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Deriving an atmospheric budget of total organic bromine using airborne in situ measurements from the western Pacific area during SHIVA

机译:使用空气传播的总有机溴的大气预算在Shiva期间使用西太平洋地区的原位测量

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During the recent SHIVA (Stratospheric Ozone: Halogen Impacts in a Varying Atmosphere) project an extensive data set of all halogen species relevant for the atmospheric budget of total organic bromine was collected in the western Pacific region using the Falcon aircraft operated by the German Aerospace agency DLR (Deutsches Zentrum für Luft- und Raumfahrt) covering a vertical range from the planetary boundary layer up to the ceiling altitude of the aircraft of 13 km. In total, more than 700 measurements were performed with the newly developed fully automated in situ instrument GHOST-MS (Gas chromatograph for the Observation of Tracers – coupled with aMass Spectrometer) by the Goethe University of Frankfurt (GUF) and with the onboard whole-air sampler WASP with subsequent groundbased state-of-the-art GC/MS analysis by the University of East Anglia (UEA). Both instruments yield good agreement for all major (CHBr_3 and CH_2Br_2) and minor (CH_2BrCl, CHBrCl_2 and CHBr_2Cl) VSLS (very short-lived substances), at least at the level of their 2σ measurement uncertainties. In contrast to the suggestion that the western Pacific could be a region of strongly increased atmospheric VSLS abundance (Pyle et al., 2011), we found only in the upper troposphere a slightly enhanced amount of total organic bromine from VSLS relative to the levels reported in Montzka and Reimann et al. (2011) for other tropical regions. From the SHIVA observations in the upper troposphere, a budget for total organic bromine, including four halons (H-1301, H-1211, H-1202, H-2402), CH3Br and the VSLS, is derived for the level of zero radiative heating (LZRH), the input region for the tropical tropopause layer (TTL) and thus also for the stratosphere. With the exception of the two minor VSLS CHBrCl_2 and CHBr_2Cl, excellent agreement with the values reported in Montzka and Reimann et al. (2011) is found, while being slightly higher than previous studies from our group based on balloon-borne measurements.
机译:在最近的Shiva(平流层臭氧:不同大气中的卤素撞击)中,使用德国航空航天局运营的Falcon飞机,在西太平洋地区收集了对大气预算的所有卤素物种的广泛数据集。 DLR(Deutsches ZentrumFür-und Raumfahrt)覆盖从行星边界层的垂直范围,直至13公里的飞机的天花板高度。总共有超过700次测量,并在原位仪器Ghost-MS(气相色谱仪中,通过歌曲法兰克福(GUF)和船上全部 - Air采样器WASP随后的地下基础的最先进的GC / MS分析,由East Anglia大学(UEA)进行分析。这两种仪器对所有主要(CHBR_3和CH_2BR_2)和次要(CH_2BRCL,CHBRCL_2和CHBR_2CL)VSL(非常短寿命的物质)产生了良好的一致性,至少在其2σ测量不确定程度上。与西太平洋的建议相比,西太平洋可能是强烈增加的大气vsls丰富(Pyle等,2011),我们仅发现在上层对流层中,相对于报告的水平,来自VSL的总机溴量略微增强在Montzka和Reimann等人。 (2011)对于其他热带地区。从上层对流层中的Shiva观察,总有机溴的预算,包括四个哈龙(H-1301,H-1211,H-1202,H-2402),CH3BR和VSL,用于零辐射的水平加热(LZRH),热带对流层层(TTL)的输入区域,因此也用于平流层。除了两个次要的VSL CHBRCL_2和CHBR_2CL之外,与Montzka和Reimann等人报告的价值观非常吻合。 (2011年)被发现,同时基于气球传播测量的小组以前的研究略高于以前的研究。

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