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全球海洋高频波动主振荡周期的纬向带状分布特征

乔方利 TALEzer 袁业立

乔方利, TALEzer, 袁业立. 全球海洋高频波动主振荡周期的纬向带状分布特征[J]. 海洋学报, 2004, 26(3): 1-7.
引用本文: 乔方利, TALEzer, 袁业立. 全球海洋高频波动主振荡周期的纬向带状分布特征[J]. 海洋学报, 2004, 26(3): 1-7.
QIAO Fang-li, TAL Ezer, YUAN Ye-li. The zonal distribution features of high frequency oscillations in the oceans derived from satellite altimeter data[J]. Haiyang Xuebao, 2004, 26(3): 1-7.
Citation: QIAO Fang-li, TAL Ezer, YUAN Ye-li. The zonal distribution features of high frequency oscillations in the oceans derived from satellite altimeter data[J]. Haiyang Xuebao, 2004, 26(3): 1-7.

全球海洋高频波动主振荡周期的纬向带状分布特征

基金项目: 国家重点基础研究发展规划资助项目——渤黄东海环流及其变异预测数值模式和海洋大气灾害应用(G1999043809)

The zonal distribution features of high frequency oscillations in the oceans derived from satellite altimeter data

  • 摘要: 基于1992年10月至2000年12月的TOPEX/Poseidon和ERS-1/2卫星高度计资料,分析了周期短于150d的高频波动及其能量的空间分布特征.在功率谱密度计算基础上,分析特定频段所含能量占周期短于150d的高濒波动总能量的百分比,发现该频段最强振荡(下文称主振荡)所对应的周期从近赤道的1个月逐步增加至南北纬30°附近的4个月,进一步分析表明主振荡周期的这种变化是连续的,与西向行星Rossby波的相速随纬度增加而变慢相对应.主振荡所对应的周期在全球海洋中呈显著的带状分布.进而表明在14°N(S)附近60d周期的振荡除通常所认为的由于潮汐混淆所造成的虚假信号之外,主要是行星Rossby波形态的真实信号.
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出版历程
  • 收稿日期:  2003-07-10
  • 修回日期:  2003-12-25

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