{ "count": 60, "next": null, "previous": null, "results": [ { "id": 4817, "url": "https://svs.gsfc.nasa.gov/4817/", "result_type": "Visualization", "release_date": "2020-04-17T00:00:00-04:00", "title": "Earth Day 2020: CERES Net TOA Radiation", "description": "CERES Net TOA Radiation, WIth LabelsThis video is also available on our YouTube channel. || ceres_w_labels.00001_print.jpg (1024x576) [98.8 KB] || ceres_w_labels.00001_searchweb.png (320x180) [51.5 KB] || ceres_w_labels.00001_thm.png (80x40) [4.4 KB] || ceres_w_labels.webm (1920x1080) [6.9 MB] || ceres_w_labels.mp4 (1920x1080) [111.3 MB] || captions_silent.29564.en_US.srt [43 bytes] || ceres_w_labels.mp4.hwshow [180 bytes] || ", "hits": 61 }, { "id": 13493, "url": "https://svs.gsfc.nasa.gov/13493/", "result_type": "Produced Video", "release_date": "2019-12-10T11:00:00-05:00", "title": "Terra Satellite 20-Year Anniversary Instruments and Applications", "description": "Music: “Blackbird” by Magnum Opus [ASCAP]; Atmosphere Music Ltd [PRS]; Volta Music; Universal Production Music || 13493_Terra_Applications_20Anniversary_FINAL.02146_print.jpg (1024x576) [230.0 KB] || 13493_Terra_Applications_20Anniversary_FINAL.02146_searchweb.png (320x180) [132.3 KB] || 13493_Terra_Applications_20Anniversary_FINAL.02146_thm.png (80x40) [8.0 KB] || 13493_Terra_Applications_20Anniversary_FINAL.mov (1920x1080) [4.1 GB] || 13493_Terra_Applications_20Anniversary_FINAL_VX-309499.webm (960x540) [73.2 MB] || 13493_Terra_Applications_20Anniversary_FINAL_VX-309499_lowres.mp4 (1280x720) [51.8 MB] || YOUTUBE_1080_13493_Terra_Applications_20Anniversary_FINAL_VX-309499_youtube_1080.mp4 (1920x1080) [269.9 MB] || YOUTUBE_720_13493_Terra_Applications_20Anniversary_FINAL_VX-309499_youtube_720.mp4 (1280x720) [272.1 MB] || 13493_Terra_Applications_20Anniversary_FINAL.en_US.srt [2.4 KB] || 13493_Terra_Applications_20Anniversary_FINAL.en_US.vtt [2.4 KB] || ", "hits": 36 }, { "id": 30781, "url": "https://svs.gsfc.nasa.gov/30781/", "result_type": "Hyperwall Visual", "release_date": "2017-05-31T00:00:00-04:00", "title": "The Earth Observing Fleet by Theme", "description": "The current Earth Observing Fleet with all satellites capturing data related to Sea Ice Cover highlighted, combined with key visualizations showing the significance of the data || fleet_data_precipitation_1080p.00001_print.jpg (1024x576) [227.2 KB] || fleet_data_precipitation_720p.mp4 (1280x720) [51.9 MB] || fleet_data_precipitation_1080p.webm (1920x1080) [3.7 MB] || fleet_data_precipitation_1080p.mp4 (1920x1080) [95.8 MB] || fleet_precipitation (4104x2304) [0 Item(s)] || fleet_data_precipitation_2304p.mp4 (4096x2304) [281.0 MB] || ", "hits": 52 }, { "id": 12346, "url": "https://svs.gsfc.nasa.gov/12346/", "result_type": "Produced Video", "release_date": "2016-09-01T14:00:00-04:00", "title": "NASA's Dawn Mission Finds Young Cryovolcano on Dwarf Planet Ceres", "description": "Analysis of images from NASA's Dawn mission reveals that dwarf planet Ceres hosts an unexpectedly young cryovolcano that formed with the past billion years.Read the full NASA.gov story here: http://www.nasa.gov/feature/goddard/2016/ceres-cryo-volcanoRead the full paper appearing Sep 2 in the journal Science here: [link to come]Read the AAAS news release here: eurekalert.org For more Ceres images and animations, visit the JPL Photojournal: photojournal.jpl.nasa.gov || ", "hits": 69 }, { "id": 30764, "url": "https://svs.gsfc.nasa.gov/30764/", "result_type": "Hyperwall Visual", "release_date": "2016-04-05T03:00:00-04:00", "title": "Dawn Images of Ceres", "description": "Occator Crater || image1.jpg (1722x1650) [758.0 KB] || ceres-images-of-dawn-occator-crater-russell-1.hwshow [281 bytes] || ", "hits": 98 }, { "id": 12140, "url": "https://svs.gsfc.nasa.gov/12140/", "result_type": "Produced Video", "release_date": "2016-02-02T14:00:00-05:00", "title": "NASA On Air: NASA's Imagery Shows Dwarf Planet Ceres (2/2/2016)", "description": "LEAD: A colorful new animation shows a simulated flight over the surface of dwarf planet Ceres, based on images from NASA's Dawn spacecraft.1. The movie shows Ceres in enhanced color, which helps to highlight subtle differences in the appearance of surface materials. Scientists believe areas with shades of blue contain younger, fresher material, including flows, pits and cracks.TAG: Ceres is the largest body in the main asteroid belt between Mars and Jupiter. It has a diameter of about 590 miles and is made up of ice and rock. || IPAD_DELIVERABLES_NASA_on_Air-CERES_iPad_1920x1080_print.jpg (1024x576) [137.7 KB] || IPAD_DELIVERABLES_NASA_on_Air-CERES_iPad_1920x1080_searchweb.png (320x180) [95.7 KB] || IPAD_DELIVERABLES_NASA_on_Air-CERES_iPad_1920x1080_thm.png (80x40) [6.3 KB] || WSI_WEATHER_CHANNEL_NASA_on_Air-CERES_1280x720.mov (1280x720) [546.9 MB] || WSI_WEATHER_CHANNEL_NASA_on_Air-CERES_1920x1080.mov (1920x1080) [487.4 MB] || NBC_TODAY_NASA_on_Air-CERES_NBC_Today.mov (1920x1080) [24.3 MB] || Weather-Channel_NASA_on_Air-CERES_WeatherChannel.wmv (1280x720) [6.0 MB] || Accuweather_NASA_on_Air-CERES_Accuweather.avi (1280x720) [4.8 MB] || BARON_SERVICE_NASA_on_Air-CERES_baron.mp4 (1920x1080) [15.7 MB] || WC_PRORES_422_NASA_on_Air-CERES_prores.mov (1920x1080) [341.1 MB] || IPAD_DELIVERABLES_NASA_on_Air-CERES_iPad_960x540.m4v (960x540) [18.6 MB] || IPAD_DELIVERABLES_NASA_on_Air-CERES_iPad_1280x720.m4v (1280x720) [35.0 MB] || IPAD_DELIVERABLES_NASA_on_Air-CERES_iPad_1920x1080.m4v (1920x1080) [56.1 MB] || WEBM_NASA_on_Air-CERES.webm (960x540) [9.6 MB] || ", "hits": 122 }, { "id": 30738, "url": "https://svs.gsfc.nasa.gov/30738/", "result_type": "Hyperwall Visual", "release_date": "2015-12-09T00:00:00-05:00", "title": "Dawn Takes a Closer Look at Occator", "description": "Occator crater on Ceres || PIA19889_print.jpg (1024x1024) [207.5 KB] || PIA19889_searchweb.png (320x180) [43.8 KB] || PIA19889_thm.png (80x40) [2.8 KB] || PIA19889.tif (1024x1024) [928.5 KB] || dawn_occator_crater_30738.key [3.5 MB] || dawn_occator_crater_30738.pptx [1016.0 KB] || dawn-takes-a-closer-look-at-occator.hwshow [275 bytes] || ", "hits": 65 }, { "id": 4245, "url": "https://svs.gsfc.nasa.gov/4245/", "result_type": "Visualization", "release_date": "2014-12-17T13:00:00-05:00", "title": "Link between Sea-Ice Fraction and Absorbed Solar Radiation over the Arctic Ocean", "description": "NASA satellite instruments have observed a marked increase in solar radiation absorbed in the Arctic since the year 2000 – a trend that aligns with the drastic decrease in Arctic sea ice during the same period. This visual shows the Arctic Sea Ice Change and the corresponding Absorbed Solar Radiation Change during June, July, and August from 2000 through 2014.This video is also available on our YouTube channel. || seaice_solarAbsorption_0344_print.jpg (1024x576) [117.1 KB] || SeaIceSolarAbsorptionChange.webm (1920x1080) [1.2 MB] || 1920x1080_16x9_60p (1920x1080) [0 Item(s)] || SeaIceSolarAbsorptionChange.mp4 (1920x1080) [12.1 MB] || composite (1920x1080) [0 Item(s)] || source (1920x1080) [0 Item(s)] || SeaIceSolarAbsorptionChange.m4v (640x360) [2.1 MB] || ", "hits": 68 }, { "id": 10893, "url": "https://svs.gsfc.nasa.gov/10893/", "result_type": "Produced Video", "release_date": "2012-01-12T11:00:00-05:00", "title": "Aqua Podcast Series", "description": "This page will soon feature six videos about the Aqua satellite mission, starting with an introductory video, followed by weekly additions of videos highlighting the AIRS, AMSR-E, MODIS, and CERES instruments, and concluding with a video featuring applications of Aqua data. || ", "hits": 26 }, { "id": 10514, "url": "https://svs.gsfc.nasa.gov/10514/", "result_type": "Produced Video", "release_date": "2009-12-11T18:00:00-05:00", "title": "Terra@10: Terra 10th Anniversary Video", "description": "The Earth-observing satellite Terra celebrates its tenth anniversary in 2009. This video highlights how Terra has helped us better understand our home planet. The satellite's five instruments - ASTER, CERES, MISR, MODIS and MOPITT - reveal how our our world is changing. For complete transcript, click here. || Terra10_ipodlarge.08402_print.jpg (1024x576) [38.3 KB] || Terra10_ipodlarge_web.png (320x180) [47.8 KB] || Terra10_ipodlarge_thm.png (80x40) [4.3 KB] || Terra10_Apple_TV.webmhd.webm (960x540) [71.4 MB] || Terra10_Youtube.mov (1280x720) [72.8 MB] || Terra10_Apple_TV.m4v (960x720) [179.0 MB] || Terra10_H.264.mov (1280x720) [146.6 MB] || Terra10_ipodlarge.m4v (640x360) [55.7 MB] || Terra10.mpg (512x288) [118.8 MB] || Terra10_ipodsmall.m4v (320x180) [24.0 MB] || Terra10.wmv (346x260) [18.2 MB] || ", "hits": 26 }, { "id": 3355, "url": "https://svs.gsfc.nasa.gov/3355/", "result_type": "Visualization", "release_date": "2006-05-20T23:55:00-04:00", "title": "A Short Tour of the Cryosphere", "description": "A newer version of this animation is available here.This narrated, 5-minute animation shows a wealth of data collected from satellite observations of the cryosphere and the impact that recent cryospheric changes are making on our planet. This is a shorter version of a narrated, 7 1/2 minute animation entitled 'A Tour of the Cryosphere'.See the above link for a detailed description of the full animation.Two sections have been removed from the original animation: one showing a flyby of the South Pole station and glaciers feeding the Ross Ice Shelf and one showing solar data related to the Earth's energy balance.For more information on the data sets used in this visualization, visit NASA's EOS DAAC website. || ", "hits": 26 }, { "id": 3181, "url": "https://svs.gsfc.nasa.gov/3181/", "result_type": "Visualization", "release_date": "2005-12-04T23:55:00-05:00", "title": "A Tour of the Cryosphere", "description": "A new HD version of this animation is available here.Click here to go to the media download section.The cryosphere consists of those parts of the Earth's surface where water is found in solid form, including areas of snow, sea ice, glaciers, permafrost, ice sheets, and icebergs. In these regions, surface temperatures remain below freezing for a portion of each year. Since ice and snow exist relatively close to their melting point, they frequently change from solid to liquid and back again due to fluctuations in surface temperature. Although direct measurements of the cryosphere can be difficult to obtain due to the remote locations of many of these areas, using satellite observations scientists monitor changes in the global and regional climate by observing how regions of the Earth's cryosphere shrink and expand.This animation portrays fluctuations in the cryosphere through observations collected from a variety of satellite-based sensors. The animation begins in Antarctica, showing ice thickness ranging from 2.7 to 4.8 kilometers thick along with swaths of polar stratospheric clouds. In a tour of this frozen continent, the animation shows some unique features of the Antarctic landscape found nowhere else on earth. Ice shelves, ice streams, glaciers, and the formation of massive icebergs can be seen. A time series shows the movement of iceberg B15A, an iceberg 295 kilometers in length which broke off of the Ross Ice Shelf in 2000. Moving farther along the coastline, a time series of the Larsen ice shelf shows the collapse of over 3,200 square kilometers ice since January 2002. As we depart from the Antarctic, we see the seasonal change of sea ice and how it nearly doubles the size of the continent during the winter.From Antarctica, the animation travels over South America showing areas of permafrost over this mostly tropical continent. We then move further north to observe daily changes in snow cover over the North American continent. The clouds show winter storms moving across the United States and Canada, leaving trails of snow cover behind. In a close-up view of the western US, we compare the difference in land cover between two years: 2003 when the region received a normal amount of snow and 2002 when little snow was accumulated. The difference in the surrounding vegetation due to the lack of spring melt water from the mountain snow pack is evident.As the animation moves from the western US to the Arctic region, the areas effected by permafrost are visible. In December, we see how the incoming solar radiation primarily heats the Southern Hemisphere. As time marches forward from December to June, the daily snow and sea ice recede as the incoming solar radiation moves northward to warm the Northern Hemisphere.Using satellite swaths that wrap the globe, the animation shows three types of instantaneous measurements of solar radiation observed on June 20, 2003: shortwave (reflected) radiation, longwave (thermal) radiation and net flux (showing areas of heating and cooling). Correlation between reflected radiation and clouds are evident. When the animation fades to show the monthly global average net flux, we see that the polar regions serve to cool the global climate by radiating solar energy back into space throughout the year.The animation shows a one-year cycle of the monthly average Arctic sea ice concentration followed by the mean September minimum sea ice for each year from 1979 through 2004. A red outline indicates the mean sea ice extent for September over 22 years, from 1979 to 2002. The minimum Arctic sea ice animation clearly shows how over the last 5 years the quantity of polar ice has decreased by 10 - 14% from the 22 year average.While moving from the Arctic to Greenland, the animation shows the constant motion of the Arctic polar ice using daily measures of sea ice activity. Sea ice flows from the Arctic into Baffin Bay as the seasonal ice expands southward. As we draw close to the Greenland coast, the animation shows the recent changes in the Jakobshavn glacier. Although Jakobshavn receded only slightly from 1042 to 2001, the animation shows significant recession over the past three years, from 2002 through 2004.This animation shows a wealth of data collected from satellite observations of the cryosphere and the impact that recent cryospheric changes are making on our planet.For more information on the data sets used in this visualization, visit NASA's EOS DAAC website. || ", "hits": 104 }, { "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": 18 }, { "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": 34 }, { "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": 74 }, { "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": 25 }, { "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": 10 }, { "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": 41 }, { "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": 107 }, { "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": 26 }, { "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": 14 }, { "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": 35 }, { "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": 36 }, { "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": 38 }, { "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": 29 }, { "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": 23 }, { "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": 20 }, { "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": 109 }, { "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": 33 }, { "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": 15 }, { "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": 18 }, { "id": 2214, "url": "https://svs.gsfc.nasa.gov/2214/", "result_type": "Visualization", "release_date": "2001-08-13T12:00:00-04:00", "title": "The Impact of Aerosols on Atmospheric Warming - Version 1", "description": "Bright and dark aerosols, combined with solar heating, create different effects in heating the atmosphere and heating the surface of the Earth. This animation zooms into the INDOEX region showing aerosol and solar reflectance (albedo) data from the Terra satellite, then displays how these inputs generate warming of the atmosphere (Atmospheric Forcing - red regions) and cooling of the surface (Surface Forcing - dark regions). Areas of missing data (due to clouds, etc.) are either black or transparent. || ", "hits": 11 }, { "id": 2215, "url": "https://svs.gsfc.nasa.gov/2215/", "result_type": "Visualization", "release_date": "2001-08-13T12:00:00-04:00", "title": "Aerosols and Warming Change with Time - Version 1", "description": "As the aerosol content and solar heating change with time, the atmosphere and the Earth's surface experience different warming and cooling. This animation displays a time series of the INDOEX region with 8-day averages showing aerosol and solar reflectance (albedo) data from the Terra satellite From these, we see how these inputs generate warming of the atmosphere (Atmospheric Forcing - red regions) and cooling of the surface (Surface Forcing - dark regions). Areas of missing data (due to clouds, etc.) are either black or transparent. || ", "hits": 8 }, { "id": 2230, "url": "https://svs.gsfc.nasa.gov/2230/", "result_type": "Visualization", "release_date": "2001-08-13T12:00:00-04:00", "title": "The Impact of Aerosols on Atmospheric Warming - Version 2", "description": "Bright and dark aerosols, combined with solar heating, create different effects in heating the atmosphere and heating the surface of the Earth. This animation zooms into the INDOEX region showing aerosol and solar reflectance (albedo) data from the Terra satellite, then displays how these inputs generate warming of the atmosphere (Atmospheric Forcing - red regions) and cooling of the surface (Surface Forcing - dark regions). Areas of missing data (due to clouds, etc.) are either black or transparent. || ", "hits": 12 }, { "id": 2231, "url": "https://svs.gsfc.nasa.gov/2231/", "result_type": "Visualization", "release_date": "2001-08-13T12:00:00-04:00", "title": "Aerosols and Warming Change with Time - Version 2", "description": "As the aerosol content and solar heating change with time, the atmosphere and the Earth's surface experience different warming and cooling. This animation displays a time series of the INDOEX region with 8-day averages showing aerosol and solar reflectance (albedo) data from the Terra satellite. From these, we see how these inputs generate warming of the atmosphere (Atmospheric Forcing - red regions) and cooling of the surface (Surface Forcing - dark regions). Areas of missing data (due to clouds, etc.) are either black or transparent. || ", "hits": 5 }, { "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": 7 }, { "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": 16 }, { "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": 3 }, { "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": 3 }, { "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": 8 }, { "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": 3 }, { "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": 14 }, { "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": 15 }, { "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": 16 }, { "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": 33 }, { "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": 11 }, { "id": 1118, "url": "https://svs.gsfc.nasa.gov/1118/", "result_type": "Visualization", "release_date": "2000-04-19T12:00:00-04:00", "title": "Terra First Light Visualizations: North America", "description": "Viewing various TERRA data sets of North America including: MODIS Image of North America, CERES shortwave/Albedo, CERES longwave, MODIS True Color, 250m MODIS TRUE (San Francisco), ASTER (Lake Tahoe), MISR (Baja), and MODIS -True Color || ", "hits": 7 }, { "id": 1136, "url": "https://svs.gsfc.nasa.gov/1136/", "result_type": "Visualization", "release_date": "2000-04-19T12:00:00-04:00", "title": "CERES Globe", "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": 13 }, { "id": 1137, "url": "https://svs.gsfc.nasa.gov/1137/", "result_type": "Visualization", "release_date": "2000-04-19T12:00:00-04:00", "title": "CERES Flat Map", "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": 9 }, { "id": 1138, "url": "https://svs.gsfc.nasa.gov/1138/", "result_type": "Visualization", "release_date": "2000-04-19T12:00:00-04:00", "title": "CERES to MISR Sequence", "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": 7 }, { "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": 7 }, { "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": 12 }, { "id": 1141, "url": "https://svs.gsfc.nasa.gov/1141/", "result_type": "Visualization", "release_date": "2000-04-19T12:00:00-04:00", "title": "Global Shortwave 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": 8 }, { "id": 1142, "url": "https://svs.gsfc.nasa.gov/1142/", "result_type": "Visualization", "release_date": "2000-04-19T12:00:00-04:00", "title": "Shortwave 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": 7 }, { "id": 1143, "url": "https://svs.gsfc.nasa.gov/1143/", "result_type": "Visualization", "release_date": "2000-04-19T12:00:00-04:00", "title": "Spinning 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": 7 }, { "id": 1144, "url": "https://svs.gsfc.nasa.gov/1144/", "result_type": "Visualization", "release_date": "2000-04-19T12:00:00-04:00", "title": "Spinning Global Shortwave 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": 8 }, { "id": 1130, "url": "https://svs.gsfc.nasa.gov/1130/", "result_type": "Visualization", "release_date": "2000-04-15T12:00:00-04:00", "title": "Terra: Focus on INDOEX (Second Version)", "description": "Showing various registered data sets of the INDOEX region (second version). 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For more information on INDOEX, please visit http://www-indoex.ucsd.edu. || INDOEX Synergy movie || a001129.00005_print.png (720x480) [455.6 KB] || a001129_pre.jpg (320x238) [7.8 KB] || a001129.webmhd.webm (960x540) [3.3 MB] || a001129.m2v (720x480) [21.1 MB] || a001129.dv (720x480) [99.4 MB] || a001129.mp4 (640x480) [5.3 MB] || IndoExSynergy.mov (320x240) [2.6 MB] || a001129.mpg (352x240) [3.8 MB] || ", "hits": 6 } ] }