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        {
            "id": 20252,
            "url": "https://svs.gsfc.nasa.gov/20252/",
            "result_type": "Animation",
            "release_date": "2017-10-18T12:00:00-04:00",
            "title": "Phobos Electric Charging",
            "description": "The interaction of the solar wind with the Martian moon Phobos creates a complex electrical environment that could impact future exploration. Complete transcript available.Watch this video on the NASA Goddard YouTube channel.Music provided by Killer Tracks: \"Innovations\" by Pascal Lengagne || PhobosChargingPreview.jpg (3840x2160) [1.6 MB] || PhobosChargingPreview_print.jpg (1024x576) [193.8 KB] || PhobosChargingPreview_searchweb.png (320x180) [95.8 KB] || PhobosChargingPreview_thm.png (80x40) [7.2 KB] || TWITTER_720-20252_Phobos_Electric_Charging_APR_twitter_720.mp4 (1280x720) [34.1 MB] || WEBM-20252_Phobos_Electric_Charging_APR.webm (960x540) [59.7 MB] || FACEBOOK_720-20252_Phobos_Electric_Charging_APR_facebook_720.mp4 (1280x720) [196.8 MB] || 20252_Phobos_Electric_Charging_APR_Output.en_US.srt [3.0 KB] || 20252_Phobos_Electric_Charging_APR_Output.en_US.vtt [3.0 KB] || YOUTUBE_4K-20252_Phobos_Electric_Charging_APR_youtube_4k.mp4 (3840x2160) [644.3 MB] || 20252_Phobos_Electric_Charging_APR.mov (3840x2160) [12.8 GB] || ",
            "hits": 85
        },
        {
            "id": 3310,
            "url": "https://svs.gsfc.nasa.gov/3310/",
            "result_type": "Visualization",
            "release_date": "2005-12-05T00:00:00-05:00",
            "title": "Ionosphere Total Electron Content - April 2001",
            "description": "A view of the ionospheric Total Electron Content (TEC) measured over North America during a storm in April 2001.  Red is high electron counts, blue is low, gray where there is no data.  From the pre-storm state, we see relatively low electron counts.  As the storm intensity increases, so do the number of electrons.  The increase will generate more interference for communications systems, GPS, etc. || ",
            "hits": 27
        },
        {
            "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": 24
        },
        {
            "id": 3313,
            "url": "https://svs.gsfc.nasa.gov/3313/",
            "result_type": "Visualization",
            "release_date": "2005-12-05T00:00:00-05:00",
            "title": "Ionosphere Total Electron Content - November 2003",
            "description": "This movie displays plume formation for a space weather event in November 2003.  In this visualization, the observer is fixed between the Sun and the Earth (slightly off the center line for better perspective).  Blue represents low ionospheric electron counts, dark red is high electron counts. || ",
            "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": 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": 20
        },
        {
            "id": 2891,
            "url": "https://svs.gsfc.nasa.gov/2891/",
            "result_type": "Visualization",
            "release_date": "2004-02-10T12:00:00-05:00",
            "title": "Aurora over the North Pole on April 17, 1999 (WMS)",
            "description": "When the charged particles flowing outward from the Sun (the solar wind) hit the Earth's magnetic field, they are channeled down the magnetic field lines to the ionosphere at the North and South Poles.  The impact of these particles on atmospheric molecules causes the molecules to emit light, which forms the visible aurora.  This visualization shows the development of the aurora over the North Pole for about three hours on April 17, 1999, as seen by the ultraviolet VIS Earth Camera on the POLAR spacecraft.  The two main features of these ultraviolet images are the very bright ultraviolet emission from the reflected solar radiation on the dayside of the Earth and the bright ring of the auroral oval circling the North Pole.  The aurora seen in this visualization is the diffuse aurora, a very large bright band that is actually too dim to be seen well from the ground by the human eye.  What we normally think of as the aurora are the even brighter curtains of light within the diffuse auroral caused by very energetic electrons.  These curtains are too small to be seen in this image.  The diffuse aurora appears as a ring around the pole rather than as a bright spot over the entire pole because the solar particles actually spend extended time wandering about within the Earth's magnetic field before traveling down a very select set of magnetic field lines to the Earth.  Near the end of this three hour period, the spacecraft was getting so close to the Earth that the edges of the globe were outside the camera's image, which accounts for the growing circular data gaps over Asia and the Pacific Ocean. || ",
            "hits": 28
        },
        {
            "id": 777,
            "url": "https://svs.gsfc.nasa.gov/777/",
            "result_type": "Visualization",
            "release_date": "1999-12-08T12:00:00-05:00",
            "title": "Polar: PIXIE at Apogee on May 11, 1999 (North)",
            "description": "On May 11, 1999, the solar wind that blows constantly from the Sun virtually disappeared.  Dropping to a small fraction of its normal density and to half its normal speed, the solar wind died down enough to allow physicists to observe particles flowing directly from the Sun's corona to Earth. This severe change in the solar wind also drastically changed the shape of Earth's magnetic field and produced a rare auroral display at Earth's North Pole. || ",
            "hits": 42
        },
        {
            "id": 778,
            "url": "https://svs.gsfc.nasa.gov/778/",
            "result_type": "Visualization",
            "release_date": "1999-12-08T12:00:00-05:00",
            "title": "Polar: PIXIE at Perigee on May 11, 1999 (North)",
            "description": "On May 11, 1999, the solar wind that blows constantly from the Sun virtually disappeared. Dropping to a small fraction of its normal density and to half its normal speed, the solar wind died down enough to allow physicists to observe particles flowing directly from the Sun's corona to Earth. This severe change in the solar wind also drastically changed the shape of Earth's magnetic field and produced a rare auroral display at Earth's North Pole. || ",
            "hits": 39
        },
        {
            "id": 779,
            "url": "https://svs.gsfc.nasa.gov/779/",
            "result_type": "Visualization",
            "release_date": "1999-12-08T12:00:00-05:00",
            "title": "Polar: PIXIE at Perigee 1 on May 11, 1999 (South)",
            "description": "On May 11, 1999, the solar wind that blows constantly from the Sun virtually disappeared. Dropping to a small fraction of its normal density and to half its normal speed, the solar wind died down enough to allow physicists to observe particles flowing directly from the Sun's corona to Earth. This severe change in the solar wind also drastically changed the shape of Earth's magnetic field and produced a rare auroral display at Earth's North Pole. || ",
            "hits": 36
        },
        {
            "id": 780,
            "url": "https://svs.gsfc.nasa.gov/780/",
            "result_type": "Visualization",
            "release_date": "1999-12-08T12:00:00-05:00",
            "title": "Polar: PIXIE at Perigee 2 on May 11, 1999 (South)",
            "description": "On May 11, 1999, the solar wind that blows constantly from the Sun virtually disappeared. Dropping to a small fraction of its normal density and to half its normal speed, the solar wind died down enough to allow physicists to observe particles flowing directly from the Sun's corona to Earth. This severe change in the solar wind also drastically changed the shape of Earth's magnetic field and produced a rare auroral display at Earth's North Pole. || ",
            "hits": 14
        },
        {
            "id": 781,
            "url": "https://svs.gsfc.nasa.gov/781/",
            "result_type": "Visualization",
            "release_date": "1999-12-08T12:00:00-05:00",
            "title": "Polar: PIXIE at T055798 on May 11, 1999 at 05:05",
            "description": "On May 11, 1999, the solar wind that blows constantly from the Sun virtually disappeared. Dropping to a small fraction of its normal density and to half its normal speed, the solar wind died down enough to allow physicists to observe particles flowing directly from the Sun's corona to Earth. This severe change in the solar wind also drastically changed the shape of Earth's magnetic field and produced a rare auroral display at Earth's North Pole. || ",
            "hits": 9
        },
        {
            "id": 782,
            "url": "https://svs.gsfc.nasa.gov/782/",
            "result_type": "Visualization",
            "release_date": "1999-12-08T12:00:00-05:00",
            "title": "Polar: PIXIE at T055798 on May 11, 1999 at 22:55",
            "description": "On May 11, 1999, the solar wind that blows constantly from the Sun virtually disappeared. Dropping to a small fraction of its normal density and to half its normal speed, the solar wind died down enough to allow physicists to observe particles flowing directly from the Sun's corona to Earth. This severe change in the solar wind also drastically changed the shape of Earth's magnetic field and produced a rare auroral display at Earth's North Pole. || ",
            "hits": 9
        },
        {
            "id": 783,
            "url": "https://svs.gsfc.nasa.gov/783/",
            "result_type": "Visualization",
            "release_date": "1999-12-08T12:00:00-05:00",
            "title": "Polar Visible Aurora: North Pole Comparison between May 11, 1999 and November 13, 1999 (Continents)",
            "description": "On May 11, 1999, the solar wind that blows constantly from the Sun virtually disappeared. Dropping to a small fraction of its normal density and to half its normal speed, the solar wind died down enough to allow physicists to observe particles flowing directly from the Sun's corona to Earth. This severe change in the solar wind also drastically changed the shape of Earth's magnetic field and produced a rare auroral display at Earth's North Pole. || ",
            "hits": 10
        },
        {
            "id": 784,
            "url": "https://svs.gsfc.nasa.gov/784/",
            "result_type": "Visualization",
            "release_date": "1999-12-08T12:00:00-05:00",
            "title": "Polar Visible Aurora: North Pole Comparison Between May 11, 1999 and November 13, 1999 (Grid)",
            "description": "On May 11, 1999, the solar wind that blows constantly from the Sun virtually disappeared. Dropping to a small fraction of its normal density and to half its normal speed, the solar wind died down enough to allow physicists to observe particles flowing directly from the Sun's corona to Earth. This severe change in the solar wind also drastically changed the shape of Earth's magnetic field and produced a rare auroral display at Earth's North Pole. || ",
            "hits": 43
        },
        {
            "id": 785,
            "url": "https://svs.gsfc.nasa.gov/785/",
            "result_type": "Visualization",
            "release_date": "1999-12-08T12:00:00-05:00",
            "title": "Polar Visible Aurora: High Solar Wind Conditions on April 17, 1999 over the North Pole",
            "description": "On May 11, 1999, the solar wind that blows constantly from the Sun virtually disappeared. Dropping to a small fraction of its normal density and to half its normal speed, the solar wind died down enough to allow physicists to observe particles flowing directly from the Sun's corona to Earth. This severe change in the solar wind also drastically changed the shape of Earth's magnetic field and produced a rare auroral display at Earth's North Pole. || ",
            "hits": 50
        },
        {
            "id": 786,
            "url": "https://svs.gsfc.nasa.gov/786/",
            "result_type": "Visualization",
            "release_date": "1999-12-08T12:00:00-05:00",
            "title": "Polar Visible Aurora: Low Solar Wind Conditions on May 11, 1999 over the North Pole",
            "description": "On May 11, 1999, the solar wind that blows constantly from the Sun virtually disappeared. Dropping to a small fraction of its normal density and to half its normal speed, the solar wind died down enough to allow physicists to observe particles flowing directly from the Sun's corona to Earth. This severe change in the solar wind also drastically changed the shape of Earth's magnetic field and produced a rare auroral display at Earth's North Pole. || ",
            "hits": 45
        },
        {
            "id": 787,
            "url": "https://svs.gsfc.nasa.gov/787/",
            "result_type": "Visualization",
            "release_date": "1999-12-08T12:00:00-05:00",
            "title": "Polar Visible Aurora: Low Solar Wind Conditions on May 11, 1999 over the South Pole",
            "description": "On May 11, 1999, the solar wind that blows constantly from the Sun virtually disappeared. Dropping to a small fraction of its normal density and to half its normal speed, the solar wind died down enough to allow physicists to observe particles flowing directly from the Sun's corona to Earth. This severe change in the solar wind also drastically changed the shape of Earth's magnetic field and produced a rare auroral display at Earth's North Pole. || ",
            "hits": 39
        },
        {
            "id": 788,
            "url": "https://svs.gsfc.nasa.gov/788/",
            "result_type": "Visualization",
            "release_date": "1999-12-08T12:00:00-05:00",
            "title": "Polar Visible Aurora: Normal Solar Wind Conditions on November 13, 1999 over the North Pole",
            "description": "On May 11, 1999, the solar wind that blows constantly from the Sun virtually disappeared. Dropping to a small fraction of its normal density and to half its normal speed, the solar wind died down enough to allow physicists to observe particles flowing directly from the Sun's corona to Earth. This severe change in the solar wind also drastically changed the shape of Earth's magnetic field and produced a rare auroral display at Earth's North Pole. || ",
            "hits": 46
        }
    ]
}