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Sensitivity of the recent methane budget to LMDz sub-grid-scale physical parameterizations

机译:近期甲烷预算对LMDz亚网格规模物理参数化的敏感性

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摘要

With the densification of surface observing networks and the development ofremote sensing of greenhouse gases from space, estimations of methane(CH) sources and sinks by inverse modeling are gaining additionalconstraining data but facing new challenges. The chemical transport model (CTM)linking the flux space to methane mixing ratio space must be able torepresent these different types of atmospheric constraints for providingconsistent flux estimations.Here we quantify the impact of sub-grid-scale physical parameterizationerrors on the global methane budget inferred by inverse modeling. We use thesame inversion setup but different physical parameterizations within oneCTM. Two different schemes for vertical diffusion, twoothers for deep convection, and one additional for thermals in the planetaryboundary layer (PBL) are tested. Different atmospheric methane data sets are used asconstraints (surface observations or satellite retrievals).At the global scale, methane emissions differ, on average, from 4.1 Tg CH per year due to the use of different sub-grid-scaleparameterizations. Inversions using satellite total-column mixing ratiosretrieved by GOSAT are less impacted, at the global scale, byerrors in physical parameterizations. Focusing on large-scale atmospherictransport, we show that inversions using the deep convection scheme ofEmanuel (1991) derive smaller interhemispheric gradients in methaneemissions, indicating a slower interhemispheric exchange. At regional scale,the use of different sub-grid-scale parameterizations induces uncertaintiesranging from 1.2 % (2.7 %) to 9.4 % (14.2 %) of methane emissionswhen using only surface measurements from a background (or anextended) surface network. Moreover, spatial distribution of methaneemissions at regional scale can be very different, depending on both thephysical parameterizations used for the modeling of the atmospherictransport and the observation data sets used to constrain the inversesystem. When usingonly satellite data from GOSAT, we show that the small biases found ininversions using a coarser version of the transport model are actuallymasking a poor representation of the stratosphere–troposphere methanegradient in the model. Improving the stratosphere–troposphere gradientreveals a larger bias in GOSAT CH satellite data, which largelyamplifies inconsistencies between the surface and satellite inversions. A simplebias correction is proposed. The results of this work provide the level ofconfidence one can have for recent methane inversions relative to physicalparameterizations included in CTMs.
机译:随着地面观测网络的致密化和来自空间的温室气体遥感的发展,通过逆模型估算甲烷(CH)源和汇的方法正在获得更多的约束数据,但面临新的挑战。将通量空间与甲烷混合比空间联系起来的化学输运模型(CTM)必须能够代表这些不同类型的大气约束条件,以提供一致的通量估计值。在此,我们量化子网格规模的物理参数误差对推断的全球甲烷预算的影响通过逆向建模。我们使用相同的反演设置,但在oneCTM中使用不同的物理参数设置。测试了两种不同的垂直扩散方案,另外两种用于深对流方案,另外一种用于行星边界层(PBL)中的热效应。不同的大气甲烷数据集被用作约束(地面观测或卫星检索)。在全球范围内,由于使用了不同的次网格规模参数,甲烷的平均排放量与每年4.1 Tg CH有所不同。在全球范围内,使用GOSAT修正的使用卫星总柱混合比进行的反演对物理参数设置中的错误影响较小。着眼于大规模的大气传输,我们表明,使用伊曼纽尔(1991)的深对流方案进行的反演会产生较小的甲烷排放半球间梯度,表明半球间交换较慢。在区域范围内,当仅使用来自背景(或扩展)地面网络的地面测量值时,使用不同的亚网格规模参数设置会导致甲烷排放量的不确定性范围为1.2%(2.7%)至9.4%(14.2%)。而且,取决于用于大气传输模型化的物理参数化和用于约束逆系统的观测数据集,甲烷排放在区域尺度上的空间分布可能会非常不同。当仅使用来自GOSAT的卫星数据时,我们表明使用较粗略的运输模型反演中发现的小偏差实际上掩盖了模型中平流层-对流层甲烷梯度的较差表示。平流层-对流层梯度的改善显示出GOSAT CH卫星数据的较大偏差,这大大放大了地表和卫星反演之间的不一致性。提出了简单偏差校正。这项工作的结果提供了人们对CTM中包含的物理参数化相关的最新甲烷转化的信心水平。

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