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Ozone gas in the stratosphere (upper atmosphere) absorbs ultraviolet light, thus protecting living things from the sun's harmful ultraviolet radiation. Man-made chemicals and weather conditions over Antarctica combine to deplete stratospheric ozone concentrations during the winter months there. (Data from Total Ozone Mapping Spectrometer [TOMS] project). Sensor: TOMS/TOMS. Data Start Date: 1/1/79. Data End Date: 7/31/05.
Topic: What -- Spectrometer
Source: http://visibleearth.nasa.gov/view_rec.php?id=7244
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Ozone gas in the stratosphere (upper atmosphere) absorbs ultraviolet light, thus protecting living things from the sun's harmful ultraviolet radiation. Man-made chemicals and weather conditions over Antarctica combine to deplete stratospheric ozone concentrations during the winter months there. (Data from Total Ozone Mapping Spectrometer [TOMS] project). Sensor: TOMS/TOMS. Data Start Date: 1/1/85. Data End Date: 7/31/05.
Topic: What -- Spectrometer
Source: http://visibleearth.nasa.gov/view_rec.php?id=7245
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Scientists use data from NASA’s Total Ozone Mapping Spectrometer (TOMS) to measure the relative amount of aerosols—solid or liquid particles suspended in the atmosphere. Aerosol types detected by the TOMS Aerosol Index include desert dust, smoke and volcanic ash located at least 2 km (1.2 miles) above the surface.Every day, TOMS measures how much UV radiation is absorbed within the atmosphere and how much is reflected back up into space. These measures directly relate to how much aerosol is...
Topic: What -- Spectrometer
Source: http://visibleearth.nasa.gov/view_rec.php?id=7190
Laser Faint Object Grating Spectrometer (Frogs) with F. Witteborn and Jesse Bregman.
Topic: What -- Spectrometer
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42
Sep 17, 2009
09/09
by
NASA/Glenn Research Center
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MASS SPECTROMETER
Topic: What -- Spectrometer
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Nov 4, 2009
11/09
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Image by Robert Simmon, based on data provided by the Tropospheric Emission Monitoring Internet Service ()
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This image shows a global map of nitrogen dioxide (NO<sub>2</sub>) in the troposphere (lower atmosphere) in 2003, prepared using data collected by the Scanning Imaging Absorption Spectrometer for Atmospheric Chartography (<a href="http://envisat.esa.int/instruments/sciamachy/">SCIAMACHY</a>) instrument aboard the European Space Agency’s <a href="http://envisat.esa.int/">Envisat</a>...
Topic: What -- Spectrometer
Source: http://visibleearth.nasa.gov/view_rec.php?id=16926
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Scientists use data from NASA’s Total Ozone Mapping Spectrometer (TOMS) to measure the relative amount of aerosols—solid or liquid particles suspended in the atmosphere. Aerosol types detected by the TOMS Aerosol Index include desert dust, smoke and volcanic ash located at least 2 km (1.2 miles) above the surface.Every day, TOMS measures how much UV radiation is absorbed within the atmosphere and how much is reflected back up into space. These measures directly relate to how much aerosol is...
Topic: What -- Spectrometer
Source: http://visibleearth.nasa.gov/view_rec.php?id=7197
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Sep 22, 2009
09/09
by
NASA/Langley Research Center (NASA-LaRC)
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The laser inside the interferometer operates under low power, effectively eliminating high voltage dangers. It has ultra-high stability, which allows almost drift-free sampling of the interferogram. This leads to reduced distortion in the spectral data products.
Topic: What -- Spectrometer
Source: http://nix.ksc.nasa.gov/info?id=LV-1998-00021&orgid=1
MASS Spectrometer
Topic: What -- Spectrometer
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Sep 17, 2009
09/09
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NASA/Glenn Research Center
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favorite 0
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MASS SPECTROMETER
Topic: What -- Spectrometer
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Scientists use data from NASA’s Total Ozone Mapping Spectrometer (TOMS) to measure the relative amount of aerosols—solid or liquid particles suspended in the atmosphere. Aerosol types detected by the TOMS Aerosol Index include desert dust, smoke and volcanic ash located at least 2 km (1.2 miles) above the surface.Every day, TOMS measures how much UV radiation is absorbed within the atmosphere and how much is reflected back up into space. These measures directly relate to how much aerosol is...
Topic: What -- Spectrometer
Source: http://visibleearth.nasa.gov/view_rec.php?id=7189
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Ozone gas in the stratosphere (upper atmosphere) absorbs ultraviolet light, thus protecting living things from the sun's harmful ultraviolet radiation. Man-made chemicals and weather conditions over Antarctica combine to deplete stratospheric ozone concentrations during the winter months there. (Data from Total Ozone Mapping Spectrometer [TOMS] project). Sensor: TOMS/TOMS. Data Start Date: 1/1/99. Data End Date: 7/31/05.
Topic: What -- Spectrometer
Source: http://visibleearth.nasa.gov/view_rec.php?id=7236
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Scientists use data from NASA’s Total Ozone Mapping Spectrometer (TOMS) to measure the relative amount of aerosols—solid or liquid particles suspended in the atmosphere. Aerosol types detected by the TOMS Aerosol Index include desert dust, smoke and volcanic ash located at least 2 km (1.2 miles) above the surface.Every day, TOMS measures how much UV radiation is absorbed within the atmosphere and how much is reflected back up into space. These measures directly relate to how much aerosol is...
Topic: What -- Spectrometer
Source: http://visibleearth.nasa.gov/view_rec.php?id=7196
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Ozone gas in the stratosphere (upper atmosphere) absorbs ultraviolet light, thus protecting living things from the sun's harmful ultraviolet radiation. Man-made chemicals and weather conditions over Antarctica combine to deplete stratospheric ozone concentrations during the winter months there. (Data from Total Ozone Mapping Spectrometer [TOMS] project). Sensor: TOMS/TOMS. Data Start Date: 1/1/05. Data End Date: 7/31/05.
Topic: What -- Spectrometer
Source: http://visibleearth.nasa.gov/view_rec.php?id=7224
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Sep 17, 2009
09/09
by
NASA/Glenn Research Center
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INFRARED IMAGING SPECTROMETER
Topic: What -- Spectrometer
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27
Sep 17, 2009
09/09
by
NASA/Glenn Research Center
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eye 27
favorite 0
comment 0
MASS SPECTROMETER
Topic: What -- Spectrometer
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Sep 18, 2009
09/09
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NASA/Glenn Research Center
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LIFE TEST BEARINGS FOR MODERATE RESOLUTION IMAGING SPECTROMETER MODIS PROGRAM
Topic: What -- Spectrometer
Instrumentation used for analysis of elements present in solid and liquid samples from optical, hydraulic, or other test systems on the Langley NASA center.
Topic: What -- Spectrometer
The installation of the Alpha Magnetic Spectrometer and the preparations taken for EVA #1 are among the mission milestones spotlighted on FD4.
Topic: What -- Spectrometer
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Ozone gas in the stratosphere (upper atmosphere) absorbs ultraviolet light, thus protecting living things from the sun's harmful ultraviolet radiation. Man-made chemicals and weather conditions over Antarctica combine to deplete stratospheric ozone concentrations during the winter months there. (Data from Total Ozone Mapping Spectrometer [TOMS] project). Sensor: TOMS/TOMS. Data Start Date: 1/1/82. Data End Date: 7/31/05.
Topic: What -- Spectrometer
Source: http://visibleearth.nasa.gov/view_rec.php?id=7233
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eye 32
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Scientists use data from NASA’s Total Ozone Mapping Spectrometer (TOMS) to measure the relative amount of aerosols—solid or liquid particles suspended in the atmosphere. Aerosol types detected by the TOMS Aerosol Index include desert dust, smoke and volcanic ash located at least 2 km (1.2 miles) above the surface.Every day, TOMS measures how much UV radiation is absorbed within the atmosphere and how much is reflected back up into space. These measures directly relate to how much aerosol is...
Topic: What -- Spectrometer
Source: http://visibleearth.nasa.gov/view_rec.php?id=7207
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Ozone gas in the stratosphere (upper atmosphere) absorbs ultraviolet light, thus protecting living things from the sun's harmful ultraviolet radiation. Man-made chemicals and weather conditions over Antarctica combine to deplete stratospheric ozone concentrations during the winter months there. (Data from Total Ozone Mapping Spectrometer [TOMS] project). Sensor: TOMS/TOMS. Data Start Date: 1/1/90. Data End Date: 7/31/05.
Topic: What -- Spectrometer
Source: http://visibleearth.nasa.gov/view_rec.php?id=7230
This image shows the Chandra X-ray Observatory observation of the sky surrounding the afterglow and host galaxy of the HETE short burst of July 9, 2005. The circle indicates the region of sky from which HETE saw the burst. The box, inset, indicates where the X-ray and optical afterglow of the burst was ultimately found. The bright X-ray afterglow of the burst is apparent in the middle of this box. The colors indicate the intensity of the X-ray emission (1.0-7.0 keV) as seen by the Advanced CCD...
Topic: What -- Spectrometer
Source: http://chandra.harvard.edu/photo/2005/grb050709/more.html
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Sep 17, 2009
09/09
by
NASA/Glenn Research Center
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INFRARED IMAGING SPECTROMETER
Topic: What -- Spectrometer
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Sep 18, 2009
09/09
by
NASA/Glenn Research Center
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eye 32
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LIFE TEST BEARINGS FOR MODERATE RESOLUTION IMAGING SPECTROMETER MODIS PROGRAM
Topic: What -- Spectrometer
Mission Overview Briefing -- JSC (Public, HD and Media Channels) During the 14-day mission, Endeavour will deliver the Alpha Magnetic Spectrometer (AMS) and spare parts including two S-band communications antennas, a high-pressure gas tank, additional spare parts for Dextre and micrometeoroid debris shields. This will be the 36th shuttle mission to the International Space Station.
Topic: What -- Spectrometer
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Ozone gas in the stratosphere (upper atmosphere) absorbs ultraviolet light, thus protecting living things from the sun's harmful ultraviolet radiation. Man-made chemicals and weather conditions over Antarctica combine to deplete stratospheric ozone concentrations during the winter months there. (Data from Total Ozone Mapping Spectrometer [TOMS] project). Sensor: TOMS/TOMS. Data Start Date: 11/1/78. Data End Date: 7/31/05.
Topic: What -- Spectrometer
Source: http://visibleearth.nasa.gov/view_rec.php?id=7240
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Ozone gas in the stratosphere (upper atmosphere) absorbs ultraviolet light, thus protecting living things from the sun's harmful ultraviolet radiation. Man-made chemicals and weather conditions over Antarctica combine to deplete stratospheric ozone concentrations during the winter months there. (Data from Total Ozone Mapping Spectrometer [TOMS] project). Sensor: TOMS/TOMS. Data Start Date: 1/1/86. Data End Date: 7/31/05.
Topic: What -- Spectrometer
Source: http://visibleearth.nasa.gov/view_rec.php?id=7249
This X-ray image of NGC 4697 was observed on January 15, 2000 for 11 hours with the Advanced CCD Imaging Spectrometer (ACIS). Chandra observations of this spiral galaxy and 3 other nearby galaxies have revealed a possible new class of X-ray sources. These mysterious X-ray sources, marked with green diamonds in the version on the left, are called "quasisoft" sources because they have a temperature in the range of one to four million degrees Celsius. Color Code:
Topic: What -- Spectrometer
Source: http://chandra.harvard.edu/photo/2004/m101/more.html
Laser Faint Object Grating Spectrometer (Frogs) with F. Witteborn and Jesse Bregman.
Topic: What -- Spectrometer
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eye 35
favorite 0
comment 0
Ozone gas in the stratosphere (upper atmosphere) absorbs ultraviolet light, thus protecting living things from the sun's harmful ultraviolet radiation. Man-made chemicals and weather conditions over Antarctica combine to deplete stratospheric ozone concentrations during the winter months there. (Data from Total Ozone Mapping Spectrometer [TOMS] project). Sensor: TOMS/TOMS. Data Start Date: 1/1/81. Data End Date: 7/31/05.
Topic: What -- Spectrometer
Source: http://visibleearth.nasa.gov/view_rec.php?id=7237
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Ozone gas in the stratosphere (upper atmosphere) absorbs ultraviolet light, thus protecting living things from the sun's harmful ultraviolet radiation. Man-made chemicals and weather conditions over Antarctica combine to deplete stratospheric ozone concentrations during the winter months there. (Data from Total Ozone Mapping Spectrometer [TOMS] project). Sensor: TOMS/TOMS. Data Start Date: 1/1/01. Data End Date: 7/31/05.
Topic: What -- Spectrometer
Source: http://visibleearth.nasa.gov/view_rec.php?id=7241
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Ozone gas in the stratosphere (upper atmosphere) absorbs ultraviolet light, thus protecting living things from the sun's harmful ultraviolet radiation. Man-made chemicals and weather conditions over Antarctica combine to deplete stratospheric ozone concentrations during the winter months there. (Data from Total Ozone Mapping Spectrometer [TOMS] project). Sensor: TOMS/TOMS. Data Start Date: 1/1/98. Data End Date: 7/31/05.
Topic: What -- Spectrometer
Source: http://visibleearth.nasa.gov/view_rec.php?id=7246
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Sep 17, 2009
09/09
by
NASA/Glenn Research Center
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eye 47
favorite 0
comment 0
INFRARED IMAGING SPECTROMETER
Topic: What -- Spectrometer
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Sep 18, 2009
09/09
by
NASA/Glenn Research Center
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eye 33
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LIFE TEST BEARINGS FOR MODERATE RESOLUTION IMAGING SPECTROMETER MODIS PROGRAM
Topic: What -- Spectrometer
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Sep 18, 2009
09/09
by
NASA/Glenn Research Center
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eye 32
favorite 0
comment 0
LIFE TEST BEARINGS FOR MODERATE RESOLUTION IMAGING SPECTROMETER MODIS PROGRAM
Topic: What -- Spectrometer
C-141 Circular Variable Filter Spectrometer & Yerkes Infrared
Topic: What -- Spectrometer
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Sep 17, 2009
09/09
by
NASA/Glenn Research Center
image
eye 34
favorite 0
comment 0
INFRARED IMAGING SPECTROMETER
Topic: What -- Spectrometer
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Aug 28, 2009
08/09
by
NASA/Glenn Research Center
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eye 35
favorite 0
comment 0
ADVANCED DIAGNOSTICS FOR COMBUSTION FOR THE ADVANCED TECHNOLOGY DEVELOPMENT PROGRAM MINIATURE MONOLITHIC SPECTROMETER
Topic: What -- Spectrometer
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Sep 10, 2009
09/09
by
NASA/Glenn Research Center
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eye 41
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SLOWLY ROTATING OPTICS BREADBOARD / HOMDYNE CORRELATION SPECTROMETER
Topic: What -- Spectrometer
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May 23, 2011
05/11
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NASA
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eye 126
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Rendezvous, capture and berthing of Orbiting and Retrievable Far and Extreme Ultraviolet Spectrometer (ORFEUS) Shuttle Pallet Satellite (SPAS) with the Remote Manipulator System (RMS) arm. The ORFEUS-SPAS is captured by the RMS arm, backdropped by the blackness of space (009-14). Closeup of the ORFEUS-SPAS on the end of the RMS arm (015-22). ORFEUS-SPAS is berthed in the payload bay (023-27).
Topic: What -- Spectrometer
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69
Sep 22, 2009
09/09
by
NASA/Langley Research Center (NASA-LaRC)
movies
eye 69
favorite 1
comment 0
FTS could generate higher resolution data products faster and more often for proposed atmospheric science missions in the next millennium. The result would be an increased ability to provide the science community with improved global imaging, better global weather and climate forecasting models, and an unprecedented capability to monitor gases and aerosols.
Topic: What -- Spectrometer
Source: http://nix.ksc.nasa.gov/info?id=LV-1998-00022&orgid=1
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119
Oct 30, 2009
10/09
by
Images by Greg Shirah, NASA Goddard Space Flight Center Scientific Visualization Studio
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eye 119
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These images from the Total Ozone Mapping Spectrometer (TOMS) show the progressive depletion of ozone over Antarctica from 1979 to 1999. This "ozone hole" has extended to cover an area as large as 10.5 million square miles in September 1998. The previous record of 10.0 million square miles was set in 1996.The Antarctic ozone hole develops each year between late August and early October. Regions with higher levels of ozone are shown in red. NASA and NOAA instruments have been measuring...
Topic: What -- Spectrometer
Source: http://visibleearth.nasa.gov/view_rec.php?id=138
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Nov 4, 2009
11/09
by
Images by Greg Shirah, NASA Goddard Space Flight Center Scientific Visualization Studio
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eye 89
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These images from the Total Ozone Mapping Spectrometer (TOMS) show the progressive depletion of ozone over Antarctica from 1979 to 1999. This "ozone hole" has extended to cover an area as large as 10.5 million square miles in September 1998. The previous record of 10.0 million square miles was set in 1996.The Antarctic ozone hole develops each year between late August and early October. Regions with higher levels of ozone are shown in red. NASA and NOAA instruments have been measuring...
Topic: What -- Spectrometer
Source: http://visibleearth.nasa.gov/view_rec.php?id=15369
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eye 321
favorite 0
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Scientists use data from NASA’s Total Ozone Mapping Spectrometer (TOMS) to measure the relative amount of aerosols—solid or liquid particles suspended in the atmosphere. Aerosol types detected by the TOMS Aerosol Index include desert dust, smoke and volcanic ash located at least 2 km (1.2 miles) above the surface.Every day, TOMS measures how much UV radiation is absorbed within the atmosphere and how much is reflected back up into space. These measures directly relate to how much aerosol is...
Topic: What -- Spectrometer
Source: http://visibleearth.nasa.gov/view_rec.php?id=7174
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eye 42
favorite 0
comment 0
Ozone gas in the stratosphere (upper atmosphere) absorbs ultraviolet light, thus protecting living things from the sun's harmful ultraviolet radiation. Man-made chemicals and weather conditions over Antarctica combine to deplete stratospheric ozone concentrations during the winter months there. (Data from Total Ozone Mapping Spectrometer [TOMS] project). Sensor: TOMS/TOMS. Data Start Date: 1/1/94. Data End Date: 7/31/05.
Topic: What -- Spectrometer
Source: http://visibleearth.nasa.gov/view_rec.php?id=7239
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eye 30
favorite 0
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Scientists use data from NASA’s Total Ozone Mapping Spectrometer (TOMS) to measure the relative amount of aerosols—solid or liquid particles suspended in the atmosphere. Aerosol types detected by the TOMS Aerosol Index include desert dust, smoke and volcanic ash located at least 2 km (1.2 miles) above the surface.Every day, TOMS measures how much UV radiation is absorbed within the atmosphere and how much is reflected back up into space. These measures directly relate to how much aerosol is...
Topic: What -- Spectrometer
Source: http://visibleearth.nasa.gov/view_rec.php?id=7191
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eye 46
favorite 0
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Ozone gas in the stratosphere (upper atmosphere) absorbs ultraviolet light, thus protecting living things from the sun's harmful ultraviolet radiation. Man-made chemicals and weather conditions over Antarctica combine to deplete stratospheric ozone concentrations during the winter months there. (Data from Total Ozone Mapping Spectrometer [TOMS] project). Sensor: TOMS/TOMS. Data Start Date: 1/1/93. Data End Date: 7/31/05.
Topic: What -- Spectrometer
Source: http://visibleearth.nasa.gov/view_rec.php?id=7238
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Scientists use data from NASA’s Total Ozone Mapping Spectrometer (TOMS) to measure the relative amount of aerosols—solid or liquid particles suspended in the atmosphere. Aerosol types detected by the TOMS Aerosol Index include desert dust, smoke and volcanic ash located at least 2 km (1.2 miles) above the surface.Every day, TOMS measures how much UV radiation is absorbed within the atmosphere and how much is reflected back up into space. These measures directly relate to how much aerosol is...
Topic: What -- Spectrometer
Source: http://visibleearth.nasa.gov/view_rec.php?id=7188
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Scientists use data from NASA’s Total Ozone Mapping Spectrometer (TOMS) to measure the relative amount of aerosols—solid or liquid particles suspended in the atmosphere. Aerosol types detected by the TOMS Aerosol Index include desert dust, smoke and volcanic ash located at least 2 km (1.2 miles) above the surface.Every day, TOMS measures how much UV radiation is absorbed within the atmosphere and how much is reflected back up into space. These measures directly relate to how much aerosol is...
Topic: What -- Spectrometer
Source: http://visibleearth.nasa.gov/view_rec.php?id=7206