A model to extend spectral and multiwavelength UV irradiances time series:: Model development and validation -: art. no. 4150

被引:9
作者
Díaz, S
Nelson, D
Deferrari, G
Camilión, C
机构
[1] Consejo Nacl Invest Cient & Tecn, Ctr Austral Invest Cient, RA-9410 Ushuaia, Tierra del Fueg, Argentina
[2] Natl Ocean & Atmospher Adm, CMDL, Boulder, CO 80305 USA
[3] NSF, Ctr Austral Invest Cient, RA-9410 Ushuaia, Tierra del Fueg, Argentina
[4] IAI, Ctr Austral Invest Cient, RA-9410 Ushuaia, Tierra del Fueg, Argentina
关键词
UV-B irradiances; ozone; ozone depletion; UV irradiance modeling; multiregressive model;
D O I
10.1029/2002JD002134
中图分类号
P4 [大气科学(气象学)];
学科分类号
0706 ; 070601 ;
摘要
[1] Measurements of spectral and multichannel UV radiation became more common in the middle and late eighties after the discovery of the "ozone hole,'' but time series for these measurements are still relatively short for the determination of trends to be applied in geophysical and biological studies. However, systematic measurements of total column ozone have been performed since the late 1950s at several stations, and global coverage has been available since the late 1970s. Also, long-term time series of broadband instruments (Pyranometers, UV and erythemally weighted) are available from many sites around the world. In this paper a multiregressive model that enables the inference of spectral or narrow band UV irradiances from total ozone column and broadband irradiance, in places where relatively short time series of UV spectral irradiances are available, is proposed. To test the model, measurements of irradiances performed at three of the stations in the NSF UV Radiation Monitoring Network, under all weather, solar zenith angle and surface conditions, were used. The model generated very good results over a wide variety of situations. Pyranometer data from the NOAA/CMDL surface radiation budget database for South Pole and Barrow Stations were used to estimate daily integrated narrow band irradiances. A time series of monthly means for the narrowband (303.030-307.692 nm) were then computed, dating back to the late 1970s.
引用
收藏
页数:12
相关论文
共 47 条
[1]  
Bodeker GE, 1996, J APPL METEOROL, V35, P1860, DOI 10.1175/1520-0450(1996)035<1860:AAFISU>2.0.CO
[2]  
2
[3]  
Booth C. R., 1998, NSF POLAR PROGRAMS U
[4]  
BOOTH CR, 1994, ANTAR RES S, V0062, P00017
[5]   Calculated upper stratospheric effects of solar UV flux and NOy variations during the 11-year solar cycle [J].
Callis, LB ;
Natarajan, M ;
Lambeth, JD .
GEOPHYSICAL RESEARCH LETTERS, 2000, 27 (23) :3869-3872
[6]   Observations of the solar irradiance in the 200-350 nm interval during the ATLAS-1 mission: A comparison among three sets of measurements - SSBUV, SOLSPEC, and SUSIM [J].
Cebula, RP ;
Thuillier, GO ;
VanHoosier, ME ;
Hilsenrath, E ;
Herse, M ;
Brueckner, GE ;
Simon, PC .
GEOPHYSICAL RESEARCH LETTERS, 1996, 23 (17) :2289-2292
[7]  
CEBULA RP, 1994, SUN VARIABLE STAR, P81
[8]   THE SOLAR-CYCLE VARIATION OF OZONE IN THE STRATOSPHERE INFERRED FROM NIMBUS-7 AND NOAA-11 SATELLITES [J].
CHANDRA, S ;
MCPETERS, RD .
JOURNAL OF GEOPHYSICAL RESEARCH-ATMOSPHERES, 1994, 99 (D10) :20665-20671
[9]  
CHUBAROVA NY, 1997, P IRS 96 CURR PROBL, P881
[10]  
CUTCHIS A, 1980, 8021 FAAEE US DEP TR