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Uncertainty Propagation From Radio Occultation Profiles to Aggregated Atmospheric Gridded Fields 从射电掩星剖面到聚集大气网格场的不确定性传播
IF 2.6 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2026-01-16 DOI: 10.1029/2025EA004389
S. Scher, F. Ladstädter, M. Schwärz, J. Innerkofler, G. Kirchengast

Radio occultation is a well-established remote sensing method that provides reliable estimates of atmospheric profiles of diverse variables, including temperature and pressure. However, as with all indirect methods, radio occultation has some inherent systematic and random error effects, which lead to observational uncertainties. While propagation of uncertainties along the processing chain for individual radio occultation profiles was described in recent studies, this uncertainty information has not yet been carried forward to climatological fields. We close this gap and present an uncertainty propagation procedure that provides uncertainty estimates for aggregated means for climate applications. Estimated random uncertainties, basic and apparent systematic uncertainties and sampling uncertainties (due to the discrete sampling by profiles) are propagated through the aggregation process, resulting in uncertainty estimates for gridded fields. We demonstrate the new procedure for two test months and representative variables, inspecting monthly mean profiles for refractivity, dry temperature and physical temperature measurements. Results show that estimated random uncertainties and residual sampling uncertainties (after sampling bias correction) have similar magnitudes, both decreasing with increasing spatial aggregation sizes and corresponding increasing number of aggregated observations. At small aggregation they are the main contributors to uncertainty in refractivity, and important contributors to uncertainty of temperature. Systematic uncertainty, whose magnitude is independent of the number of profiles, is for refractivity the main source of uncertainty for larger aggregation sizes, and for pressure and dry temperature at all commonly used aggregation sizes. All uncertainty components exhibit pronounced spatial variation over the globe, with polar regions showing the greatest uncertainty.

无线电掩星是一种完善的遥感方法,可提供各种变量(包括温度和压力)的大气剖面的可靠估计。然而,与所有间接方法一样,无线电掩星具有一些固有的系统和随机误差效应,从而导致观测的不确定性。虽然在最近的研究中描述了不确定性沿着单个无线电掩星剖面的处理链传播,但这种不确定性信息尚未被转移到气候领域。我们缩小了这一差距,并提出了一个不确定性传播程序,该程序为气候应用的汇总平均值提供了不确定性估计。估计的随机不确定性、基本的和明显的系统不确定性以及抽样不确定性(由于剖面的离散抽样)通过聚合过程传播,从而产生网格场的不确定性估计。我们演示了两个测试月的新程序和代表性变量,检查了折射率、干温度和物理温度测量的月平均剖面。结果表明,随机不确定性估计值和抽样偏差校正后的剩余抽样不确定性值具有相似的量级,均随着空间聚集尺度的增大和聚集观测数的增加而减小。在小聚集时,它们是造成折射率不确定度的主要因素,也是造成温度不确定度的重要因素。系统不确定度的大小与剖面的数量无关,对于折射率来说,系统不确定度是较大团聚体尺寸的不确定度的主要来源,对于所有常用团聚体尺寸的压力和干温度来说,系统不确定度也是不确定度的主要来源。所有不确定性分量在全球范围内都表现出明显的空间变化,其中极地地区的不确定性最大。
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引用次数: 0
Enhancing Active Channel Delineation in Alluvial Rivers Using Monthly Aggregation of Sentinel-2 Imagery 利用Sentinel-2影像月聚合增强冲积河流活动河道圈定
IF 2.6 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2026-01-14 DOI: 10.1029/2025EA004642
Elisa Bozzolan, Elisa Matteligh, Andrea Brenna, Martina Cecchetto, Nicola Surian, Patrice Carbonneau, Simone Bizzi

The active channel of alluvial rivers delineates areas of geomorphic activity over a defined time window. While increasing satellite data availability enables monthly active channel delineations, multi-year analyses often rely on temporal aggregates (e.g., annual medians) to reduce computational costs and intra-annual variability. The potential of monthly information to improve active channels delineation and geomorphic interpretation remains largely unexplored. In this work, we delineated active channels for the Po River (Italy) by aggregating monthly Sentinel-2 classifications of river water and sediment bars into annual frequency maps at 10 m resolution. Annual aggregation mitigated monthly sediment underestimation (12%) but also amplified model overestimation biases (15%). Monthly classification persistence (e.g., classified as active channel for more than N months/year) was then used to reduce these errors and produce active channel areas that closely match those manually delineated from 30 cm orthophotos. The spatiotemporal variability of monthly classifications also show that the active channel area of dynamic reaches can vary ∼50% over the year. These changes revealed areas most prone to water-stage fluctuations, sediment transport, as well as zones seasonally or progressively colonized by vegetation—patterns hidden in single orthophotos or annual medians. Less dynamic reaches, by contrast, showed minimal differences between annual and monthly-based delineation methods. These findings emphasize the importance of adapting temporal aggregation to the river type and process analysed, with sub-annual resolutions better capturing, in dynamic rivers, seasonal and progressive active channel reconfigurations, along with their interaction with sediment and vegetation dynamics.

冲积河流的活动河道在一定的时间窗口内划定了地貌活动区域。虽然越来越多的卫星数据可用性可以实现每月活动通道的描绘,但多年分析通常依赖于时间总量(例如,年中位数)来减少计算成本和年内变率。每月的信息潜力,以改善活动通道的划定和地貌解释仍在很大程度上未被探索。在这项工作中,我们通过将每月Sentinel-2分类的河水和沉积物汇总到10米分辨率的年度频率图中,描绘了波河(意大利)的活跃通道。年累积减轻了每月沉积物的低估(12%),但也放大了模型高估的偏差(15%)。然后使用每月分类持久性(例如,分类为活动通道超过N个月/年)来减少这些误差,并产生与从30厘米正射影像手动划定的活动通道区域密切匹配的活动通道区域。月分类的时空变异性也表明,动态河段的活跃通道面积在年内变化约50%。这些变化揭示了最容易发生水期波动、沉积物运输的地区,以及季节性或逐渐被植被模式覆盖的地区,这些模式隐藏在单张正射影像或年中位数中。相比之下,较少动态的河段在基于年和基于月的划定方法之间的差异很小。这些发现强调了使时间聚集适应所分析的河流类型和过程的重要性,在动态河流中,次年分辨率更好地捕获了季节性和渐进式活跃河道重构,以及它们与沉积物和植被动态的相互作用。
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引用次数: 0
Automatic Earthquake Declustering Using the Nearest-Neighbor Distance 使用最近邻距离的自动地震聚类
IF 2.6 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2026-01-14 DOI: 10.1029/2025EA004539
P. Bountzis, E. Lippiello, S. Baccari, G. Petrillo

In the widely adopted description of seismic occurrence, earthquakes are categorized as either background or triggered events. In this work, we present a fully automated, non-parametric algorithm for distinguishing between these two categories, a process known as seismic declustering, based on the widely used nearest-neighbor (NN) metric. We introduce a new measure, the susceptibility index, which identifies an optimal threshold to discriminate between background and triggered events within the NN metric. Through statistical testing on simulated epidemic type aftershock sequence catalogs, we demonstrate that our method yields classification metrics exceeding 90%, outperforming state-of-the art algorithms. Notably, we show that a single threshold is sufficient for reliable discrimination within a given data set. The identification of this threshold requires memory capacity and computational time that scale linearly and quadratically with the data set size, respectively, making the method particurarly suited for large earthquake catalogs. We also apply our method to the relocated Southern California catalog and the GeoNet catalog of New Zealand (NZ). Our method effectively adapts across the different tectonic settings, capturing the variability of background seismicity rates between the shallow crustal events of Southern California and the tectonically diverse seismicity of NZ.

在广泛采用的地震发生描述中,地震分为背景事件和触发事件。在这项工作中,我们提出了一种全自动的非参数算法,用于区分这两种类别,这一过程称为地震聚类,基于广泛使用的最近邻(NN)度量。我们引入了一种新的度量,即敏感性指数,它在神经网络度量中识别出区分背景事件和触发事件的最佳阈值。通过对模拟流行病型余震序列目录的统计测试,我们证明我们的方法产生的分类指标超过90%,优于最先进的算法。值得注意的是,我们表明,在给定的数据集内,单个阈值足以进行可靠的区分。这个阈值的识别需要内存容量和计算时间,它们分别与数据集大小成线性和二次比例,这使得该方法特别适合大型地震目录。我们还将我们的方法应用于重新定位的南加州目录和新西兰(NZ)的GeoNet目录。我们的方法有效地适应了不同的构造环境,捕捉了南加州浅层地壳事件和新西兰构造多样性地震活动之间背景地震活动率的变化。
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引用次数: 0
The THEMIS Control Network of Mars 忒弥斯火星控制网
IF 2.6 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2026-01-12 DOI: 10.1029/2025EA004758
R. L. Fergason, L. Weller, M. T. Bland

The accurate co-registration of geospatial data is necessary to answer questions that cross-cut disciplines and are key to understanding fundamental questions about our Solar System. To address this need and provide an updated product for Mars that is tied to a common reference frame, we have photogrammetrically controlled Thermal Emission Imaging System (THEMIS) daytime and nighttime infrared IR images. Using this improved image position knowledge, we generated orthorectified daytime and nighttime IR mosaics of Mars at 100 m per pixel for the ±65° latitude region of Mars. The updated spacecraft position and pointing information for the images is also released as SPICE kernels. The co-registration between individual THEMIS images achieves sub-pixel precision, and the average accuracy with which we know the position of any feature within the THEMIS controlled products is approximately 200 m horizontally. A globally controlled image set, with quantified accuracy and precision, is necessary to facilitate exploration and discovery for all bodies in the Solar System. Controlling THEMIS data allows multi-instrument science to be performed with significantly higher confidence as precise co-registration, and the accuracy knowledge of that registration, is necessary for analyses designed to extract information from the subtle differences between multiple images. A global image mosaic of Mars where uncertainties in the absolute image position are well characterized serves a wide range of purposes, including landing site evaluations, providing an accurate base to which high-resolution images (e.g., CTX and HiRISE) can be tied, and enables the fusion of multiple data types within a single framework.

地理空间数据的精确联合登记对于回答交叉学科的问题是必要的,也是理解太阳系基本问题的关键。为了满足这一需求,并为火星提供与共同参考框架相关联的更新产品,我们拥有摄影测量控制的热发射成像系统(THEMIS)白天和夜间红外图像。利用这种改进的图像位置知识,我们在火星±65°纬度地区以每像素100米的速度生成了正校正的火星白天和夜间红外马赛克。更新的航天器位置和指向图像的信息也作为SPICE内核发布。单个THEMIS图像之间的共同配准达到亚像素精度,我们知道THEMIS受控产品中任何特征位置的平均精度约为200米水平。一个全局控制的图像集,具有量化的准确度和精度,是促进探索和发现太阳系中所有天体所必需的。控制THEMIS数据可以使多仪器科学以更高的置信度进行,因为精确的共同配准以及该配准的准确性知识对于从多幅图像之间的细微差异中提取信息的分析是必要的。在火星的全球图像马赛克中,绝对图像位置的不确定性被很好地描述为广泛的目的,包括着陆点评估,为高分辨率图像(例如CTX和HiRISE)提供精确的基础,并使多种数据类型能够在单一框架内融合。
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引用次数: 0
SMAP Satellite Microwave Radiometry to Monitor River Flow and Lake Level in the Lower Mekong Basin SMAP卫星微波辐射法监测湄公河下游流域的河流流量和湖泊水位
IF 2.6 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2026-01-12 DOI: 10.1029/2025EA004436
A. Podkowa, S. V. Nghiem, Z. Kugler, G. R. Brakenridge

The NASA Soil Moisture Active Passive Mission (SMAP) satellite passive microwave radiometry (PMR) capability is demonstrated for measurements of river stage, river discharge, and lake level with in situ gauging data in the Lower Mekong Basin (LMB). Five river gauging locations with distinct characteristics in the Mekong River system and a location for the Tonle Sap Lake were selected. The SMAP PMR method was validated with forward-split, backward-split, and full-record approaches. Results from the three different validations were consistent and well compared with in situ gauging data at all the locations. Both the narrowest (42-m width, Songkhram River) and the widest river (1,735-m width, Mekong River) achieved high correlation values ≥0.9 and Nash-Sutcliffe Efficiencies >0.8. The SMAP PMR observations of rivers and lake captured seasonal and interannual patterns of river change corresponding to flood and drought conditions. The synergy of SMAP with satellite Ka-band PMR and Soil Moisture and Ocean Salinity (SMOS) data over multiple decades identified flood and drought events, and abrupt changes in river flows in the LMB corresponding to the operations of the two largest dams, Xiaowan and Nuozhadu, on the Lancang (upper Mekong) River. After these two dams went into operation, wet-season flow stage in the lower Mekong River did not again reach the 2.33-year flood stage, and dry-season water level dropped below the lowest stage recorded in the 2015 exceptional drought year. The PMR method enables river and lake monitoring with global coverage on a daily to nearly daily basis over decades.

NASA土壤湿度主动式被动任务(SMAP)卫星被动微波辐射测量(PMR)能力被用于测量湄公河下游流域(LMB)的河段、河流流量和湖泊水位。选择了湄公河水系中具有鲜明特征的五个河流测量点和洞里萨湖的一个位置。采用前向分割、后向分割和全记录方法对SMAP PMR方法进行了验证。三种不同验证的结果与所有位置的原位测量数据相比都是一致的。最窄的河流(42米宽的宋河)和最宽的河流(1735米宽的湄公河)的相关值均为≥0.9,Nash-Sutcliffe效率为0.8。SMAP对河流和湖泊的PMR观测捕获了与洪水和干旱条件相对应的河流变化的季节和年际模式。SMAP与卫星ka波段PMR和土壤水分和海洋盐度(SMOS)数据的协同作用,确定了澜沧江(湄公河上游)小湾和诺扎渡两座最大水坝运行时LMB的洪涝和干旱事件以及河流流量的突变。两座大坝投运后,湄公河下游汛期水位没有再达到2.33年的汛期水位,旱季水位也跌破了2015年异常干旱年的最低水位。PMR方法可以在几十年的时间里每天或几乎每天对全球范围内的河流和湖泊进行监测。
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引用次数: 0
Physics-Guided CNN-LSTM Model With Multi-Head Attention for Aerosol Optical Depth Prediction 气溶胶光学深度预测的多头关注物理引导CNN-LSTM模型
IF 2.6 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2026-01-07 DOI: 10.1029/2025EA004461
Liu Zeyang, Tan Yujun, Zhou Shengnan, Li Yarong, Zhang Jing, Yang Yadong, Shi Zhongrong, Zhou Xiancun

Accurate aerosol optical depth (AOD) prediction remains challenging due to complex aerosol-radiation interactions and highly variable spatio-temporal patterns. Three critical scientific issues motivate this work: understanding whether and how physical principles can enhance deep learning predictions, identifying which aerosol properties most strongly govern AOD variations, and improving the prediction of extreme AOD events critical for air quality management. Herein, utilizing MERRA-2 reanalysis data (1980–2024) over the Huaihe River Basin in eastern China, a Physics-Guided deep learning framework is presented for Aerosol Optical Depth (AOD) prediction. The model proposed integrates Convolutional Neural Networks (CNN), Long Short-TermMemory (LSTM) networks, and multi-head attention mechanisms to capture both spatio-temporal features and physical relationships of aerosol properties. Three key aspects are involved: First, a hybrid deep learning model is developed and evaluated, which combines CNNs for spatial correlation extraction, bidirectional LSTM for temporal dependency modeling, and multi-head attention for feature interaction learning. Second, a comprehensive feature importance analysis is conducted by examining the relationships between different aerosol properties (mass concentration, scattering coefficient, and Ångström exponent) and AOD prediction, offering physical insights into the model's decision-making process. Third, a specialized approach is proposed for extreme AOD event prediction, focusing on early detection and accurate forecasting of high-AOD episodes. Overall, the results demonstrate the model's efficacy in capturing both regular AOD variations and extreme events, with the Physics-Guided architecture showing superior performance compared to traditional methods. This integrated approach enhances AOD prediction accuracy and deepens insights into aerosol-radiation interactions, thereby improving atmospheric monitoring and air quality forecasting. While MERRA-2 has inherent temporal delays, this framework provides valuable capabilities for historical trend analysis, numerical model validation, and can be readily adapted for real-time applications through transfer learning with satellite observations.

由于复杂的气溶胶-辐射相互作用和高度可变的时空模式,准确的气溶胶光学深度(AOD)预测仍然具有挑战性。三个关键的科学问题激发了这项工作:了解物理原理是否以及如何增强深度学习预测,确定哪些气溶胶特性最强烈地控制AOD变化,以及改进对空气质量管理至关重要的极端AOD事件的预测。本文利用中国东部淮河流域MERRA-2再分析数据(1980-2024),提出了一个物理导向的气溶胶光学深度(AOD)预测深度学习框架。该模型集成了卷积神经网络(CNN)、长短期记忆(LSTM)网络和多头注意机制,以捕捉气溶胶特性的时空特征和物理关系。首先,开发并评估了一种混合深度学习模型,该模型将cnn用于空间相关性提取,双向LSTM用于时间依赖性建模,多头关注用于特征交互学习。其次,通过考察不同气溶胶特性(质量浓度、散射系数和Ångström指数)与AOD预测之间的关系,进行综合特征重要性分析,为模型决策过程提供物理见解。第三,提出了一种专门的极端AOD事件预测方法,重点关注高AOD事件的早期发现和准确预测。总体而言,结果证明了该模型在捕获常规AOD变化和极端事件方面的有效性,与传统方法相比,物理引导架构表现出更优越的性能。这种综合方法提高了AOD预测的准确性,加深了对气溶胶-辐射相互作用的认识,从而改善了大气监测和空气质量预测。虽然MERRA-2具有固有的时间延迟,但该框架为历史趋势分析、数值模型验证提供了有价值的能力,并且可以通过与卫星观测的迁移学习很容易地适应实时应用。
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引用次数: 0
Baseline Climatology of Gravity Waves From ∼30 to ∼70 km Established With Lidar Observations Over a Decade at McMurdo (77.84°S, 166.67°E), Antarctica: Implications for Vertical Wave Evolution 南极洲麦克默多(77.84°S, 166.67°E)近十年激光雷达观测建立的~ 30 ~ ~ 70 km重力波基线气气学:对垂直波演变的影响
IF 2.6 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2026-01-07 DOI: 10.1029/2025EA004435
Jackson Jandreau, Xinzhao Chu
<p>Lidar observations of atmospheric gravity waves (GWs) have been made spanning 14 years above McMurdo Station, Antarctica. Using these extensive observations and interleaved data processing techniques which enable bias-free/noise-floor-free estimation of GW parameters, this study forms seasonal baselines for GW potential energy densities (<span></span><math> <semantics> <mrow> <msub> <mi>E</mi> <mi>pm</mi> </msub> <mo>,</mo> <msub> <mi>E</mi> <mi>pv</mi> </msub> </mrow> <annotation> ${E}_{mathit{pm}},{E}_{mathit{pv}}$</annotation> </semantics></math>), ground-based frequency (<span></span><math> <semantics> <mrow> <mi>ω</mi> </mrow> <annotation> $omega $</annotation> </semantics></math>) spectrum, and vertical wavenumber (<span></span><math> <semantics> <mrow> <mi>m</mi> <mo>)</mo> </mrow> <annotation> $m)$</annotation> </semantics></math> spectrum in the stratosphere (30–50 km) and mesosphere (50–70 km). The stratospheric <span></span><math> <semantics> <mrow> <msub> <mi>E</mi> <mrow> <mi>p</mi> <mi>m</mi> </mrow> </msub> </mrow> <annotation> ${E}_{pm}$</annotation> </semantics></math> is dominated by an annual oscillation with a winter maximum. Spring/fall <span></span><math> <semantics> <mrow> <msub> <mi>E</mi> <mrow> <mi>p</mi> <mi>m</mi> </mrow> </msub> </mrow> <annotation> ${E}_{pm}$</annotation> </semantics></math> profiles show decreased GW dissipation/breaking in 46–56 km. The wintertime <span></span><math> <semantics> <mrow> <msub> <mi>E</mi> <mrow> <mi>p</mi> <mi>m</mi> </mrow> </msub> </mrow> <annotation> ${E}_{pm}$</annotation> </semantics></math> profile shows two bending points, where the GW scale height steepens above 39 km and steepens further above 50 km. These bending points are
在南极洲麦克默多站上空进行了长达14年的大气重力波(GWs)激光雷达观测。利用这些广泛的观测和交错数据处理技术,本研究形成了GW势能密度的季节性基线(E pm,E pv ${E}_{mathit{pm}},{E}_{mathit{pv}}$),地面频率(ω $omega $)频谱,平流层(30 ~ 50 km)和中间层(50 ~ 70 km)垂直波数(m) $m)$谱。平流层的E p m ${E}_{pm}$主要是一个有冬季最大值的年振荡。春季/秋季E p m ${E}_{pm}$剖面显示46-56 km的GW耗散/断裂减少。冬季E p m ${E}_{pm}$剖面显示两个弯曲点,其中GW比例尺高度在39 km以上变陡,在50 km以上进一步变陡。这些弯曲点与尺度有关,其中λ z ${lambda }_{z}$ = 2-8 km的剖面仅在39 km处弯曲,λ z ${lambda }_{z}$ = 8-30 km的型材仅在50 km处弯曲。GW m $m$ - 30 ~ 50 km的光谱与50 ~ 70 km的光谱相似$m$ -高m $m$的光谱,但在低m的光谱不同M $m$,而频率ω $omega $ -频谱在所有ω $omega $上均匀增长。光谱观测是在线性不稳定性、饱和级联和扩散滤波理论的背景下进行的,但确切的机制还有待确定。这些弯曲点和光谱趋势表明高度范围一致,GW耗散增强。我们认为这种耗散可能是中层大气中次生GWs产生的一个潜在来源,但光雷达数据本身并不能证实这一点,值得进一步研究。
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引用次数: 0
Spaceborne Canopy Height Products Should Be Complemented With Airborne Laser Scanning Data: Toward a European Canopy Height Model 星载冠层高度产品应与机载激光扫描数据相补充:朝向欧洲冠层高度模型
IF 2.6 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2026-01-07 DOI: 10.1029/2025EA004544
Vítězslav Moudrý, Ruben Remelgado, Matthias Forkel, Michele Torresani, Gaia Vaglio Laurin, Eliška Šárovcová, Virginia E. Garcia Millan, Fabian Jörg Fischer, Tommaso Jucker, Michal Gallay, Patrick Kacic, Christopher R. Hakkenberg, Žiga Kokalj, Krzysztof Stereńczak, Yousef Erfanifard, Duccio Rocchini, Jiří Prošek, Stephanie Roilo, Kateřina Gdulová, Anna F. Cord, Michela Perrone, Juan Alberto Molina-Valero, Jiří Šmída, Peter Surový, Zlatica Melichová, Marco Malavasi, Rudolf Urban, Martin Štroner, Dominik Seidel, Szilárd Szabó, László Bertalan, Anette Eltner, Roberto Cazzolla Gatti, Ján Kaňuk, Vojtěch Barták, Daniel Franke, Benjamin Brede, Qian Song, Mikhail Urbazaev, W. Daniel Kissling

Measuring and mapping vegetation structure is essential for understanding the functioning of terrestrial ecosystems and for informing environmental policies. Recent years have seen a growing demand for high-resolution data on vegetation structure, driving their prediction at fine resolutions (1–30 m) at state, continental, and global spatial extents by combining satellite data with machine learning. As these initiatives expand, it is crucial to actively discuss the quality and usability of these products. Here, we briefly summarize current efforts to map vegetation structure and show that continental-to-global canopy height models (CHMs) exhibit significant errors in canopy heights compared to national airborne laser scanning (ALS) data. We recommend that regions with abundant ALS data, such as Europe, prioritize using ALS-based canopy height metrics rather than relying on less accurate predictions from satellite products. Despite variations in ALS data characteristics, such as temporal inconsistencies and differences in acquisition characteristics and classification accuracy, the generation of spatially contiguous canopy height products in raster format at fine spatial resolution is necessary and feasible. This requires coordinating efforts for data and survey harmonization, developing standardized processing pipelines and continent-wide ALS products, and ensuring free access for research and environmental policy. We show that ALS data now cover most of Europe, with newer surveys achieving higher point densities, improving their suitability for vegetation mapping. Beyond numerous applications in forestry, ecology, and conservation, such data sets are crucial for calibrating future Earth Observation missions, making them essential for producing reliable and accurate global, fine-resolution vegetation structure data.

测量和绘制植被结构对于了解陆地生态系统的功能和为环境政策提供信息至关重要。近年来,人们对高分辨率植被结构数据的需求不断增长,通过将卫星数据与机器学习相结合,推动了在国家、大陆和全球空间范围内以精细分辨率(1-30米)进行预测。随着这些计划的扩展,积极讨论这些产品的质量和可用性是至关重要的。在此,我们简要总结了目前在绘制植被结构方面的努力,并表明与国家机载激光扫描(ALS)数据相比,大陆到全球的冠层高度模型(CHMs)在冠层高度方面存在显著误差。我们建议拥有丰富ALS数据的地区,如欧洲,优先使用基于ALS的冠层高度指标,而不是依赖卫星产品的不太准确的预测。尽管ALS数据特征存在时间不一致性、采集特征和分类精度等差异,但在精细空间分辨率下以栅格格式生成空间连续的冠层高度产品是必要和可行的。这需要协调数据和调查的统一,开发标准化的处理管道和遍及整个大陆的ALS产品,并确保研究和环境政策的自由获取。我们发现ALS数据现在覆盖了欧洲大部分地区,更新的调查获得了更高的点密度,提高了它们对植被测绘的适用性。除了在林业、生态和保护领域的众多应用之外,这些数据集对于校准未来的地球观测任务至关重要,对于生成可靠、准确的全球精细植被结构数据至关重要。
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引用次数: 0
A Case Study of One Local Severe Convection Process Caused by Meso-β-Scale Vortex in a Forming Southwest China Vortex in Spring With Large Eddy Simulation 春季西南涡旋形成过程中中尺度涡引起的一次局地强对流过程的大涡模拟
IF 2.6 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2026-01-03 DOI: 10.1029/2025EA004514
Xiaolong Cheng, Hui Luo, Yueqing Li

The fifth generation of ECMWF atmospheric reanalyses data (ERA5), operational observed data, S-band radar data and Large Eddy Simulation (LES) tool were employed to investigate the evolution of local small-scale convection in Ziyang City of Sichuan Province on 11 April 2022 in spring. The meso-β-scale vortex and 700-hPa wind shear in the Sichuan Basin horizontally merged and formed the Southwest China vortex. The local convection induced heavy rainfall, hail and thunderstorm in the northeast of the organizing meso-β-scale vortex. The well-developed meso-β-scale vortex became the center of Southwest China vortex. The horizontal scale and time scale of the meso-β-vortex were 20–50 km and 2–3 hr, respectively. The newly formed convections over the northeast of the meso-β-scale vortex developed in the middle troposphere and quickly separated from the main body of the meso-β-scale vortex with the guided airflow. The convective organization at the northeastern forepart of the meso-β-scale vortex was reproduced in LES results. The strong convection and meso-β-scale vortex were basically activated in the same period. The significant isobaric surfaces for strong convection formation were from 750 to 500 hPa. And cold air in the middle and lower troposphere rarely affected the convective process. Local convections were mainly triggered by strong vertically meridional wind shear.

利用ECMWF第五代大气再分析资料(ERA5)、实际观测资料、s波段雷达资料和大涡模拟(LES)工具,对2022年4月11日四川资阳市春季局地小尺度对流演变进行了研究。四川盆地中尺度涡与700 hpa风切变水平合并形成西南涡。在组织的中β尺度涡旋东北部,局地对流诱发了强降雨、冰雹和雷暴。发育良好的中β尺度涡成为西南涡旋的中心。中尺度β涡水平尺度为20 ~ 50 km,时间尺度为2 ~ 3 hr。中β尺度涡旋东北方向新形成的对流在对流层中部发展,在气流引导下迅速与中β尺度涡旋主体分离。中β尺度涡旋东北前部的对流组织在LES结果中得到了再现。强对流和中β尺度涡旋基本在同一时期激活。750 ~ 500 hPa是形成强对流的重要等压面。对流层中下层冷空气对对流过程影响较小。局地对流主要由强垂直经向风切变触发。
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引用次数: 0
Effect of Land Cover Type on 3D Deformation Recovery From Synthetically Deformed High Resolution Satellite Optical Imagery 地表覆盖类型对综合变形高分辨率卫星光学影像三维变形恢复的影响
IF 2.6 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2025-12-31 DOI: 10.1029/2025EA004477
C. Hanagan, S. B. DeLong, N. G. Reitman

The limits of detection for earthquake surface deformation in the spatial domain have improved with advances in remote sensing imagery data availability, resolution, and analysis. Sub-pixel correlation and digital elevation model (DEM) differencing from sub-meter, earthquake-spanning satellite optical imagery has enhanced surface rupture mapping and deformation measurements. However, knowledge of measurement accuracy and uncertainty is limited. To address this, we construct orthophotos and digital elevation models (DEMs) from repeat high resolution (∼0.5 m) satellite optical imagery along two sections of the Garlock fault, California with clear fault geomorphology and differing land cover. We deform later sets of DEMs and images with synthetic earthquakes containing both diffuse and discrete horizontal and vertical displacements. Sub-pixel image correlation and DEM differencing demonstrate how vegetation degrades recovered displacement accuracy. In barren land cover, horizontal displacements are detectable to an expected ∼1/10th-pixel size. With shrubs, trees, and grass, detectable displacements increase to >1/2-pixel size, and filtering results by correlation score and using elevation values as input rather than image values improves accuracy. Vertical displacement detection thresholds remain lower in vegetation, at >1-pixel size. Higher slope angles degrade displacement recovery, worsened by vegetation. Diminishing seasonal separation improves accuracy over vegetated regions, though not to the level achieved in barren environments. These results will inform research and operational efforts on the utility of high resolution satellite optical imagery for detecting deformation in varied land cover. Furthermore, they reveal where alternative measurements, such as from LiDAR or radar interferometry, are required to mitigate the effects of vegetation and capture fine-scale crustal deformation.

随着遥感图像数据的可用性、分辨率和分析的进步,地震地表变形在空间域的检测极限得到了改善。亚像元相关和数字高程模型(DEM)与亚米、地震跨越卫星光学图像的差异增强了地表破裂制图和变形测量。然而,测量精度和不确定度的知识是有限的。为了解决这个问题,我们沿着加利福尼亚Garlock断层的两个部分构建了重复高分辨率(~ 0.5 m)卫星光学图像的正像图和数字高程模型(dem),这些断层具有清晰的断层地貌和不同的土地覆盖。我们用包含弥漫性和离散的水平和垂直位移的合成地震对后来的dem和图像进行变形。亚像素图像相关和DEM差异表明植被是如何降低恢复位移精度的。在贫瘠的土地覆盖中,水平位移可检测到预期的1/10像素大小。对于灌木、树木和草,可检测的位移增加到1/2像素大小,通过相关性评分过滤结果并使用高程值而不是图像值作为输入,可以提高精度。植被的垂直位移检测阈值仍然较低,为1像素大小。坡度越大,驱替恢复就越差,植被的影响更大。减少季节间隔提高了植被地区的精度,尽管没有达到在贫瘠环境中达到的水平。这些结果将为利用高分辨率卫星光学图像探测不同土地覆盖的变形提供研究和业务方面的信息。此外,它们还揭示了在哪些地方需要激光雷达或雷达干涉测量等替代测量方法来减轻植被的影响,并捕获精细尺度的地壳变形。
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