日本地球惑星科学連合2021年大会

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[E] 口頭発表

セッション記号 A (大気水圏科学) » A-OS 海洋科学・海洋環境

[A-OS11] Ocean Mixing Frontiers

2021年6月5日(土) 10:45 〜 12:15 Ch.09 (Zoom会場09)

コンビーナ:日比谷 紀之(東京大学大学院理学系研究科地球惑星科学専攻)、座長:日比谷 紀之(東京大学大学院理学系研究科地球惑星科学専攻)

11:45 〜 12:00

[AOS11-11] Observed spectral distortion of temperature microstructure

*Takashi Ijichi1、Louis St. Laurent2 (1.Department of Earth and Planetary Science, Graduate School of Science, The University of Tokyo、2.Applied Physics Laboratory, University of Washington)

キーワード:temperature microstructure, finestructure contamination

Measurements of temperature microstructure from fast response thermistors are becoming more prevalent in the ocean-mixing community to estimate dissipation rates of both turbulent kinetic energy and thermal variance. This dissipation estimation method relies on the spectral shape of scalar microstructure prescribed in the high-Reynolds number turbulence theory. Using diverse datasets, we discuss some problematic cases where observed temperature spectra deviate from the corresponding theoretical one, leading to potential bias in dissipation estimates. From a technical viewpoint, the high-frequency thermistor response is suggested to depend on a vehicle flight condition. When temperature microstructure was measured on board autonomous underwater gliders, the thermistor response is found to be better corrected by a single-pole frequency function with a stronger vehicle speed dependence rather than the conventional double-pole function supported from free-falling vertical microstructure profiler data. From a physics viewpoint, the viscous-convective subrange is found to be greatly contaminated by thermohaline finestructure associated with salt finger convection. The Ozmidov wavenumber is suggested to be a threshold parameter that distinguishes turbulent microstructure from such finestructure contamination.