首页> 外文期刊>Atmospheric chemistry and physics >Estimate of bias in Aura TES HDO/H_2O profiles from comparison of TES and in situ HDO/H_2O measurements at the Mauna Loa observatory
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Estimate of bias in Aura TES HDO/H_2O profiles from comparison of TES and in situ HDO/H_2O measurements at the Mauna Loa observatory

机译:通过比较莫纳罗阿天文台的TES和原位HDO / H_2O测量,估算Aura TES HDO / H_2O剖面中的偏差

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摘要

The Aura satellite Tropospheric Emission Spectrometer (TES) instrument is capable of measuring the HDO/H_2O ratio in the lower troposphere using thermal infrared radiances between 1200 and 1350 cm~(-1). However, direct validation of these measurements is challenging due to a lack of in situ measured vertical profiles of the HDO/H_2O ratio that are spatially and temporally co-located with the TES observations. From 11 October through 5 November 2008, we undertook a campaign to measure HDO and H_2O at the Mauna Loa observatory in Hawaii for comparison with TES observations. The Mauna Loa observatory is situated at 3.1 km above sea level or approximately 680 hPa, which is approximately the altitude where the TES HDO/H_2O observations show the most sensitivity. Another advantage of comparing in situ data from this site to estimates derived from thermal IR radiances is that the volcanic rock is heated by sunlight during the day, thus providing significant thermal contrast between the surface and atmosphere; this thermal contrast increases the sensitivity to near surface estimates of tropospheric trace gases. The objective of this inter-comparison is to better characterize a bias in the TES HDO data, which had been previously estimated to be approximately 5 % too high for a column integrated value between 850 hPa and 500 hPa. We estimate that the TES HDO profiles should be corrected downwards by approximately 4.8 % and 6.3 % for Versions 3 and 4 of the data respectively. These corrections must account for the vertical sensitivity of the TES HDO estimates. We estimate that the precision of this bias correction is approximately 1.9 %. The accuracy is driven by the corrections applied to the in situ HDO and H_2O measurements using flask data taken during the inter-comparison campaign and is estimated to be less than 1 %. Future comparisons of TES data to accurate vertical profiles of in situ measurements are needed to refine this bias estimate.
机译:Aura卫星对流层发射光谱仪(TES)能够使用1200至1350 cm〜(-1)之间的热红外辐射来测量对流层下层的HDO / H_2O比。但是,由于缺乏原位测量的HDO / H_2O比垂直分布和与TES观测值在空间和时间上共存的位置,因此直接验证这些测量结果具有挑战性。从2008年10月11日至11月5日,我们在夏威夷的莫纳罗阿天文台开展了一项测量HDO和H_2O的活动,以与TES观测结果进行比较。莫纳罗阿(Mauna Loa)天文台位于海拔3.1公里处或大约680 hPa,大约是TES HDO / H_2O观测值显示最高灵敏度的高度。比较该站点的现场数据与热红外辐射得出的估计值的另一个优势是,火山岩在白天被太阳光加热,从而在地表与大气之间形成明显的热反差。这种热反差增加了对流层痕量气体对近地表估计的敏感性。这种相互比较的目的是更好地描述TES HDO数据中的偏差,该偏差先前估计对于850 hPa和500 hPa之间的色谱柱积分值大约太高5%。我们估计,对于数据的第3版和第4版,TES HDO配置文件应分别向下修正约4.8%和6.3%。这些校正必须考虑TES HDO估算值的垂直敏感性。我们估计该偏差校正的精度约为1.9%。该精度是由使用内部比对活动中获得的烧瓶数据对原位HDO和H_2O测量进行的校正来驱动的,估计其小于1%。需要对TES数据与现场测量的准确垂直剖面进行将来的比较,以完善该偏差估计。

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