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Tropospheric infrared mapping spectrometers (TIMS) for Air Quality measurements

机译:用于空气质量测量的对流层红外线映射光谱仪(TIMS)

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We are currently developing grating mapping spectrometers (GMS) with very high spectral resolution, very low noise, and very wide field of view. These also would be very compact facilitating deployment in either a leo or geo application. The measurement set could be very comprehensive, addressing air quality, climate change and meteorology, or subsets of these. For this presentation we'll focus on potential applications of these GMS for air quality measurements of the species ozone O_3, formaldehyde HCHO and carbon monoxide CO. We will discuss these applications at various levels of complexity and the commensurate value for application to understanding and forecasting air quality. At lowest complexity we would utilize a single GMS operating in the solar reflective infrared region for column measurements of O_3 and HCHO. A more complex approach would utilize a second and/or third GMS for thermal emissive O_3 measurements that provide improved vertical resolution, and for CO profile. Our major emphasis is the lowest tropospheric air layer 0-2 km. For realistic models of these GMS we'll present retrieval performance as predicted by a linear error analysis. In a polar leo orbit the most complex approach could provide twice daily global mapping with some footprints as small as 1.6 km at nadir. We'll present results from an in house lab demonstration GMS. This demo is a predecessor to an advanced design that we are currently developing with support of the NASA ESTO Instrument Incubator Program (IIP).
机译:我们目前正在开发光栅映射光谱仪(GMS),具有非常高的光谱分辨率,非常低的噪声和非常广泛的视野。这些也将非常紧凑的促进Leo或Geo应用程序的部署。测量集可以非常全面,解决空气质量,气候变化和气象,或这些气候变化和气象。对于本演示文献,我们将专注于这些GMS的潜在应用,用于物种臭氧O_3,甲醛HCHO和一氧化碳公司的空气质量测量。我们将在各种复杂性和相应的应用中讨论这些应用程序,以便申请理解和预测空气质量。在最低复杂性,我们将利用在太阳能反射红外区域中操作的单个GMS,用于O_3和HCHO的列测量。更复杂的方法将利用第二和/或第三GMS用于热发射O_3测量,其提供改进的垂直分辨率和CO型材。我们的主要重点是0-2公里的最低的对流层空气层。对于这些GMS的现实模型,我们将呈现通过线性错误分析预测的检索性能。在极地Leo轨道中,最复杂的方法可以提供每日两次全球映射,其中一些足迹在Nadir中为1.6公里。我们将呈现在House Lab演示GMS中的结果。该演示是我们目前正在开发的先进设计的前身,支持NASA Esto仪器孵化程序(IIP)。

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