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タイトル: Observed Features of Langmuir Turbulence Forced by Misaligned Wind and Waves Under Destabilizing Buoyancy Flux
著者: Yoshikawa, Yutaka  kyouindb  KAKEN_id  orcid https://orcid.org/0000-0001-7149-5248 (unconfirmed)
Baba, Yasuyuki  kyouindb  KAKEN_id  orcid https://orcid.org/0000-0002-9444-8142 (unconfirmed)
Mizutani, Hideaki
Shimoda, Chikara
Kubo, Teruhiro
著者名の別形: 吉川, 裕
馬場, 康之
水谷, 英朗
久保, 輝広
キーワード: Mixing
Turbulence
Langmuir circulation
発行日: 1-Nov-2018
出版者: American Meteorological Society
誌名: Journal of Physical Oceanography
巻: 48
号: 11
開始ページ: 2737
終了ページ: 2759
抄録: Several features of Langmuir turbulence remain unquantified despite its potentially large impacts on ocean surface mixing. For example, its vertical velocity variance, expected to be proportional to based on numerical simulations, was proportional to in recent field observations, where is the friction velocity and is surface Stokes velocity. To investigate unquantified features of Langmuir turbulence, we conducted a field experiment around a marine observation tower in a shallow sea off the southern coast of Japan in early winter when winds and waves (often swells) were often misaligned. Coherent structures similar to Langmuir cells were successfully identified in the horizontal and vertical structures of turbulent flows measured with upward- and horizontally looking acoustic Doppler current profilers (ADCPs). ADCPs and several anemometers attached at the tower showed that turbulent vertical velocity variance was large when the Langmuir number and Hoenikker number (; where B is surface buoyancy flux and H is the water depth) were both small and that the orientation of the cells was generally aligned in the direction of Lagrangian current shear. These results agree well with the previous numerical results. As in the previous observations, however, the vertical velocity variance appeared to be proportional to . In our experiment, this curious feature was explained by compensatory effects between waves and convection. Misaligned wind with waves also seems to characterize the observed Langmuir turbulence, though further quantitative analysis is required to confirm this result.
著作権等: ©2018 American Meteorological Society.
The full-text file will be made open to the public on 1 May 2019 in accordance with publisher's 'Terms and Conditions for Self-Archiving'.
URI: http://hdl.handle.net/2433/263180
DOI(出版社版): 10.1175/JPO-D-18-0038.1
出現コレクション:学術雑誌掲載論文等

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