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    "results": [
        {
            "id": 14827,
            "url": "https://svs.gsfc.nasa.gov/14827/",
            "result_type": "Produced Video",
            "release_date": "2025-04-24T15:00:00-04:00",
            "title": "TRACERS Instrument Development & Testing at the University of Iowa",
            "description": "NASA’s Tandem Reconnection and Cusp Electrodynamics Reconnaissance Satellites, or TRACERS, is embarking on its integration and testing campaign, during which all of the instruments and components will be added to the spacecraft structure, tested to ensure they will survive the harsh environments of launch and space, and made ready to execute its mission. The TRACERS mission will help scientists understand an explosive process called magnetic reconnection and its effects in Earth’s atmosphere. Magnetic reconnection occurs when magnetic fields and particles from the Sun interact with Earth’s magnetic field. By understanding this process, scientists will be able to better understand and prepare for impacts of solar activity on Earth, such as auroras and disruptions to telecommunications.Below are clips of TRACERS’ instrument design, build, and testing at the University of Iowa in Iowa City, Iowa.Learn more about the mission: https://science.nasa.gov/mission/tracers/ || ",
            "hits": 53
        },
        {
            "id": 14667,
            "url": "https://svs.gsfc.nasa.gov/14667/",
            "result_type": "Produced Video",
            "release_date": "2024-08-22T14:00:00-04:00",
            "title": "ESCAPADE Instrument Build and Testing",
            "description": "The Escape and Plasma Acceleration and Dynamics Explorers, or ESCAPADE, will use two identical spacecraft to investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape.The first multi-spacecraft orbital science mission to the Red Planet, ESCAPADE’s twin orbiters will take simultaneous observations from different locations around Mars to reveal the planet’s real-time response to space weather and how the Martian magnetosphere changes over time.ESCAPADE will analyze how Mars’ magnetic field guides particle flows around the planet, how energy and momentum are transported from the solar wind through the magnetosphere, and what processes control the flow of energy and matter into and out of the Martian atmosphere. The data returned from the ESCAPADE spacecraft will provide new insight into the evolution of Mars’ climate, contributing to the body of research investigating how Mars began losing its atmosphere and water system.The ESCAPADE mission is managed by the Space Sciences Laboratory at the University of California, Berkeley, with key partners Rocket Lab, NASA's Goddard Space Flight Center, Embry-Riddle Aeronautical University, Advanced Space LLC, and Blue Origin. || ",
            "hits": 42
        },
        {
            "id": 14635,
            "url": "https://svs.gsfc.nasa.gov/14635/",
            "result_type": "Produced Video",
            "release_date": "2024-07-22T12:00:00-04:00",
            "title": "ESCAPADE Mission Spacecraft Beauty Passes",
            "description": "NASA’s Escape and Plasma Acceleration and Dynamics Explorers (ESCAPADE) mission will study the interaction between the solar wind and Martian atmosphere. Two identical spacecraft will orbit around the Red Planet to understand the structure, composition, variability, and dynamics of Mars’ unique hybrid magnetosphere, including its real-time response to space weather.The mission will leverage its unique dual viewpoint on the Mars environment to explore how the solar wind strips atmosphere away from Mars to better understand how its climate has changed over time — so much that Mars no longer supports liquid water on its surface. The pair will be the first coordinated multi-spacecraft orbital science mission to Mars.ESCAPADE is part of the NASA Small Innovative Missions for Planetary Exploration (SIMPLEx) program. The mission is managed by the University of California Berkeley’s Space Sciences Laboratory, with key partners Rocket Lab, NASA Goddard Space Flight Center, Embry-Riddle Aeronautical University, Advanced Space LLC, and Blue Origin. || ",
            "hits": 105
        },
        {
            "id": 13722,
            "url": "https://svs.gsfc.nasa.gov/13722/",
            "result_type": "Produced Video",
            "release_date": "2020-09-21T13:00:00-04:00",
            "title": "NASA Sees High Temperatures, Wildfires, and Annual Sea Ice Minimum Extent in Warming Arctic",
            "description": "Music: Curves Ahead by Donn Wilkerson [BMI] and Genetic Analyzer by Le Fat Club [SACEM]Complete transcript available. || Sea_Ice_Thumbnail.jpg (1920x1080) [550.9 KB] || Sea_Ice_Thumbnail_searchweb.png (320x180) [93.9 KB] || Sea_Ice_Thumbnail_thm.png (80x40) [9.2 KB] || Arctic_Sea_Ice_FINAL.mp4 (1920x1080) [741.6 MB] || Arctic_Sea_Ice_FINAL.webm (1920x1080) [41.5 MB] || ArcticSeaIce2020.en_US.srt [6.9 KB] || ArcticSeaIce2020.en_US.vtt [6.9 KB] || ",
            "hits": 34
        },
        {
            "id": 13072,
            "url": "https://svs.gsfc.nasa.gov/13072/",
            "result_type": "Produced Video",
            "release_date": "2018-09-19T12:00:00-04:00",
            "title": "Parker Solar Probe First Light Data",
            "description": "Just over a month into its mission, Parker Solar Probe has returned first-light data from each of its four instrument suites. These early observations – while not yet examples of the key science observations Parker Solar Probe will take closer to the Sun – show that each of the instruments is working well. The instruments work in tandem to measure the Sun's electric and magnetic fields, particles from the Sun and the solar wind, and capture images of the environment around the spacecraft. The mission’s first close approach to the Sun will be in November 2018, but even now, the instruments are able to gather measurements of what’s happening in the solar wind closer to Earth. || ",
            "hits": 132
        },
        {
            "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": 65
        },
        {
            "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": 95
        },
        {
            "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": 63
        },
        {
            "id": 40122,
            "url": "https://svs.gsfc.nasa.gov/gallery/mars/",
            "result_type": "Gallery",
            "release_date": "2012-06-28T00:00:00-04:00",
            "title": "Mars Missions and Science",
            "description": "This multimedia gallery assembles and organizes Mars content on the Scientific Visualization Studio website. Highlights of NASA Goddard Space Flight Center’s animations, visualizations, videos, images and graphics relating to Mars science and missions can be found here.",
            "hits": 243
        },
        {
            "id": 90,
            "url": "https://svs.gsfc.nasa.gov/90/",
            "result_type": "Visualization",
            "release_date": "1995-11-07T12:00:00-05:00",
            "title": "SAMPEX - Yohkoh: Solar Modification of Relativistic Electrons in the Earth's Radiation Belts",
            "description": "The Solar Anomalous and Magnetospheric Particle Explorer, SAMPEX, measures fluxes of energetic particles from the sun, the Earth's magnetosphere, and cosmic ray sources over a broad range of energies. The four instruments aboard SAMPEX are the Low-Energy Ion Analyzer (LEICA), The Heavy Ion Large Telescope (HILT), The Mass Spectrometer Telescope (MAST), and the Proton-Electron Telescope (PET). The Soft X-ray Telescope on the Yohkoh satellite takes daily full-disk soft X-ray images of the Sun. Comparing data sets from the two satellites allows correlation of electron fluxes in the Earth's radiation belts with solar output. || ",
            "hits": 42
        },
        {
            "id": 89,
            "url": "https://svs.gsfc.nasa.gov/89/",
            "result_type": "Visualization",
            "release_date": "1995-01-01T12:00:00-05:00",
            "title": "SAMPEX - A Synoptic View of Earth's Electron Radiation Belts: North Pole Energetic Fluxes from HILT",
            "description": "The Solar Anomalous and Magnetospheric Particle Explorer, SAMPEX, measures fluxes of energetic particles from the sun, the Earth's magnetosphere, and cosmic ray sources over a broad range of energies. The four instruments aboard SAMPEX are the Low-Energy Ion Analyzer (LEICA), The Heavy Ion Large Telescope (HILT), The Mass Spectrometer Telescope (MAST), and the Proton-Electron Telescope (PET). || ",
            "hits": 35
        },
        {
            "id": 1385,
            "url": "https://svs.gsfc.nasa.gov/1385/",
            "result_type": "Visualization",
            "release_date": "1995-01-01T12:00:00-05:00",
            "title": "SAMPEX - A Synoptic View of Earth's Electron Radiation Belts: South Pole Energetic Fluxes from HILT",
            "description": "The Solar Anomalous and Magnetospheric Particle Explorer, SAMPEX, measures fluxes of energetic particles from the sun, the Earth's magnetosphere, and cosmic ray sources over a broad range of energies.  The four instruments aboard SAMPEX are the Low-Energy Ion Analyzer (LEICA), The Heavy Ion Large Telescope (HILT), The Mass Spectrometer Telescope (MAST), and the Proton-Electron Telescope (PET). || ",
            "hits": 12
        },
        {
            "id": 1386,
            "url": "https://svs.gsfc.nasa.gov/1386/",
            "result_type": "Visualization",
            "release_date": "1995-01-01T12:00:00-05:00",
            "title": "SAMPEX - A Synoptic View of Earth's Electron Radiation Belts: North Pole Energetic Fluxes from PET",
            "description": "The Solar Anomalous and Magnetospheric Particle Explorer, SAMPEX, measures fluxes of energetic particles from the sun, the Earth's magnetosphere, and cosmic ray sources over a broad range of energies.  The four instruments aboard SAMPEX are the Low-Energy Ion Analyzer (LEICA), The Heavy Ion Large Telescope (HILT), The Mass Spectrometer Telescope (MAST), and the Proton-Electron Telescope (PET). || ",
            "hits": 11
        },
        {
            "id": 1387,
            "url": "https://svs.gsfc.nasa.gov/1387/",
            "result_type": "Visualization",
            "release_date": "1995-01-01T12:00:00-05:00",
            "title": "SAMPEX - A Synoptic View of Earth's Electron Radiation Belts: South Pole Energetic Fluxes from PET",
            "description": "The Solar Anomalous and Magnetospheric Particle Explorer, SAMPEX, measures fluxes of energetic particles from the sun, the Earth's magnetosphere, and cosmic ray sources over a broad range of energies.  The four instruments aboard SAMPEX are the Low-Energy Ion Analyzer (LEICA), The Heavy Ion Large Telescope (HILT), The Mass Spectrometer Telescope (MAST), and the Proton-Electron Telescope (PET). || ",
            "hits": 12
        }
    ]
}