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Entropy budget of an atmosphere in radiative-convective equilibrium.

机译:辐射对流平衡中大气的熵收支。

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摘要

The entropy budget of an atmosphere in radiative-convective equilibrium is analyzed here. The differential heating of the atmosphere, resulting from surface heat fluxes and tropospheric radiative cooling, results into a net entropy sink. In statistical equilibrium, this entropy sink is balanced by the entropy production due to various irreversible processes such as frictional dissipation, diffusion of heat, diffusion of water vapor and irreversible phase changes. Determining the relative contribution of each individual irreversible process to the entropy budget provides important information on the behavior of convection. In particular, following Rennó and Ingersoll (1996) and Emanuel and Bister (1996), it is shown that the entropy budget can be used to derive vertical velocity, Convective Available Potential Energy (CAPE) and intermittency of convective systems.; The differences between dry and moist convection are investigated by combining theoretical arguments with numerical simulations with a high resolution Cloud Ensemble Model. In these numerical simulations, the dominant irreversible entropy source for dry convection is due to frictional dissipation. In contrast, for moist convection, the irreversible entropy production is dominated by irreversible phase changes and diffusion of water vapor. In addition, a large fraction of the frictional dissipation in moist convection results from falling precipitation. This specific behavior indicates that moist convection acts more like an atmospheric dryer than a heat engine. These findings differ significantly from the assumptions made in Rennó and Ingersoll (1996) and Emanuel and Bister (1996). It is also shown that the irreversible entropy production by phase change and diffusion of water vapor is directly related to the convective transport of latent heat. The behavior of convective systems thus depends on how the heat transport is divided between sensible and latent heat.; Finally, the study of the entropy budget is extended to include the effects of the large-scale circulation. The energy, entropy and water vapor transports by a large-scale flow can reinforce convective activity in regions of large-scale ascent while reducing it in regions of subsidence.
机译:在此分析了辐射对流平衡中大气的熵预算。由表面热通量和对流层辐射冷却引起的大气差异加热导致净熵下降。在统计平衡中,由于各种不可逆的过程(例如摩擦耗散,热扩散,水蒸气的扩散和不可逆的相变),该熵沉被熵产生所平衡。确定每个不可逆过程对熵预算的相对贡献可提供有关对流行为的重要信息。特别是,根据Rennó和Ingersoll(1996)以及Emanuel和Bister(1996),证明了熵预算可用于导出垂直速度,对流可用势能(CAPE)和对流系统的间歇性。通过将理论参数与带有高分辨率云团模型的数值模拟相结合,研究了干对流和湿对流之间的差异。在这些数值模拟中,干对流的主要不可逆熵源是摩擦耗散。相反,对于湿对流,不可逆的熵产生主要由不可逆的相变和水蒸气的扩散决定。另外,潮湿对流中的大部分摩擦耗散是由于降水下降造成的。这种特殊的行为表明,湿对流的作用更像是大气干燥器,而不是热机。这些发现与Rennó和Ingersoll(1996)以及Emanuel和Bister(1996)的假设有很大不同。还表明,由水蒸气的相变和扩散引起的不可逆的熵产生与潜热的对流传输直接相关。因此,对流系统的行为取决于传热在显热和潜热之间的分配方式。最后,将熵预算的研究扩展到包括大规模循环的影响。大规模流动产生的能量,熵和水蒸气可以增强大面积上升区域的对流活动,而在下沉区域则减少对流活动。

著录项

  • 作者

    Pauluis, Olivier M.;

  • 作者单位

    Princeton University.;

  • 授予单位 Princeton University.;
  • 学科 Physics Atmospheric Science.
  • 学位 Ph.D.
  • 年度 2000
  • 页码 274 p.
  • 总页数 274
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 大气科学(气象学);
  • 关键词

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