Testing theories of atmospheric gravity wave saturation and dissipation

Chester S. Gardner
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引用次数: 57

Abstract

Numerous mechanisms have been proposed to account for the dissipation and saturation of gravity waves in the atmosphere. We review the leading wave dissipation paradigms and identify the experimental data required to test definitively the fundamental physics upon which these theories are based. We also examine the separability of the joint vertical wave number (m) and temporal frequency (ω) spectrum and the separability of the unambiguous two-dimensional horizontal wave number spectrum. Definitive tests of the Linear Instability (Dewan and Good, 1986), Saturated-Cascade (Dewan, 1994), and Diffusive Filtering Theories (Gardner, 1994) and separability of the (m, ω) spectrum are within the observational capabilities of modern remote sensing instruments. The Diffusive Damping (Weinstock, 1990) and Doppler Spreading Theories (Hines, 1991) are untestable in their present forms. Separability of the two-dimensional horizontal wave number spectrum is difficult to test using current technology, although analysis of airglow images may provide some insight.

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大气重力波饱和和耗散测试理论
已经提出了许多机制来解释大气中重力波的耗散和饱和。我们回顾了主要的波耗散范式,并确定了最终测试这些理论所依据的基础物理学所需的实验数据。我们还研究了垂直波数(m)和时间频率(ω)联合谱的可分性以及明确的二维水平波数谱的可分性。线性不稳定性(Dewan和Good, 1986年)、饱和级联(Dewan, 1994年)和扩散滤波理论(Gardner, 1994年)以及(m, ω)频谱的可分性的最终测试都在现代遥感仪器的观测能力范围内。扩散阻尼理论(Weinstock, 1990)和多普勒扩散理论(Hines, 1991)目前的形式是无法检验的。二维水平波数谱的可分性很难用现有技术测试,尽管对气辉图像的分析可能会提供一些见解。
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