{
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    "results": [
        {
            "id": 4241,
            "url": "https://svs.gsfc.nasa.gov/4241/",
            "result_type": "Visualization",
            "release_date": "2014-11-26T13:00:00-05:00",
            "title": "Radiation Belts & Plasmapause",
            "description": "Visualization of the radiation belts with confined charged particles (blue & yellow) and plasmapause boundary (blue-green surface) || Earth_BeltsPlasmapauseParticles_Oblique.noslate_GSEmove.HD1080i.0400_print.jpg (1024x576) [136.6 KB] || Earth_BeltsPlasmapauseParticles_Oblique.noslate_GSEmove.HD1080i.0400_web.png (320x180) [96.2 KB] || Earth_BeltsPlasmapauseParticles_Oblique.noslate_GSEmove.HD1080i.0400_searchweb.png (320x180) [96.2 KB] || Earth_BeltsPlasmapauseParticles_Oblique.noslate_GSEmove.HD1080i.0400_thm.png (80x40) [6.9 KB] || BeltsPlasmapauseParticles_HD1080.mov (1920x1080) [28.3 MB] || Earth_BeltsPlasmapauseParticles_Oblique_HD1080.mp4 (1920x1080) [16.6 MB] || BeltsPlasmapauseParticles_HD720.mov (1280x720) [10.6 MB] || 1920x1080_16x9_30p (1920x1080) [0 Item(s)] || Earth_BeltsPlasmapauseParticles_Oblique_HD1080.webm (960x540) [2.3 MB] || BeltsPlasmapauseParticles_iPod.m4v (640x360) [3.7 MB] || radiation-belts--plasmapause.hwshow [342 bytes] || ",
            "hits": 125
        },
        {
            "id": 3311,
            "url": "https://svs.gsfc.nasa.gov/3311/",
            "result_type": "Visualization",
            "release_date": "2005-12-05T00:00:00-05:00",
            "title": "Zoom-in to plasmapause-induced TEC enhancement - April 2001",
            "description": "Space weather events which disturb the plasmapause (displayed here as a green surface enclosing the Earth) can propagate down to the Earth's ionosphere.  There they enhance the ionosphere electron content which can disrupt radio signals from satellites.NOTE:  This visualization shows the Earth's magnetic dipole field lines rotating rigidly with the Earth.  Technically, this is inaccurate.  Ions and electrons in the lower atmosphere can create currents which can make these lines 'drag' with Earth's rotation, but this will occur mostly near the Earth and not higher up.  More details on this process can be found in the FAQ at the The Exploration of the Earth's Magnetosphere web site, Does the Earth's magnetic field rotate?. || ",
            "hits": 15
        },
        {
            "id": 3312,
            "url": "https://svs.gsfc.nasa.gov/3312/",
            "result_type": "Visualization",
            "release_date": "2005-12-05T00:00:00-05:00",
            "title": "The 'Big Picture' View of the Plasmapause and Ionospheric Electron Content - April 2001",
            "description": "This visualization presents a wide-angle overview of the plasmapause-Earth system.  Electron content data is mapped to the sphere of the Earth.  As the space storm progresses, the structure of the plasmapause becomes distorted but is still constrained by the structure of the Earth's dipolar magnetic field. || ",
            "hits": 17
        },
        {
            "id": 3314,
            "url": "https://svs.gsfc.nasa.gov/3314/",
            "result_type": "Visualization",
            "release_date": "2005-12-05T00:00:00-05:00",
            "title": "Time-varying Plasmapause and Electron data - April 2001",
            "description": "This is another view of the plasmapause and electron content data for the April 11, 2001 time frame (similar to ID 3312).  This point of view is shifted slightly to the sunlit side of the Earth to present a better view of the plume formation. || ",
            "hits": 13
        },
        {
            "id": 3315,
            "url": "https://svs.gsfc.nasa.gov/3315/",
            "result_type": "Visualization",
            "release_date": "2005-12-05T00:00:00-05:00",
            "title": "Tour of the Plasmapause - April 2001",
            "description": "The near-Earth space environment is filled with plasma formed when the sun's ultraviolet rays electrify the upper parts of the Earth's atmosphere.  This region is called the plasmasphere and its outer boundary is called the plasmapause.  Here we view the plasmasphere in a static state as the observer takes a slow polar-orbiting tour of the region. || ",
            "hits": 19
        },
        {
            "id": 3316,
            "url": "https://svs.gsfc.nasa.gov/3316/",
            "result_type": "Visualization",
            "release_date": "2005-12-05T00:00:00-05:00",
            "title": "Zoom-in to Plasmapause-Induced TEC Enhancement - April 2001 (Version 2)",
            "description": "Space weather events which disturb the plasmapause (displayed here as a green surface enclosing the Earth) can propagate down to the Earth's ionosphere. There they enhance the ionosphere electron content which can disrupt radio signals from satellites. This movie is a variation on animation ID 3311 with slightly different camera motions. NOTE: This visualization shows the Earth's magnetic dipole field lines rotating rigidly with the Earth. Technically, this is inaccurate. Ions and electrons in the lower atmosphere can create currents which can make these lines 'drag' with Earth's rotation, but this will occur mostly near the Earth and not higher up. More details on this process can be found in the FAQ at the The Exploration of the Earth's Magnetosphere web site, Does the Earth's magnetic field rotate?. || ",
            "hits": 13
        },
        {
            "id": 3317,
            "url": "https://svs.gsfc.nasa.gov/3317/",
            "result_type": "Visualization",
            "release_date": "2005-12-05T00:00:00-05:00",
            "title": "Zoom-in to plasmapause-induced TEC enhancement - April 2001",
            "description": "Space weather events which disturb the plasmapause can propagate down to the Earth's ionosphere.  There they enhance the ionosphere electron content which can disrupt radio signals from satellites.  This is a re-timed version of ID 3311.  This version is designed to play synchronously with ID 3310, ID 3312, and ID 3314.NOTE:  This visualization shows the Earth's magnetic dipole field lines rotating rigidly with the Earth.  Technically, this is inaccurate.  Ions and electrons in the lower atmosphere can create currents which can make these lines 'drag' with Earth's rotation, but this will occur mostly near the Earth and not higher up.  More details on this process can be found in the FAQ at the The Exploration of the Earth's Magnetosphere web site, Does the Earth's magnetic field rotate?. || ",
            "hits": 19
        },
        {
            "id": 3049,
            "url": "https://svs.gsfc.nasa.gov/3049/",
            "result_type": "Visualization",
            "release_date": "2004-12-15T12:00:00-05:00",
            "title": "Radiation Belts and Plasmapause Fluctuate Under Solar Storm",
            "description": "In this visualization, we see the interaction of the radiation belts (violet/white), the plasmapause (green surface) and magnetopause (gray surface).NOTE: This visualization shows the Earth's magnetic dipole field lines rotating rigidly with the Earth. Technically, this is inaccurate. Ions and electrons in the lower atmosphere can create currents which can make these lines 'drag' with Earth's rotation, but this will occur mostly near the Earth and not higher up. More details on this process can be found in the FAQ at the The Exploration of the Earth's Magnetosphere web site, Does the Earth's magnetic field rotate?. || ",
            "hits": 62
        },
        {
            "id": 3050,
            "url": "https://svs.gsfc.nasa.gov/3050/",
            "result_type": "Visualization",
            "release_date": "2004-12-15T12:00:00-05:00",
            "title": "Tour of the Plasmasphere and Plasmapause",
            "description": "The plasmasphere is a region of ionospheric plasma which co-rotates with the Earth, carried by the magnetic field lines.  This plasma tends to be colder (i.e. the ions have lower average energy) than the outer region of the magnetosphere.  The plasmapause marks the outer boundary of this region.  This visualization is a simple fly-around tour of the plasmapause (green) in a relatively quiescent state.  For this visualization, the 3-dimensional structure was constructed from the equatorial profile of the plasmapause (as measured by IMAGE/EUV data) by extending the region along field lines of a simple dipole field. || ",
            "hits": 40
        },
        {
            "id": 3051,
            "url": "https://svs.gsfc.nasa.gov/3051/",
            "result_type": "Visualization",
            "release_date": "2004-12-15T12:00:00-05:00",
            "title": "Plasmapause Convects to the Magnetopause During Halloween Solar Storm",
            "description": "The plasmasphere is a region of ionospheric plasma which co-rotates with the Earth, carried by the magnetic field lines.  The plasmapause marks the outer boundary of this region.  This colder plasma is more easily moved by the electric fields created by strong solar storms.  In the Halloween 2003 event, these fields convected some of the cold plasma out to the magnetopause (gray, semi-transparent surface) and reduced the size of the cold plasma region near the Earth.  For this visualization, the 3-dimensional structure was constructed from the equatorial profile of the plasmapause (as measured by IMAGE/EUV data) by extending the region along field lines of a simple dipole field.NOTE:  This visualization shows the Earth's magnetic dipole field lines rotating rigidly with the Earth.  Technically, this is inaccurate.  Ions and electrons in the lower atmosphere can create currents which can make these lines 'drag' with Earth's rotation, but this will occur mostly near the Earth and not higher up.  More details on this process can be found in the FAQ at the The Exploration of the Earth's Magnetosphere web site, Does the Earth's magnetic field rotate?. || ",
            "hits": 17
        },
        {
            "id": 1170,
            "url": "https://svs.gsfc.nasa.gov/1170/",
            "result_type": "Visualization",
            "release_date": "2000-05-24T12:00:00-04:00",
            "title": "Plasmasphere With Earth Inset in EUV",
            "description": "This version of IMAGE observing the Earth's plasmasphere includes an inset showing the size of the Earth. || The Earths plasmasphere, as seen by IMAGE-EUV. || a001170.00095_print.png (720x480) [418.1 KB] || a001170_thm.png (80x40) [4.9 KB] || a001170_pre.jpg (320x242) [6.1 KB] || a001170_pre_searchweb.jpg (320x180) [52.2 KB] || a001170.webmhd.webm (960x540) [694.1 KB] || a001170.dv (720x480) [54.7 MB] || a001170.mp4 (640x480) [2.9 MB] || a001170.mpg (352x240) [2.1 MB] || ",
            "hits": 11
        },
        {
            "id": 1172,
            "url": "https://svs.gsfc.nasa.gov/1172/",
            "result_type": "Visualization",
            "release_date": "2000-05-24T12:00:00-04:00",
            "title": "Plasmasphere Close-up With Earth Inset",
            "description": "The Earths plasmasphere, as seen by IMAGE-EUV. || a001172.00005_print.png (720x480) [549.0 KB] || a001172_thm.png (80x40) [5.8 KB] || a001172_pre.jpg (320x242) [8.9 KB] || a001172_pre_searchweb.jpg (320x180) [68.3 KB] || a001172.webmhd.webm (960x540) [944.5 KB] || a001172.dv (720x480) [54.7 MB] || a001172.mp4 (640x480) [2.9 MB] || a001172.mpg (352x240) [1.8 MB] || ",
            "hits": 14
        },
        {
            "id": 1174,
            "url": "https://svs.gsfc.nasa.gov/1174/",
            "result_type": "Visualization",
            "release_date": "2000-05-24T12:00:00-04:00",
            "title": "IMAGE Views the Plasmasphere in EUV",
            "description": "The IMAGE spacecraft views the Earth's plasmasphere. This animation has no earth inset || The Earths plasmasphere, as seen by IMAGE-EUV. || a001174.00005_print.png (720x480) [439.4 KB] || a001174_thm.png (80x40) [4.7 KB] || a001174_pre.jpg (320x242) [5.9 KB] || a001174_pre_searchweb.jpg (320x180) [51.3 KB] || a001174.webmhd.webm (960x540) [723.1 KB] || a001174.dv (720x480) [54.7 MB] || a001174.mp4 (640x480) [2.9 MB] || a001174.mpg (352x240) [2.1 MB] || ",
            "hits": 23
        },
        {
            "id": 1176,
            "url": "https://svs.gsfc.nasa.gov/1176/",
            "result_type": "Visualization",
            "release_date": "2000-05-24T12:00:00-04:00",
            "title": "Plasmasphere with Earth Inset",
            "description": "May 16, 2000 || Plasmasphere movie, as seen by IMAGE-EUV || a001176.00005_print.png (720x480) [416.6 KB] || a001176_thm.png (80x40) [4.8 KB] || a001176_pre.jpg (320x242) [5.9 KB] || a001176_pre_searchweb.jpg (320x180) [52.2 KB] || a001176.webmhd.webm (960x540) [647.0 KB] || a001176.dv (720x480) [51.3 MB] || a001176.mp4 (640x480) [2.7 MB] || a001176.mpg (352x240) [2.1 MB] || ",
            "hits": 15
        },
        {
            "id": 1177,
            "url": "https://svs.gsfc.nasa.gov/1177/",
            "result_type": "Visualization",
            "release_date": "2000-05-24T12:00:00-04:00",
            "title": "Plasmasphere Without Earth Inset",
            "description": "May 16, 2000 || Plasmasphere movie, as seen by IMAGE-EUV || a001177.00005_print.png (720x480) [404.8 KB] || a001177_thm.png (80x40) [4.7 KB] || a001177_pre.jpg (320x242) [5.7 KB] || a001177_pre_searchweb.jpg (320x180) [50.6 KB] || a001177.webmhd.webm (960x540) [606.7 KB] || a001177.dv (720x480) [51.3 MB] || a001177.mp4 (640x480) [2.8 MB] || a001177.mpg (352x240) [1.9 MB] || ",
            "hits": 14
        }
    ]
}