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首页> 外文期刊>Atmospheric Measurement Techniques Discussions >MAX-DOAS measurements of HONO slant column densities during the MAD-CAT campaign: inter-comparison, sensitivity studies on spectral analysis settings, and error budget
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MAX-DOAS measurements of HONO slant column densities during the MAD-CAT campaign: inter-comparison, sensitivity studies on spectral analysis settings, and error budget

机译:MAD-CAT活动期间HONO斜柱密度的MAX-DOAS测量:相互比较,光谱分析设置的灵敏度研究和误差预算

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pstrongAbstract./strong In order to promote the development of the passive DOAS technique the Multi Axis DOAS a?? Comparison campaign for Aerosols and Trace gases (MAD-CAT) was held at the Max Planck Institute for Chemistry in Mainz, Germany, from June to October??2013. Here, we systematically compare the differential slant column densities (dSCDs) of nitrous acid (HONO) derived from measurements of seven different instruments. We also compare the tropospheric difference of SCDs (delta SCD) of HONO, namely the difference of the SCDs for the non-zenith observations and the zenith observation of the same elevation sequence. Different research groups analysed the spectra from their own instruments using their individual fit software. All the fit errors of HONO dSCDs from the instruments with cooled large-size detectors are mostly in the range of 0.1 to 0.3span class="thinspace"/spana????a??span class="thinspace"/span10sup15/supspan class="thinspace"/spanmoleculesspan class="thinspace"/spancmsupa??2/sup for an integration time of 1span class="thinspace"/spanmin. The fit error for the mini MAX-DOAS is around 0.7span class="thinspace"/spana????a??span class="thinspace"/span10sup15/supspan class="thinspace"/spanmoleculesspan class="thinspace"/spancmsupa??2/sup. Although the HONO delta SCDs are normally smaller than 6span class="thinspace"/spana????a??span class="thinspace"/span10sup15/supspan class="thinspace"/spanmoleculesspan class="thinspace"/spancmsupa??2/sup, consistent time series of HONO delta SCDs are retrieved from the measurements of different instruments. Both fits with a sequential Fraunhofer reference spectrum (FRS) and a daily noon FRS lead to similar consistency. Apart from the mini-MAX-DOAS, the systematic absolute differences of HONO delta SCDs between the instruments are smaller than 0.63span class="thinspace"/spana????a??span class="thinspace"/span10sup15/supspan class="thinspace"/spanmoleculesspan class="thinspace"/spancmsupa??2/sup. The correlation coefficients are higher than 0.7 and the slopes of linear regressions deviate from unity by less than 16span class="thinspace"/span% for the elevation angle of 1?°. The correlations decrease with an increase in elevation angle. All the participants also analysed synthetic spectra using the same baseline DOAS settings to evaluate the systematic errors of HONO results from their respective fit programs. In general the errors are smaller than 0.3span class="thinspace"/spana????a??span class="thinspace"/span10sup15/supspan class="thinspace"/spanmoleculesspan class="thinspace"/spancmsupa??2/sup, which is about half of the systematic difference between the real measurements.brbrThe differences of HONO delta SCDs retrieved in the selected three spectral ranges 335a??361, 335a??373 and 335a??390span class="thinspace"/spannm are considerable (up to 0.57span class="thinspace"/spana????a??span class="thinspace"/span10sup15/supspan class="thinspace"/spanmoleculesspan class="thinspace"/spancmsupa??2/sup) for both real measurements and synthetic spectra. We performed
机译:> >摘要。为了促进无源DOAS技术的发展,多轴DOAS技术应运而生。 2013年6月至2013年10月,在德国美因兹的马克斯·普朗克化学研究所举行了关于气溶胶和微量气体的比较运动(MAD-CAT)。在这里,我们系统地比较了从七种不同仪器的测量结果中得出的亚硝酸(HONO)的差分斜柱密度(dSCD)。我们还比较了HONO的SCD的对流层差异(δSCD),即对于相同高度序列的非天顶观测和天顶观测,SCD的差异。不同的研究小组使用各自的拟合软件分析了自己仪器的光谱。带冷却的大型检测器的仪器的HONO dSCD的所有拟合误差大多在0.1到0.3 class =“ thinspace”> a ???? a ?? class =“ thinspace“> 10 15 class =” thinspace“> 分子 class =” thinspace“> cm a ?? 2 < / sup>的积分时间为1 class =“ thinspace”> min。小型MAX-DOAS的拟合误差约为0.7 class =“ thinspace”> a ???? a ?? class =“ thinspace”> 10 15 < / sup> class =“ thinspace”> 分子 class =“ thinspace”> cm a ?? 2 。尽管HONO增量SCD通常小于6 class =“ thinspace”> a ???? a ?? class =“ thinspace”> 10 15 class =“ thinspace”> 分子 class =“ thinspace”> cm a ?? 2 ,可从中检索到一致的HONO delta SCD时间序列。测量不同的仪器。两者均符合顺序的弗劳恩霍夫参考光谱(FRS)和每日正午FRS的一致性。除了mini-MAX-DOAS,仪器之间HONO delta SCD的系统绝对差小于0.63 class =“ thinspace”> a ??? a ?? class =“ thinspace “> 10 15 class =” thinspace“> 分子 class =” thinspace“> cm a ?? 2 。当仰角为1°°时,相关系数高于0.7,线性回归的斜率偏离单位偏差小于16 class =“ thinspace”> %。随着仰角的增加,相关性减小。所有参与者还使用相同的基线DOAS设置分析了合成光谱,以评估他们各自的拟合程序产生的HONO结果的系统误差。通常,错误小于0.3 class =“ thinspace”> a ???? a ?? class =“ thinspace”> 10 15 < span class =“ thinspace”> 分子 class =“ thinspace”> cm a ?? 2 ,大约是实际测量值之间系统差异的一半。 在选定的三个光谱范围335a ?? 361、335a ?? 373和335a ?? 390中获得的HONO delta SCD的差异非常大(向上)到0.57 class =“ thinspace”> a ???? a ?? class =“ thinspace”> 10 15 class =“ thinspace” > 分子 class =“ thinspace”> cm a ?? 2 )进行实际测量和合成光谱分析。我们执行了

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