Fast simulation tool for ultraviolet radiation at the earth's surface

被引:55
作者
Engelsen, O [1 ]
Kylling, A
机构
[1] Norwegian Polar Res Inst, Polar Environm Ctr, N-9296 Tromso, Norway
[2] Norwegian Inst Air Res, NILU, N-2027 Kjeller, Norway
关键词
radiative transfer modeling; UV index; UV-A; UV-B; UV-R; simulations; UV radiation doses;
D O I
10.1117/1.1885472
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
FastRT is a fast, yet accurate, UV simulation tool that computes downward surface UV doses, UV indices, and irradiances in the spectral range 290 to 400 nm with a resolution as small as 0.05 nm. It computes a full UV spectrum within a few milliseconds on a standard PC, and enables the user to convolve the spectrum with user-defined and built-in spectral response functions including the International Commission on Illumination (CIE) erythemal response function used for UV index calculations. The program accounts for the main radiative input parameters, i.e., instrumental characteristics, solar zenith angle, ozone column, aerosol loading, clouds, surface albedo, and surface altitude. FastRT is based on look-up tables of carefully selected entries of atmospheric transmittances and spherical albedos, and exploits the smoothness of these quantities with respect to atmospheric, surface, geometrical, and spectral parameters. An interactive site, http://nadir.nilu.no/similar to olaeng/fastr/fastrt.html, enables the public to run the FastRT program with most input options. This page also contains updated information about FastRT and links to freely downloadable source codes and binaries. (c) 2005 society of Photo-Optical Instrumentation Engineers.
引用
收藏
页码:1 / 7
页数:7
相关论文
共 24 条
[1]  
Abreu L., 1996, Contract 19628, 0132
[2]  
Anderson G, 1986, AFGLTR860110
[3]   Uncertainty of measurements of spectral solar UV irradiance [J].
Bernhard, G ;
Seckmeyer, G .
JOURNAL OF GEOPHYSICAL RESEARCH-ATMOSPHERES, 1999, 104 (D12) :14321-14345
[4]   SOLAR UVB-ALBEDO OF VARIOUS SURFACES [J].
BLUMTHALER, M ;
AMBACH, W .
PHOTOCHEMISTRY AND PHOTOBIOLOGY, 1988, 48 (01) :85-88
[5]   A NEW SPHERICAL MODEL FOR COMPUTING THE RADIATION-FIELD AVAILABLE FOR PHOTOLYSIS AND HEATING AT TWILIGHT [J].
DAHLBACK, A ;
STAMNES, K .
PLANETARY AND SPACE SCIENCE, 1991, 39 (05) :671-683
[6]   ESTIMATE OF THE WAVELENGTH DEPENDENCY OF ULTRAVIOLET CARCINOGENESIS IN HUMANS AND ITS RELEVANCE TO THE RISK ASSESSMENT OF A STRATOSPHERIC OZONE DEPLETION [J].
DEGRUIJL, FR ;
VANDERLEUN, JC .
HEALTH PHYSICS, 1994, 67 (04) :319-325
[7]   Fast simulation tool for UV radiation and diagnosis of measured UV spectra [J].
Engelsen, O ;
Kylling, A .
ULTRAVIOLET GROUND- AND SPACE-BASED MEASUREMENTS, MODELS AND EFFECTS III, 2003, 5156 :409-419
[8]   SPECTRAL ALBEDO MEASUREMENTS IN THE UV AND VISIBLE REGION OVER DIFFERENT TYPES OF SURFACES [J].
FEISTER, U ;
GREWE, R .
PHOTOCHEMISTRY AND PHOTOBIOLOGY, 1995, 62 (04) :736-744
[9]  
GONZI S, 2002, AEROSOL CLIMATOLOGY
[10]   LIGHT-SCATTERING IN PLANETARY ATMOSPHERES [J].
HANSEN, JE ;
TRAVIS, LD .
SPACE SCIENCE REVIEWS, 1974, 16 (04) :527-610