Collaborative Research: Observations and Modeling of Primary and Secondary Gravity Waves at all Altitudes over the Andes

大气重力波（GWs）是当空气包裹受到干扰并超过其平衡位置时产生的振荡运动。这些通常是由地形或雷暴引发的。gw对于在整个大气中运输和分配能量和动量至关重要，影响各种过程。在不同类型的GWs中，由高空风调整和湍流引起的二次重力波（SGW）尤为重要。然而，他们这一代是这一现象中最不为人所知的。该项目计划整合观测（卫星和地面）和最先进的数值模型，以提高对重力波的理解。这项工作的目的是增进对(a)初级和次级重力波动力学，(b)大气和其他地球物理流体中发生的湍流和不稳定过程的理解。这些知识可以用于改进天气和气候模型，从而产生更准确的预测，从而有利于商业航空。该项目将为STEM教育做出贡献，为一名研究生、两名博士后研究人员和一名早期职业科学家提供支持。这项工作由航空、物理和动力气象项目以及大气和地球空间科学部共同资助，以支持提高各种机构类型的研究能力、能力和基础设施的项目，如GEO EMBRACE dcl所述。该项目旨在通过使用新颖的观测和机器学习方法解决与GW动力学相关的引人注目的科学问题。计划在这次调查中使用的多仪器数据包括：1)美国宇航局Aqua卫星上的大气红外探测器，用于平流层，2)Na激光雷达，中层温度成像仪，航空航天夜光成像仪，安第斯激光雷达天文台的流星雷达，以及3)火地岛上的类似仪器。计划将一种新的机器学习方法与传统天气模型一起用于这项调查。该项目将定量地了解(a) GW断裂在SGW产生中的作用和重要性，(b)不稳定性和湍流动力学，以及(c) MLT的GW和SGW强迫。这些研究也将促进对SGW来源及其特征的认识。最后，机器学习的成果可能为全球大气模式中不能直接解决大部分GW效应的初级和次级GW的参数化改进打开一个新的窗口。该奖项反映了美国国家科学基金会的法定使命，并通过使用基金会的知识价值和更广泛的影响审查标准进行评估，被认为值得支持。

Atmospheric Gravity waves (GWs) are generated when air parcels get disturbed and overshoot their equilibrium position causing oscillatory motions. These are often triggered by the topography, or thunderstorms. GWs are essential for transporting and distributing energy and momentum throughout the atmosphere, influencing various processes. Among the different types of GWs, secondary gravity waves (SGW) (caused by upper-altitude wind readjustments and turbulence) are particularly important. However, their generation is the least understood aspect of this phenomenon. This project plans to integrate observations (satellite as well as ground-based) and state-of-the-art numerical models to improve the understanding of gravity waves. The effort aims to advance the understanding of (a) both primary and secondary gravity waves dynamics, (b) turbulence and instability processes that occur in the atmosphere and other geophysical fluids. This knowledge can be applied to improve weather and climate models, resulting in more accurate predictions that are beneficial for commercial aviation. This project will contribute to STEM education providing support to a graduate student, two postdoctoral researchers and an early career scientist. This work is jointly funded by Aeronomy, Physical & Dynamical Meteorology programs and Division of Atmospheric and Geospace Sciences to support projects that increase research capabilities, capacity and infrastructure at a wide variety of institution types, as outlined in the GEO EMBRACE DCLThe project aims to address compelling science questions related to GW dynamics by using novel observations and machine learning methods. Multi-instrument data planned to be used in this investigation include: 1) the Atmospheric Infrared Sounder aboard NASA's Aqua satellite for the stratosphere, 2) the Na lidar, Mesosphere Temperature Mapper, Aerospace nightglow imager, and meteor radar at the Andes Lidar Observatory, and 3) comparable instruments on Tierra del Fuego. A new machine learning approach along with conventional weather models are planned to be used for this investigation. This project will provide a quantitative understanding of the (a) roles and importance of GW breaking in SGW generation, (b) instability and turbulence dynamics, and (c) GW and SGW forcing of the MLT. These studies will also advance the understanding of SGW sources and their characteristics. Finally, the machine learning efforts may open a new window for improved parameterizations of primary and secondary GWs in global atmospheric models where the bulk of GW effects cannot be resolved directly.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.