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    "results": [
        {
            "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": 95
        },
        {
            "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": 99
        },
        {
            "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": 43
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        {
            "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": 22
        },
        {
            "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": 40
        },
        {
            "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": 485
        },
        {
            "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": 61
        },
        {
            "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": 28
        },
        {
            "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": 763
        },
        {
            "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": 67
        },
        {
            "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": 55
        },
        {
            "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": 373
        },
        {
            "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": 60
        },
        {
            "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": 87
        },
        {
            "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": 75
        },
        {
            "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": 35
        },
        {
            "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": 146
        },
        {
            "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": 82
        },
        {
            "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": 43
        },
        {
            "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": 56
        }
    ]
}