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首页> 外文期刊>Frontiers in Marine Science >Measuring Global Ocean Heat Content to estimate the Earth Energy Imbalance
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Measuring Global Ocean Heat Content to estimate the Earth Energy Imbalance

机译:测量全球海洋热量,以估算地球能量失衡

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The energy radiated by the Earth towards space does not compensate the incoming radiation from the Sun leading to a small positive energy imbalance at the top of the atmosphere (0.4-1.Wm-2). This imbalance is coined Earth’s Energy Imbalance (EEI). It is mostly caused by anthropogenic greenhouse gases emissions and is driving the current warming of the planet. Precise monitoring of EEI is critical to assess the current status of climate change and the future evolution of climate. But the monitoring of EEI is challenging as EEI is two order of magnitude smaller than the radiation fluxes in and out of the Earth. Over 93% of the excess energy that is gained by the Earth in response to the positive EEI accumulates into the ocean in the form of heat. This accumulation of heat can be tracked with the ocean observing system such that today, the monitoring of Ocean Heat Content (OHC) and its long-term change provide the most efficient approach to estimate EEI. In this community paper we review the current four state-of-the-art methods to estimate global OHC changes and evaluate their relevance to derive EEI estimate on different time scales. These four methods make use of : 1) direct observations of in situ temperature; 2) satellite-based measurements of the ocean surface net heat fluxes; 3) satellite-based estimates of the thermal expansion of the ocean and 4) ocean reanalyses that assimilate observations from both satellite and in situ instruments. For each method we review the potential and the uncertainty of the method to estimate global OHC changes. We also analyze gaps in the current capability of each method and identify ways of progress for the future to fulfill the requirements of EEI monitoring. Achieving the observation of EEI with sufficient accuracy will depend on merging the remote sensing techniques with in situ measurements of key variables as an integral part of the Ocean Observing System.
机译:地球向太空辐射的能量不能补偿来自太阳的入射辐射,从而导致大气层顶部的正能量不平衡小(0.4-1.Wm-2)。这种失衡是地球的能量失衡(EEI)造成的。它主要是由人为温室气体排放引起的,并正在推动地球的目前变暖。 EEI的精确监控对于评估当前气候变化状况和未来气候变化至关重要。但是对EEI的监测具有挑战性,因为EEI比进出地球的辐射通量小两个数量级。地球响应正EEI所获得的多余能量中,有93%以上以热的形式积累到海洋中。可以使用海洋观测系统跟踪这种热量积聚,因此,今天,对海洋热量(OHC)及其长期变化的监视提供了估算EEI的最有效方法。在本社区文件中,我们回顾了当前四种最先进的方法来估计全球OHC变化,并评估它们的相关性以得出不同时间尺度上的EEI估计值。这四种方法利用:1)直接观察原位温度; 2)基于卫星的海洋表面净热通量测量; 3)基于卫星的海洋热膨胀估算,以及4)海洋重新分析,吸收了来自卫星和原位仪器的观测值。对于每种方法,我们都会评估该方法的潜力和不确定性,以估算全球OHC变化。我们还分析了每种方法的当前能力方面的差距,并确定了将来满足EEI监控要求的进展方式。实现足够准确的EEI观测将取决于将遥感技术与关键变量的原位测量相结合,作为海洋观测系统的组成部分。

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