Irradiance Measurements in the Upper OceanSource: Journal of Physical Oceanography:;1977:;Volume( 007 ):;issue: 006::page 952DOI: 10.1175/1520-0485(1977)007<0952:IMITUO>2.0.CO;2Publisher: American Meteorological Society
Abstract: Observations were made of downward solar radiation as a function of depth during an experiment in the North Pacific (35°N, 155°W). The irradiance meter employed was sensitive to solar radiation of wavelength 400?1000 nm arriving from above at a horizontal surface. Because of selective absorption of the short and long wavelengths, the irradiance decreases much faster than exponential in the upper few meters, falling to one-third of the incident value between 2 and 3 m depth. Below 10 m the decrease was exponential at a rate characteristic of moderately clear water of Type IA. Neglecting one case having low sun altitude, the observations are well represented by the expression I/I0=Rez/?1+(1?R)ez?2, where I is the irradiance at depth ?z, I0 is the irradiance at the surface less reflected solar radiation, R=0.62, ?1 and ?2 are attenuation lengths equal to 1.5 and 20 m, respectively, and z is the vertical space coordinate, positive upward with the origin at mean sea level. The depth at which the irradiance falls to 10% of its surface value is nearly the same as observations of Secchi depth when cases with high wind speed or low solar altitude are neglected. Parameters R, ?1, and ?2 are computed for the entire range of oceanic water types.
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contributor author | Paulson, Clayton A. | |
contributor author | Simpson, James J. | |
date accessioned | 2017-06-09T14:44:41Z | |
date available | 2017-06-09T14:44:41Z | |
date copyright | 1977/11/01 | |
date issued | 1977 | |
identifier issn | 0022-3670 | |
identifier other | ams-25773.pdf | |
identifier uri | http://onlinelibrary.yabesh.ir/handle/yetl/4162593 | |
description abstract | Observations were made of downward solar radiation as a function of depth during an experiment in the North Pacific (35°N, 155°W). The irradiance meter employed was sensitive to solar radiation of wavelength 400?1000 nm arriving from above at a horizontal surface. Because of selective absorption of the short and long wavelengths, the irradiance decreases much faster than exponential in the upper few meters, falling to one-third of the incident value between 2 and 3 m depth. Below 10 m the decrease was exponential at a rate characteristic of moderately clear water of Type IA. Neglecting one case having low sun altitude, the observations are well represented by the expression I/I0=Rez/?1+(1?R)ez?2, where I is the irradiance at depth ?z, I0 is the irradiance at the surface less reflected solar radiation, R=0.62, ?1 and ?2 are attenuation lengths equal to 1.5 and 20 m, respectively, and z is the vertical space coordinate, positive upward with the origin at mean sea level. The depth at which the irradiance falls to 10% of its surface value is nearly the same as observations of Secchi depth when cases with high wind speed or low solar altitude are neglected. Parameters R, ?1, and ?2 are computed for the entire range of oceanic water types. | |
publisher | American Meteorological Society | |
title | Irradiance Measurements in the Upper Ocean | |
type | Journal Paper | |
journal volume | 7 | |
journal issue | 6 | |
journal title | Journal of Physical Oceanography | |
identifier doi | 10.1175/1520-0485(1977)007<0952:IMITUO>2.0.CO;2 | |
journal fristpage | 952 | |
journal lastpage | 956 | |
tree | Journal of Physical Oceanography:;1977:;Volume( 007 ):;issue: 006 | |
contenttype | Fulltext |