean-Atmosphere Data Set (ICOADS).", "hits": 98 }, { "id": 14492, "url": "https://svs.gsfc.nasa.gov/14492/", "result_type": "Produced Video", "release_date": "2024-01-05T08:50:00-05:00", "title": "XRISM Reveals Its First Look at X-ray Cosmos", "description": "XRISM’s Resolve instrument captured data from supernova remnant N132D in the Large Magellanic Cloud to create the most detailed X-ray spectrum of the object ever made. The spectrum reveals peaks associated with silicon, sulfur, argon, calcium, and iron. Inset at right is an image of N132D captured by XRISM’s Xtend instrument.Credit: JAXA/NASA/XRISM Resolve and Xtend || Resolve_N132D_Spectrum.jpg (3840x2395) [1.0 MB] || Resolve_N132D_Spectrum_searchweb.png (320x180) [45.7 KB] || Resolve_N132D_Spectrum_thm.png (80x40) [4.7 KB] || ", "hits": 139 }, { "id": 14497, "url": "https://svs.gsfc.nasa.gov/14497/", "result_type": "Produced Video", "release_date": "2024-01-04T11:00:00-05:00", "title": "Sun Emits X5 Flare on December 31, 2023", "description": "NASA’s Solar Dynamics Observatory captured this image of a solar flare – as seen in the bright flash on the left – on Dec. 31. 2023. The image shows a blend of 171 and 131 Angstrom extreme ultraviolet light that highlights the extremely hot material in flares and which is colorized in blue and gold.Credit: NASA/GSFC/SDO || SDO_Dec_31_2023_X5_171-131_print.jpg (1024x1024) [233.9 KB] || SDO_Dec_31_2023_X5_171-131.jpg (4096x4096) [2.8 MB] || SDO_Dec_31_2023_X5_171-131_searchweb.png (320x180) [118.6 KB] || SDO_Dec_31_2023_X5_171-131_thm.png (80x40) [8.8 KB] || ", "hits": 90 }, { "id": 14434, "url": "https://svs.gsfc.nasa.gov/14434/", "result_type": "Produced Video", "release_date": "2023-11-28T09:20:00-05:00", "title": "NASA’s Fermi Mission Finds 300 Gamma-Ray Pulsars", "description": "This visualization shows 294 gamma-ray pulsars, first plotted on an image of the entire starry sky as seen from Earth and then transitioning to a view from above our galaxy. The symbols show different types of pulsars. Young pulsars blink in real time except for the Crab, which pulses slower because its rate is only slightly lower than the video frame rate. Millisecond pulsars remain steady, pulsing too quickly to see. The Crab, Vela, and Geminga were among the 11 gamma-ray pulsars known before Fermi launched. Other notable objects are also highlighted. Distances are shown in light-years (abbreviated ly).Credit: NASA’s Goddard Space Flight CenterMusic: \"Fascination\" from Universal Production MusicWatch this video on the NASA.gov Video YouTube channel.Complete transcript available. || Pulsar_Still.jpg (3840x2160) [3.5 MB] || Pulsar_Still_searchweb.png (320x180) [105.5 KB] || Pulsar_Still_thm.png (80x40) [7.0 KB] || 14434_Fermi_Pulsar_Locations_1080.mp4 (1920x1080) [93.9 MB] || 14434_Fermi_Pulsar_Locations_1080.webm (1920x1080) [10.0 MB] || Pulsar_Captions.en_US.srt [46 bytes] || Pulsar_Captions.en_US.vtt [56 bytes] || 14434_Fermi_Pulsar_Locations_4k_Good.mp4 (3840x2160) [112.8 MB] || 14434_Fermi_Pulsar_Locations_4k_Best.mp4 (3840x2160) [689.2 MB] || 14434_Fermi_Pulsar_Locations_ProRes_3840x2160_2997.mov (3840x2160) [4.5 GB] || ", "hits": 215 }, { "id": 5187, "url": "https://svs.gsfc.nasa.gov/5187/", "result_type": "Visualization", "release_date": "2023-11-16T08:00:00-05:00", "title": "Moon Phase and Libration, 2024", "description": " || The data in the table for all of 2024 can be downloaded as a JSON file or as a text file. || moon.0001.jpg (730x730) [87.6 KB] || comp.0001.tif (5760x3240) [14.8 MB] || ", "hits": 1400 }, { "id": 5188, "url": "https://svs.gsfc.nasa.gov/5188/", "result_type": "Visualization", "release_date": "2023-11-16T08:00:00-05:00", "title": "Moon Phase and Libration, 2024 South Up", "description": " || The data in the table for all of 2024 can be downloaded as a JSON file or as a text file. || moon.0001.jpg (730x730) [87.3 KB] || comp.0001.tif (5760x3240) [15.0 MB] || ", "hits": 206 }, { "id": 14401, "url": "https://svs.gsfc.nasa.gov/14401/", "result_type": "Produced Video", "release_date": "2023-10-31T10:00:00-04:00", "title": "NASA’s Eclipse Art", "description": "“The greatest scientists are artists as well.” ~Albert EinsteinArt and science have been treated as separate disciplines but have more in common than is often realized. Creativity is critical to making scientific breakthroughs, and art is often an expression (or product) of scientific knowledge. And both art and science begin in the experience of awe, of beholding something grand. The experience of a solar eclipse is a prime example of where these two human endeavors meet.Eclipses are celestial events we can predict with extreme precision, and their occurrence reveals fundamental truths about our place in the universe. Yet, as many eclipse watchers will attest, there is no anticipating how you will feel when experiencing one. The emotional resonance of eclipses is underlined by their presence in artforms in cultures across the world going back millennia.To celebrate the special role of eclipses in connecting art and science, creatives across NASA will be sharing their eclipse-inspired artwork in anticipation of two solar eclipses that will cross the United States on October 14, 2023, and April 8, 2024.The first two pieces in the series are presented below, with short biographies of their creators. || ", "hits": 80 }, { "id": 40502, "url": "https://svs.gsfc.nasa.gov/gallery/2024total-solar-eclipse-gallery/", "result_type": "Gallery", "release_date": "2023-10-31T00:00:00-04:00", "title": "2024 Total Solar Eclipse", "description": "On April 8, 2024, a total solar eclipse will cross North America, passing over Mexico, the United States, and Canada. A total solar eclipse happens when the Moon passes between the Sun and Earth, completely blocking the face of the Sun. The sky will darken as if it were dawn or dusk.A total solar eclipse happens when the Moon passes between the Sun and Earth, completely blocking the face of the Sun. People viewing the eclipse from locations where the Moon’s shadow completely covers the Sun – known as the path of totality – will experience a total solar eclipse. The sky will darken, as if it were dawn or dusk. Weather permitting, people along the path of totality will see the Sun’s corona, or outer atmosphere, which is usually obscured by the bright face of the Sun.Learn more about this total solar eclipse: solarsystem.nasa.gov/eclipses/2024\n", "hits": 412 }, { "id": 5175, "url": "https://svs.gsfc.nasa.gov/5175/", "result_type": "Visualization", "release_date": "2023-10-12T00:00:00-04:00", "title": "TEMPO - Nitrogen Dioxide Air Pollution Over North America - Additional Views", "description": "In this visualization, high levels of nitrogen dioxide can be seen over multiple urban areas across the U.S., Canada, Mexico and the Caribbean. As the day progresses, the morning pollution often dissipates. Later in the afternoon, it will rise again as the cities enter their second rush hour of the day. Because TEMPO uses visible sunlight to make measurements, it cannot see pollution below clouds or at night. Cloudy areas appear as missing data in the visualization. This visualization shows data from August 28-31, 2023. || tempo_no2_north-america.02402_print.jpg (1024x576) [170.3 KB] || tempo_no2_north-america.02402_searchweb.png (180x320) [67.8 KB] || tempo_no2_north-america.02402_thm.png (80x40) [5.6 KB] || tempo_no2_north-america_1080p60.mp4 (1920x1080) [23.3 MB] || tempo_no2_north-america (3840x2160) [0 Item(s)] || tempo_no2_north-america_2160p60.mp4 (3840x2160) [84.5 MB] || tempo_no2_north-america_2160p30.mp4 (3840x2160) [84.8 MB] || tempo_no2_north-america.mov (3840x2160) [5.6 GB] || a005175_tempo_no2_north-america_2160p30.hwshow [60 bytes] || ", "hits": 59 }, { "id": 40503, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-earth-science/", "result_type": "Gallery", "release_date": "2023-08-28T00:00:00-04:00", "title": "Hyperwall Power Playlist - Earth Science Focus", "description": "This is a collection of our most powerful, newsworthy, and frequently used Hyperwall-ready visualizations, along with several that haven't gotten the attention they deserve. They're especially great for more general or top-level science talks, or to \"set the scene\" before a deep dive into a more focused subject or dataset. We've tried to cover the subject areas our speakers focus on most. \n\nIf you're not seeing what you're looking for, there is a huge library of visualizations more localized or specialized in subject - please use the Search function above, and filter \"Result type\" for \"Hyperwall Visual.\"\n\n If you'd like to use one of these visualizations in your Hyperwall presentation, we'll need to know which element on which page. On the visualization's web page, below the visual you'd like to use, you'll see a Link icon next to the Download button. All we need is for you to click on that icon and include that link in your presentation Powerpoint/Keynote or visualization list. Additionally, please check our Hyperwall How-To Guide for tips on designing your Hyperwall presentation, file specifications, and Powerpoint/Keynote templates.", "hits": 255 }, { "id": 40505, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-planetary-science-focus/", "result_type": "Gallery", "release_date": "2023-08-28T00:00:00-04:00", "title": "Hyperwall Power Playlist - Planetary Science Focus", "description": "This is a collection of our most powerful, newsworthy, and frequently used Hyperwall-ready visualizations, along with several that haven't gotten the attention they deserve. They're especially great for more general or top-level science talks, or to \"set the scene\" before a deep dive into a more focused subject or dataset. We've tried to cover the subject areas our speakers focus on most. \n\nIf you're not seeing what you're looking for, there is a huge library of visualizations more localized or specialized in subject - please use the Search function above, and filter \"Result type\" for \"Hyperwall Visual.\"\n\n If you'd like to use one of these visualizations in your Hyperwall presentation, we'll need to know which element on which page. On the visualization's web page, below the visual you'd like to use, you'll see a Link icon next to the Download button. All we need is for you to click on that icon and include that link in your presentation Powerpoint/Keynote or visualization list. Additionally, please check our Hyperwall How-To Guide for tips on designing your Hyperwall presentation, file specifications, and Powerpoint/Keynote templates.", "hits": 339 }, { "id": 40507, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-heliophysics-focus/", "result_type": "Gallery", "release_date": "2023-08-28T00:00:00-04:00", "title": "Hyperwall Power Playlist - Heliophysics Focus", "description": "This is a collection of our most powerful, newsworthy, and frequently used Hyperwall-ready visualizations, along with several that haven't gotten the attention they deserve. They're especially great for more general or top-level science talks, or to \"set the scene\" before a deep dive into a more focused subject or dataset. We've tried to cover the subject areas our speakers focus on most. \n\nIf you're not seeing what you're looking for, there is a huge library of visualizations more localized or specialized in subject - please use the Search function above, and filter \"Result type\" for \"Hyperwall Visual.\"\n\n If you'd like to use one of these visualizations in your Hyperwall presentation, we'll need to know which element on which page. On the visualization's web page, below the visual you'd like to use, you'll see a Link icon next to the Download button. All we need is for you to click on that icon and include that link in your presentation Powerpoint/Keynote or visualization list. Additionally, please check our Hyperwall How-To Guide for tips on designing your Hyperwall presentation, file specifications, and Powerpoint/Keynote templates.", "hits": 195 }, { "id": 40518, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-astrophysics-focus/", "result_type": "Gallery", "release_date": "2023-08-28T00:00:00-04:00", "title": "Hyperwall Power Playlist - Astrophysics Focus", "description": "This is a collection of our most powerful, newsworthy, and frequently used Hyperwall-ready visualizations, along with several that haven't gotten the attention they deserve. They're especially great for more general or top-level science talks, or to \"set the scene\" before a deep dive into a more focused subject or dataset. We've tried to cover the subject areas our speakers focus on most. \n\nIf you're not seeing what you're looking for, there is a huge library of visualizations more localized or specialized in subject - please use the Search function above, and filter \"Result type\" for \"Hyperwall Visual.\"\n\n If you'd like to use one of these visualizations in your Hyperwall presentation, we'll need to know which element on which page. On the visualization's web page, below the visual you'd like to use, you'll see a Link icon next to the Download button. All we need is for you to click on that icon and include that link in your presentation Powerpoint/Keynote or visualization list. Additionally, please check our Hyperwall How-To Guide for tips on designing your Hyperwall presentation, file specifications, and Powerpoint/Keynote templates.", "hits": 331 }, { "id": 5142, "url": "https://svs.gsfc.nasa.gov/5142/", "result_type": "Visualization", "release_date": "2023-08-24T10:45:00-04:00", "title": "TEMPO - Nitrogen Dioxide Air Pollution Over North America", "description": "High levels of nitrogen dioxide can be seen over multiple urban areas across the North America and the Caribbean. Detailed views of three regions show high levels of nitrogen dioxide over cities in the morning and enhanced levels of nitrogen dioxide over major highways. As the day progresses, morning pollution often dissipates then rises again as cities enter their second rush hour. Since TEMPO uses visible sunlight to make measurements, cloudy areas appear as missing data in the visualization.", "hits": 242 }, { "id": 5136, "url": "https://svs.gsfc.nasa.gov/5136/", "result_type": "Visualization", "release_date": "2023-08-22T00:00:00-04:00", "title": "STEREO-A Returns by Earth", "description": "The Solar Terrestrial Relations Observatory (STEREO) mission was launched on October 25, 2006, with the purpose of tracing the flow of energy and matter from the Sun to Earth. The STEREO mission began with two spacecraft: STEREO-A and STEREO-B. Each was launched into Sun-orbiting trajectories - STEREO-A moving ahead of Earth, and STEREO-B moving behind Earth (STEREO's Routes to Solar Orbits). In mid-August 2023, the still-operational STEREO-A (STEREO-B went offline in October 2014) will pass Earth for the first time since its launch 17 years ago. Like race cars driving different speeds around a circular track, STEREO-A is traveling slightly faster than Earth around the Sun. After launch, STEREO-A pulled ahead of Earth and extended its lead a little bit more with each orbit. Now, STEREO-A’s lead is so great that it is catching up to Earth from behind and is about to “lap” Earth, having completed 18 circuits around the Sun while Earth completed just 17. || ", "hits": 95 }, { "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": 14375, "url": "https://svs.gsfc.nasa.gov/14375/", "result_type": "Infographic", "release_date": "2023-06-27T10:00:00-04:00", "title": "NASA’s Roman and ESA’s Euclid Will Team Up To Investigate Dark Energy", "description": "Euclid (left) is a medium-class ESA mission. The Nancy Grace Roman Space Telescope (right) is an upcoming NASA flagship mission. Both will study the history of the universe and bring new insight to the mystery of dark energy.Credit: NASA's Goddard Space Flight Center; ESA/ATG medialab || Euclid-Roman_Graphic_Final.jpg (1920x1080) [476.1 KB] || Euclid-Roman_Graphic_Final_searchweb.png (320x180) [101.4 KB] || Euclid-Roman_Graphic_Final_thm.png (80x40) [7.9 KB] || ", "hits": 66 }, { "id": 14317, "url": "https://svs.gsfc.nasa.gov/14317/", "result_type": "Produced Video", "release_date": "2023-03-28T13:50:00-04:00", "title": "NASA Missions Probe What May Be a 1-In-10,000-Year Gamma-ray Burst", "description": "The Hubble Space Telescope’s Wide Field Camera 3 revealed the infrared afterglow (circled) of the BOAT GRB and its host galaxy, seen nearly edge-on as a sliver of light extending to the burst's upper left. This animation flips between images taken on Nov. 8 and Dec. 4, 2022, one and two months after the eruption. Given its brightness, the burst’s afterglow may remain detectable by telescopes for several years. Each picture combines three near-infrared images taken at wavelengths from 1 to 1.5 microns and is 34 arcseconds across. Credit: NASA, ESA, CSA, STScI, A. Levan (Radboud University); Image Processing: Gladys Kober || GRB_WFC3IR1108+1204_circled.gif (512x512) [3.5 MB] || ", "hits": 121 }, { "id": 14301, "url": "https://svs.gsfc.nasa.gov/14301/", "result_type": "Produced Video", "release_date": "2023-03-08T10:00:00-05:00", "title": "Millions of Galaxies Emerge in New Simulated Images From NASA's Roman", "description": "This video begins by showing the most distant galaxies in the simulated deep field image in red. As it zooms out, layers of nearer (yellow and white) galaxies are added to the frame. By studying different cosmic epochs, Roman will be able to trace the universe's expansion history, study how galaxies developed over time, and much more.Credit: Caltech-IPAC/R. Hurt and M. Troxel || Roman_Zoom_still.jpg (1920x1080) [515.9 KB] || Roman_Zoom_still_searchweb.png (320x180) [106.4 KB] || Roman_Zoom_still_thm.png (80x40) [6.6 KB] || Roman_Zoom-HD2K.mp4 (1920x1080) [25.3 MB] || Roman_Zoom-HD2K.webm (1920x1080) [2.7 MB] || ", "hits": 72 }, { "id": 5074, "url": "https://svs.gsfc.nasa.gov/5074/", "result_type": "Visualization", "release_date": "2023-02-15T15:00:00-05:00", "title": "Mons Mouton, a Newly Named Lunar Mountain", "description": "A view of the mountain with the Earth on the horizon. At the Moon's south pole, the south pole of the Earth is up. || earthview.0001_print.jpg (1024x576) [69.9 KB] || earthview.0001_searchweb.png (320x180) [40.5 KB] || earthview.0001_thm.png (80x40) [3.9 KB] || mouton_earthview_1080p30.mp4 (1920x1080) [2.1 MB] || mouton_earthview_720p30.mp4 (1280x720) [1.2 MB] || mouton_earthview_1920p30.mp4 (1080x1920) [2.7 MB] || earthview (1080x1920) [0 Item(s)] || mouton_earthview_720p30.webm (1280x720) [757.5 KB] || mouton_earthview_2160p30.mp4 (3840x2160) [5.5 MB] || mouton_earthview_360p30.mp4 (640x360) [448.1 KB] || earthview (3840x2160) [0 Item(s)] || mouton_earthview_1080p30.mp4.hwshow || ", "hits": 763 }, { "id": 5070, "url": "https://svs.gsfc.nasa.gov/5070/", "result_type": "Visualization", "release_date": "2023-02-06T00:00:00-05:00", "title": "Nitrogen Dioxide Over the United States, 2005-2022", "description": "NO2 over the United States as measured by OMI, with labels || NO2_US_2005-2022.399_print.jpg (1024x576) [171.6 KB] || NO2_US_2005-2022.399_searchweb.png (320x180) [80.6 KB] || NO2_US_2005-2022.399_thm.png (80x40) [5.9 KB] || w_dates (3840x2160) [0 Item(s)] || NO2_US_2005-2022_2160p30.mp4 (3840x2160) [20.0 MB] || NO2_US_2005-2022_2160p30.webm (3840x2160) [2.7 MB] || ", "hits": 198 }, { "id": 5024, "url": "https://svs.gsfc.nasa.gov/5024/", "result_type": "Visualization", "release_date": "2023-01-31T22:00:00-05:00", "title": "20 years of AIRS Global Carbon Dioxide (CO₂) measurements (2002-October 2022)", "description": "Data visualization of global carbon dioxide (CO₂) for the period September 2002-October 2022, showcasing data products from NASA's Aqua mission. Data visualization assets are designed for HD resolution. || co2airs_60South_1920x108030p.0794_print.jpg (1024x576) [170.8 KB] || 60South_exr (1920x1080) [0 Item(s)] || co2airs_60South_1920x1080p30.mp4 (1920x1080) [25.0 MB] || co2airs_60South_1920x108030p.0794.exr (1920x1080) [5.5 MB] || co2airs_60South_1920x1080p30.webm (1920x1080) [3.0 MB] || co2airs_60South_1920x1080p30.mp4.hwshow [194 bytes] || ", "hits": 133 }, { "id": 14276, "url": "https://svs.gsfc.nasa.gov/14276/", "result_type": "Produced Video", "release_date": "2023-01-12T08:00:00-05:00", "title": "Strong Solar Flare Erupts from Sun on January 10, 2023", "description": "An X1.0 class solar flare flashes on the left edge of the Sun on January 10, 2023. This image was captured by NASA's Solar Dynamics Observatory and shows a blend of light from the 304 and 131 angstrom wavelengths.Credit: NASA/GSFC/SDO || 1-10-23_2251UT_131_304_X1.jpg (4096x4096) [2.0 MB] || JHV_2023-01-10_18.38.48-0001.png (4096x4096) [19.1 MB] || 1-10-23_2251UT_131_304_X1_searchweb.png (320x180) [104.2 KB] || 1-10-23_2251UT_131_304_X1_thm.png (80x40) [6.9 KB] || ", "hits": 58 }, { "id": 14271, "url": "https://svs.gsfc.nasa.gov/14271/", "result_type": "Produced Video", "release_date": "2023-01-11T12:00:00-05:00", "title": "Sun Emits X1.9 Flare on January 9, 2023", "description": "An X1.9 class solar flare flashes on the left edge of the Sun on January 9, 2023. This image was captured by NASA's Solar Dynamics Observatory and shows a blend of light from the 171, 131 and 304 angstrom wavelengths.Credit: NASA/GSFC/SDO || Jan92023_1849UT_171-131-304_X1pt9.jpg (1034x972) [372.5 KB] || Jan92023_1849UT_171-131-304_X1pt9_searchweb.png (320x180) [106.8 KB] || Jan92023_1849UT_171-131-304_X1pt9_thm.png (80x40) [7.8 KB] || ", "hits": 27 }, { "id": 14209, "url": "https://svs.gsfc.nasa.gov/14209/", "result_type": "Produced Video", "release_date": "2023-01-09T17:10:00-05:00", "title": "NASA’s Compton Mission Glimpses Supersized Neutron Stars", "description": "This simulation tracks the gravitational wave and density changes as two orbiting neutron stars crash together. Dark purple colors represent the lowest densities, while yellow-white shows the highest. An audible tone and a visual frequency scale (at left) track the steady rise in the frequency of gravitational waves as the neutron stars close. When the objects merge at 42 seconds, the gravitational waves suddenly jump to frequencies of thousands of hertz and bounce between two primary tones (quasiperiodic oscillations, or QPOs). The presence of these signals in such simulations led to the search and discovery of similar phenomena in the light emitted by short gamma-ray bursts.Credit: NASA's Goddard Space Flight Center and STAG Research Centre/Peter HammondComplete transcript available.Watch this video on the NASA Goddard YouTube channel.Visual description:On a black background with a faint gray grid, two multicolored blobs representing merging neutron stars circle and close. The colors indicate density. Yellow-white indicates the highest densities, at the centers of the objects. The colors change to orange and red at their periphery, with purple colors representing matter torn from and swirling with the neutron stars as they orbit. The grid shrinks as the camera pulls back to capture a wider view of the merger. A pale orange display at left shows the changing frequency of the gravitational waves generated, which is also indicated by the rising tone. As the merger occurs, the screen shows a spinning yellow blob at center immersed in a large cloud of magneta and purple debris. || Merger_Simulation_Annotated_Still_2.jpg (1920x1080) [180.7 KB] || 14209_Hypermassive_QPO_Simulation_Zoom_YOUTUBE_1080.webm (1920x1080) [12.1 MB] || 14209_Hypermassive_QPO_Simulation_Zoom_YOUTUBE_1080.mp4 (1920x1080) [129.3 MB] || 14209_Hypermassive_QPO_Simulation_Zoom_YOUTUBE_BEST_1080.mp4 (1920x1080) [161.8 MB] || 14209_NS_Merger_QPO_SRT_Captions.en_US.srt [1.6 KB] || 14209_NS_Merger_QPO_SRT_Captions.en_US.vtt [1.6 KB] || 14209_Hypermassive_QPO_Simulation_Zoom_YOUTUBE_ProRes_1920x1080_2997.mov (1920x1080) [1.0 GB] || ", "hits": 261 }, { "id": 14270, "url": "https://svs.gsfc.nasa.gov/14270/", "result_type": "Produced Video", "release_date": "2023-01-06T16:00:00-05:00", "title": "Sun Emits X1.2 Flare on January 5, 2023", "description": "An X1.2 class solar flare flashes on the left edge of the Sun on January 5, 2023. This image was captured by NASA's Solar Dynamics Observatory and shows a blend of light from the 171 and 304 angstrom wavelengths.Credit: NASA/GSFC/SDO || 1-6-23_057UT_X1pt2Flare_304-171_4k.jpg (4096x4096) [3.2 MB] || 1-6-23_057UT_X1pt2Flare_304-171_4k_searchweb.png (320x180) [105.4 KB] || 1-6-23_057UT_X1pt2Flare_304-171_4k_thm.png (80x40) [7.7 KB] || ", "hits": 43 }, { "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": 14279, "url": "https://svs.gsfc.nasa.gov/14279/", "result_type": "Produced Video", "release_date": "2022-12-14T00:00:00-05:00", "title": "Mid-level Solar Flare Erupts from Sun on December 14, 2022", "description": "An M6.2 class solar flare flashes on the right side of the Sun on December 14, 2022. This imagery was captured by NASA's Solar Dynamics Observatory and shows light in the 131 angstrom wavelengths.Credit: NASA/SDO || M6pt3Flare12142022_131.gif (500x500) [4.5 MB] || ", "hits": 40 }, { "id": 5048, "url": "https://svs.gsfc.nasa.gov/5048/", "result_type": "Visualization", "release_date": "2022-11-09T13:00:00-05:00", "title": "Moon Phase and Libration, 2023", "description": "Dial-A-Moon || moon.0001.jpg (730x730) || comp.0001.tif (5760x3240) || || ", "hits": 1085 }, { "id": 5049, "url": "https://svs.gsfc.nasa.gov/5049/", "result_type": "Visualization", "release_date": "2022-11-09T13:00:00-05:00", "title": "Moon Phase and Libration, 2023 South Up", "description": "Dial-A-Moon || moon.0001.jpg (730x730) || comp.0001.tif (5760x3240) || || ", "hits": 164 }, { "id": 14275, "url": "https://svs.gsfc.nasa.gov/14275/", "result_type": "Produced Video", "release_date": "2022-10-02T07:00:00-04:00", "title": "Sun Releases X1.0 Flare on October 2, 2022", "description": "An X1.0 class solar flare flashes on the right edge of the Sun on October 2, 2022. This image was captured by NASA's Solar Dynamics Observatory and shows a blend of light from the 171 and 304 angstrom wavelengths.Credit: NASA/GSFC/SDO || Oct_2_2022_X1_flare_131-171.jpg (4096x4096) [3.8 MB] || Oct_2_2022_X1_flare_131-171_searchweb.png (320x180) [98.8 KB] || Oct_2_2022_X1_flare_131-171_thm.png (80x40) [7.7 KB] || ", "hits": 35 }, { "id": 5025, "url": "https://svs.gsfc.nasa.gov/5025/", "result_type": "Visualization", "release_date": "2022-09-14T17:30:00-04:00", "title": "20 years of AIRS Global Carbon Dioxide (CO₂) measurements (2002-May 2022)", "description": "Data visualization of global carbon dioxide (CO₂) for the period September 2002-May 2022, showcasing data products from NASA's Aqua mission. Data visualization assets are designed for HD resolution. || co2airs_60South_1920x108030p.0779.png (1920x1080) [1.8 MB] || co2airs_60South_1920x108030p.0779_print.jpg (1024x576) [171.8 KB] || co2airs_60South_1920x108030p.mp4 (1920x1080) [31.8 MB] || 60South_exr (1920x1080) [0 Item(s)] || co2airs_60South_1920x108030p.webm (1920x1080) [3.0 MB] || co2airs_60South_1920x108030p.mp4.hwshow [194 bytes] || ", "hits": 54 }, { "id": 4963, "url": "https://svs.gsfc.nasa.gov/4963/", "result_type": "Visualization", "release_date": "2022-08-19T00:00:00-04:00", "title": "Fifty Days of Continuous Sun from Solar Dynamics Observatory (171A filter)", "description": "Solar Dynamics Observatory (SDO) operates in a geosynchronous orbit around Earth to obtain a continuous view of the Sun. The particular instrument in this visualization records imagery in the ultraviolet portion of the spectrum at wavelengths normally absorbed by Earth's atmosphere - so we need to observe them from space.This movie was generated as a test case for a new movie pipeline for SDO, here's SDO AIA 171A imagery, sampled every two minutes for 50 days (April 12 through June 3, 2014), resulting in 30 minutes of continuous play (at 20 frames per second). || ", "hits": 43 }, { "id": 4990, "url": "https://svs.gsfc.nasa.gov/4990/", "result_type": "Visualization", "release_date": "2022-05-28T00:00:00-04:00", "title": "20 years of AIRS Global Carbon Dioxide (CO₂) measurements (2002- March 2022)", "description": "Data visualization of global carbon dioxide (CO2) for the period September 2002-March 2022, showcasing data products from NASA's Aqua mission. Data visualization assets are designed for HD resolution. || co2airs_60South_1920x108030p.0771.png (1920x1080) [1.8 MB] || co2airs_60South_1920x1080p30.mp4 (1920x1080) [24.2 MB] || composite_60South (1920x1080) [0 Item(s)] || co2airs_60South_1920x1080p30.webm (1920x1080) [2.9 MB] || co2airs_60South_1920x1080p30.mp4.hwshow [228 bytes] || ", "hits": 80 }, { "id": 14160, "url": "https://svs.gsfc.nasa.gov/14160/", "result_type": "Produced Video", "release_date": "2022-05-21T13:00:00-04:00", "title": "Sun Emits X1.5 Flare on May 10, 2022", "description": "Short video of the X1.5 flare emitted by the Sun on May 10, 2022 and captured by the Solar Dynamics Observatory in three wavelengths of extreme ultraviolet light that highlight different temperatures and features of the Sun's atmosphere, the corona.Credit: NASA/GSFC/SDOMusic: \"Examples\" from Universal Production MusicComplete transcript available. || May102022_X1pt5Flare_171-131-304.jpg (1920x1080) [979.2 KB] || May102022_X1pt5Flare_171-131-304_searchweb.png (320x180) [55.6 KB] || May102022_X1pt5Flare_171-131-304_thm.png (80x40) [4.4 KB] || 14160_May102022_X1pt5_Flare_ProRes_1920x1080_2997.mov (1920x1080) [829.3 MB] || 14160_May102022_X1pt5_Flare_Best_1080.mp4 (1920x1080) [138.6 MB] || 14160_May102022_X1pt5_Flare_1080.mp4 (1920x1080) [57.0 MB] || 14160_May102022_X1pt5_Flare_ProRes_1920x1080_2997.webm (1920x1080) [5.6 MB] || 14160_May102022_X1pt5_Flare_SRT_Captions.en_US.srt [547 bytes] || 14160_May102022_X1pt5_Flare_SRT_Captions.en_US.vtt [560 bytes] || ", "hits": 62 }, { "id": 14159, "url": "https://svs.gsfc.nasa.gov/14159/", "result_type": "Produced Video", "release_date": "2022-05-06T12:00:00-04:00", "title": "Active Sun in Early May, 2022", "description": "NASA’s Solar Dynamics Observatory captured this image of an X1.1 solar flare – as seen in the bright flash in the upper right portion of the image – on May 3, 2022 at 13:25 UTC. The image is a wavelength of extreme ultraviolet light – 131 angstrom – that highlights the extremely hot material in flares and which is colorized teal.Credit: NASA/SDO || 20220503_FlareX11_131A.00146_print.jpg (1024x1024) [302.4 KB] || 20220503_FlareX11_131A.00146_searchweb.png (320x180) [60.4 KB] || 20220503_FlareX11_131A.00146_thm.png (80x40) [5.1 KB] || 20220503_FlareX11_131A.00146.tiff (4096x4096) [64.0 MB] || ", "hits": 30 }, { "id": 14152, "url": "https://svs.gsfc.nasa.gov/14152/", "result_type": "Produced Video", "release_date": "2022-05-02T11:00:00-04:00", "title": "Strong Solar Flare Erupts from Sun on April 30, 2022", "description": "NASA’s Solar Dynamics Observatory captured this image sequence of an X1.1 solar flare – as seen in the bright flash in the upper right portion of the image – on April 30, 2022. The image is a blend of three wavelengths of extreme ultraviolet light that highlights the extremely hot material in flares and which is colorized in red. The three wavelengths are 131 angstrom, 171 angstrom and 304 angstrom. The sequence has a cadence of one image every 15 minutes and covers 8pm EDT April 29th to 8pm EDT April 30th.Credit: NASA/SDO || April_30_X1_flare_131-171-304.gif (500x500) [6.1 MB] || April_30_X1_flare_4k.mov (4096x4096) [654.3 MB] || April_30_X1_flare_4k.mp4 (4096x4096) [27.5 MB] || April_30_X1_flare_4k.webm (4096x4096) [4.9 MB] || ", "hits": 42 }, { "id": 14145, "url": "https://svs.gsfc.nasa.gov/14145/", "result_type": "Produced Video", "release_date": "2022-04-22T00:00:00-04:00", "title": "Late April Flares", "description": "NASA’s Solar Dynamics Observatory captured this image of an M9.6 solar flare – as seen in the bright flash in the upper left portion of the image– on April 20, 2022. The image shows a blend of 171 and 131 angstrom light, subsets of extreme ultraviolet light that highlight the extremely hot material in flares, and which are colorized in yellow. Credit NASA/SDO || April_21_M9pt6_Flare_171-131.jpg (4096x4096) [4.0 MB] || ", "hits": 55 }, { "id": 4994, "url": "https://svs.gsfc.nasa.gov/4994/", "result_type": "Visualization", "release_date": "2022-04-18T00:00:00-04:00", "title": "Nitrogen Dioxide Over the United States, 2005-2021", "description": "NO2 over the United States as measured by OMI, with labels || NO2_US_2021.0399_print.jpg (1024x576) [170.4 KB] || NO2_US_2021.0399_searchweb.png (320x180) [80.6 KB] || NO2_US_2021.0399_thm.png (80x40) [5.9 KB] || w_labels (3840x2160) [32.0 KB] || NO2_US_2021_2160p30.mp4 (3840x2160) [20.0 MB] || NO2_US_2021_2160p30.webm (3840x2160) [2.7 MB] || ", "hits": 66 }, { "id": 14119, "url": "https://svs.gsfc.nasa.gov/14119/", "result_type": "Produced Video", "release_date": "2022-04-15T15:00:00-04:00", "title": "52 Years and Counting - NASA Celebrates our Home Planet on Earth Day Live Shots", "description": "Quick link to associated B-ROLL for the live shotsClick here for more about how NASA is marking EARTH DAYQuick link to canned interview in Spanish with Santiago Gassó / NASA Earth ScientistQuick link to canned interview in English with Lesley Ott/ NASA Earth Scientist || Earthday_Banne_1.jpeg (1821x431) [151.1 KB] || Earthday_Banne_1_print.jpg (1024x242) [54.3 KB] || Earthday_Banne_1_searchweb.png (320x180) [85.4 KB] || Earthday_Banne_1_thm.png (80x40) [7.3 KB] || ", "hits": 38 }, { "id": 14129, "url": "https://svs.gsfc.nasa.gov/14129/", "result_type": "Produced Video", "release_date": "2022-04-01T07:00:00-04:00", "title": "Mid-level Solar Flare Erupts from Sun on March 31, 2022", "description": "This is a close-up image captured by NASA’s Solar Dynamics Observatory of today’s solar flare. The image shows a a blend of 131 and 171 angstrom extreme ultraviolet light that highlights the extremely hot material in flares.Credit: NASA/GSFC/SDO || March_31_M9pt7_flare_131-171_1080.jpg (1920x1080) [381.4 KB] || March_31_M9pt7_flare_131-171_1080_searchweb.png (320x180) [87.3 KB] || March_31_M9pt7_flare_131-171_1080_thm.png (80x40) [6.9 KB] || ", "hits": 69 }, { "id": 14128, "url": "https://svs.gsfc.nasa.gov/14128/", "result_type": "Produced Video", "release_date": "2022-03-30T16:00:00-04:00", "title": "Significant Solar Flare Erupts From Sun on March 30, 2022", "description": "An X1.3 class solar flare flashes in center of the Sun on Mar. 30, 2022. This image was captured by NASA's Solar Dynamics Observatory and shows a blend of light from the 171 and 131 angstrom wavelengths.Credit: NASA/GSFC/SDO || Mar302022FlareX1pt3_171-131Blend_2k.jpg (2048x2048) [617.2 KB] || Mar302022FlareX1pt3_171-131Blend_2k_print.jpg (1024x1024) [196.3 KB] || Mar302022FlareX1pt3_171-131Blend_2k_searchweb.png (320x180) [105.8 KB] || Mar302022FlareX1pt3_171-131Blend_2k_thm.png (80x40) [8.3 KB] || ", "hits": 60 }, { "id": 14105, "url": "https://svs.gsfc.nasa.gov/14105/", "result_type": "Produced Video", "release_date": "2022-03-22T10:00:00-04:00", "title": "Simulated Galaxy Redshift Cubes", "description": "This video dissolves between the entire collection of redshift cubes in 55 seconds. A shorter, faster version is available below.Credit: NASA’s Goddard Space Flight Center/F. Reddy and Z. Zhai, Y. Wang (IPAC) and A. Benson (Carnegie Observatories)Watch this video on the NASA.gov Video YouTube channel.Complete transcript available. || Cube_Spin_110-Short_mkII_still.jpg (1920x1080) [577.0 KB] || Cube_Spin_110-Short_mkII_still_print.jpg (1024x576) [158.1 KB] || Cube_Spin_110-Short_mkII_still_thm.png (80x40) [6.3 KB] || Cube_Spin_110-Short_mkII_still_searchweb.png (320x180) [79.4 KB] || 14105_110_RedshiftGalaxyCube_Dissolve_1080.mp4 (1920x1080) [59.2 MB] || 14105_110_RedshiftGalaxyCube_Dissolve_ProRes_1920x1080_2997.mov (1920x1080) [970.0 MB] || 14105_110_RedshiftGalaxyCube_Dissolve_1080.webm (1920x1080) [7.0 MB] || 14105_110_RedshiftGalaxyCube_Dissolve_SRT_Captions.en_US.srt [956 bytes] || 14105_110_RedshiftGalaxyCube_Dissolve_SRT_Captions.en_US.vtt [969 bytes] || ", "hits": 185 }, { "id": 4478, "url": "https://svs.gsfc.nasa.gov/4478/", "result_type": "Visualization", "release_date": "2022-03-18T09:00:00-04:00", "title": "The Reference Elevation Model of Antarctica (REMA)", "description": "This visualization explores the spatial resolution of the REMA data. The camera starts out at a global view of Antarctica before zooming into the Ross Archipelago region. RADARSAT DEM data is shown as the camera pushes in, showing the limits of the data resolution. A wipe transition reveals the REMA data, exposing additional details as the camera moves down towards the surface. Terrain is represented as a mesh to show the full resolution of the data. The camera flies up a valley, exploring the detailed REMA data. LIMA imagery is revealed at the end of the visualization. This video is also available on our YouTube channel. || REMA_comp_04_hw_04150_print.jpg (1024x576) [77.2 KB] || REMA_comp_04_hw_04150_searchweb.png (180x320) [45.3 KB] || REMA_comp_04_hw_04150_thm.png (80x40) [3.4 KB] || REMA_comp_04_4k_1080p30_2.webm (1920x1080) [21.7 MB] || REMA_comp_04_4k_1080p30_2.mp4 (1920x1080) [166.5 MB] || REMA_comp_04_4k_1080p60_2.mp4 (1920x1080) [171.3 MB] || captions_silent.25620.en_US.srt [43 bytes] || REMA_comp_04_4k_2160p30_2.mp4 (3840x2160) [587.2 MB] || REMA_comp_04_4k_2160p60_2.mp4 (3840x2160) [593.2 MB] || REMA_comp_04_4k_1080p30_2.mp4.hwshow [191 bytes] || ", "hits": 142 }, { "id": 4972, "url": "https://svs.gsfc.nasa.gov/4972/", "result_type": "Visualization", "release_date": "2022-03-09T09:00:00-05:00", "title": "Increasingly Dangerous Climate for Agricultural Workers", "description": "A warming climate will create challenges for agricultural workers. This visualization shows the increased number of days per year that are expected to have a NOAA Heat Index greater than 103 degrees Fahrenheit based on two different climate scenarios (SSP2-4.5 and SSP5-8.5). The visualization also plots the number of days exceeding this threshold for five select locations in the United States. The map projection in Robinson and the color map is cividis. || AgWorkerClimateGraph_4k.00899_print.jpg (1024x576) [152.0 KB] || AgWorkerClimateGraph_4k.00899_searchweb.png (180x320) [57.1 KB] || AgWorkerClimateGraph_4k.00899_thm.png (80x40) [5.8 KB] || AgWorkerClimateGraph_HD.mp4 (1920x1080) [13.8 MB] || AgWorkerClimateGraph_HD.webm (1920x1080) [3.4 MB] || AgWorkerClimateGraph_4k.mp4 (3840x2160) [37.3 MB] || AgWorkerClimateGraph_HD.mp4.hwshow [189 bytes] || ", "hits": 68 }, { "id": 14090, "url": "https://svs.gsfc.nasa.gov/14090/", "result_type": "Produced Video", "release_date": "2022-02-12T00:00:00-05:00", "title": "Fermi's 12-year View of the Gamma-ray Sky", "description": "This image shows the entire sky as seen by Fermi's Large Area Telescope. The most prominent feature is the bright, diffuse glow running along the middle of the map, which marks the central plane of our Milky Way galaxy. The gamma rays there are mostly produced when energetic particles accelerated in the shock waves of supernova remnants collide with gas atoms and even light between the stars. Many of the star-like features above and below the Milky Way plane are distant galaxies powered by supermassive black holes. Many of the bright sources along the plane are pulsars. The image was constructed from 12 years of observations using front-converting gamma rays with energies greater than 1 GeV. Hammer projection.Credit: NASA/DOE/Fermi LAT Collaboration || Fermi_144-month_Fermi_all-sky_hammer_2160x1080.png (2160x1080) [2.4 MB] || Fermi_144-month_Fermi_all-sky_hammer_2160x1080_print.jpg (1024x512) [306.6 KB] || Fermi_144-month_Fermi_all-sky_hammer_4000x2000.png (4000x2000) [7.0 MB] || Fermi_144-month_Fermi_all-sky_hammer_3600x1800.png (3600x1800) [4.9 MB] || ", "hits": 163 }, { "id": 40436, "url": "https://svs.gsfc.nasa.gov/gallery/black-hole-week/", "result_type": "Gallery", "release_date": "2022-02-12T00:00:00-05:00", "title": "Black Hole Week", "description": "This gallery brings together resources related to NASA’s Black Hole Week — videos, social media products, news stories, still images, and assets. This week is a celebration of celestial objects with gravity so intense that even light cannot escape them. Our goal is that no matter where people turn that week they will run into a black hole. (Figuratively, of course — we don’t want anyone falling in!)", "hits": 284 }, { "id": 14095, "url": "https://svs.gsfc.nasa.gov/14095/", "result_type": "Produced Video", "release_date": "2022-02-09T09:00:00-05:00", "title": "NASA’s New Views of Venus’ Surface From Space", "description": "NASA’s Parker Solar Probe has taken its first visible light images of the surface of Venus from space. Smothered in thick clouds, Venus’ surface is usually shrouded from sight. But in two recent flybys of the planet, Parker used its Wide-Field Imager, or WISPR, to image the entire nightside in wavelengths of the visible spectrum – the type of light that the human eye can see – and extending into the near-infrared.The images, combined into a video, reveal a faint glow from the surface that shows distinctive features like continental regions, plains, and plateaus. A luminescent halo of oxygen in the atmosphere can also be seen surrounding the planet.Link to NASA.gov feature.Link to associated research paper. || ", "hits": 861 }, { "id": 4957, "url": "https://svs.gsfc.nasa.gov/4957/", "result_type": "Visualization", "release_date": "2021-12-14T12:00:00-05:00", "title": "Parker Solar Probe: The Origins of Switchbacks", "description": "Most of the magnetic field measured at Parker during this time is directed sunward (blue field lines and vectors). A switchback occurs when the field changes direction almost 180 degrees for a short period of time. FIELDS instrument magnetic vector data are projected from the spacecraft position as arrows. The arrows are colored deep blue for sunward vectors, deep red for anti-sunward, and in between for directions off from this line. The heliospheric magnetic field lines are represented as gold. || ParkerSP.ChaseCloseupAft.Switchbacks20181106A.FIELDS.clockSlate_EarthTarget.HD1080.00990_print.jpg (1024x576) [114.9 KB] || ParkerSP.ChaseCloseupAft.Switchbacks20181106A.FIELDS.clockSlate_EarthTarget.HD1080.00990_searchweb.png (320x180) [71.7 KB] || ParkerSP.ChaseCloseupAft.Switchbacks20181106A.FIELDS.clockSlate_EarthTarget.HD1080.00990_thm.png (80x40) [4.5 KB] || Switchbacks20181106A (1920x1080) [0 Item(s)] || ParkerSP.ChaseCloseupAft.Switchbacks20181106A.FIELDS.HD1080_p30.mp4 (1920x1080) [25.7 MB] || ParkerSP.ChaseCloseupAft.Switchbacks20181106A.FIELDS.HD1080_p30.webm (1920x1080) [4.4 MB] || Switchbacks20181106A (3840x2160) [0 Item(s)] || ParkerSP.ChaseCloseupAft.Switchbacks20181106A.FIELDS.UHD3840_2160p30.mp4 (3840x2160) [100.2 MB] || ParkerSP.ChaseCloseupAft.Switchbacks20181106A.FIELDS.HD1080_p30.mp4.hwshow [229 bytes] || ", "hits": 87 }, { "id": 4958, "url": "https://svs.gsfc.nasa.gov/4958/", "result_type": "Visualization", "release_date": "2021-12-14T12:00:00-05:00", "title": "Parker Solar Probe: Crossing the Alfven Surface", "description": "Split window view illustrating the orbit of Parker with the orbit trail colored based on the Mach number of the solar wind and the magnetic field lines (represented as gold) connecting back to the Sun. The Mach number drops below unity (one) when a field line transitions between two different coronal hole regions (the blue and red regions marked on the Sun). || Parker_SolarCloseup.combo.HD1080.00480_print.jpg (1024x576) [121.9 KB] || Parker_SolarCloseup.combo.HD1080.00480_searchweb.png (320x180) [74.1 KB] || Parker_SolarCloseup.combo.HD1080.00480_thm.png (80x40) [5.2 KB] || Parker_SolarCloseup.combo.HD1080 (1920x1080) [0 Item(s)] || Parker_SolarCloseup.combo.HD1080_p30.mp4 (1920x1080) [45.8 MB] || Parker_SolarCloseup.combo.HD1080_p30.webm (1920x1080) [5.6 MB] || Parker_SolarCloseup.combo.UHD2160 (3840x2160) [0 Item(s)] || Parker_SolarCloseup.combo.UHD2160_p30.mp4 (3840x2160) [124.5 MB] || Parker_SolarCloseup.combo.HD1080_p30.mp4.hwshow [202 bytes] || ", "hits": 233 }, { "id": 14035, "url": "https://svs.gsfc.nasa.gov/14035/", "result_type": "Produced Video", "release_date": "2021-12-14T12:00:00-05:00", "title": "AGU 2021 - Major discoveries as NASA’s Parker Solar Probe closes in on the Sun", "description": "NASA’s Parker Solar Probe has now done what no spacecraft has done before—it has officially touched the Sun. Launched in 2018 to study the Sun’s biggest mysteries, the spacecraft has now grazed the edge of the solar atmosphere and gathered new close-up observations of our star. This is allowing us to see the Sun as never before—including the findings in two new papers, which were presented at AGU, that are helping scientists answer fundamental questions about the Sun.PANELISTSDr. Nicola Fox• Heliophysics Division Director of the Science Mission Directorate at NASA HeadquartersDr. Nour Raouafi• Project Scientist for NASA’s Parker Solar Probe• The Johns Hopkins Applied Physics Laboratory Dr. Justin Kasper• Principal Investigator for Solar Wind Electrons Alphas and Protons (SWEAP) Investigation on Parker Solar Probe • BWX Technologies, Inc., University of MichiganProf. Stuart D. Bale• Principal Investigator for Fields Experiment (FIELDS) on Parker Solar Probe • University of California, Berkeley Dr. Kelly Korreck• Program Scientist at NASA Headquarters• Smithsonian Astrophysical Observatory || ", "hits": 161 }, { "id": 4959, "url": "https://svs.gsfc.nasa.gov/4959/", "result_type": "Visualization", "release_date": "2021-12-13T00:00:00-05:00", "title": "Reduction in Tropospheric NOx and Ozone Corresponding to Worldwide COVID-19 Lockdowns", "description": "When the world went into lockdown to slow the spread of COVID-19, air pollution emissions started to rapidly decrease leaving a global atmospheric fingerprint detected by a team of scientists at NASA’s Jet Propulsion Laboratory using satellite measurements. These traces provided an unexpected window into what low-emissions world could look like, thus providing a means for identifying effective environmental policies. While many countries in the last few decades have implemented environmental policies to reduce human health risk from air pollution by controlling emissions, the impacts of those policies have not always been clear. The global lockdowns in response to COVID-19 represent a well-observed “scenario-of-opportunity” that allows us to assess how atmospheric emission and composition responds to reduced human activity. COVID-19 lockdowns effectively showed how reducing NOx emissions affects the global atmosphere. Its identifying signature shows up as in the atmosphere’s altered ability to produce harmful ozone pollution and ozone’s reduced influence on Earth’s heat balance that affects climate. These effects are not uniform across the world and depend on the location and season of the emission reductions.The results of this research indicate that in order to design effective environmental policies which benefit both air quality and climate, decision-makers need to carefully consider the complex relationships between emissions and atmospheric composition. || ", "hits": 40 }, { "id": 4955, "url": "https://svs.gsfc.nasa.gov/4955/", "result_type": "Visualization", "release_date": "2021-11-18T10:00:00-05:00", "title": "Moon Phase and Libration, 2022", "description": "Dial-A-Moon || moon.0001.jpg (730x730) || comp.0001.tif (5760x3240) || || ", "hits": 912 }, { "id": 4956, "url": "https://svs.gsfc.nasa.gov/4956/", "result_type": "Visualization", "release_date": "2021-11-18T09:59:00-05:00", "title": "Moon Phase and Libration, 2022 South Up", "description": "Dial-A-Moon || moon.0001.jpg (730x730) || comp.0001.tif (5760x3240) || || ", "hits": 352 }, { "id": 4954, "url": "https://svs.gsfc.nasa.gov/4954/", "result_type": "Visualization", "release_date": "2021-11-11T00:00:00-05:00", "title": "Mercury Makes Waves Cruising through the Solar Wind", "description": "Mercury orbits the Sun in a unique regime. The solar wind is still fresh from the Sun, and the Sun’s magnetic field strength (which drops with the square of distance) is rapidly waning. Furthermore, Mercury’s highly elliptical orbit means the planet passes through a wider range of distances from the Sun than any other planet. As a result, Mercury provides a unique opportunity to study how the Sun’s influence on a planet varies with distance.These animations provide a conceptual schematic of the results of one such investigation as described in “Occurrence rate of ultra-low frequency waves in the foreshock of Mercury increases with heliocentric distance.” Using data from NASA’s MESSENGER spacecraft, the authors has detected Ultra Low Frequency (ULF) waves rebounding from Mercury’s foreshock, the turbulent area where solar wind particles collide with Mercury’s magnetosphere. These waves are caused by solar wind protons – the steady stream of particles escaping the Sun –collide with and reflect off of this foreshock against the stream of the solar wind. The authors discovered that the ULF wave production rate varied throughout Mercury’s orbit. MESSENGER detected more ULF waves as Mercury moved farther from the Sun in its orbit, and fewer as it approached the Sun. The results support an existing theory that claimed that ULF waves are affected in part by the strength of the solar magnetic field, which is at its weakest when Mercury is farthest from the Sun. || ", "hits": 134 }, { "id": 13982, "url": "https://svs.gsfc.nasa.gov/13982/", "result_type": "Produced Video", "release_date": "2021-10-28T14:00:00-04:00", "title": "Active October Sun Emits X-class Flare", "description": "Brighter than a shimmering ghost, faster than the flick of a black cat’s tail, the Sun cast a spell in our direction, just in time for Halloween. This imagery captured by NASA’s Solar Dynamics Observatory covers a busy few days of activity between Oct. 25-28 that ended with a significant solar flare. From late afternoon Oct. 25 through mid-morning Oct. 26, an active region on the left limb of the Sun flickered with a series of small flares and petal-like eruptions of solar material. Meanwhile, the Sun was sporting more active regions at its lower center, directly facing Earth. On Oct. 28, the biggest of these released a significant flare, which peaked at 11:35 a.m. EDT. Credit: NASA/GSFC/SDOMusic: \"Immersion\" from Above and Below. Written and produced by Lars LeonhardWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || ActiveOctober_Still.jpg (1920x1080) [956.2 KB] || 13982_ActiveOctober_ProRes_1920x1080_2997.mov (1920x1080) [2.4 GB] || 13982_ActiveOctober_1080_Best.mp4 (1920x1080) [436.2 MB] || 13982_ActiveOctober_1080.mp4 (1920x1080) [188.1 MB] || 13982_ActiveOctober_1080_Best.webm (1920x1080) [19.7 MB] || 13982_ActiveOctober_SRT_Captions.en_US.srt [574 bytes] || 13982_ActiveOctober_SRT_Captions.en_US.vtt [587 bytes] || ", "hits": 74 } ] }