{ "count": 175, "next": "https://svs.gsfc.nasa.gov/api/search/?limit=100&offset=100&search=Spectrometer", "previous": null, "results": [ { "id": 14867, "url": "https://svs.gsfc.nasa.gov/14867/", "result_type": "Produced Video", "release_date": "2025-07-15T14:00:00-04:00", "title": "GEMx Animations", "description": "Conceptual animation illustrating the ER-2 aircraft collecting spectroscopic mineral data over the American West. || GEMxThumbnail.png (1948x1052) [1.5 MB] || GEMxThumbnail_print.jpg (1024x553) [118.0 KB] || GEMxThumbnail_searchweb.png (320x180) [55.7 KB] || GEMxThumbnail_thm.png (80x40) [8.2 KB] || GEMx_Interface_1080p.mov (1920x1080) [37.6 MB] || GEMx_Interface_4k.mp4 (3840x2160) [36.0 MB] || GEMx_Interface_ProRes.mov (3840x2160) [4.1 GB] || ", "hits": 62 }, { "id": 5566, "url": "https://svs.gsfc.nasa.gov/5566/", "result_type": "Animation", "release_date": "2025-07-03T14:59:59-04:00", "title": "TEMPO Air Quality Monitoring: Three Example Cases", "description": "Three visualizations demonstrating the air quality monitoring capabilities of the TEMPO mission.", "hits": 98 }, { "id": 31345, "url": "https://svs.gsfc.nasa.gov/31345/", "result_type": "Visualization", "release_date": "2025-06-11T18:59:59-04:00", "title": "One Year of PACE OCI Chlorophyll", "description": "The Ocean Color Instrument (OCI) on the Plankton, Aerosol, Cloud, ocean Ecosystem (PACE) satellite is a spectrometer designed to identify and quantify phytoplankton. This is a year-long visualization of the level 3 mapped chlorophyll data.", "hits": 121 }, { "id": 14851, "url": "https://svs.gsfc.nasa.gov/14851/", "result_type": "Produced Video", "release_date": "2025-06-04T14:00:00-04:00", "title": "GEMx Illustrations", "description": "Conceptual illustration depicting the ER-2 aircraft and the AVIRIS instrument searching for critical minerals as part of the GEMx campaign. || GEMx_Illustration_withTEXT_vFinal.png (3840x2160) [17.0 MB] || GEMx_Illustration_withTEXT_vFinal_print.jpg (1024x576) [287.6 KB] || GEMx_Illustration_withTEXT_vFinal_searchweb.png (320x180) [123.2 KB] || GEMx_Illustration_withTEXT_vFinal_thm.png (80x40) [8.2 KB] || ", "hits": 31 }, { "id": 14838, "url": "https://svs.gsfc.nasa.gov/14838/", "result_type": "Produced Video", "release_date": "2025-05-14T00:00:00-04:00", "title": "NASA FireSense (Fort Stewart-Hunter Army Airfield, Georgia)", "description": "On April 14th-20th, 2025, NASA’s FireSense project led a multi-agency prescribed burn research operation at Fort Stewart-Hunter Army Field, Georgia, in partnership with the U.S. Department of War (DoW). The DoW led the prescribed burn activities, while NASA FireSense coordinated field and airborne sampling with academic and agency partners, including the DoW Strategic Environmental Research and Development Program (SERDP) and DoW Environmental Security Technology Certification Program (ESTCP). The campaign targeted vegetation, fire, and smoke measurements, and aims to enhance understanding of fire behavior and smoke dynamics in order to provide actionable information to practitioners.NASA FireSense Website || ", "hits": 84 }, { "id": 14831, "url": "https://svs.gsfc.nasa.gov/14831/", "result_type": "Hyperwall Visual", "release_date": "2025-04-29T18:59:59-04:00", "title": "Seeing Earth as Only NASA Can", "description": "NASA's first image of Earth was taken by Explorer 6 in 1959. It was a grainy, black-and-white photo captured from 17,000 miles above the planet's surface and depicted little more than a sliver of cloud cover over the Pacific Ocean. Nearly 70 years later, NASA's vantage point of Earth has advanced dramatically — forever changing the way we see our home planet. As we continue reaching for the stars, training a careful eye on Earth keeps things in perspective.", "hits": 648 }, { "id": 14830, "url": "https://svs.gsfc.nasa.gov/14830/", "result_type": "Produced Video", "release_date": "2025-04-23T09:00:00-04:00", "title": "Carruthers Geocorona Observatory Images", "description": "The Carruthers Geocorona Observatory is a SmallSat mission at Lagrange Point 1 (L1) where it will use an advanced ultraviolet imager to monitor Earth’s exosphere — the outermost layer of the atmosphere — and the exosphere’s response to solar-driven space weather. Carruthers is poised to become the first SmallSat to operate at L1 and the first to deliver continuous exospheric observations from this vantage point.Led by the University of Illinois Urbana-Champaign, the mission is scheduled to launch no earlier than 2025 as a rideshare component of NASA’s Interstellar Mapping and Acceleration Probe (IMAP) mission, which will explore the boundaries of the heliosphere, the bubble that is inflated by the solar wind and surrounds the Sun and planets. The Carruthers Geocorona Observatory is a vital addition to NASA’s fleet of heliophysics satellites. NASA Heliophysics Division missions study a vast, interconnected system from the Sun to the space surrounding Earth and other planets to the farthest limits of the Sun’s constantly flowing streams of solar wind. || ", "hits": 115 }, { "id": 14808, "url": "https://svs.gsfc.nasa.gov/14808/", "result_type": "Produced Video", "release_date": "2025-03-24T15:00:00-04:00", "title": "Largest Organics Yet Discovered on Mars", "description": "Researchers analyzing pulverized rock onboard NASA’s Curiosity rover have found the largest organic compounds on the Red Planet to date.Complete transcript available.Universal Production Music: “Labyrinth of Discovery” by Emma Zarobyan [SOCAN]Watch this video on the NASA Goddard YouTube channel. || Mars_Large_Organics_Thumbnail_V3_print.jpg (1024x576) [234.9 KB] || Mars_Large_Organics_Thumbnail_V3.jpg (1280x720) [810.1 KB] || Mars_Large_Organics_Thumbnail_V3.png (1280x720) [1.3 MB] || Mars_Large_Organics_Thumbnail_V3_searchweb.png (320x180) [103.3 KB] || Mars_Large_Organics_Thumbnail_V3_thm.png [7.1 KB] || Mars_Large_Organics_Thumbnail_V3_web.png (320x180) [103.3 KB] || 14808_Mars_Large_Organics_720.mp4 (1280x720) [23.4 MB] || 14808_Mars_Large_Organics_1080.mp4 (1920x1080) [131.1 MB] || MarsLargeOrganicsCaptions.en_US.srt [2.1 KB] || MarsLargeOrganicsCaptions.en_US.vtt [2.0 KB] || 14808_Mars_Large_Organics_4K.mp4 (3840x2160) [1.6 GB] || 14808_Mars_Large_Organics_ProRes.mov (3840x2160) [9.7 GB] || ", "hits": 461 }, { "id": 14781, "url": "https://svs.gsfc.nasa.gov/14781/", "result_type": "Produced Video", "release_date": "2025-02-25T13:00:00-05:00", "title": "NASA Interview Opportunities: Two Moon Deliveries with NASA Instruments Days from Landing", "description": "Associated cut b-roll will be added by 5 p.m. EST on Thursday, Feb. 27. || CLPS.jpeg (1800x720) [219.2 KB] || CLPS_print.jpg (1024x409) [94.0 KB] || CLPS_searchweb.png (320x180) [46.3 KB] || CLPS_thm.png [5.8 KB] || ", "hits": 379 }, { "id": 14728, "url": "https://svs.gsfc.nasa.gov/14728/", "result_type": "B-Roll", "release_date": "2024-12-06T12:00:00-05:00", "title": "Geological Earth Mapping Experiment (GEMx) B-roll", "description": "The Geological Earth Mapping Experiment (GEMx) is a joint campaign between NASA and the U.S. Geological Survey (USGS) to map portions of the southwest United States for critical minerals using advanced airborne imaging. Spectral data from hundreds of wavelengths of reflected light can provide new information about Earth’s surface and atmosphere to help scientists understand Earth’s geology and biology, as well as the effects of climate change. The research project will use NASA’s Airborne Visible/Infrared Imaging Spectrometer (AVIRIS), the Modified Daedalus Wildfire scanning spectrometer (MASTER), and other airborne spectrocopic instruments flown on NASA’s ER-2 and Gulfstream V aircraft to collect the measurements over the country’s arid and semi-arid regions, including parts of California, Nevada, Arizona, and New Mexico.GEMx VISIONS PortalGEMx Campaign Information || ", "hits": 31 }, { "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": 550 }, { "id": 14650, "url": "https://svs.gsfc.nasa.gov/14650/", "result_type": "Produced Video", "release_date": "2024-11-25T00:00:00-05:00", "title": "EXCITE 2024: Infrared Detector and Spectrometer", "description": "EXCITE (EXoplanet Climate Infrared TElescope) is designed to study atmospheres around exoplanets, or worlds beyond our solar system, during long-duration scientific balloon trips over Antarctica.These images, taken in July 2024, show Peter Nagler and Nat DeNigris preparing EXCITE’s infrared detector and installing it into the mission’s spectrometer at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. At the time, the EXCITE team was gearing up for a test flight in Fort Sumner, New Mexico. || ", "hits": 45 }, { "id": 5389, "url": "https://svs.gsfc.nasa.gov/5389/", "result_type": "Visualization", "release_date": "2024-11-14T00:00:00-05:00", "title": "Tracking methane with EMIT and AVIRIS-3", "description": "Methane plumes can now be detected using the airborne AVIRIS-3 spectrometer in addition to EMIT on the International Space Station.", "hits": 174 }, { "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": 69 }, { "id": 5272, "url": "https://svs.gsfc.nasa.gov/5272/", "result_type": "Visualization", "release_date": "2024-05-21T08:00:00-04:00", "title": "Methane plumes detected by EMIT Space Mission", "description": "The Earth Surface Mineral Dust Source Investigation (EMIT) mission uses an imaging spectrometer to detect the unique pattern of reflected and absorbed light – called a spectral fingerprint – from various materials on Earth's surface and in its atmosphere. Perched on the International Space Station, EMIT was originally intended to map the prevalence of minerals in Earth's arid regions, such as the deserts of Africa and Australia. Scientists verified that EMIT could also detect the spectral fingerprints of methane and carbon dioxide which enables mapping of emissions from the energy, waste, and agriculture sectors. || ", "hits": 140 }, { "id": 14584, "url": "https://svs.gsfc.nasa.gov/14584/", "result_type": "Produced Video", "release_date": "2024-05-08T09:00:00-04:00", "title": "XRISM Spots Iron Fingerprints in Nearby Active Galaxy", "description": "The Resolve instrument aboard XRISM (X-ray Imaging and Spectroscopy Mission) captured data from the center of galaxy NGC 4151, where a supermassive black hole is slowly consuming material from the surrounding accretion disk. The resulting spectrum reveals the presence of iron in the peak around 6.5 keV and the dips around 7 keV, light thousands of times more energetic that what our eyes can see. Background: An image of NGC 4151 constructed from a combination of X-ray, optical, and radio light. Credit: Spectrum: JAXA/NASA/XRISM Resolve. Background: X-rays, NASA/CXC/CfA/J.Wang et al.; optical, Isaac Newton Group of Telescopes, La Palma/Jacobus Kapteyn Telescope; radio, NSF/NRAO/VLAAlt text: A XRISM spectrum of NGC 4151 with a multiwavelength snapshot of the galaxy in the background. Descriptive text: The spectrum image is labeled, “XRISM Resolve Spectrum of NGC 4151.” It shows a graph where the bottom is labeled, “X-ray energy (keV),” with a range from 5 to 9. The left side is labeled, “X-ray brightness.” A squiggly white line starts just under halfway up the left side. It peaks at just under 6.5 keV, nearly reaching the top of the graph. Then it starts to slope gently downward, with several sharp dips around 7 keV. In the background is a dim image of galaxy NGC 4151, where the center is a whiteish blue, surrounding by clouds of red and yellow. || Spectrum_v4.jpg (2300x2050) [426.6 KB] || ", "hits": 121 }, { "id": 14463, "url": "https://svs.gsfc.nasa.gov/14463/", "result_type": "Produced Video", "release_date": "2024-04-30T11:00:00-04:00", "title": "XRISM Mission Captures Unmatched Data With Just 36 Pixels", "description": "Watch to learn more about how the Resolve instrument aboard XRISM captures extraordinary data on the make-up of galaxy clusters, exploded stars, and more using only 36 pixels.Credit: NASA’s Goddard Space Flight CenterMusic: \"Stop and Hide\" and \"Wading Through\" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || XRISM_36_Pixels_Still.jpg (1920x1080) [959.9 KB] || XRISM_36_Pixels_Still_searchweb.png (320x180) [94.7 KB] || XRISM_36_Pixels_Still_thm.png (80x40) [7.0 KB] || 14463_XRISM_36Pixels_Good.mp4 (1920x1080) [148.9 MB] || 14463_XRISM_36Pixels_Best.mp4 (1920x1080) [514.8 MB] || 14463_XRISM_36Pixels_Captions.en_US.srt [4.6 KB] || 14463_XRISM_36Pixels_Captions.en_US.vtt [4.4 KB] || 14463_XRISM_36Pixels_ProRes_1920x1080_2997.mov (1920x1080) [2.4 GB] || ", "hits": 72 }, { "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": 130 }, { "id": 14405, "url": "https://svs.gsfc.nasa.gov/14405/", "result_type": "Produced Video", "release_date": "2023-08-25T10:00:00-04:00", "title": "XRISM: Exploring the Hidden X-ray Cosmos", "description": "Watch this video to learn more about XRISM (X-ray Imaging and Spectroscopy Mission), a collaboration between JAXA (Japan Aerospace Exploration Agency) and NASA.Credit: NASA's Goddard Space Flight CenterMusic Credits: Universal Production MusicLights On by Hugh Robert Edwin Wilkinson Dreams by Jez Fox and Rohan JonesChanging Tide by Rob ManningWandering Imagination by Joel GoodmanIn Unison by Samuel Sim || YTframe_XRISM_Exploring_XrayCosmos.jpg (1280x720) [668.5 KB] || YTframe_XRISM_Exploring_XrayCosmos_searchweb.png (320x180) [100.3 KB] || YTframe_XRISM_Exploring_XrayCosmos_thm.png (80x40) [7.6 KB] || XRISM_Exploring_the_Hidden_Xray_Cosmos.en_US_FR.en_US.srt [7.8 KB] || XRISM_Exploring_the_Hidden_Xray_Cosmos.en_US_FR.en_US.vtt [7.4 KB] || XRISM_Exploring_the_Hidden_Xray_Cosmos.webm (3840x2160) [107.8 MB] || XRISM_Exploring_the_Hidden_Xray_Cosmos.mp4 (3840x2160) [3.4 GB] || XRISM_Exploring_the_Hidden_Xray_Cosmos.mov (3840x2160) [21.6 GB] || ", "hits": 234 }, { "id": 12956, "url": "https://svs.gsfc.nasa.gov/12956/", "result_type": "Produced Video", "release_date": "2023-08-15T10:00:00-04:00", "title": "Spectroscopy, Explained", "description": "Video producer Sophia Roberts explains the basic principles behind spectroscopy, the science of reading light to determine the size, distance, spin and chemical composition of distant objects in space. Complete transcript available.Music Credits:Universal Production MusicOxygenate the Idea – by Amon Turner, Banksman, Eben StoneJungle Bounce – by Siddharth NadkarniSilent Patient – by Paul Reeves Background Story - by Peter LarsenData Dynamism – by Florian Moenks and Aron Wright Watch this video on the NASA Goddard YouTube channel. || Spectroscopy,_Explained_Thumbnail.jpg (3840x2160) [2.2 MB] || Spectroscopy,_Explained_Thumbnail_searchweb.png (320x180) [75.1 KB] || Spectroscopy,_Explained_Thumbnail_thm.png (80x40) [6.3 KB] || Spectroscopy,_Explained_Final_1080.mp4 (1920x1080) [412.9 MB] || SpectroscopyExplainedAdjustedCaptions.en_US.srt [11.1 KB] || SpectroscopyExplainedAdjustedCaptions.en_US.vtt [10.5 KB] || Spectroscopy_Explained.webm (3840x2160) [125.6 MB] || Spectroscopy_Explained.mp4 (3840x2160) [1.1 GB] || Spectroscopy,_Explained_Final_Best_4k.mp4 (3840x2160) [2.5 GB] || Spectroscopy,_Explained_Final_ProRes.mov (3840x2160) [43.3 GB] || ", "hits": 349 }, { "id": 14374, "url": "https://svs.gsfc.nasa.gov/14374/", "result_type": "Infographic", "release_date": "2023-08-03T11:00:00-04:00", "title": "A Guide to Cosmic Temperatures", "description": "Explore the temperatures of the cosmos, from absolute zero to the hottest temperatures yet achieved, with this infographic. Targets for the XRISM mission include supernova remnants, binary systems with stellar-mass black holes, galaxies powered by supermassive black holes, and vast clusters of galaxies.Credit: NASA's Goddard Space Flight Center/Scott WiessingerMachine-readable PDF copy || Cosmic_Temperatures_Infographic_Final_small.jpg (1383x2048) [1.3 MB] || Cosmic_Temperatures_Infographic_Final_Full.png (5530x8192) [60.5 MB] || Cosmic_Temperatures_Infographic_Final_Full.jpg (5530x8192) [10.3 MB] || Cosmic_Temperatures_Infographic_Final_8bit.png (5530x8192) [24.5 MB] || Cosmic_Temperatures_Infographic_Final_Half.png (2765x4096) [7.0 MB] || Cosmic_Temperatures_Infographic_Final_Half.jpg (2765x4096) [4.7 MB] || ", "hits": 968 }, { "id": 14340, "url": "https://svs.gsfc.nasa.gov/14340/", "result_type": "Produced Video", "release_date": "2023-04-27T10:00:00-04:00", "title": "VP Kamala Harris and President of the Republic of Korea Yoon Suk Yeol at NASA’s Goddard Space Flight Center", "description": "B-roll of the tour with Vice President Kamala Harris and President of the Republic of Korea Yoon Suk Yeol || VPOTUS_KoreanPresident_Visit_GSFC.00168_print.jpg (1024x576) [103.2 KB] || VPOTUS_KoreanPresident_Visit_GSFC.00168_searchweb.png (320x180) [81.3 KB] || VPOTUS_KoreanPresident_Visit_GSFC.00168_thm.png (80x40) [6.8 KB] || VPOTUS_KoreanPresident_Visit_GSFC.mov (1920x1080) [6.4 GB] || VPOTUS_KoreanPresident_Visit_GSFC.mp4 (1920x1080) [859.0 MB] || VPOTUS_KoreanPresident_Visit_GSFC.webm (1920x1080) [26.4 MB] || Tour_Captions.en_US.srt [1.3 KB] || Tour_Captions.en_US.vtt [1.2 KB] || ", "hits": 27 }, { "id": 31219, "url": "https://svs.gsfc.nasa.gov/31219/", "result_type": "Hyperwall Visual", "release_date": "2023-03-29T00:00:00-04:00", "title": "ABoVe Methane Airborne", "description": "ABoVE video and visualization || ABoVe_Methane_airborne.00180_print.jpg (1024x576) [298.9 KB] || ABoVe_Methane_airborne.00180_searchweb.png (320x180) [121.2 KB] || ABoVe_Methane_airborne.00180_thm.png (80x40) [7.7 KB] || ABoVE-update_1080p30.webm (1920x1080) [17.1 MB] || ABoVE-update_1080p30.mp4 (1920x1080) [131.4 MB] || v2 (3840x2160) [0 Item(s)] || ABoVE-update_2160p30.mp4 (3840x2160) [426.5 MB] || ", "hits": 39 }, { "id": 40456, "url": "https://svs.gsfc.nasa.gov/gallery/xrism/", "result_type": "Gallery", "release_date": "2023-02-03T00:00:00-05:00", "title": "XRISM", "description": "XRISM (X-ray Imaging and Spectroscopy Mission) is a JAXA/NASA collaborative mission with ESA participation. It launched from Japan in September of 2023 and is investigating the X-ray sky using high-resolution spectroscopy and imaging.", "hits": 285 }, { "id": 20374, "url": "https://svs.gsfc.nasa.gov/20374/", "result_type": "Animation", "release_date": "2022-12-12T00:00:00-05:00", "title": "XRISM Beauty Shots", "description": "XRISM turntable animations, available both as 4K/30 and 60 fps movies and as frames. The exposed tank behind the truss structure on the side opposite the solar panels houses the Resolve instrument.Credit: NASA's Goddard Space Flight Center Conceptual Image Lab || XRISM_360_4k_30fps_4444ProRes.00001_print.jpg (1024x576) [56.9 KB] || XRISM_360_4k_30fps_4444ProRes.00001_searchweb.png (180x320) [21.2 KB] || XRISM_360_4k_30fps_4444ProRes.00001_thm.png (80x40) [2.3 KB] || XRISM_360_4k_30fps_h264.mov (1920x1080) [25.3 MB] || XRISM_360_4k_60fps_h264.mov (1920x1080) [112.2 MB] || XRISM_360_4k_30fps (3840x2160) [0 Item(s)] || XRISM_360_4k_60fps (3840x2160) [0 Item(s)] || XRISM_360_4k_30fps_4444ProRes.webm [0 bytes] || XRISM_360_4k_30fps_h264.mp4 (3840x2160) [24.7 MB] || XRISM_360_4k_60fps_h264.mp4 (3840x2160) [73.8 MB] || XRISM_360_4k_30fps_4444ProRes.mov (3840x2160) [1.7 GB] || XRISM_360_4k_60fps_4444ProRes.mov (3840x2160) [10.0 GB] || ", "hits": 47 }, { "id": 14244, "url": "https://svs.gsfc.nasa.gov/14244/", "result_type": "Produced Video", "release_date": "2022-11-25T00:00:00-05:00", "title": "XRISM Resolve Animation", "description": "This animation illustrates how the microcalorimeter array at the heart of XRISM's revolutionary Resolve soft X-ray spectrometer works. X-ray light collected by a telescope strikes the detector. Each photon heats the material by an amount directly proportional to its energy. The instrument, which is cooled to 50 millikelvins, just above absolute zero, detects this minute temperature change.Credit: NASA's Goddard Space Flight Center || XRISM_Calorimeter-STILL_print.jpg (1024x576) [64.0 KB] || XRISM_Calorimeter-STILL.jpg (3840x2160) [716.3 KB] || XRISM_Calorimeter-STILL_searchweb.png (320x180) [55.3 KB] || XRISM_Calorimeter-STILL_thm.png (80x40) [5.5 KB] || XRISM_Calorimeter-STILL_web.png (320x180) [55.3 KB] || XRISM_Calorimeter-STILL.tiff (3840x2160) [63.3 MB] || XRISM_Calorimeter_Simple_ProRes_3840x2160_60.mov (3840x2160) [1.8 GB] || 3840x2160_16x9_60p (3840x2160) [64.0 KB] || XRISM_Calorimeter_Simple-H264_Best_3840x2160_5994.mov (3840x2160) [448.6 MB] || XRISM_Calorimeter_Simple-H264_Good_3840x2160_2997.mov (3840x2160) [27.1 MB] || XRISM_Calorimeter_Simple_ProRes_3840x2160_60.webm (3840x2160) [4.9 MB] || ", "hits": 141 }, { "id": 31200, "url": "https://svs.gsfc.nasa.gov/31200/", "result_type": "Hyperwall Visual", "release_date": "2022-11-01T07:00:00-04:00", "title": "EMIT Spots Methane Hotspots", "description": "A plume of methane is detected flowing from an area southeast of Carlsbad, New Mexico. || PIA25592_new_mexico_methane.png (1547x805) [1.8 MB] || PIA25592_new_mexico_methane_print.jpg (1024x532) [183.9 KB] || PIA25592_new_mexico_methane_searchweb.png (320x180) [109.3 KB] || PIA25592_new_mexico_methane_thm.png (80x40) [6.9 KB] || PIA25592_new_mexico_methane.hwshow [222 bytes] || ", "hits": 63 }, { "id": 14136, "url": "https://svs.gsfc.nasa.gov/14136/", "result_type": "Produced Video", "release_date": "2022-04-20T00:00:00-04:00", "title": "Webb Instrument Overview", "description": "A look at the instruments on the Webb Telescope. || Webb_Instruments-Thumbnail-2.jpg (1920x1080) [1.3 MB] || Webb_Instruments-Thumbnail-2_print.jpg (1024x576) [676.3 KB] || Webb_Instruments-Thumbnail-2_searchweb.png (320x180) [111.5 KB] || Webb_Instruments-Thumbnail-2_web.png (320x180) [111.5 KB] || Webb_Instruments-Thumbnail-2_thm.png (80x40) [13.8 KB] || WEBB_Instrument_Package-closecap.en_US.srt [4.9 KB] || WEBB_Instrument_Package.webm (4096x2160) [68.8 MB] || WEBB_Instrument_Package.mp4 (4096x2160) [276.0 MB] || ", "hits": 19 }, { "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": 64 }, { "id": 20345, "url": "https://svs.gsfc.nasa.gov/20345/", "result_type": "Animation", "release_date": "2022-03-01T00:00:00-05:00", "title": "TROPICS Mission Animations", "description": "The NASA Time-Resolved Observations of Precipitation structure and storm Intensity with a Constellation of Smallsats (TROPICS) mission is a constellation of state-of-the-science observing platforms that will measure temperature and humidity soundings and precipitation with spatial resolution comparable to current operational passive microwave sounders but with unprecedented temporal resolution (median revisit time of 50 minutes).Credit: NASA's Goddard Space Flight Center Conceptual Image Lab || Tropics_Beauty_Shot_ProRes.00540_print.jpg (1024x576) [95.4 KB] || Tropics_Beauty_Shot_H264_1080.mp4 (1920x1080) [76.4 MB] || Tropics_Beauty_Shot_H264_1080.webm (1920x1080) [3.4 MB] || Tropics_Beauty_Shot_H264_4k.mp4 (3840x2160) [309.1 MB] || Tropics_Beauty_Shot_ProRes.mov (3840x2160) [3.1 GB] || 3840x2160_16x9_30p (3840x2160) [64.0 KB] || Tropics_Beauty_Shot_ProRes.webm (3840x2160) [10.3 MB] || ", "hits": 40 }, { "id": 14112, "url": "https://svs.gsfc.nasa.gov/14112/", "result_type": "Produced Video", "release_date": "2022-02-28T07:00:00-05:00", "title": "Webb's Near Infrared Spectrograph (NIRSpec) Instrument Light Path Animation", "description": "Animation of the light path inside the Near Infrared Spectrometer (NIRSpec) on the Webb Telescope. Showing simulated data.Credit: European Space Agency || NIRSPEC_IFU_with_graph_v3.00030_print.jpg (1024x576) [39.9 KB] || NIRSPEC_IFU_with_graph_v3.00030_searchweb.png (320x180) [19.7 KB] || NIRSPEC_IFU_with_graph_v3.00030_web.png (320x180) [19.7 KB] || NIRSPEC_IFU_with_graph_v3.00030_thm.png (80x40) [2.1 KB] || NIRSPEC_IFU_with_graph_v3.mp4 (1920x1080) [311.7 MB] || NIRSPEC_IFU_with_graph_v3.webm (1920x1080) [12.7 MB] || ", "hits": 65 }, { "id": 14094, "url": "https://svs.gsfc.nasa.gov/14094/", "result_type": "Produced Video", "release_date": "2022-02-09T00:00:00-05:00", "title": "NASA Earth Valentines", "description": "We've got that look of love! Earth-observing satellites and astronauts capture our planet’s beauty every day. Share a Valentine with the one you can’t keep your eyes off of, inspired by some of our NASA missions. || ", "hits": 21 }, { "id": 20351, "url": "https://svs.gsfc.nasa.gov/20351/", "result_type": "Animation", "release_date": "2021-11-09T10:00:00-05:00", "title": "The DAVINCI Mission to Venus", "description": "DAVINCI the Movie || DaVinci1021cut422HQ.00130_print.jpg (1024x438) [75.7 KB] || DaVinci1021cut422HQ.00130_searchweb.png (180x320) [61.3 KB] || DaVinci1021cut422HQ.00130_thm.png (80x40) [5.3 KB] || DaVinci1021cut1080h264.mp4 (1920x820) [208.7 MB] || DaVinci1021cut720422HQ.mov (1682x720) [3.5 GB] || DaVinci1021cut720h264.mp4 (1280x548) [133.2 MB] || DaVinci1021cut720h264.webm (1280x548) [22.0 MB] || DaVinci1021cut422HQ.mov (5045x2160) [20.3 GB] || DaVinci1021cut1080422HQ.mov (2523x1080) [5.6 GB] || 20351_DAVINCIMissiontoVenus_CAPTIONS.en_US.srt [3.8 KB] || 20351_DAVINCIMissiontoVenus_CAPTIONS.en_US.vtt [3.6 KB] || ", "hits": 212 }, { "id": 13977, "url": "https://svs.gsfc.nasa.gov/13977/", "result_type": "Produced Video", "release_date": "2021-10-29T00:00:00-04:00", "title": "Tech on Deck series", "description": "The International Space Station photographed by Expedition 56 crew members from a Soyuz spacecraft after undocking.NExIS is NASA’s Exploration and In-space Services projects division. || iss_image.png (2614x1140) [4.5 MB] || iss_image_print.jpg (1024x446) [118.6 KB] || iss_image_web.png (320x139) [67.6 KB] || iss_image_thm.png (80x40) [9.6 KB] || ", "hits": 22 }, { "id": 13950, "url": "https://svs.gsfc.nasa.gov/13950/", "result_type": "Produced Video", "release_date": "2021-10-05T06:00:00-04:00", "title": "NASA Just Days Away From Launching Probe To Mysterious Asteroid Belt To Explore \"Fossils\" Of The Early Solar System Live Shots", "description": "Quick link to edited B-ROLL for the live shotsQuick link to canned interview with Donya Douglas-Bradshaw Lucy Project ManagerQuick link to canned interview with Cory Prykull, Lockheed Martin Space, Lucy Assembly, Test & Launch Operations Lead || Lucy_banner.png (1550x464) [1.3 MB] || Lucy_banner_print.jpg (1024x306) [134.8 KB] || Lucy_banner_searchweb.png (320x180) [139.1 KB] || Lucy_banner_thm.png (80x40) [12.5 KB] || ", "hits": 38 }, { "id": 31165, "url": "https://svs.gsfc.nasa.gov/31165/", "result_type": "Hyperwall Visual", "release_date": "2021-09-29T00:00:00-04:00", "title": "Tracking Power Plant Methane Emissions", "description": "A mosaic of AVIRIS-NG images tracks emissions from the Valley Generating Station in California || aviris-ng_methane_valley_generating_station_mosaic_print.jpg (1024x576) [231.4 KB] || aviris-ng_methane_valley_generating_station_mosaic.png (5760x3240) [28.1 MB] || aviris-ng_methane_valley_generating_station_mosaic_searchweb.png (320x180) [124.5 KB] || aviris-ng_methane_valley_generating_station_mosaic_thm.png (80x40) [6.0 KB] || aviris-ng_methane_valley_generating_station_mosaic.hwshow [261 bytes] || ", "hits": 27 }, { "id": 13809, "url": "https://svs.gsfc.nasa.gov/13809/", "result_type": "Produced Video", "release_date": "2021-02-10T09:55:00-05:00", "title": "Exploring Our Solar System with Dr. Amy Simon", "description": "Dr. Amy Simon has always been fascinated with space. From a young age she dreamed of lifting off in the Space Shuttle, just like her hero Sally Ride. Over the years her interest in space remained, and she eventually found herself working at NASA.Dr. Simon is the Senior Scientist for Planetary Atmospheres Research in the Solar System Exploration Division at the NASA Goddard Space Flight Center. Her scientific research involves the study of the composition, dynamics, and cloud structure in jovian planet atmospheres, primarily from spacecraft observations like the Hubble Space Telescope.Dr. Simon is also involved in multiple robotic flight missions, as well as future mission concept development. She was a co-investigator on the Cassini Composite Infrared Spectrometer (CIRS) and is the Deputy Instrument Scientist for the OSIRIS-REx Visible and near-IR Spectrometer (OVIRS), as well as the Landsat 9 TIRS2 instrument, and the Lucy L'Ralph instrument Deputy PI. She is PI of the Hubble Outer Planet Atmospheres Legacy (OPAL) program. She recently served as science co-lead of the NASA Ice Giants Mission Concept study.This inspiring woman shows the world that anything is possible, and that you should always work hard to follow your passion in life.For more information, visit https://nasa.gov/hubble. Music Credits: \"Falling Freet\" by Christian Tschuggnall [AKM] and Michael Edwards [APRA] via Atmosphere Music Ltd. [PRS] and Universal Production Music.“Darwin’s Extraordinary Journey” by Laurent Dury [SACEM] via Koka Media [SACEM], Universal Publishing Production Music France [SACEM] and Universal Production Music. || ", "hits": 257 }, { "id": 13280, "url": "https://svs.gsfc.nasa.gov/13280/", "result_type": "Produced Video", "release_date": "2020-08-19T00:00:00-04:00", "title": "Assembling XRISM's X-ray Mirrors", "description": "Team members Lawrence Lozipone of Stinger Ghaffarian Technologies, Inc. and Yang Soong, a researcher at the University of Maryland, College Park, work with flight mirrors for the X-ray Imaging and Spectroscopy Mission (XRISM). Nested aluminum mirror segments – 1,624 of them for each X-ray Mirror Assembly – focus the incoming X-rays for the satellite's science instruments. Credit: NASA's Goddard Space Flight Center || XRISM_Cleanroom_B-roll_1080Still.jpg (1920x1080) [727.5 KB] || XRISM_Cleanroom_B-roll_ProRes_1920x1080_30.mov (1920x1080) [7.0 GB] || XRISM_Cleanroom_B-roll_1080.mp4 (1920x1080) [991.6 MB] || XRISM_Cleanroom_B-roll_ProRes_1920x1080_30.webm (1920x1080) [52.0 MB] || ", "hits": 55 }, { "id": 13589, "url": "https://svs.gsfc.nasa.gov/13589/", "result_type": "Produced Video", "release_date": "2020-04-28T00:00:00-04:00", "title": "PACE OCI Instrument Under Construction", "description": "PACE's primary sensor, the Ocean Color Instrument (OCI), is a highly advanced optical spectrometer that will be used to measure properties of light over portions of the electromagnetic spectrum. It will enable continuous measurement of light at finer wavelength resolution than previous NASA satellite sensors, extending key system ocean color data records for climate studies.The color of the ocean is determined by the interaction of sunlight with substances or particles present in seawater such as chlorophyll, a green pigment found in most phytoplankton species. By monitoring global phytoplankton distribution and abundance with unprecedented detail, the OCI will help us to better understand the complex systems that drive ocean ecology. || 041320-OCI_Package_FINAL_MP4.00960_print.jpg (1024x576) [146.2 KB] || 041320-OCI_Package_FINAL_MP4.00960_searchweb.png (320x180) [109.4 KB] || 041320-OCI_Package_FINAL_MP4.00960_thm.png (80x40) [7.7 KB] || 041320-OCI_Package_FINAL_MP4.00960_web.png (320x180) [109.4 KB] || 041320-OCI_Package_FINAL_MP4.mp4 (1920x1080) [82.8 MB] || 041320-OCI_Package_FINAL_MP4.webm (1920x1080) [11.1 MB] || 041320OCI_Package_FINAL_MP4.en_US.srt [1.7 KB] || 041320OCI_Package_FINAL_MP4.en_US.vtt [1.7 KB] || ", "hits": 19 }, { "id": 13597, "url": "https://svs.gsfc.nasa.gov/13597/", "result_type": "Produced Video", "release_date": "2020-04-27T12:00:00-04:00", "title": "Animation of the NIRSpec Instrument", "description": "Turntable animation of the James Webb Space Telescope NIRSpec instrument. || NIRSPEC_TT.00001_print.jpg (1024x576) [32.2 KB] || NIRSPEC_TT.00001_searchweb.png (180x320) [29.8 KB] || NIRSPEC_TT.00001_thm.png (80x40) [2.2 KB] || NIRSPEC_TT.mov (3840x2160) [396.3 MB] || NIRSPEC_TT.mp4 (3840x2160) [14.6 MB] || NIRSPEC_TT.webm (3840x2160) [1.9 MB] || ", "hits": 65 }, { "id": 13568, "url": "https://svs.gsfc.nasa.gov/13568/", "result_type": "Produced Video", "release_date": "2020-03-02T10:00:00-05:00", "title": "OSIRIS-REx Observes a Black Hole", "description": "On Nov. 11, 2019, while the REXIS instrument was performing detailed science observations of Bennu, it captured X-rays radiating from a point off the asteroid’s edge. This video shows the REXIS team building the instrument and the data received when it glimpsed MAXI J0637-430.Music is \"Castles and Cathedrals\" from Universal Production Music. || 13568_thumb.jpg (3840x2160) [891.9 KB] || 13568_REXIS_BLACKHOLE_MASTER.00367_searchweb.png (320x180) [102.0 KB] || 13568_REXIS_BLACKHOLE_MASTER.00367_thm.png (80x40) [6.6 KB] || 13568_REXIS_BLACKHOLE_MASTER1_facebook_720.mp4 (1280x720) [124.5 MB] || 13568_REXIS_BLACKHOLE_MASTER1_twitter_720.mp4 (1280x720) [21.4 MB] || 13568_REXIS_BLACKHOLE_MASTER1.webm (960x540) [48.3 MB] || 13568_REXIS_BLACKHOLE_MASTER1.mov (3840x2160) [9.4 GB] || 13568_Caption.en_US.srt [2.6 KB] || 13568_Caption.en_US.vtt [2.6 KB] || ", "hits": 42 }, { "id": 13566, "url": "https://svs.gsfc.nasa.gov/13566/", "result_type": "Produced Video", "release_date": "2020-03-01T09:00:00-05:00", "title": "Hubble Archive - Servicing Mission 3B, STS-109", "description": "Servicing Mission 3B was actually the fourth visit to Hubble. NASA split the original Servicing Mission 3 into two parts and conducted 3A in December of 1999. During SM3B a new science instrument will be installed: the Advanced Camera for Surveys (ACS). Several other activities were accomplished as well over a 12-day mission with 5 spacewalks.Four astronauts trained for five scheduled spacewalks to upgrade and service the Hubble Space Telescope during the STS-109 mission in early 2002. Three veteran astronauts, John M.Grunsfeld, James H. Newman, and Richard M. Linnehan, were joined by Michael J. Massimino, who will be making his first space flight.Grunsfeld had flown three times, STS-67 in 1995, STS-81 in 1997, and STS-103 in 1999 when he performed two spacewalks to service the Hubble Space Telescope. Newman, veteran of three space flights, STS-51 in 1993, STS-69 in 1995, and STS-88 in 1998, had conducted four previous spacewalks. Linnehan had flown on STS-78 in 1996 and STS-90 in 1998. Massimino is a member of the 1996 astronaut class.Scott Altman, (Cmdr., USN), a two-time shuttle veteran, commanded the STS-109 mission. He was joined on the flight deck by pilot Duane Carey, (Lt. Col., USAF), making his first space flight, and flight engineer Nancy Currie (Lt. Col, USA, Ph.D.). Currie had three previous space flights to her credit. || ", "hits": 82 }, { "id": 13562, "url": "https://svs.gsfc.nasa.gov/13562/", "result_type": "Produced Video", "release_date": "2020-02-25T16:00:00-05:00", "title": "The Science of Dragonfly", "description": "Dragonfly’s suite of science instruments will investigate the chemistry and habitability of Titan.Universal Production Music: “Clediss” by Thomas Stempfle and Tom Sue, “Downloading Landscapes” by Andrew Michael Britton and David Stephen GoldsmithWatch this video on the NASA Goddard YouTube channel.Complete transcript available. || FACEBOOK_720_13562_Dragonfly_Science_MASTER_facebook_720.mp4 (1280x720) [145.8 MB] || DragonflySciencePreview_print.jpg (1024x576) [96.9 KB] || DragonflySciencePreview.jpg (3840x2160) [637.4 KB] || DragonflySciencePreview_searchweb.png (320x180) [72.4 KB] || DragonflySciencePreview_thm.png (80x40) [5.5 KB] || TWITTER_720_13562_Dragonfly_Science_MASTER_twitter_720.mp4 (1280x720) [27.2 MB] || 13562_Dragonfly_Science_MASTER.webm (960x540) [46.9 MB] || 13562_Dragonfly_Science_CAPTIONS.en_US.srt [3.4 KB] || 13562_Dragonfly_Science_CAPTIONS.en_US.vtt [3.4 KB] || 13562_Dragonfly_Science_YouTube.mp4 (3840x2160) [2.7 GB] || 13562_Dragonfly_Science_MASTER.mov (3840x2160) [16.6 GB] || ", "hits": 140 }, { "id": 20311, "url": "https://svs.gsfc.nasa.gov/20311/", "result_type": "Animation", "release_date": "2020-02-25T16:00:00-05:00", "title": "Dragonfly Animation Resource Page", "description": "Dragonfly on Titan || DF_End_Pan_4K_Prores.00420_print.jpg (1024x576) [77.6 KB] || DF_End_Pan_H264_1080.mp4 (1920x1080) [27.1 MB] || DF_End_Pan_4K_H264.mp4 (3840x2160) [15.4 MB] || DF_End_Pan_4K_Prores_PNG (3840x2160) [0 Item(s)] || DF_End_Pan_4K_Prores.webm (3840x2160) [7.0 MB] || DF_End_Pan_4K_Prores.mov (3840x2160) [1.7 GB] || ", "hits": 278 }, { "id": 13531, "url": "https://svs.gsfc.nasa.gov/13531/", "result_type": "Produced Video", "release_date": "2020-01-31T00:00:00-05:00", "title": "XRISM: Calorimeter Spectrometer Insert and Mirror Tests", "description": "XRISM team members pose with the XRISM Calorimeter Spectrometer Insert in a NASA Goddard clean room. From left to right, they are Bryan James, Mike Sampson, Tomomi Watanabe, Pete Barfknecht, Scott Porter, and Sinclair Douglas.Credit: Larry Gilbert/NASA || GSFC_20191101__2020-2568_07.jpg (3000x1995) [3.6 MB] || GSFC_20191101__2020-2568_07_searchweb.png (320x180) [111.9 KB] || GSFC_20191101__2020-2568_07_thm.png (80x40) [7.7 KB] || ", "hits": 57 }, { "id": 13530, "url": "https://svs.gsfc.nasa.gov/13530/", "result_type": "Produced Video", "release_date": "2020-01-30T00:00:00-05:00", "title": "Mirror Quadrants for XRISM", "description": "XRISM team member Yang Soong, a researcher at the University of Maryland, College Park, displays completed mirror elements for an X-ray Mirror Assembly developed for the JAXA/NASA mission. Credit: Taylor Mickal/NASA || GSFC_20190619_XRISM_XMA_Soong_06.jpg (6000x4000) [12.7 MB] || ", "hits": 85 }, { "id": 4755, "url": "https://svs.gsfc.nasa.gov/4755/", "result_type": "Visualization", "release_date": "2019-12-12T14:00:00-05:00", "title": "Mars Upper Level Winds Observed by MAVEN - Visualizations", "description": "MAVEN observes upper level Martian winds over the course of about two years. || maven_upper_winds_60fps.0104__cam_mainShape_190909182423_beauty.1780_print.jpg (1024x576) [42.9 KB] || maven_upper_winds_60fps.0104__cam_mainShape_190909182423_beauty.1780_searchweb.png (320x180) [49.1 KB] || maven_upper_winds_60fps.0104__cam_mainShape_190909182423_beauty.1780_thm.png (80x40) [4.0 KB] || maven_upper_winds_campaigns_1080p60.mp4 (1920x1080) [51.0 MB] || maven_upper_winds_campaigns_1080p30.mp4 (1920x1080) [46.4 MB] || maven_upper_winds.0104_cam_mainShape_190909182423_beauty_1080p30.webm (1920x1080) [9.6 MB] || campaigns (3840x2160) [0 Item(s)] || maven_upper_winds_campaigns_2160p60.mp4 (3840x2160) [162.2 MB] || maven_upper_winds_campaigns_2160p30.mp4 (3840x2160) [146.8 MB] || 4755_MAVEN_Wind_Currents_Full.mov (3840x2160) [9.7 GB] || maven_upper_winds_campaigns_1080p30.mp4.hwshow [201 bytes] || ", "hits": 55 }, { "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": 13207, "url": "https://svs.gsfc.nasa.gov/13207/", "result_type": "Produced Video", "release_date": "2019-07-12T10:00:00-04:00", "title": "OSIRIS-REx Social Media Interviews", "description": "This page contains interviews with personnel from the Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer (OSIRIS-REx) mission, edited for social media. The OSIRIS-REx spacecraft launched Sept. 8, 2016, and began orbiting asteroid Bennu on Dec. 31, 2018. Its primary science objective is to study Bennu and collect a sample for return to Earth in 2023. Bennu is a carbon-rich asteroid that records the earliest history of our solar system, and which may contain the raw ingredients of life. || ", "hits": 25 }, { "id": 13094, "url": "https://svs.gsfc.nasa.gov/13094/", "result_type": "Produced Video", "release_date": "2018-11-08T13:00:00-05:00", "title": "Multimessenger Timeline Resources", "description": "The media elements below appear in the multimessenger astronomy video \"Luck Favors the Prepared.\" || A simple animation of a gamma ray moving through space.Credit: NASA's Goddard Space Flight Center || Gamma_Ray_animation.00001_print.jpg (1024x576) [15.9 KB] || Gamma_Ray_animation.00001_print_searchweb.png (320x180) [22.1 KB] || Gamma_Ray_animation.00001_print_thm.png (80x40) [2.3 KB] || Gamma_Ray_animation.mov (1280x720) [51.5 MB] || Gamma_Ray_animation.webm (1280x720) [773.0 KB] || || ", "hits": 83 }, { "id": 4690, "url": "https://svs.gsfc.nasa.gov/4690/", "result_type": "Visualization", "release_date": "2018-10-31T00:00:00-04:00", "title": "Tracking Snow Water Equivalent in the Tuolumne Basin", "description": "This visualization focuses on the Tuolumne Basin, located within the boundaries of Yosemite National Park, which supplies water via the Hetch Hetchy aqueduct to the San Francisco Bay Area. Snow Water Equivalent (SWE) data collected by the Airborne Snow Observatory (ASO) between 2014 and 2017 is depicted in blues and whites, showing how the snowpack changes over time. This version includes a colorbar. || aso_wColorbar_1500_print.jpg (1024x576) [175.2 KB] || aso_wColorbar_1500_searchweb.png (320x180) [127.9 KB] || aso_wColorbar_1500_thm.png (80x40) [8.0 KB] || aso_tuolumne_wColorbar (1920x1080) [0 Item(s)] || aso_wColorbar_1080p30.mp4 (1920x1080) [60.8 MB] || aso_wColorbar_1080p30.webm (1920x1080) [7.6 MB] || aso_wColorbar_1080p30.mp4.hwshow [187 bytes] || ", "hits": 34 }, { "id": 4677, "url": "https://svs.gsfc.nasa.gov/4677/", "result_type": "Visualization", "release_date": "2018-08-27T00:00:00-04:00", "title": "2005-2016 USA NO2 Hyperwall Show", "description": "USA NO2, Updated to 2016 || USA_4_17_HW.0000_print.jpg (1024x576) [140.2 KB] || USA_4_17_HW.0000_searchweb.png (320x180) [75.5 KB] || USA_4_17_HW.0000_thm.png (80x40) [5.8 KB] || USA_4_17_HW_1080p30.mp4 (1920x1080) [5.0 MB] || 5760x3240_16x9_30p (5760x3240) [0 Item(s)] || USA_4_17_HW_2160p30.webm (3840x2160) [955.7 KB] || USA_4_17_HW_2160p30.mp4 (3840x2160) [16.4 MB] || USA_4_17_HW_1080p30.mp4.hwshow [185 bytes] || ", "hits": 32 }, { "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": 12967, "url": "https://svs.gsfc.nasa.gov/12967/", "result_type": "Produced Video", "release_date": "2018-06-07T13:00:00-04:00", "title": "Ancient Organics Discovered on Mars - Broadcast Graphics", "description": "NASA-TV graphics illustrating Curiosity's findings on Mars, broadcast on June 7, 2018 from Goddard Space Flight Center. All clips are formatted in 1280x720 or higher resolution. Learn more about this discovery. || ", "hits": 243 }, { "id": 12962, "url": "https://svs.gsfc.nasa.gov/12962/", "result_type": "Produced Video", "release_date": "2018-05-24T13:00:00-04:00", "title": "Searching for Signs of Life on Mars", "description": "The European Space Agency's Rosalind Franklin rover will search for signs of life on Mars, using a NASA-built instrument called MOMA. Complete transcript available.Watch this video on the NASA Goddard YouTube channel.Music provided by Killer Tracks: \"Fast Motion\" by Stephen Daniel Lemaire, \"Game Show Spheres 5-6\" by Anselm Kreuzer, \"Floating\" by Ben Niblett & Jon Cotton || ExoMarsPreview.jpg (1920x1080) [175.9 KB] || ExoMarsPreview_searchweb.png (320x180) [80.6 KB] || ExoMarsPreview_thm.png (80x40) [6.3 KB] || TWITTER_720_12962_MOMA_Profile_Master_APR_twitter_720.mp4 (1280x720) [69.5 MB] || 12962_MOMA_Profile_Master.webm (960x540) [125.9 MB] || FACEBOOK_720_12962_MOMA_Profile_Master_APR_facebook_720.mp4 (1280x720) [377.8 MB] || YOUTUBE_1080_12962_MOMA_Profile_Master_APR_youtube_1080.mp4 (1920x1080) [510.9 MB] || 12962_MOMA_Profile_Master_youtube_hq.mov (1920x1080) [856.3 MB] || 12962_MOMA_Profile_Master_APR_Output.en_US.srt [6.0 KB] || 12962_MOMA_Profile_Master_APR_Output.en_US.vtt [6.0 KB] || 12962_MOMA_Profile_Master_APR.mov (1920x1080) [7.2 GB] || Moma.hwshow [108 bytes] || ", "hits": 59 }, { "id": 20231, "url": "https://svs.gsfc.nasa.gov/20231/", "result_type": "Animation", "release_date": "2018-05-24T13:00:00-04:00", "title": "Mars Organic Molecule Analyzer: Animations", "description": "MOMA uses ultraviolet laser pulses to release and ionize organic compounds captured within crushed Martian surface and near-surface materials. Because each laser pulse lasts less than two billionths of a second, this process effectively ionizes more heat-resistant materials than those accessed by traditional oven-heating (pyrolysis) methods. Pulsed laser processing preserves weak molecular bonds, and enables the identification of organic compounds even in the presence of highly reactive perchlorates commonly found in Martian surface materials. || MOMAposterFull.jpg (1920x1080) [130.9 KB] || MOMAposterFull_print.jpg (1024x576) [73.3 KB] || MOMAposterFull_searchweb.png (320x180) [36.8 KB] || MOMAposterFull_web.png (320x180) [36.8 KB] || MOMAposterFull_thm.png (80x40) [3.7 KB] || ldms (1920x1080) [0 Item(s)] || MOMA-LDMS_h264.mp4 (1920x1080) [91.5 MB] || MOMA-LDMS_1080p60.mp4 (1920x1080) [24.4 MB] || MOMA-LDMS_1080p60.webm (1920x1080) [8.3 MB] || MOMA-LDMS.mov (1920x1080) [2.1 GB] || Moma-LDMS.hwshow [67 bytes] || ", "hits": 91 }, { "id": 13002, "url": "https://svs.gsfc.nasa.gov/13002/", "result_type": "B-Roll", "release_date": "2018-05-24T00:00:00-04:00", "title": "Mars Organic Molecule Analyzer: Footage", "description": "The Mars Organic Molecule Analyzer, or MOMA, is a miniaturized, highly sophisticated organic chemistry laboratory headed to the red planet aboard ESA's Rosalind Franklin rover (formerly ExoMars). The MOMA mass spectrometer subsystem and main electronics were built and tested at NASA's Goddard Space Flight Center. This editor's resource page contains video footage and images of MOMA in broadcast resolution. || ", "hits": 58 }, { "id": 30942, "url": "https://svs.gsfc.nasa.gov/30942/", "result_type": "Hyperwall Visual", "release_date": "2018-05-03T00:00:00-04:00", "title": "The first Ice, Cloud, and land Elevation Satellite (ICESat)", "description": "ICESat launch animation and sensor operation || VTS_01_1_trim_00561.jpg (1280x720) [131.3 KB] || VTS_01_1_trim_720p.mp4 (1280x720) [61.6 MB] || VTS_01_1_trim.webm (720x480) [29.8 MB] || ", "hits": 89 }, { "id": 4610, "url": "https://svs.gsfc.nasa.gov/4610/", "result_type": "Visualization", "release_date": "2018-01-19T15:00:00-05:00", "title": "GOLD: Instrument Scanning Coverage", "description": "Visualization of GOLD orbiting Earth with image scanning. This version presents the singly-ionized oxygen density from the IRI model. || IRIGOLDscan.GOLDview3_Oion.clockSlate_CRTT.HD1080i.001400_print.jpg (1024x576) [90.3 KB] || IRIGOLDscan.GOLDview3_Oion.clockSlate_CRTT.HD1080i.001400_searchweb.png (320x180) [79.2 KB] || IRIGOLDscan.GOLDview3_Oion.clockSlate_CRTT.HD1080i.001400_thm.png (80x40) [6.1 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || IRIGOLDscan.GOLDview4_Oion.HD1080i_p30.mp4 (1920x1080) [38.5 MB] || IRIGOLDscan.GOLDview4_Oion.HD1080i_p30.webm (1920x1080) [10.0 MB] || IRIGOLDscan.GOLDview4_Oion.HD1080i_p30.mp4.hwshow [204 bytes] || ", "hits": 126 }, { "id": 12788, "url": "https://svs.gsfc.nasa.gov/12788/", "result_type": "Produced Video", "release_date": "2017-12-11T10:00:00-05:00", "title": "Exploring A Crater", "description": "The Goddard Instrument Field Team, as a part of the RIS4E Project, explores Kilbourne Hole, a maar crater in the Potrillo volcanic field in New Mexico.Music provided by Killer Tracks: \"We Are Invincible\" - Billy Lincoln, Thomas Dean Pugh-Fields. \"Indie Smiles\" - Wally Gagel, Xandy Barry.Archival footage of Jack Schmitt provided by Stephen Slater.Watch this video on the NASA.gov Video YouTube channel. || ExploringCrater-Thumbnail.jpg (1920x1080) [1.1 MB] || ExploringCrater-Thumbnail_searchweb.png (320x180) [103.2 KB] || ExploringCrater-Thumbnail_thm.png (80x40) [7.1 KB] || 12788-ExploringACrater-YouTUBEHD.mp4 (1920x1080) [438.1 MB] || 12788-ExploringACrater-FacebookHD.mp4 (1920x1080) [374.6 MB] || 12788-ExploringACrater-MASTER.mov (1920x1080) [3.8 GB] || 12788-ExploringACrater-YouTUBEHD.webm (1920x1080) [33.0 MB] || 12788ExploringACrater-Captions.en_US.srt [5.5 KB] || 12788ExploringACrater-Captions.en_US.vtt [5.5 KB] || ", "hits": 29 }, { "id": 30918, "url": "https://svs.gsfc.nasa.gov/30918/", "result_type": "Hyperwall Visual", "release_date": "2017-12-04T00:00:00-05:00", "title": "Total Column Ozone from EP-TOMS and MERRA-2 GMI", "description": "Total Column Ozone from EP-TOMS and MERRA-2 GMIThe ozone layer is Earth’s protection from harmful ultraviolet radiation. NASA has a long history of measuring total column ozone using a variety of instruments, typically with polar orbiting satellites measuring backscattered solar radiation. This produces near global coverage over the course of a day over the sunlit portion of Earth. Some missing data occurs between swaths, over the polar region during winter, and during satellite outages. This animation shows the evolution of daily composites of total column ozone as observed with Earth Probe Total Ozone Mapping Spectrometer (EP-TOMS), on the right panel, from July 1, 2002 to Oct. 31, 2002. On the left panel is the total column ozone from the MERRA-2 GMI simulation, with hourly time resolution over the same time period. MERRA-2 GMI is a Goddard Earth Observing System version 5 (GEOS-5) “replay” simulation at 0.5° (~50km) horizontal resolution, driven by MERRA-2 reanalyzed winds, temperature, and pressure, coupled to the comprehensive Global Modeling Initiative (GMI) stratosphere-troposphere chemical mechanism. This animation shows the onset of the Antarctic ozone hole formation during austral winter of the dynamically active 2002 season and its breakdown during spring. In September 2002, the Antarctic polar vortex split into 2 lobes following the first and only observed major stratospheric warming in the Southern Hemisphere over our observational record. By combining NASA’s observations and chemistry simulations we have a clearer view of the evolution of Earth’s ozone layer over the recent past. || oman_toz_2002_pngs_1080.00001_print.jpg (1024x576) [117.1 KB] || oman_toz_2002_pngs_1080.00001_searchweb.png (320x180) [61.2 KB] || oman_toz_2002_pngs_1080.00001_web.png (320x180) [61.2 KB] || oman_toz_2002_pngs_1080.00001_thm.png (80x40) [6.0 KB] || oman_toz_2002_pngs_1080.webm (1920x1080) [10.5 MB] || oman_toz_2002_pngs_1080.mp4 (1920x1080) [187.7 MB] || ", "hits": 70 }, { "id": 12673, "url": "https://svs.gsfc.nasa.gov/12673/", "result_type": "Produced Video", "release_date": "2017-11-15T10:00:00-05:00", "title": "HIRMES: SOFIA's latest high-resolution Mid-infrared Spectrometer", "description": "Learn more about HIRMES, the latest addition to NASA's airplane-based infrared telescope, SOFIA.Credit: NASA's Goddard Space Flight CenterMusic: \"Sparkle Shimmer\" and \"The Orion Arm\", both from Killer Tracks.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || SOFIA_Protoplanetary_Disk_Still_print.jpg (1024x576) [90.0 KB] || SOFIA_Protoplanetary_Disk_Still.jpg (3840x2160) [568.6 KB] || SOFIA_Protoplanetary_Disk_Still_searchweb.png (320x180) [76.3 KB] || SOFIA_Protoplanetary_Disk_Still_web.png (320x180) [76.3 KB] || SOFIA_Protoplanetary_Disk_Still_thm.png (80x40) [7.2 KB] || 12673_SOFIA_HIRMES_ProRes_1920x1080_2997.mov (1920x1080) [3.5 GB] || 12673_SOFIA_HIRMES_H264_Best_1920x1080_2997.mov (1920x1080) [768.4 MB] || 12673_SOFIA_HIRMES_Good_1920x1080_2997.m4v (1920x1080) [302.0 MB] || 12673_SOFIA_HIRMES_Compatible.m4v (960x540) [112.3 MB] || 12673_SOFIA_HIRMES_H264_Best_1920x1080_2997.webm (1920x1080) [33.6 MB] || 12673_SOFIA_HIRMES_SRT_Captions.en_US.srt [5.4 KB] || 12673_SOFIA_HIRMES_SRT_Captions.en_US.vtt [5.1 KB] || ", "hits": 40 }, { "id": 12742, "url": "https://svs.gsfc.nasa.gov/12742/", "result_type": "Produced Video", "release_date": "2017-10-11T00:00:00-04:00", "title": "NASA Satellites See Wildfires from Space", "description": "As wildfires burn across California, NASA satellites help gather data about where the fires are and how smoke travels across the state.The smoke from the fires is even visible a million miles away from Earth, captured by NASA's Earth Polychromatic Imaging Camera (EPIC) onboard NOAA's Deep Space Climate Observatory (DSCOVR). The Terra spacecraft can see fires in both daylight and at night, helping aid firefighters in tracking and stopping the blazes. NASA's unique vantage point in space helps better understand our home planet.Terra Imagery from NASA Worldview || ", "hits": 97 }, { "id": 30903, "url": "https://svs.gsfc.nasa.gov/30903/", "result_type": "Hyperwall Visual", "release_date": "2017-10-03T00:00:00-04:00", "title": "Two Titans", "description": "Two views of Saturn's moon Titan || PIA21624_print.jpg (1024x518) [43.1 KB] || PIA21624_searchweb.png (320x180) [51.4 KB] || PIA21624_thm.png (80x40) [5.2 KB] || PIA21624.tif (2024x1024) [3.9 MB] || two-titans.hwshow [186 bytes] || ", "hits": 81 }, { "id": 12714, "url": "https://svs.gsfc.nasa.gov/12714/", "result_type": "Produced Video", "release_date": "2017-09-14T00:00:00-04:00", "title": "Goddard Team Reflects on 20 Years of Cassini", "description": "The people behind Cassini's Composite Infrared Spectrometer (CIRS) reflect on their years-long experience working with their team - relationships formed, children born, challenges conquered, and their feelings as the Cassini mission comes to an end. CIRS was built and is operated at NASA's Goddard Space Flight Center in Greenbelt, Maryland. Cassini is making its final dive into Saturn on September 15, 2017.Read the web feature on nasa.gov. || ", "hits": 19 }, { "id": 12709, "url": "https://svs.gsfc.nasa.gov/12709/", "result_type": "Produced Video", "release_date": "2017-09-12T10:00:00-04:00", "title": "Cassini's Infrared Saturn", "description": "Since arriving at Saturn in 2004, Cassini has used its Composite Infrared Spectrometer (CIRS) to study the ringed planet and its moons in heat radiation. Complete transcript available.Watch this video on the NASA Goddard YouTube channel.Music provided by Killer Tracks: \"Particle Waves,\" \"Odyssey,\" \"Solaris,\" \"Expansive,\"\"Horizon Ahead,\" \"Ion Bridge,\" \"Outer Space\" || CassiniCIRSpreviewShort.jpg (1920x1080) [591.6 KB] || CassiniCIRSpreviewShort_searchweb.png (320x180) [125.9 KB] || CassiniCIRSpreviewShort_thm.png (80x40) [8.4 KB] || 12709_Cassini_CIRS_Short_TWTR.mp4 (1280x720) [102.0 MB] || WEBM-12709_Cassini_CIRS_Short_APR.webm (960x540) [191.9 MB] || 12709_Cassini_CIRS_Short_FB.mp4 (1280x720) [574.1 MB] || 12709_Cassini_CIRS_Short_YT_Output.en_US.srt [10.3 KB] || 12709_Cassini_CIRS_Short_YT_Output.en_US.vtt [10.3 KB] || 12709_Cassini_CIRS_Short_YT.mp4 (1920x1080) [1.2 GB] || 12709_Cassini_CIRS_Short_APR.mov (1920x1080) [6.0 GB] || 12709_Cassini_CIRS_Short_YT.hwshow [96 bytes] || ", "hits": 54 }, { "id": 4527, "url": "https://svs.gsfc.nasa.gov/4527/", "result_type": "Visualization", "release_date": "2016-12-14T14:00:00-05:00", "title": "ICON and GOLD: Instrument Scanning Coverage", "description": "Visualization of ICON and GOLD orbiting Earth with image scanning. This version presents several geospace models, including the singly-ionized oxygen density, the low-latitude geomagnetic field, and the high-altitude winds (100km and 350km altitudes). || IRIGOLDscan.GOLDview3_OionHwindIGRF.clockSlate_CRTT.UHD3840.001140_print.jpg (1024x576) [130.5 KB] || IRIGOLDscan.GOLDview3_OionHwindIGRF.clockSlate_CRTT.UHD3840.001140_searchweb.png (320x180) [85.0 KB] || IRIGOLDscan.GOLDview3_OionHwindIGRF.clockSlate_CRTT.UHD3840.001140_thm.png (80x40) [5.9 KB] || IRIGOLDscan.GOLDview3_OionHwindIGRF.HD1080i_p30.mp4 (1920x1080) [82.0 MB] || IRIGOLDscan.GOLDview3_OionHwindIGRF (1920x1080) [0 Item(s)] || IRIGOLDscan.GOLDview3_OionHwindIGRF.HD1080i_p30.webm (1920x1080) [7.6 MB] || IRIGOLDscan.GOLDview3_OionHwindIGRF (3840x2160) [0 Item(s)] || IRIGOLDscan.GOLDview3_OionHwindIGRF_2160p30.mp4 (3840x2160) [258.1 MB] || ", "hits": 56 }, { "id": 12443, "url": "https://svs.gsfc.nasa.gov/12443/", "result_type": "Produced Video", "release_date": "2016-12-07T10:00:00-05:00", "title": "OSIRIS-REx Technology: OCAMS", "description": "The OSIRIS-REx camera suite will provide global maps and close-up images of asteroid Bennu, along with information about the carbon-rich asteroid's chemical makeup.This video is available for download in 4k resolution.Watch this video on the NASA Goddard YouTube channel.Complete transcript available.Music Credits: \"Ultimate Question\" and \"Victory Or Failure\" by Guy & Zab Skornik [SACEM] || OCAMS_Preview_12443.jpg (3840x2160) [2.1 MB] || OCAMS_Preview_12443_thm.png (80x40) [8.8 KB] || OCAMS_Preview_12443_searchweb.png (320x180) [126.0 KB] || 12443_OCAMS_Profile_APR.mov (1920x1080) [5.5 GB] || LARGE_MP4_12443_OCAMS_Profile_APR_large.mp4 (1920x1080) [218.7 MB] || 12443_OCAMS_Profile_appletv.m4v (1280x720) [108.3 MB] || 12443_OCAMS_Profile_appletv_subtitles.m4v (1280x720) [108.3 MB] || 12443_OCAMS_Profile.webm (960x540) [87.6 MB] || 12443_OCAMS_Profile_H264_v2.mp4 (3840x2160) [743.3 MB] || 12443_OCAMS_Profile_APR_4k_60fps.mov (3840x2160) [20.2 GB] || 12443_OCAMS_Profile_APR_Output.en_US.srt [3.7 KB] || 12443_OCAMS_Profile_APR_Output.en_US.vtt [3.8 KB] || 12443_OCAMS_Profile_ipod_sm.mp4 (320x240) [37.6 MB] || ", "hits": 48 }, { "id": 40311, "url": "https://svs.gsfc.nasa.gov/gallery/tomsvisualizationsby-year/", "result_type": "Gallery", "release_date": "2016-10-18T09:18:01-04:00", "title": "TOMS Visualizations by Year", "description": "The Total Ozone Mapping Spectrometer, launched in July 1996 onboard an Earth Probe Satellite (TOMS/EP), continues NASA's long-term daily mapping of the global distribution of the Earth's atmospheric ozone. TOMS/EP will again take high-resolution measurements of the total column amount of ozone from space that began with NASA's Nimbus-7 satellite in 1978 and continued with the TOMS aboard a Russian Meteor-3 satellite until the instrument stopped working in December 1994. This NASA-developed instrument, measures ozone indirectly by mapping ultraviolet light emitted by the Sun to that scattered from the Earth's atmosphere back to the satellite. The TOMS instrument has mapped in detail the global ozone distribution as well as the Antarctic \"ozone hole,\" which forms September through November of each year.\n\nThis is a list of visualizations relating to TOMS, ordered by the year the data was taken.\n\nFor more information on TOMS, please visit https://science.nasa.gov/missions/toms.", "hits": 14 }, { "id": 40310, "url": "https://svs.gsfc.nasa.gov/gallery/tomslinks/", "result_type": "Gallery", "release_date": "2016-10-18T09:16:33-04:00", "title": "TOMS Links", "description": "The Total Ozone Mapping Spectrometer, launched in July 1996 onboard an Earth Probe Satellite (TOMS/EP), continues NASA's long-term daily mapping of the global distribution of the Earth's atmospheric ozone. TOMS/EP will again take high-resolution measurements of the total column amount of ozone from space that began with NASA's Nimbus-7 satellite in 1978 and continued with the TOMS aboard a Russian Meteor-3 satellite until the instrument stopped working in December 1994. This NASA-developed instrument, measures ozone indirectly by mapping ultraviolet light emitted by the Sun to that scattered from the Earth's atmosphere back to the satellite. The TOMS instrument has mapped in detail the global ozone distribution as well as the Antarctic \"ozone hole,\" which forms September through November of each year.\n\nThis is a list of visualizations relating to TOMS.\n\nFor more information on TOMS, please visit https://science.nasa.gov/missions/toms.", "hits": 16 }, { "id": 3973, "url": "https://svs.gsfc.nasa.gov/3973/", "result_type": "Visualization", "release_date": "2016-10-13T17:00:00-04:00", "title": "The Story of Ozone Depletion", "description": "The Antarctic ozone hole is caused by human-produced chlorine-containing chlorofluorocarbons (CFCs) and bromine-containing halons. These compounds had a variety of commercial uses, including hair sprays, refrigerants, and fire suppressants.This story about the cause of ozone depletion was originally developed for the NASA hyperwall, where nine different animations can be shown simultaneously. The animations shown here are derived from the Goddard Earth Observing System (GEOS) model and cover two periods. The first period is from August through November 2004, and the second is from December 2004 through March 2005. The first period animations are shown on this page. The second period animations may be downloaded through the Download links below.The chlorine compounds that destroy ozone have now been regulated under the international Montreal Protocol agreement. Because of this agreement, the ozone hole is projected to disappear around 2060-2070. NASA and the international community continue to monitor Antarctic ozone. || ", "hits": 186 }, { "id": 12379, "url": "https://svs.gsfc.nasa.gov/12379/", "result_type": "Produced Video", "release_date": "2016-09-28T10:00:00-04:00", "title": "Space Radiation Highlights", "description": "A collection of space radiation highlights featuring:NASA's Van Allen ProbesNASA's CubeSats || ", "hits": 126 }, { "id": 20258, "url": "https://svs.gsfc.nasa.gov/20258/", "result_type": "Animation", "release_date": "2016-08-17T14:00:00-04:00", "title": "OSIRIS-REx Spacecraft and Instrument Animations", "description": "OSIRIS-REx is a solar-powered spacecraft built by Lockheed Martin Space Systems. The spacecraft bus measures 3.2 meters high by 2.4 meters wide (about 10x8 feet). With its solar arrays deployed, the spacecraft spans 6.2 meters in length (over 20 feet). A high-gain antenna on the sun-pointed side of OSIRIS-REx enables communication with Earth. On the opposite side is the TAGSAM, a 3.4-meter-long, folding arm that will reach out and grab a sample of the mission's target, near-Earth asteroid Bennu. || ", "hits": 75 }, { "id": 12309, "url": "https://svs.gsfc.nasa.gov/12309/", "result_type": "Produced Video", "release_date": "2016-07-25T10:00:00-04:00", "title": "OSIRIS-REx Technology: OVIRS", "description": "OSIRIS-REx will use its visible and infrared spectrometer (OVIRS) to study the chemical composition of Bennu, a near-Earth asteroid that may hold clues to the origins of life.Watch this video on the NASA Goddard YouTube channel.Complete transcript available. || OvirsPreview3.jpg (1920x1080) [859.9 KB] || OvirsPreview3_searchweb.png (320x180) [122.7 KB] || OvirsPreview3_thm.png (80x40) [8.7 KB] || 12309_OVIRS_Profile_APR.mov (1920x1080) [8.7 GB] || 12309_OVIRS_Profile_large.mp4 (1920x1080) [340.1 MB] || 12309_OVIRS_Profile_H264.mp4 (1280x720) [340.6 MB] || 12309_OVIRS_Profile_appletv.m4v (1280x720) [169.3 MB] || 12309_OVIRS_Profile.webm (960x540) [135.6 MB] || 12309_OVIRS_Profile_appletv_subtitles.m4v (1280x720) [169.4 MB] || 12309_OVIRS_Profile_APR_Output.en_US.srt [7.0 KB] || 12309_OVIRS_Profile_APR_Output.en_US.vtt [7.0 KB] || 12309_OVIRS_Profile_ipod_sm.mp4 (320x240) [58.3 MB] || ", "hits": 116 }, { "id": 12282, "url": "https://svs.gsfc.nasa.gov/12282/", "result_type": "Produced Video", "release_date": "2016-07-11T09:00:00-04:00", "title": "OSIRIS-REx Technology: REXIS", "description": "Scientists Richard Binzel, Rebecca Masterson, and Branden Allen discuss how the REXIS instrument aboard OSIRIS-REx works.Watch this video on the NASA Goddard YouTube channel. || REXIStitlecard.jpg (1920x1080) [982.7 KB] || REXIStitlecard_searchweb.png (320x180) [107.5 KB] || REXIStitlecard_thm.png (80x40) [25.1 KB] || 12282_REXIS_Instrument_Profile_MASTER_youtube_hq.mov (1920x1080) [911.9 MB] || 12282_REXIS_Instrument_Profile_MASTER.mpeg (1280x720) [938.8 MB] || 12282_REXIS_Instrument_Profile_MASTER.webm (960x540) [113.7 MB] || 12282_REXIS_Instrument_Profile_MASTER_appletv.m4v (1280x720) [143.4 MB] || 12282_REXIS_Instrument_Profile_MASTER_prores.mov (1280x720) [3.7 GB] || 12282_REXIS_Instrument_Profile_MASTER_appletv_subtitles.m4v (1280x720) [143.5 MB] || 12282_REXIS_Instrument_Profile_MASTER_Output.en_US.srt [5.3 KB] || 12282_REXIS_Instrument_Profile_MASTER_Output.en_US.vtt [5.3 KB] || 12282_REXIS_Instrument_Profile_MASTER_ipod_sm.mp4 (320x240) [48.8 MB] || ", "hits": 41 }, { "id": 12160, "url": "https://svs.gsfc.nasa.gov/12160/", "result_type": "Produced Video", "release_date": "2016-07-06T13:00:00-04:00", "title": "Hitomi Microcalorimeter Array Animation (4k)", "description": "This animation illustrates how the microcalorimeter array at the heart of Hitomi's revolutionary Soft X-ray Spectrometer works. X-ray light collected by a telescope strikes the detector. Each photon heats the material by an amount directly proportional to its energy. The instrument, which is cooled to near absolute zero, detects this minute temperature change. Credit: NASA's Goddard Space Flight Center || Astro-H_Calorimeter-STILL_print.jpg (1024x576) [64.0 KB] || Astro-H_Calorimeter-STILL.jpg (3840x2160) [716.3 KB] || Astro-H_Calorimeter-STILL_searchweb.png (320x180) [55.3 KB] || Astro-H_Calorimeter-STILL_web.png (320x180) [55.3 KB] || Astro-H_Calorimeter-STILL_thm.png (80x40) [5.5 KB] || Astro-H_Calorimeter-STILL.tiff (3840x2160) [63.3 MB] || Astro-H_Calorimeter_Simple-H264_Good_3840x2160_2997.mov (3840x2160) [27.1 MB] || Astro-H_Calorimeter_Simple_ProRes_3840x2160_60.webm (3840x2160) [4.9 MB] || Astro-H_Calorimeter_Simple-H264_Best_3840x2160_5994.mov (3840x2160) [448.6 MB] || Astro-H_Calorimeter_Simple_ProRes_3840x2160_60.mov (3840x2160) [1.8 GB] || ", "hits": 23 }, { "id": 12297, "url": "https://svs.gsfc.nasa.gov/12297/", "result_type": "Produced Video", "release_date": "2016-07-06T13:00:00-04:00", "title": "Hitomi Measures X-ray Winds of the Perseus Galaxy Cluster", "description": "A revolutionary instrument aboard the ill-fated Hitomi satellite returned the most detailed measurements yet made of the million-degree atmosphere at the core of a galaxy cluster. Watch the video to learn more.Credit: NASA's Goddard Space Flight CenterMusic: \"Natural Awe\" and \"To the Tower\" from Killer TracksComplete transcript available. || Astro-H_Calorimeter-STILL_print.jpg (1024x576) [64.7 KB] || Astro-H_Calorimeter-STILL_searchweb.png (320x180) [55.3 KB] || Astro-H_Calorimeter-STILL_web.png (320x180) [55.3 KB] || Astro-H_Calorimeter-STILL_thm.png (80x40) [5.4 KB] || Astro-H_Calorimeter-STILL.tiff (3840x2160) [63.3 MB] || 12297_Hitomi_SXS_FINAL_ipod_sm.mp4 (320x240) [43.0 MB] || 12297_Hitomi_SXS_FINAL_lowres.mp4 (480x272) [33.7 MB] || PRORES_B-ROLL_12297_Hitomi_SXS_FINAL_prores.webm [0 bytes] || PRORES_B-ROLL_12297_Hitomi_SXS_FINAL_prores.mov (1280x720) [1.7 GB] || NASA_TV_12297_Hitomi_SXS_FINAL.mpeg (1280x720) [796.7 MB] || APPLE_TV_12297_Hitomi_SXS_FINAL_appletv-2.m4v (1280x720) [127.0 MB] || 12297_Hitomi_SXS_FINAL_youtube_hq.mov (1920x1080) [1.1 GB] || 12297_Hitomi_SXS_FINAL_ProRes_1920x1080_2997.mov (1920x1080) [3.1 GB] || ", "hits": 96 }, { "id": 30787, "url": "https://svs.gsfc.nasa.gov/30787/", "result_type": "Hyperwall Visual", "release_date": "2016-06-22T00:00:00-04:00", "title": "NASA Spots Single Methane Leak from Space", "description": "Comparison of detected methane plumes over Aliso Canyon, California, acquired 11 days apart in Jan. 2016 by: (left) NASA's AVIRIS instrument on a NASA ER-2 aircraft at 4.1 miles (6.6 kilometers) altitude and (right) by the Hyperion instrument on NASA's Earth Observing-1 satellite in low-Earth orbit at approximately 700km. || hyperion_methane_aliso_canyon_PIA20716.png (1920x1080) [2.0 MB] || hyperion_methane_aliso_canyon_PIA20716_print.jpg (1024x576) [189.5 KB] || hyperion_methane_aliso_canyon_PIA20716_searchweb.png (320x180) [126.3 KB] || hyperion_methane_aliso_canyon_PIA20716_thm.png (80x40) [8.5 KB] || hyperion_methane_aliso_canyon_PIA20716.hwshow [244 bytes] || ", "hits": 17 }, { "id": 12262, "url": "https://svs.gsfc.nasa.gov/12262/", "result_type": "Produced Video", "release_date": "2016-05-19T19:00:00-04:00", "title": "NASA Launches Super-Pressure Balloon", "description": "NASA successfully launched a super pressure balloon (SPB) from Wanaka Airport, New Zealand, at 11:35 a.m. Tuesday, May 17, (7:35 p.m. EDT Monday, May 16) on a potentially record-breaking, around-the-world test flight.The balloon flies at an altitude of about 110,000 feet, in a layer of Earth's atmosphere known as the stratosphere.The purpose of the flight is to test and validate the SPB technology with the goal of long-duration flight (100+ days) at mid-latitudes. In addition, the gondola is carrying the Compton Spectrometer and Imager (COSI) gamma-ray telescope as a mission of opportunity.Another mission of opportunity is the Carolina Infrasound instrument, a small, 3-kilogram payload with infrasound microphones designed to record acoustic wave field activity in the stratosphere. Developed by the University of North Carolina at Chapel Hill, previous balloon flights of the instrument have recorded low-frequency sounds in the stratosphere, some of which are believed to be new to science.As the balloon travels around the Earth, it may be visible from the ground, particularly at sunrise and sunset, to those who live in the southern hemisphere’s mid-latitudes, such as Argentina and South Africa.NASA’s scientific balloons offer low-cost, near-space access for conducting scientific investigations in fields such as astrophysics, heliophysics and atmospheric research.NASA’s Wallops Flight Facility in Virginia manages the agency’s scientific balloon flight program with 10 to 15 flights each year from launch sites worldwide. Orbital ATK, which operates NASA’s Columbia Scientific Balloon Facility in Palestine, Texas, provides mission planning, engineering services and field operations for NASA’s scientific balloon program. The CSBF team has launched more than 1,700 scientific balloons in the over 35 years of operation.Track the flight's progress in real-time here. || ", "hits": 106 }, { "id": 12194, "url": "https://svs.gsfc.nasa.gov/12194/", "result_type": "Produced Video", "release_date": "2016-04-07T12:55:00-04:00", "title": "The Compton Legacy: A Quarter-century of Gamma-ray Science", "description": "This illustration of the Compton Gamma Ray Observatory shows the locations of its four instruments, the Burst And Transient Source Experiment (BATSE), the Oriented Scintillation Spectrometer Experiment (OSSE), the Imaging Compton Telescope (COMPTEL), and the Energetic Gamma Ray Experiment Telescope (EGRET). Credit: NASA's Goddard Space Flight Center || GRO_cutaway_labels_1080.jpg (1920x1081) [668.9 KB] || GRO_cutaway_labels_2160.jpg (3840x2161) [5.2 MB] || GRO_cutaway_labels_2160_searchweb.png (320x180) [116.1 KB] || GRO_cutaway_labels_2160_thm.png (80x40) [12.2 KB] || ", "hits": 93 }, { "id": 30765, "url": "https://svs.gsfc.nasa.gov/30765/", "result_type": "Hyperwall Visual", "release_date": "2016-04-05T03:00:00-04:00", "title": "Rosetta Images of Comet 67P", "description": "Comet 67p seen from Rosetta || MainImage.jpg (878x863) [432.2 KB] || MainImage_searchweb.png (320x180) [33.5 KB] || MainImage_thm.png (80x40) [2.4 KB] || rosetta-images-of-comet-67p-full-comet.hwshow [280 bytes] || ", "hits": 135 }, { "id": 12167, "url": "https://svs.gsfc.nasa.gov/12167/", "result_type": "Produced Video", "release_date": "2016-03-14T06:00:00-04:00", "title": "Student Scientists: Building REXIS", "description": "College students in Boston are getting the chance to help NASA explore an asteroid. These student scientists have built an instrument called REXIS, which will fly on the OSIRIS-REx spacecraft that launches in September 2016. This video puts a spotlight on a group of these students and their experience on the REXIS project.Watch this video on the NASAgovVideo YouTube channel. || 12167_Student_Scientists_Building_REXIS_MASTER_youtube_hq_print.jpg (1024x576) [141.0 KB] || 12167_Student_Scientists_Building_REXIS_MASTER_youtube_hq_searchweb.png (320x180) [101.5 KB] || 12167_Student_Scientists_Building_REXIS_MASTER_youtube_hq_thm.png (80x40) [7.3 KB] || 12167_Student_Scientists_Building_REXIS_MASTER_youtube_hq.mov (1920x1080) [1.2 GB] || 12167_Student_Scientists_Building_REXIS_MASTER_prores.mov (1280x720) [4.3 GB] || 12167_Student_Scientists_Building_REXIS_MASTER.webm (960x540) [132.0 MB] || 12167_Student_Scientists_Building_REXIS_MASTER_appletv.m4v (1280x720) [162.8 MB] || 12167_Student_Scientists_Building_REXIS_MASTER_youtube_hq.webm (1920x1080) [35.1 MB] || 12167_Student_Scientists_Building_REXIS_MASTER_appletv_subtitles.m4v (1280x720) [163.0 MB] || 12167_Student_Scientists_Building_REXIS_MASTER.en_US.srt [6.7 KB] || 12167_Student_Scientists_Building_REXIS_MASTER.en_US.vtt [6.7 KB] || 12167_Student_Scientists_Building_REXIS_MASTER_ipod_sm.mp4 (320x240) [58.1 MB] || ", "hits": 21 }, { "id": 12120, "url": "https://svs.gsfc.nasa.gov/12120/", "result_type": "Produced Video", "release_date": "2016-02-22T14:00:00-05:00", "title": "NASA Goddard Spectrometer Launches on Hitomi Observatory", "description": "An artist's rendering of Hitomi in orbit.Credit: JAXA || Astro_h_art.jpg (3179x4500) [2.5 MB] || Astro_h_art_searchweb.png (180x320) [102.0 KB] || Astro_h_art_thm.png (80x40) [6.9 KB] || ", "hits": 39 }, { "id": 4407, "url": "https://svs.gsfc.nasa.gov/4407/", "result_type": "Visualization", "release_date": "2015-12-15T11:00:00-05:00", "title": "Monthly burned area from the Global Fire Emissions Database (GFED)", "description": "The final animation of the monthly burned area percent shown in the Robinson projection with a colorbar and date overlay || comp_burned_area_pct.2234_print.jpg (1024x576) [128.4 KB] || comp_burned_area_pct.2234_searchweb.png (320x180) [78.4 KB] || comp_burned_area_pct.2234_thm.png (80x40) [6.4 KB] || comp_burned_area_pct.2234_web.png (320x180) [78.4 KB] || comp_burned_area_pct_1080p30.mp4 (1920x1080) [44.1 MB] || comp_burned_area_pct_1080p30.webm (1920x1080) [8.4 MB] || robinson_final (1920x1080) [0 Item(s)] || Comp_burned_area_pct_720p30.mp4 (1280x720) [26.2 MB] || robinson_final (3840x2160) [0 Item(s)] || comp_burned_area_4407.key [29.7 MB] || comp_burned_area_4407.pptx [27.1 MB] || comp_burned_area_pct_4k_2160p30.mp4 (3840x2160) [142.3 MB] || comp_burned_area_pct_1080p30.mp4.hwshow [228 bytes] || ", "hits": 112 }, { "id": 12095, "url": "https://svs.gsfc.nasa.gov/12095/", "result_type": "Produced Video", "release_date": "2015-12-15T10:30:00-05:00", "title": "AGU El Nino Press Conference Release Materials", "description": "Forty percent of California's annual water supply comes in the form of atmospheric rivers, tendrils of moisture that travel from the Pacific Ocean and rain out when they move over the coast. New research on how El Niño affects atmospheric rivers headed for the California coast suggest that while the number of atmospheric rivers California receives (typically ten per year) will not change during an El Niño, they will be stronger, warmer, and thus wetter. || ", "hits": 14 }, { "id": 4410, "url": "https://svs.gsfc.nasa.gov/4410/", "result_type": "Visualization", "release_date": "2015-12-14T17:00:00-05:00", "title": "2005-2014 NO₂ Hyperwall Shows", "description": "Global NO2 Concentrations, Endpoint Fade 2005, 2014 || hyperwall_global_fade.0001_print.jpg (1024x576) [108.3 KB] || hyperwall_global_fade.0001_print_searchweb.png (320x180) [65.5 KB] || hyperwall_global_fade.0001_print_thm.png (80x40) [6.1 KB] || global_no2_conc_fade_1080p30.mp4 (1920x1080) [5.9 MB] || global_no2_conc_fade_1080p30.webm (1920x1080) [1.1 MB] || hyperwall_global_fade_prores.mp4 (1280x720) [638.8 KB] || hyperwall_global_fade (5760x3240) [0 Item(s)] || hyperwall_global_fade_4410.key [4.1 MB] || hyperwall_global_fade_4410.pptx [1.6 MB] || ", "hits": 22 }, { "id": 11962, "url": "https://svs.gsfc.nasa.gov/11962/", "result_type": "Produced Video", "release_date": "2015-07-20T15:00:00-04:00", "title": "The NIRSpec Instrument is Prepped for Micro-Shutter Array and Focal Plane Assembly Replacement", "description": "B-roll video of Airbus engineers removing the cover from the Near InfraRed Spectrometer (NIRSpec) instrument || Screen_Shot_2015-07-20_at_3.24.48_PM.png (1878x1051) [2.3 MB] || Screen_Shot_2015-07-20_at_3.24.48_PM_print.jpg (1024x573) [122.2 KB] || Screen_Shot_2015-07-20_at_3.24.48_PM_searchweb.png (320x180) [104.5 KB] || Screen_Shot_2015-07-20_at_3.24.48_PM_thm.png (80x40) [12.9 KB] || NIRSpec_Cover_Removal_b-roll_h264.webm (1280x720) [46.0 MB] || NIRSpec_Cover_Removal_b-roll_ProRes-master.mov (1280x720) [5.9 GB] || NIRSpec_Cover_Removal_b-roll_h264.mov (1280x720) [348.0 MB] || ", "hits": 15 }, { "id": 11950, "url": "https://svs.gsfc.nasa.gov/11950/", "result_type": "Produced Video", "release_date": "2015-07-13T11:00:00-04:00", "title": "New Horizons Interview with Dennis Reuter", "description": "Instrument scientist Dennis Reuter answers questions about Pluto, NASA’s New Horizons spacecraft, and the Ralph infrared and visible spectrometer.Watch this video on the NASAexplorer YouTube channel.For complete transcript, click here. || New_Horizons_4Q_poster_v3_print.jpg (1024x576) [113.6 KB] || New_Horizons_4Q_poster_v3.png (1920x1080) [7.9 MB] || New_Horizons_4Q_poster_v3_searchweb.png (320x180) [68.1 KB] || New_Horizons_4Q_poster_v3_thm.png (80x40) [8.5 KB] || G2015-061_New_Horizons_4Q_MASTER.mov (1920x1080) [3.1 GB] || G2015-061_New_Horizons_4Q_MASTER_H264.mov (1920x1080) [769.5 MB] || WMV_G2015-061_New_Horizons_4Q_MASTER_1280x720.wmv (1280x720) [54.3 MB] || YOUTUBE_HQ_G2015-061_New_Horizons_4Q_MASTER_youtube_hq.mov (1280x720) [232.3 MB] || NASA_TV_G2015-061_New_Horizons_4Q_MASTER.mpeg (1280x720) [426.6 MB] || APPLE_TV_G2015-061_New_Horizons_4Q_MASTER_appletv.m4v (1280x720) [58.8 MB] || G2015-061_New_Horizons_4Q_MASTER.webm (1920x1080) [12.9 MB] || APPLE_TV_G2015-061_New_Horizons_4Q_MASTER_appletv_subtitles.m4v (1280x720) [58.8 MB] || G2015-061_New_Horizons_4Q_MASTER_H264.en_US.srt [2.0 KB] || G2015-061_New_Horizons_4Q_MASTER_H264.en_US.vtt [2.0 KB] || NASA_PODCAST_G2015-061_New_Horizons_4Q_MASTER_ipod_sm.mp4 (320x240) [21.1 MB] || ", "hits": 55 }, { "id": 11869, "url": "https://svs.gsfc.nasa.gov/11869/", "result_type": "Produced Video", "release_date": "2015-05-08T10:00:00-04:00", "title": "NASA On Air: Big Ozone Holes Headed For Extinction By 2040 (5/8/2015)", "description": "LEAD: NASA scientists report that the ozone hole over Antarctica is slowly recovering.1. The ozone hole is the result of man-made chlorine and bromine chemicals reacting with thin ice clouds at 60,000 feet where temperatures are bitterly cold, less than –110 Degrees Fahrenheit.2. The ozone hole varies from twice to three times the size of the United States.3. Since the Montreal Protocol agreement in 1987, emissions have been regulated and ozone-depleting chemical levels have been slowly declining.4. With a new analysis, NASA scientists say that the ozone hole will be consistently smaller than less than twice the United States.TAG: Scientists will continue to use satellites to monitor the recovery of the ozone hole and they hope to see its full recovery before the end of the century. || WC_Ozone2040-1920-MASTER_iPad_1920x0180_print.jpg (1024x576) [115.0 KB] || WC_Ozone2040-1920-MASTER_iPad_1920x0180_searchweb.png (320x180) [78.1 KB] || WC_Ozone2040-1920-MASTER_iPad_1920x0180_web.png (320x180) [78.1 KB] || WC_Ozone2040-1920-MASTER_iPad_1920x0180_thm.png (80x40) [5.4 KB] || WC_Ozone2040-1920-MASTER_1920x1080.mov (1920x1080) [648.2 MB] || WC_Ozone2040-1920-MASTER_1280x720.mov (1280x720) [766.3 MB] || WC_Ozone2040-1920-MASTER_NBC_Today.mov (1920x1080) [241.4 MB] || WC_Ozone2040-1920-MASTER_WEA_CEN.wmv (1280x720) [17.3 MB] || WC_Ozone2040-1920-MASTER_converted.avi (1280x720) [19.0 MB] || WC_Ozone2040-1920-MASTER_baron.mp4 (1920x1080) [20.6 MB] || WC_Ozone2040-1920-MASTER_prores.mov (1920x1080) [518.5 MB] || WC_Ozone2040-1920-MASTER_iPad_960x540.m4v (960x540) [71.1 MB] || WC_Ozone2040-1920-MASTER_iPad_1280x720.m4v (1280x720) [116.2 MB] || WC_Ozone2040-1920-MASTER_iPad_1920x0180.m4v (1920x1080) [241.4 MB] || WC_Ozone2040-1920-MASTER_iPad_960x540.webm (960x540) [3.4 MB] || ", "hits": 44 }, { "id": 11781, "url": "https://svs.gsfc.nasa.gov/11781/", "result_type": "Produced Video", "release_date": "2015-05-06T12:00:00-04:00", "title": "Big Ozone Holes Headed For Extinction By 2040", "description": "The next three decades will see an end of the era of big ozone holes. In a new study, scientists from NASA Goddard Space Flight Center say that the ozone hole will be consistently smaller than 8 million square miles by the year 2040.Ozone-depleting chemicals in the atmosphere cause an ozone hole to form over Antarctica during the winter months in the Southern Hemisphere. Since the Montreal Protocol agreement in 1987, emissions have been regulated and chemical levels have been declining. However, the ozone hole has still remained bigger than 8 million square miles since the early 1990s, with exact sizes varying from year to year.The size of the ozone hole varies due to both temperature and levels of ozone-depleting chemicals in the atmosphere. In order to get a more accurate picture of the future size of the ozone hole, scientists used NASA’s AURA satellite to determine how much the levels of these chemicals in the atmosphere varied each year. With this new knowledge, scientists can confidently say that the ozone hole will be consistently smaller than 8 million square miles by the year 2040. Scientists will continue to use satellites to monitor the recovery of the ozone hole and they hope to see its full recovery before the end of the century.Research: Inorganic chlorine variability in the Antarctic vortex and implications for ozone recovery.Journal: Geophysical Research: Atmospheres, December 18, 2014.Link to paper: http://onlinelibrary.wiley.com/doi/10.1002/2014JD022295/abstract.Here is the YouTube video. || ", "hits": 131 }, { "id": 11867, "url": "https://svs.gsfc.nasa.gov/11867/", "result_type": "Produced Video", "release_date": "2015-05-06T12:00:00-04:00", "title": "Instagram: Big Ozone Holes Headed For Extinction By 2040", "description": "The next three decades will see an end of the era of big ozone holes. In a new study, scientists from NASA Goddard Space Flight Center say that the ozone hole will be consistently smaller than 8 million square miles by the year 2040.Ozone-depleting chemicals in the atmosphere cause an ozone hole to form over Antarctica during the winter months in the Southern Hemisphere. Since the Montreal Protocol agreement in 1987, emissions have been regulated and chemical levels have been declining. However, the ozone hole has still remained bigger than 8 million square miles since the early 1990s, with exact sizes varying from year to year.The size of the ozone hole varies due to both temperature and levels of ozone-depleting chemicals in the atmosphere. In order to get a more accurate picture of the future size of the ozone hole, scientists used NASA’s AURA satellite to determine how much the levels of these chemicals in the atmosphere varied each year. With this new knowledge, scientists can confidently say that the ozone hole will be consistently smaller than 8 million square miles by the year 2040. Scientists will continue to use satellites to monitor the recovery of the ozone hole and they hope to see its full recovery before the end of the century.Research: Inorganic chlorine variability in the Antarctic vortex and implications for ozone recovery.Journal: Geophysical Research: Atmospheres, December 18, 2014.Link to paper: http://onlinelibrary.wiley.com/doi/10.1002/2014JD022295/abstract. || ", "hits": 28 }, { "id": 11821, "url": "https://svs.gsfc.nasa.gov/11821/", "result_type": "Produced Video", "release_date": "2015-03-25T14:00:00-04:00", "title": "Suzaku, Herschel Link a Black-hole 'Wind' to a Galactic Gush", "description": "This movie illustrates how black-hole feedback works in quasars. Dense gas and dust in the center simultaneously fuels the black hole and shrouds it from view. The black-hole wind propels large-scale outflows of cold gas and powers a shock wave that clears gas and dust from the central galaxy.Video credit: NASA's Goddard Space Flight Center || Suzaku_Quasar_Wind_STILL.png (1920x1080) [8.1 MB] || Suzaku_Quasar_Wind_STILL_print.jpg (1024x576) [41.8 KB] || Suzaku_Quasar_Wind_STILL_searchweb.png (320x180) [55.0 KB] || Suzaku_Quasar_Wind_STILL_web.png (320x180) [55.0 KB] || Suzaku_Quasar_Wind_STILL_thm.png (80x40) [7.9 KB] || 11821_Suzaku_Quasar_Wind_FINAL_appletv.webm (960x540) [3.3 MB] || 11821_Suzaku_Quasar_Wind_FINAL.mov (1920x1080) [333.5 MB] || 1920x1080_16x9_30p (1920x1080) [32.0 KB] || 11821_Suzaku_Quasar_Wind_FINAL-H264_Best_1920x1080_2997.mov (1920x1080) [295.2 MB] || 11821_Suzaku_Quasar_Wind_FINAL-H264_Good_1920x1080_2997.mov (1920x1080) [36.8 MB] || 11821_Suzaku_Quasar_Wind_FINAL-MPEG4_1920X1080_2997.mp4 (1920x1080) [13.0 MB] || 11821_Suzaku_Quasar_Wind_FINAL_1280x720.wmv (1280x720) [13.8 MB] || 11821_Suzaku_Quasar_Wind_FINAL_appletv.m4v (960x540) [13.6 MB] || 11821_Suzaku_Quasar_Wind_FINAL_ipod_lg.m4v (640x360) [5.2 MB] || 11821_Suzaku_Quasar_Wind_FINAL_ipod_sm.mp4 (320x240) [2.6 MB] || ", "hits": 50 }, { "id": 11741, "url": "https://svs.gsfc.nasa.gov/11741/", "result_type": "Produced Video", "release_date": "2015-01-28T00:00:00-05:00", "title": "Soil Moisture Active Passive (SMAP) Live Shot Page 1.29.15", "description": "NASA scientists talk about the launch of the Soil Moisture Active Passive - or SMAP - satellite scheduled to launch on Jan 29. SMAP will take stock of the water hidden just beneath your feet, in the topsoil. Knowing how much water is in the soil, and whether it is frozen or thawed, has profound applications for society, from better forecasting of natural disasters like floods and droughts to helping prevent food shortages.How SMAP's radiometer works.How SMAP will help weather forecasts.More about SMAP.NASA TV's video file. || ", "hits": 41 }, { "id": 30571, "url": "https://svs.gsfc.nasa.gov/30571/", "result_type": "Hyperwall Visual", "release_date": "2015-01-15T00:00:00-05:00", "title": "Science with SOFIA", "description": "First image in presentation || sofia_montage_print.jpg (1024x575) [201.0 KB] || sofia_montage.png (4098x2304) [7.8 MB] || sofia_montage_searchweb.png (320x180) [106.7 KB] || sofia_montage_web.png (320x179) [106.7 KB] || sofia_montage_thm.png (80x40) [8.4 KB] || randolf_klein_sofia.hwshow [60 bytes] || Dr. Randolf Klein's AAS presentation from January 2015 || ", "hits": 30 }, { "id": 11571, "url": "https://svs.gsfc.nasa.gov/11571/", "result_type": "Produced Video", "release_date": "2014-06-23T10:00:00-04:00", "title": "JWST Microshutters Moved for Thermal, Accoustic and Vibration Testing", "description": "A new Microshutter Array for the Webb Telescope's Near Infrared Spectrometer (NIRSpec) is packed and transported by hand one building away at NASA Goddard Space Flight Center to undergo thermal cycling testing and checkouts at it operational temperature of 35 kelvin or -397 Fahrenheit. || ", "hits": 23 }, { "id": 11522, "url": "https://svs.gsfc.nasa.gov/11522/", "result_type": "Produced Video", "release_date": "2014-05-07T12:00:00-04:00", "title": "The Best Observed X-class Flare", "description": "On March 29, 2014 the sun released an X-class flare. It was observed by NASA's Interface Region Imaging Spectrograph, or IRIS; NASA's Solar Dynamics Observatory, or SDO; NASA's Reuven Ramaty High Energy Solar Spectroscopic Imager, or RHESSI; the Japanese Aerospace Exploration Agency's Hinode; and the National Solar Observatory's Dunn Solar Telescope located at Sacramento Peak in New Mexico. To have a record of such an intense flare from so many observatories is unprecedented. Such research can help scientists better understand what catalyst sets off these large explosions on the sun. Perhaps we may even some day be able to predict their onset and forewarn of the radio blackouts solar flares can cause near Earth – blackouts that can interfere with airplane, ship and military communications. || ", "hits": 84 }, { "id": 4164, "url": "https://svs.gsfc.nasa.gov/4164/", "result_type": "Visualization", "release_date": "2014-05-07T10:00:00-04:00", "title": "A Multi-Mission View of a Solar Flare: Optical to Gamma-rays", "description": "To improve our understanding of complex phenomena such as solar flares, a wide variety of tools are needed. In the case of astronomy, those tools enable us to analyze the light in many different wavelengths and many different ways.Many different instruments are observing the Sun almost continuously, both from space and on the surface of the Earth. On March 29, 2014, the Dunn Solar Telescope at Sacramento Peak, New Mexico was observing a solar active region and requested other observatories to watch as well. As a result of this coordination, the region was being observed by a large number of different instruments, ground and space-based, when it subsequently erupted with an X-class flare. This visualization presents various combinations of the datasets collected during this effort. The color text represents the dominant color of the dataset in the imagery.Solar Dynamics Observatory (SDO): HMI (617.1nm). This data represents the Sun is visible light similar to how we see it from the ground.Solar Dynamics Observatory (SDO): AIA (17.1nm). Solar ultraviolet emission, which can only be seen from space, reveals plasma flowing, and escaping, along magnetic fields.IRIS Slit-Jaw Imager: 140.0nm. This high-resolution imager also contains a slit (the dark vertical line in the center of the field) which directs the light to an ultraviolet spectrometer which is used to extract even more information about the light. The imager slews back-and-forth across the region, providing spectra over a larger area of the Sun.Hinode/X-ray Telescope: x-ray band. Indicates very hot plasma.RHESSI: 50-100 keV. High-energy gamma-ray emission. Emission from these locations represent the very highest energy photons from the flare event.Dunn Solar Telescope: G-band filter. This filter, showing much of the solar surface (photosphere) in visible light, provides a detailed view of the sunspots and convection cells. The view moves because the instrument was repointed several times during the observation.Dunn Solar Telescope: IBIS ( Hydrogen alpha, 656.3nm; Calcium 854.2 nm; Iron 630.15nm). This is the small rectangular view within the Dunn Solar Telescope G-band view. This instrument can tune the wavelength during the observation, which provides views of the solar atmosphere at different depths. || ", "hits": 50 }, { "id": 11520, "url": "https://svs.gsfc.nasa.gov/11520/", "result_type": "B-Roll", "release_date": "2014-04-08T12:00:00-04:00", "title": "NIRSpec Instrument Gets Integrated into Webb's ISIM - B-ROLL", "description": "Engineers install the Near Infrared Spectrometer (NIRSpec) onto the Webb Telescope's Integrated Science Instrument Module (ISIM) in NASA Goddard Space Flight Center cleanroom. This delicate procedure took place during March 24 and March 25, 2014 in preparation for the cryogenic test of a fully integrated ISIM structure to occur this summer. The Near-Infrared Spectrograph (NIRSpec) is a near infrared multi-object dispersive spectrograph capable of simultaneously observing more than 100 sources over a field-of-view (FOV) larger than 3' x 3'. The NIRSpec will be the first spectrograph in space that has this capability. Targets in the Field of View are normally selected by opening groups of shutters in a micro-shutter array (MSA) to form multiple apertures. The microshutters are arranged in a waffle-like grid that contains more than 62000 shutters with each cell measuring 100 µm x 200 µm. Sweeping a magnet across the surface of the MSA opens all operable shutters. Individual shutters may then be addressed and closed electronically. NIRSpec is also capable of Fixed-slit and Integral-field spectroscopy and provides medium-resolution spectroscopy over a wavelength range of 1 - 5 µm and lower-resolution spectroscopy from 0.6 - 5 µm.NIRSpec will address all of the four main JWST science themes, and much more. It will enable large spectroscopic surveys of faint galaxies at high redshift, obtain sensitive spectra of transiting exoplanets and image line emission from protoplanetary disks and protostars. NIRSpec is being built for the European Space Agency (ESA) by the Airbus Group with Dr. Pierre Ferruit guiding its development as the ESA JWST Project Scientist. Peter Jakobsen, the NIRSpec Instrument PI, retired in December 2011. || ", "hits": 19 }, { "id": 11510, "url": "https://svs.gsfc.nasa.gov/11510/", "result_type": "Produced Video", "release_date": "2014-04-08T11:00:00-04:00", "title": "NIRSpec Instrument Gets Integrated into Webb's ISIM", "description": "Engineers install the Near Infrared Spectrometer (NIRSpec) onto the Webb Telescope's Integrated Science Instrument Module (ISIM) in NASA Goddard Space Flight Center cleanroom. This delicate procedure took place during March 24 and March 25, 2014 in preparation for the cryogenic test of a fully integrated ISIM structure to occur this summer. The Near-Infrared Spectrograph (NIRSpec) is a near infrared multi-object dispersive spectrograph capable of simultaneously observing more than 100 sources over a field-of-view (FOV) larger than 3' x 3'. The NIRSpec will be the first spectrograph in space that has this capability. Targets in the Field of View are normally selected by opening groups of shutters in a micro-shutter array (MSA) to form multiple apertures. The microshutters are arranged in a waffle-like grid that contains more than 62000 shutters with each cell measuring 100 µm x 200 µm. Sweeping a magnet across the surface of the MSA opens all operable shutters. Individual shutters may then be addressed and closed electronically. NIRSpec is also capable of Fixed-slit and Integral-field spectroscopy and provides medium-resolution spectroscopy over a wavelength range of 1 - 5 µm and lower-resolution spectroscopy from 0.6 - 5 µm.NIRSpec will address all of the four main JWST science themes, and much more. It will enable large spectroscopic surveys of faint galaxies at high redshift, obtain sensitive spectra of transiting exoplanets and image line emission from protoplanetary disks and protostars. NIRSpec is being built for the European Space Agency (ESA) by the Airbus Group with Dr. Pierre Ferruit guiding its development as the ESA JWST Project Scientist. Peter Jakobsen, the NIRSpec Instrument PI, retired in December 2011. || ", "hits": 15 }, { "id": 11434, "url": "https://svs.gsfc.nasa.gov/11434/", "result_type": "Produced Video", "release_date": "2013-12-10T13:00:00-05:00", "title": "Comet ISON before and during Perihelion", "description": "After a year of observations, scientists waited with bated breath on Nov. 28, 2013, as Comet ISON made its closest approach to the sun, known as perihelion. Would the comet disintegrate in the fierce heat and gravity of the sun? Or survive intact to appear as a bright comet in the pre-dawn sky? Some remnant of ISON did indeed make it around the sun, but it quickly dimmed and fizzled as seen with NASA's solar observatories. This does not mean scientists were disappointed, however. On Dec. 10, 2013, researchers presented science results from the comet's last days at the 2013 Fall American Geophysical Union meeting in San Francisco, Calif. They described how this unique comet lost mass in advance of reaching perihelion and most likely broke up during its closest approach, as well, as summarized what this means for determining what the comet was made of. The panel shared results from the Solar and Heliospheric Observatory (SOHO), the Solar Terrestrial Relations Observatory (STEREO), the Mars Reconnaissance Orbiter (MRO) and MESSENGER to present a picture of ISON's trip around the sun, which appears to have led to its demise. The panel also reported on why ISON was not seen in images from the Solar Dynamics Observatory (SDO). || ", "hits": 67 } ] }