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Idealised Models Of Sea Ice Thickness Dynamics.

机译:海冰厚度动力学的理想化模型。

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摘要

Thickness distributions of sea ice (g(h)) display a ubiquitous exponential decay (’tail’) in ice above approximately 2 meters thick. This work uses idealised models to examine the root causes of the exponential tail of the sea ice thickness distribution. The ice of thickness greater than 2 meters is formed through the fracture and piling of ice caused by interactions between floes, driven by winds and currents. The material properties of sea ice are complex and mathematical descriptions of the relationship between force and deformation of a floe are still a topic of study. Smoluchowski Coagulation Models (SCMs) are used to develop an abstract representation of redistribution dynamics. SCMs describe populations whose members of fixed size combine at size-dependent rates. SCMs naturally produce exponential or quasi-exponential distributions. An SCM coupled with a thermodynamic component produces qualitatively realistic g(h) under a wide range of conditions. Using the abstract representation of redistribution dynamics from SCMs, a model developed from physical processes specific to sea ice is introduced. Redistribution events occur at rates dependent on the change in potential energy. This model is demonstrated to produce qualitatively realistic g(h). Sensitivity analysis shows that primary model sensitivities are to the relative strengths of the dynamic and thermodynamic components of the model; and to the relative occurrence of ice ridging, shearing and rafting. The exact relationship between the rate of redistribution events and the energy they consume is shown to be of lesser importance. We conclude that the exponential tail of g(h) is a mathematical consequence of the coagulative nature of the ice thickness redistribution process, rather than the material properties of sea ice. These model results suggest the strongest controls on the form of the tail are the relative strengths of thermodynamic and dynamic action, and the relative occurrence of ice ridging, shearing and rafting.
机译:海冰的厚度分布(g(h))在大约2米厚的冰中显示出普遍存在的指数衰减(“尾巴”)。这项工作使用理想化的模型来检查海冰厚度分布的指数尾部的根本原因。厚度大于2米的冰是由风和海流驱动的絮凝物之间的相互作用引起的冰的破裂和堆积形成的。海冰的材料特性很复杂,关于浮力与变形之间关系的数学描述仍然是研究的主题。 Smoluchowski凝血模型(SCM)用于开发重新分布动力学的抽象表示。 SCM描述了其固定大小成员以大小相关的速率合并的人口。 SCM自然会产生指数分布或准指数分布。在广泛的条件下,结合热力学成分的SCM会产生定性的g(h)。使用来自SCM的重新分布动力学的抽象表示,引入了一个从特定于海冰的物理过程开发的模型。重新分布事件的发生速率取决于势能的变化。该模型证明可以产生定性逼真的g(h)。敏感性分析表明,主要模型敏感性是对模型动态和热力学成分的相对强度的影响。以及相对而言发生冰,剪切和漂流。重新分配事件的速率与其消耗的能量之间的确切关系显示为次要的。我们得出结论,g(h)的指数尾部是冰厚度重新分布过程的凝结性质的数学结果,而不是海冰的材料特性。这些模型结果表明,对尾部形状的最强控制是热力学和动力作用的相对强度,以及起冰,剪切和漂流的相对发生。

著录项

  • 作者

    Godlovitch, Daniel.;

  • 作者单位

    University of Victoria (Canada).;

  • 授予单位 University of Victoria (Canada).;
  • 学科 Applied Mathematics.;Physical Oceanography.
  • 学位 Ph.D.
  • 年度 2011
  • 页码 125 p.
  • 总页数 125
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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