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WeatherBench 2: A Benchmark for the Next Generation of Data-Driven Global Weather Models WeatherBench 2:下一代数据驱动型全球天气模式的基准
IF 6.8 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-06-18 DOI: 10.1029/2023MS004019
Stephan Rasp, Stephan Hoyer, Alexander Merose, Ian Langmore, Peter Battaglia, Tyler Russell, Alvaro Sanchez-Gonzalez, Vivian Yang, Rob Carver, Shreya Agrawal, Matthew Chantry, Zied Ben Bouallegue, Peter Dueben, Carla Bromberg, Jared Sisk, Luke Barrington, Aaron Bell, Fei Sha

WeatherBench 2 is an update to the global, medium-range (1–14 days) weather forecasting benchmark proposed by (Rasp et al., 2020, https://doi.org/10.1029/2020ms002203), designed with the aim to accelerate progress in data-driven weather modeling. WeatherBench 2 consists of an open-source evaluation framework, publicly available training, ground truth and baseline data as well as a continuously updated website with the latest metrics and state-of-the-art models: https://sites.research.google/weatherbench. This paper describes the design principles of the evaluation framework and presents results for current state-of-the-art physical and data-driven weather models. The metrics are based on established practices for evaluating weather forecasts at leading operational weather centers. We define a set of headline scores to provide an overview of model performance. In addition, we also discuss caveats in the current evaluation setup and challenges for the future of data-driven weather forecasting.

WeatherBench 2 是对(Rasp 等人,2020 年,https://doi.org/10.1029/2020ms002203)提出的全球中程(1-14 天)天气预报基准的更新,旨在加快数据驱动天气建模的进展。WeatherBench 2 由一个开源评估框架、公开可用的训练、地面实况和基线数据以及一个持续更新的网站组成,该网站提供最新的指标和最先进的模型:https://sites.research.google/weatherbench。本文介绍了评估框架的设计原则,并展示了当前最先进的物理和数据驱动天气模型的结果。衡量标准是基于主要业务气象中心评估天气预报的既定做法。我们定义了一组标题分数,以提供模型性能概览。此外,我们还讨论了当前评估设置中的注意事项以及数据驱动天气预报未来面临的挑战。
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引用次数: 0
Zeitlin Truncation of a Shallow Water Quasi-Geostrophic Model for Planetary Flow 齐特林截断行星流浅水准地转模型
IF 6.8 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-06-15 DOI: 10.1029/2023MS003901
A. D. Franken, M. Caliaro, P. Cifani, B. J. Geurts

In this work, we consider a Shallow-Water Quasi Geostrophic equation on the sphere, as a model for global large-scale atmospheric dynamics. This equation, previously studied by Verkley (2009, https://doi.org/10.1175/2008jas2837.1) and Schubert et al. (2009, https://doi.org/10.3894/james.2009.1.2), possesses a rich geometric structure, called Lie-Poisson, and admits an infinite number of conserved quantities, called Casimirs. In this paper, we develop a Casimir preserving numerical method for long-time simulations of this equation. The method develops in two steps: first, we construct an N-dimensional Lie-Poisson system that converges to the continuous one in the limit N → ; second, we integrate in time the finite-dimensional system using an isospectral time integrator, developed by Modin and Viviani (2020, https://doi.org/10.1017/jfm.2019.944). We demonstrate the efficacy of this computational method by simulating a flow on the entire sphere for different values of the Lamb parameter. We particularly focus on rotation-induced effects, such as the formation of jets. In agreement with shallow water models of the atmosphere, we observe the formation of robust latitudinal jets and a decrease in the zonal wind amplitude with latitude. Furthermore, spectra of the kinetic energy are computed as a point of reference for future studies.

在这项研究中,我们将球面上的浅水准地养方程视为全球大尺度大气动力学的模型。Verkley (2009, https://doi.org/10.1175/2008jas2837.1) 和 Schubert 等人 (2009, https://doi.org/10.3894/james.2009.1.2) 曾对该方程进行过研究,它具有丰富的几何结构(称为 Lie-Poisson),并允许存在无穷多个守恒量(称为 Casimirs)。在本文中,我们开发了一种卡西米尔守恒数值方法,用于该方程的长时间模拟。该方法分为两个步骤:首先,我们构建了一个 N 维的 Lie-Poisson 系统,该系统在极限 N → ∞ 时收敛于连续系统;其次,我们使用 Modin 和 Viviani (2020, https://doi.org/10.1017/jfm.2019.944) 开发的等谱时间积分器对有限维系统进行时间积分。我们通过模拟整个球面上不同兰姆参数值的流动,证明了这种计算方法的有效性。我们特别关注旋转引起的效应,如喷流的形成。与浅水大气模型相一致,我们观察到形成了强大的纬向喷流,并且带状风振幅随纬度的变化而减小。此外,我们还计算了动能谱,作为今后研究的参考。
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引用次数: 0
Inversion of Sea Surface Currents From Satellite-Derived SST-SSH Synergies With 4DVarNets 利用卫星获取的 SST-SSH 与 4DVarNets 的协同作用反演海面洋流
IF 6.8 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-06-15 DOI: 10.1029/2023MS003609
R. Fablet, B. Chapron, J. Le Sommer, F. Sévellec

Satellite altimetry offers a unique approach for direct sea surface current observation, but it is limited to measuring the surface-constrained geostrophic component. Ageostrophic dynamics, prevalent at horizontal scales below 100 km and time scales below 10 days, are often underestimated by ocean reanalyzes employing data assimilation schemes. To address this limitation, we introduce a novel deep learning scheme, rooted in a variational data assimilation formulation with trainable observations and a priori terms, that harnesses the synergies between satellite-derived sea surface observations, namely sea surface height (SSH) and sea surface temperature (SST), to enhance sea surface current reconstruction. Numerical experiments, conducted using realistic simulations, in a case study area of the Gulf Stream, demonstrate the potential of the proposed scheme to capture ageostrophic dynamics at time scales of 2.5–3.0 days and horizontal scales of 0.5°–0.7°. The analysis of diverse observation configurations, encompassing nadir along-track altimetry, wide-swath SWOT (Surface Water and Ocean Topography) altimetry, and SST data, highlights the pivotal role of SST features in retrieving a significant portion of the ageostrophic dynamics (approximately 47%). These findings underscore the potential of deep learning and 4DVarNet schemes in improving ocean reanalyzes and enhancing our understanding of ocean dynamics.

卫星测高法为直接观测海面洋流提供了一种独特的方法,但它仅限于测量受海面约束的地营成分。在 100 公里以下水平尺度和 10 天以下时间尺度上普遍存在的地转营养动力学常常被采用数据同化方案的海洋再分析所低估。为了解决这一局限性,我们引入了一种新的深度学习方案,该方案植根于可训练观测数据和先验项的变分数据同化公式,利用卫星海面观测数据(即海面高度(SSH)和海面温度(SST))之间的协同作用来加强海面洋流重建。在墨西哥湾流案例研究区进行的实际模拟数值实验表明,所提出的方案有潜力捕捉时间尺度为 2.5-3.0 天、水平尺度为 0.5-0.7 度的老化动态。对不同观测配置(包括天底沿轨测高、宽波长 SWOT(地表水和海洋地形)测高和 SST 数据)的分析突出表明,SST 特征在检索很大一部分(约 47%)老养动态方面起着关键作用。这些发现强调了深度学习和 4DVarNet 方案在改进海洋再分析和加强我们对海洋动力学的理解方面的潜力。
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引用次数: 0
Moisture Dependence of an African Easterly Wave Within the West African Monsoon System 西非季风系统中非洲东风浪潮的水汽依赖性
IF 6.8 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-06-15 DOI: 10.1029/2023MS004070
K. M. Núñez Ocasio, C. A. Davis, Z. L. Moon, Q. A. Lawton

The growth and propagation of African easterly waves (AEWs) remains an active area of research, especially for those that become tropical cyclones (TCs). This is partly due to the complex role of moisture, realized through AEW-convection interactions. The goal of this study is to understand how environmental moisture plays a role in influencing the growth and propagation of a case of an AEW-convection system, that became a TC and how that role relates to the West African Monsoon System. Moisture sensitivity experiments were performed in a regional and convection-permitting novel configuration. It is found that in a moister environment, diabatic heating associated with convection coupled to the wave is shallower, ultimately, weakening the wave amplitude. Energetics are reduced in a moister environment as the African easterly jet strengthens, yet narrows, and shifts northward limiting interaction with the monsoon and the wave-convection system. The more intense monsoonal flow in a moister environment can instigate the decoupling between convection and AEW as deep convection is more likely in the ridge rather than in the trough region. Over western Africa, more continuous rainfall over the Guinea Highlands can inhibit phase locking with the AEW. In a moister environment, the mean zonal flow is weaker and as a result, the westward translation speed of the wave due to mean flow advection is slower than in the other experiments. While the mean flow advection dominates the translation, further differences in phase speed arise from differences in convection within the wave.

非洲东风波(AEWs)的生长和传播仍然是一个活跃的研究领域,特别是对于那些变成热带气旋(TCs)的东风波。这部分是由于通过非洲东风-对流相互作用实现的水汽的复杂作用。本研究的目的是了解环境湿度如何影响成为热带气旋的 AEW 对流系统的生长和传播,以及这种作用与西非季风系统的关系。在区域和允许对流的新配置中进行了湿度敏感性实验。实验发现,在湿度较高的环境中,与波浪耦合的对流相关的绝热加热较浅,最终会减弱波幅。在湿润的环境中,由于非洲东风喷流增强,但却变窄,并向北移动,限制了与季风和波浪对流系统的相互作用,从而降低了能量。在较湿润的环境中,季风气流更加强烈,这可能会导致对流与 AEW 脱钩,因为深对流更有可能出现在海脊而不是海槽区域。在非洲西部,几内亚高原更持续的降雨会抑制与 AEW 的相位锁定。在湿度较高的环境中,平均带流较弱,因此平均流平流导致的波浪西移速度比其他试验慢。虽然平均流平流在平移中占主导地位,但波浪内部对流的不同也会导致相位速度的进一步差异。
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引用次数: 0
Global Optimization of Soil Texture Maps From Satellite-Observed Soil Moisture Drydowns and Its Implementation in Noah-MP Land Surface Model 根据卫星观测到的土壤水分干缩量绘制土壤纹理图的全球优化及其在 Noah-MP 陆面模型中的应用
IF 6.8 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-06-14 DOI: 10.1029/2023MS004142
Qing He, Hui Lu, Kun Yang, Taikan Oki, Jianhong Zhou, Long Zhao, Panpan Yao, Jie He, Aihui Wang, Yawei Xu

Soil moisture (SM) plays an important role in regulating regional weather and climate. However, the simulations of SM in current land surface models (LSMs) contain large biases and model spreads. One primary reason contributing to such model biases could be the misrepresentation of soil texture in LSMs, since current available large-scale soil texture data are often generated from extrapolation algorithm based on a scarce number of in-situ geological measurements. Fortunately, recent advancements in satellite technology provide a unique opportunity to constrain the soil texture data sets by introducing observed information at large spatial scales. Here, two major soil texture baseline data sets (Global Soil Data sets for Earth system science, GSDE and Harmonized World Soil Data from Food and Agriculture Organization, HWSD) are optimized with satellite-estimated soil hydraulic parameters. The optimized soil maps show increased (decreased) sand (clay) content over arid regions. The soil organic carbon (SOC) content increases globally especially over regions with dense vegetation cover. The optimized soil texture data sets are then used to run simulations in one example LSM, that is, Noah LSM with Multiple Parameters. Results show that the simulated SM with satellite-optimized soil texture maps is improved at both grid and in-situ scales. Intercase comparison analyses show the SM improvement differs between simulations using different soil maps and soil hydraulic schemes. Our results highlight the importance of incorporating observation-oriented calibration on soil texture in current LSMs. This study also joins the call for a better soil profile representation in the next generation of Earth System Models (ESMs).

土壤水分在调节区域天气和气候方面发挥着重要作用。然而,目前的陆地表面模式(LSM)对土壤水分的模拟存在很大的偏差和模式差异。造成这种模型偏差的一个主要原因可能是 LSM 中对土壤质地的错误描述,因为目前可用的大尺度土壤质地数据通常是根据数量稀少的原位地质测量数据通过外推算法生成的。幸运的是,卫星技术的最新进展提供了一个独特的机会,通过引入大空间尺度的观测信息来约束土壤质地数据集。在此,利用卫星估算的土壤水力参数对两个主要的土壤质地基线数据集(地球系统科学全球土壤数据集 GSDE 和粮食及农业组织统一世界土壤数据 HWSD)进行了优化。优化后的土壤分布图显示,干旱地区沙(粘)含量增加(减少)。在全球范围内,土壤有机碳(SOC)含量增加,尤其是在植被茂密的地区。优化后的土壤质地数据集被用于在一个示例 LSM(即多参数 Noah LSM)中进行模拟。结果表明,利用卫星优化的土壤质地图模拟的 SM 在网格和原地尺度上都有所改进。案例间对比分析表明,使用不同土壤分布图和土壤水力方案进行模拟时,SM 的改善程度是不同的。我们的研究结果凸显了将以观测为导向的土壤质地校准纳入当前 LSM 的重要性。这项研究也呼吁在下一代地球系统模式(ESM)中更好地表现土壤剖面。
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引用次数: 0
Adaptive Covariance Hybridization for the Assimilation of SST Observations Within a Coupled Earth System Reanalysis 在耦合地球系统再分析中采用自适应协方差混合法同化 SST 观测数据
IF 6.8 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-06-14 DOI: 10.1029/2023MS003888
Sébastien Barthélémy, François Counillon, Yiguo Wang

Ensemble data assimilation methods, such as the Ensemble Kalman Filter (EnKF), are well suited for climate reanalysis because they feature flow-dependent covariance. However, because Earth System Models are heavy computationally, the method uses a few tens of members. Sampling error in the covariance matrix can introduce biases in the deep ocean, which may cause a drift in the reanalysis and in the predictions. Here, we assess the potential of the hybrid covariance approach (EnKF-OI) to counteract sampling error. The EnKF-OI combines the flow-dependent covariance computed from a dynamical ensemble with another covariance matrix that is static but less prone to sampling error. We test the method within the Norwegian Climate Prediction Model, which combines the Norwegian Earth System Model and the EnKF. We test the performance of the reanalyzes in an idealized twin experiment, where we assimilate synthetic sea surface temperature observations monthly over 1980–2010. The dynamical and static ensembles consist respectively of 30 members and 315 seasonal members sampled from a pre-industrial run. We compare the performance of the EnKF to an EnKF-OI with a global hybrid coefficient, referred to as standard hybrid, and an EnKF-OI with adaptive hybrid coefficients estimated in space and time. Both hybrid covariance methods cure the bias introduced by the EnKF at intermediate and deep water. The adaptive EnKF-OI performs best overall by addressing sampling noise and rank deficiencies issues and can sustain low analysis errors by doing smaller updates than the standard hybrid version.

集合数据同化方法,如集合卡尔曼滤波器(EnKF),非常适合气候再分析,因为它们具有随流量变化的协方差。然而,由于地球系统模型的计算量很大,该方法只使用几十个成员。协方差矩阵中的采样误差会给深海带来偏差,从而可能导致再分析和预测结果的漂移。在此,我们评估了混合协方差方法(EnKF-OI)抵消采样误差的潜力。EnKF-OI 将从动态集合中计算出的与流相关的协方差与另一个静态但不易出现采样误差的协方差矩阵相结合。我们在挪威气候预测模式中测试了该方法,该模式结合了挪威地球系统模式和EnKF。我们在一个理想化的孪生实验中测试了再分析的性能,在该实验中,我们同化了1980-2010年期间每月的合成海面温度观测数据。动态集合和静态集合分别由 30 个成员和 315 个季节成员组成,这些成员是从工业化前的运行中采样的。我们将 EnKF 的性能与带有全局混合系数(称为标准混合系数)的 EnKF-OI 和带有在空间和时间上估计的自适应混合系数的 EnKF-OI 进行了比较。这两种混合协方差方法都能消除 EnKF 在中层和深层水引入的偏差。自适应 EnKF-OI 通过解决采样噪声和等级缺陷问题,总体表现最佳,并且与标准混合版本相比,更新次数更少,因此能维持较低的分析误差。
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引用次数: 0
Understanding Disturbance Regimes From Patterns in Modeled Forest Biomass 从模拟森林生物量的模式了解干扰机制
IF 6.8 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-06-14 DOI: 10.1029/2023MS004099
Siyuan Wang, Hui Yang, Sujan Koirala, Matthias Forkel, Markus Reichstein, Nuno Carvalhais

Natural and anthropogenic disturbances are important drivers of tree mortality, shaping the structure, composition, and biomass distribution of forest ecosystems. Differences in disturbance regimes, characterized by the frequency, extent, and intensity of disturbance events, result in structurally different landscapes. In this study, we design a model-based experiment to investigate the links between disturbance regimes and spatial biomass patterns. First, the effects of disturbance events on biomass patterns are simulated using a simple dynamic carbon cycle model based on different disturbance regime attributes, which are characterized via three parameters: μ (probability scale), α (clustering degree), and β (intensity slope). 856,800 dynamically stable biomass patterns were then simulated using combined disturbance regime, primary productivity, and background mortality. As independent variables, we use biomass synthesis statistics from simulated biomass patterns to retrieve three disturbance regime parameters. Results show confident inversion of all three “true” disturbance parameters, with Nash-Sutcliffe efficiency of 94.8% for μ, 94.9% for α, and 97.1% for β. Biomass histogram statistics primarily dominate the prediction of μ and β, while texture features have a more substantial influence on α. Overall, these results demonstrate the association between biomass patterns and disturbance regimes. Given the increasing availability of Earth observation of biomass, our findings open a new avenue to understand better and parameterize disturbance regimes and their links with vegetation dynamics under climate change. Ultimately, at a large scale, this approach would improve our current understanding of controls and feedback at the biosphere-atmosphere interface in the present Earth system models.

自然和人为干扰是导致树木死亡的重要因素,它们影响着森林生态系统的结构、组成和生物量分布。以干扰事件的频率、范围和强度为特征的干扰机制的差异会导致不同的景观结构。在本研究中,我们设计了一个基于模型的实验来研究干扰机制与空间生物量模式之间的联系。首先,我们使用一个简单的动态碳循环模型模拟了干扰事件对生物量模式的影响,该模型基于不同的干扰机制属性,通过三个参数来表征:μ(概率标度)、α(集群度)和β(强度斜率)。然后,利用综合干扰机制、初级生产力和背景死亡率模拟 856 800 种动态稳定的生物量模式。作为自变量,我们利用模拟生物量模式中的生物量综合统计来检索三个干扰机制参数。结果显示,对所有三个 "真实 "干扰参数的反演都很有把握,μ的纳什-萨特克利夫效率为94.8%,α为94.9%,β为97.1%。生物量直方图统计主要主导μ和β的预测,而纹理特征对α的影响更大。总之,这些结果表明了生物量模式与干扰制度之间的联系。鉴于对生物量的地球观测越来越多,我们的发现为更好地理解和参数化气候变化下的扰动机制及其与植被动态之间的联系开辟了一条新途径。最终,在大范围内,这种方法将改善我们目前对现有地球系统模型中生物圈-大气界面的控制和反馈的理解。
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引用次数: 0
A Pressure Projection Scheme With Near-Spectral Accuracy for Nonhydrostatic Flow in Domains With Open Boundaries 一种近谱精度的压力投影方案,适用于具有开放边界的域中的非静水流体
IF 6.8 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-06-14 DOI: 10.1029/2023MS004040
K. B. Winters, Mariona Claret, M.-Pascale Lelong, Yann Ourmières

We describe a pressure projection scheme for the simulation of incompressible flow in cubic domains with open boundaries based on fast Fourier transforms. The scheme is implemented in flow_solve, a numerical code designed for process studies of rotating, density-stratified flow. The main algorithmic features of the open-boundary code are the near-spectral accuracy of the discrete differentiation and a dynamic two-dimensional domain decomposition that scales efficiently to large numbers of processors. The simulated flows are not required to be periodic or to satisfy symmetry conditions at the open boundaries owing to the use of mixed series expansions combining cosine and singular Bernoulli polynomial basis functions. These expansions facilitate the imposition of inhomogeneous boundary conditions and allow the code to be used for offline, one-way nesting within an arbitrarily embedded subdomain of a larger scale simulation. The projection scheme is designed to exploit a simple and powerful numerical engine: inversion of Poisson's equation with homogeneous Neumann boundary conditions using fast cosine transforms. Here, we describe the mathematical transformations used to accommodate the imposition of space- and time-varying boundary conditions. The utility of the approach for process studies and for nesting within submesoscale-resolving ocean models is demonstrated with simulations of wind-driven near-inertial waves in the upper ocean.

我们介绍了一种基于快速傅立叶变换的压力投影方案,用于模拟具有开放边界的立方域中的不可压缩流动。该方案是在 flow_solve 中实施的,这是一种专为旋转、密度分层流动过程研究而设计的数值代码。开放边界代码的主要算法特点是离散微分的近谱精度和动态二维域分解,可高效地扩展到大量处理器。由于使用了余弦函数和奇异伯努利多项式基函数的混合序列展开,模拟流动不需要周期性,也不需要满足开放边界的对称条件。这些扩展便于施加非均质边界条件,并允许在更大规模模拟的任意嵌入子域内使用代码进行离线单向嵌套。投影方案旨在利用一个简单而强大的数值引擎:使用快速余弦变换反演具有同质诺伊曼边界条件的泊松方程。在此,我们将介绍用于适应空间和时间变化边界条件的数学变换。通过模拟上层海洋的风驱动近惯性波,证明了该方法在过程研究和亚中尺度分辨率海洋模型嵌套中的实用性。
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引用次数: 0
Development of WACCM With the Non-Hydrostatic MPAS-A Dynamical Core 利用非静力学 MPAS-A 动力核心开发 WACCM
IF 6.8 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-06-14 DOI: 10.1029/2023MS004108
S. Kamali, H.-L. Liu, W. Skamarock, J. Klemp, F. Vitt, P. H. Lauritzen

The non-hydrostatic Model for Prediction Across Scales-Atmosphere (MPAS-A) dynamical core has recently been adapted for the Specified Chemistry Whole Atmosphere Community Climate Model (SC-WACCM). In this study, the mean zonal wind and temperature climatology from SC-WACCM/MPAS-A is compared with the results from SC-WACCM using the finite volume and spectral element dynamical cores, as well as the zonal wind and temperature climatology of Upper Atmosphere Research Satellite mission and SABER. The simulations have been performed at horizontal resolutions of ∼100 km. Generally a good agreement is seen between the results from the three dynamical cores, which verifies that the new dynamical core is working with WACCM.

非静水跨尺度预报模式-大气(MPAS-A)动力核心最近被调整用于指定化学全大气社区气候模式(SC-WACCM)。本研究将 SC-WACCM/MPAS-A 的平均带风和温度气候学结果与 SC-WACCM 使用有限体积和谱元动力核心的结果,以及高层大气研究卫星任务和 SABER 的带风和温度气候学结果进行了比较。模拟的水平分辨率为 100 千米。总体而言,三个动力核心的结果非常吻合,这验证了新的动力核心与 WACCM 的协同工作。
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引用次数: 0
RaFSIP: Parameterizing Ice Multiplication in Models Using a Machine Learning Approach RaFSIP:使用机器学习方法为模型中的冰乘法参数化
IF 6.8 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-06-14 DOI: 10.1029/2023MS003923
Paraskevi Georgakaki, Athanasios Nenes

Accurately representing mixed-phase clouds (MPCs) in global climate models (GCMs) is critical for capturing climate sensitivity and Arctic amplification. Secondary ice production (SIP), can significantly increase ice crystal number concentration (ICNC) in MPCs, affecting cloud properties and processes. Here, we introduce a machine-learning (ML) approach, called Random Forest SIP (RaFSIP), to parameterize SIP in stratiform MPCs. RaFSIP is trained on 16 grid points with 10-km horizontal spacing derived from a 2-year simulation with the Weather Research and Forecasting (WRF) model, including explicit SIP microphysics. Designed for a temperature range of 0 to −25°C, RaFSIP simplifies the description of rime splintering, ice-ice collisional break-up, and droplet-shattering using only a limited set of inputs. RaFSIP was evaluated offline before being integrated into WRF, demonstrating its stable online performance in a 1-year simulation keeping the same model setup as during training. Even when coupled with the 50-km grid spacing domain of WRF, RaFSIP reproduces ICNC predictions within a factor of 3 when compared to simulations with explicit SIP microphysics. The coupled WRF-RaFSIP scheme replicates regions of enhanced SIP and accurately maps ICNCs and liquid water content, particularly at temperatures above −10°C. Uncertainties in RaFSIP minimally impact surface cloud radiative forcing in the Arctic, resulting in radiative biases under 3 Wm−2 compared to simulations with detailed microphysics. Although the performance of RaFSIP in convective clouds remains untested, its adaptable nature allows for data set augmentation to address this aspect. This framework opens possibilities for GCM simplification and process description through physics-guided ML algorithms.

在全球气候模式(GCMs)中准确表示混合相云(MPCs)对于捕捉气候敏感性和北极放大效应至关重要。二次产冰(SIP)会显著增加混合相云中的冰晶数浓度(ICNC),从而影响云的属性和过程。在此,我们引入了一种名为随机森林 SIP(RaFSIP)的机器学习(ML)方法,用于对层状 MPC 中的 SIP 进行参数化。RaFSIP 在 16 个网格点上进行训练,网格点的水平间距为 10 公里,这些网格点来自天气研究与预报(WRF)模型的两年模拟,包括明确的 SIP 微物理。RaFSIP 的设计温度范围为 0 至 -25°C,仅使用有限的输入集简化了对冰渣劈裂、冰-冰碰撞破裂和水滴破碎的描述。RaFSIP 在集成到 WRF 之前进行了离线评估,在为期 1 年的模拟中证明了其稳定的在线性能,并保持了与训练时相同的模型设置。即使与 WRF 的 50 千米网格间距域耦合,RaFSIP 与显式 SIP 微物理模拟相比,也能在 3 倍范围内重现 ICNC 预测结果。WRF-RaFSIP 耦合方案复制了 SIP 增强区域,并精确绘制了 ICNC 和液态水含量图,尤其是在温度高于 -10°C 时。RaFSIP 的不确定性对北极地区表层云辐射强迫的影响很小,与详细微物理模拟相比,辐射偏差小于 3 Wm-2。尽管 RaFSIP 在对流云中的性能仍有待检验,但其适应性强的特点允许通过增加数据集来解决这方面的问题。该框架为通过物理引导的 ML 算法简化 GCM 和描述过程提供了可能性。
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引用次数: 0
期刊
Journal of Advances in Modeling Earth Systems
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