UV 380 nm Reflectivity of the Earth's Surface

The 380 nm radiance measurements of TOMS (Total Ozone Mapping Spectrometer) have been converted into a global data set of daily (1979 to 1992) Lambert equivalent reflectivities R of the Earth's surface and boundary layer (clouds, aerosols, surface haze, and snow/ice). Since UV surface reflectiv...

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Main Authors: Herman, J. R., Larko, D., Celarier, E.
Language:unknown
Published: 2000
Subjects:
Online Access:http://hdl.handle.net/2060/20000033459
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spelling ftnasantrs:oai:casi.ntrs.nasa.gov:20000033459 2023-05-15T14:03:46+02:00 UV 380 nm Reflectivity of the Earth's Surface Herman, J. R. Larko, D. Celarier, E. Unclassified, Unlimited, Publicly available Feb. 22, 2000 application/pdf http://hdl.handle.net/2060/20000033459 unknown Document ID: 20000033459 http://hdl.handle.net/2060/20000033459 No Copyright CASI Geophysics 2000 ftnasantrs 2015-03-15T02:44:44Z The 380 nm radiance measurements of TOMS (Total Ozone Mapping Spectrometer) have been converted into a global data set of daily (1979 to 1992) Lambert equivalent reflectivities R of the Earth's surface and boundary layer (clouds, aerosols, surface haze, and snow/ice). Since UV surface reflectivity is between 2 and 8% for both land and water during all seasons of the year (except for ice and snow cover), reflectivities larger than the surface value indicates the presence of clouds, haze, or aerosols in the satellite field of view. Statistical analysis of 14 years of daily data show that most snow/ice-free regions of the Earth have their largest fraction of days each year when the reflectivity is low (R less than 10%). The 380 nm reflectivity data shows that the true surface reflectivity is 2 to 3% lower than the most frequently occurring reflectivity value for each TOMS scene. The most likely cause of this could be a combination of frequently occurring boundary-layer water or aerosol haze. For most regions, the observation of extremely clear conditions needed to estimate the surface reflectivity from space is a comparatively rare occurrence. Certain areas (e.g., Australia, southern Africa, portions of northern Africa) are cloud-free more than 80% of the year, which exposes these regions to larger amounts of UV radiation than at comparable latitudes in the Northern Hemisphere. Regions over rain-forests, jungle areas, Europe and Russia, the bands surrounding the Arctic and Antarctic regions, and many ocean areas have significant cloud cover (R greater than 15%) more than half of each year. In the low to middle latitudes, the areas with the heaviest cloud cover (highest reflectivity for most of the year) are the forest areas of northern South America, southern Central America, the jungle areas of equatorial Africa, and high mountain regions such as the Himalayas or the Andes. The TOMS reflectivity data show the presence of large nearly clear ocean areas and the effects of the major ocean currents on cloud production. Other/Unknown Material Antarc* Antarctic Arctic NASA Technical Reports Server (NTRS) Antarctic Arctic
institution Open Polar
collection NASA Technical Reports Server (NTRS)
op_collection_id ftnasantrs
language unknown
topic Geophysics
spellingShingle Geophysics
Herman, J. R.
Larko, D.
Celarier, E.
UV 380 nm Reflectivity of the Earth's Surface
topic_facet Geophysics
description The 380 nm radiance measurements of TOMS (Total Ozone Mapping Spectrometer) have been converted into a global data set of daily (1979 to 1992) Lambert equivalent reflectivities R of the Earth's surface and boundary layer (clouds, aerosols, surface haze, and snow/ice). Since UV surface reflectivity is between 2 and 8% for both land and water during all seasons of the year (except for ice and snow cover), reflectivities larger than the surface value indicates the presence of clouds, haze, or aerosols in the satellite field of view. Statistical analysis of 14 years of daily data show that most snow/ice-free regions of the Earth have their largest fraction of days each year when the reflectivity is low (R less than 10%). The 380 nm reflectivity data shows that the true surface reflectivity is 2 to 3% lower than the most frequently occurring reflectivity value for each TOMS scene. The most likely cause of this could be a combination of frequently occurring boundary-layer water or aerosol haze. For most regions, the observation of extremely clear conditions needed to estimate the surface reflectivity from space is a comparatively rare occurrence. Certain areas (e.g., Australia, southern Africa, portions of northern Africa) are cloud-free more than 80% of the year, which exposes these regions to larger amounts of UV radiation than at comparable latitudes in the Northern Hemisphere. Regions over rain-forests, jungle areas, Europe and Russia, the bands surrounding the Arctic and Antarctic regions, and many ocean areas have significant cloud cover (R greater than 15%) more than half of each year. In the low to middle latitudes, the areas with the heaviest cloud cover (highest reflectivity for most of the year) are the forest areas of northern South America, southern Central America, the jungle areas of equatorial Africa, and high mountain regions such as the Himalayas or the Andes. The TOMS reflectivity data show the presence of large nearly clear ocean areas and the effects of the major ocean currents on cloud production.
author Herman, J. R.
Larko, D.
Celarier, E.
author_facet Herman, J. R.
Larko, D.
Celarier, E.
author_sort Herman, J. R.
title UV 380 nm Reflectivity of the Earth's Surface
title_short UV 380 nm Reflectivity of the Earth's Surface
title_full UV 380 nm Reflectivity of the Earth's Surface
title_fullStr UV 380 nm Reflectivity of the Earth's Surface
title_full_unstemmed UV 380 nm Reflectivity of the Earth's Surface
title_sort uv 380 nm reflectivity of the earth's surface
publishDate 2000
url http://hdl.handle.net/2060/20000033459
op_coverage Unclassified, Unlimited, Publicly available
geographic Antarctic
Arctic
geographic_facet Antarctic
Arctic
genre Antarc*
Antarctic
Arctic
genre_facet Antarc*
Antarctic
Arctic
op_source CASI
op_relation Document ID: 20000033459
http://hdl.handle.net/2060/20000033459
op_rights No Copyright
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