Initial and transient growth of symmetric instability

IF 2.8 2区 地球科学 Q1 OCEANOGRAPHY Journal of Physical Oceanography Pub Date : 2023-11-08 DOI:10.1175/jpo-d-23-0048.1
Satoshi Kimura
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Abstract

Abstract The mechanism of initial and transient perturbations of symmetric instability (SI) in a hydrostatic flow with lateral shear is analyzed by applying the generalized stability analysis. It is well known that the SI’s most rapidly growing motion is along isopycnals, and the growth rates consist of growing, neutral, and decaying modes. The eigenvectors of these 3 modes are not orthogonal to each other, hence the initial and transient perturbations bear little resemblance to the normal mode. Our findings indicate that the emergence of normal modes occurs within a time span of 1-3 inertial periods, which we refer to as the transient state. The overall growth of perturbation energy is divided into three components: geostrophic shear production (GSP), lateral shear production (LSP), and meridional buoyancy flux (MB). During the transient state, the perturbation energy is partly driven by MB, contrary to the normal mode which has zero MB. The relative energy contribution is evaluated through the ratio to GSP. While the MB to GSP ratio of the initial mode is higher than that of the normal mode, the LSP to GSP ratio remains constant. In the absence of the fastest-growing normal mode, MB can serve as the predominant initial energy source. The precise transition in the energy regime is contingent upon the geostrophic Richardson number and Rossby number.
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对称不稳定性的初始和瞬态增长
摘要应用广义稳定性分析方法,分析了带横向剪切的静流体对称失稳初始扰动和瞬态扰动的机理。众所周知,SI最快速增长的运动是沿等轴运动,其增长速率包括增长模式、中性模式和衰减模式。这3种模态的特征向量不是相互正交的,因此初始和瞬态扰动与正态模态几乎没有相似之处。我们的研究结果表明,正常模式的出现发生在1-3个惯性周期的时间跨度内,我们称之为瞬态。扰动能量的总体增长分为地转剪切产生(GSP)、侧向剪切产生(LSP)和经向浮力通量(MB)三个分量。在瞬态时,微扰能量部分是由微波驱动的,而非零微波的正常模式。相对能量贡献通过与GSP的比值来评估。当初始模式的MB / GSP值高于正常模式时,LSP / GSP值保持不变。在没有增长最快模式的情况下,MB可以作为主要的初始能量源。能量状态的精确跃迁取决于地转理查德森数和罗斯比数。
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来源期刊
CiteScore
2.40
自引率
20.00%
发文量
200
审稿时长
4.5 months
期刊介绍: The Journal of Physical Oceanography (JPO) (ISSN: 0022-3670; eISSN: 1520-0485) publishes research related to the physics of the ocean and to processes operating at its boundaries. Observational, theoretical, and modeling studies are all welcome, especially those that focus on elucidating specific physical processes. Papers that investigate interactions with other components of the Earth system (e.g., ocean–atmosphere, physical–biological, and physical–chemical interactions) as well as studies of other fluid systems (e.g., lakes and laboratory tanks) are also invited, as long as their focus is on understanding the ocean or its role in the Earth system.
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