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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:SHIVA期间使用西太平洋地区的机载原位测量得出总有机溴的大气预算

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During the recent SHIVA (Stratospheric Ozone: Halogen Impacts in a VaryingAtmosphere) project an extensive data set of all halogen species relevant forthe atmospheric budget of total organic bromine was collected in the westernPacific region using the Falcon aircraft operated by the German Aerospaceagency DLR (Deutsches Zentrum für Luft- und Raumfahrt) covering avertical range from the planetary boundary layer up to the ceiling altitudeof the aircraft of 13 km. In total, more than 700 measurements wereperformed with the newly developed fully automated in situ instrumentGHOST-MS (Gas chromatograph for theObservation of Tracers – coupled with aMass Spectrometer) by the Goethe University of Frankfurt(GUF) and with the onboard whole-air sampler WASP with subsequent ground-based state-of-the-art GC / MS analysis by the University of East Anglia(UEA). Both instruments yield good agreement for all major (CHBr3 andCH2Br2) and minor (CH2BrCl, CHBrCl2 and CHBr2Cl)VSLS (very short-lived substances), at least at the level of their 2σmeasurement uncertainties.In contrast to the suggestion that the western Pacific could be a region ofstrongly increased atmospheric VSLS abundance (Pyle et al., 2011), we foundonly in the upper troposphere a slightly enhanced amount of total organicbromine from VSLS relative to the levels reported in Montzka and Reimann etal. (2011) for other tropical regions.From the SHIVA observations in the upper troposphere, a budget for totalorganic 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 thusalso for the stratosphere.With the exception of the two minor VSLS CHBrCl2 and CHBr2Cl,excellent agreement with the values reported in Montzka and Reimann et al. (2011)is found, while being slightly higher than previous studies from ourgroup based on balloon-borne measurements.
机译:在最近的SHIVA(平流层臭氧:不断变化的大气中的卤素影响)项目中,使用由德国航空航天局DLR(Deutsches ZentrumfürLuft-und Raumfahrt)的覆盖范围从行星边界层到飞机最高天花板高度13 km。使用最新开发的全自动原位仪器GHOST-MS( G as c h romatograph对 O b进行了总共700多次测量法兰克福歌德大学(GUF)的 s 赛车-结合了 M ass S 光谱仪) )和机载全空气采样器WASP,以及随后由东英吉利大学(UEA)进行的地面先进的GC / MS分析。两种仪器均对所有主要(CHBr 3 和CH 2 Br 2 )和次要(CH 2 BrCl ,CHBrCl 2 和CHBr 2 Cl)VSLS(非常短寿命的物质),至少处于其2σ测量不确定度的水平。 关于西太平洋可能是大气VSLS丰度大大增加的区域的建议(Pyle等人,2011),我们发现仅在对流层中,相对于Montzka和Reimann等人报道的水平,来自VSLS的总有机溴含量略有增加。 (2011)对于其他热带地区。 从对流层上层的SHIVA观测中,总有机溴的预算包括四个哈龙(H-1301,H-1211,H-1202,H-2402), CH 3 Br和VSLS是针对零辐射加热(LZRH),热带对流层顶层(TTL)以及平流层的输入区域得出的。 除了两个较小的VSLS CHBrCl 2 和CHBr 2 Cl外,与Montzka和Reimann等人报道的值非常吻合。 (2011)被发现,但略高于基于气球测量的本组以前的研究。

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