首页> 外文期刊>Atmospheric Chemistry and Physics Discussions >Constraining the Nsub2/subOsub5/sub UV absorption cross section from spectroscopic trace gas measurements in the tropical mid-stratosphere
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Constraining the Nsub2/subOsub5/sub UV absorption cross section from spectroscopic trace gas measurements in the tropical mid-stratosphere

机译:热带平流层中的光谱痕量气体测量结果限制了N 2 O 5 紫外吸收截面

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pstrongAbstract./strong The absorption cross section of Nsub2/subOsub5/sub, σsubNsub2/subOsub5/sub/sub(λ, iT/i), which is known from laboratory measurements with the uncertainty of a factor of 2 (Table 4-2 in (Jet Propulsion Laboratory) JPL-2011; the spread in laboratory data, however, points to an uncertainty in the range of 25 to 30%, Sander et al., 2011), was investigated by balloon-borne observations of the relevant trace gases in the tropical mid-stratosphere. The method relies on the observation of the diurnal variation of NOsub2/sub by limb scanning DOAS (differential optical absorption spectroscopy) measurements (Weidner et al., 2005; Kritten et al., 2010), supported by detailed photochemical modelling of NOsuby/sub (NOsubx/sub(= NO + NOsub2/sub) + NOsub3/sub + 2Nsub2/subOsub5/sub + ClONOsub2/sub + HOsub2/subNOsub2/sub + BrONOsub2/sub + HNOsub3/sub) photochemistry and a non-linear least square fitting of the model result to the NOsub2/sub observations. Simulations are initialised with Osub3/sub measured by direct sun observations, the NOsuby/sub partitioning from MIPAS-B (Michelson Interferometer for Passive Atmospheric Sounding a?? Balloon-borne version) observations in similar air masses at night-time, and all other relevant species from simulations of the SLIMCAT (Single Layer Isentropic Model of Chemistry And Transport) chemical transport model (CTM). Best agreement between the simulated and observed diurnal increase of NOsub2/sub is found if the σsubNsub2/subOsub5/sub/sub(λ, iT/i) is scaled by a factor of 1.6 ?± 0.8 in the UV-C (200a??260 nm) and by a factor of 0.9 ?± 0.26 in the UV-B/A (260a??350 nm), compared to current recommendations. As a consequence, at 30 km altitude, the Nsub2/subOsub5/sub lifetime against photolysis becomes a factor of 0.77 shorter at solar zenith angle (SZA) of 30° than using the recommended σsubNsub2/subOsub5/sub/sub(λ, iT/i), and stays more or less constant at SZAs of 60°. Our scaled Nsub2/subOsub5/sub photolysis frequency slightly reduces the lifetime (0.2a??0.6%) of ozone in the tropical mid- and upper stratosphere, but not to an extent to be important for global ozone./p.
机译:> >摘要。N 2 O 5 ,σ N 2 的吸收截面O 5 (&lambda ;, T ),这在实验室测量中已知,不确定度为2(喷气推进器中的表4-2) JPL-2011;实验室数据的扩散表明,不确定性在25%到30%之间(Sander等人,2011),是通过对热带中相关痕量气体进行的气球观测研究的平流层中部。该方法依赖于通过肢体扫描DOAS(微分光吸收光谱法)测量观察NO 2 的日变化(Weidner等,2005; Kritten等,2010),并得到了详细的支持。 NO y (NO x (= NO + NO 2 )+ NO 3 + 2N 2 O 5 + ClONO 2 + HO 2 NO 2 + BrONO 2 + HNO 3 )的光化学反应和模型的非线性最小二乘拟合,结果符合NO 2 的观测结果。通过直接太阳观测测量的O 3 初始化模拟,从MIPAS-B(用于大气被动探测的米歇尔森干涉仪-气球传播型)的NO y 分区进行观测在夜间的类似空气质量中,以及所有其他相关物种均来自SLIMCAT(化学和运输的单层等熵模型)化学运输模型(CTM)的模拟。如果&subigma; N 2 O 5 ,则可以模拟和观察到NO 2 的日增重之间的最佳一致性。 (λ, T )在UV-C(200a≤260 nm)中缩放为1.6±±0.8,在UV-B /中缩放为0.9±±0.26。与目前的推荐值相比,A(260a?350 nm)。结果,在30 km的高度,抗太阳光分解的N 2 O 5 寿命在太阳天顶角(SZA)为30°时缩短了0.77倍。比使用推荐的σ N 2 O 5 (&lambda ;, T )并保持或多或少SZA恒定为60°。我们标定的N 2 O 5 光解频率稍微降低了热带平流层中上层臭氧的寿命(0.2a ?? 0.6%),但没有达到一定程度对全球臭氧很重要。

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