论文标题

纬度依赖性重力波源变化对中间和上层大气的影响

Effects of latitude-dependent gravity wave source variations on the middle and upper atmosphere

论文作者

Yiğit, Erdal, Medvedev, Alexander S., Ern, Manfred

论文摘要

各种天气现象在下部大气中产生大气重力波(GWS)。它们向上传播,将能量和动力传播到更高的高度,并在将它们沉积在中层和上层大气中时明显影响一般循环。我们使用具有实施的非线性整个大气GW参数化的三维第一原理通用循环模型(GCM)来研究波动活动的全球气候,并在高度到上热层时产生了影响。数值实验是由GW动量通量和温度方差指导的,如SABER(使用宽带发射辐射测定法的Saber(使用宽带发射辐射测定法)在NASA的时机上(热层电离层中层中层中层能量动力学)在2010年测得的。这包括北方夏季较低平流层中GW活性的纬度依赖性和幅度。将建模结果与剑术温度和总绝对动量通量进行了比较,以及高层大气层研究卫星(UARS)数据中的数据层和较低热层中的数据。模拟表明,为了重现中间大气中观察到的循环和波动活性,必须在低大气层的源水平上使用所测量的GW通量。这是因为观察结果包含更广泛的GW,而参数化仅捕获与中层和上层大气动力学相关的一部分。考虑到源的纬度变化可显着改善模拟。

Atmospheric gravity waves (GWs) are generated in the lower atmosphere by various weather phenomena. They propagate upward, carry energy and momentum to higher altitudes, and appreciably influence the general circulation upon depositing them in the middle and upper atmosphere. We use a three-dimensional first-principle general circulation model (GCM) with an implemented nonlinear whole atmosphere GW parameterization to study the global climatology of wave activity and produced effects at altitudes up to the upper thermosphere. The numerical experiments were guided by the GW momentum fluxes and temperature variances as measured in 2010 by the SABER (Sounding of the Atmosphere using Broadband Emission Radiometry) instrument onboard NASA's TIMED (Thermosphere Ionosphere Mesosphere Energetics Dynamics) satellite. This includes the latitudinal dependence and magnitude of GW activity in the lower stratosphere for the boreal summer season. The modeling results were compared to the SABER temperature and total absolute momentum flux, and Upper Atmosphere Research Satellite (UARS) data in the mesosphere and lower thermosphere. Simulations suggest that, in order to reproduce the observed circulation and wave activity in the middle atmosphere, smaller than the measured GW fluxes have to be used at the source level in the lower atmosphere. This is because observations contain a broader spectrum of GWs, while parameterizations capture only a portion relevant to the middle and upper atmosphere dynamics. Accounting for the latitudinal variations of the source appreciably improves simulations.

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