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    "results": [
        {
            "id": 3175,
            "url": "https://svs.gsfc.nasa.gov/3175/",
            "result_type": "Visualization",
            "release_date": "2005-06-21T00:00:00-04:00",
            "title": "Outgoing Shortwave 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 reflected solar radiation measured by CERES during 29 orbits on June 20 and 21 of 2003 over infrared cloud images for the same period. Reflected solar radiation is shortwave radiation, and the most intense reflection comes from clouds. || ",
            "hits": 12
        },
        {
            "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": 20
        },
        {
            "id": 3177,
            "url": "https://svs.gsfc.nasa.gov/3177/",
            "result_type": "Visualization",
            "release_date": "2005-06-21T00:00:00-04:00",
            "title": "Net Radiation 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 net radiation flux within view of CERES during 29 orbits on June 20 and 21 of 2003. The net flux is the incoming solar flux minus the outgoing reflected (shortwave) and thermal (longwave) radiation. If the flux in a region is positive, the Earth is being warmed by the sun in that region, while cooling regions have a negative flux. It is clear from the animation that the most intensive heating occurs in ocean regions with few clouds, while the second most intense are cloud-free regions over vegetated land areas. Deserts, cloudy regions, and ice caps all reflect enough solar radiation to reduce the amount of heating. Regions of night are, of course, cooling regions because there is no incoming flux at all. || ",
            "hits": 55
        },
        {
            "id": 3178,
            "url": "https://svs.gsfc.nasa.gov/3178/",
            "result_type": "Visualization",
            "release_date": "2005-06-21T00:00:00-04:00",
            "title": "Incoming Solar 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 incoming solar radiation within view of CERES during 29 orbits on June 20 and 21 of 2003. Because this is incoming solar flux, its magnitude only depends on the position of the sun, and, because the orbit is synchronized with the sun, the orbit crosses the equator in the daylight at about 1:30 PM local time on every orbit. This data is not actually measured from CERES, but is calculated to compare with the outgoing radiation that CERES does measure. Note that the infrared cloud image shown under the solar data shows high infrared as dark (land) and low infrared as light (clouds). || ",
            "hits": 26
        },
        {
            "id": 3179,
            "url": "https://svs.gsfc.nasa.gov/3179/",
            "result_type": "Visualization",
            "release_date": "2005-06-21T00:00:00-04:00",
            "title": "Scene Identification 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 scene identification as measured by CERES during 29 orbits on June 20 and 21 of 2003. By comparing the incoming solar radiation with the outgoing reflected and thermal radiation, it is possible to identify the type of area being viewed, whether it be land, clouds, ocean, or ice. This scene identification is used together with the radiation flux measurements to build up a complete picture of the Earth's energy budget over time. || ",
            "hits": 18
        },
        {
            "id": 3089,
            "url": "https://svs.gsfc.nasa.gov/3089/",
            "result_type": "Visualization",
            "release_date": "2005-02-01T12:00:00-05:00",
            "title": "Average Clear-sky Albedo (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 albedo from July, 2002 through June, 2004 as measured by the CERES instrument. This is the fraction of the incoming solar radiation that is reflected back into space by regions of the Earth on cloud-free days. The regions of highest albedo are regions of snow and ice, followed by desert regions. Oceans have the lowest albedo, and reflect very little of the incoming solar radiation. It is not possible to measure the albedo during the winter months at the poles, since there is no incoming solar radiation during these times. || ",
            "hits": 37
        },
        {
            "id": 3090,
            "url": "https://svs.gsfc.nasa.gov/3090/",
            "result_type": "Visualization",
            "release_date": "2005-02-01T12:00:00-05:00",
            "title": "Average Total-sky Albedo (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 albedo from July, 2002 through June, 2004 as measured by the CERES instrument.  This is the fraction of the incoming solar radiation that is reflected back into space by regions of the Earth.  The regions of highest albedo are regions of snow and ice, followed by desert regions and regions where there is significant cloud cover during the year.  Oceans have the lowest albedo.  It is not possible to measure the albedo during the winter months at the poles, since there is no incoming solar radiation during these times. || ",
            "hits": 78
        },
        {
            "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": 20
        },
        {
            "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": 30
        },
        {
            "id": 3093,
            "url": "https://svs.gsfc.nasa.gov/3093/",
            "result_type": "Visualization",
            "release_date": "2005-02-01T12:00:00-05:00",
            "title": "Average Clear-sky Net Radiant 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 clear-sky average net radiant flux from July, 2002 through June, 2004 as measured by the CERES instrument.  This is  the incoming radiation minus the outgoing reflected or thermal energy given off by areas of the Earth when the sky is cloud-free.  Regions in red and yellow have a net incoming flux and are being heated.  Regions in blue have a net outgoing flux and are being cooled.  Regions in black are in rough equilibrium.  Summertime oceans are heated the most, while high latitude winter regions are cooled the most, probably because of the longer winter nights.  Note that the Earth's ice sheets are almost always regions of  cooling.  On average, the heating and cooling amounts must balance, or the Earth will change temperature and the climate will change. || ",
            "hits": 15
        },
        {
            "id": 3094,
            "url": "https://svs.gsfc.nasa.gov/3094/",
            "result_type": "Visualization",
            "release_date": "2005-02-01T12:00:00-05:00",
            "title": "Average Total-sky Net Radiant 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 net radiant flux from July, 2002 through June, 2004 as measured by the CERES instrument.  This is the incoming radiation minus the outgoing reflected or thermal energy given off by areas of the Earth.  Regions in red and yellow have a net incoming flux and are being heated. Regions in blue have a net outgoing flux and are being cooled.  Regions in black are in rough equilibrium.  Cloud-free summertime oceans are heated the most, while high latitude winter regions are cooled the most, probably because of the longer winter nights.  Note that regions that reflect a lot of sunlight, such as the polar ice sheets and the Sahara desert are almost always in equilibrium or are cooling regions. || ",
            "hits": 16
        },
        {
            "id": 3095,
            "url": "https://svs.gsfc.nasa.gov/3095/",
            "result_type": "Visualization",
            "release_date": "2005-02-01T12:00:00-05:00",
            "title": "Average Total-sky Incoming Solar 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 incoming solar radiation from July, 2002 through June, 2004 as measured by the CERES instrument. This average data set is constant in longitude because of the Earth's rotation, but clearly shows the seasonal cycle as the sun heats the Northern Hemisphere more in summer than in winter. Note that the polar regions are abnormally bright in the local summer and dark in the local winter because whole day is either light or dark in those seasons. || ",
            "hits": 35
        },
        {
            "id": 3096,
            "url": "https://svs.gsfc.nasa.gov/3096/",
            "result_type": "Visualization",
            "release_date": "2005-02-01T12:00:00-05:00",
            "title": "Average Clear-sky Outgoing Shortwave 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 shortwave radiation from July, 2002 through June, 2004 as measured by the CERES instrument.  This is the sunlight that is directly reflected back into space by ice, desert, and other physical areas on the Earth when the sky is cloud-free.  The ice sheets can be clearly seen to reflect the most sunlight, with desert areas next.  Oceans absorb the most sunlight, more than the vegetated land areas such as the tropical rain forest and temperate forests and plains. || ",
            "hits": 13
        },
        {
            "id": 3097,
            "url": "https://svs.gsfc.nasa.gov/3097/",
            "result_type": "Visualization",
            "release_date": "2005-02-01T12:00:00-05:00",
            "title": "Average Total-sky Outgoing Shortwave 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 shortwave radiation from July, 2002 through June, 2004 as measured by the CERES instrument.  This is the sunlight that is directly reflected back into space by clouds, ice, desert, and other physical areas on the Earth.  Although clouds are very reflective, they come and going during the month, so more reflection is seen on average from ice sheets, which change very little during a monthly period.  Note that the cloud-free parts of the ocean are relatively dark, indicating that oceans absorb more sunlight than they reflect. || ",
            "hits": 11
        },
        {
            "id": 3104,
            "url": "https://svs.gsfc.nasa.gov/3104/",
            "result_type": "Visualization",
            "release_date": "2005-02-01T12:00:00-05:00",
            "title": "Instantaneous Scene Identification (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 th e climate. An instrument named CERES orbits the Earth every 99 minutes and measures the reflected solar energy. This animation shows the scene identification as measured by CERES during 29 orbits on June 20 and 21 of 2003. By comparing the incoming solar radiation with the outgoing reflected and thermal radiation, it is possible to identify the type of area being viewed, whether it be land, clouds, ocean, or ice. This scene identification is used together with the radiation flux measurements to build up a complete picture of the Earth's energy budget over time. || ",
            "hits": 21
        },
        {
            "id": 3105,
            "url": "https://svs.gsfc.nasa.gov/3105/",
            "result_type": "Visualization",
            "release_date": "2005-02-01T12:00:00-05:00",
            "title": "Instantaneous Incoming Solar 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 incoming solar radiation within view of CERES during 29 orbits on June 20 and 21 of 2003. Because this is incoming solar flux, its magnitude only depends on the position of the sun, and, because the orbit is synchronized with the sun, the orbit crosses the equator in the daylight at about 1:30 PM local time on every orbit. This data is not actually measured from CERES, but is calculated to compare with the outgoing radiation that CERES does measure. || ",
            "hits": 65
        },
        {
            "id": 3106,
            "url": "https://svs.gsfc.nasa.gov/3106/",
            "result_type": "Visualization",
            "release_date": "2005-02-01T12:00:00-05:00",
            "title": "Instantaneous Net Radiation 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 net radiation flux within view of CERES during 29 orbits on June 20 and 21 of 2003. The net flux is the incoming solar flux minus the outgoing reflected (shortwave) and thermal (longwave) radiation. If the flux in a region is positive, the Earth is being warmed by the sun in that region, while cooling regions have a negative flux. It is clear from the animation that the most intensive heating occurs in ocean regions with few clouds, while the second most intense are cloud-free regions over vegetated land areas. Deserts, cloudy regions, and ice caps all reflect enough solar radiation to reduce the amount of heating. Regions of night are, of course, cooling regions because there is no incoming flux at all. || ",
            "hits": 30
        },
        {
            "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": 14
        },
        {
            "id": 3108,
            "url": "https://svs.gsfc.nasa.gov/3108/",
            "result_type": "Visualization",
            "release_date": "2005-02-01T12:00:00-05:00",
            "title": "Instantaneous Outgoing Shortwave 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 reflected solar radiation measured by CERES during 29 orbits on June 20 and 21 of 2003.  Reflected solar radiation is shortwave radiation, and the most intense reflection comes from clouds, followed by ice.  Land reflects only a small amount of radiation, but ocean reflects the least, which is the reason that the sun heats the oceans so effectively.  Of course, there is no reflected solar radiation in regions of night. || ",
            "hits": 27
        },
        {
            "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": 12
        },
        {
            "id": 2156,
            "url": "https://svs.gsfc.nasa.gov/2156/",
            "result_type": "Visualization",
            "release_date": "2001-06-20T12:00:00-04:00",
            "title": "One Year of Terra/CERES Data (Reflected Solar Radiation) Daily Data",
            "description": "This animation displays a little over one year of Terra/CERES data (March 1, 2000 to May 25, 2001) at one day resolution. The data are 2.5 degree resolution. The band is reflected solar radiation (often referred to as 'shortwave' in the literature). Bright areas correspond to cloud tops or snowcover. || ",
            "hits": 12
        },
        {
            "id": 2157,
            "url": "https://svs.gsfc.nasa.gov/2157/",
            "result_type": "Visualization",
            "release_date": "2001-06-20T12:00:00-04:00",
            "title": "One Year of Terra/CERES Data (Outgoing Longwave Radiation) Daily Data",
            "description": "This animation displays one year of Outgoing Longwave Radiation (OLR) Terra/CERES data (March 1, 2000 to May 25, 2001) at one day resolution. The data are 2.5 degree resolution. || Movie at one frame per day of Terra-CERES OLR data. || a002157.00005_print.png (720x480) [513.3 KB] || a002157_pre.jpg (320x242) [10.1 KB] || a002157.webmhd.webm (960x540) [22.4 MB] || a002157.dv (720x480) [432.9 MB] || a002157.mpg (352x240) [16.4 MB] || ",
            "hits": 17
        },
        {
            "id": 2158,
            "url": "https://svs.gsfc.nasa.gov/2158/",
            "result_type": "Visualization",
            "release_date": "2001-06-20T12:00:00-04:00",
            "title": "14-Day Boxcar Averaged Terra/CERES (Reflected Solar Radiation)",
            "description": "This animation displays one year of Reflected Solar Radiation (RSR) Terra/CERES data (March 1, 2000 to May 25, 2001) with a 14-day boxcar average. Endpoints have the average re-weighted for the smaller amount of data. The data are 2.5 degree resolution. || ",
            "hits": 5
        },
        {
            "id": 2159,
            "url": "https://svs.gsfc.nasa.gov/2159/",
            "result_type": "Visualization",
            "release_date": "2001-06-20T12:00:00-04:00",
            "title": "14-Day Boxcar Averaged Terra/CERES Data (Outgoing Longwave Radiation)",
            "description": "This animation displays one year of Outgoing Longwave Radiation (OLR) Terra/CERES data (March 1, 2000 to May 25, 2001) with a 14-day boxcar average. Endpoints have the average re-weighted for the smaller amount of data. The data are 2.5 degree resolution. || ",
            "hits": 5
        },
        {
            "id": 2167,
            "url": "https://svs.gsfc.nasa.gov/2167/",
            "result_type": "Visualization",
            "release_date": "2001-06-20T12:00:00-04:00",
            "title": "Terra/CERES on the American Southwest: May 2001",
            "description": "Terra/CERES views the American southwest during the heatwave of May 2001.  The animation is generated for outgoing longwave radiation (heat). || Movie of the American Southwest during a heatwave.  April-May 2001. || a002167.00005_print.png (720x480) [580.5 KB] || a002167_pre.jpg (320x242) [8.7 KB] || a002167.webmhd.webm (960x540) [1.9 MB] || a002167.dv (720x480) [55.5 MB] || a002167.mpg (352x240) [1.9 MB] || ",
            "hits": 5
        },
        {
            "id": 2168,
            "url": "https://svs.gsfc.nasa.gov/2168/",
            "result_type": "Visualization",
            "release_date": "2001-06-20T12:00:00-04:00",
            "title": "Terra/CERES Views the Americas in Reflected Solar Radiation - Daily Data",
            "description": "Terra/CERES views the Americas in Reflected Solar Radiation (March 1, 2000 to May 25, 2001). These are daily data. || Movie of the Americas in RSR - daily data. || a002168.00005_print.png (720x480) [623.8 KB] || a002168_pre.jpg (320x242) [11.4 KB] || a002168.webmhd.webm (960x540) [31.6 MB] || a002168.dv (720x480) [432.9 MB] || a002168.mpg (352x240) [16.6 MB] || ",
            "hits": 6
        },
        {
            "id": 2169,
            "url": "https://svs.gsfc.nasa.gov/2169/",
            "result_type": "Visualization",
            "release_date": "2001-06-20T12:00:00-04:00",
            "title": "Terra/CERES Views the Americas in Outgoing Longwave Radiation - Daily Data",
            "description": "Terra/CERES views the Americas in Outgoing Longwave Radiation (March 1, 2000 to May 25, 2001). These are daily data. || Movie of the Americas in OLR. || a002169.00005_print.png (720x480) [621.3 KB] || a002169_pre.jpg (320x242) [9.1 KB] || a002169.webmhd.webm (960x540) [22.3 MB] || a002169.dv (720x480) [432.7 MB] || a002169.mpg (352x240) [16.4 MB] || ",
            "hits": 8
        },
        {
            "id": 2170,
            "url": "https://svs.gsfc.nasa.gov/2170/",
            "result_type": "Visualization",
            "release_date": "2001-06-20T12:00:00-04:00",
            "title": "Terra/CERES Outgoing Longwave and Reflected Solar Radiation: Boxcar Averaged",
            "description": "Terra/CERES views the world in outgoing longwave radiation (left) and reflected solar radiation (right). This is a 14-day boxcar averaged datas ets from March 1, 2001 to May 25, 2001. || Side-by-side Earth views of 14-day boxcar averaged OLR & RSR data. || a002170.00005_print.png (720x480) [424.9 KB] || a002170_pre.jpg (320x240) [7.0 KB] || a002170.webmhd.webm (960x540) [2.5 MB] || a002170.dv (720x480) [72.0 MB] || a002170.mpg (320x240) [2.1 MB] || ",
            "hits": 11
        },
        {
            "id": 2171,
            "url": "https://svs.gsfc.nasa.gov/2171/",
            "result_type": "Visualization",
            "release_date": "2001-06-20T12:00:00-04:00",
            "title": "Terra/CERES Outgoing Longwave and Reflected Solar Radiation: Daily Data",
            "description": "Terra/CERES views the world in outgoing longwave radiation (left) and reflected solar radiation (right). This is daily data from March 1, 2000 to May 25, 2001. || Synchronized, side-by-side views of the Earth in RSR & OLR. || a002171.00005_print.png (720x480) [451.5 KB] || a002171_pre.jpg (320x238) [7.8 KB] || a002171.webmhd.webm (960x540) [24.2 MB] || a002171.dv (720x480) [432.9 MB] || a002171.mpg (352x240) [16.4 MB] || ",
            "hits": 21
        },
        {
            "id": 2172,
            "url": "https://svs.gsfc.nasa.gov/2172/",
            "result_type": "Visualization",
            "release_date": "2001-06-20T12:00:00-04:00",
            "title": "Terra/CERES Views the World in Reflected Solar Radiation - Daily Data",
            "description": "Terra/CERES views the world in Reflected Solar Radiation. These are daily data from March 1, 2000 to May 25, 2001. || Movie of the Earth in RSR. || a002172.00005_print.png (720x480) [390.8 KB] || a002172_pre.jpg (320x242) [6.8 KB] || a002172.webmhd.webm (960x540) [23.9 MB] || a002172.dv (720x480) [433.0 MB] || a002172.mpg (352x240) [16.5 MB] || ",
            "hits": 26
        },
        {
            "id": 2173,
            "url": "https://svs.gsfc.nasa.gov/2173/",
            "result_type": "Visualization",
            "release_date": "2001-06-20T12:00:00-04:00",
            "title": "Terra/CERES Views the World in Outgoing Longwave Radiation - Daily data",
            "description": "Terra/CERES views the world in outgoing longwave radiation. These are daily data from March 1, 2000 to May 25, 2001. || Movie of daily OLR data on a spinning Earth. || a002173.00005_print.png (720x480) [430.1 KB] || a002173_pre.jpg (320x242) [6.6 KB] || a002173.webmhd.webm (960x540) [19.8 MB] || a002173.dv (720x480) [433.0 MB] || a002173.mpg (352x240) [16.5 MB] || ",
            "hits": 27
        },
        {
            "id": 2174,
            "url": "https://svs.gsfc.nasa.gov/2174/",
            "result_type": "Visualization",
            "release_date": "2001-06-20T12:00:00-04:00",
            "title": "Terra/CERES Views the Pakistan Heat Wave: May 2001",
            "description": "Terra/CERES views the Pakistan heat wave. || Movie of OLR changes in May 2001 near Pakistan. || a002174.00005_print.png (720x480) [630.4 KB] || a002174_pre.jpg (320x242) [9.8 KB] || a002174.webmhd.webm (960x540) [2.4 MB] || a002174.dv (720x480) [55.5 MB] || a002174.mpg (352x240) [1.5 MB] || May 5, 2001 || PakistanOLR3445.jpg (2560x1920) [420.0 KB] || PakistanOLR3445_web.jpg (320x240) [14.8 KB] || PakistanOLR3445.tif (2560x1920) [2.9 MB] || ",
            "hits": 12
        }
    ]
}