The contribution of unknown weak water vapor lines to the absorption of solar radiation

被引:30
作者
Learner, RCM [1 ]
Zhong, W
Haigh, JD
Belmiloud, D
Clarke, J
机构
[1] Univ London Imperial Coll Sci Technol & Med, Dept Phys, London SW7 2BZ, England
[2] UCL, Dept Phys & Astron, London WC1E 6BT, England
关键词
D O I
10.1029/1999GL003681
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Thousands of unknown water vapour weak lines in the spectral region between 13200 and 22700 cm(-1) are deduced from extrapolations of experimental results. These lines are then included in the HITRAN database and used in line-by-line calculations of atmospheric opacity with standard atmospheric profiles. The weak lines predicted by a theoretical model are also used in the line-by-line model to estimate their contribution to the absorption of solar radiation. The additional absorption of solar radiation is of order 1.5 to 2.5 W/m(2) at 45 mm precipitable water, about 8.5% to 14% of the absorption due to HITRAN lines in the spectral region. The effect is also compared with that of a continuum model.
引用
收藏
页码:3609 / 3612
页数:4
相关论文
共 20 条
[1]   DYNAMICS OF OZONE PHOTOABSORPTION - A THEORETICAL-STUDY OF THE CHAPPUIS BAND [J].
BANICHEVICH, A ;
PEYERIMHOFF, SD ;
BESWICK, JA ;
ATABEK, O .
JOURNAL OF CHEMICAL PHYSICS, 1992, 96 (09) :6580-6590
[2]   THE HIGH-RESOLUTION SPECTRUM OF WATER-VAPOR BETWEEN 16500 AND 25250 CM-1 [J].
CAMYPEYRET, C ;
FLAUD, JM ;
MANDIN, JY ;
CHEVILLARD, JP ;
BRAULT, J ;
RAMSAY, DA ;
VERVLOET, M ;
CHAUVILLE, J .
JOURNAL OF MOLECULAR SPECTROSCOPY, 1985, 113 (01) :208-228
[3]   ABSORPTION OF SOLAR-RADIATION BY CLOUDS - OBSERVATIONS VERSUS MODELS [J].
CESS, RD ;
ZHANG, MH ;
MINNIS, P ;
CORSETTI, L ;
DUTTON, EG ;
FORGAN, BW ;
GARBER, DP ;
GATES, WL ;
HACK, JJ ;
HARRISON, EF ;
JING, X ;
KIEHL, JT ;
LONG, CN ;
MORCRETTE, JJ ;
POTTER, GL ;
RAMANATHAN, V ;
SUBASILAR, B ;
WHITLOCK, CH ;
YOUNG, DF ;
ZHOU, Y .
SCIENCE, 1995, 267 (5197) :496-499
[4]  
Clough S. A., 1989, Atmos. Res, V23, P229, DOI DOI 10.1016/0169-8095(89)90020-3
[5]  
Edwards D. P, 1992, TN367 NCAR
[6]   The high-resolution spectrum of water vapor between 11600 and 12750 cm(-1) [J].
Flaud, JM ;
CamyPeyret, C ;
Bykov, A ;
Naumenko, O ;
Petrova, T ;
Scherbakov, A ;
Sinitsa, L .
JOURNAL OF MOLECULAR SPECTROSCOPY, 1997, 183 (02) :300-309
[7]   Improved spectral parameters for the three most abundant isotopomers of the oxygen molecule [J].
Gamache, RR ;
Goldman, A ;
Rothman, LS .
JOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER, 1998, 59 (3-5) :495-509
[8]  
KAIN JS, 1999, UNPUB CHEM PHYS LETT
[10]   THE HIGH-RESOLUTION SPECTRUM OF WATER-VAPOR BETWEEN 13200 AND 16500 CM-1 [J].
MANDIN, JY ;
CHEVILLARD, JP ;
CAMYPEYRET, C ;
FLAUD, JM ;
BRAULT, JW .
JOURNAL OF MOLECULAR SPECTROSCOPY, 1986, 116 (01) :167-190