{
    "count": 26,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 13503,
            "url": "https://svs.gsfc.nasa.gov/13503/",
            "result_type": "Produced Video",
            "release_date": "2019-12-10T13:00:00-05:00",
            "title": "How NASA Studies The Space Near Earth",
            "description": "NASA studies the space around our home planet, a region we call geospace. It might appear empty, but geospace is bustling with electrically charged particles and magnetic fields — all of which can impact the technology and satellites we have flying through it. NASA uses specialized tools to study changing conditions in geospace, known as space weather. Each examines geospace in its own way. Together, they help us visualize, and better understand, the invisible processes shaping the space that is closest to home. || ",
            "hits": 67
        },
        {
            "id": 20099,
            "url": "https://svs.gsfc.nasa.gov/20099/",
            "result_type": "Animation",
            "release_date": "2007-02-12T12:00:00-05:00",
            "title": "Proton Aurora",
            "description": "This animation shows a magnetic reconnection event with proton aurora data from the IMAGE spacecraft. || Proton aurora animation || Image_recon060000602_print.jpg (1024x698) [32.6 KB] || Image_recon0600_web.png (320x216) [276.8 KB] || reconD1.webmhd.webm (960x540) [7.5 MB] || 720x486_4x3_29.97p (720x486) [64.0 KB] || reconD1.mov (720x486) [38.3 MB] || recon.mpg (352x240) [7.9 MB] || recon.mov (360x240) [14.4 MB] || ",
            "hits": 66
        },
        {
            "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": 14
        },
        {
            "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": 15
        },
        {
            "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": 9
        },
        {
            "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": 16
        },
        {
            "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": 9
        },
        {
            "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": 80
        },
        {
            "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": 54
        },
        {
            "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": 22
        },
        {
            "id": 20036,
            "url": "https://svs.gsfc.nasa.gov/20036/",
            "result_type": "Animation",
            "release_date": "2004-12-03T12:00:00-05:00",
            "title": "IMAGE and Cluster View Magnetic Reconnection",
            "description": "The IMAGE and Cluster spacecraft were ideally positioned in their orbits to view the reconnection event which led to the proton aurora formation. || ",
            "hits": 19
        },
        {
            "id": 20037,
            "url": "https://svs.gsfc.nasa.gov/20037/",
            "result_type": "Animation",
            "release_date": "2004-12-03T12:00:00-05:00",
            "title": "Proton Aurora Forms from Reconnection Event",
            "description": "Solar wind protons can breach the Earth's magnetic field through a magnetic reconnection event.  Sometimes when this happens we see a (proton) aurora when the solar protons make it to the Earth's atmosphere. || ",
            "hits": 54
        },
        {
            "id": 2964,
            "url": "https://svs.gsfc.nasa.gov/2964/",
            "result_type": "Visualization",
            "release_date": "2004-07-08T12:00:00-04:00",
            "title": "IMAGE Views of the Aurora from Space",
            "description": "The IMAGE spacecraft observed intense auroral displays in the Fall of 2003 as the material from the coronal mass ejection swept past the Earth.  The pressure against the Earth's magnetosphere caused it to dump more electrons into the upper atmosphere, creating auroral displays, as we see here over the South Pole.  This is a view of the IMAGE data reprojected onto a model of the Earth. || ",
            "hits": 43
        },
        {
            "id": 2861,
            "url": "https://svs.gsfc.nasa.gov/2861/",
            "result_type": "Visualization",
            "release_date": "2003-12-04T12:00:00-05:00",
            "title": "Reconnection: Solar Wind Breaches the Earth's Magnetic Shield",
            "description": "The Far Ultraviolet camera aboard the IMAGE spacecraft captured this view of a proton aurora (the bright spot near the center of the view) as well as the ring of the electron aurora. The protons for this aurora came from the incoming solar wind. They made it though the Earth's magnetic shield in a magnetic reconnection event higher in the magnetosphere which was detected by the Cluster satellite. Note: A 'corner' appears in the data in the beginning as the IMAGE spacecraft moves into a position where it can view the entire north polar region. || ",
            "hits": 40
        },
        {
            "id": 2435,
            "url": "https://svs.gsfc.nasa.gov/2435/",
            "result_type": "Visualization",
            "release_date": "2002-05-09T12:00:00-04:00",
            "title": "IMAGE/LENA Observes Oxygen Atoms in the near-Earth Environment",
            "description": "Electrically charged oxygen atoms (green) are ejected into the magnetosphere due to heating in the ionosphere.  The red 'thermometer' displays the intensity of the solar wind (dynamic pressure) measured by the Geotail spacecraft.  The yellow 'thermometer' represents the source intensity or hydrogen counts as measured by IMAGE/LENA. || ",
            "hits": 17
        },
        {
            "id": 2444,
            "url": "https://svs.gsfc.nasa.gov/2444/",
            "result_type": "Visualization",
            "release_date": "2002-05-09T12:00:00-04:00",
            "title": "IMAGE/HENA Views Oxygen in the Magnetosphere (Rainbow Version)",
            "description": "IMAGE/HENA observes the oxygen ions, expelled from the Earth's atmosphere by the solar wind, return to the polar regions via the magnetic field. || Movie of IMAGE-HENA data using a rainbow color table for oxygen intensity. || a002444.00100_print.png (720x480) [373.3 KB] || HENArainbow_pre.jpg (320x288) [13.5 KB] || a002444.webmhd.webm (960x540) [8.1 MB] || a002444.dv (720x480) [112.3 MB] || HENArainbow.mpg (320x288) [942.9 KB] || ",
            "hits": 14
        },
        {
            "id": 2445,
            "url": "https://svs.gsfc.nasa.gov/2445/",
            "result_type": "Visualization",
            "release_date": "2002-05-09T12:00:00-04:00",
            "title": "IMAGE/HENA Views Oxygen in the Magnetosphere (Blue Version)",
            "description": "IMAGE/HENA observes the oxygen ions, expelled from the Earth's atmosphere by the solar wind, return to the polar regions via the magnetic field. || Movie of IMAGE-HENA data using a blue color table for oxygen intensity. || a002445.00010_print.png (720x480) [371.4 KB] || HENAblue_pre.jpg (320x320) [7.9 KB] || a002445.webmhd.webm (960x540) [8.1 MB] || a002445.dv (720x480) [153.6 MB] || HENAblue.mpg (320x320) [1.3 MB] || ",
            "hits": 11
        },
        {
            "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": 1171,
            "url": "https://svs.gsfc.nasa.gov/1171/",
            "result_type": "Visualization",
            "release_date": "2000-05-24T12:00:00-04:00",
            "title": "Aurora With Earth Inset",
            "description": "Earths aurora, as seen by IMAGE. || a001171.00005_print.png (720x480) [439.3 KB] || a001171_pre.jpg (320x242) [6.8 KB] || a001171_thm.png (80x40) [4.7 KB] || a001171_pre_searchweb.jpg (320x180) [54.4 KB] || a001171.webmhd.webm (960x540) [797.7 KB] || a001171.dv (720x480) [61.6 MB] || a001171.mp4 (640x480) [3.3 MB] || a001171.mpg (352x240) [2.3 MB] || ",
            "hits": 47
        },
        {
            "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": 18
        },
        {
            "id": 1173,
            "url": "https://svs.gsfc.nasa.gov/1173/",
            "result_type": "Visualization",
            "release_date": "2000-05-24T12:00:00-04:00",
            "title": "Aurora Close-up With Earth Inset",
            "description": "Earths aurora, as seen by IMAGE. || a001173.00005_print.png (720x480) [480.6 KB] || a001173_thm.png (80x40) [5.0 KB] || a001173_pre.jpg (320x242) [7.7 KB] || a001173_pre_searchweb.jpg (320x180) [58.5 KB] || a001173.webmhd.webm (960x540) [908.0 KB] || a001173.dv (720x480) [61.6 MB] || a001173.mp4 (640x480) [3.3 MB] || a001173.mpg (352x240) [2.2 MB] || ",
            "hits": 10
        },
        {
            "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": 27
        },
        {
            "id": 1175,
            "url": "https://svs.gsfc.nasa.gov/1175/",
            "result_type": "Visualization",
            "release_date": "2000-05-24T12:00:00-04:00",
            "title": "Aurora Without Earth Inset",
            "description": "A view of aurora from the IMAGE satellite without an earth inset || A movie of the Earths aurora, as seen by IMAGE. || a001175.00005_print.png (720x480) [422.7 KB] || a001175_thm.png (80x40) [4.5 KB] || a001175_pre.jpg (320x242) [6.4 KB] || a001175_pre_searchweb.jpg (320x180) [50.2 KB] || a001175.webmhd.webm (960x540) [725.0 KB] || a001175.dv (720x480) [61.6 MB] || a001175.mp4 (640x480) [3.3 MB] || a001175.mpg (352x240) [2.2 MB] || ",
            "hits": 6
        },
        {
            "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": 8
        },
        {
            "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": 6
        }
    ]
}