Details
| Original language | English |
|---|---|
| Title of host publication | Ultraviolet Ground- and Space-based Measurements, Models, and Effects V |
| Place of Publication | Bellingham |
| Publisher | SPIE |
| Pages | 1-10 |
| Number of pages | 10 |
| ISBN (print) | 0-8194-5891-0 |
| Publication status | Published - 15 Feb 2007 |
| Event | Ultraviolet Ground- and Space-based Measurements, Models, and Effects V - San Diego, CA, United States Duration: 31 Jul 2005 → 1 Aug 2005 |
Publication series
| Name | Proceedings of SPIE - The International Society for Optical Engineering |
|---|---|
| Publisher | SPIE |
| Volume | 5886 |
| ISSN (Print) | 0277-786X |
Abstract
Spectral measurements of direct solar ultraviolet irradiance are very important for many applications in the field of atmospheric sciences. Despite its usefulness, few UV monitoring sites include such measurements in their regular observational programs. Standardization of measurement methodologies and calibration techniques is required in order to reach the quality standard of global irradiance measurements. This study presents preliminary results from an intercomparison campaign of seven UV spectroradiometers of different types that took place at the high altitude site of Izana (28.3°N, 16.5°W, 2367 m above sea level), in Tenerife, Canary Islands in June 2005. The campaign is focused primarily on spectral measurements of direct solar irradiance. Among the objectives is to improve the quality of direct solar irradiance spectral measurements, through instrumental modifications and standardization of calibration techniques, as well as to assess the significance of the differences in the field of view of the spectroradiometers with respect to aerosols and to solar zenith angle. Under the low aerosol conditions prevailing during this campaign, we aimed to establish the differences among the various instruments under "ideal" conditions. Moreover, continuous measurements under stable total ozone and aerosol optical depth will be used to determine the extraterrestrial solar flux, through the application of the Langley extrapolation method. A first comparison of sky radiance measurements of the zenith light and of various directions on the sky show effects of sensitivity to polarization of one type of instruments and the variability of the provisional radiance calibration of 4 instruments.
Keywords
- Direct, Solar UV irradiance, UV Radiation
ASJC Scopus subject areas
- Materials Science(all)
- Electronic, Optical and Magnetic Materials
- Physics and Astronomy(all)
- Condensed Matter Physics
- Computer Science(all)
- Computer Science Applications
- Mathematics(all)
- Applied Mathematics
- Engineering(all)
- Electrical and Electronic Engineering
Cite this
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Ultraviolet Ground- and Space-based Measurements, Models, and Effects V. Bellingham: SPIE, 2007. p. 1-10 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 5886).
Research output: Chapter in book/report/conference proceeding › Conference contribution › Research › peer review
}
TY - GEN
T1 - Intercomparison of solar UV direct irradiance spectral measurements at Izana in June 2005
AU - Bais, A.
AU - Blumthaler, M.
AU - Webb, A.
AU - Seckmeyer, G.
AU - Thiel, S.
AU - Kazadzis, S.
AU - Redondas, A.
AU - Kift, R.
AU - Kouremeti, N.
AU - Schallhart, B.
AU - Schmitt, R.
AU - Pisulla, D.
AU - Diaz, J. P.
AU - Garcia, O.
AU - Diaz Rodriguez, A. M.
AU - Smedley, A.
N1 - Copyright: Copyright 2008 Elsevier B.V., All rights reserved.
PY - 2007/2/15
Y1 - 2007/2/15
N2 - Spectral measurements of direct solar ultraviolet irradiance are very important for many applications in the field of atmospheric sciences. Despite its usefulness, few UV monitoring sites include such measurements in their regular observational programs. Standardization of measurement methodologies and calibration techniques is required in order to reach the quality standard of global irradiance measurements. This study presents preliminary results from an intercomparison campaign of seven UV spectroradiometers of different types that took place at the high altitude site of Izana (28.3°N, 16.5°W, 2367 m above sea level), in Tenerife, Canary Islands in June 2005. The campaign is focused primarily on spectral measurements of direct solar irradiance. Among the objectives is to improve the quality of direct solar irradiance spectral measurements, through instrumental modifications and standardization of calibration techniques, as well as to assess the significance of the differences in the field of view of the spectroradiometers with respect to aerosols and to solar zenith angle. Under the low aerosol conditions prevailing during this campaign, we aimed to establish the differences among the various instruments under "ideal" conditions. Moreover, continuous measurements under stable total ozone and aerosol optical depth will be used to determine the extraterrestrial solar flux, through the application of the Langley extrapolation method. A first comparison of sky radiance measurements of the zenith light and of various directions on the sky show effects of sensitivity to polarization of one type of instruments and the variability of the provisional radiance calibration of 4 instruments.
AB - Spectral measurements of direct solar ultraviolet irradiance are very important for many applications in the field of atmospheric sciences. Despite its usefulness, few UV monitoring sites include such measurements in their regular observational programs. Standardization of measurement methodologies and calibration techniques is required in order to reach the quality standard of global irradiance measurements. This study presents preliminary results from an intercomparison campaign of seven UV spectroradiometers of different types that took place at the high altitude site of Izana (28.3°N, 16.5°W, 2367 m above sea level), in Tenerife, Canary Islands in June 2005. The campaign is focused primarily on spectral measurements of direct solar irradiance. Among the objectives is to improve the quality of direct solar irradiance spectral measurements, through instrumental modifications and standardization of calibration techniques, as well as to assess the significance of the differences in the field of view of the spectroradiometers with respect to aerosols and to solar zenith angle. Under the low aerosol conditions prevailing during this campaign, we aimed to establish the differences among the various instruments under "ideal" conditions. Moreover, continuous measurements under stable total ozone and aerosol optical depth will be used to determine the extraterrestrial solar flux, through the application of the Langley extrapolation method. A first comparison of sky radiance measurements of the zenith light and of various directions on the sky show effects of sensitivity to polarization of one type of instruments and the variability of the provisional radiance calibration of 4 instruments.
KW - Direct
KW - Solar UV irradiance
KW - UV Radiation
UR - http://www.scopus.com/inward/record.url?scp=29344434703&partnerID=8YFLogxK
U2 - 10.1117/12.619925
DO - 10.1117/12.619925
M3 - Conference contribution
AN - SCOPUS:29344434703
SN - 0-8194-5891-0
T3 - Proceedings of SPIE - The International Society for Optical Engineering
SP - 1
EP - 10
BT - Ultraviolet Ground- and Space-based Measurements, Models, and Effects V
PB - SPIE
CY - Bellingham
T2 - Ultraviolet Ground- and Space-based Measurements, Models, and Effects V
Y2 - 31 July 2005 through 1 August 2005
ER -