{
    "count": 6,
    "next": null,
    "previous": null,
    "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": 91
        },
        {
            "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": 35
        },
        {
            "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": 359
        },
        {
            "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": 176
        },
        {
            "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": 68
        },
        {
            "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": 58
        }
    ]
}