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Halogen Occultation Experiment (HALOE) altitude registration of atmospheric profile measurements: lessons learned and improvements made during the data validation phase

机译:大气廓线测量的卤素掩星实验(HALOE)高度记录:在数据验证阶段吸取的教训和改进

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Abstract: Measurements by the Halogen Occultation Experiment (HALOE), on board the Upper Atmosphere Research Satellite (UARS) are producing high quality atmospheric profiles of trace gases involved in ozone chemistry. Using eight IR channels to sense the atmospheric absorption of sunlight, HALOE is providing scientists with high quality global fields of HCl, HF, O$-3$/, CH$-4$/, NO, NO$-2$/, H$-2$/O, aerosol extinctions and temperature, shedding new light on the dynamics and chemistry of the atmosphere. Critical to the retrieval of atmospheric constituent profiles from space-borne spectroscopic sensors is the ability to determine the true path through the atmosphere of measured radiation. Since becoming operational in October 1991 new effort has been put into validating and refining the techniques required to estimate the tangent point altitude associated with each signal sample. This is accomplished by measuring transmission of sunlight in the CO$-2$/ 2.8 micron region, and registering the CO$-2$/ transmission profile with a modeled transmission profile based on temperature and pressure data from NMC or UKMO and an assumed CO$-2$/ mixing ratio. In this paper we report on lessons learned during the data validation phase, and improvements made to the altitude registration process. The parameters and processes involved include CO$- 2$/ limb radiance inversion, signal processing, zenith angle estimation, refraction calculations, registration regions and aerosol effects. We also present the results of sensitivity and error analyses which reveal the accuracy required for each estimated parameter in order to register within the specified error budget. !3
机译:摘要:通过上层大气研究卫星(UARS)上的卤素掩星实验(HALOE)进行的测量正在产生涉及臭氧化学的痕量气体的高质量大气廓线。 HALOE使用八个红外通道感应大气中吸收的阳光,为科学家提供了HCl,HF,O $ -3 $ /,CH $ -4 $ /,NO,NO $ -2 $ /,H的高质量全球场$ -2 $ / O,气溶胶的消光和温度,为大气的动力学和化学提供了新的亮点。从星载光谱传感器中检索大气成分剖面的关键是确定通过测量辐射的大气的真实路径的能力。自1991年10月投入使用以来,已投入新的精力来验证和完善估计与每个信号样本相关的切点高度所需的技术。这是通过测量CO $ -2 $ / 2.8微米区域中太阳光的透射率,并根据NMC或UKMO的温度和压力数据以及假定的CO值将CO $ -2 $ /透射率曲线与模型化的透射率曲线进行配准来实现的。 $ -2 $ /混合比例。在本文中,我们报告了在数据验证阶段吸取的教训以及对海拔高度注册过程的改进。涉及的参数和过程包括CO 2-2 /肢体辐射度反演,信号处理,天顶角估计,折射计算,配准区域和气溶胶效应。我们还介绍了灵敏度和误差分析的结果,这些结果揭示了每个估计参数所需的准确度,以便在指定的误差预算内进行记录。 !3

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