{ "count": 61, "next": null, "previous": null, "results": [ { "id": 14756, "url": "https://svs.gsfc.nasa.gov/14756/", "result_type": "Produced Video", "release_date": "2025-01-13T16:00:00-05:00", "title": "50 Years of GOES", "description": "Music:“Realms of the Sky” by Frederik Helmut Wiedmann [GMR]; Icon Trailer Music; Universal Production Music“Exoplanet” by Jeff Penny [ASCAP]; Emperia Musicworks; Universal Production Music“Solo Trip” by Nicholas Smith [PRS]; Ideal.e; Universal Production Music“Reaching the Skies” by Ben Hicks [ASCAP]; Emperia Musicworks; Universal Production Music“Aetherion” by Lincoln Dale Davis [BMI]; Emperia Musicworks; Universal Production MusicThis video can be freely shared and downloaded. While the video in its entirety can be shared without permission, some individual imagery provided by FootageFirm.com, Sebolla74/Pond5 and danr13/Pond5 are obtained through permission and may not be excised or remixed in other products. For more information on NASA’s media guidelines, visit https://www.nasa.gov/multimedia/guidelines/index.html || YouTubeThumbnail_GOES50th_GOESandEarth.jpg (1920x1080) [1.2 MB] || YouTubeThumbnail_GOES50th_GOESandEarth.png (1280x720) [1.5 MB] || 14756_GOES_50th_FINAL_UHD.00500_print.jpg (1024x576) [167.0 KB] || 14756_GOES_50th_FINAL_UHD.00500_searchweb.png (320x180) [95.9 KB] || 14756_GOES_50th_FINAL_UHD.00500_thm.png [7.4 KB] || 14756_GOES_50th_FINAL_1080.mp4 (1920x1080) [178.6 MB] || 14756_GOES_50th_FINAL_UHD.en_US.srt [6.7 KB] || 14756_GOES_50th_FINAL_UHD.en_US.vtt [6.4 KB] || 14756_GOES_50th_FINAL_1080.en_US.srt [6.7 KB] || 14756_GOES_50th_FINAL_1080.en_US.vtt [6.4 KB] || 14756_GOES_50th_FINAL_UHD.webm (3840x2160) [20.5 MB] || 14756_GOES_50th_FINAL_UHD.mp4 (3840x2160) [684.3 MB] || ", "hits": 52 }, { "id": 5443, "url": "https://svs.gsfc.nasa.gov/5443/", "result_type": "Visualization", "release_date": "2024-12-17T00:00:00-05:00", "title": "Heliophysics Sentinels 2024", "description": "There have been some changes since the 2022 Heliophysics Fleet. AIM and ICON have been decommissioned while two other instruments have been added. AWE is an instrument mounted on the ISS, and RAD is a particle detector on the Curiosity Mars rover. As of Winter 2024, here's a tour of the NASA Heliophysics fleet from the near-Earth satellites out to the Voyagers beyond the heliopause. || ", "hits": 75 }, { "id": 14545, "url": "https://svs.gsfc.nasa.gov/14545/", "result_type": "Produced Video", "release_date": "2024-03-10T09:55:00-04:00", "title": "Hubble: Our Cosmic Time Machine", "description": "The Hubble Space Telescope is many things. It’s an observatory, a satellite, and an icon of cultural and scientific significance – but perhaps most interestingly, Hubble is also a time machine.Hubble isn’t that far away, locked in a low-Earth orbit just a few hundred miles up that takes about 90 minutes to complete. But with its position just above Earth’s murky atmosphere, Hubble’s transformative view of our universe literally lets us witness our universe’s past. It allows us to effectively travel back in time.The answer is simply light! Watch this video to learn more about Hubble: Humanity’s cosmic time machine!For more information, visit https://nasa.gov/hubble. Credit: NASA's Goddard Space Flight Center Paul Morris: Lead Producer Elizabeth Tammi: ScriptMusic Credit:\"Neon Dreamscape\" by Craig Connelly [PRS] via Focus Music (Publishing) Ltd [PRS], and Universal Production Music.Video Credit:Big Sandwich Rotating On Yellow Backgroundbonjansen/Pond5Eating Grilled Cheese And Ham SandwichBlackBoxGuild/Pond5Woman Listening To Music On Headphones And Dancing To The Rhythmpaul_prescott/Pond5Corporate Employees During Meeting In Office Discussing Topics Related To Salesbarracudamusic/Pond5Teacher Teaching Mathematics On Chalkboard In ClassroomFancyStudio/Pond5Time Lapse Of A Car On A Main Road Driving Home At Nighticsnaps/Pond5Businessman Eating Sandwich And Smiling To Camera In The Citymotion_poland/Pond5Family Tree Animation With Text That Grows. Children And FutureBlackBoxGuild/Pond5Tracking Shot Of Knight Fight In Court. Knight Blocking PunchBlackBoxGuild/Pond5Samurai Posing Towards Mt. FujiBlackBoxGuild/Pond5The Night Sky Is A Showcase Of Twinkling Stars And ConstellationsBlackBoxGuild/Pond5Wide Shot Of An Ancient Hominid, Neanderthal, Homo Sapiens Is Sitting NearBlackBoxGuild/Pond5Majungasaurus Watches As A Meteor Approaches Prehistoric EarthBlackBoxGuild/Pond5Businessman Eating Sandwich During Break In The Parkmotion_poland/Pond5Scooping Peanut Butter Out Of The Jar With A Plastic SpoonBlackBoxGuild/Pond5Death Valley National Park Milky Way Galaxy Time Lapse Night Sky Above Telescopelovemushroom/Pond5Cosmic Speed Of Light Travel Between Nebula Clouds And Star SystemBlackBoxGuild/Pond5Group Of Primitive Savages Hunting Animals In ForestFractalPictures/Pond53D Space Tardis Background Videobeatvideostock/Pond5Sliced White Bread Falling. Slow Motionsoraphotography/Pond5Detail showing Mansa Musa sitting on a throne and holding a gold coinAttributed to Abraham Cresques - This file comes from Gallica Digital Library and is Public DomainSound Effect Credits:Plop SFX PackWARP EFX/Motion ArrayMedieval And Fantasy BattleNargoMusic/Motion ArrayCar Door Closetuttkile/Motion ArraySpace Age Flight MotionslivingroomClassics/Motion ArrayField Ambiencedauzkobza/Motion ArrayEarthquakeNickoMusic/Motion ArrayDeep Cinematic WhooshesOut There Audio/Motion ArrayMedieval Battlefield AmbienceMotion Audio/Motion ArrayGlitch Whooshreadsounds/Motion ArrayDesigned Drop Bass With Slow-moWOW SOUND/Motion ArrayClassic Laser ShotsSFXpecial/Motion ArrayCampfireBad Atmospheric/Motion ArrayFast Driving In Sport CarDjsapa/Motion ArrayNeon LampMedia_M/Motion ArrayPull String Light SwitchAudio Planet/Motion ArrayTime Machine SFXJiltedG/Motion ArrayMotion Whoosh SwipeBeison/Motion Array || ", "hits": 88 }, { "id": 40503, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-earth-science/", "result_type": "Gallery", "release_date": "2023-08-28T00:00:00-04:00", "title": "Hyperwall Power Playlist - Earth Science Focus", "description": "This is a collection of our most powerful, newsworthy, and frequently used Hyperwall-ready visualizations, along with several that haven't gotten the attention they deserve. They're especially great for more general or top-level science talks, or to \"set the scene\" before a deep dive into a more focused subject or dataset. We've tried to cover the subject areas our speakers focus on most. \n\nIf you're not seeing what you're looking for, there is a huge library of visualizations more localized or specialized in subject - please use the Search function above, and filter \"Result type\" for \"Hyperwall Visual.\"\n\n If you'd like to use one of these visualizations in your Hyperwall presentation, we'll need to know which element on which page. On the visualization's web page, below the visual you'd like to use, you'll see a Link icon next to the Download button. All we need is for you to click on that icon and include that link in your presentation Powerpoint/Keynote or visualization list. Additionally, please check our Hyperwall How-To Guide for tips on designing your Hyperwall presentation, file specifications, and Powerpoint/Keynote templates.", "hits": 255 }, { "id": 40505, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-planetary-science-focus/", "result_type": "Gallery", "release_date": "2023-08-28T00:00:00-04:00", "title": "Hyperwall Power Playlist - Planetary Science Focus", "description": "This is a collection of our most powerful, newsworthy, and frequently used Hyperwall-ready visualizations, along with several that haven't gotten the attention they deserve. They're especially great for more general or top-level science talks, or to \"set the scene\" before a deep dive into a more focused subject or dataset. We've tried to cover the subject areas our speakers focus on most. \n\nIf you're not seeing what you're looking for, there is a huge library of visualizations more localized or specialized in subject - please use the Search function above, and filter \"Result type\" for \"Hyperwall Visual.\"\n\n If you'd like to use one of these visualizations in your Hyperwall presentation, we'll need to know which element on which page. On the visualization's web page, below the visual you'd like to use, you'll see a Link icon next to the Download button. All we need is for you to click on that icon and include that link in your presentation Powerpoint/Keynote or visualization list. Additionally, please check our Hyperwall How-To Guide for tips on designing your Hyperwall presentation, file specifications, and Powerpoint/Keynote templates.", "hits": 339 }, { "id": 40507, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-heliophysics-focus/", "result_type": "Gallery", "release_date": "2023-08-28T00:00:00-04:00", "title": "Hyperwall Power Playlist - Heliophysics Focus", "description": "This is a collection of our most powerful, newsworthy, and frequently used Hyperwall-ready visualizations, along with several that haven't gotten the attention they deserve. They're especially great for more general or top-level science talks, or to \"set the scene\" before a deep dive into a more focused subject or dataset. We've tried to cover the subject areas our speakers focus on most. \n\nIf you're not seeing what you're looking for, there is a huge library of visualizations more localized or specialized in subject - please use the Search function above, and filter \"Result type\" for \"Hyperwall Visual.\"\n\n If you'd like to use one of these visualizations in your Hyperwall presentation, we'll need to know which element on which page. On the visualization's web page, below the visual you'd like to use, you'll see a Link icon next to the Download button. All we need is for you to click on that icon and include that link in your presentation Powerpoint/Keynote or visualization list. Additionally, please check our Hyperwall How-To Guide for tips on designing your Hyperwall presentation, file specifications, and Powerpoint/Keynote templates.", "hits": 195 }, { "id": 40518, "url": "https://svs.gsfc.nasa.gov/gallery/hyperwall-power-playlist-astrophysics-focus/", "result_type": "Gallery", "release_date": "2023-08-28T00:00:00-04:00", "title": "Hyperwall Power Playlist - Astrophysics Focus", "description": "This is a collection of our most powerful, newsworthy, and frequently used Hyperwall-ready visualizations, along with several that haven't gotten the attention they deserve. They're especially great for more general or top-level science talks, or to \"set the scene\" before a deep dive into a more focused subject or dataset. We've tried to cover the subject areas our speakers focus on most. \n\nIf you're not seeing what you're looking for, there is a huge library of visualizations more localized or specialized in subject - please use the Search function above, and filter \"Result type\" for \"Hyperwall Visual.\"\n\n If you'd like to use one of these visualizations in your Hyperwall presentation, we'll need to know which element on which page. On the visualization's web page, below the visual you'd like to use, you'll see a Link icon next to the Download button. All we need is for you to click on that icon and include that link in your presentation Powerpoint/Keynote or visualization list. Additionally, please check our Hyperwall How-To Guide for tips on designing your Hyperwall presentation, file specifications, and Powerpoint/Keynote templates.", "hits": 331 }, { "id": 14365, "url": "https://svs.gsfc.nasa.gov/14365/", "result_type": "Produced Video", "release_date": "2023-06-14T11:00:00-04:00", "title": "NASA’s Laser Communications: To the Space Station and Beyond", "description": "NASA’s Laser Communications: To the Space Station and Beyond Finished Production || Illuma-T_Final.09238_print.jpg (1024x576) [69.7 KB] || Illuma-T_Final.09238_searchweb.png (320x180) [62.9 KB] || Illuma-T_Final.09238_thm.png (80x40) [5.5 KB] || ILLUMA-T_Final.mp4 (1920x1080) [727.7 MB] || Illuma-T_Final.mov (1920x1080) [8.1 GB] || Illuma-T_Final.webm (1920x1080) [27.5 MB] || ILLUMA-T.en_US.srt [5.4 KB] || ILLUMA-T.en_US.vtt [5.1 KB] || ", "hits": 41 }, { "id": 40455, "url": "https://svs.gsfc.nasa.gov/gallery/spacecraft-animations/", "result_type": "Gallery", "release_date": "2023-01-24T00:00:00-05:00", "title": "Satellite Animations", "description": "A collection of spacecraft beauty pass animations for current missions.", "hits": 297 }, { "id": 4898, "url": "https://svs.gsfc.nasa.gov/4898/", "result_type": "Visualization", "release_date": "2022-11-23T00:00:00-05:00", "title": "Heliophysics Sentinels 2022", "description": "There has been one significant change since the 2020 Heliophysics Fleet. SET has been decommissioned. As of Fall 2022, here's a tour of the NASA Heliophysics fleet from the near-Earth satellites out to the Voyagers beyond the heliopause.Excepting the Voyager missions, the satellite orbits are color coded for their observing program:Magenta: TIM (Thermosphere, Ionosphere, Mesosphere) observationsYellow: solar observations and imageryCyan: Geospace and magnetosphereViolet: Heliospheric observations || ", "hits": 42 }, { "id": 14108, "url": "https://svs.gsfc.nasa.gov/14108/", "result_type": "Produced Video", "release_date": "2022-02-21T15:00:00-05:00", "title": "GOES Satellites Wildfire Detection and Monitoring", "description": "Music: “Enduring Faith,” by Frederik Wiedmann [BMI]; Icon Trailer Music; Universal Production MusicAdditional GOES-T Footage Courtesy of:Lockheed MartinAdditional Wildfire Footage:CALFIRE_Official/flickr under CC BY-NC 2.0National Interagency Fire CenterCALFIRE_Official/Alaska Fire Service/flickr || 14108_WildfireDetectionandMonitoring_FINAL.03921_print.jpg (1024x576) [140.5 KB] || 14108_WildfireDetectionandMonitoring_FINAL.03921_searchweb.png (320x180) [95.6 KB] || 14108_WildfireDetectionandMonitoring_FINAL.03921_thm.png (80x40) [6.5 KB] || 14108_WildfireDetectionandMonitoring_FINAL_720.mp4 (1280x720) [52.9 MB] || 14108_GOEST_WildfireDetectionandMonitoring_FINAL_lowres.mp4 (1280x720) [60.4 MB] || 14108_WildfireDetectionandMonitoring_FINAL_720.webm (1280x720) [24.7 MB] || 14108_GOEST_WildfireDetectionandMonitoring_FINAL.mp4 (1920x1080) [142.4 MB] || 14108_WildfireDetectionandMonitoring_FINAL_1080.mp4 (1920x1080) [278.3 MB] || 14108_GOEST_WildfireDetectionandMonitoring_FINAL.en_US.srt [5.1 KB] || 14108_GOEST_WildfireDetectionandMonitoring_FINAL.en_US.vtt [4.9 KB] || 14108_GOEST_WildfireDetectionandMonitoring_FINAL_UHD_YOUTUBE.mp4 (3840x2160) [905.9 MB] || 14108_WildfireDetectionandMonitoring_FINAL.mov (1920x1080) [4.8 GB] || ", "hits": 98 }, { "id": 14073, "url": "https://svs.gsfc.nasa.gov/14073/", "result_type": "Produced Video", "release_date": "2022-02-03T00:00:00-05:00", "title": "GOES-T Overview and Beauty Shots", "description": "GOES-T Overview and Upcoming Launch Music: \"Spacey Wave,\" by JC Lemay [SACEM]; Koka; Universal Production MusicAdditional footage provided by Lockheed Martin || GOEST_Overview_FINAL.01901_print.jpg (1024x576) [161.9 KB] || GOEST_Overview_FINAL.01901_searchweb.png (320x180) [98.2 KB] || GOEST_Overview_FINAL.01901_thm.png (80x40) [7.2 KB] || GOEST_Overview_FINAL_VX-319617_lowres.mp4 (1280x720) [50.4 MB] || GOEST_Overview_FINAL_VX-319617_lowres.webm (1280x720) [20.7 MB] || GOEST_Overview_FINAL_1080p.mp4 (1920x1080) [230.5 MB] || GOEST_Overview_FINAL_720p.mp4 (1280x720) [229.7 MB] || GOEST_Overview_FINAL.en_US.srt [3.8 KB] || GOEST_Overview_FINAL.en_US.vtt [3.6 KB] || GOEST_Overview_FINAL.mp4 (3840x2160) [915.1 MB] || GOEST_Overview_FINAL.mov (3840x2160) [15.2 GB] || ", "hits": 25 }, { "id": 4917, "url": "https://svs.gsfc.nasa.gov/4917/", "result_type": "Visualization", "release_date": "2021-11-29T11:00:00-05:00", "title": "ICON Snaps a Peek at the Ionospheric Dynamo", "description": "Visualization of ICON in Earth orbit, camera ahead of the spacecraft looking back on spacecraft and limb of Earth. Magenta curves are lines of Earth's geomagnetic field. Field-of-view (FOV) of MIGHTI imagers (green frustums) and the longitudinal wind vectors (green arrows) it measures are shown. MIGHTI imagers FOV eventually fades out. Vertical plasma speed (red arrows) is measured at the spacecraft. Magnetic field lines turn yellow as measurements of winds by MIGHT provide a connection to influence the plasma velocity measured at the spacecraft, redirecting the plasma flow from upward to downward. || ICONDataView.ICONSyncView+x_.clockSlate_CRTT.HD1080i.000750_print.jpg (1024x576) [135.0 KB] || ICONDataView.ICONSyncView+x_.clockSlate_CRTT.HD1080i.000750_searchweb.png (320x180) [79.4 KB] || ICONDataView.ICONSyncView+x_.clockSlate_CRTT.HD1080i.000750_thm.png (80x40) [5.7 KB] || ICONSyncView+x (1920x1080) [0 Item(s)] || ICONDataView.ICONSyncView+x.HD1080i_p30.mp4 (1920x1080) [36.4 MB] || ICONDataView.ICONSyncView+x.HD1080i_p30.webm (1920x1080) [5.1 MB] || ICONSyncView+x (3840x2160) [0 Item(s)] || ICONDataView.ICONSyncView+x.2160p30.mp4 (3840x2160) [114.3 MB] || ICONDataView.ICONSyncView+x.HD1080i_p30.mp4.hwshow || ", "hits": 52 }, { "id": 14025, "url": "https://svs.gsfc.nasa.gov/14025/", "result_type": "Produced Video", "release_date": "2021-11-29T11:00:00-05:00", "title": "Strong Winds Power Electric Fields in the Upper Atmosphere", "description": "Using observations from NASA’s ICON mission, scientists presented the first direct measurements of Earth’s long-theorized dynamo on the edge of space: a wind-driven electrical generator that spans the globe 60-plus miles above our heads. The dynamo churns in the ionosphere, the electrically charged boundary between Earth and space. It’s powered by tidal winds in the upper atmosphere that are faster than most hurricanes and rise from the lower atmosphere, creating an electrical environment that can affect satellites and technology on Earth. The new work, published today in Nature Geoscience, improves our understanding of the ionosphere, which helps scientists better predict space weather and protect our technology from its effects.More information: https://www.nasa.gov/feature/goddard/2021/strong-winds-power-electric-fields-in-upper-atmosphere-icon/ || ", "hits": 102 }, { "id": 13495, "url": "https://svs.gsfc.nasa.gov/13495/", "result_type": "Produced Video", "release_date": "2021-03-09T14:00:00-05:00", "title": "GLOBE Observer: Tree Height", "description": "Music: “Treehouse Imaginations” by Zachary Scott Lemmon [BMI], Killer Tracks [BMI], Icon Trailer Music; Universal Production Music; SFX: Elk Chorus - Yellowstone National Park, NPS/Jennifer Jerrett Additional footage provided by Artbeats and Pond5 || TreeHeight.jpg (1920x1080) [2.8 MB] || TreeHeight_searchweb.png (320x180) [125.3 KB] || TreeHeight_thm.png (80x40) [9.7 KB] || 13495_GO_ShortTreeHeight_Final.mov (1920x1080) [1.9 GB] || 13495_GO_ShortTreeHeight_Final_lowres.mp4 (1280x720) [25.3 MB] || FACEBOOK_720_13495_GO_ShortTreeHeight_Final_facebook_720.mp4 (1280x720) [92.7 MB] || YOUTUBE_1080_13495_GO_ShortTreeHeight_Final_youtube_1080.mp4 (1920x1080) [127.7 MB] || 13495_GO_ShortTreeHeight_Final.webm (960x540) [32.3 MB] || 13495_GO_TreeHeight_Short_FINAL.en_US.srt [1.9 KB] || 13495_GO_TreeHeight_Short_FINAL.en_US.vtt [1.9 KB] || ", "hits": 69 }, { "id": 4887, "url": "https://svs.gsfc.nasa.gov/4887/", "result_type": "Visualization", "release_date": "2021-03-01T10:00:00-05:00", "title": "Heliophysics Sentinels 2020 (Forecast Version)", "description": "In addition to the NASA missions used in research for space weather (see 2020 Heliophysics Fleet) there are additional missions operated by NOAA used for space weather forecasting. As of spring 2020, here's a tour of the NASA and NOAA Heliophysics fleets from the near-Earth satellites out to the inner solar system.The satellite orbits are color coded for their observing program:Magenta: TIM (Thermosphere, Ionosphere, Mesosphere) observationsYellow: solar observations and imageryCyan: Geospace and magnetosphereViolet: Heliospheric observations || ", "hits": 36 }, { "id": 4822, "url": "https://svs.gsfc.nasa.gov/4822/", "result_type": "Visualization", "release_date": "2020-09-15T10:00:00-04:00", "title": "Heliophysics Sentinels 2020", "description": "There have been few changes since the 2018 Heliophysics Fleet. Van Allen Probes and SORCE have been decommissioned, while Solar Orbiter, ICON and SET have been added. As of spring 2020, here's a tour of the NASA Heliophysics fleet from the near-Earth satellites out to the Voyagers beyond the heliopause.Excepting the Voyager missions, the satellite orbits are color coded for their observing program:Magenta: TIM (Thermosphere, Ionosphere, Mesosphere) observationsYellow: solar observations and imageryCyan: Geospace and magnetosphereViolet: Heliospheric observations || ", "hits": 36 }, { "id": 13494, "url": "https://svs.gsfc.nasa.gov/13494/", "result_type": "Produced Video", "release_date": "2019-12-11T13:00:00-05:00", "title": "AGU 2019 - New Science from NASA's Parker Solar Probe Mission", "description": "Little more than a year into its mission, Parker Solar Probe has returned gigabytes of data on the Sun and its atmosphere. The very first science from the Parker mission is just beginning to be shared, and five researchers presented new findings from the mission at the fall meeting of the American Geophysical Union on Dec. 11, 2019. Their research hints at the processes behind both the Sun's continual outflow of material — the solar wind — and more infrequent solar storms that can disrupt technology and endanger astronauts, along with new insight into space dust that creates the Geminids meteor shower.Speakers:Nicholeen Viall - Research Astrophysicist, NASA's Goddard Space Flight CenterTim Horbury - Professor of Physics, Imperial College LondonKelly Korreck - Astrophysicist, Head of Science Operations for SWEAP Suite, Harvard and Smithsonian Center for AstrophysicsNathan Schwadron - Presidential Chair, Norman S. and Anna Marie Waite Professor, University of New HampshireKarl Battams - Computational Scientist, U.S. Naval Research Laboratory || ", "hits": 101 }, { "id": 13502, "url": "https://svs.gsfc.nasa.gov/13502/", "result_type": "Produced Video", "release_date": "2019-12-10T17:00:00-05:00", "title": "AGU 2019 — Postcards from the edge of space: New images, new phenomena, and new insights", "description": "In a Dec. 10 press event at the fall meeting of the American Geophysical Union in San Francisco, California, three scientists presented new images of the ionosphere, the dynamic region where Earth’s atmosphere meets space. Home to astronauts and everyday technology like radio and GPS, the ionosphere constantly responds to changes from space above and Earth below.The collection of images presented include the first images from NASA’s ICON, new science results from NASA’s GOLD, and observations of a fleeting, never-before-studied aurora. Together, they bring color to invisible processes that have widespread implications for the part of space that is closest to home.SPEAKERS:• Jennifer Briggs, Pepperdine University, Malibu, California, United States• Richard Eastes, University of Colorado Boulder, Boulder, Colorado, United States• Thomas Immel, University of California Berkeley, Berkeley, California, United States || ", "hits": 53 }, { "id": 20299, "url": "https://svs.gsfc.nasa.gov/20299/", "result_type": "Animation", "release_date": "2019-12-04T13:00:00-05:00", "title": "Parker Science Result animations", "description": "On Dec. 4, 2019, four new papers in the journal Nature describe what scientists working with data from NASA's Parker Solar Probe have learned from this unprecedented exploration of our star — and what they look forward to learning next. These findings reveal new information about the behavior of the material and particles that speed away from the Sun, bringing scientists closer to answering fundamental questions about the physics of our star. These animations represent five of those findings. || ", "hits": 201 }, { "id": 13335, "url": "https://svs.gsfc.nasa.gov/13335/", "result_type": "Produced Video", "release_date": "2019-10-04T10:00:00-04:00", "title": "NASA’s Mission to Explore the Connection Between Earth’s Weather and Space", "description": "Broll and Canned Interviews will be added on October 9th at 5:45 a.m. Click HERE for audio sound bites with NASA Scientist Sarah Jones.Click HERE for a canned interview with NASA Scientist Alex Young.Click HERE for a canned interview with NASA Scientist Alex Young looking off camera. || Screen_Shot_2019-10-01_at_4.31.11_PM.png (2764x382) [2.0 MB] || Screen_Shot_2019-10-01_at_4.31.11_PM_print.jpg (1024x141) [52.3 KB] || Screen_Shot_2019-10-01_at_4.31.11_PM_searchweb.png (320x180) [112.1 KB] || Screen_Shot_2019-10-01_at_4.31.11_PM_thm.png (80x40) [6.6 KB] || ", "hits": 46 }, { "id": 13221, "url": "https://svs.gsfc.nasa.gov/13221/", "result_type": "Produced Video", "release_date": "2019-06-10T10:00:00-04:00", "title": "NASA Tech on SpaceX Falcon Heavy Launch - Media Telecon Resources", "description": "NASA is sending four technology missions that will help improve future spacecraft design and performance into space on the next SpaceX Falcon Heavy rocket launch. Experts will discuss these technologies, and how they complement NASA’s Moon to Mars exploration plans, during a media teleconference Monday, June 10 at 1 p.m. EDT.Audio of the teleconference will be streamed live online at: https://www.nasa.gov/liveParticipants in the briefing will be:Jim Reuter, acting associate administrator of NASA’s Space Technology Mission Directorate, will discuss how technology drives exploration to the Moon and beyond.Jill Seubert, deputy principal investigator for the Deep Space Atomic Clock at NASA’s Jet Propulsion Laboratory, will discuss how to advance exploration in deep space with a miniaturized, ultra-precise, mercury-ion atomic clock that is orders of magnitude more stable than today’s best navigation clocks.Don Cornwell, director of the Advanced Communications and Navigation Division of NASA’s Space Communications and Navigation program, will discuss how a more stable, space-based atomic clock could benefit future missions to the Moon and Mars.Christopher McLean, principal investigator for NASA’s Green Propellant Infusion Mission (GPIM) at Ball Aerospace, will discuss the demonstration of a green alternative to conventional chemical propulsion systems for next-generation launch vehicles and spacecraft. Joe Cassady, executive director for space at Aerojet Rocketdyne, will discuss the five thrusters and propulsion system aboard GPIM.Nicola Fox, director of the Heliophysics Division of NASA’s Science Mission Directorate, will discuss Space Environment Testbeds and the importance of protecting satellites from space radiation.Richard Doe, payload program manager for the Enhanced Tandem Beacon Experiment at SRI International, will discuss how a pair of NASA CubeSats will work with six satellites of the National Oceanographic and Atmospheric Administration’s (NOAA’s) COSMIC-2 mission to study disruptions of signals that pass through Earth’s upper atmosphere.To participate in the teleconference, media must contact Clare Skelly at 202-358-4273 or clare.a.skelly@nasa.gov by 10 a.m. June 10. Media questions may be submitted on Twitter during the teleconference using the hashtag #askNASA.NASA’s four missions will share a ride on the Falcon Heavy with about 20 satellites from government and research institutions that make up the Department of Defense’s Space Test Program-2 (STP-2) mission. SpaceX and the U.S. Air Force Space and Missile Systems Center, which manages STP-2, are targeting 11:30 p.m. Saturday, June 22, for launch from historic Launch Complex 39A at NASA’s Kennedy Space Center in Florida.Charged with returning astronauts to the Moon within five years, NASA’s Artemis lunar exploration plans are based on a two-phase approach: the first is focused on speed – landing astronauts on the Moon by 2024 – while the second will establish a sustained human presence on and around the Moon by 2028. We will use what we learn on the Moon to prepare to send astronauts to Mars. The technology missions on this launch will advance a variety of future exploration missions.For more information about NASA’s Moon to Mars exploration plans, visit:https://www.nasa.gov/moontomarsFor more information about the NASA technologies aboard this launch, visit:https://www.nasa.gov/spacexLearn more about NASA’s Deep Space Atomic Clock: https://www.nasa.gov/mission_pages/tdm/clock/index.htmlLearn more about NASA’s Green Propellant Infusion Mission: https://www.nasa.gov/mission_pages/tdm/green/index.htmlSPACE TEST PROGRAM-2 || ", "hits": 64 }, { "id": 13107, "url": "https://svs.gsfc.nasa.gov/13107/", "result_type": "Produced Video", "release_date": "2018-11-06T16:00:00-05:00", "title": "ICON Video File", "description": "Slug: NASA Mission to Study the Boundary Between Earth and Space The Ionospheric Connection Explorer, or ICON, will study the dynamic zone high in our atmosphere where Earth weather and space weather meet — a region that plays a major role in the safety of our satellites and reliability of communications signals.TRT: 5:25 Edited B-roll RT: :35Interview Excerpts RT: 1:24 Additional B-roll RT: 1:28 Supers(s): NASACenter Contact: Karen Fox, karen.f.fox@nasa.gov, 301-286-6284HQ Contact: Dwayne Brown, dwayne.c.brown@nasa.gov, 202-358-1726 || ", "hits": 15 }, { "id": 13106, "url": "https://svs.gsfc.nasa.gov/13106/", "result_type": "Produced Video", "release_date": "2018-11-06T03:30:00-05:00", "title": "Tour the Plane Giving NASA’s ICON a Ride to Space", "description": "Early in the morning of Nov. 7, 2018, NASA launches the Ionospheric Connection Explorer, or ICON, a spacecraft that will explore the dynamic region where Earth meets space. ICON launches on a Northrop Grumman Pegasus XL rocket, which is carried aloft by the Stargazer L-1011 aircraft.Join NASA on a behind-the-scenes tour of this plane, once a jet airliner and now uniquely retrofitted to boost spacecraft into low-Earth orbit. Learn about ICON’s science and meet the people — including an engineer, technician, and pilot — who will help launch the spacecraft into orbit.Learn more at: nasa.gov/icon || ", "hits": 31 }, { "id": 12902, "url": "https://svs.gsfc.nasa.gov/12902/", "result_type": "Produced Video", "release_date": "2018-10-22T10:00:00-04:00", "title": "The Secrets behind Earth’s Multi-colored Glow", "description": "What does our planet look like from space? Most are familiar with the beloved images of the blue marble or pale blue dot — Earth from 18,000 and 3.7 billion miles away, respectively. But closer to home, within the nearest region of space, you might encounter an unfamiliar sight. If you peer down on Earth from just 300 miles above the surface, near the orbit of the International Space Station, you can see vibrant swaths of red and green or purple and yellow light emanating from the upper atmosphere. This is airglow. Airglow occurs when atoms and molecules in the upper atmosphere, excited by sunlight, emit light in order to shed their excess energy. Or, it can happen when atoms and molecules that have been ionized by sunlight collide with and capture a free electron. In both cases, they eject a particle of light — called a photon — in order to relax again. The phenomenon is similar to auroras, but where auroras are driven by high-energy particles originating from the solar wind, airglow is energized by day-to-day solar radiation. || ", "hits": 606 }, { "id": 12974, "url": "https://svs.gsfc.nasa.gov/12974/", "result_type": "Produced Video", "release_date": "2018-10-21T12:00:00-04:00", "title": "ICON's Launch Site", "description": "The Ionospheric Connection Explorer, or ICON, will study the frontier of space: the dynamic zone high in our atmosphere where Earth weather and space weather meet. In fall 2018, the mission launches on an Northrop Grumman (formerly Orbital ATK) Pegasus XL rocket from NASA's Kennedy Space Center in Florida. || ", "hits": 44 }, { "id": 12971, "url": "https://svs.gsfc.nasa.gov/12971/", "result_type": "Produced Video", "release_date": "2018-10-19T13:00:00-04:00", "title": "Unboxing a New NASA Spacecraft", "description": "Go behind the scenes as we unbox NASA’s Ionospheric Connection Explorer, or ICON, after its arrival at Vandenberg Air Force Base in California. Northrop Grumman engineer Steve Turek and NASA EDGE’s Chris Giersch walk us through the whole process of unboxing a spacecraft – from the instrument that records every tiny bump on its journey to the special crane used to lift the spacecraft to its new home.ICON launches in fall 2018 from NASA's Kennedy Space Center in Florida to study Earth’s interface to space. Read more about the ICON mission: nasa.gov/icon || ", "hits": 26 }, { "id": 13096, "url": "https://svs.gsfc.nasa.gov/13096/", "result_type": "Produced Video", "release_date": "2018-10-18T13:00:00-04:00", "title": "ICON Pre-Launch Live Shots", "description": "B-roll and canned interviews will be added on Wednesday, Oct 24 by 6:00pm || ICON_WebBanner_2018.jpg (3792x597) [550.7 KB] || ICON_WebBanner_2018_print.jpg (1024x161) [101.5 KB] || ICON_WebBanner_2018_searchweb.png (320x180) [119.7 KB] || ICON_WebBanner_2018_thm.png (80x40) [6.5 KB] || ", "hits": 33 }, { "id": 12947, "url": "https://svs.gsfc.nasa.gov/12947/", "result_type": "Produced Video", "release_date": "2018-10-16T12:00:00-04:00", "title": "Launching an ICON", "description": "The Ionospheric Connection Explorer will explore the mysteries of where Earth meets space. || STORYCOVER_ICON_Image_Portrait16x9_1024x576.jpg (1024x576) [187.1 KB] || STORYCOVER_ICON_Image_Portrait16x9.jpg (2550x1434) [637.0 KB] || STORYCOVER_NEW_ICON_Image_Portrait.jpg (2550x3300) [707.1 KB] || STORYCOVER_ICON_Image_Portrait16x9_searchweb.png (320x180) [82.4 KB] || STORYCOVER_ICON_Image_Portrait16x9_thm.png (80x40) [5.7 KB] || ", "hits": 46 }, { "id": 13051, "url": "https://svs.gsfc.nasa.gov/13051/", "result_type": "Produced Video", "release_date": "2018-08-24T13:55:00-04:00", "title": "NASA's OSIRIS-REx Approaches Asteroid Bennu", "description": "NASA's OSIRIS-REx asteroid sample return mission launched in 2016 and now (August, 2018) is entering its approach phase. OSIRIS-REx will arrive at asteroid Bennu in December, 2018. OSIRIS-REx will help unveil the mysteries of our solar system's formation.For more information, go to nasa.gov/osirisrex or asteroidmission.org. || ", "hits": 25 }, { "id": 12963, "url": "https://svs.gsfc.nasa.gov/12963/", "result_type": "Produced Video", "release_date": "2018-06-02T15:00:00-04:00", "title": "Airglow Imagery", "description": "Airglow occurs when atoms and molecules in the upper atmosphere, excited by sunlight, emit light in order to shed their excess energy. The phenomenon is similar to auroras, but where auroras are driven by high-energy particles originating from the solar wind, airglow is sparked by day-to-day solar radiation. Airglow carries information on the upper atmosphere’s temperature, density, and composition, but it also helps us trace how particles move through the region itself. Vast, high-altitude winds sweep through the ionosphere, pushing its contents around the globe — and airglow’s subtle dance follows their lead, highlighting global patterns. || ", "hits": 1157 }, { "id": 12975, "url": "https://svs.gsfc.nasa.gov/12975/", "result_type": "Produced Video", "release_date": "2018-06-02T15:00:00-04:00", "title": "ICON Photos", "description": "The Ionospheric Connection Explorer, or ICON, is a low-Earth orbiting satellite that will give us new information about how Earth’s atmosphere interacts with near-Earth space — a give-and-take that plays a major role in the safety of our satellites and reliability of communications signals.Specifically, ICON investigates the connections between the neutral atmosphere — which extends from here near the surface to far above us, at the edge of space — and the electrically charged part of the atmosphere, called the ionosphere. The particles of the ionosphere carry electrical charge that can disrupt communications signals, cause satellites in low-Earth orbit to become electrically charged, and, in extreme cases, cause power outages on the ground. || ", "hits": 56 }, { "id": 12910, "url": "https://svs.gsfc.nasa.gov/12910/", "result_type": "Produced Video", "release_date": "2018-06-02T13:00:00-04:00", "title": "ICON Launch Sequence", "description": "The Ionospheric Connection Explorer, or ICON, will study the frontier of space: the dynamic zone high in our atmosphere where Earth weather and space weather meet. In fall 2018, the mission launches on an Northrop Grumman (formerly Orbital ATK) Pegasus XL rocket from NASA's Kennedy Space Center in Florida. || ", "hits": 42 }, { "id": 12960, "url": "https://svs.gsfc.nasa.gov/12960/", "result_type": "Infographic", "release_date": "2018-05-31T19:00:00-04:00", "title": "Ionosphere Graphics", "description": "Stretching from roughly 50 to 400 miles above Earth’s surface, the ionosphere is an electrified layer of the upper atmosphere, generated by extreme ultraviolet radiation from the Sun. It’s neither fully Earth nor space, and instead, reacts to both terrestrial weather below and solar energy streaming in from above, forming a complex space weather system of its own. The particles of the ionosphere carry electrical charge that can disrupt communications signals, cause satellites in low-Earth orbit to become electrically charged, and, in extreme cases, cause power outages on the ground. Positioned on the edge of space and intermingled with the neutral atmosphere, the ionosphere’s response to conditions on Earth and in space is difficult to pin down. || ", "hits": 439 }, { "id": 12961, "url": "https://svs.gsfc.nasa.gov/12961/", "result_type": "Produced Video", "release_date": "2018-05-24T19:00:00-04:00", "title": "ICON Graphics", "description": "The Ionospheric Connection Explorer, or ICON, is a low-Earth orbiting satellite that will give us new information about how Earth’s atmosphere interacts with near-Earth space — a give-and-take that plays a major role in the safety of our satellites and reliability of communications signals. Specifically, ICON investigates the connections between the neutral atmosphere — which extends from here near the surface to far above us, at the edge of space — and the electrically charged part of the atmosphere, called the ionosphere. The particles of the ionosphere carry electrical charge that can disrupt communications signals, cause satellites in low-Earth orbit to become electrically charged, and, in extreme cases, cause power outages on the ground. || ", "hits": 50 }, { "id": 40346, "url": "https://svs.gsfc.nasa.gov/gallery/icon/", "result_type": "Gallery", "release_date": "2018-03-27T00:00:00-04:00", "title": "ICON", "description": "The Ionospheric Connection Explorer, or ICON, is a low-Earth orbiting satellite that will give us new information about how Earth’s atmosphere interacts with near-Earth space — a give-and-take that plays a major role in the safety of our satellites and reliability of communications signals. \n\nSpecifically, ICON investigates the connections between the neutral atmosphere — which extends from near Earth’s surface to far above us, at the edge of space— and the electrically charged part of the atmosphere, called the ionosphere. The particles of the ionosphere carry electrical charge that can disrupt communications signals, cause satellites in low-Earth orbit to become electrically charged, and, in extreme cases, cause power outages on the ground.", "hits": 142 }, { "id": 12823, "url": "https://svs.gsfc.nasa.gov/12823/", "result_type": "Produced Video", "release_date": "2018-02-05T12:00:00-05:00", "title": "Where Earth Meets Space", "description": "NASA’s newest mission, GOLD, will explore the ever-changing boundary between Earth and space. || 12827_GOLD_SES14satellite.00300_print.png (1920x1080) [2.2 MB] || 12827_GOLD_SES14satellite.00300_print_1024x576.jpg (1024x576) [122.0 KB] || 12827_GOLD_SES14satellite.00300_print_print.jpg (1024x576) [133.7 KB] || 12827_GOLD_SES14satellite.00300_print_searchweb.png (320x180) [82.5 KB] || 12827_GOLD_SES14satellite.00300_print_thm.png (80x40) [5.7 KB] || ", "hits": 248 }, { "id": 12825, "url": "https://svs.gsfc.nasa.gov/12825/", "result_type": "Infographic", "release_date": "2018-01-24T12:00:00-05:00", "title": "GOLD Resources", "description": "The Global-scale Observations of the Limb and Disk, or GOLD, mission is designed to explore the nearest reaches of space. Capturing never-before-seen images of Earth’s upper atmosphere, GOLD explores in unprecedented detail our space environment — which is home to astronauts, radio signals used to guide airplanes and ships, as well as satellites that provide communications and GPS systems. The more we know about the fundamental physics of this region of space, the more we can protect our assets there.Gathering observations from geostationary orbit above the Western Hemisphere, GOLD measures the temperature and composition of neutral gases in Earth’s thermosphere. This part of the atmosphere co-mingles with the ionosphere, which is made up of charged particles. Both the Sun from above and terrestrial weather from below can change the types, numbers, and characteristics of the particles found here — and GOLD helps track those changes.Activity in this region is responsible for a variety of key space weather events. GOLD scientists are particularly interested in the cause of dense, unpredictable bubbles of charged gas that appear over the equator and tropics, sometimes causing communication problems. As we discover the very nature of the Sun-Earth interaction in this region, the mission could ultimately lead to ways to improve forecasts of such space weather and mitigate its effects. || ", "hits": 68 }, { "id": 40345, "url": "https://svs.gsfc.nasa.gov/gallery/gold/", "result_type": "Gallery", "release_date": "2018-01-17T00:00:00-05:00", "title": "GOLD – Global-scale Observations of the Limb and Disk", "description": "NASA’s Global-scale Observations of the Limb and Disk (GOLD) mission focuses on two parts of Earth’s upper atmosphere stretching from about 50 to 400 miles in altitude — the neutral layer called the thermosphere, and the electrically charged particles that make up the ionosphere. From its vantage point on a commercial communications satellite in geostationary orbit, the GOLD instrument makes hemisphere-wide observations of the ionosphere about every 30 minutes. This unprecedented birds-eye view is giving scientists new insights into how this region changes.\n\nGOLD launched on Jan. 25, 2018, from the Guiana Space Centre in Kourou, French Guiana, aboard an Ariane 5 rocket as a hosted payload on the SES-14 commercial satellite.\n\nLearn more: https://science.nasa.gov/mission/gold/", "hits": 113 }, { "id": 12817, "url": "https://svs.gsfc.nasa.gov/12817/", "result_type": "Produced Video", "release_date": "2018-01-05T13:00:00-05:00", "title": "Why NASA Is Exploring The Edge Of Our Planet", "description": "The Global-scale Observations of the Limb and Disk, or GOLD, instrument launches aboard a commercial communications satellite in January 2018 to inspect the dynamic intermingling of space and Earth’s uppermost atmosphere. Together, GOLD and another NASA mission, Ionospheric Connection Explorer spacecraft, or ICON, will provide the most comprehensive of Earth’s upper atmosphere we’ve ever had.Above the ozone layer, the ionosphere is a part of Earth’s atmosphere where particles have been cooked into a sea of electrically-charged electrons and ions by the Sun’s radiation. The ionosphere is co-mingled with the very highest — and quite thin — layers of Earth’s neutral upper atmosphere, making this region an area that is constantly in flux undergoing the push-and-pull between Earth’s conditions and those in space. Increasingly, these layers of near-Earth space are part of the human domain, as it’s home not only to astronauts, but to radio signals used to guide airplanes and ships, and satellites that provide our communications and GPS systems. Understanding the fundamental processes that govern our upper atmosphere and ionosphere is crucial to improve situational awareness that helps protect astronauts, spacecraft and humans on the ground.GOLD, in geostationary orbit over the Western Hemisphere, will build up a full-disk view of the ionosphere and upper atmosphere every half hour, providing detailed large-scale measurements of related processes — a cadence which makes it the first mission to be able to monitor the true weather of the upper atmosphere. GOLD is also able to focus in on a tighter region and scan more quickly, to complement additional research plans as needed. || ", "hits": 62 }, { "id": 12820, "url": "https://svs.gsfc.nasa.gov/12820/", "result_type": "Produced Video", "release_date": "2018-01-04T00:00:00-05:00", "title": "Going for GOLD: Exploring the Interface to Space", "description": "Going for GOLD: Exploring the Interface to Space || 12820_GOLD_FB_Live.00001_print.jpg (1024x576) [125.3 KB] || 12820_GOLD_FB_Live.00001_searchweb.png (320x180) [84.7 KB] || 12820_GOLD_FB_Live.00001_thm.png (80x40) [6.6 KB] || 12820_GOLD_FB_Live.mp4 (1280x720) [5.1 GB] || 12820_GOLD_FB_Live.mov (1280x720) [41.9 GB] || 12820_GOLD_FB_Live.webm (960x540) [1.7 GB] || 12820_GOLD_FB_Live.en_US.srt [119.6 KB] || 12820_GOLD_FB_Live.en_US.vtt [112.9 KB] || ", "hits": 27 }, { "id": 12532, "url": "https://svs.gsfc.nasa.gov/12532/", "result_type": "Produced Video", "release_date": "2017-11-07T14:00:00-05:00", "title": "Welcome to the Ionosphere", "description": "Music credit: Foxy Trot by Luis Enriquez Bacalov Complete transcript available.Watch this video on the NASA Goddard YouTube channel. || ionosphere_thumb.jpg (1920x1080) [69.9 KB] || ionosphere_thumb_searchweb.png (320x180) [57.3 KB] || ionosphere_thumb_thm.png (80x40) [6.3 KB] || APPLE_TV-12532_Welcome_to_the_ionosphere_bsideV4_appletv.webm (1280x720) [24.0 MB] || APPLE_TV-12532_Welcome_to_the_ionosphere_bsideV4_appletv.m4v (1280x720) [116.4 MB] || APPLE_TV-12532_Welcome_to_the_ionosphere_bsideV4_appletv_subtitles.m4v (1280x720) [116.5 MB] || YOUTUBE_1080-12532_Welcome_to_the_ionosphere_bsideV4_youtube_1080.mp4 (1920x1080) [346.2 MB] || NASA_TV-12532_Welcome_to_the_ionosphere_bsideV4.mpeg (1280x720) [691.7 MB] || 12532_Welcome_to_the_ionosphere_bsideV2_lowres.en_US.srt [3.8 KB] || 12532_Welcome_to_the_ionosphere_bsideV2_lowres.en_US.vtt [3.8 KB] || 12532_Welcome_to_the_ionosphere_bsideV4_lowres.mp4 (480x272) [29.2 MB] || LARGE_MP4-12532_Welcome_to_the_ionosphere_bsideV4_large.mp4 (3840x2160) [220.8 MB] || NASA_PODCAST-12532_Welcome_to_the_ionosphere_bsideV4_ipod_sm.mp4 (320x240) [37.3 MB] || 12532_Welcome_to_the_ionosphere_bsideV4.mov (3840x2160) [10.1 GB] || ", "hits": 175 }, { "id": 4594, "url": "https://svs.gsfc.nasa.gov/4594/", "result_type": "Visualization", "release_date": "2017-10-31T10:00:00-04:00", "title": "ICON Scans the Ionosphere", "description": "ICON orbits Earth at 575 kilometers altitude, measuring the composition and motions of the ionosphere. || IRIDaily.limbwICON_OionHwindIGRF.clockSlate_CRTT.HD1080i.000870_print.jpg (1024x576) [105.7 KB] || IRIDaily.limbwICON_OionHwindIGRF.clockSlate_CRTT.HD1080i.000870_searchweb.png (320x180) [63.8 KB] || IRIDaily.limbwICON_OionHwindIGRF.clockSlate_CRTT.HD1080i.000870_thm.png (80x40) [5.0 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || IRIDaily.limbwICON_OionHwindIGRF.HD1080i_p30.mp4 (1920x1080) [76.4 MB] || IRIDaily.limbwICON_OionHwindIGRF.HD1080i_p30.webm (1920x1080) [10.9 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || IRIDaily.limbwICON_OionHwindIGRF.UHD3840_2160p30.mp4 (3840x2160) [217.4 MB] || IRIDaily.limbwICON_OionHwindIGRF.HD1080i_p30.mp4.hwshow [210 bytes] || ", "hits": 105 }, { "id": 12699, "url": "https://svs.gsfc.nasa.gov/12699/", "result_type": "Produced Video", "release_date": "2017-10-18T14:00:00-04:00", "title": "Meet ICON: NASA’s Airglow Explorer", "description": "Music credit: Design Principle by Wayne RobertsComplete transcript available. || iss_composite_test_182.jpg (4256x2832) [12.8 MB] || iss_composite_test_182_searchweb.png (320x180) [99.0 KB] || iss_composite_test_182_thm.png (80x40) [6.2 KB] || LARGE_MP4-12699_ICON_Overview_V2__large.mp4 (1920x1080) [148.3 MB] || NASA_TV-12699_ICON_Overview_V2_.mpeg (1280x720) [494.2 MB] || APPLE_TV-12699_ICON_Overview_V2__appletv.m4v (1280x720) [75.3 MB] || YOUTUBE_1080-12699_ICON_Overview_V2__youtube_1080.mp4 (1920x1080) [234.8 MB] || PRORES_B-ROLL-12699_ICON_Overview_V2__prores.mov (1280x720) [1.9 GB] || YOUTUBE_HQ-12699_ICON_Overview_V2__youtube_hq.mov (1920x1080) [539.3 MB] || 12699_ICON_Overview_V2_.mov (1920x1080) [3.7 GB] || LARGE_MP4-12699_ICON_Overview_V2__large.webm (1920x1080) [16.3 MB] || APPLE_TV-12699_ICON_Overview_V2__appletv_subtitles.m4v (1280x720) [75.3 MB] || 12699_ICON_Overview_V2.en_US.srt [2.4 KB] || 12699_ICON_Overview_V2.en_US.vtt [2.5 KB] || NASA_PODCAST-12699_ICON_Overview_V2__ipod_sm.mp4 (320x240) [25.4 MB] || 12699_ICON_Overview_V2__lowres.mp4 (480x272) [20.3 MB] || ", "hits": 49 }, { "id": 40337, "url": "https://svs.gsfc.nasa.gov/gallery/lrosolar-eclipse/", "result_type": "Gallery", "release_date": "2017-07-17T00:00:00-04:00", "title": "LRO and Solar Eclipse Events", "description": "This page features videos for the 2017 Solar Eclipse Events being coordinated with the LRO Mission production team.", "hits": 150 }, { "id": 40335, "url": "https://svs.gsfc.nasa.gov/gallery/interfaceto-space/", "result_type": "Gallery", "release_date": "2017-06-23T00:00:00-04:00", "title": "Interface to Space", "description": "The ionosphere is layer of the upper atmosphere (60-1000 km up) where the neutral atoms and molecules of the lower atmosphere transition to the plasma of space.", "hits": 97 }, { "id": 20265, "url": "https://svs.gsfc.nasa.gov/20265/", "result_type": "Animation", "release_date": "2017-04-03T13:00:00-04:00", "title": "ICON Beauty Pass", "description": "Beauty pass showing ICON observing the ionosphere. Credit: NASA/GSFC/CIL || AirGlow_final_ProRes.00001_print.jpg (1024x576) [87.7 KB] || AirGlow_final_ProRes.00001_web.png (320x180) [74.1 KB] || AirGlow_final_ProRes.00001_searchweb.png (180x320) [74.1 KB] || AirGlow_final_ProRes.00001_thm.png (80x40) [6.0 KB] || AirGlow_final_H264.mov (1920x1080) [19.5 MB] || 1920x1080_16x9_60p (1920x1080) [0 Item(s)] || AirGlow_final_ProRes.webm (1920x1080) [1.0 MB] || AirGlow_final_ProRes.mov (1920x1080) [304.3 MB] || ", "hits": 28 }, { "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": 63 }, { "id": 12457, "url": "https://svs.gsfc.nasa.gov/12457/", "result_type": "Produced Video", "release_date": "2016-12-14T12:00:00-05:00", "title": "AGU Ionosphere Press Conference", "description": "The ionosphere is a layer of charged particles in Earth’s atmosphere that extends from about 50 to 360 miles above the surface of Earth. Processes in the ionosphere also create bright swaths of color in the sky, known as airglow. Credit: NASA GSFC || AGUIonosphereV4_1.jpg (1280x960) [109.7 KB] || ", "hits": 57 }, { "id": 30822, "url": "https://svs.gsfc.nasa.gov/30822/", "result_type": "Infographic", "release_date": "2016-12-06T00:00:00-05:00", "title": "NASA's Heliophysics Fleet", "description": "The current Heliophysics fleet || hpd-fleet-chart-jan-2024_print.jpg (1024x576) [180.0 KB] || hpd-fleet-chart-jan-2024.png (3840x2160) [7.3 MB] || hpd-fleet-chart-jan-2024_searchweb.png (320x180) [91.3 KB] || hpd-fleet-chart-jan-2024_thm.png (80x40) [7.2 KB] || nasas-fleets-by-division-helio-jewel.hwshow [228 bytes] ||", "hits": 65 }, { "id": 4498, "url": "https://svs.gsfc.nasa.gov/4498/", "result_type": "Visualization", "release_date": "2016-10-27T14:00:00-04:00", "title": "ICON and GOLD: Exploring the Interface to Space", "description": "A basic view of the orbits for ICON (Ionospheric Connections Explorer) and GOLD (Global-scale Observations of the Limb and Disk). These missions will conduct measurements of ionospheric composition, ionization, and winds to better understand the connection between space weather and its terrestrial impacts.In this visualization, we present GOLD (in geostationary orbit around Earth) and ICON (in low Earth orbit). The colors over Earth represent model data from the IRI (International Reference Ionosphere) model of the density of the singly-ionized oxygen atom at an altitude of 350 kilometers. Red represents high density. The ion density is enhanced above and below the geomagnetic equator (not perfectly aligned with the geographic equator) on the dayside due to the ionizing effects of solar ultraviolet radiation combined with the effects of high-altitude winds and the geomagnetic field. || ", "hits": 34 }, { "id": 4503, "url": "https://svs.gsfc.nasa.gov/4503/", "result_type": "Visualization", "release_date": "2016-10-27T14:00:00-04:00", "title": "Exploring the Ionosphere: The View from GOLD", "description": "Closeup view of Earth from the perspective of the GOLD instrument. This version interpolates the IRI model to a higher time cadence for a smoother animation. || IRIDaily.GOLDview_O+ion_O+ionSlice.clockSlate_CRTT.UHD3840.001002_print.jpg (1024x576) [50.7 KB] || IRIDaily.GOLDview_O+ion_O+ionSlice.IRIinterp.HD1080i_p30.mp4 (1920x1080) [56.7 MB] || IRI.interpolate (1920x1080) [0 Item(s)] || IRIDaily.GOLDview_O+ion_O+ionSlice.IRIinterp.HD1080i_p30.webm (1920x1080) [17.1 MB] || IRI.interpolate (3840x2160) [0 Item(s)] || IRIDaily.GOLDview_O+ion_O+ionSlice.IRIinterp_4503.key [57.9 MB] || IRIDaily.GOLDview_O+ion_O+ionSlice.IRIinterp_4503.pptx [57.6 MB] || IRIDaily.GOLDview_O+ion_O+ionSlice.IRIinterp_2160p30.mp4 (3840x2160) [200.2 MB] || ", "hits": 39 }, { "id": 12220, "url": "https://svs.gsfc.nasa.gov/12220/", "result_type": "Produced Video", "release_date": "2016-04-21T11:00:00-04:00", "title": "Earth's Ionosphere", "description": "See why the night sky is never completely dark. || c-1024.jpg (1024x576) [81.4 KB] || c-1280.jpg (1280x720) [102.7 KB] || c-1920.jpg (1920x1080) [162.3 KB] || c-1024_print.jpg (1024x576) [90.5 KB] || c-1024_searchweb.png (320x180) [49.3 KB] || c-1024_web.png (320x180) [49.3 KB] || c-1024_thm.png (80x40) [4.6 KB] || ", "hits": 195 }, { "id": 40271, "url": "https://svs.gsfc.nasa.gov/gallery/live-shots-gallery/", "result_type": "Gallery", "release_date": "2015-11-27T00:00:00-05:00", "title": "Live Shots Gallery Collection", "description": "Collection of live shot pages of b-roll and interviews!", "hits": 550 }, { "id": 4153, "url": "https://svs.gsfc.nasa.gov/4153/", "result_type": "Visualization", "release_date": "2014-03-25T01:00:00-04:00", "title": "GPM/GMI First Light", "description": "Eleven days after the Feb. 27 launch of the Global Precipitation Measurement (GPM) Core Observatory, the two instruments aboard took their first joint images of an interesting precipitation event. On March 10, the Core Observatory passed over an extra-tropical cyclone about 1055 miles (1700 kilometers) due east of Japan's Honshu Island. The storm formed from the collision of a cold front wrapping around a warm front, emerging over the ocean near Okinawa on March 8. It moved northeast over the ocean south of Japan, drawing cold air west-to-east over the land, a typical winter weather pattern that also brought heavy snow over Hokkaido, the northernmost of the four main islands. After the GPM images were taken, the storm continued to move eastward, slowly intensifying before weakening in the central North Pacific.This visualization shows data from the GPM Microwave Imager, which observes different types of precipitation with 13 channels. Scientists analyze that data and then use it to calculate the light to heavy rain rates and falling snow within the storm.For more information on this topic: GPM web siteOther multimedia items related to this story: GPM GMI First Light (#11508) GPM DPR First Light (#11509) || ", "hits": 24 }, { "id": 4076, "url": "https://svs.gsfc.nasa.gov/4076/", "result_type": "Visualization", "release_date": "2013-05-15T00:00:00-04:00", "title": "Landsat-8 Long Swath", "description": "Landsat-8 launched February 11th, 2013. This visualization shows one of the first full swaths of data taken on April 19th, 2013, only one week after Landsat-8 ascended to its final altitude of 438 miles (705 km). || ", "hits": 147 }, { "id": 4058, "url": "https://svs.gsfc.nasa.gov/4058/", "result_type": "Visualization", "release_date": "2013-03-27T00:00:00-04:00", "title": "Space Weather @ Mars: The CME of March 5, 2013", "description": "These images were produced from a space weather model known as ENLIL named after the Sumerian storm god. It shows the way a coronal mass ejection (CME) on March 5, 2013, was expected to travel. The view on the left is top down, while the one on the right shows Earth from the side.To protect their space assets from excessive radiation, NASA and other organizations research the fundamental processes behind space weather such as CMEs, integrating them into research models, which are run continuously at the Community-Coordinated Modeling Center (CCMC) at NASA Goddard.When CMEs occur on the sun, models are generated with the best event information available at the time and propagated forward to estimate regions in the solar system that might be affected. The models take about an hour or two to run. The CMEs themselves usually take one or two days to reach other planets or spacecraft.The March 5 CME moved towards Mars and the STEREO-B spacecraft (blue spacecraft icon). This allowed mission operators to take steps to protect STEREO-B as well as spacecraft operating around and on Mars. || ", "hits": 40 }, { "id": 10250, "url": "https://svs.gsfc.nasa.gov/10250/", "result_type": "Produced Video", "release_date": "2008-06-03T00:00:00-04:00", "title": "GLASTcast for iTunes", "description": "The GLAST mission launched on June 11, 2008 and has been returning remarkable and revolutionary discoveries ever since. Recently renamed to the Fermi Space Telescope, after Nobel Prize winner Enrico Fermi, the mission is expected to discover dozens of new pulsars within the first year alone. The telescope is also giving us new insights into gamma-ray bursts and the massive jets that erupt from distant galaxies. Stay tuned — the mission of NASA's Fermi telescope is just getting started. || ", "hits": 32 }, { "id": 40001, "url": "https://svs.gsfc.nasa.gov/gallery/the-galleries/", "result_type": "Gallery", "release_date": "2000-01-01T00:00:00-05:00", "title": "The Galleries", "description": "No description available.", "hits": 6758 }, { "id": 40056, "url": "https://svs.gsfc.nasa.gov/gallery/ionosphere/", "result_type": "Gallery", "release_date": "2000-01-01T00:00:00-05:00", "title": "Ionosphere", "description": "No description available.", "hits": 42 }, { "id": 689, "url": "https://svs.gsfc.nasa.gov/689/", "result_type": "Visualization", "release_date": "1999-07-14T12:00:00-04:00", "title": "TRACE: Viewing a Coronal Loop with a Diagram of the Earth for Scale.", "description": "Zooming into the sun to show an animation of the Bastille Day solar flare from TRACE imagery || a000689.00010_print.png (720x480) [443.9 KB] || TRACE_pre.jpg (320x240) [6.2 KB] || a000689_pre.jpg (320x242) [6.3 KB] || a000689.webmhd.webm (960x540) [3.6 MB] || a000689.dv (720x480) [54.9 MB] || a000689.mp4 (640x480) [4.6 MB] || TRACE.mov (320x240) [934.9 KB] || a000689.mpg (352x240) [3.0 MB] || ", "hits": 49 } ] }