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A sparse reconstruction method for the estimation of multi-resolution emission fields via atmospheric inversion

机译:一种通过大气反演估算多分辨率发射场的稀疏重建方法

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Atmospheric inversions are frequently used to estimate fluxes of atmosphericgreenhouse gases (e.g., biospheric CO2 flux fields) at Earth's surface.These inversions typically assume that flux departures from a prior model arespatially smoothly varying, which are then modeled using a multi-variateGaussian. When the field being estimated is spatially rough, multi-variateGaussian models are difficult to construct and a wavelet-based field modelmay be more suitable. Unfortunately, such models are very high dimensionaland are most conveniently used when the estimation method can simultaneouslyperform data-driven model simplification (removal of model parameters thatcannot be reliably estimated) and fitting. Such sparse reconstruction methodsare typically not used in atmospheric inversions. In this work, we devise a sparse reconstruction method, and illustrate it in an idealized atmospheric inversion problem for theestimation of fossil fuel CO2 (ffCO2) emissions in the lower 48 statesof the USA.Our new method is based on stagewise orthogonal matching pursuit (StOMP), amethod used to reconstruct compressively sensed images. Our adaptationsbestow three properties to the sparse reconstruction procedure which areuseful in atmospheric inversions. We have modified StOMP to incorporate priorinformation on the emission field being estimated and to enforcenon-negativity on the estimated field. Finally, though based on wavelets, ourmethod allows for the estimation of fields in non-rectangular geometries, e.g.,emission fields inside geographical and political boundaries.Our idealized inversions use a recently developed multi-resolution (i.e.,wavelet-based) random field model developed for ffCO2 emissions andsynthetic observations of ffCO2 concentrations from a limited set ofmeasurement sites. We find that our method for limiting the estimated fieldwithin an irregularly shaped region is about a factor of 10 faster thanconventional approaches. It also reduces the overall computational cost bya factor of 2. Further, the sparse reconstruction scheme imposesnon-negativity without introducing strong nonlinearities, such as thoseintroduced by employing log-transformed fields, and thus reaps the benefitsof simplicity and computational speed that are characteristic of linearinverse problems.
机译:大气反演通常用于估算地球表面大气温室气体的通量(例如生物圈CO 2 通量场)。这些反演通常假设先验模型的通量偏差在空间上是平滑变化的,然后进行建模使用多元高斯。当所估计的场在空间上是粗糙的时,难以构建多元高斯模型,并且基于小波的场模型可能更合适。不幸的是,当估计方法可以同时执行数据驱动的模型简化(删除无法可靠估计的模型参数)和拟合时,此类模型的维数很高,最方便使用。这种稀疏的重建方法通常不用于大气反演中。在这项工作中,我们设计了一种稀疏的重建方法,并在理想的大气反演问题中进行了举例说明,以估算下层48中的化石燃料CO 2 (ffCO 2 )排放量 我们的新方法基于阶段性正交匹配追踪(StOMP),该方法用于重建压缩感测图像。我们的改编为稀疏的重建过程赋予了三个特性,这些特性在大气反演中很有用。我们对StOMP进行了修改,以在被估计的发射场上合并先验信息,并在被估计的场上实施非负性。最后,尽管基于小波,我们的方法仍可以估计非矩形几何体中的场,例如地理和政治边界内的发射场。 我们理想化的反演使用了最近开发的多分辨率(即小波)有限的测量站点建立的基于ffCO 2 排放的随机场模型和ffCO 2 浓度的综合观测结果。我们发现,用于限制不规则形状区域内估计场的方法比常规方法快约10倍。它还使总体计算成本降低了2倍。此外,稀疏重建方案在不引入强非线性(例如采用对数变换的字段引入的非线性)的情况下强加了非负性,从而获得了线性逆的特征:简单和计算速度快问题。

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