{
    "count": 13,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 13212,
            "url": "https://svs.gsfc.nasa.gov/13212/",
            "result_type": "Produced Video",
            "release_date": "2019-05-22T00:00:00-04:00",
            "title": "NASA Science Live: Storms Across the Solar System (Episode 04)",
            "description": "NASA Science Live: Storms Across the Solar SystemProgram Aired May 22, 2019 || 13212_NSL_Ep4_youtube_720.00001_print.jpg (1024x576) [83.3 KB] || 13212_NSL_Ep4_youtube_720.00001_searchweb.png (320x180) [81.7 KB] || 13212_NSL_Ep4_youtube_720.00001_thm.png (80x40) [5.7 KB] || 13212_NSL_Ep4_lowres.mp4 (1280x720) [551.2 MB] || 13212_NSL_Ep4_youtube_720.mp4 (1280x720) [3.1 GB] || 13212_NSL_Ep4.mov (1280x720) [19.4 GB] || 13212_NSL_Ep4.webm (960x540) [824.7 MB] || 13212_NSL_Ep4.mov.en_US.srt [69.0 KB] || 13212_NSL_Ep4.mov.en_US.vtt [65.1 KB] || ",
            "hits": 34
        },
        {
            "id": 4109,
            "url": "https://svs.gsfc.nasa.gov/4109/",
            "result_type": "Visualization",
            "release_date": "2013-10-02T00:00:00-04:00",
            "title": "Lunar Far Side: From Luna 3 to LRO",
            "description": "In October of 1959, the Luna 3 spacecraft launched from the Baikonur Cosmodrome in Kazakhstan. Luna 3 was the third spacecraft to reach the Moon and the first to send back pictures of the Moon's far side. The pictures were noisy and indistinct, but because the Moon always presents the same face to the Earth, they offered views of a part of the Moon that had never been seen before.The far side of the Moon is surprisingly different. The most striking difference evident in the Luna 3 pictures is the absence of the large, dark seas of cooled lava, called maria, that cover a substantial fraction of the Earth-facing near side. The far side is instead densely peppered with impact craters of every size and age.Fifty years later, in June of 2009, Lunar Reconnaissance Orbiter (LRO) launched from Kennedy Space Center in Florida. Using LRO's global elevation maps and photographic mosaics, both of which are of unprecedented quality and detail, it's possible to accurately recreate the view captured in the pictures from Luna 3. As seen here, Luna 3 was directly over 12°N 120°E at a distance of 61,700 kilometers above the surface, and its camera was banked 17.5° clockwise from vertical relative to the Moon's north pole.The thicker blue longitude line at 90°E, along the left side of the LRO image, marks the boundary between the near and far sides of the Moon. To the left of that line are the familiar maria Crisium (the circular spot near the 9 o'clock position), Marginis, Smythii (both east of Crisium), Humboldtianum (in the north), Australe (near the south pole), and the eastern edge of Fecunditatis. The bright spot near the center of the disk is a complex of unnamed craters bordered by King, Langemak, Gregory, and Abul Wafa craters. The brightness is enhanced because it's near the subsolar point. The dark, sharp-edged shield shape in the southern hemisphere, with the white dot in the middle, is Tsiolkovskiy crater and its central peak. The dark spot to the southeast of Tsiolkovskiy is the crater Jules Verne. The mare in the northeast is Moscoviense. || ",
            "hits": 628
        },
        {
            "id": 10270,
            "url": "https://svs.gsfc.nasa.gov/10270/",
            "result_type": "Produced Video",
            "release_date": "2008-07-15T00:00:00-04:00",
            "title": "Cosmic Origins Spectrograph - Exploring Physics Across the Universe",
            "description": "The Cosmic Origins Spectrograph, a fourth-generation instrument, designed by Dr. James Green and his University of Colorado colleagues for the cosmic web study in the 90's, will replace the Corrective Optics Space Telescope Axial Replacement (COSTAR.)Once installed on the Hubble Space Telescope during the upcoming servicing mission this year, COS will dramatically advance physics and astrophysics research on the origin of the Universe, astronomical objects, evolution of galaxies, and planetary system formations. In addition, the spectroscope will significantly enhance the spectroscopic capabilities of the telescope at ultraviolet wavelengths, provide scientists with unparalleled opportunities for observing faint sources of ultraviolet and cosmic web light that will absorb new cosmic information and help the telescope investigate the collected data until the end of its mission, currently 2013.For complete transcript, click here. || G08-013HD-COS-fulres_HD_FinalCut_A-V2_101427_print.jpg (1024x576) [122.4 KB] || G08-013HD-COS-fulres_HD_FinalCut_A-V2_1_web.png (320x180) [261.6 KB] || G08-013HD-COS-fulres_HD_FinalCut_A-V2_1_thm.png (80x40) [17.9 KB] || G08-013HD-COS-fulres_AppleTV.webmhd.webm (960x540) [63.9 MB] || G08-013HD-COS-720p30.mp4 (1280x720) [282.4 MB] || G08-013HD-COS-fulres_YouTube.mov (1280x720) [75.8 MB] || G08-013HD-COS-fulres_AppleTV.m4v (960x540) [157.9 MB] || G08-013HD-COS-fulres_HD_FinalCut_A-V2_1.mpg (640x360) [67.8 MB] || G08-013HD-COS-iPod-lg.m4v (640x355) [50.1 MB] || G2008-013HD-COS_full_res.wmv (346x260) [32.0 MB] || ",
            "hits": 24
        },
        {
            "id": 20065,
            "url": "https://svs.gsfc.nasa.gov/20065/",
            "result_type": "Animation",
            "release_date": "2005-04-27T12:00:00-04:00",
            "title": "Lightning Makes a Safe Zone in the Earth's Radiation Belts",
            "description": "Radio waves generated by terrestrial lighting get propagated by electrons along the Earth's magnetic field lines and sweep high-energy electrons away from their path. This opens a 'Safe Zone' in the radiation belts. || ",
            "hits": 29
        },
        {
            "id": 3115,
            "url": "https://svs.gsfc.nasa.gov/3115/",
            "result_type": "Visualization",
            "release_date": "2005-03-08T12:00:00-05:00",
            "title": "Gaps in the Earth's Radiation Belts",
            "description": "The Earth's radiation belts (violet & white) change considerably due to a number of influences, ranging from a changing solar wind to the lightning on the Earth. Here we see a range of variation in the electron flux in early December 2003. White indicates higher electron flux than violet. The gray curves represent the lines of the Earth's magnetic field. These radiation belts are constructed on a per-orbit basis with data from SAMPEX. || ",
            "hits": 28
        },
        {
            "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": 20
        },
        {
            "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": 29
        },
        {
            "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": 36
        },
        {
            "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": 44
        },
        {
            "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": 19
        },
        {
            "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": 24
        },
        {
            "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": 16
        },
        {
            "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": 24
        }
    ]
}