The Martian Planetary Boundary Layer: Turbulent kinetic energy and fundamental similarity scales

被引：0

作者：

G. M. Martínez

F. Valero

L. Vázquez

H. M. Elliott

机构：

[1] University of Michigan,Department of Atmospheric, Oceanic, and Space Sciences

[2] Universidad Complutense de Madrid,Facultad de Física

[3] Universidad Complutense de Madrid,Facultad de Informática

来源：

Solar System Research | 2013年 / 47卷

关键词：

Turbulent Kinetic Energy; Large Eddy Simulation; Planetary Boundary Layer; Solar System Research; Planetary Boundary Layer Height;

D O I：

暂无

中图分类号：

学科分类号：

摘要：

We review selected in situ measurements and models aimed at the study of the Martian Planetary Boundary Layer (PBL). We also discuss critically the advantages and limitations of applying similarity theories to the Martian PBL and calculate the fundamental scales predicted by these theories. Finally, we obtain values of the turbulent kinetic energy (TKE) and address its budget by weighting the significance of the different terms involved in it. In situ measurements taken by the Viking and Pathfinder missions along with similarity theories conveniently adapted to Mars are used to obtain the fundamental scales, the TKE and its budget.

引用

页码：446 / 453

页数：7

共 47 条

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