Ehramjian, Version 2 data of the National Science Foundation’s Ultraviolet Radiation Monitoring Network
edition, labeled ‘‘Version 2.’ ’ The new version was corrected for wavelength shift errors and deviations of the spectroradiometer from the ideal cosine response. A comprehensive uncertainty budget of the new data set was established. Below 400 nm the expanded standard uncertainty (coverage factor 2...
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.576.8929 2023-05-15T18:22:40+02:00 Ehramjian, Version 2 data of the National Science Foundation’s Ultraviolet Radiation Monitoring Network G. Bernhard C. R. Booth J. C. Ehramjian The Pennsylvania State University CiteSeerX Archives application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.576.8929 http://uv.biospherical.com/Version2/Paper/2004JD004937.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.576.8929 http://uv.biospherical.com/Version2/Paper/2004JD004937.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://uv.biospherical.com/Version2/Paper/2004JD004937.pdf text ftciteseerx 2016-01-08T12:47:54Z edition, labeled ‘‘Version 2.’ ’ The new version was corrected for wavelength shift errors and deviations of the spectroradiometer from the ideal cosine response. A comprehensive uncertainty budget of the new data set was established. Below 400 nm the expanded standard uncertainty (coverage factor 2) varies between 4.6 and 7.2%, depending on wavelength and sky condition. The uncertainty of biologically relevant UV irradiances is approximately 6%. Compared to the previously published data set, Version 2 UV data are higher by 5–14%, depending on wavelength, solar zenith angle (SZA), and year of observation. By comparing Version 2 data with results of a radiative transfer model, the good consistency and homogeneity of the new data set were confirmed. The data set is used to establish a UV climatology for the South Pole, focusing on the effects of aerosols, clouds, and total column ozone. Clouds are predominantly optically thin; 71 % of all clouds have an optical depth between 0 and 1. The average attenuation of UV irradiance at 345 nm by clouds is less than 5 % and no attenuations greater than 23 % were observed. Attenuation by homogeneous clouds is generally larger in the visible than in the UV. The wavelength dependence of cloud Text South pole Unknown South Pole |
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description |
edition, labeled ‘‘Version 2.’ ’ The new version was corrected for wavelength shift errors and deviations of the spectroradiometer from the ideal cosine response. A comprehensive uncertainty budget of the new data set was established. Below 400 nm the expanded standard uncertainty (coverage factor 2) varies between 4.6 and 7.2%, depending on wavelength and sky condition. The uncertainty of biologically relevant UV irradiances is approximately 6%. Compared to the previously published data set, Version 2 UV data are higher by 5–14%, depending on wavelength, solar zenith angle (SZA), and year of observation. By comparing Version 2 data with results of a radiative transfer model, the good consistency and homogeneity of the new data set were confirmed. The data set is used to establish a UV climatology for the South Pole, focusing on the effects of aerosols, clouds, and total column ozone. Clouds are predominantly optically thin; 71 % of all clouds have an optical depth between 0 and 1. The average attenuation of UV irradiance at 345 nm by clouds is less than 5 % and no attenuations greater than 23 % were observed. Attenuation by homogeneous clouds is generally larger in the visible than in the UV. The wavelength dependence of cloud |
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The Pennsylvania State University CiteSeerX Archives |
format |
Text |
author |
G. Bernhard C. R. Booth J. C. Ehramjian |
spellingShingle |
G. Bernhard C. R. Booth J. C. Ehramjian Ehramjian, Version 2 data of the National Science Foundation’s Ultraviolet Radiation Monitoring Network |
author_facet |
G. Bernhard C. R. Booth J. C. Ehramjian |
author_sort |
G. Bernhard |
title |
Ehramjian, Version 2 data of the National Science Foundation’s Ultraviolet Radiation Monitoring Network |
title_short |
Ehramjian, Version 2 data of the National Science Foundation’s Ultraviolet Radiation Monitoring Network |
title_full |
Ehramjian, Version 2 data of the National Science Foundation’s Ultraviolet Radiation Monitoring Network |
title_fullStr |
Ehramjian, Version 2 data of the National Science Foundation’s Ultraviolet Radiation Monitoring Network |
title_full_unstemmed |
Ehramjian, Version 2 data of the National Science Foundation’s Ultraviolet Radiation Monitoring Network |
title_sort |
ehramjian, version 2 data of the national science foundation’s ultraviolet radiation monitoring network |
url |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.576.8929 http://uv.biospherical.com/Version2/Paper/2004JD004937.pdf |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_source |
http://uv.biospherical.com/Version2/Paper/2004JD004937.pdf |
op_relation |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.576.8929 http://uv.biospherical.com/Version2/Paper/2004JD004937.pdf |
op_rights |
Metadata may be used without restrictions as long as the oai identifier remains attached to it. |
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