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In situ measurements of upper atmospheric atomic oxygen: The ATOX resonant fluorescence/absorption sensor.

机译:高空原子氧的原位测量:ATOX共振荧光/吸收传感器。

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Within the Earth's mesosphere and lower thermosphere (MALT) (50--130 km) lies an important structured layer of atomic oxygen (O), created by the photo-dissociation of diatomic oxygen. The abundance and high reactivity of O plays a critical role in the heat budget, and therefore the dynamics of the region, and is a primary contributor of chemical excitation causing night and day airglow. Because of uncertainties in O concentrations, our quantitative understanding of the thermal and chemical processes within the MALT has been limited.; Over the past two decades, the technique most utilized for the determination of O concentrations has been the measurement of resonant fluorescence of the O(3S- 3P) triplet. U&barbelow;tah S&barbelow;tate U&barbelow;niversity (USU) is one of several groups that have embraced the technique, developing and flying the ATomic OXygen (ATOX) sensor system on sounding rockets. This dissertation reports on a set of observations from two sounding rocket flights launched from the University of Alaska's Poker Flat Research Range, CODA I and CODA II, which flew instruments based on this technique.; While the resonant fluorescence technique appears well suited for the measurement of O in the MALT, the dynamics of the sounding rockets which carry the sensor system create challenges that the system and data analysts must overcome. Primary challenges include density flow field disturbances, Doppler shift of the source lamp emission, and contamination. It has been well documented that these challenges, especially the flow field disturbances, make it difficult to accurately measure O concentration profiles.; This research has quantified the effect of the three major disturbances, seen as errors, and attempts to correct for each. Computations show that the largest errors are introduced by flow field disturbances. With a strong dependence upon measurement attitude and mission geometry, errors in the ram direction are often in excess of 300%. Errors as large as 100% are introduced by Doppler shift of the lamp output, and errors upwards of 40% are introduced into the absorption measurements due to contamination. The approach discussed herein can potentially reduce errors in both the fluorescence and absorption measurements to within 15--20% of undisturbed values. Furthermore, since the corrections are applied across the entire measurement region, direct comparison of upleg and downleg measurements is now possible.
机译:在地球的中层和下热层(MALT)(50--130 km)内,存在着一个重要的结构化原子氧(O)结构层,它是由双原子氧的光离解形成的。 O的丰度和高反应性在热量收支和区域动态中起着至关重要的作用,并且是引起夜间和白天气辉的化学激发的主要因素。由于O浓度的不确定性,我们对MALT中的热和化学过程的定量理解受到限制。在过去的二十年中,最常用于确定O浓度的技术是O(3S-3P)三重态共振荧光的测量。美国大学(USU)是采用该技术的几个小组之一,他们在探测火箭上开发并飞行了原子氧(ATOX)传感器系统。这篇论文报告了阿拉斯加大学扑克室研究范围CODA I和CODA II发射的两次探空火箭飞行的一组观测结果,这些飞行器基于这种技术飞行了仪器。虽然共振荧光技术似乎非常适合于MALT中的O的测量,但是携带传感器系统的探空火箭的动力学带来了系统和数据分析人员必须克服的挑战。主要挑战包括密度流场干扰,源灯发射的多普勒频移和污染。有充分的文献证明,这些挑战,特别是流场干扰,使得难以准确测量O浓度分布。这项研究已经量化了三种主要干扰的影响,这些干扰被视为错误,并尝试对每种干扰进行纠正。计算表明,最大的误差是由流场干扰引起的。由于高度依赖于测量姿态和任务的几何形状,所以冲压方向的误差通常超过300%。灯输出的多普勒频移会引起高达100%的误差,而由于污染,吸收测量中会引入40%以上的误差。本文讨论的方法可以潜在地将荧光和吸收测量中的误差减少到未干扰值的15--20%之内。此外,由于将校正应用于整个测量区域,因此现在可以直接比较上下支腿的测量结果。

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