{
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    "next": null,
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    "results": [
        {
            "id": 4618,
            "url": "https://svs.gsfc.nasa.gov/4618/",
            "result_type": "Visualization",
            "release_date": "2018-01-31T00:00:00-05:00",
            "title": "Geostationary Operational Environmental Satellite (GOES) East and West",
            "description": "This animation depicts the areas of the Earth viewed by GOES-East and GOES-West from their vantage point 22,236 miles above the equator.This video is also available on our YouTube channel. || goes_EastWest.000945_print.jpg (1024x576) [50.9 KB] || goes_EastWest.000945_searchweb.png (320x180) [48.6 KB] || goes_EastWest.000945_thm.png (80x40) [2.9 KB] || goes_EastWest (1920x1080) [0 Item(s)] || goes_EastWest_1080p30.mp4 (1920x1080) [48.2 MB] || goes_EastWest_1080p30.webm (1920x1080) [6.5 MB] || goes_EastWest_1080p30.mp4.hwshow [187 bytes] || ",
            "hits": 187
        },
        {
            "id": 579,
            "url": "https://svs.gsfc.nasa.gov/579/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "UARS: The Upper Atmosphere Research Satellite",
            "description": "This video summarizes science and data obtained by the Upper Atmosphere Research Satellite (UARS) mission.  UARS was launched in 1991 to study ozone depletion and the processes that control the stratospheric ozone layer.  Although the mission was intended to last only 18 months, UARS continued to operate 7.5 years after launch with 8 of the 10 instruments at the time this video was made. UARS has been one of the most successful NASA satellite programs. The spacecraft was developed and is managed by NASA's Goddard Space Flight Center. || ",
            "hits": 50
        },
        {
            "id": 808,
            "url": "https://svs.gsfc.nasa.gov/808/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Viewing the MLS Instrument on UARS",
            "description": "The Microwave Limb Sounder (MLS) measures microwave emission from ozone and chlorine monoxide, a major ozone destroying radical. || Locating MLS on UARS || a000808.00010_print.png (720x480) [437.1 KB] || a000808_pre.jpg (320x242) [7.0 KB] || a000808.webmhd.webm (960x540) [1.6 MB] || a000808.dv (720x480) [34.8 MB] || a000808.mp4 (640x480) [1.9 MB] || a000808.mpg (352x240) [1.1 MB] || ",
            "hits": 33
        },
        {
            "id": 809,
            "url": "https://svs.gsfc.nasa.gov/809/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "MLS Looking at the Limb",
            "description": "The chemistry of ozone destruction involves very small quantities of stratospheric gases which change rapidly with altitude. UARS is able to determine the altitude variation of these gases by looking at the atmosphere edge on. This is called limb sounding.  The Microwave Limb Sounder (MLS) measures microwave emission from ozone and chlorine monoxide, a major ozone destroying radical. || ",
            "hits": 39
        },
        {
            "id": 810,
            "url": "https://svs.gsfc.nasa.gov/810/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Viewing the ISAMS and CLAES Instruments on UARS",
            "description": "Key to understanding the chlorine chemistry in the polar stratosphere is the measurement of polar stratospheric clouds, chlorine monoxide, and the reservoir gas chlorine nitrate.  Polar stratospheric clouds  are seen by the  Improved Stratospheric and Mesospheric Sounder, ISAMS, and chlorine nitrate has been measured by the Cryogen Limb Array Etalon Spectrometer, CLAES.  Both ISAMS and CLAES make measurements by looking at  infrared emission from cloud particles and trace gases. || ",
            "hits": 37
        },
        {
            "id": 811,
            "url": "https://svs.gsfc.nasa.gov/811/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Viewing the HALOE Instrument on UARS",
            "description": "The Halogen Occultation Experiment, HALOE, was designed to carefully monitor hydrogen fluoride and hydrogen chloride, byproducts of CFC destruction in the stratosphere. || ",
            "hits": 34
        },
        {
            "id": 812,
            "url": "https://svs.gsfc.nasa.gov/812/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "HALOE Looking at the Sun",
            "description": "The Halogen Occultation Experiment, HALOE, was designed to carefully monitor  hydrogen fluoride and hydrogen chloride, byproducts of CFC destruction in the stratosphere. HALOE operates by observing the absorption of infrared radiation by these molecules against the rising and setting sun. || ",
            "hits": 36
        },
        {
            "id": 813,
            "url": "https://svs.gsfc.nasa.gov/813/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Viewing the WINDII Instrument on UARS",
            "description": "The Wind  Imaging Interferometer, WINDII, measures the winds in the mesosphere, using air glow. || Locating WINDII on UARS || a000813.00005_print.png (720x480) [378.6 KB] || a000813_thm.png (80x40) [5.1 KB] || a000813_pre.jpg (320x242) [5.5 KB] || a000813_pre_searchweb.jpg (320x180) [30.0 KB] || a000813.webmhd.webm (960x540) [4.5 MB] || a000813.dv (720x480) [56.2 MB] || a000813.mp4 (640x480) [3.1 MB] || a000813.mpg (352x240) [1.6 MB] || ",
            "hits": 50
        },
        {
            "id": 814,
            "url": "https://svs.gsfc.nasa.gov/814/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Viewing the HRDI Instrument on UARS",
            "description": "The High Resolution Doppler Interferometer, HRDI, measures winds in both the stratosphere and mesosphere. || Locating HRDI on UARS || a000814.00005_print.png (720x480) [453.3 KB] || a000814_thm.png (80x40) [5.4 KB] || a000814_pre.jpg (320x242) [8.5 KB] || a000814_pre_searchweb.jpg (320x180) [58.3 KB] || a000814.webmhd.webm (960x540) [4.1 MB] || a000814.mp4 (640x480) [2.8 MB] || a000814.dv (720x480) [51.8 MB] || a000814.mpg (352x240) [1.8 MB] || ",
            "hits": 38
        },
        {
            "id": 815,
            "url": "https://svs.gsfc.nasa.gov/815/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Viewing the ACRIM Instrument on UARS",
            "description": "To understand the solar effects on the ozone layer, UARS was equipped with three instruments to measure the sun. One of them, the Active Cavity Radiometer Irradiance Monitor, ACRIM, measures the total energy output from the sun. || ",
            "hits": 51
        },
        {
            "id": 816,
            "url": "https://svs.gsfc.nasa.gov/816/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Viewing the SUSIM and SOLSTICE Instruments on UARS",
            "description": "The Solar Ultraviolet Spectral Irradiance Monitor, SUSIM, and the Solar/Stellar Irradiance Comparison Experiment, SOLSTICE, measure the sun's ultraviolet radiation. || ",
            "hits": 38
        },
        {
            "id": 817,
            "url": "https://svs.gsfc.nasa.gov/817/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Viewing the PEM Instrument on UARS",
            "description": "UARS measures the flux of energetic particles from space using the Particle Environment Monitor, PEM. These high energy particles cause ozone depletion at high altitudes by producing nitrogen and hydrogen radicals. || ",
            "hits": 42
        }
    ]
}