{
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    "results": [
        {
            "id": 31059,
            "url": "https://svs.gsfc.nasa.gov/31059/",
            "result_type": "Hyperwall Visual",
            "release_date": "2019-11-13T00:00:00-05:00",
            "title": "CERES top of Atmosphere Fluxes",
            "description": "These maps show monthly top of atmosphere radiative fluxes from March 2000 to the present from the Energy Balanced and Filled (EBAF) data product. These data are produced by averaging observations collected by the Clouds and the Earth's Radiant Energy System (CERES) sensors on NASA's Aqua and Terra satellites, filling in gaps and constraining the fluxes to remove the inconsistency between average global net TOA flux and heat storage in the Earth-atmosphere system. || ",
            "hits": 335
        },
        {
            "id": 30604,
            "url": "https://svs.gsfc.nasa.gov/30604/",
            "result_type": "Hyperwall Visual",
            "release_date": "2015-06-28T00:00:00-04:00",
            "title": "CERES Radiation Fluxes",
            "description": "These maps show monthly reflected-shortwave radiation from March 2000 to the present from the Energy Balanced and Filled (EBAF) data product. These data are produced by averaging observations collected by the Clouds and the Earth's Radiant Energy System (CERES) sensors on NASA's Aqua and Terra satellites, filling in gaps and constraining the fluxes to remove the inconsistency between average global net TOA flux and heat storage in the Earth-atmosphere system. || ",
            "hits": 775
        },
        {
            "id": 3176,
            "url": "https://svs.gsfc.nasa.gov/3176/",
            "result_type": "Visualization",
            "release_date": "2005-06-21T00:00:00-04:00",
            "title": "Outgoing Longwave Flux Compared to Clouds (WMS)",
            "description": "The Earth's climate is determined by energy transfer from the sun to the Earth's land, oceans, and atmosphere. As the Earth rotates, the sun lights up only part of the Earth at a time, and some of that incoming solar energy is reflected and some is absorbed, depending on type of area it lights. The amount of reflection and absorption is critical to the climate. An instrument named CERES orbits the Earth every 99 minutes and measures the reflected solar energy. This animation shows the outgoing thermal radiation measured by CERES during 29 orbits on June 20 and 21 of 2003 over global infrared cloud images. Thermal radiation is longwave radiation and depends on the temperature of the earth, with the most intense radiation coming from the warmest regions and the least from cold clouds in the atmosphere. Although cold clouds and the cold Antarctic night regions can be seen in this data, the Earth radiates pretty uniformly in the longwave bands because the atmosphere distributes the heat of the sun to the whole planet. || ",
            "hits": 42
        },
        {
            "id": 3091,
            "url": "https://svs.gsfc.nasa.gov/3091/",
            "result_type": "Visualization",
            "release_date": "2005-02-01T12:00:00-05:00",
            "title": "Average Clear-sky Outgoing Longwave Flux (WMS)",
            "description": "The Earth's climate is determined by energy transfer from the sun to the Earth's land, oceans, and atmosphere.  As the Earth rotates, the sun lights up only part of the Earth at a time, and some of that incoming solar energy is reflected and some is absorbed, depending on type of area it lights.  The average amount of reflection and absorption is critical to the climate, because the absorbed energy heats up the Earth until it is radiated away as thermal radiation.   This animation shows the monthly average clear-sky outgoing longwave radiation from July, 2002 through June, 2004 as measured by the CERES instrument.  This is the thermal radiation given off by the warm Earth when the sky is cloud free.  The Earth's rotation and the movement of warm air from the equator to the poles make the Earth roughly uniformin temperature.  The most visible features are the cold poles in winter and the significant regions of snow coverage in the northern hemisphere, also in winter. || ",
            "hits": 27
        },
        {
            "id": 3092,
            "url": "https://svs.gsfc.nasa.gov/3092/",
            "result_type": "Visualization",
            "release_date": "2005-02-01T12:00:00-05:00",
            "title": "Average Total-sky Outgoing Longwave Flux (WMS)",
            "description": "The Earth's climate is determined by energy transfer from the sun to the Earth's land, oceans, and atmosphere.  As the Earth rotates, the sun lights up only part of the Earth at a time, and some of that incoming solar energy is reflected and some is absorbed, depending on type of area it lights.  The average amount of reflection and absorption is critical to the climate, because the absorbed energy heats up the Earth until it is radiated away as thermal radiation.  This animation shows the monthly average outgoing longwave radiation from July, 2002 through June, 2004 as measured by the CERES instrument.  This is the thermal radiation given off by the warm Earth.  The Earth's rotation and the movement of warm air from the equator to the poles make the Earth roughly  uniform in temperature.  The most visible features are the cold poles in winter and the cold clouds along the equator which trap the outgoing thermal radiation. || ",
            "hits": 42
        },
        {
            "id": 3107,
            "url": "https://svs.gsfc.nasa.gov/3107/",
            "result_type": "Visualization",
            "release_date": "2005-02-01T12:00:00-05:00",
            "title": "Instantaneous Outgoing Longwave Flux (WMS)",
            "description": "The Earth's climate is determined by energy transfer from the sun to the Earth's land, oceans, and atmosphere.  As the Earth rotates, the sun lights up only part of the Earth at a time, and some of that incoming solar energy is reflected and some is absorbed, depending on type of area it lights. The amount of reflection and absorption is critical to the climate.  An instrument named CERES orbits the Earth every 99 minutes and measures the reflected solar energy.  This animation shows the outgoing thermal radiation measured by CERES during 29 orbits on June 20 and 21 of 2003.  Thermal radiation is longwave radiation and depends on the temperature of the earth, with the most intense radiation coming from the warmest regions and the least from cold clouds in the atmosphere.  Although cold clouds and the cold Antarctic night regions can be seen in this data, the Earth radiates pretty uniformly in the longwave bands because the atmosphere distributes the heat of the sun to the whole planet. || ",
            "hits": 6
        },
        {
            "id": 2328,
            "url": "https://svs.gsfc.nasa.gov/2328/",
            "result_type": "Visualization",
            "release_date": "2001-12-12T12:00:00-05:00",
            "title": "Terra/CERES View of the Earth",
            "description": "Data sets from the Terra/CERES instrument || Outgoing Longwave Radiation (Average May 11-25, 2000) || ceres_olr_20010511_25_avg.jpg (1800x1098) [414.4 KB] || ceres_olr_20010511_25_avg_web.jpg (320x195) [12.7 KB] || ceres_olr_20010511_25_avg_thm.png (80x40) [5.5 KB] || ceres_olr_20010511_25_avg_web_searchweb.jpg (320x180) [89.5 KB] || ceres_olr_20010511_25_avg.tif (1800x1098) [941.4 KB] || ",
            "hits": 14
        },
        {
            "id": 1139,
            "url": "https://svs.gsfc.nasa.gov/1139/",
            "result_type": "Visualization",
            "release_date": "2000-04-19T12:00:00-04:00",
            "title": "Global Longwave from CERES",
            "description": "CERES stands for Clouds and the Earth's Radiant Energy System.  More information about CERES can be found at (http://terra.nasa.gov/Brochure/Sect_4-3.html) and (http://ceres.larc.nasa.gov/ceres_brochure.php). || ",
            "hits": 10
        },
        {
            "id": 1140,
            "url": "https://svs.gsfc.nasa.gov/1140/",
            "result_type": "Visualization",
            "release_date": "2000-04-19T12:00:00-04:00",
            "title": "Longwave Radiation from CERES Unwrapped",
            "description": "CERES stands for Clouds and the Earth's Radiant Energy System. More information about CERES can be found at (http://terra.nasa.gov/Brochure/Sect_4-3.html) and (http://ceres.larc.nasa.gov/ceres_brochure.php). || ",
            "hits": 6
        },
        {
            "id": 1022,
            "url": "https://svs.gsfc.nasa.gov/1022/",
            "result_type": "Visualization",
            "release_date": "1999-11-10T12:00:00-05:00",
            "title": "Single Globe Radiant Energy Dataset",
            "description": "Movie of time-variation of longwave radiation on a rotating globe. || a001022.00005_print.png (720x480) [375.2 KB] || a001022_thm.png (80x40) [3.2 KB] || a001022_pre.jpg (320x242) [4.8 KB] || a001022_pre_searchweb.jpg (320x180) [35.6 KB] || a001022.webmhd.webm (960x540) [4.6 MB] || a001022.dv (720x480) [186.7 MB] || a001022.mpg (352x240) [7.2 MB] || ",
            "hits": 16
        },
        {
            "id": 1296,
            "url": "https://svs.gsfc.nasa.gov/1296/",
            "result_type": "Visualization",
            "release_date": "1996-08-10T12:00:00-04:00",
            "title": "HoloGlobe: Outgoing Longwave Radiation for 1988 on a Globe",
            "description": "This is one of a series of animations that were produced to be part of the narrated video shown in the HoloGlobe exhibit at the Smithsonian Museum of Natural History and the Earth Today exhibit at the Smithsonian Air and Space Museum.  This particular animation was not used in the final video. || ",
            "hits": 21
        },
        {
            "id": 1297,
            "url": "https://svs.gsfc.nasa.gov/1297/",
            "result_type": "Visualization",
            "release_date": "1996-08-10T12:00:00-04:00",
            "title": "HoloGlobe: Outgoing Longwave Radiation for 1988 on a Globe (with Dates)",
            "description": "This is one of a series of animations that were produced to be part of the narrated video shown in the HoloGlobe exhibit at the Smithsonian Museum of Natural History and the Earth Today exhibit at the Smithsonian Air and Space Museum.  This particular animation was not used in the final video. || ",
            "hits": 7
        },
        {
            "id": 1298,
            "url": "https://svs.gsfc.nasa.gov/1298/",
            "result_type": "Visualization",
            "release_date": "1996-08-10T12:00:00-04:00",
            "title": "HoloGlobe: Outgoing Longwave Radiation for 1988 on a Flat Earth",
            "description": "This is one of a series of animations that were produced to be part of the narrated video shown in the HoloGlobe exhibit at the Smithsonian Museum of Natural History and the Earth Today exhibit at the Smithsonian Air and Space Museum.  This particular animation was not used in the final video. || ",
            "hits": 16
        },
        {
            "id": 1299,
            "url": "https://svs.gsfc.nasa.gov/1299/",
            "result_type": "Visualization",
            "release_date": "1996-08-10T12:00:00-04:00",
            "title": "HoloGlobe: Outgoing Longwave Radiation for 1988 on a Flat Earth (with Dates)",
            "description": "This is one of a series of animations that were produced to be part of the narrated video shown in the HoloGlobe exhibit at the Smithsonian Museum of Natural History and the Earth Today exhibit at the Smithsonian Air and Space Museum.  This particular animation was not used in the final video. || ",
            "hits": 50
        }
    ]
}