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首页> 外文期刊>Journal of Geophysical Research, D. Atmospheres: JGR >High supersaturation and modes of ice nucleation in thin tropopause cirrus: Simulation of the 13 July 2002 Cirrus Regional Study of Tropical Anvils and Cirrus Layers case
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High supersaturation and modes of ice nucleation in thin tropopause cirrus: Simulation of the 13 July 2002 Cirrus Regional Study of Tropical Anvils and Cirrus Layers case

机译:对流层稀薄卷云的高过饱和度和冰成核模式:2002年7月13日卷云对热带砧和卷云区域的研究

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摘要

A unique and extensive data set of cirrus properties collected on 13 July 2002 during CRYSTAL-FACE provides the framework for simulations using cloud models to interpret the observations and to develop recommendations for microphysical parameterizations in large-scale models. Several outstanding issues in the simulations of cirrus clouds are addressed using detailed bin-resolving and bulk microphysics models. A new heterogeneous ice nucleation formulation based on extended classical theory with simultaneous dependence on temperature and saturation ratio is applied for the first time to thin tropopause cirrus. The simulated cloud microphysical properties are similar to observations, suggesting that tropopause cirrus may potentially form as a result of heterogeneous immersion freezing of internally mixed aerosols serving as ice nuclei (IN). The potential for mixed aerosols to serve as IN in tropopause cirrus is consistent with measurements of comparable amounts of soluble and insoluble material in cirrus residues and aerosols during CRYSTAL-FACE. Simulations using homogeneous nucleation theory are also able to produce comparable microphysical properties if the heterogeneous mode is turned off; hence the homogeneous mode cannot be excluded if insoluble material capable of serving as IN is not available. The calculated critical ice supersaturation for the onset of heterogeneous nucleation at these cold temperatures (~200 K) was 70–80% (for the assumed aerosol nucleation parameters) and 15–20% higher for homogeneous nucleation. The calculated supersaturation relaxation time ranged from ~1–2 hours in the center of the cloud to 3–6 hours near the boundaries, which may explain the high values of ice supersaturation (30–80%) observed in this cloud. Analysis of the supersaturation budget showed that supersaturation was generally nonequilibrium, and relaxation from the initial critical values to near equilibrium occurred only after several hours. The bulk model was able to simulate this case and in particular the slow crystal growth and large supersaturation because of its detailed treatment of ice nucleation and supersaturation. The fraction of condensed ice relative to excess vapor predicted by both models was 40–60% for several hours, indicating that bulk models with zero supersaturation (instantaneous condensation of all excess vapor) would substantially overpredict the ice water path and optical thickness.
机译:2002年7月13日在CRYSTAL-FACE期间收集的一组独特的卷云特性数据,提供了使用云模型进行模拟以解释观测结果并为大型模型中的微物理参数化提出建议的框架。卷云模拟中的几个突出问题已使用详细的箱解析和体微物理学模型解决。首次将基于扩展经典理论并同时依赖于温度和饱和度比率的新的非均质冰成核配方首次应用于薄对流层顶卷云。模拟的云微物理性质与观测结果相似,表明对流层顶卷云可能是由于内部混合的气溶胶(作为冰核(IN))的非均质浸泡冻结而潜在形成的。混合气溶胶在对流层顶卷云中充当IN的潜力与CRYSTAL-FACE期间卷云残渣和气溶胶中可溶和不溶物质的可比较量的测量结果一致。如果关闭了异质模式,使用均相成核理论的模拟也能够产生可比较的微物理特性。因此,如果没有可以用作IN的不溶物,则不能排除均质模式。在这些寒冷温度(〜200 K)下,计算出的非均匀成核的临界冰过饱和度为70–80%(对于假定的气溶胶成核参数),而对于均匀成核则为15–20%。计算得出的过饱和弛豫时间范围从云中心的1-2小时到边界附近的3-6小时不等,这可能解释了在云中观测到的冰过饱和值很高(30-80%)。对过饱和预算的分析表明,过饱和通常是不平衡的,只有几个小时后才会发生从初始临界值到接近平衡的松弛。体模型能够模拟这种情况,特别是由于缓慢处理晶体成核和过饱和,从而特别是缓慢的晶体生长和较大的过饱和。两个模型预测的相对于过量蒸气的凝结冰比例在几个小时内为40-60%,这表明过饱和度为零的散装模型(所有过量蒸气的瞬时凝结)会大大预测冰水路径和光学厚度。

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