日本地球惑星科学連合2019年大会

講演情報

[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-OS09] 海洋混合学:物質循環・気候・生態系の維持と長周期変動の解明

2019年5月27日(月) 15:30 〜 17:00 301B (3F)

コンビーナ:安田 一郎(東京大学大気海洋研究所)、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)、西岡 純(北海道大学低温科学研究所)、伊藤 進一(東京大学大気海洋研究所)、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)

16:30 〜 16:45

[AOS09-22] Instabilities of finite-amplitude internal wave beams

*大貫 陽平1田中 祐希2 (1.九州大学応用力学研究所、2.東京大学大学院理学系研究科地球惑星科学専攻)

キーワード:内部波、不安定、海水混合

Previous studies have shown that instability of small-amplitude internal wave beams, generated by a surface tide flowing over topography, is most significant at a particular latitude where parametric subharmonic instability (PSI) excites inertial oscillations. Here we extend the discussion to the case of finite-amplitude beams using a new kind of Floquet approach. The disturbance growth rate obtained is quantified in terms of two non-dimensional parameters A and F: velocity shear divided by the buoyancy frequency and the Coriolis parameter divided by the beam frequency. If A is small, PSI is indeed the principle mode under the condition F < 0.5 with the maximum growth rate achieved when the equality holds. As A is increased, however, instability comes to occur even for F > 0.5 but the location of the maximum instability shifts towards lower F, thus totally changing its latitudinal dependence. The resulting energy spectrum is significantly Doppler shifted, and therefore distinguished from that made by PSI. These findings are useful to quantify the energy loss of internal wave beams that causes water mixing prevailing in the major generation sites of internal tides.