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首页> 外文期刊>Journal of Geophysical Research, D. Atmospheres: JGR >On the dependence of albedo on cloud microphysics over marine stratocumulus clouds regimes determined from Clouds and the Earth's Radiant Energy System (CERES) data
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On the dependence of albedo on cloud microphysics over marine stratocumulus clouds regimes determined from Clouds and the Earth's Radiant Energy System (CERES) data

机译:根据云层和地球辐射能系统(CERES)数据确定的反照率对海洋平流层积云状态下云微物理的依赖性

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The dependence of the top-of-the-atmosphere (TOA) albedo A on cloud microphysical properties was investigated for the three largest maritime stratocumulus clouds regimes: off California, Southeast Pacific (Chile-Peru), and southwest Africa (Namibia-Angola). Absolute S and relative S_R albedo susceptibilities to perturbations in cloud droplet number concentrations N_d, defined as dA/dN_d and dA/dln(N_d) respectively, were calculated for the season having maximum cloud cover during the period 2006-2010. Satellite-based susceptibilities were computed by combining an adiabatically based N_d estimate and liquid water path (LWP) derived from Terra Moderate Resolution Imaging Spectroradiometer (MODIS) retrievals matched with TOA A from the Clouds and the Earth's Radiant Energy System. Empirical susceptibility maps were calculated for three constant LWP intervals at 25, 50, and 90 g m~(-2).* It was found that S increases with LWP, with small and spatially homogeneous values for low LWP, and a contrasting increase far offshore for larger LWP values. An overall increase of S_R with LWP was also observed, with larger values near the coast for LWP = 25 and 50 g m~(-2).* A relatively homogeneous spatial pattern of maximum S_R values covered most of each regime's domain for a LWP of 90 g m~(-2).* These results highlight the importance of LWP in modulating the albedo susceptibility. The dependencies of S and S_R on LWP are mostly explained by variations in the mean N_d and cloud optical thickness (τ), with an increase of S with LWP linked to a decrease in N_d, whereas S_R increased with τ and A, until reaching a maximum for A and τ near 0.36-0.4 and 12-14 respectively, and decreasing thereafter, consistent with expectations based on two-stream estimates. Larger S_R values in the Southeast Pacific are thought to be the consequence of a drier and more pristine atmosphere. Radiative transfer simulations with realistic values of above-cloud water vapor path and aerosol optical thickness showed that differing atmospheric compositions could explain why the Chile-Peru regime was the marine stratocumulus cloud deck most susceptible to change its TOA albedo due to fractional changes in N_d.
机译:针对加利福尼亚,东南太平洋(智利-秘鲁)和西南非洲(纳米比亚-安哥拉)这三种最大的海上平层积云制度,研究了大气最高(TOA)反照率A对云微物理性质的依赖性。 。针对2006-2010年期间最大云量覆盖的季节,计算了分别定义为dA / dN_d和dA / dln(N_d)的云滴数浓度N_d的扰动的绝对S和相对S_R反照率。通过将基于绝热的N_d估计值和从Terra中分辨率成像光谱仪(MODIS)检索得到的液态水路径(LWP)与来自云和地球辐射能系统的TOA A相结合,计算出基于卫星的磁化率。对于25、50和90 gm〜(-2)的三个恒定的LWP间隔,计算了经验药敏图。*发现S随着LWP的增加而增加,对于低LWP而言,S值较小且在空间上均一,而远海处则相反对于较大的LWP值。随着LWP的增加,S_R总体增加,在LWP分别为25和50 gm〜(-2)时,海岸附近的值更大。*最大S_R值的相对均匀的空间格局覆盖了LWP为90 gm〜(-2)。*这些结果突出了LWP在调节反照率敏感性中的重要性。 S和S_R对LWP的依赖性主要是通过平均N_d和云光学厚度(τ)的变化来解释的,随着LWP的增加,S的增加与N_d的减少有关,而S_R随τ和A的增加而增加,直到达到a。 A和τ的最大值分别接近0.36-0.4和12-14,此后减小,与基于两流估计的预期一致。东南太平洋的较大S_R值被认为是更干燥和更原始的气氛的结果。辐射传递模拟具有高于云层的水蒸气路径和气溶胶光学厚度的实际值,表明不同的大气成分可以解释为什么智利-秘鲁政权是海洋平流层云层,因为N_d的分数变化最容易改变其TOA反照率。

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