由Argo观测到的麦登-朱利安振荡的深海冲击在Argo漂浮器上漂浮
Adrian J Matthews1, Patama Singhruck, Karen J Heywood
1School of Environmental Sciences, University of East Anglia, Norwich NR4 7TJ, UK. a.j.matthews@uea.ac.uk
概括
马登-朱利安振荡 (MJO) 显著影响深海热带海洋,驱动大规模的凯尔文波. 这一发现揭示了大气模式和深海动态之间的关键联系.
科学领域:
- 海洋学 海洋学 海洋学
- 大气科学 大气科学
- 气候动力学 气候动力学
背景情况:
- 马登-朱利安振荡 (MJO) 是热带天气变化的主要驱动因素.
- 了解MJO对深海的影响对于气候建模至关重要.
- 之前的研究主要集中在MJO的大气组成部分.
研究的目的:
- 提供MJO深海热带海洋组成部分的最终证据.
- 为了研究由MJO相关的风力应力异常引起的海洋凯尔文波.
- 量化与MJO相关的深海异常的幅度.
主要方法:
- 使用来自Argo阵列的数据进行概况浮动.
- 分析前所未有的时空覆盖全球海洋上层2000米的数据.
- 研究表面风力应力异常及其对海洋凯尔文波的影响.
主要成果:
- 证实了MJO的深热带海洋组成部分.
- 确定向东传播的海洋赤道凯尔文波延伸到1500米.
- 观察到的深海异常幅度高达年度周期幅度的六倍.
结论:
- 通过凯尔文波,MJO迫使海洋深层有显著的变化.
- 这种深海能量沉对于理解厄尔尼诺-南方振荡 (ENSO) 至关重要.
- 这些发现有助于解释深海测量和改善气候预测.
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