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Estimating Upper Silesian coal mine methane emissions from airborne in situ observations and dispersion modeling

机译:估算上部Silesian煤矿甲烷排放原位观察和分散模拟

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Abundant mining and industrial activities located in the Upper Silesian Coal Basin (USCB) lead to large emissions of the potent greenhouse gas (GHG) methane (CH 4 ). The strong localization of CH 4 emitters (mostly confined to known coal mine ventilation shafts) and the large emissions of 448 and 720? kt?CH 4 ?yr ?1 reported in the European Pollutant Release and Transfer Register (E-PRTR?2017) and the Emissions Database for Global Atmospheric Research (EDGAR?v4.3.2), respectively, make the USCB a prime research target for validating and improving CH 4 flux estimation techniques. High-precision observations of this GHG were made downwind of local (e.g., single facilities) to regional-scale (e.g.,?agglomerations) sources in the context of the CoMet 1.0 campaign in early summer 2018. A quantum cascade–interband cascade laser (QCL–ICL)-based spectrometer adapted for airborne research was deployed aboard the German Aerospace Center (DLR) Cessna 208B to sample the planetary boundary layer (PBL) in situ. Regional CH 4 emission estimates for the USCB are derived using a model approach including assimilated wind soundings from three ground-based Doppler lidars. Although retrieving estimates for individual emitters is difficult using only single flights due to sparse data availability, the combination of two flights allows for exploiting different meteorological conditions (analogous to a sparse tomography algorithm) to establish confidence on facility-level estimates. Emission rates from individual sources not only are needed for unambiguous comparisons between bottom-up and top-down inventories but also become indispensable if (independently verifiable) sanctions are to be imposed on individual companies emitting GHGs. An uncertainty analysis is presented for both the regional-scale and facility-level emission estimates. We find instantaneous coal mine emission estimates of 451/423? ± ?77 / 79? kt?CH 4 ?yr ?1 for the morning/afternoon flight of 6?June?2018. The derived fuel-exploitation emission rates coincide ( ± 6? % ) with annual-average inventorial data from E-PRTR?2017 although they are distinctly lower ( ?28 ? % / ?32 ? % ) than values reported in EDGAR?v4.3.2. Discrepancies in available emission inventories could potentially be narrowed down with sufficient observations using the method described herein to bridge the gap between instantaneous emission estimates and yearly averaged inventories.
机译:位于上部Silesian煤盆(USCB)的丰富的采矿和工业活动导致有效的温室气体(GHG)甲烷(CH 4)的大量排放。 CH 4发射器的强大定位(主要限于已知的煤矿通风轴)和448和720的大排放量? KT?CH 4?1在欧洲污染物释放和转移寄存器(E-PRTR?2017)和全球大气研究的排放数据库(Edgar?v4.3.2)中报告,使USCB成为一个主要研究目标验证和改进CH 4磁通估计技术。在2018年夏季夏季夏季彗星1.0活动的环境中,将此GHG的高精度观测沿着区域规模(例如,单个设施)向地区规模(例如,?凝聚)来源。量子级联 - 间 - 间带级联激光器( QCL-ICL)基于德国航空航天中心(DLR)Cessna 208B的德国航空航天中心(DLR)Cessna 208B的QCL-ICL)的谱仪,以原位对行星边界层(PBL)进行采样。 USCB的区域CH 4发射估计是使用模型方法来源的,包括来自三个基于三普勒Lidars的被同化的风声。虽然仅由于稀疏数据可用性仅使用单次飞行来检索单个发射器的估计,但是两个航班的组合允许利用不同的气象条件(类似于稀疏断层摄影算法)来建立对设施级别估计的信心。单个来源的排放率不仅需要在自下而下和自上而下的库存之间明确比较,而且如果要对排放温室气体的个别公司施加制裁(可验证的)制裁也是必不可少的。为区域规模和设施级排放估计提供了不确定性分析。我们发现瞬时煤矿发射估计为451/423? ±77/79? KT?CH 4?YR?1在早晨/下午飞行6?六月?2018年。衍生的燃料开发排放率与来自E-PRTR的年平均来的数据重合(±6?%)2017年,虽然它们明显降低(?28?%/?32?%)而不是Edgar?V4中报告的价值。 3.2。可用排放清单中的差异可能与使用本文所述的方法弥合瞬时发射估计和年平均库存之间的差距来缩小足够的观察。

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