{
    "count": 5,
    "next": null,
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    "results": [
        {
            "id": 5643,
            "url": "https://svs.gsfc.nasa.gov/5643/",
            "result_type": "Visualization",
            "release_date": "2026-05-12T12:00:00-04:00",
            "title": "The Ring Current in Earth's Magnetosphere",
            "description": "The ring current is a dynamic, doughnut-shaped region around Earth where charged particles flow in opposite directions along magnetic field lines, creating electrical currents. During a solar storm, changes in the ring current can lead to charge buildup on satellites, increased satellite drag, and magnetic fluctuations and induced currents on the ground that can affect pipelines and power lines.",
            "hits": 978
        },
        {
            "id": 5622,
            "url": "https://svs.gsfc.nasa.gov/5622/",
            "result_type": "Visualization",
            "release_date": "2026-03-05T18:00:00-05:00",
            "title": "Artemis II: Sending Humans Beyond the Magnetosphere",
            "description": "Artemis II will be the first time in over 50 years that humans venture beyond Earth's protective magnetic shield, called the magnetosphere. This visualization captures the spacecraft's journey as the Orion spacecraft leaves the safety of the magnetosphere (shown here in green) and travels into open space, where it will encounter the solar wind streaming from the Sun.",
            "hits": 426
        },
        {
            "id": 5435,
            "url": "https://svs.gsfc.nasa.gov/5435/",
            "result_type": "Visualization",
            "release_date": "2024-12-12T12:00:00-05:00",
            "title": "Geomagnetic and Atmospheric Response to May 2024 Solar Storm",
            "description": "This visualization shows the Earth's magnetosphere being hit by a geomagnetic storm. The MAGE model simulates real events that happened throughout May 10-11, 2024.White orbit trails: All satellites orbiting Earth during the stormOrange orbits: Proposed orbits for six GDC spacecraftOrange-to-purple lines: Magnetic field lines around EarthBlue trails: Solar wind velocity tracersGreen clouds: Electric field current intensityCredit:NASA Scientific Visualization Studio and NASA DRIVE Science Center for Geospace Storms || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_print.jpg (1024x576) [191.2 KB] || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_searchweb.png (320x180) [102.0 KB] || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_web.png (320x180) [102.0 KB] || multiField_11-25-2024b_magnetosphere_pc_anim_satellites_4k.00450_thm.png (80x40) [6.4 KB] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_1080p30.mp4 (1920x1080) [253.6 MB] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_3x3Hyperwall (5760x3240) [2880 Item(s)] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_3x3Hyperwall_2160p30.mp4 (3840x2160) [773.4 MB] || multiField_12-30-2024b_magnetosphere_pc_anim_satellites_3x3Hyperwall_3240p30_h265.mp4 (5760x3240) [779.4 MB] || ",
            "hits": 435
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        {
            "id": 5214,
            "url": "https://svs.gsfc.nasa.gov/5214/",
            "result_type": "Visualization",
            "release_date": "2024-02-08T08:00:00-05:00",
            "title": "Geomagnetic Storm Causes Satellite Loss for Fulldome",
            "description": "In February 2022, a Coronal Mass Ejection led to 38 commercial satellites being lost. Solar plasma from a geomagnetic storm heated the atmosphere, causing denser gases to expand into the satellites’ orbit, which increased atmospheric drag on the satellites and caused them to de-orbit. Johns Hopkins APL-led Center for Geospace Storms (CGS) is building a Multiscale Atmosphere-Geospace Environment (MAGE) supercomputer model to predict space weather. The physics-based MAGE simulation reproduced the storm-time atmospheric density enhancement much better than empirical or standalone ionosphere-thermosphere models, emphasizing the need for fully-coupled whole-of-geospace models for predicting space weather events.This is 4k fulldome imagery intended for projection in a planetarium or other hemispherical dome theater. || ",
            "hits": 154
        },
        {
            "id": 5193,
            "url": "https://svs.gsfc.nasa.gov/5193/",
            "result_type": "Visualization",
            "release_date": "2023-12-11T09:00:00-05:00",
            "title": "Geomagnetic Storm Causes Satellite Loss",
            "description": "In February 2022, a Coronal Mass Ejection led to 38 commercial satellites being lost. Solar plasma from a geomagnetic storm heated the atmosphere, causing denser gases to expand into the satellites’ orbit, which increased atmospheric drag on the satellites and caused them to de-orbit. Johns Hopkins APL-led Center for Geospace Storms (CGS) is building a Multiscale Atmosphere-Geospace Environment (MAGE) supercomputer model to predict space weather. The physics-based MAGE simulation reproduced the storm-time atmospheric density enhancement much better than empirical or standalone ionosphere-thermosphere models, emphasizing the need for fully-coupled whole-of-geospace models for predicting space weather events. || ",
            "hits": 3139
        }
    ]
}