研究生: |
江紫綾 Tzu-Ling Chiang |
---|---|
論文名稱: |
北南海流況之研究 Circulation structure in the northern South China Sea |
指導教授: |
吳朝榮
Wu, Chau-Ron |
學位類別: |
碩士 Master |
系所名稱: |
地球科學系 Department of Earth Sciences |
論文出版年: | 2006 |
畢業學年度: | 94 |
語文別: | 中文 |
論文頁數: | 85 |
中文關鍵詞: | 海洋數值模式 、南海暖流 、渦旋脫離 |
英文關鍵詞: | ocean numerical modeling, South China Sea Warm Current, eddy shedding |
論文種類: | 學術論文 |
相關次數: | 點閱:290 下載:23 |
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南海(South China Sea,SCS)位於0°N~23°N、99°~121°E,是一個東北-西南走向半封閉性的海盆。其對外的通道多為水深較淺或水道狹窄的海峽,唯有東北部的呂宋海峽具有較廣闊及縱深的水道。
本研究,利用POM(Princeton Ocean Model)建構一個高解析度的區域海流數值模式來模擬並描述南海的流況。運用巢狀嵌合模式系統之方法,利用較大模式範圍輸出之結果,提供南海模式所需之初始條件及邊界條件。並使用AVHRR(Advanced Very High Resolution Radiometer)的海表面溫度。
南海模式(South China Sea Model,SCSM)的範圍東西向介於99°~124°E,南北向介於2°~27°N,水平解析度為1/16°x 1/16°,垂直方向有26個σ層,執行時間為1999~2003年。
本模式可重現南海季節、季內變化,並可成功地模擬出南海暖流(South China Sea Warm Current,SCSWC)。經由分析及試驗得知,風應力的變化並沒有立即地影響南海暖流。另外亦求得呂宋海峽附近之渦旋脫離週期於夏天為90~120天,冬天為40~50天,冬天形成之渦旋個數較多。渦旋脫離後向西行進的速率大約是0.09~0.11公尺/秒,與此區域之第一斜壓羅士培波(1st baroclinic Rossby wave)之行進速率相近。
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