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Investigating the performance of a greenhouse gas observatory in Hefei, China

机译:调查合肥市温室气体天文台的性能

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摘要

A ground-based high-resolution Fourier transform spectrometer (FTS)station has been established in Hefei, China to remotely measure CO, COand other greenhouse gases based on near-infrared solar absorption spectra.Total column measurements of atmospheric CO and CO weresuccessfully obtained from July 2014 to April 2016. The spectra collectedwith an InSb detector in the first year were compared with those collected byan InGaAs detector from July 2015, demonstrating that InGaAs spectra havebetter signal-to-noise ratios and rms of spectral fitting residuals relativeto InSb spectra. Consequently, the measurement precision of the retrievedXCO and XCO for InGaAs spectra is superior to InSb spectra, with about0.04 and 0.09 % for XCO, and 1.07 and 2.00 % for XCO withinclear-sky days respectively. Daily and monthly averages of column-averaged dryair mole fraction of CO show a clear seasonal cycle, while the dailyand monthly averages of XCO displayed no seasonal variation. Also, we analysedthe relationship of the anomalies of XCO and XCO, found that thecorrelations are only observable for individual days, and the data underdifferent prevailing wind conditions during the observations displayed weakcorrelation. The observations based on the high-resolution FTS were alsocompared with the temporally coinciding measurements taken with alow-resolution solar FTS instrument, the EM27/SUN. Ratioing the dailyaveraged XCO of EM27 and FTS gives an overall calibration factor of0.996 ± 0.001. We also compared ground-based observations from theTsukuba TCCON station with our observations, the results showing that thevariation in phase and seasonal amplitude of XCO are similar to ourresults, but the variation of XCO in Tsukuba is quite different from our datain Hefei. To further evaluate our retrieved data, we made use of satellitemeasurements. The direct comparison of our observations with the GreenhouseGases Observing Satellite (GOSAT) data shows good agreement of daily medianXCO, with a bias of −0.52 ppm and standard deviation of 1.63 ppm. The correlation coefficient () is 0.79 for daily medianXCO between our FTS and GOSAT observations. Daily median OrbitingCarbon Observatory 2 (OCO-2) data produce a positive bias of 0.81 ppm andstandard deviation of 1.73 ppm relative to our ground-based data. Our daily median XCO also show strong correlation withOCO-2 data, with correlation coefficient () of 0.83. Although therewere a limited number of data during the observations due to instrumentdowntime and adverse weather, the results confirm the suitability of theobservatory for ground-based long-term measurements of greenhouse gases withhigh precision and accuracy, and fulfil the requirements of the Total CarbonColumn Observing Network (TCCON).
机译:在中国合肥建立了地面高分辨率傅里叶变换光谱仪(FTS)站,可基于近红外太阳吸收光谱对CO,CO和其他温室气体进行远程测量。 2014年7月至2016年4月。将第一年使用InSb检测器收集的光谱与2015年7月以来InGaAs检测器收集的光谱进行比较,证明InGaAs光谱相对于InSb光谱具有更好的信噪比和光谱拟合残差的均方根值。因此,在InGaAs光谱中检索到的XCO和XCO的测量精度优于InSb光谱,在晴朗的日子里,XCO的分别约为0.04和0.09%,XCO的分别为1.07和2.00%。 CO的柱平均干燥空气摩尔分数的日和月平均值显示出一个清晰的季节周期,而XCO的日和月平均值没有显示出季节变化。此外,我们分析了XCO和XCO异常之间的关系,发现相关性仅在个别天中可以观察到,并且在观测期间不同主要风况下的数据显示出弱相关性。基于高分辨率FTS的观测结果也与使用低分辨率太阳能FTS仪器EM27 / SUN进行的时间一致测量值进行了比较。将EM27和FTS的每日平均XCO进行比例,得出总校准系数为0.996±0.001。我们还将筑波TCCON站的地面观测资料与我们的观测资料进行了比较,结果表明,XCO的相位和季节振幅的变化与我们的结果相似,但筑波的XCO的变化与合肥的数据有很大不同。为了进一步评估检索到的数据,我们使用了卫星测量。我们的观测结果与“温室气体观测卫星”(GOSAT)数据的直接比较表明,每日中值XCO很好地吻合,偏差为-0.52 ppm,标准偏差为1.63 ppm。我们的FTS和GOSAT观测值之间的每日中值XCO的相关系数()为0.79。相对于我们的地面数据,每天的轨道碳天文台2(OCO-2)数据的正偏差为0.81 ppm,标准偏差为1.73 ppm。我们的每日XCO中值与OCO-2数据也显示出很强的相关性,相关系数()为0.83。尽管由于仪器停机和恶劣天气而导致观测期间的数据数量有限,但结果证实了该天文台适用于地面长期,高精度和高精度的温室气体测量,并满足了Total CarbonColumn观测网的要求(TCCON)。

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