{
    "count": 37,
    "next": null,
    "previous": null,
    "results": [
        {
            "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": 58
        },
        {
            "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": 44
        },
        {
            "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": 38
        },
        {
            "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": 43
        },
        {
            "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": 46
        },
        {
            "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": 52
        },
        {
            "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": 45
        },
        {
            "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": 53
        },
        {
            "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": 35
        },
        {
            "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": 44
        },
        {
            "id": 818,
            "url": "https://svs.gsfc.nasa.gov/818/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Earth Probe TOMS Orbiting the Earth",
            "description": "A composite image of the Earth from SeaWIFS is used as the background of this beauty shot of Earth Probe TOMS. || Earth Probe TOMS orbiting the Earth || a000818.00010_print.png (720x480) [698.3 KB] || a000818_thm.png (80x40) [6.4 KB] || a000818_pre.jpg (320x242) [16.6 KB] || a000818_pre_searchweb.jpg (320x180) [98.7 KB] || a000818.webmhd.webm (960x540) [13.5 MB] || a000818.dv (720x480) [196.0 MB] || a000818.mp4 (640x480) [10.6 MB] || a000818.mpg (352x240) [6.9 MB] || ",
            "hits": 13
        },
        {
            "id": 819,
            "url": "https://svs.gsfc.nasa.gov/819/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "UARS Title Sequence",
            "description": "Title sequence for the UARS video, both with and without words. || Title sequence with words || a000819_w_title.00010_print.png (720x480) [349.3 KB] || a000819_pre.jpg (320x242) [3.9 KB] || a000819_w_title.webmhd.webm (960x540) [6.5 MB] || a000819_w_title.dv (720x480) [89.1 MB] || a000819_w_title.mp4 (640x480) [4.9 MB] || a000819.mpg (352x240) [2.8 MB] || ",
            "hits": 6
        },
        {
            "id": 820,
            "url": "https://svs.gsfc.nasa.gov/820/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "UARS 3D Wireframe",
            "description": "UARS wireframe model transitioning to a full image of the satellite || a000820.00005_print.png (720x480) [419.4 KB] || a000820_thm.png (80x40) [5.4 KB] || a000820_pre.jpg (320x242) [10.6 KB] || a000820_pre_searchweb.jpg (320x180) [57.4 KB] || a000820.webmhd.webm (960x540) [4.3 MB] || a000820.mp4 (640x480) [3.6 MB] || a000820.dv (720x480) [66.0 MB] || a000820.mpg (352x240) [1.9 MB] || ",
            "hits": 11
        },
        {
            "id": 821,
            "url": "https://svs.gsfc.nasa.gov/821/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "UARS Looking at the Limb",
            "description": "Beauty shot of UARS with the Earth passing beneath || a000821.00095_print.png (720x480) [447.2 KB] || a000821_thm.png (80x40) [5.3 KB] || a000821_pre.jpg (320x242) [7.7 KB] || a000821_pre_searchweb.jpg (320x180) [59.1 KB] || a000821.webmhd.webm (960x540) [5.3 MB] || a000821.mp4 (640x480) [3.8 MB] || a000821.dv (720x480) [70.6 MB] || a000821.mpg (352x240) [2.7 MB] || ",
            "hits": 65
        },
        {
            "id": 822,
            "url": "https://svs.gsfc.nasa.gov/822/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "UARS Flyover Fading to CHEM",
            "description": "A flyover of the Earth by UARS fades to the next generation of ozone-monitoring satellites, CHEM (now called Aura) || a000822.00005_print.png (720x480) [333.6 KB] || a000822_thm.png (80x40) [2.8 KB] || a000822_pre.jpg (320x242) [3.4 KB] || a000822_pre_searchweb.jpg (320x180) [18.7 KB] || a000822.webmhd.webm (960x540) [3.8 MB] || a000822.mp4 (640x480) [6.1 MB] || a000822.dv (720x480) [110.3 MB] || a000822.mpg (352x240) [4.2 MB] || ",
            "hits": 47
        },
        {
            "id": 823,
            "url": "https://svs.gsfc.nasa.gov/823/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Chemical Model Animation of O2 being Broken Up and Reforming as O3",
            "description": "Ozone is formed when high energy ultra-violet radiation from the sun breaks apart  molecular oxygen.  An oxygen atom then combines with an oxygen molecule producing a new molecule with three atoms of oxygen, ozone. || ",
            "hits": 479
        },
        {
            "id": 824,
            "url": "https://svs.gsfc.nasa.gov/824/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Chemical Model Animation of O3 Absorbing Low-energy UV",
            "description": "Ozone is  a strong absorber of lower energy ultraviolet radiation which can kill living organisms.  This radiation is absorbed by the ozone layer when it breaks the ozone bonds.  An oxygen atom is released, but the atom quickly re-combines with another oxygen molecule to regenerate ozone. || ",
            "hits": 344
        },
        {
            "id": 825,
            "url": "https://svs.gsfc.nasa.gov/825/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Chemical Model Animation of O3 Losing an Oxygen Atom to a Radical",
            "description": "Ozone is very reactive. It easily loses the third oxygen atom in the presence of other highly reactive compounds called radicals, which contain chlorine, hydrogen, nitrogen, or bromine.  Minute quantities of these radicals can cause large decreases in ozone because they  are not consumed in the reaction. This is called a catalytic cycle. || ",
            "hits": 193
        },
        {
            "id": 826,
            "url": "https://svs.gsfc.nasa.gov/826/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Chemical Model Animation of CFCs Releasing Chlorine to Form Reservoir Gases",
            "description": "Most stratospheric chlorine comes from man-made compounds called chlorofluorocarbons or CFCs.  CFCs, widely used in refrigerators and air conditioners, are quite harmless and non-reactive in the lower atmosphere.  Carried slowly upward by the earth's winds, they can survive the 5 year journey to the upper stratosphere. Here, above most of the ozone layer, the sun's ultraviolet radiation breaks down the CFCs into the more reactive chlorine compounds that destroy ozone.  Chlorine can react with methane to form hydrogen chloride.  Chlorine can also react with ozone forming the radical chlorine monoxide.  Chlorine monoxide then combines with the radical nitrogen dioxide to form stable chlorine nitrate. Chlorine nitrate and hydrogen chloride are called reservoir gases for the chlorine radical.  These reservoir gases usually contain more than ninety percent of the chlorine in the lower stratosphere. || ",
            "hits": 312
        },
        {
            "id": 827,
            "url": "https://svs.gsfc.nasa.gov/827/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Chemical Model Animation of Chlorine Release from Reservoir Gases over Antarctica",
            "description": "Over the Antarctic continent, ice clouds form in the  cold winter darkness.  On the surface of the cloud particles, chlorine nitrate and hydrogen chloride react and release chlorine.  The chlorine then reacts with ozone forming chlorine monoxide and starting the catalytic ozone destruction cycle.  The massive ozone loss results in the development of the Antarctic ozone hole. || ",
            "hits": 119
        },
        {
            "id": 828,
            "url": "https://svs.gsfc.nasa.gov/828/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Graph Showing Ozone Decreasing by 5% from 1979 to 1993",
            "description": "From 1979 to 1993, the average amount of ozone in the stratosphere has decreased by about 5%. || Graph of total ozone in the stratosphere from 1979 to 1993 || a000828.00010_print.png (720x480) [447.7 KB] || a000828_thm.png (80x40) [4.3 KB] || a000828_pre.jpg (320x242) [8.9 KB] || a000828_pre_searchweb.jpg (320x180) [49.9 KB] || a000828.webmhd.webm (960x540) [3.5 MB] || a000828.mp4 (640x480) [1.9 MB] || a000828.dv (720x480) [57.9 MB] || a000828.mpg (352x240) [2.0 MB] || ",
            "hits": 74
        },
        {
            "id": 829,
            "url": "https://svs.gsfc.nasa.gov/829/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "CLAES Measurements of CFC-12 in the Stratosphere",
            "description": "CLAES made the first global measurements of CFCs in the stratosphere.  CFCs enter the stratosphere through upwelling in the tropics.  The CFCs decrease with height as they are broken down by UV radiation.  CFCs are the major source of stratospheric chlorine.  Red indicates large amounts of CFC-12. || ",
            "hits": 95
        },
        {
            "id": 830,
            "url": "https://svs.gsfc.nasa.gov/830/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "HALOE Measurements of HCl in the Stratosphere (1992 - 1998)",
            "description": "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.  When UARS was first launched, measurements by HALOE showed that CFC byproducts were still increasing in the stratosphere.  But the newest HALOE measurements now show that CFC by-products are no longer increasing.   UARS has shown that the stratosphere is starting to respond to the international ban on CFC manufacture. || ",
            "hits": 48
        },
        {
            "id": 831,
            "url": "https://svs.gsfc.nasa.gov/831/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Water Vapor Measurements from HALOE (1992-1997)",
            "description": "An animated graph showing HALOE measurements of the water vapor amounts in the upper stratosphere, illustrating that it takes about 5 years for CFCs to reach the upper atmosphere.  Tropical water vapor changes slowly with seasonal cycles.  These changes, shown here as thick bands, were found to slowly ascend. These measurements tell us how fast the CFCs and other pollutants rise into the stratosphere. || ",
            "hits": 51
        },
        {
            "id": 833,
            "url": "https://svs.gsfc.nasa.gov/833/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Sun Spot Number Compared with Solar UV from SUSIM (1991-1997)",
            "description": "An animated graph showing the eleven-year sun spot cycle, as shown by measurements of sun spot number. Following this graph, an animation compares sun spot number measurements for the 1990s with direct measurements of the change in solar ultraviolet irradiance from SUSIM. || ",
            "hits": 53
        },
        {
            "id": 834,
            "url": "https://svs.gsfc.nasa.gov/834/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Ozone Layer Shielding Our Planet",
            "description": "An animation showing the ozone layer shielding our planet from the sun's intense ultraviolet radiation.  Ozone absorbs nearly all of the biologically damaging UV radiation from the sun. || ",
            "hits": 171
        },
        {
            "id": 835,
            "url": "https://svs.gsfc.nasa.gov/835/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "TOMS Data Showing the Ozone Hole over Antarctica (8/20/92 - 10/19/92)",
            "description": "TOMS Ozone over Antarctica from 8-20-92 to 10-19-92.  The ozone hole is indicated in shades of blue.  The missing data region over the south pole is due to the inability of the TOMS instrument to measure data during the polar night. || a000835.00005_print.png (720x480) [514.0 KB] || a000835_thm.png (80x40) [5.2 KB] || a000835_pre.jpg (320x242) [9.4 KB] || a000835_pre_searchweb.jpg (320x180) [59.5 KB] || a000835.webmhd.webm (960x540) [4.2 MB] || a000835.dv (720x480) [82.6 MB] || a000835.mp4 (640x480) [4.2 MB] || a000835.mpg (352x240) [3.2 MB] || ",
            "hits": 82
        },
        {
            "id": 836,
            "url": "https://svs.gsfc.nasa.gov/836/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Stratospheric Ozone Transport in the Northern Hemisphere (2/19/92 - 3/19/92)",
            "description": "This animation, derived from both remote sensing measurements of ozone and a computational ozone transport model, illustrates the complexity of ozone transport in the stratosphere. || ",
            "hits": 56
        },
        {
            "id": 837,
            "url": "https://svs.gsfc.nasa.gov/837/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Ozone and Chlorine Monoxide over Antarctica from MLS (1/12/93 - 9/17/93)",
            "description": "The  Microwave Limb Sounder (MLS) measures microwave emission from ozone and chlorine monoxide, a major ozone destroying radical.  Right after UARS was launched, MLS began to measure large concentrations of chlorine monoxide over the south pole.  These dramatic images clearly showed the extent of the south polar ozone destruction and confirmed the connection between man-made chlorine and the formation to  the Antarctic ozone hole. Why is so much  chlorine monoxide found over the Antarctic?  UARS measurements have confirmed that CFCs enter the stratosphere in the tropics.  As they rise above the ozone layer, ultraviolet molecules release chlorine, which then can react with methane to form hydrogen chloride.  Chlorine can also react with ozone forming the radical chlorine monoxide.  Chlorine monoxide then combines with the radical nitrogen dioxide to form stable chlorine nitrate.  Chlorine nitrate and hydrogen chloride are called reservoir gases for the chlorine radical.  These reservoir gases usually contain more than ninety percent of the chlorine in the lower stratosphere. || ",
            "hits": 135
        },
        {
            "id": 838,
            "url": "https://svs.gsfc.nasa.gov/838/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Chlorine Nitrate over the Arctic from CLAES (2/12/93 - 3/16/93)",
            "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.  Chlorine nitrate has been measured by the Cryogen Limb Array Etalon Spectrometer, CLAES.  CLAES makes measurements by looking at infrared emission from cloud particles and trace gases.  CLAES measurements help to show that the polar stratospheric clouds which form in the cold Arctic stratosphere have converted most  of the chlorine nitrate into the radical chlorine monoxide. In 1992, UARS measurements showed conclusively that an an Arctic ozone hole is beginning to form. || ",
            "hits": 42
        },
        {
            "id": 839,
            "url": "https://svs.gsfc.nasa.gov/839/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Chlorine Nitrate from CLAES and Chlorine Monoxide from MLS over the Arctic (2/12/93 - 3/10/93)",
            "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. Chlorine nitrate has been measured by CLAES and chlorine monoxide by MLS. The CLAES and MLS measurements together help to show that the polar stratospheric clouds which form in the cold Arctic stratosphere have converted most of the chlorine nitrate into the radical chlorine monoxide. In 1992, UARS measurements showed conclusively that an an Arctic ozone hole is beginning to form. || ",
            "hits": 62
        },
        {
            "id": 840,
            "url": "https://svs.gsfc.nasa.gov/840/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Various Film Clips from the UARS Video",
            "description": "A series of B-roll film clips used as source material for the UARS video (SVS animation 579). || a000840.00090_print.png (720x480) [465.3 KB] || a000840_pre.jpg (320x238) [13.8 KB] || a000840_thm.png (80x40) [6.9 KB] || a000840_pre_searchweb.jpg (320x180) [88.0 KB] || a000840.webmhd.webm (960x540) [159.9 MB] || a000840.dv (720x480) [2.1 GB] || a000840.mp4 (640x480) [122.1 MB] || ",
            "hits": 47
        },
        {
            "id": 841,
            "url": "https://svs.gsfc.nasa.gov/841/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "UARS Video Credits",
            "description": "Credits for the UARS video || a000841.00080_print.png (720x480) [525.9 KB] || a000841_thm.png (80x40) [4.9 KB] || a000841_pre.jpg (320x242) [8.3 KB] || a000841_pre_searchweb.jpg (320x180) [58.9 KB] || a000841.webmhd.webm (960x540) [23.6 MB] || a000841.dv (720x480) [329.7 MB] || a000841.mp4 (640x480) [18.0 MB] || a000841.mpg (352x240) [12.4 MB] || ",
            "hits": 25
        },
        {
            "id": 842,
            "url": "https://svs.gsfc.nasa.gov/842/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "UARS Voice Over",
            "description": "This entry represents the narration track for the UARS video (SVS animation 579).  This item is not available separately. || a000842_pre.jpg (320x238) [13.8 KB] || a000842_thm.png (80x40) [6.9 KB] || a000842_pre_searchweb.jpg (320x180) [88.0 KB] || Video slate image reads, \"The Upper Atmosphere Research SatelliteUARS Voice Over01:54:26:22 to 02:07:58:13\". || a000842_slate.jpg (720x528) [120.7 KB] || a000842_slate_web.png (320x234) [106.1 KB] || ",
            "hits": 6
        },
        {
            "id": 843,
            "url": "https://svs.gsfc.nasa.gov/843/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "UARS Soundtrack",
            "description": "This entry represents the music track for the UARS video. || The music track for the UARS video is not available separately.  This track is available as part of the full video as animation 579. || a000843_pre.jpg (320x242) [8.3 KB] || a000843_thm.png (80x40) [4.9 KB] || a000843_pre_searchweb.jpg (320x180) [58.9 KB] || ",
            "hits": 6
        },
        {
            "id": 1378,
            "url": "https://svs.gsfc.nasa.gov/1378/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Energetic Particle Flux over the Arctic from PEM (11/9/91)",
            "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": 10
        },
        {
            "id": 1379,
            "url": "https://svs.gsfc.nasa.gov/1379/",
            "result_type": "Visualization",
            "release_date": "1999-04-09T12:00:00-04:00",
            "title": "Graph Showing Antarctic Ozone Decreasing by 60% from the 1950s to the 1980s",
            "description": "During the spring of 1985, British researchers using ground-based instruments measured dramatic changes in the ozone layer. As much as sixty percent of the ozone over Antarctica was rapidly disappearing each spring. || ",
            "hits": 62
        }
    ]
}