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- Maejima Yasumitsu
- Ocean Research Institute, The University of Tokyo
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- Iga Keita
- Ocean Research Institute, The University of Tokyo
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- Niino Hiroshi
- Ocean Research Institute, The University of Tokyo
抄録
Upper-tropospheric vortices having a horizontal wavelength of 300-400 km were observed on water vapor images of the Japanese geostationary satellite (MTSAT-1). Grid point values predicted by the Regional Spectral Model of the Japan Meteorological Agency show that the vortices were located along a zonal belt with strong cyclonic shear and horizontal convergence. A quasi-geostrophic linear stability analysis of the basic flow having horizontal and vertical shear shows that the fastest growing mode has a horizontal wavelength, a phase speed and a growth rate that reasonably agree with those of the satellite observation. The amplitude of the fastest growing mode is confined to a region having a meridional width of 2 degrees and a vertical depth of 2 km. An energy budget analysis shows that barotropic instability is the dominant generation mechanism for the growing mode.
収録刊行物
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- SOLA
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SOLA 2 80-83, 2006
公益社団法人 日本気象学会
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キーワード
詳細情報 詳細情報について
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- CRID
- 1390282680198475904
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- NII論文ID
- 130004448407
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- ISSN
- 13496476
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- 本文言語コード
- en
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- データソース種別
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- JaLC
- Crossref
- CiNii Articles
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- 抄録ライセンスフラグ
- 使用不可