南极降水的蒸发控制:利用创新水示踪诊断法进行的 ECHAM6 模型研究

Qinggang Gao, L. Sime, Alison J. McLaren, T. Bracegirdle, Emilie Capron, Rachael H. Rhodes, H. Steen‐Larsen, Xiaoxu Shi, Martin Werner
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摘要

摘要提高我们对南极降水控制的认识对于深入了解过去和未来的极地及全球环境变化至关重要。在此,我们在大气环流模式 ECHAM6 中开发了创新的水追踪诊断方法。这些追踪器提供了有关南极降水的水汽源位置和特性的新的详细信息。在工业化前的模拟中,源于公海的南极年平均降水量的源纬度范围为 49-35∘S,源海面温度范围为 9.8-16.3 ∘C,源 2 米相对湿度范围为 75.6 %-83.3 %,源 10 米风速(vel10)范围为 10.1-11.3 m s-1。这些结果与现有文献的估计一致。与南极沿海降水相比,南极中部降水通过高空输送途径来自更多赤道(遥远)来源。这归因于潮湿的等熵框架,即向极地的水汽输送往往遵循恒定的等效潜在温度。然而,我们发现这一趋势有明显偏差,尤其是在对流层低层,这可能是由于辐射冷却造成的。强降水的来源是长程水汽输送:与其他降水相比,强降水的赤道(遥远)来源要多 2.9∘(300 公里,南极洲平均值)。与南极环流模式(SAM)正相期间的降水相比,南极环流模式负相期间的降水也来自更多的向赤道方向的水汽源(增加了 2.4∘,南极洲的平均值),这可能是由于南极环流模式负相期间行星波被放大所致。此外,年平均降水量的源速度 10 平均比降水量来源的水汽源位置的年平均速度 10 高 2.1 m s-1。这表明,驱动南极降水的水汽蒸发是在比平均风力更大的条件下发生的。我们量化了南大洋表面风对南极降水水汽可用性的动态控制。总之,创新的水追踪诊断技术增强了我们对南极降水控制因素的了解。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Evaporative controls on Antarctic precipitation: an ECHAM6 model study using innovative water tracer diagnostics
Abstract. Improving our understanding of the controls on Antarctic precipitation is critical for gaining insights into past and future polar and global environmental changes. Here we develop innovative water tracing diagnostics in the atmospheric general circulation model ECHAM6. These tracers provide new detailed information on moisture source locations and properties of Antarctic precipitation. In the preindustrial simulation, annual mean Antarctic precipitation originating from the open ocean has a source latitude range of 49–35∘ S, a source sea surface temperature range of 9.8–16.3 ∘C, a source 2 m relative humidity range of 75.6 %–83.3 %, and a source 10 m wind velocity (vel10) range of 10.1 to 11.3 m s−1. These results are consistent with estimates from existing literature. Central Antarctic precipitation is sourced from more equatorward (distant) sources via elevated transport pathways compared to coastal Antarctic precipitation. This has been attributed to a moist isentropic framework; i.e. poleward vapour transport tends to follow constant equivalent potential temperature. However, we find notable deviations from this tendency especially in the lower troposphere, likely due to radiative cooling. Heavy precipitation is sourced by longer-range moisture transport: it comes from 2.9∘ (300 km, averaged over Antarctica) more equatorward (distant) sources compared to the rest of precipitation. Precipitation during negative phases of the Southern Annular Mode (SAM) also comes from more equatorward moisture sources (by 2.4∘, averaged over Antarctica) compared to precipitation during positive SAM phases, likely due to amplified planetary waves during negative SAM phases. Moreover, source vel10 of annual mean precipitation is on average 2.1 m s−1 higher than annual mean vel10 at moisture source locations from which the precipitation originates. This shows that the evaporation of moisture driving Antarctic precipitation occurs under windier conditions than average. We quantified this dynamic control of Southern Ocean surface wind on moisture availability for Antarctic precipitation. Overall, the innovative water tracing diagnostics enhance our understanding of the controlling factors of Antarctic precipitation.
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