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    "results": [
        {
            "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 || ",
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        },
        {
            "id": 13688,
            "url": "https://svs.gsfc.nasa.gov/13688/",
            "result_type": "Produced Video",
            "release_date": "2020-08-17T11:45:00-04:00",
            "title": "NASA Explores Earth's Magnetic \"Dent\"",
            "description": "Music: \"Now We Wait\" by Kamal David Kamruddin [PRS]This video can be freely shared and downloaded. While the video in its entirety can be shared without permission, some individual imagery provided by pond5.com and Artbeats is obtained through permission and may not be excised or remixed in other products. Specific details on stock footage may be found here. For more information on NASA’s media guidelines, visit https://www.nasa.gov/multimedia/guidelines/index.html.Complete transcript available. || South_Atlantic_Anomaly_Still_2.jpg (1920x1080) [346.0 KB] || South_Atlantic_Anomaly_Still_2_print.jpg (1024x576) [139.2 KB] || South_Atlantic_Anomaly_Still_2_searchweb.png (320x180) [43.0 KB] || South_Atlantic_Anomaly_Still_2_web.png (320x180) [43.0 KB] || South_Atlantic_Anomaly_Still_2_thm.png (80x40) [4.8 KB] || 13688_South_Atlantic_Anomaly_Fine.mov (1920x1080) [2.6 GB] || 13688_South_Atlantic_Anomaly_Fine.webm (960x540) [65.7 MB] || 13688_South_Atlantic_Anomaly_Fine.mp4 (1920x1080) [292.9 MB] || 13688_South_Atlantic_Anomaly_Fine_lowres.mp4 (1280x720) [52.3 MB] || SAA.en_US.srt [3.5 KB] || SAA.en_US.vtt [3.5 KB] || ",
            "hits": 167
        },
        {
            "id": 4840,
            "url": "https://svs.gsfc.nasa.gov/4840/",
            "result_type": "Visualization",
            "release_date": "2020-08-17T11:00:00-04:00",
            "title": "South Atlantic Anomaly: 2015 through 2025",
            "description": "South Atlantic Anomaly from 2015 through 2025 showing the geomagnetic intensity at the Earth's surface and the core-mantle boundary.  There are versions that include the dates and colorbars and versions without the date and colorbat.This video is also available on our YouTube channel. || saa_intensity_comp2160_p60.4898_print.jpg (1024x576) [58.0 KB] || saa_intensity_comp2160_p60.4898_print_searchweb.png (320x180) [49.9 KB] || saa_intensity_comp2160_p60.4898_print_thm.png (80x40) [3.8 KB] || saa_intensity_comp_1080p30.mp4 (1920x1080) [31.9 MB] || saa_intensity_comp_1080p60.mp4 (1920x1080) [34.4 MB] || saa_intensity_dataOnly_1080_p30.mp4 (1920x1080) [29.3 MB] || saa_intensity_dataOnly_1080_p60.mp4 (1920x1080) [31.3 MB] || saa_intensity_dataOnly_1080_p30.webm (1920x1080) [9.1 MB] || dataOnly (1920x1080) [0 Item(s)] || saa_intensity_comp2160_p30.mp4 (3840x2160) [86.1 MB] || saa_intensity_comp2160_p60.mp4 (3840x2160) [93.1 MB] || comp (3840x2160) [0 Item(s)] || captions_silent.29860.en_US.srt [43 bytes] || saa_intensity_dataOnly_1080_p30.mp4.hwshow [197 bytes] || ",
            "hits": 1555
        },
        {
            "id": 4670,
            "url": "https://svs.gsfc.nasa.gov/4670/",
            "result_type": "Visualization",
            "release_date": "2018-08-01T09:00:00-04:00",
            "title": "Geothermal Heat Flux Reveals the Iceland Hotspot Track underneath Greenland",
            "description": "This visualization shows the Greenland geothermal heat flux map, the track of the Iceland hotspot through Greenland, and the plate tectonic motion of Greenland over the hotspot during the past 100 million years.This video is also on the NASA YouTube channel. || hotspot.0240_print.jpg (1024x576) [157.4 KB] || hotspot.0240_searchweb.png (320x180) [100.2 KB] || hotspot.0240_thm.png (80x40) [7.9 KB] || hotspot_1080p30.mp4 (1920x1080) [17.1 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || hotspot_720p30.mp4 (1280x720) [8.7 MB] || hotspot_720p30.webm (1280x720) [3.0 MB] || hotspot_360p30.mp4 (640x360) [3.4 MB] || hotspot_1080p30.mp4.hwshow [181 bytes] || ",
            "hits": 172
        },
        {
            "id": 13025,
            "url": "https://svs.gsfc.nasa.gov/13025/",
            "result_type": "Produced Video",
            "release_date": "2018-08-01T09:00:00-04:00",
            "title": "NASA Scientist Reveals Greenland's Geologic Past",
            "description": "A new map of Greenland's geothermal heat flux is helping to reveal the path of the North American tectonic plate over geologic time. Complete transcript available.Watch this video on the NASA Goddard YouTube channel.Music Provided by Killer Tracks: \"Valfri\" by James Alexander Dorman || FACEBOOK_720_13025_Greenland_Hotspot_MASTER_facebook_720.mp4 (1280x720) [173.9 MB] || Greenland_Tectonic_Preview_print.jpg (1024x576) [383.0 KB] || Greenland_Tectonic_Preview.jpg (3840x2160) [3.0 MB] || Greenland_Tectonic_Preview_searchweb.png (320x180) [136.6 KB] || Greenland_Tectonic_Preview_thm.png (80x40) [8.8 KB] || TWITTER_720_13025_Greenland_Hotspot_MASTER_twitter_720.mp4 (1280x720) [28.6 MB] || 13025_Greenland_Hotspot_MASTER.webm (960x540) [53.0 MB] || YOUTUBE_1080_13025_Greenland_Hotspot_MASTER_youtube_1080.mp4 (1920x1080) [228.2 MB] || YOUTUBE_1080_13025_Greenland_Hotspot_MASTER_youtube_1080_Output.en_US.srt [2.5 KB] || YOUTUBE_1080_13025_Greenland_Hotspot_MASTER_youtube_1080_Output.en_US.vtt [2.5 KB] || YOUTUBE_4K_13025_Greenland_Hotspot_MASTER_youtube_4k.mp4 (3840x2160) [543.3 MB] || 13025_Greenland_Hotspot_MASTER_youtube_hq.mov (3840x2160) [1.3 GB] || 13025_Greenland_Hotspot_MASTER.mov (3840x2160) [6.3 GB] || ",
            "hits": 57
        },
        {
            "id": 12456,
            "url": "https://svs.gsfc.nasa.gov/12456/",
            "result_type": "Produced Video",
            "release_date": "2016-12-12T18:45:00-05:00",
            "title": "Tracking Ocean Heat With Magnetic Fields",
            "description": "As Earth warms, much of the extra heat is stored in the planet’s ocean – but monitoring the magnitude of that heat content is a difficult task. A surprising feature of the tides could help, however. Scientists at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, are developing a new way to use satellite observations of magnetic fields to measure heat stored in the ocean.Music: War Torn by Brad Smith [BMI] Complete transcript available.Watch this video on the NASA Goddard YouTube channel. || 12456-ocean-heat-AGU-web.jpg (1920x1080) [354.1 KB] || 12456-ocean-heat-AGU-web_searchweb.png (320x180) [122.0 KB] || 12456-ocean-heat-AGU-web_thm.png (80x40) [7.7 KB] || 12456-ocean-heat-APR_VX-680579_large.mp4 (1920x1080) [59.1 MB] || 12456-ocean-heat-APR_VX-680579_appletv.m4v (1280x720) [30.6 MB] || 12456-ocean-heat-AGU-720p.mp4 (1280x720) [59.5 MB] || 12456-ocean-heat-AGU.mp4 (1920x1080) [59.9 MB] || 12456-ocean-heat-APR_VX-680579.webm (960x540) [23.6 MB] || 12456-ocean-heat-APR_VX-680579_appletv_subtitles.m4v (1280x720) [30.7 MB] || 12456-ocean-heat-captions.en_US.srt [891 bytes] || 12456-ocean-heat-captions.en_US.vtt [904 bytes] || 12456-ocean-heat-APR_VX-680579_ipod_sm.mp4 (320x240) [10.9 MB] || 12456-ocean-heat-APR_VX-680579_prores.mov (1280x720) [791.2 MB] || 12456-ocean-heat-APR_VX-680579_youtube_hq.mov (1920x1080) [212.0 MB] || 12456-ocean-heat-APR_VX-680579.mpeg (1280x720) [196.6 MB] || ",
            "hits": 45
        },
        {
            "id": 12450,
            "url": "https://svs.gsfc.nasa.gov/12450/",
            "result_type": "Produced Video",
            "release_date": "2016-12-12T18:30:00-05:00",
            "title": "Ocean Tides and Magnetic Fields",
            "description": "Seawater is an electrical conductor, and therefore interacts with the magnetic field.  As the tides cycle around the ocean basins, the ocean water essentially tries to pull the geomagnetic field lines along.Because the salty water is a good, but not great, conductor, the interaction is relatively weak.  Scientists at NASA Goddard Space Flight Center are developing improved methods to isolate the signal from ocean tides and use that information to determine the heat content of the ocean.Music: \"Memory Of A Lifetime\" by J Ehrlich [SESAC], Jean-Christophe Beck [BMI]Complete transcript available.Watch this video on the NASA Goddard YouTube channel. || 12450-Tidal-Magnetic-Animation-APR_large.00545_print.jpg (1024x576) [189.1 KB] || 12450-Tidal-Magnetic-Animation-APR_large.00545_searchweb.png (320x180) [93.6 KB] || 12450-Tidal-Magnetic-Animation-APR_large.00545_thm.png (80x40) [5.8 KB] || 12450-Tidal-Magnetic-Animation-APR.webm (960x540) [26.5 MB] || 12450-Tidal-Magnetic-Animation-APR_prores.mov (1280x720) [989.0 MB] || 12450-Tidal-Magnetic-Animation-APR_large.mp4 (1920x1080) [66.1 MB] || 12450-Tidal-Magnetic-Animation-APR_youtube_hq.mov (1920x1080) [1.0 GB] || 12450-Tidal-Magnetic-Animation-APR_appletv.m4v (1280x720) [32.1 MB] || 12450-Tidal-Magnetic-Animation-APR_appletv_subtitles.m4v (1280x720) [32.2 MB] || 1920x1080_16x9_30p (1920x1080) [128.0 KB] || 12450-Tidal-Magnetic-Animation.en_US.srt [1.4 KB] || 12450-Tidal-Magnetic-Animation.en_US.vtt [1.4 KB] || 12450-Tidal-Magnetic-Animation-APR_ipod_sm.mp4 (320x240) [11.5 MB] || ",
            "hits": 306
        },
        {
            "id": 4480,
            "url": "https://svs.gsfc.nasa.gov/4480/",
            "result_type": "Visualization",
            "release_date": "2016-08-15T14:00:00-04:00",
            "title": "Prompt Electron Acceleration in the Radiation Belts",
            "description": "Electrons gyrating along the lines of Earth's magnetic field make another orbit around Earth and strike the Van Allen Probe A AGAIN! || PromptAccel_EventCloseup_SlowOblique.slate_RigRHS.HD1080i.0540_print.jpg (1024x576) [139.2 KB] || PromptAccel_EventCloseup_SlowOblique.slate_RigRHS.HD1080i.0540_searchweb.png (320x180) [90.9 KB] || PromptAccel_EventCloseup_SlowOblique.slate_RigRHS.HD1080i.0540_thm.png (80x40) [6.0 KB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || PromptAccel.HD1080i_p30.mp4 (1920x1080) [48.5 MB] || PromptAccel.HD1080i_p30.webm (1920x1080) [3.1 MB] || PromptAccel_EventCloseup_SlowOblique.HD1080i_720p30.mp4 (1280x720) [24.1 MB] || 3840x2160_16x9_30p (3840x2160) [0 Item(s)] || PromptAccel_EventCloseup_SlowOblique_2160p30.mp4 (3840x2160) [141.9 MB] || PromptAccel.HD1080i_p30.mp4.hwshow [189 bytes] || ",
            "hits": 278
        },
        {
            "id": 3822,
            "url": "https://svs.gsfc.nasa.gov/3822/",
            "result_type": "Visualization",
            "release_date": "2011-02-14T00:00:00-05:00",
            "title": "Stereoscopic Magnetic Field Lines",
            "description": "This stereoscopic visualization shows a simple model of the Earth's magnetic field. The magnetic field partially shields the Earth from harmful charged particles emanating from the sun. The field is stretched back away from Sun by solar particle and radiation pressures.The geomagnetic field is generated (and regenerated) as the conducting fluid of the Earth's mantle and core, driven by convection of heat from deeper in the interior, induces an electromotive force (EMF) with the existing magnetic field.  This process is very similar to the way an electric generator generates a voltage.  That voltage then drives an induced current in the conducting fluid, which also produces a magnetic field.  This feedback mechanism helps maintain the field, continuously converting the thermal energy in the Earth into magnetic field energy.The magnetic field line data used in this visualization is from a simplified static model. More complex models deform the magnetic field over time as the Earth rotates and experiences solar pressures. Many of the field lines (particulary near the back, away from the Sun) should eventually connect (north and south poles), but the 3d model used in this visualization does not extend far enough to see this.The day/night terminator is aligned with the Sun and is therefore aligned with the magnetic field too. This visualization is based on a previous monoscopic visualizaton that included magnetic field line data. || ",
            "hits": 243
        },
        {
            "id": 3605,
            "url": "https://svs.gsfc.nasa.gov/3605/",
            "result_type": "Visualization",
            "release_date": "2009-07-06T00:00:00-04:00",
            "title": "Magnetospheric Multiscale Mission (MMS) Dayside Orbit Animation for the Preliminary Design Review (PDR)",
            "description": "This visualization uses simulated ephemerides to show the proposed orbits of the Magnetospheric Multiscale Mission (MMS) during the \"dayside magnetosheath/magnetopause\" orbit phase. The movie initially shows the general orientation of the orbit with respect to the Earth, Moon, and Sun. It then zooms in to \"ride\" along with the spacecraft. We then zoom in even closer to show that there are actually four spacecraft flying in a tetrahedral formation. Finally, we see how the 4 spacecraft skim the magnetosheath such that, occasionally, some of the spacecraft are inside (e.g., MMS #1) and some are outside (e.g., MMS #2, #3, and #4) of the magnetosheath boundary.This visualization was created in support of the MMS Preliminary Design Review (PDR) which was held May 4 - 7, 2009. || ",
            "hits": 37
        },
        {
            "id": 3606,
            "url": "https://svs.gsfc.nasa.gov/3606/",
            "result_type": "Visualization",
            "release_date": "2009-07-06T00:00:00-04:00",
            "title": "Magnetospheric Multiscale Mission (MMS) Nightside Orbit Animation for the Preliminary Design Review (PDR)",
            "description": "This visualization uses simulated ephemerides to show the proposed orbits of the Magnetospheric Multiscale Mission (MMS) during the \"nightside\" orbit phase. The movie initially shows the general orientation of the orbit with respect to the Earth, Moon, and Sun. It then moves in towards the Earth revealing Earth's magnetic field. The camera then moves down towards the dark side of the Earth showing how MMS will fly through the tail of the magnetosphereThis visualization was created in support of the MMS Preliminary Design Review (PDR) which was held May 4th through May 7th of 2009. || ",
            "hits": 33
        }
    ]
}