从卫星高度计数据推断的深海的潮能量显著消散
1College of Oceanic and Atmospheric Sciences, Oregon State University, Corvallis 97331, USA. egbert@oce.orst.edu
Nature
|June 24, 2000
概括
海洋潮在深海中消耗大量能量,而不仅仅是浅海. 这种由海底地形驱动的深海潮消散,大大有助于海洋混合和热循环.
科学领域:
- 海洋学 海洋学 海洋学
- 地质物理学 地质物理学
- 流体动力学 流体动力学
背景情况:
- 海洋潮是能量消耗的主要来源,对月球历史和海洋混合有影响.
- 从历史上看,潮能量消耗主要归因于浅海的底部摩擦.
- 证据表明,开放的海洋通过由海底地形产生的内部波浪消散,但估计有所不同.
研究的目的:
- 实证地绘制和量化海洋中的潮能量消耗.
- 为了确定深海潮消散对海洋混合的贡献.
主要方法:
- 利用了来自Topex/Poseidon的卫星高度计数据.
- 经验地绘制了全球海洋的潮能量消散模式.
主要成果:
- 大约1太瓦 (TW) 的潮能量,占总消散量的25-30%,发生在深海.
- 深海消散集中在粗的海底地形区域附近.
- 潮消散可以提供大规模海洋热循环所需的一半能量.
结论:
- 深海的潮消耗是相当大的能量消耗,与浅水消耗相当.
- 潮能量消耗在推动海洋混合和热循环中发挥着至关重要的作用.
- 这一发现修订了我们对海洋能源预算和动态的理解.
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