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            <Abstract>During the summer of 1988, wildfires burned about 1.4 million acres in and around Yellowstone National Park.  Spurred by the driest summer in park history, the fires started in early July and lasted until early October.  The worst day was August 20, when tremendous winds pushed the fires to burn over 150,000 acres.  Although the scars from these fires are still visible in Landsat imagery from space over ten years later, the patchwork nature of the fire footprint left many unburned areas from which plant species have regenerated very successfully.  This animation shows how the fires progressed in the period from June 30 though October 2, 1988, by which time the fall rain and snow had stopped the fire growth.  These maps are based on daily ground observations by fire lookouts in the park and by infrared imaging cameras flown over the park at night.  These observations are considered accurate to within about 100 meters.</Abstract>
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              <Abstract>This animation shows the progression of the fires in and around Yellowstone National Park during the summer of 1988, overlayed on a false-color image from Landsat 7..  Independent fires are shown in different colors, and the most recently burned areas are shown in a brighter color.  This version provides only the transparent overlay.</Abstract>
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            <Abstract>During the summer of 1988, wildfires burned about 1.4 million acres in and around Yellowstone National Park.  Spurred by the driest summer in park history, the fires started in early July and lasted until early October.  The worst day was August 20, when tremendous winds pushed the fires to burn over 150,000 acres.  Although the scars from these fires are still visible in Landsat imagery from space over ten years later, the patchwork nature of the fire footprint left many unburned areas from which plant species have regenerated very successfully.  This animation shows how the fires progressed in the period from June 30 though October 2, 1988, by which time the fall rain and snow had stopped the fire growth.  These maps are based on daily ground observations by fire lookouts in the park and by infrared imaging cameras flown over the park at night.  These observations are considered accurate to within about 100 meters.

This image can be composited with the previous animation.</Abstract>
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          <Title>African Fires during 2002</Title>
          <Abstract>This animation shows fire activity in Africa from January 1, 2002 to December 31, 2002.  The fires are shown as tiny particles with each particle depicting the geographic region in which fire was detected.  The color of a particle represents the number of days since a sizable amount of fire was detected in that region, with red representing less than 20 days, orange representing 20 to 40 days, yellow representing 40 to 60 days, and gray to black representing more than 60 days.  This data was measured by the MODIS instrument on the Terra satellite.  MODIS detects fires by measuring the brightness temperature of a region in several frequency bands and looking for hot spots where this temperature is greater than the surrounding region.</Abstract>
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            <Title>African Fires during 2002 (1024x1024 Animation)</Title>
            <Abstract>This animation shows fire activity in Africa from January 1, 2002 to December 31, 2002.  The fires are shown as tiny particles with each particle depicting the geographic region in which fire was detected.  The color of a particle represents the number of days since a sizable amount of fire was detected in that region, with red representing less than 20 days, orange representing 20 to 40 days, yellow representing 40 to 60 days, and gray to black representing more than 60 days.  This data was measured by the MODIS instrument on the Terra satellite.  MODIS detects fires by measuring the brightness temperature of a region in several frequency bands and looking for hot spots where this temperature is greater than the surrounding region.</Abstract>
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            <Abstract>This animation shows fire activity in Africa from January 1, 2002 to December 31, 2002.  The fires are shown as tiny particles with each particle depicting the geographic region in which fire was detected.  The color of a particle represents the number of days since a sizable amount of fire was detected in that region, with red representing less than 20 days, orange representing 20 to 40 days, yellow representing 40 to 60 days, and gray to black representing more than 60 days.  This data was measured by the MODIS instrument on the Terra satellite.  MODIS detects fires by measuring the brightness temperature of a region in several frequency bands and looking for hot spots where this temperature is greater than the surrounding region.

This image can be composited with the previous animation.</Abstract>
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          <Title>Tropospheric Ozone Impacts Global Climate Warming (644x289 Animation)</Title>
          <Abstract>In the first global assessment of the impact of ozone on climate warming, scientists at the NASA Goddard Institute for Space Studies (GISS), New York, evaluated how ozone in the lowest part of the atmosphere (the troposphere)  changed temperatures over the past 100 years. Using the best available estimates of global emissions of gases that create ozone, the GISS computer model study reveals how much this single air pollutant and greenhouse gas has contributed to warming in specific regions of the world.

Ozone was responsible for one-third to half of the observed warming trend in the Arctic during winter and spring, according to the new research. Ozone is transported from the industrialized countries in the Northern Hemisphere to the Arctic quite efficiently during these seasons. The findings will be published soon in the American Geophysical Union's Journal of Geophysical Research-Atmospheres.

The impact of ozone air pollution on climate warming is difficult to pinpoint because, unlike other greenhouse gases such as carbon dioxide, ozone does not last long enough in the lower atmosphere to spread uniformly around the globe. Its warming impact is much more closely tied to the region it originated from. To capture this complex picture, the GISS scientists used a suite of three-dimensional computer models that starts with data on ozone sources and then tracks how ozone chemically evolved and moved around the world over the past century.

The research was supported by NASA's Atmospheric Chemistry Modeling and Analysis Program.</Abstract>
          <KeywordList>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Climate Indicators:Air Temperature Indices</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Chemistry/Oxygen Compounds:Ozone</Keyword>
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          <Attribution>
            <Title>National Aeronautics and Space Administration</Title>
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            <Abstract>This animation shows anomalous global temperature averages from December through May in the years 1880 through 2000.  </Abstract>
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          <Title>2005 Hurricanes: Clouds and Sea Surface Temperature (1024x512 Animation)</Title>
          <Abstract>This visualization shows sea surface temperatures during most of the 2005 hurricane season.  Overlaid are infrared cloud data, storm track data, and storm name labels.  Warm ocean waters provide the heat energy that fuels hurricanes.  Notice the correspondence between the storm tracks and the sea surface temperature response; this is particulary noticeable for hurricanes Dennis, Emily, and Katrina, where the hurricanes churn up the ocean so that cooler water rises to the surface.  This version shows the entire Atlantic hurricane region and depicts all of the 2005 hurricanes except Zeta, which appeared at the very end of the year.</Abstract>
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            <Keyword vocabulary="DLESE">Atmospheric science</Keyword>
            <Keyword vocabulary="SVS">Hurricane</Keyword>
            <Keyword vocabulary="DLESE">Natural hazards</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Phenomena:Hurricanes</Keyword>
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            <Abstract>The TMI instrument on the TRMM satellite measures microwaves emitted from the Earth's land and water.  By comparing emission from different microwave frequencies, the characteristics of ice and water in the atmosphere can be determined.  For example, 85 GHz microwaves are scattered by ice crystals in tropical cyclones, making cyclone rain bands appear 'colder' than the surrounding areas.  By comparing 85 GHz temperatures in different polarizations with other frequency band measurements, accurate measurements of rainfall in the atmosphere can be made.  This animation shows eight days of global TMI 85 GHz measurements in the Gulf of Mexico during Hurricane Katrina.  The hurricane Katrina rainbands clearly show up in these images.</Abstract>
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This image can be composited with the previous animation.</Abstract>
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            <Abstract>The TMI instrument on the TRMM satellite measures microwaves emitted from the Earth's land and water.  By comparing emission from different microwave frequencies, the characteristics of ice and water in the atmosphere can be determined.  For example, 85 GHz microwaves are scattered by ice crystals in tropical cyclones, making cyclone rain bands appear 'colder' than the surrounding areas.  By comparing 85 GHz temperatures in different polarizations with other frequency band measurements, accurate measurements of rainfall in the atmosphere can be made.  This animation shows four days of TMI 85 GHz measurements, one orbit at a time.  Hurricane Katrina was in the Gulf of Mexico at the time and clearly shows up in the measurements.</Abstract>
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            <Abstract>GOES-12 longwave infrared imagery of Hurricane Katrina from August 26, 2005 through August 30, 2005.</Abstract>
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          <Title>Global Large-scale Precipitation during Hurricane Frances (1000x721 Animation)</Title>
          <Abstract>Water vapor is a small but significant constituent of the atmosphere, warming the planet due to the greenhouse effect and condensing to form clouds.  As moisture-laden air rises, the relative humidity increases until it saturates the air, at which time precipitation occurs.  If the uplift of air is due to large-scale atmospheric motion, then the precipitation is called large-scale, or dynamic.  This animation shows the large-scale precipitation for the whole globe from September 1, 2004, through September 5, 2004, during the period of Hurricane Frances in the western Atlantic Ocean and Typhoon Songda in the western Pacific Ocean.  Large-scale precipitation tends to be continuous and to come from decks of stratus clouds rather than from thunderstorms.</Abstract>
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            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Water Vapor:Precipitable Water</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Human Dimensions:Natural Hazards:Meteorological Hazards</Keyword>
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            <Abstract>Global large-scale precipitation rate from the 0.25 degree resolution fvGCM atmospheric model for the period 9/1/2005 through 9/5/2005.
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          <Abstract>Water vapor is a small but significant constituent of the atmosphere, warming the planet due to the greenhouse effect and condensing to form clouds.  As moisture-laden air rises, the relative humidity increases until it saturates the air, at which time precipitation occurs.  If the uplift of air is due to strong updrafts and unstable air systems, as in thunderstorms, then the precipitation is called convective.  This animation shows the convective precipitation for the whole globe from September 1, 2004, through September 5, 2004, during the period of Hurricane Frances in the western Atlantic Ocean and Typhoon Songda in the western Pacific Ocean.  Convective precipitation is more intense but less long-lasting than large-scale precipitation.</Abstract>
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          <Abstract>The Earth's atmosphere exerts pressure based on the weight of the air above, so the pressure reduces with rising altitude.  This rate of pressure reduction with altitude is based on the temperature of the air, with the pressure of colder air reducing faster with altitude than warmer air.  Therefore, a surface of constant pressure has a lower altitude at the poles than the equator.  This animation shows the altitude above sea level (the geopotential height) of the 300 hectopascal (hPa) pressure surface for the whole globe from September 1, 2004, through September 5, 2004, during the period of Hurricane Frances in the western Atlantic Ocean and Typhoon Songda in the western Pacific Ocean.  This pressure is about one-third of the normal pressure at sea level.  The largest downward slope of this surface occurs in the mid-latitudes and is shown in yellow in the animation.  At this region, air is trying to flow from the equator towards the poles to reduce the slope, but the rotation of the Earth forces the flow to divert to the east, forming the strong west-to-east jet stream flows in these regions.  Frances and Songda can be seen as sharp yellow dots of reduced height in their respective locations.</Abstract>
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          <Abstract>The Earth's atmosphere exerts pressure based on the weight of the air above.  Differences in pressure from place-to-place cause winds to try to flow from high pressure to low pressure regions to even out the differences, but the Earth's rotation and wind friction with the surface act to slow or divert the winds.  This animation shows the high altitude wind speeds for the whole globe from September 1, 2004, through September 5, 2004, during the period of Hurricane Frances in the western Atlantic Ocean and Typhoon Songda in the western Pacific Ocean.  At high altitudes, the difference between between high pressures from warm tropical air and low pressures from cold polar air try to force air from the tropics toward the poles, but the Earth's rotation diverts this flow to the east, resulting in the high velocity west-to-east jet stream flows at mid-latitudes.  The circular flows from Frances and Songda can barely be seen at this altitude.</Abstract>
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            <Abstract>Global winds at 200 hPa geopotential height from the 0.25 degree resolution fvGCM atmospheric model for the period 9/1/2005 through 9/5/2005.</Abstract>
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          <Abstract>Water vapor is a small but significant constituent of the atmosphere, warming the planet due to the greenhouse effect and condensing to form clouds which both warm and cool the Earth in different circumstances.  Warm, moisture-laden air moving out from the tropics brings rainfall to the temperate zones.  This animation shows the atmospheric water vapor for the whole globe from September 1, 2004, through September 5, 2004, during the period of Hurricane Frances in the western Atlantic Ocean and Typhoon Songda in the western Pacific Ocean.  The band of water vapor over the tropics is the intertropical convergence zone, where converging trade winds and high temperatures force large amounts of water high into the atmosphere.  Both Hurricane Frances and Typhoon Songda exhibit significant spiral bands of high water vapor.</Abstract>
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            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Phenomena:Typhoons</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Water Vapor:Precipitable Water</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Human Dimensions:Natural Hazards:Meteorological Hazards</Keyword>
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          <Abstract>The weight of the Earth's atmosphere exerts pressure on the surface of the Earth.  This pressure varies from place-to-place and from time-to-time due to surface irregularities, uneven heating of the atmosphere by the sun, and the Earth's rotation.  Differences in pressure from place-to-place cause winds to try to flow from high pressure to low pressure regions to even out the differences, but the Earth's rotation and wind friction with the surface act to slow or divert the winds.  This animation shows the surface wind speeds for the whole globe from September 1, 2004, through September 5, 2004, during the period of Hurricane Frances in the western Atlantic Ocean and Typhoon Songda in the western Pacific Ocean.  The highest, smoothest winds occur over the oceans where there are no surface irregularities to break up the flow, while flows over land tend to be irregular and highly variable.  The highest winds occur in Hurricane Frances and Typhoon Songda, but note that the hurricane's wind speeds reduce dramatically when crossing Florida.</Abstract>
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            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Phenomena:Typhoons</Keyword>
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            <Keyword vocabulary="GCMD">EARTH SCIENCE:Human Dimensions:Natural Hazards:Meteorological Hazards</Keyword>
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            <Title>Hurricane Emily (Sequence)</Title>
            <Abstract>Emily was a record-setting storm for many reasons. When it formed on July 11, Emily became the earliest fifth named storm on record. As it moved through the Caribbean, Emily intensified into a powerful Category 4 storm with winds over 250 kilometers per hour (150 mph) and gusts as high as 300 kilometers per hour (184 mph), making it the most powerful storm to form before August. The previous record was set by Hurricane Dennis, which ripped through the Caribbean during the first week of July 2005. Emily's Category 4 status also made 2005 the only year to produce two Category 4 storms before the end of July.</Abstract>
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              <Abstract>Emily was a record-setting storm for many reasons. When it formed on July 11, Emily became the earliest fifth named storm on record. As it moved through the Caribbean, Emily intensified into a powerful Category 4 storm with winds over 250 kilometers per hour (150 mph) and gusts as high as 300 kilometers per hour (184 mph), making it the most powerful storm to form before August. The previous record was set by Hurricane Dennis, which ripped through the Caribbean during the first week of July 2005. Emily's Category 4 status also made 2005 the only year to produce two Category 4 storms before the end of July.</Abstract>
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              <Abstract>Emily was a record-setting storm for many reasons. When it formed on July 11, Emily became the earliest fifth named storm on record. As it moved through the Caribbean, Emily intensified into a powerful Category 4 storm with winds over 250 kilometers per hour (150 mph) and gusts as high as 300 kilometers per hour (184 mph), making it the most powerful storm to form before August. The previous record was set by Hurricane Dennis, which ripped through the Caribbean during the first week of July 2005. Emily's Category 4 status also made 2005 the only year to produce two Category 4 storms before the end of July.</Abstract>
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              <Abstract>Emily was a record-setting storm for many reasons. When it formed on July 11, Emily became the earliest fifth named storm on record. As it moved through the Caribbean, Emily intensified into a powerful Category 4 storm with winds over 250 kilometers per hour (150 mph) and gusts as high as 300 kilometers per hour (184 mph), making it the most powerful storm to form before August. The previous record was set by Hurricane Dennis, which ripped through the Caribbean during the first week of July 2005. Emily's Category 4 status also made 2005 the only year to produce two Category 4 storms before the end of July.</Abstract>
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              <Abstract>Emily was a record-setting storm for many reasons. When it formed on July 11, Emily became the earliest fifth named storm on record. As it moved through the Caribbean, Emily intensified into a powerful Category 4 storm with winds over 250 kilometers per hour (150 mph) and gusts as high as 300 kilometers per hour (184 mph), making it the most powerful storm to form before August. The previous record was set by Hurricane Dennis, which ripped through the Caribbean during the first week of July 2005. Emily's Category 4 status also made 2005 the only year to produce two Category 4 storms before the end of July.</Abstract>
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              <Abstract>Emily was a record-setting storm for many reasons. When it formed on July 11, Emily became the earliest fifth named storm on record. As it moved through the Caribbean, Emily intensified into a powerful Category 4 storm with winds over 250 kilometers per hour (150 mph) and gusts as high as 300 kilometers per hour (184 mph), making it the most powerful storm to form before August. The previous record was set by Hurricane Dennis, which ripped through the Caribbean during the first week of July 2005. Emily's Category 4 status also made 2005 the only year to produce two Category 4 storms before the end of July.</Abstract>
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          <Abstract>As the Sun's energy reaches the Earth, it is either reflected, absorbed by the clouds, or absorbed by the Earth's surface.  The part absorbed by the surface heats the Earth, which causes surface water to evaporate to the air, particularly over oceans or moist land.  Similarly, a cold surface causes water to condense from the air onto the land or ocean.  Latent heat flux is the amount of energy moving from the surface to the air due to evapolation (positive values) or from the air to the land due to condensation (negative values).  This animation shows the latent heat flux for the whole globe from September 1, 2004, through September 5, 2004, during the period of Hurricane Frances in the western Atlantic Ocean and Typhoon Songda in the western Pacific Ocean.  The animation clearly shows the evaporation over land only during the heat of the day, while the evaporation over the ocean is continuous throughout the day.  The highest positive latent heat flux occurs during hurricanes and typhoons, as these events are powered by the movement of heat energy from the warm ocean to the atmosphere, seen here in Hurricane Frances and Typhoon Songda.  Significant negative latent heat flux is somewhat rare and occurs over the ocean only during certain configurations of air and surface conditions.</Abstract>
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          <Abstract>As the Sun's energy reaches the Earth, it is either reflected, absorbed by the clouds, or absorbed by the Earth's surface.  The part absorbed by the Earth's surface heats the Earth, which then heats the air just above the surface.  This process occurs rapidly in the case of dry land and slowly in the case of the oceans. This animation shows the surface air temperature at an altitude of 2 meters for the whole globe from September 1, 2004, through September 5, 2004, during the period of Hurricane Frances in the western Atlantic Ocean and Typhoon Songda in the western Pacific Ocean.  The animation clearly shows the air over land reacting rapidly to solar heating during the day and cooling at night, while the daily solar cyle is not visible in the temperature of the air over the ocean.  A very dynamic region of changing air temperature is visible in the interaction between the cold air over Antarctica and the warmer mid-latitude air over the southern oceans during this region of polar night.  Hurricane Frances and Typhhon Songda are just barely visible as circulating temperature patterns in the western Atlantic and Pacific Oceans.</Abstract>
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          <Abstract>The weight of the Earth's atmosphere exerts pressure on the surface of the Earth.  This pressure varies from place-to-place due the variations in the Earth's surface since higher altitudes have less atmosphere above them than lower altitudes.  Atmospheric pressure also varies from time-to-time due to the uneven heating of the atmosphere by the sun and the rotation of the Earth, causing weather.  This animation shows the atmospheric surface pressure for the whole globe from September 1, 2004, through September 5, 2004, during the period of Hurricane Frances in the western Atlantic Ocean and Typhoon Songda in the western Pacific Ocean.  The major changes in pressure occur over land where the surface altitude varies, but the sharp, moving low pressures areas for Frances and Songda can be clearly seen in the oceans.  Since changing surface pressure areas over land are hard to see in these images due to the strong altitude variations, plots of the atmospheric surface pressure are almost never used to study the weather.  A different plot, of sea-level pressure, is used instead.</Abstract>
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              <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Precipitation:Snow</Keyword>
              <Keyword vocabulary="GCMD">EARTH SCIENCE:Cryosphere:Snow/Ice:Snow Cover</Keyword>
              <Keyword vocabulary="GCMD">EARTH SCIENCE:Hydrosphere:Snow/Ice:Snow Cover</Keyword>
            </KeywordList>
            <CRS>CRS:84</CRS>
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          <Title>Global Atmospheric Sea Level Pressure during Hurricane Frances (1000x721 Animation)</Title>
          <Abstract>The weight of the Earth's atmosphere exerts pressure on the surface of the Earth.  This pressure varies from place-to-place due the variations in the Earth's surface since higher altitudes have less atmosphere above them than lower altitudes.  Atmospheric pressure also varies from time-to-time due to the uneven heating of the atmosphere by the sun and the rotation of the Earth, causing weather.  In order to see the changes in pressure which affect the weather, the variation due to altitude is removed from the surface pressure, creating a quantity called sea level pressure.  This animation shows the atmospheric sea level pressure for the whole globe from September 1, 2004, through September 5, 2004, during the period of Hurricane Frances in the western Atlantic Ocean and Typhoon Songda in the western Pacific Ocean.  The sharp, moving low pressures areas for Frances and Songda can be clearly seen in the oceans.  Even with the direct effect of altitude removed, cold high-altitude regions such as the South Pole and the Himalayan Plateau still exhibit lower-than-normal pressures, probably due to the interaction of cold air over those regions with the warmer air in the surrounding regions.</Abstract>
          <KeywordList>
            <Keyword vocabulary="DLESE">Atmospheric science</Keyword>
            <Keyword vocabulary="DLESE">Natural hazards</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Phenomena:Hurricanes</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Phenomena:Typhoons</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Pressure:Sea Level Pressure</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Human Dimensions:Natural Hazards:Meteorological Hazards</Keyword>
            <Keyword vocabulary="GCMD">Location:Global</Keyword>
            <Keyword vocabulary="SVS">Hurricane Frances</Keyword>
          </KeywordList>
          <CRS>CRS:84</CRS>
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          <Dimension name="time" units="ISO8601" default="2004-09-06T00Z">2004-09-01T03Z/2004-09-06T00Z/PT3H</Dimension>
          <Attribution>
            <Title>National Aeronautics and Space Administration</Title>
            <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
             xlink:type="simple"
             xlink:href="http://svs.gsfc.nasa.gov/vis/a000000/a003100/a003182/"/>
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            <Name>opaque</Name>
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            <Abstract>Global atmospheric sea level pressure from the 0.25 degree resolution fvGCM atmospheric model for the period 9/1/2005 through 9/5/2005.</Abstract>
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              <Format>image/png</Format>
              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
               xlink:type="simple"
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        <Layer opaque="1" noSubsets="1" fixedWidth="1024" fixedHeight="512">
          <Name>3179_21773</Name>
          <Title>Scene Identification Compared to Clouds (1024x512 Animation)</Title>
          <Abstract>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.</Abstract>
          <KeywordList>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Reflectance</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Clouds:Cloud Reflectance</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Cryosphere:Sea Ice:Reflectance</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Land Surface:Surface Radiative Properties:Reflectance</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Oceans:Ocean Heat Budget:Reflectance</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Oceans:Sea Ice:Reflectance</Keyword>
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          <CRS>CRS:84</CRS>
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          <Attribution>
            <Title>National Aeronautics and Space Administration</Title>
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            <Abstract>This animation shows 29 orbits (2 days) of CERES measurements of regions of solar reflectivity, from June 20-21, 2003.  The measurements are superimposed over a global infrared cloud cover composite from the same period.</Abstract>
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          <Title>Incoming Solar Flux Compared to Clouds (1024x512 Animation)</Title>
          <Abstract>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).</Abstract>
          <KeywordList>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Incoming Solar Radiation</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Solar Irradiance</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Clouds:Cloud Reflectance</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Sun-earth Interactions:Solar Activity:Solar Irradiance</Keyword>
          </KeywordList>
          <CRS>CRS:84</CRS>
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          <Dimension name="time" units="ISO8601" default="2003-06-22T00:56Z">2003-06-20T02:44Z/2003-06-22T00:56Z/PT1H39M</Dimension>
          <Attribution>
            <Title>National Aeronautics and Space Administration</Title>
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            <Abstract>This animation shows incoming solar flux corresponding to 29 orbits (2 days) of CERES measurements, from June 20-21, 2003. This data is calculated using data from SORCE for the flux magnitude at the Earths orbit, coupled with solar incidence angles based on CERES measurement locations and times.  The measurements are superimposed over a global infrared cloud cover composite from the same period.</Abstract>
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              <Format>image/png</Format>
              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
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        <Layer opaque="1" noSubsets="1" fixedWidth="1024" fixedHeight="512">
          <Name>3177_21760</Name>
          <Title>Net Radiation Flux Compared to Clouds (1024x512 Animation)</Title>
          <Abstract>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.</Abstract>
          <KeywordList>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Net Radiation</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Radiative Flux</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Clouds:Cloud Top Temperature</Keyword>
          </KeywordList>
          <CRS>CRS:84</CRS>
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          <Attribution>
            <Title>National Aeronautics and Space Administration</Title>
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            <Abstract>This animation shows net radiation flux corresponding to 29 orbits (2 days) of CERES measurements, from June 20-21, 2003. This data is calculated from CERES outgoing longwave and shortwave measurements, along with a corresponding calculated incoming solar flux.  The measurements are superimposed over a global infrared cloud cover composite from the same period.  </Abstract>
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          <Title>Outgoing Longwave Flux Compared to Clouds (1024x512 Animation)</Title>
          <Abstract>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.</Abstract>
          <KeywordList>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Outgoing Longwave Radiation</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Clouds:Cloud Top Temperature</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Oceans:Ocean Heat Budget:Longwave Radiation</Keyword>
          </KeywordList>
          <CRS>CRS:84</CRS>
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          <Dimension name="time" units="ISO8601" default="2003-06-22T00:56Z">2003-06-20T02:44Z/2003-06-22T00:56Z/PT1H39M</Dimension>
          <Attribution>
            <Title>National Aeronautics and Space Administration</Title>
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            <Name>opaque</Name>
            <Title>Opaque</Title>
            <Abstract>This animation shows 29 orbits (2 days) of outgoing longwave radiation, form June 20-21, 2003.  The measurements are superimposed over a global infrared cloud cover composite from the same period.</Abstract>
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              <Format>image/png</Format>
              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
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          <Name>3175_21743</Name>
          <Title>Outgoing Shortwave Flux Compared to Clouds (1024x512 Animation)</Title>
          <Abstract>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.</Abstract>
          <KeywordList>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Shortwave Radiation</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Clouds:Cloud Reflectance</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Oceans:Ocean Heat Budget:Shortwave Radiation</Keyword>
          </KeywordList>
          <CRS>CRS:84</CRS>
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          <Dimension name="time" units="ISO8601" default="2003-06-22T00:56Z">2003-06-20T02:44Z/2003-06-22T00:56Z/PT1H39M</Dimension>
          <Attribution>
            <Title>National Aeronautics and Space Administration</Title>
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            <Abstract>This animation shows 29 orbits (2 days) of CERES measurements of outgoing shortwave radiation, from June 20-21, 2003.  The measurements are superimposed over a global infrared cloud cover composite from the same period.</Abstract>
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              <Format>image/png</Format>
              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
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          <Title>Wind Anomalies during El Nino/La Nina Event of 1997-1998 (2040x504 Animation)</Title>
          <Abstract>The El Nino/La Nina event in 1997-1999 was particularly intense, but was also very well observed by satellites and buoys. Deviations from normal winds speeds and directions of the were computed using data from the Special Sensor Microwave/Imager (SSMI) on the Tropical Rainfall Measuring Mission (TRMM) satellite.</Abstract>
          <KeywordList>
            <Keyword vocabulary="DLESE">Physical oceanography</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Winds:Surface Winds</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Climate Indicators:Teleconnections:El Nino Southern Oscillation</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Oceans:Ocean Winds:Surface Winds</Keyword>
            <Keyword vocabulary="GCMD">Location:Pacific Ocean</Keyword>
          </KeywordList>
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              <Abstract>Hurricane Fabian threatened the Eastern Coast of the United States before it turned northward and hit the island of Bermuda instead.  Fabian came within 50 miles to the west of Bermuda on September 5th, 2003, with sustained winds of 117 miles per hour and with gusts of up to 130 miles per hour.</Abstract>
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              <Abstract>Hurricane Fabian threatened the Eastern Coast of the United States before it turned northward and hit the island of Bermuda instead.  Fabian came within 50 miles to the west of Bermuda on September 5th, 2003, with sustained winds of 117 miles per hour and with gusts of up to 130 miles per hour.</Abstract>
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          <Abstract>Big cities influence the environment around them. For example, urban areas are typically warmer than their surroundings. Cities are strikingly visible in computer models that simulate the Earth's land surface. This visualization shows sensible heat flux predicted by the Land Information System (LIS) for a day in June 2001. (Sensible heat flux refers to transfer of heat from the earth's surface to the air above; for further explanation see http://www.uwsp.edu/geo/faculty/ritter/geog101/textbook/energy/energy_balance.html). Sensible heat flux is higher in the cities--that is, they transfer more heat to the atmosphere--because the surface there is warmer than in the surroundings. Only part of the global computation is shown, focusing on the highly urbanized northeast corridor in the United States, including the cities of Boston, New York, Philadelphia, Baltimore, and Washington.</Abstract>
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          <Abstract>Big cities influence the environment around them. For example, urban areas are typically warmer than their surroundings. Cities are strikingly visible in computer models that simulate the Earth's land surface. This visualization shows latent heat flux predicted by the Land Information System (LIS) for a day in June 2001. (Latent heat flux refers to the transfer of energy from the Earth's surface to the air above by evaporation of water on the surface; for a more detailed explanation see http://www.uwsp.edu/geo/faculty/ritter/geog101/textbook/energy/energy_balance.html). Latent heat flux is lower in the cities because there is less evaporation there. Only part of the global computation is shown, focusing on the highly urbanized northeast corridor in the United States, including the cities of Boston, New York, Philadelphia, Baltimore, and Washington.</Abstract>
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          <Title>Urban Signatures: Thermal Radiation (1000x1000 Image)</Title>
          <Abstract>Big cities influence the environment around them. For example, urban areas are typically warmer than their surroundings. Cities are strikingly visible in computer models that simulate the Earth's land surface. This visualization shows outgoing thermal radiation predicted by the Land Information System (LIS) for a day in June 2001. Cities are warmer, so they emit more longwave (infrared) radiation. Only part of the global computation is shown, focusing on the highly urbanized northeast corridor in the United States, including the cities of Boston, New York, Philadelphia, Baltimore, and Washington.

Additional Credit:
NASA GSFC Land Information System (http://lis.gsfc.nasa.gov/)</Abstract>
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            <Abstract>This image shows outgoing thermal radiation
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urban areas stand out very distinctly against their less
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          <Title>Urban Signatures: Evaporation (1000x1000 Image)</Title>
          <Abstract>Big cities influence the environment around them. For example, urban areas are typically warmer than their surroundings. Cities are strikingly visible in computer models that simulate the Earth's land surface. This visualization shows evaporation rates predicted by the Land Information System (LIS) for a day in June 2001. Evaporation is lower in the cities because water tends to run off pavement and into drains, rather than being absorbed by soil and plants from which it later evaporates. Only part of the global computation is shown, focusing on the highly urbanized northeast corridor in the United States, including the cities of Boston, New York, Philadelphia, Baltimore, and Washington.

Additional Credit:
NASA GSFC Land Information System (http://lis.gsfc.nasa.gov/)</Abstract>
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          <Abstract>Hurricane Charley was the first of four hurricanes to hit the United States in 2004.</Abstract>
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        <Layer opaque="0" noSubsets="1" fixedWidth="720" fixedHeight="360">
          <Name>3144_21247</Name>
          <Title>Global Lightning Flash Rate Density (720x360 Image)</Title>
          <Abstract>Lightning is a brief but intense electrical discharge between positive and negative regions of a thunderstorm.The Lightning Imaging Sensor (LIS) on the Tropical Rainfall Measuring Mission (TRMM) satellite was designed to study the distribution and variability of total lightning on a global basis. The Optical Transient Detector (OTD) was an earlier lightning detector flying aboard the Microlab-1 spacecraft. The data shown here are compiled from LIS (1998-2002) and OTD (1995-1999) observations. Because each satellite saw only a part of the Earth at any one time, these data use complex algorithms to estimate total flash rate density (number of flashes per square kilometer per year) based on the flashes observed and the amount of time the satellite views each area.</Abstract>
          <KeywordList>
            <Keyword vocabulary="DLESE">Atmospheric science</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Electricity:Lightning</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Phenomena:Lightning</Keyword>
            <Keyword vocabulary="GCMD">Location:Global</Keyword>
          </KeywordList>
          <CRS>CRS:84</CRS>
          <EX_GeographicBoundingBox>
            <westBoundLongitude>-180</westBoundLongitude>
            <eastBoundLongitude>180</eastBoundLongitude>
            <southBoundLatitude>-90</southBoundLatitude>
            <northBoundLatitude>90</northBoundLatitude>
          </EX_GeographicBoundingBox>
          <BoundingBox CRS="CRS:84" minx="-180" miny="-90" maxx="180" maxy="90"/>
          <Attribution>
            <Title>National Aeronautics and Space Administration</Title>
            <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
             xlink:type="simple"
             xlink:href="http://svs.gsfc.nasa.gov/vis/a000000/a003100/a003144/"/>
            <LogoURL width="312" height="258">
              <Format>image/png</Format>
              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
               xlink:type="simple"
               xlink:href="http://svs.gsfc.nasa.gov/svs_icons/nasalogo.png"/>
            </LogoURL>
          </Attribution>
          <MetadataURL type="FGDC:1998">
            <Format>text/plain</Format>
            <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
             xlink:type="simple"
             xlink:href="http://svs.gsfc.nasa.gov/vis/a000000/a003100/a003144/a003144.fgdc"/>
          </MetadataURL>
          <Style>
            <Name>overlay</Name>
            <Title>Transparent Overlay Only</Title>
            <Abstract>This image shows the global lightning flash
rate density for the entire observing period. The data pixels
are 0.5deg on a side (720x360 pixels globally). This single
image is equivalent to the final frame of animation #3143, but
at a spatial resolution that is 5 times
better.</Abstract>
            <LegendURL width="320" height="90">
              <Format>image/png</Format>
              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
               xlink:type="simple"
               xlink:href="http://svs.gsfc.nasa.gov/vis/a000000/a003100/a003144/lightdens_bar.png"/>
            </LegendURL>
          </Style>
        </Layer>
        <Layer opaque="1" noSubsets="1">
          <Title>Global Lightning Accumulation</Title>
          <Abstract>Lightning is a brief but intense electrical discharge between positive and negative regions of a thunderstorm.  The Lightning Imaging Sensor (LIS) on the Tropical Rainfall Measuring Mission (TRMM) satellite was designed to study the distribution and variability of total lightning on a global basis. The Optical Transient Detector (OTD) was an earlier lightning detector flying aboard the Microlab-1 spacecraft.  The data shown here are compiled from LIS (1998-2002) and OTD (1995-1999) observations. Because each satellite saw only a part of the Earth at any one time, these data use complex algorithms to estimate total flash rate based on the flashes observed and the amount of time the satellite views each area.
NOTE: This animation is primarily designed to be used through the Web Mapping Services (WMS) protocol.  Each frame in the animation actually represents an accumulation of a number of years of data up through a particular day of the year.  Because of a limitation in the WMS protocol, each frame is marked only with a single date representing the last date for which the data was accumulated.</Abstract>
          <KeywordList>
            <Keyword vocabulary="DLESE">Atmospheric science</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Electricity:Lightning</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Phenomena:Lightning</Keyword>
            <Keyword vocabulary="GCMD">Location:Global</Keyword>
          </KeywordList>
          <Attribution>
            <Title>National Aeronautics and Space Administration</Title>
            <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
             xlink:type="simple"
             xlink:href="http://svs.gsfc.nasa.gov/vis/a000000/a003100/a003143/"/>
            <LogoURL width="312" height="258">
              <Format>image/png</Format>
              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
               xlink:type="simple"
               xlink:href="http://svs.gsfc.nasa.gov/svs_icons/nasalogo.png"/>
            </LogoURL>
          </Attribution>
          <MetadataURL type="FGDC:1998">
            <Format>text/plain</Format>
            <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
             xlink:type="simple"
             xlink:href="http://svs.gsfc.nasa.gov/vis/a000000/a003100/a003143/a003143.fgdc"/>
          </MetadataURL>
          <DataURL>
            <Format>text/html</Format>
            <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
             xlink:type="simple"
             xlink:href="http://thunder.nsstc.nasa.gov/primer/"/>
          </DataURL>
          <Layer opaque="0" noSubsets="1" fixedWidth="144" fixedHeight="72">
            <Name>3143_21314</Name>
            <Title>Low Resolution (144x72 Animation)</Title>
            <Abstract>Lightning is a brief but intense electrical discharge between positive and negative regions of a thunderstorm.  The Lightning Imaging Sensor (LIS) on the Tropical Rainfall Measuring Mission (TRMM) satellite was designed to study the distribution and variability of total lightning on a global basis. The Optical Transient Detector (OTD) was an earlier lightning detector flying aboard the Microlab-1 spacecraft.  The data shown here are compiled from LIS (1998-2002) and OTD (1995-1999) observations. Because each satellite saw only a part of the Earth at any one time, these data use complex algorithms to estimate total flash rate based on the flashes observed and the amount of time the satellite views each area.
NOTE: This animation is primarily designed to be used through the Web Mapping Services (WMS) protocol.  Each frame in the animation actually represents an accumulation of a number of years of data up through a particular day of the year.  Because of a limitation in the WMS protocol, each frame is marked only with a single date representing the last date for which the data was accumulated.</Abstract>
            <KeywordList>
              <Keyword vocabulary="DLESE">Atmospheric science</Keyword>
              <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Electricity:Lightning</Keyword>
              <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Phenomena:Lightning</Keyword>
              <Keyword vocabulary="GCMD">Location:Global</Keyword>
            </KeywordList>
            <CRS>CRS:84</CRS>
            <EX_GeographicBoundingBox>
              <westBoundLongitude>-180</westBoundLongitude>
              <eastBoundLongitude>180</eastBoundLongitude>
              <southBoundLatitude>-90</southBoundLatitude>
              <northBoundLatitude>90</northBoundLatitude>
            </EX_GeographicBoundingBox>
            <BoundingBox CRS="CRS:84" minx="-180" miny="-90" maxx="180" maxy="90"/>
            <Dimension name="time" units="ISO8601" default="2002-12-31">2002-01-01/2002-06-29/P1D,2002-06-31,2002-07-01/2002-12-31/P1D</Dimension>
            <MetadataURL type="FGDC:1998">
              <Format>text/plain</Format>
              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
               xlink:type="simple"
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            </MetadataURL>
            <DataURL>
              <Format>text/html</Format>
              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
               xlink:type="simple"
               xlink:href="http://thunder.nsstc.nasa.gov/primer/"/>
            </DataURL>
            <Style>
              <Name>overlay</Name>
              <Title>Transparent Overlay Only</Title>
              <Abstract>This animation shows an accumulation of daily
lightning climatology values for a typical year. That is, the
first frame shows the number of flashes per square kilometer
that occurred on a typical January 1 during the multi-year data
collection period, the second frame shows the total of Jan 1 and
Jan 2 flashes, the third frame shows Jan 1 through Jan 3, and so
on until the last frame (#365) which shows the total
accumulation for a typical year. As the year progresses, more
and more of the Earth experiences lightning, and hard-hit areas
experience more strikes. The most intense activity is in central
Africa. Areas where no lightning was measured are transparent,
letting the background image show through. The data pixels are
2.5deg on a side (144x72 pixels globally), and each frame has
been magnified to 720x360 pixels for greater
clarity.  This version provides only the transparent overlay.</Abstract>
              <LegendURL width="320" height="90">
                <Format>image/png</Format>
                <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
                 xlink:type="simple"
                 xlink:href="http://svs.gsfc.nasa.gov/vis/a000000/a003100/a003143/lightacc_bar.png"/>
              </LegendURL>
            </Style>
            <Style>
              <Name>composite</Name>
              <Title>Overlay Composited with Background</Title>
              <Abstract>This animation shows an accumulation of daily
lightning climatology values for a typical year. That is, the
first frame shows the number of flashes per square kilometer
that occurred on a typical January 1 during the multi-year data
collection period, the second frame shows the total of Jan 1 and
Jan 2 flashes, the third frame shows Jan 1 through Jan 3, and so
on until the last frame (#365) which shows the total
accumulation for a typical year. As the year progresses, more
and more of the Earth experiences lightning, and hard-hit areas
experience more strikes. The most intense activity is in central
Africa. Areas where no lightning was measured are transparent,
letting the background image show through. The data pixels are
2.5deg on a side (144x72 pixels globally), and each frame has
been magnified to 720x360 pixels for greater
clarity.  This version provides the transparent overlay composited with a background image.</Abstract>
              <LegendURL width="320" height="90">
                <Format>image/png</Format>
                <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
                 xlink:type="simple"
                 xlink:href="http://svs.gsfc.nasa.gov/vis/a000000/a003100/a003143/lightacc_bar.png"/>
              </LegendURL>
            </Style>
          </Layer>
          <Layer opaque="1" noSubsets="1" fixedWidth="144" fixedHeight="72">
            <Name>3143_21314_bg</Name>
            <Title>Background Image for Global Lightning Accumulation (WMS)</Title>
            <Abstract>Lightning is a brief but intense electrical discharge between positive and negative regions of a thunderstorm.  The Lightning Imaging Sensor (LIS) on the Tropical Rainfall Measuring Mission (TRMM) satellite was designed to study the distribution and variability of total lightning on a global basis. The Optical Transient Detector (OTD) was an earlier lightning detector flying aboard the Microlab-1 spacecraft.  The data shown here are compiled from LIS (1998-2002) and OTD (1995-1999) observations. Because each satellite saw only a part of the Earth at any one time, these data use complex algorithms to estimate total flash rate based on the flashes observed and the amount of time the satellite views each area.
NOTE: This animation is primarily designed to be used through the Web Mapping Services (WMS) protocol.  Each frame in the animation actually represents an accumulation of a number of years of data up through a particular day of the year.  Because of a limitation in the WMS protocol, each frame is marked only with a single date representing the last date for which the data was accumulated.

This image can be composited with the previous animation.</Abstract>
            <KeywordList>
              <Keyword vocabulary="DLESE">Atmospheric science</Keyword>
              <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Electricity:Lightning</Keyword>
              <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Phenomena:Lightning</Keyword>
              <Keyword vocabulary="GCMD">Location:Global</Keyword>
            </KeywordList>
            <CRS>CRS:84</CRS>
            <EX_GeographicBoundingBox>
              <westBoundLongitude>-180</westBoundLongitude>
              <eastBoundLongitude>180</eastBoundLongitude>
              <southBoundLatitude>-90</southBoundLatitude>
              <northBoundLatitude>90</northBoundLatitude>
            </EX_GeographicBoundingBox>
            <BoundingBox CRS="CRS:84" minx="-180" miny="-90" maxx="180" maxy="90"/>
            <MetadataURL type="FGDC:1998">
              <Format>text/plain</Format>
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               xlink:type="simple"
               xlink:href="http://svs.gsfc.nasa.gov/vis/a000000/a003100/a003143/a003143.fgdc"/>
            </MetadataURL>
            <DataURL>
              <Format>text/html</Format>
              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
               xlink:type="simple"
               xlink:href="http://thunder.nsstc.nasa.gov/primer/"/>
            </DataURL>
          </Layer>
          <Layer opaque="0" noSubsets="1" fixedWidth="720" fixedHeight="360">
            <Name>3143_21313</Name>
            <Title>Medium Resolution (720x360 Animation)</Title>
            <Abstract>Lightning is a brief but intense electrical discharge between positive and negative regions of a thunderstorm.  The Lightning Imaging Sensor (LIS) on the Tropical Rainfall Measuring Mission (TRMM) satellite was designed to study the distribution and variability of total lightning on a global basis. The Optical Transient Detector (OTD) was an earlier lightning detector flying aboard the Microlab-1 spacecraft.  The data shown here are compiled from LIS (1998-2002) and OTD (1995-1999) observations. Because each satellite saw only a part of the Earth at any one time, these data use complex algorithms to estimate total flash rate based on the flashes observed and the amount of time the satellite views each area.
NOTE: This animation is primarily designed to be used through the Web Mapping Services (WMS) protocol.  Each frame in the animation actually represents an accumulation of a number of years of data up through a particular day of the year.  Because of a limitation in the WMS protocol, each frame is marked only with a single date representing the last date for which the data was accumulated.</Abstract>
            <KeywordList>
              <Keyword vocabulary="DLESE">Atmospheric science</Keyword>
              <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Electricity:Lightning</Keyword>
              <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Phenomena:Lightning</Keyword>
              <Keyword vocabulary="GCMD">Location:Global</Keyword>
            </KeywordList>
            <CRS>CRS:84</CRS>
            <EX_GeographicBoundingBox>
              <westBoundLongitude>-180</westBoundLongitude>
              <eastBoundLongitude>180</eastBoundLongitude>
              <southBoundLatitude>-90</southBoundLatitude>
              <northBoundLatitude>90</northBoundLatitude>
            </EX_GeographicBoundingBox>
            <BoundingBox CRS="CRS:84" minx="-180" miny="-90" maxx="180" maxy="90"/>
            <Dimension name="time" units="ISO8601" default="2002-12-31">2002-01-01/2002-06-29/P1D,2002-06-31,2002-07-01/2002-12-31/P1D</Dimension>
            <MetadataURL type="FGDC:1998">
              <Format>text/plain</Format>
              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
               xlink:type="simple"
               xlink:href="http://svs.gsfc.nasa.gov/vis/a000000/a003100/a003143/a003143.fgdc"/>
            </MetadataURL>
            <DataURL>
              <Format>text/html</Format>
              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
               xlink:type="simple"
               xlink:href="http://thunder.nsstc.nasa.gov/primer/"/>
            </DataURL>
            <Style>
              <Name>overlay</Name>
              <Title>Transparent Overlay Only</Title>
              <Abstract>This animation shows an accumulation of daily
lightning climatology values for a typical year. That is, the
first frame shows the number of flashes per square kilometer
that occurred on a typical January 1 during the multi-year data
collection period, the second frame shows the total of Jan 1 and
Jan 2 flashes, the third frame shows Jan 1 through Jan 3, and so
on until the last frame (#365) which shows the total
accumulation for a typical year. As the year progresses, more
and more of the Earth experiences lightning, and hard-hit areas
experience more strikes. The most intense activity is in central
Africa. Areas where no lightning was measured are transparent,
letting the background image show through. The data pixels are
2.5deg on a side (144x72 pixels globally), and each frame has
been magnified to 720x360 pixels for greater
clarity.  This version provides only the transparent overlay.</Abstract>
              <LegendURL width="320" height="90">
                <Format>image/png</Format>
                <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
                 xlink:type="simple"
                 xlink:href="http://svs.gsfc.nasa.gov/vis/a000000/a003100/a003143/lightacc_bar.png"/>
              </LegendURL>
            </Style>
            <Style>
              <Name>composite</Name>
              <Title>Overlay Composited with Background</Title>
              <Abstract>This animation shows an accumulation of daily
lightning climatology values for a typical year. That is, the
first frame shows the number of flashes per square kilometer
that occurred on a typical January 1 during the multi-year data
collection period, the second frame shows the total of Jan 1 and
Jan 2 flashes, the third frame shows Jan 1 through Jan 3, and so
on until the last frame (#365) which shows the total
accumulation for a typical year. As the year progresses, more
and more of the Earth experiences lightning, and hard-hit areas
experience more strikes. The most intense activity is in central
Africa. Areas where no lightning was measured are transparent,
letting the background image show through. The data pixels are
2.5deg on a side (144x72 pixels globally), and each frame has
been magnified to 720x360 pixels for greater
clarity.  This version provides the transparent overlay composited with a background image.</Abstract>
              <LegendURL width="320" height="90">
                <Format>image/png</Format>
                <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
                 xlink:type="simple"
                 xlink:href="http://svs.gsfc.nasa.gov/vis/a000000/a003100/a003143/lightacc_bar.png"/>
              </LegendURL>
            </Style>
          </Layer>
          <Layer opaque="1" noSubsets="1" fixedWidth="720" fixedHeight="360">
            <Name>3143_21313_bg</Name>
            <Title>Background Image for Global Lightning Accumulation (WMS)</Title>
            <Abstract>Lightning is a brief but intense electrical discharge between positive and negative regions of a thunderstorm.  The Lightning Imaging Sensor (LIS) on the Tropical Rainfall Measuring Mission (TRMM) satellite was designed to study the distribution and variability of total lightning on a global basis. The Optical Transient Detector (OTD) was an earlier lightning detector flying aboard the Microlab-1 spacecraft.  The data shown here are compiled from LIS (1998-2002) and OTD (1995-1999) observations. Because each satellite saw only a part of the Earth at any one time, these data use complex algorithms to estimate total flash rate based on the flashes observed and the amount of time the satellite views each area.
NOTE: This animation is primarily designed to be used through the Web Mapping Services (WMS) protocol.  Each frame in the animation actually represents an accumulation of a number of years of data up through a particular day of the year.  Because of a limitation in the WMS protocol, each frame is marked only with a single date representing the last date for which the data was accumulated.

This image can be composited with the previous animation.</Abstract>
            <KeywordList>
              <Keyword vocabulary="DLESE">Atmospheric science</Keyword>
              <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Electricity:Lightning</Keyword>
              <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Phenomena:Lightning</Keyword>
              <Keyword vocabulary="GCMD">Location:Global</Keyword>
            </KeywordList>
            <CRS>CRS:84</CRS>
            <EX_GeographicBoundingBox>
              <westBoundLongitude>-180</westBoundLongitude>
              <eastBoundLongitude>180</eastBoundLongitude>
              <southBoundLatitude>-90</southBoundLatitude>
              <northBoundLatitude>90</northBoundLatitude>
            </EX_GeographicBoundingBox>
            <BoundingBox CRS="CRS:84" minx="-180" miny="-90" maxx="180" maxy="90"/>
            <MetadataURL type="FGDC:1998">
              <Format>text/plain</Format>
              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
               xlink:type="simple"
               xlink:href="http://svs.gsfc.nasa.gov/vis/a000000/a003100/a003143/a003143.fgdc"/>
            </MetadataURL>
            <DataURL>
              <Format>text/html</Format>
              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
               xlink:type="simple"
               xlink:href="http://thunder.nsstc.nasa.gov/primer/"/>
            </DataURL>
          </Layer>
        </Layer>
        <Layer opaque="0" noSubsets="1" fixedWidth="680" fixedHeight="300">
          <Name>3133_21151</Name>
          <Title>Transatlantic Dust from North Africa (680x300 Animation)</Title>
          <Abstract>Desert storms in northern Africa raise dust that is carried in the upper atmosphere across the Atlantic Ocean. The dust, which may carry potentially hazardous bacteria and fungi, can land as far west as the Carribean and the Americas.</Abstract>
          <KeywordList>
            <Keyword vocabulary="DLESE">Atmospheric science</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Aerosols:Aerosol Radiance</Keyword>
          </KeywordList>
          <CRS>CRS:84</CRS>
          <EX_GeographicBoundingBox>
            <westBoundLongitude>-130</westBoundLongitude>
            <eastBoundLongitude>82.5</eastBoundLongitude>
            <southBoundLatitude>-15</southBoundLatitude>
            <northBoundLatitude>60</northBoundLatitude>
          </EX_GeographicBoundingBox>
          <BoundingBox CRS="CRS:84" minx="-130" miny="-15" maxx="82.5" maxy="60"/>
          <Dimension name="time" units="ISO8601" default="2000-07-31">2000-07-01/2000-07-31/P1D</Dimension>
          <Attribution>
            <Title>National Aeronautics and Space Administration</Title>
            <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
             xlink:type="simple"
             xlink:href="http://svs.gsfc.nasa.gov/vis/a000000/a003100/a003133/"/>
            <LogoURL width="312" height="258">
              <Format>image/png</Format>
              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
               xlink:type="simple"
               xlink:href="http://svs.gsfc.nasa.gov/svs_icons/nasalogo.png"/>
            </LogoURL>
          </Attribution>
          <MetadataURL type="FGDC:1998">
            <Format>text/plain</Format>
            <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
             xlink:type="simple"
             xlink:href="http://svs.gsfc.nasa.gov/vis/a000000/a003100/a003133/a003133.fgdc"/>
          </MetadataURL>
          <Style>
            <Name>overlay</Name>
            <Title>Transparent Overlay Only</Title>
            <Abstract>This animation shows aerosol index over northern Africa and the Atlantic Ocean from July 1 through July 31, 2000. Each image pixel corresponds to an area 1 degree in longitude by 1.25 degrees in latitude.</Abstract>
            <LegendURL width="320" height="90">
              <Format>image/png</Format>
              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
               xlink:type="simple"
               xlink:href="http://svs.gsfc.nasa.gov/vis/a000000/a003100/a003133/aerosols2000_bar.png"/>
            </LegendURL>
          </Style>
        </Layer>
        <Layer opaque="0" noSubsets="1" fixedWidth="640" fixedHeight="384">
          <Name>3132_21145</Name>
          <Title>Aerosols from 2003 Southern California Fires (640x384 Animation)</Title>
          <Abstract>A devastating series of fires occurred in Southern California during October 2003. The effects of these fires were detectable from space. The Total Ozone Mapping Spectrometer (TOMS) instrument measures aerosol particles (microscopic airborne dust and smoke). TOMS was able to detect aerosols from these fires moving West over the Pacific Ocean and East over the continental United States.</Abstract>
          <KeywordList>
            <Keyword vocabulary="DLESE">Atmospheric science</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Aerosols:Aerosol Radiance</Keyword>
          </KeywordList>
          <CRS>CRS:84</CRS>
          <EX_GeographicBoundingBox>
            <westBoundLongitude>-160</westBoundLongitude>
            <eastBoundLongitude>-60</eastBoundLongitude>
            <southBoundLatitude>10</southBoundLatitude>
            <northBoundLatitude>58</northBoundLatitude>
          </EX_GeographicBoundingBox>
          <BoundingBox CRS="CRS:84" minx="-160" miny="10" maxx="-60" maxy="58"/>
          <Dimension name="time" units="ISO8601" default="2003-11-01">2003-10-23/2003-11-01/P1D</Dimension>
          <Attribution>
            <Title>National Aeronautics and Space Administration</Title>
            <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
             xlink:type="simple"
             xlink:href="http://svs.gsfc.nasa.gov/vis/a000000/a003100/a003132/"/>
            <LogoURL width="312" height="258">
              <Format>image/png</Format>
              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
               xlink:type="simple"
               xlink:href="http://svs.gsfc.nasa.gov/svs_icons/nasalogo.png"/>
            </LogoURL>
          </Attribution>
          <MetadataURL type="FGDC:1998">
            <Format>text/plain</Format>
            <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
             xlink:type="simple"
             xlink:href="http://svs.gsfc.nasa.gov/vis/a000000/a003100/a003132/a003132.fgdc"/>
          </MetadataURL>
          <DataURL>
            <Format>text/html</Format>
            <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
             xlink:type="simple"
             xlink:href="http://toms.gsfc.nasa.gov/aerosols/aerosols.html"/>
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            <Abstract>This animation shows aerosol index over the western US from Oct 23 through November 1, 2003. Each image pixel corresponds to an area 1 degree in longitude by 1.25 degrees in latitude.</Abstract>
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          <Title>Continental Effects of 2004 Alaskan Fires (904x384 Animation)</Title>
          <Abstract>Wildfires started by lightning burned more than 80,000 acres in Alaska in June 2004. The effects of these fires can be seen across North America with the Total Ozone Mapping Spectrometer (TOMS) instrument on the Earth Probe spacecraft. TOMS detects the presence of UV-absorbing tropospheric aerosols across the globe.</Abstract>
          <KeywordList>
            <Keyword vocabulary="DLESE">Atmospheric science</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Aerosols:Aerosol Radiance</Keyword>
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          <CRS>CRS:84</CRS>
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          <Attribution>
            <Title>National Aeronautics and Space Administration</Title>
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            <Abstract>This animation shows aerosol index over Alaska from June 21 through July 10, 2004. Each image pixel corresponds to an area 1 degree in longitude by 1.25 degrees in latitude.</Abstract>
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          <Title>Daily Erythemal Index (UV exposure) for 2000-2001 (288x180 Animation)</Title>
          <Abstract>The Erythemal Index is a measure of ultraviolet (UV) radiation at ground level on the Earth. (The word 'erythema' means an abnormal redness of the skin, such as is caused by spending too much time in the sun--a sunburn is damage to your skin cells caused by UV radiation.) Atmospheric ozone shields life at the surface from most of the harmful components of solar radiation. Chemical processes in the atmosphere can affect the level of protection provided by the ozone in the upper atmosphere. This thinning of the atmospheric ozone in the stratosphere leads to elevated levels of UV at ground level and increases the risks of DNA damage in living organisms.</Abstract>
          <KeywordList>
            <Keyword vocabulary="DLESE">Atmospheric science</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Ultraviolet Radiation</Keyword>
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          <Attribution>
            <Title>National Aeronautics and Space Administration</Title>
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            <Abstract>This animation shows daily erythemal index for 2000-01 through 2001-12. Data gaps have been filled and the frames have been smoothed. The image size is 288x180 pixels (288x176 pixels for the MPEG movie); each pixel corresponds to an area 1 degree in longitude by 1.25 degrees in latitude.</Abstract>
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          <Title>Monthly Average Erythemal Index (UV exposure) for 2000-2001 (288x180 Animation)</Title>
          <Abstract>The Erythemal Index is a measure of ultraviolet (UV) radiation at ground level on the Earth. (The word 'erythema' means an abnormal redness of the skin, such as is caused by spending too much time in the sun--a sunburn is damage to your skin cells caused by UV radiation.) Atmospheric ozone shields life at the surface from most of the harmful components of solar radiation. Chemical processes in the atmosphere can affect the level of protection provided by the ozone in the upper atmosphere. This thinning of the atmospheric ozone in the stratosphere leads to elevated levels of UV at ground level and increases the risks of DNA damage in living organisms.</Abstract>
          <KeywordList>
            <Keyword vocabulary="DLESE">Atmospheric science</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Ultraviolet Radiation</Keyword>
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          <CRS>CRS:84</CRS>
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          <BoundingBox CRS="CRS:84" minx="-180" miny="-90" maxx="180" maxy="90"/>
          <Dimension name="time" units="ISO8601" default="2001-12">2000-01/2001-12/P1M</Dimension>
          <Attribution>
            <Title>National Aeronautics and Space Administration</Title>
            <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
             xlink:type="simple"
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          <Style>
            <Name>overlay</Name>
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            <Abstract>This animation shows monthly average erythemal index for 2000-01 through 2001-12. The image size is 288x180 pixels (288x176 pixels for the MPEG movie); each pixel corresponds to an area 1 degree in longitude by 1.25 degrees in latitude.</Abstract>
            <LegendURL width="320" height="90">
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              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
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          <Name>3114_21621</Name>
          <Title>Daily Erythemal Index (UV exposure) Measurements for 2000-2001 (288x180 Animation)</Title>
          <Abstract>The Erythemal Index is a measure of ultraviolet (UV) radiation at ground level on the Earth. (The word 'erythema' means an abnormal redness of the skin, such as is caused by spending too much time in the sun--a sunburn is damage to your skin cells caused by UV radiation.) Atmospheric ozone shields life at the surface from most of the harmful components of solar radiation. Chemical processes in the atmosphere can affect the level of protection provided by the ozone in the upper atmosphere. This thinning of the atmospheric ozone in the stratosphere leads to elevated levels of UV at ground level and increases the risks of DNA damage in living organisms.</Abstract>
          <KeywordList>
            <Keyword vocabulary="DLESE">Atmospheric science</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Ultraviolet Radiation</Keyword>
          </KeywordList>
          <CRS>CRS:84</CRS>
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          <BoundingBox CRS="CRS:84" minx="-180" miny="-90" maxx="180" maxy="90"/>
          <Dimension name="time" units="ISO8601" default="2001-12-31">2000-01-01/2001-12-31/P1D</Dimension>
          <Attribution>
            <Title>National Aeronautics and Space Administration</Title>
            <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
             xlink:type="simple"
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          <Style>
            <Name>opaque</Name>
            <Title>Opaque</Title>
            <Abstract>This animation shows daily erythemal index for 2000-01-01 through 2001-12-31. Each days image is built up from observations taken near local solar noon; the western Pacific is measured near the beginning of the day (in Greenwich Mean Time - GMT), and the eastern Pacific is measured near the end of the GMT day. There is a 24-hour discontinuity in the data at 180th meridian. Diagonal bands with no data are areas that the satellite did not view on a particular day. The image size is 288x180 pixels (288x176 pixels for the MPEG movie); each pixel corresponds to an area 1 degree in longitude by 1.25 degrees in latitude.</Abstract>
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              <Format>image/png</Format>
              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
               xlink:type="simple"
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        </Layer>
        <Layer opaque="0" noSubsets="1" fixedWidth="369" fixedHeight="491">
          <Name>3110_20956</Name>
          <Title>Vegetation Images Show Drought in Western US (369x491 Animation)</Title>
          <Abstract>Satellite data can gauge the health of plants, which is a good indicator of drought. The Normalized Difference Vegetation Index (NDVI) measures how dense and green plant leaves are. NDVI images are useful as a measure of drought when compared to 'normal' plant health. Scientists calculate average NDVI values for an area to find out what is normal at a particular time of year. This animation uses satellite imagery to show changes in vegetation between 1999 and 2003. In 2002, drought had settled across the Midwest. Large dark brown sections of eastern Colorado show where vegetation was less lush and healthy than normal. This version of the visualization is a wide view showing the western United States. The data were measured by the vegetation instrument on Europe's SPOT-4 satellite, and were provided by DigitalGlobe/SPOT under agreement with the U.S. Department of Agriculture Foreign Agricultural Service (USDA/FAS).</Abstract>
          <KeywordList>
            <Keyword vocabulary="DLESE">Climatology</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Phenomena:Drought</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Biosphere:Vegetation:Vegetation Index</Keyword>
          </KeywordList>
          <CRS>CRS:84</CRS>
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          <Dimension name="time" units="ISO8601" default="2003-09-30">1999-06-10/1999-07-20/P10D,1999-07-31/1999-08-20/P10D,1999-08-31/1999-09-30/P10D,2000-06-10/2000-07-20/P10D,2000-07-31/2000-08-20/P10D,2000-08-31/2000-09-30/P10D,2001-06-10/2001-07-20/P10D,2001-07-31/2001-08-20/P10D,2001-08-31/2001-09-30/P10D,2002-06-10/2002-07-20/P10D,2002-07-31/2002-08-20/P10D,2002-08-31/2002-09-30/P10D,2003-06-10/2003-07-20/P10D,2003-07-31/2003-08-20/P10D,2003-08-31/2003-09-30/P10D</Dimension>
          <Attribution>
            <Title>National Aeronautics and Space Administration</Title>
            <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
             xlink:type="simple"
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          <Style>
            <Name>overlay</Name>
            <Title>Transparent Overlay Only</Title>
            <Abstract>This animation shows NDVI over the western US in ten-day intervals from 1999-06-10 through 2003-09-30. The area shown extends from California to Colorado, and from Canada to Mexico. The horizontal scale is 0.0735 degrees-pixel in the E-W direction and 0.0450 degrees-pixel N-S.</Abstract>
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              <Format>image/png</Format>
              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
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        <Layer opaque="0" noSubsets="1" fixedWidth="512" fixedHeight="256">
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          <Title>Solar Irradiance (512x256 Animation)</Title>
          <Abstract>The Earth's climate is determined by energy transfer from the sun to the Earth's land, oceans, and atmosphere.  As the Earth moves around the sun, the fact that the Earth's axis is tilted means that the sun's overhead position moves from the Northern Hemisphere to the Southern Hemisphere and back from one summer to the next.  This effect causes winters to be cold and summers warm in the Northern Hemisphere and the opposite in the Southern Hemisphere.  This animation shows the incoming solar irradiance on the Earth at noon on the Greenwich meridian during an entire year, illustrating this movement.  The magnitude of this irradiance comes from measurements by the TIM instrument on SORCE.  Since the Earth's orbit is elliptical, the magnitude of the solar irradiance at the Earth is least when the Earth is farthest from the sun and greatest when the earth is closest.  This 6 or 7 percent change can be seen in the animation by watching the dark bands move.  When the bands expand from the bright spot, the Earth is getting closer to the sun, from July through December, and when they contract the Earth is moving away, from January through June.  The sun's irradiance is also variable from day to day, but that effect is about ten times smaller than the effect of the earth's orbit.</Abstract>
          <KeywordList>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Incoming Solar Radiation</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Solar Irradiance</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Sun-earth Interactions:Solar Activity:Solar Irradiance</Keyword>
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          <Dimension name="time" units="ISO8601" default="2004-06-19T12:00:00Z">2003-06-20T12:00:00Z/2004-06-19T12:00:00Z/P1D</Dimension>
          <Attribution>
            <Title>National Aeronautics and Space Administration</Title>
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             xlink:href="http://lasp.colorado.edu/sorce/"/>
          </DataURL>
          <Style>
            <Name>overlay</Name>
            <Title>Transparent Overlay Only</Title>
            <Abstract>This animation shows the solar radiance on the Earth
at noon on the Greenwich meriidian for June 20, 2003 through June 19, 2004
as calculated from measurements made by the TIM instrument on SORCE.</Abstract>
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              <Format>image/png</Format>
              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
               xlink:type="simple"
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          <Name>3108_21485</Name>
          <Title>Instantaneous Outgoing Shortwave Flux (1024x512 Animation)</Title>
          <Abstract>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.</Abstract>
          <KeywordList>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Shortwave Radiation</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Oceans:Ocean Heat Budget:Shortwave Radiation</Keyword>
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          <CRS>CRS:84</CRS>
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          <BoundingBox CRS="CRS:84" minx="-180" miny="-90" maxx="180" maxy="90"/>
          <Dimension name="time" units="ISO8601" default="2003-06-22T00:56Z">2003-06-20T02:44Z/2003-06-22T00:56Z/PT1H39M</Dimension>
          <Attribution>
            <Title>National Aeronautics and Space Administration</Title>
            <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
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             xlink:type="simple"
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          </DataURL>
          <Style>
            <Name>opaque</Name>
            <Title>Opaque</Title>
            <Abstract>This animation shows 29 orbits (2 days) of CERES
measurements of outgoing shortwave radiation, from June 20-21, 2003.</Abstract>
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              <Format>image/png</Format>
              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
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          <Name>3107_21484</Name>
          <Title>Instantaneous Outgoing Longwave Flux (1024x512 Animation)</Title>
          <Abstract>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.</Abstract>
          <KeywordList>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Outgoing Longwave Radiation</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Oceans:Ocean Heat Budget:Longwave Radiation</Keyword>
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            <Abstract>This animation shows 29 orbits (2 days) of CERES
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          <Title>Instantaneous Net Radiation Flux (1024x512 Animation)</Title>
          <Abstract>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.</Abstract>
          <KeywordList>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Net Radiation</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Radiative Flux</Keyword>
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            <Abstract>This animation shows net radiation flux corresponding
to 29 orbits (2 days) of CERES measurements, from June 20-21, 2003.  This data
is calculated from CERES outgoing longwave and shortwave measurements, along
with a corresponding calculated incoming solar flux.</Abstract>
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          <Name>3105_20926</Name>
          <Title>Instantaneous Incoming Solar Flux (1024x512 Animation)</Title>
          <Abstract>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.</Abstract>
          <KeywordList>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Incoming Solar Radiation</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Solar Irradiance</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Sun-earth Interactions:Solar Activity:Solar Irradiance</Keyword>
          </KeywordList>
          <CRS>CRS:84</CRS>
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            <Abstract>This animation shows incoming solar flux corresponding
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coupled with solar incidence angles based on CERES measurement locations and
times.</Abstract>
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              <Format>image/png</Format>
              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
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        <Layer opaque="0" noSubsets="1" fixedWidth="1024" fixedHeight="512">
          <Name>3104_20920</Name>
          <Title>Instantaneous Scene Identification (1024x512 Animation)</Title>
          <Abstract>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.</Abstract>
          <KeywordList>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Reflectance</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Clouds:Cloud Reflectance</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Cryosphere:Sea Ice:Reflectance</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Land Surface:Surface Radiative Properties:Reflectance</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Oceans:Ocean Heat Budget:Reflectance</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Oceans:Sea Ice:Reflectance</Keyword>
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          <CRS>CRS:84</CRS>
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          <Attribution>
            <Title>National Aeronautics and Space Administration</Title>
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          <Style>
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            <Abstract>This animation shows 29 orbits (2 days) of CERES
measurements of regions of solar reflectivity, from June 20-21, 2003.</Abstract>
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              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
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          <Title>Temperature from new Microwave Limb Sounder on Aura (72x89 Animation)</Title>
          <KeywordList>
            <Keyword vocabulary="DLESE">Atmospheric science</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Temperature:Air Temperature</Keyword>
            <Keyword vocabulary="GCMD">Location:Global</Keyword>
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          <Attribution>
            <Title>National Aeronautics and Space Administration</Title>
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            <Abstract>This animation shows temperature in the atmosphere from August 13 through October 15, 2004. Red represents higher temperatures; blue represents lower temperatures. The spatial resolution is low: each pixel covers an area of 5 degrees longitude by 2 degrees latitude, so the entire world (except for 1 degree at each pole) is covered by the 72x89 pixel images.</Abstract>
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          <KeywordList>
            <Keyword vocabulary="DLESE">Atmospheric science</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Water Vapor:Water Vapor</Keyword>
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          <Attribution>
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            <Abstract>This animation shows water vapor (H2O) in the atmosphere from August 13 through October 15, 2004. Red represents high concentrations; blue represents low concentrations. The spatial resolution is low: each pixel covers an area of 5 degrees longitude by 2 degrees latitude, so the entire world (except for 1 degree at each pole) is covered by the 72x89 pixel images.</Abstract>
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          <Abstract>Nitric Acid (HNO3) in the atmosphere as measured by the Microwave Limb Sounder (MLS) instrument on NASA's Aura satellite. MLS can simultaneously measure several trace gases and ozone-destroying chemicals in the upper troposphere and photosphere. In this series of animiations we present chlorine monoxide (ClO), hydrogen chloride (HCl), nitric acid (HNO3), ozone (O3), water vapor (H2O) and temperature measurements. These are 'first light' data taken when the MLS was operated for the first time. Nitric acid is created from the nitrogen oxide emitted by automobiles.</Abstract>
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            <Keyword vocabulary="DLESE">Atmospheric science</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Chemistry/Nitrogen Compounds:Nitric Acid</Keyword>
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             xlink:type="simple"
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          </DataURL>
          <Style>
            <Name>opaque</Name>
            <Title>Opaque</Title>
            <Abstract>This animation shows nitric acid (HNO3) in the atmosphere from August 13 through October 15, 2004. Red represents high concentrations; blue represents low concentrations. The spatial resolution is low: each pixel covers an area of 5 degrees longitude by 2 degrees latitude, so the entire world (except for 1 degree at each pole) is covered by the 72x89 pixel images.</Abstract>
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              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
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          <Title>Hydrogen Chloride from new Microwave Limb Sounder on Aura (72x89 Animation)</Title>
          <Abstract>Hydrogen chloride (HCl) in the atmosphere as measured by the Microwave Limb Sounder (MLS) instrument on NASA's Aura satellite. MLS can simultaneously measure several trace gases and ozone-destroying chemicals in the upper troposphere and photosphere. In this series of animiations we present chlorine monoxide (ClO), hydrogen chloride (HCl), nitric acid (HNO3), ozone (O3), water vapor (H2O) and temperature measurements. These are 'first light' data taken when the MLS was operated for the first time. Ozone-destroying chlorine (Cl) atoms are neutralized when they bond with hydrogen (H) to form HCl.</Abstract>
          <KeywordList>
            <Keyword vocabulary="DLESE">Atmospheric science</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Chemistry/Halons and Halogens:Hydrogen Chloride</Keyword>
            <Keyword vocabulary="GCMD">Location:Global</Keyword>
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          <CRS>CRS:84</CRS>
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          <BoundingBox CRS="CRS:84" minx="-180" miny="-89" maxx="180" maxy="89"/>
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          <Attribution>
            <Title>National Aeronautics and Space Administration</Title>
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          <Style>
            <Name>opaque</Name>
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            <Abstract>This animation shows hydrogen chloride (HCl) in the atmosphere from August 13 through October 15, 2004. Red represents high concentrations; blue represents low concentrations. The spatial resolution is low: each pixel covers an area of 5 degrees longitude by 2 degrees latitude, so the entire world (except for 1 degree at each pole) is covered by the 72x89 pixel images.</Abstract>
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        <Layer opaque="1" noSubsets="1">
          <Title>Polar Vortex</Title>
          <Abstract>The polar vortex is an atmospheric regional event that isolates polar air from the air at temperate latitudes, producing conditions favorable for wintertime polar ozone depletion and other chemical perturbations.  The location, size, and shape of the polar vortex is derived from potential vorticity (PV) data.</Abstract>
          <KeywordList>
            <Keyword vocabulary="SVS">Atmosphere</Keyword>
            <Keyword vocabulary="SVS">Pole</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Winds:Vorticity</Keyword>
            <Keyword vocabulary="GCMD">Location:Antarctica</Keyword>
          </KeywordList>
          <Attribution>
            <Title>National Aeronautics and Space Administration</Title>
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          </MetadataURL>
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            <Name>3098_20877</Name>
            <Title>Polar Vortex (1024x512 Animation)</Title>
            <Abstract>The polar vortex is an atmospheric regional event that isolates polar air from the air at temperate latitudes, producing conditions favorable for wintertime polar ozone depletion and other chemical perturbations.  The location, size, and shape of the polar vortex is derived from potential vorticity (PV) data.</Abstract>
            <KeywordList>
              <Keyword vocabulary="SVS">Atmosphere</Keyword>
              <Keyword vocabulary="SVS">Pole</Keyword>
              <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Winds:Vorticity</Keyword>
              <Keyword vocabulary="GCMD">Location:Antarctica</Keyword>
            </KeywordList>
            <CRS>CRS:84</CRS>
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              <westBoundLongitude>-180</westBoundLongitude>
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            <Style>
              <Name>overlay</Name>
              <Title>Transparent Overlay Only</Title>
              <Abstract>This animation shows a flat map version of the southern polar vortex at 550 degrees Kelvin during part of 2004.  This version provides only the transparent overlay.</Abstract>
            </Style>
            <Style>
              <Name>composite</Name>
              <Title>Overlay Composited with Background</Title>
              <Abstract>This animation shows a flat map version of the southern polar vortex at 550 degrees Kelvin during part of 2004.  This version provides the transparent overlay composited with a background image.</Abstract>
            </Style>
          </Layer>
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            <Name>3098_20877_bg</Name>
            <Title>Background Image for Polar Vortex (WMS)</Title>
            <Abstract>The polar vortex is an atmospheric regional event that isolates polar air from the air at temperate latitudes, producing conditions favorable for wintertime polar ozone depletion and other chemical perturbations.  The location, size, and shape of the polar vortex is derived from potential vorticity (PV) data.

This image can be composited with the previous animation.</Abstract>
            <KeywordList>
              <Keyword vocabulary="SVS">Atmosphere</Keyword>
              <Keyword vocabulary="SVS">Pole</Keyword>
              <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Winds:Vorticity</Keyword>
              <Keyword vocabulary="GCMD">Location:Antarctica</Keyword>
            </KeywordList>
            <CRS>CRS:84</CRS>
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          <Name>3097_20871</Name>
          <Title>Average Total-sky Outgoing Shortwave Flux (144x72 Animation)</Title>
          <Abstract>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.</Abstract>
          <KeywordList>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Shortwave Radiation</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Oceans:Ocean Heat Budget:Shortwave Radiation</Keyword>
          </KeywordList>
          <CRS>CRS:84</CRS>
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          <BoundingBox CRS="CRS:84" minx="-180" miny="-90" maxx="180" maxy="90"/>
          <Dimension name="time" units="ISO8601" default="2004-06">2002-07/2004-06/P1M</Dimension>
          <Attribution>
            <Title>National Aeronautics and Space Administration</Title>
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          </DataURL>
          <Style>
            <Name>overlay</Name>
            <Title>Transparent Overlay Only</Title>
            <Abstract>This animation shows the monthly average total-sky outgoing
shortwave flux from CERES for July 2002 through June 2004.</Abstract>
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              <Format>image/png</Format>
              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
               xlink:type="simple"
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          <Name>3096_20865</Name>
          <Title>Average Clear-sky Outgoing Shortwave Flux (144x72 Animation)</Title>
          <Abstract>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.</Abstract>
          <KeywordList>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Shortwave Radiation</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Oceans:Ocean Heat Budget:Shortwave Radiation</Keyword>
          </KeywordList>
          <CRS>CRS:84</CRS>
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          <BoundingBox CRS="CRS:84" minx="-180" miny="-90" maxx="180" maxy="90"/>
          <Dimension name="time" units="ISO8601" default="2004-06">2002-07/2004-06/P1M</Dimension>
          <Attribution>
            <Title>National Aeronautics and Space Administration</Title>
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          <Style>
            <Name>overlay</Name>
            <Title>Transparent Overlay Only</Title>
            <Abstract>This animation shows the monthly average clear-sky outgoing
shortwave flux from CERES for July 2002 through June 2004.</Abstract>
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              <Format>image/png</Format>
              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
               xlink:type="simple"
               xlink:href="http://svs.gsfc.nasa.gov/vis/a000000/a003000/a003096/swflxclsbar.0000.png"/>
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        </Layer>
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          <Name>3095_20859</Name>
          <Title>Average Total-sky Incoming Solar Flux (144x72 Animation)</Title>
          <Abstract>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 contant 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.</Abstract>
          <KeywordList>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Incoming Solar Radiation</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Solar Irradiance</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Sun-earth Interactions:Solar Activity:Solar Irradiance</Keyword>
          </KeywordList>
          <CRS>CRS:84</CRS>
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            <westBoundLongitude>-180</westBoundLongitude>
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          <Attribution>
            <Title>National Aeronautics and Space Administration</Title>
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          <Style>
            <Name>overlay</Name>
            <Title>Transparent Overlay Only</Title>
            <Abstract>This animation shows the monthly average total-sky incoming solar flux
from CERES for July 2002 through June 2004.</Abstract>
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              <Format>image/png</Format>
              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
               xlink:type="simple"
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          <Name>3094_20853</Name>
          <Title>Average Total-sky Net Radiant Flux (144x72 Animation)</Title>
          <Abstract>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.</Abstract>
          <KeywordList>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Net Radiation</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Radiative Flux</Keyword>
          </KeywordList>
          <CRS>CRS:84</CRS>
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          <Attribution>
            <Title>National Aeronautics and Space Administration</Title>
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          <Style>
            <Name>overlay</Name>
            <Title>Transparent Overlay Only</Title>
            <Abstract>This animation shows the monthly average total-sky net
radiant flux from CERES for July 2002 through June 2004.</Abstract>
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              <Format>image/png</Format>
              <OnlineResource xmlns:xlink="http://www.w3.org/1999/xlink" 
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          <Title>Average Clear-sky Net Radiant Flux (144x72 Animation)</Title>
          <Abstract>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.</Abstract>
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            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Net Radiation</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Radiative Flux</Keyword>
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          <Name>3092_20841</Name>
          <Title>Average Total-sky Outgoing Longwave Flux (144x72 Animation)</Title>
          <Abstract>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.</Abstract>
          <KeywordList>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Outgoing Longwave Radiation</Keyword>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Oceans:Ocean Heat Budget:Longwave Radiation</Keyword>
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            <Abstract>This animation shows the monthly average total-sky outgoing
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          <Title>Average Clear-sky Outgoing Longwave Flux (144x72 Animation)</Title>
          <Abstract>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.</Abstract>
          <KeywordList>
            <Keyword vocabulary="GCMD">EARTH SCIENCE:Atmosphere:Atmospheric Radiation:Outgoing Longwave Radiation</Keyword>
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          <Abstract>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 