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    "results": [
        {
            "id": 14628,
            "url": "https://svs.gsfc.nasa.gov/14628/",
            "result_type": "Produced Video",
            "release_date": "2024-08-28T11:30:00-04:00",
            "title": "Discovering Earth’s Third Global Energy Field",
            "description": "High above the Earth’s North and South Poles, a steady stream of particles escapes from our atmosphere into space. Scientists call this mysterious outflow the “polar wind,” and for almost 60 years, spacecraft have been flying through it as scientists have theorized about its cause. The leading theory was that a planet-wide electric field was drawing those particles up into space. But this so-called ambipolar electric field, if it exists, is so weak that all attempts to measure it have failed – until now.In 2022, scientists traveled to Svalbard, a small archipelago in Norway, to launch a rocket in an attempt to measure Earth’s ambipolar electric field for the first time. This was NASA’s Endurance rocketship mission, and this is its story.To learn more, visit: https://science.nasa.gov/science-research/heliophysics/nasa-discovers-long-sought-global-electric-field-on-earth/ || ",
            "hits": 360
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        {
            "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": 78
        },
        {
            "id": 4824,
            "url": "https://svs.gsfc.nasa.gov/4824/",
            "result_type": "Visualization",
            "release_date": "2020-05-25T00:00:00-04:00",
            "title": "MAVEN Observes Solar Particle Velocities and the Induced Magnetic Field",
            "description": "MAVEN orbits Mars and measures solar particle velocities and variations in the solar wind’s magnetic field. || maven_vels_magField.03000_print.jpg (1024x576) [92.5 KB] || maven_vels_magField.03000_searchweb.png (320x180) [63.5 KB] || maven_vels_magField.03000_thm.png (80x40) [4.2 KB] || maven_vels_magField_1080p30.mp4 (1920x1080) [83.1 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || maven_vels_magField_1080p30.webm (1920x1080) [19.0 MB] || 4824_MAVEN_Solar_Wind_Data_1080_30p.mov (1920x1080) [2.6 GB] || maven_vels_magField_1080p30.mp4.hwshow [193 bytes] || ",
            "hits": 115
        },
        {
            "id": 4649,
            "url": "https://svs.gsfc.nasa.gov/4649/",
            "result_type": "Visualization",
            "release_date": "2018-05-29T10:00:00-04:00",
            "title": "Plasma Zoo: Gyroresonant Scattering",
            "description": "In a background magnetic field, represented by the cyan arrows, two electrons are propagating to the right, executing identical gyromotion.  A circularly polarized electromagnetic wave approaches the upper electron from the left. || GyroresonanceV3_RideAlong_inertial.HD1080i.0150_print.jpg (1024x576) [85.3 KB] || GyroresonanceV3_RideAlong_inertial.HD1080i.0150_searchweb.png (320x180) [55.9 KB] || GyroresonanceV3_RideAlong_inertial.HD1080i.0150_thm.png (80x40) [4.3 KB] || RideAlong (1920x1080) [0 Item(s)] || GyroresonanceV3_RideAlong.HD1080i_p30.mp4 (1920x1080) [17.2 MB] || GyroresonanceV3_RideAlong.HD1080i_p30.webm (1920x1080) [2.3 MB] || GyroresonanceV3_RideAlong_inertial.HD1080i.0150.tif (1920x1080) [2.4 MB] || RideAlong (3840x2160) [0 Item(s)] || GyroresonanceV3_RideAlong.UHD3840_2160p30.mp4 (3840x2160) [49.4 MB] || GyroresonanceV3_RideAlong.HD1080i_p30.mp4.hwshow [203 bytes] || ",
            "hits": 81
        },
        {
            "id": 4568,
            "url": "https://svs.gsfc.nasa.gov/4568/",
            "result_type": "Visualization",
            "release_date": "2017-05-18T10:00:00-04:00",
            "title": "Exploring Reconnection - Guide Field Off",
            "description": "This visualization shows an oblique view of the reconnection region.  Magnetic field direction is represented by the cyan lines.  The color trail represents an electron moving in the field.  Color of the particle trail represents a dimensionless speed of the particle, with blue for slow and red for fast. || GuideFieldOff_oblique_inertial.HD1080i.0300_print.jpg (1024x576) [118.2 KB] || GuideFieldOff_oblique_inertial.HD1080i.0300_searchweb.png (320x180) [70.8 KB] || GuideFieldOff_oblique_inertial.HD1080i.0300_thm.png (80x40) [4.4 KB] || GuideFieldOff_oblique (1920x1080) [0 Item(s)] || GuideFieldOff_oblique_inertial.HD1080i_p30.mp4 (1920x1080) [6.3 MB] || GuideFieldOff_oblique_inertial.HD1080i_p30.webm (1920x1080) [776.5 KB] || GuideFieldOff_oblique_inertial.HD1080i_p30.mp4.hwshow [208 bytes] || ",
            "hits": 85
        },
        {
            "id": 4569,
            "url": "https://svs.gsfc.nasa.gov/4569/",
            "result_type": "Visualization",
            "release_date": "2017-05-18T10:00:00-04:00",
            "title": "Exploring Reconnection - Guide Field On",
            "description": "This visualization shows an oblique view of the reconnection region. Magnetic field direction is represented by the cyan lines. The color trail represents an electron moving in the field. Color of the particle trail represents a dimensionless speed of the particle, with blue for slow and red for fast. || GuideFieldOn_oblique_inertial.HD1080i.0300_print.jpg (1024x576) [129.7 KB] || GuideFieldOn_oblique_inertial.HD1080i.0300_searchweb.png (320x180) [76.2 KB] || GuideFieldOn_oblique_inertial.HD1080i.0300_thm.png (80x40) [4.6 KB] || GuideFieldOn_oblique (1920x1080) [0 Item(s)] || GuideFieldOn_oblique.HD1080i_p30.mp4 (1920x1080) [6.5 MB] || GuideFieldOn_oblique.HD1080i_p30.webm (1920x1080) [761.3 KB] || GuideFieldOn_oblique.HD1080i_p30.mp4.hwshow [198 bytes] || ",
            "hits": 281
        },
        {
            "id": 4560,
            "url": "https://svs.gsfc.nasa.gov/4560/",
            "result_type": "Visualization",
            "release_date": "2017-03-31T09:00:00-04:00",
            "title": "Alfvén Waves - Basic",
            "description": "Alfven waves represented by undulation in the magnetic field vector. || AlfvenWaveBasic_staticXwide_inertial.HD1080i.0300_print.jpg (1024x576) [158.5 KB] || AlfvenWaveBasic_staticXwide_inertial.HD1080i.0300_thm.png (80x40) [4.6 KB] || AlfvenWaveBasic_staticXwide_inertial.HD1080i.0300_web.png (320x180) [71.9 KB] || WavesOnly (1920x1080) [128.0 KB] || AlfvenWaveBasic_staticXwide.HD1080i_p30.mp4 (1920x1080) [34.0 MB] || AlfvenWaveBasic_staticXwide.HD1080i_p30.webm (1920x1080) [4.9 MB] || ",
            "hits": 456
        },
        {
            "id": 4561,
            "url": "https://svs.gsfc.nasa.gov/4561/",
            "result_type": "Visualization",
            "release_date": "2017-03-31T09:00:00-04:00",
            "title": "Alfvén Waves - Kinetic",
            "description": "Kinetic Alfven waves represented by undulation in the magnetic field vector. || AlfvenWaveKinetic_staticXwide_inertial.HD1080i.0300_print.jpg (1024x576) [155.7 KB] || WavesOnly (1920x1080) [128.0 KB] || AlfvenWaveKinetic_staticXwide.HD1080i_p30.mp4 (1920x1080) [37.9 MB] || AlfvenWaveKinetic_staticXwide.HD1080i_p30.webm (1920x1080) [4.9 MB] || ",
            "hits": 126
        },
        {
            "id": 4261,
            "url": "https://svs.gsfc.nasa.gov/4261/",
            "result_type": "Visualization",
            "release_date": "2015-02-02T00:00:00-05:00",
            "title": "Plasma Zoo: Gyromotion in Two Dimensions",
            "description": "Visualization from two camera positions of simple 2-dimensional gyro-motion of charged particles in a magnetic field. || GyromotionPlane_inertial.HD1080i.0600_print.jpg (1024x576) [120.0 KB] || GyromotionPlane_inertial.HD1080i.0600_searchweb.png (320x180) [77.2 KB] || GyromotionPlane_inertial.HD1080i.0600_thm.png (80x40) [5.3 KB] || GyromotionPlane_inertial.HD1080i.0600_web.png (320x180) [77.2 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || GyromotionPlane.HD1080.webm (1920x1080) [3.6 MB] || GyromotionPlane_inertial_1080.mp4 (1920x1080) [21.6 MB] || GyromotionPlane.HD1080.mov (1920x1080) [117.5 MB] || ",
            "hits": 77
        },
        {
            "id": 4262,
            "url": "https://svs.gsfc.nasa.gov/4262/",
            "result_type": "Visualization",
            "release_date": "2015-02-02T00:00:00-05:00",
            "title": "Plasma Zoo: Gyromotion in Three Dimensions",
            "description": "Visualization from two camera positions of simple 3-dimensional gyro-motion of charged particles in a magnetic field. || GyromotionZ_inertial.HD1080i.0600_print.jpg (1024x576) [120.9 KB] || GyromotionZ_inertial.HD1080i.0600_searchweb.png (320x180) [78.1 KB] || GyromotionZ_inertial.HD1080i.0600_thm.png (80x40) [5.4 KB] || GyromotionZ_inertial.HD1080i.0600_web.png (320x180) [78.1 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || GyromotionZ.HD1080.webm (1920x1080) [3.6 MB] || GyromotionZ_inertial_1080.mp4 (1920x1080) [22.1 MB] || GyromotionZ.HD1080.mov (1920x1080) [118.8 MB] || ",
            "hits": 130
        },
        {
            "id": 4263,
            "url": "https://svs.gsfc.nasa.gov/4263/",
            "result_type": "Visualization",
            "release_date": "2015-02-02T00:00:00-05:00",
            "title": "Plasma Zoo: Particle Drift in a Magnetic Gradient",
            "description": "Visualization from two camera positions of simple gyro-motion of charged particles in a changing magnetic field. || BGradient_inertial.HD1080i.0600_print.jpg (1024x576) [124.3 KB] || BGradient_inertial.HD1080i.0600_searchweb.png (320x180) [81.3 KB] || BGradient_inertial.HD1080i.0600_thm.png (80x40) [5.6 KB] || BGradient_inertial.HD1080i.0600_web.png (320x180) [81.3 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || BGradient.HD1080.webm (1920x1080) [3.7 MB] || BGradient_inertial_1080.mp4 (1920x1080) [22.2 MB] || BGradient.HD1080.mov (1920x1080) [121.1 MB] || ",
            "hits": 178
        },
        {
            "id": 4264,
            "url": "https://svs.gsfc.nasa.gov/4264/",
            "result_type": "Visualization",
            "release_date": "2015-02-02T00:00:00-05:00",
            "title": "Plasma Zoo: Field-Aligned Current (Birkeland Current)",
            "description": "Visualization from two camera positions of gyro-motion of charged particles in parallel electric and magnetic fields. || EBParallel_inertial.HD1080i.0600_print.jpg (1024x576) [123.4 KB] || EBParallel_inertial.HD1080i.0600_searchweb.png (320x180) [80.8 KB] || EBParallel_inertial.HD1080i.0600_web.png (320x180) [80.8 KB] || EBParallel_inertial.HD1080i.0600_thm.png (80x40) [5.6 KB] || EBParallel.cam1 (1920x1080) [0 Item(s)] || EBParallel.cam1.HD1080.webm (1920x1080) [3.6 MB] || EBParallel_cam1_HD1080.mp4 (1920x1080) [22.3 MB] || EBParallel.cam1.HD1080.mov (1920x1080) [120.0 MB] || ",
            "hits": 226
        },
        {
            "id": 4265,
            "url": "https://svs.gsfc.nasa.gov/4265/",
            "result_type": "Visualization",
            "release_date": "2015-02-02T00:00:00-05:00",
            "title": "Plasma Zoo: E-cross-B Drift",
            "description": "Visualization from two camera positions of gyro-motion of charged particles in perpendicular electric and magnetic fields. || EBvOrthogonal_inertial.HD1080i.0600_print.jpg (1024x576) [123.3 KB] || EBvOrthogonal_inertial.HD1080i.0600_searchweb.png (320x180) [79.0 KB] || EBvOrthogonal_inertial.HD1080i.0600_thm.png (80x40) [5.5 KB] || EBvOrthogonal_inertial.HD1080i.0600_web.png (320x180) [79.0 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || EBvOrthogonal.HD1080.webm (1920x1080) [3.6 MB] || EBvOrthogonal_inertial_1080.mp4 (1920x1080) [22.2 MB] || EBvOrthogonal.HD1080.mov (1920x1080) [120.0 MB] || ",
            "hits": 338
        },
        {
            "id": 11498,
            "url": "https://svs.gsfc.nasa.gov/11498/",
            "result_type": "Produced Video",
            "release_date": "2014-03-05T09:00:00-05:00",
            "title": "MAVEN Particles & Fields Package",
            "description": "To planetary scientists, the Martian atmosphere presents an intriguing mystery: today it's a thin, cold wisp of carbon dioxide with just one percent the pressure of Earth's atmosphere, but long ago it was thick and warm enough to support lakes and rivers on the Martian surface. How did Mars lose so much of its early atmosphere? Scientists think that the solar wind may be responsible, and NASA's Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft is designed to find out. The instruments of MAVEN's Particles & Fields package will study the interaction of the solar wind with Mars's upper atmosphere, helping scientists to better understand how Mars became the freeze-dried planet that we see today. || ",
            "hits": 126
        }
    ]
}