RAPID: Evaluation of the Impact of Near-surface Turbulence on the Active Temperature, Ozone and Moisture Microwave Spectrometer (ATOMMS) Measurements

十多年来，首席研究员（PI）和他的团队一直在开发一种大气遥感系统，称为主动温度，臭氧和湿度微波光谱仪（ATOMMS）。ATOMMS结合了全球定位系统（GPS）无线电掩星（RO）和微波临边探测器（MLS）技术的最佳功能，通过无线电掩星（的一个子集）主动探测MLS通过被动发射观测到的吸收线。对现有资料的分析表明，ATOMMS将把对流层和中层大气水汽和中层大气臭氧廓线的分辨率提高到1- 5%，温度提高到0.5K，位势高度提高到10-20 m，在晴朗和多云的空气中，垂直分辨率都达到~200 m。这种前所未有的性能将通过平均化显著提高。由于掩星信号源是在每次掩星之前或之后立即观测到的，因此ATOMMS是自校准的，这消除了长期漂移。这些能力将满足气候变化监测、研究和决策的关键需求。这项研究的重点是几个关键的，近期的研究目标与ATOMMS的发展。该项目的目标是：（1）完成接近完成的ATOMMS仪器的第一个版本，（2）完成仪器的实验室测试和性能评估，（3）使用该仪器首次测量近地表湍流对ATOMMS信号的影响，以及（4）根据最近的理论预测评估这种影响。接近完成的ATOMMS仪器的第一个版本在183 GHz附近提供了两个音调，这是进行有用的差分吸收测量所需的最小数量。简单地说，一个音调测量吸收加上由于天线指向等其他效应而引起的不必要的幅度变化，而第二个音调仅测量不必要的幅度变化。结果，两个音调的幅度的比率在很大程度上去除了不想要的相对宽带效应，如由折射率的真实的部分的湍流波动引起的那些效应，同时保留了大部分期望的气体吸收特征。刚拿到博士学位。该小组确定了一个新的误差源：大气折射率虚部的湍流波动，它将产生与大气折射率真实的部分波动所产生的振幅波动不同的显著振幅波动。地面测量将首次测量由折射率的真实的和虚部的近地表湍流波动引起的ATOMMS信号的闪烁（“星星的闪烁”）的幅度，并提供必要的关键信息，以隔离和更好地了解这一新的误差来源。以上概述的四个步骤对于ATOMMS遥感能力的总体评价和演示至关重要，必须在ATOMMS进入飞行测试和演示阶段之前完成，如果ATOMMS后续建议获得资助，飞行测试和演示阶段将继续进行。这些研究目标是重要的和充分合理的科学，即使ATOMMS后续提案没有得到资助，因为他们将确定和文件的同行评审的文献中的性能的一个新的RO气候仪器和不确定的误差源的ATOMMS气候监测系统的最终性能至关重要。这个项目的智力价值是隔离和量化最近公认的关键误差源。湍流试验将提供信息，以隔离、量化和减少由于假想和真实的湍流活动中的湍流波动而引起的振幅振荡。如果没有这些测量和随后的分析，就不可能量化这一关键误差，从而使ATOMMS的评估不完整，其最终性能也不确定。长期目标是一个由十几个或更多的小型航天器组成的星座，进行ATOMMS掩星测量，这将提供密集的全球覆盖，并在每个轨道上进行完全的云层穿透和昼夜采样。鉴于其独特和强大的组合特性的关键气候，ATOMMS应该是全球气候观测系统的一个关键要素，全球气候观测系统是解决气候变化问题的一个关键组成部分。

For more than ten years, the principal Investigator (PI) and his group have been developing an atmospheric remote sensing system called the Active Temperature, Ozone and Moisture Microwave Spectrometer (ATOMMS). ATOMMS combines the best features of the Global Positioning System (GPS) radio occultation (RO) and the Microwave Limb Sounder (MLS) techniques by actively probing via radio occultation (a subset of) the absorption lines that MLS observes via passive emission. Analyses of available data shows that ATOMMS will profile tropospheric and middle atmosphere water vapor and middle atmosphere ozone to 1-5%, temperature to 0.5K, and geopotential heights to 10-20 m, all with ~200 m vertical resolution, in both clear and cloudy air. This unprecedented performance will improve significantly with averaging. Because the occultation signal source is observed immediately before or after each occultation, ATOMMS is self-calibrating, which eliminates long-term drift. These capabilities will fulfill crucial needs for climate change monitoring, research and policymaking. This research focuses on several critical, near-term research objectives associated with the ATOMMS development. The objectives of this project are to (1) complete the nearly finished first version of the ATOMMS instrument, (2) complete the instrument testing and performance evaluation in the laboratory, (3) use the instrument to measure for the first time the impact of near-surface turbulence on the ATOMMS signals and (4) assess that impact against recent theoretical predictions. The nearly completed, first version of the ATOMMS instrument provides two tones near 183 GHz which is the minimum number needed to make useful differential absorption measurements. Simplistically, one tone measures absorption plus unwanted amplitude variations due to other effects such as antenna pointing and the 2nd tone measures just the unwanted amplitude variations. As a result, the ratio of the amplitudes of the two tones largely removes unwanted relatively broadband effects like those caused by turbulent fluctuations of the real part of the index of refraction while retaining most of the desired gaseous absorption signature. A recent Ph.D. in the group identified a new error source: turbulent fluctuations in the imaginary part of the atmospheric index of refraction that will produce significant amplitude scintillations separate from and in addition to those due to fluctuations in the real part of the refractivity. The ground measurements will for the first time measure the magnitude of the scintillations ("twinkling of a star") of the ATOMMS signals caused by near-surface turbulent fluctuations in the real and imaginary parts of the index of refraction and provide critical information needed to isolate and better understand this new source of error. The four steps summarized above are critical in the overall evaluation and demonstration of the ATOMMS remote sensing capability and must be completed prior to ATOMMS progressing to its flight testing and demonstration phase that will proceed if the ATOMMS follow-on proposal is funded. These research objectives are important and well-justified scientifically even if the ATOMMS follow-on proposal is not funded because they will determine and document in the peer-reviewed literature the performance of a new RO climate instrument and an uncertain error source critical to the ultimate performance of the ATOMMS climate monitoring system. The intellectual merit of this project is to isolate and quantify a recently recognized key source of error. The turbulence testing will provide the information to isolate, quantify and reduce amplitude scintillations due to turbulent fluctuations in the imaginary and real refractivity. Without these measurements and subsequent analysis, it will not be possible to quantify this critical error leaving the assessment of ATOMMS incomplete and its ultimate performance uncertain. The long term goal is a constellation of a dozen or more small spacecraft making ATOMMS occultation measurements which will provide dense, global coverage with complete cloud-penetration and diurnal sampling every orbit. Given its unique and powerful combination of qualities critical to characterizing climate, ATOMMS should be a key element in the global climate observing system Global Climate Observing System (GCOS) which is a crucial component in solving the climate change problem.