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Prospects of Predicting the Polar Motion Based on the Results of the Second Earth Orientation Parameters Prediction Comparison Campaign 根据第二次地球方位参数预测对比活动的结果预测极地运动的前景
IF 2.9 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-11-05 DOI: 10.1029/2023EA003278
Tomasz Kur, Justyna Śliwińska-Bronowicz, Malgorzata Wińska, Henryk Dobslaw, Jolanta Nastula, Aleksander Partyka, Santiago Belda, Christian Bizouard, Dale Boggs, Sara Bruni, Lue Chen, Mike Chin, Sujata Dhar, Robert Dill, PengShuo Duan, Jose M. Ferrandiz, Junyang Gou, Richard Gross, Sonia Guessoum, Songtao Han, Robert Heinkelmann, ChengLi Huang, Christopher Irrgang, Jacek Kudrys, Jia Li, Marcin Ligas, Lintao Liu, Weitao Lu, Volker Mayer, Wei Miao, Maciej Michalczak, Sadegh Modiri, Michiel Otten, Todd Ratcliff, Shrishail Raut, Jan Saynisch-Wagner, Matthias Schartner, Erik Schoenemann, Harald Schuh, M. Kiani Shahvandi, Benedikt Soja, Xiaoqing Su, Daniela Thaller, Maik Thomas, Guocheng Wang, Yuanwei Wu, CanCan Xu, Xueqing Xu, Xinyu Yang, Xin Zhao, Zhijin Zhou

Growing interest in Earth Orientation Parameters (EOP) resulted in various approaches to the EOP prediction algorithms, as well as in the exploitation of distinct input data, including the observed EOP values from various operational data centers and modeled effective angular momentum functions. Considering these developments and recently emerged new methodologies, the Second Earth Orientation Parameters Prediction Comparison Campaign (2nd EOP PCC) was pursued in 2021–2022. The campaign was led by Centrum Badań Kosmicznych Polskiej Akademii Nauk in cooperation with Deutsches GeoForschungsZentrum and under the auspices of the International Earth Rotation and Reference Systems Service. This paper provides the analysis and evaluation of the polar motion predictions submitted during the 2nd EOP PCC with the prediction horizons between 10 and 30 days. Our analysis shows that predictions are highly reliable with only a few occasional discrepancies identified in the submitted files. We demonstrate the accuracy of EOP predictions by (a) calculating the mean absolute error relative to polar motion observations from September 2021 through December 2022 and (b) assessing the stability of the predictions in time. The analysis shows unequal results for the x and y components of polar motion (PMx and PMy, respectively). Predictions of PMy are usually more accurate and have a smaller spread across all submitted files when compared to PMx. We present an analysis of similarity between the participants to indicate what methods and input data give comparable output. We also prepared the ranking of prediction methods for polar motion summarizing the achievements of the campaign.

人们对地球方位参数(EOP)的兴趣与日俱增,从而产生了各种地球方位参数预测算法方法,以及对不同输入数据的利用,包括来自不同运行数据中心的观测到的地球方位参数值和建模的有效角动量函数。考虑到这些发展和最近出现的新方法,2021-2022 年开展了第二次地球定向参数预测比较活动(第二次 EOP PCC)。该活动由波兰国家科学院巴丹-科斯米契尼奇中心(Centrum Badań Kosmicznych Polskiej Akademii Nauk)牵头,与德国地球研究中心(Deutsches GeoForschungsZentrum)合作,并由国际地球自转和参考系统服务组织(International Earth Rotation and Reference Systems Service)赞助。本文对第二届 EOP PCC 期间提交的极地运动预测进行了分析和评估,预测范围为 10 至 30 天。我们的分析表明,预测结果非常可靠,在提交的文件中仅偶尔发现了一些差异。我们通过(a)计算与 2021 年 9 月至 2022 年 12 月极地运动观测数据相对的平均绝对误差,以及(b)评估预测结果在时间上的稳定性,来证明 EOP 预测的准确性。分析表明,极地运动 x 和 y 分量(分别为 PMx 和 PMy)的结果并不相同。与 PMx 相比,PMy 的预测通常更准确,在所有提交的文件中的分布也更小。我们对参赛者之间的相似性进行了分析,以说明哪些方法和输入数据可提供相似的输出结果。我们还准备了极地运动预测方法的排名,以总结此次活动的成果。
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引用次数: 0
Empirical Model of SSUSI-Derived Auroral Ionization Rates SSUSI 得出的极光电离率的经验模型
IF 2.9 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-11-03 DOI: 10.1029/2024EA003578
Stefan Bender, Patrick J. Espy, Larry J. Paxton

We present an empirical model for auroral (90–150 km) electron–ion pair production rates, ionization rates for short, derived from Special Sensor Ultraviolet Spectrographic Imager electron energy and flux data. Using the Fang et al. (2010, https://doi.org/10.1029/2010gl045406) parametrization for mono-energetic electrons, and the NRLMSISE-00 neutral atmosphere model (Picone et al., 2002, https://doi.org/10.1029/2002ja009430), the calculated ionization rate profiles are binned in 2-hr magnetic local time and 3.6°geomagnetic latitude to yield time series of ionization rates at 5-km altitude steps. We fit each of these time series to the geomagnetic indices Kp, PC, and Ap, the 81-day averaged solar F10.7 ${mathrm{F}}_{10.7}$ radio flux index, and a constant term. The resulting empirical model can easily be incorporated into coupled chemistry–climate models to include particle precipitation effects.

我们提出了一个极光(90-150 公里)电子-离子对产生率(简称电离率)的经验模型,该模型由特殊传感器紫外线分光成像仪的电子能量和通量数据得出。利用 Fang 等人(2010 年,https://doi.org/10.1029/2010gl045406)的单能量电子参数化和 NRLMSISE-00 中性大气模型(Picone 等人,2002 年,https://doi.org/10.1029/2002ja009430),将计算出的电离率剖面按 2 小时磁当地时间和 3.6°地磁纬度进行分档,得出 5 公里高度的电离率时间序列。我们将这些时间序列分别与地磁指数 Kp、PC 和 Ap、81 天平均太阳 F 10.7 ${mathrm{F}}_{10.7}$ 无线电通量指数以及一个常数项进行拟合。由此产生的经验模型可以很容易地纳入化学-气候耦合模型,以包括粒子沉降效应。
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引用次数: 0
Low-Frequency Reconstruction for Full Waveform Inversion by Unsupervised Learning 通过无监督学习实现全波形反演的低频重构
IF 2.9 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-11-03 DOI: 10.1029/2024EA003565
Ningcheng Ciu, Tao Lei, Wei Zhang

Obtaining reliable low-frequency seismic data is crucial for effectively reducing cycle-skipping in full waveform inversion. However, acquiring high signal-to-noise ratio low-frequency information from field data remains a challenge. An effective solution to mitigate cycle-skipping is to utilize low-frequency information synthesized by neural networks to obtain low-wavenumber initial models. Previous attempts to reconstruct synthetic low-frequency data using supervised learning methods have shown feasibility but were limited to training with synthetic data that required labeled information. In this study, we employed an unsupervised learning method, namely cycle-consistent adversarial networks (CycleGAN), to reconstruct large-scale-feature related low-frequency information based on the high-frequency input data. Unlike supervised learning, CycleGAN allows the use of field data as input to train the network, which is more closely aligned with practical applications. Nevertheless, this approach presents challenges in terms of training complexity and potential output stability. To overcome these challenges, we reconstructed an appropriate target data set that combines high, medium, and low-frequency components and incorporated additional loss functions to enhance the network's output performance. We conducted quantitative evaluations of the method's sensitivity to the target data set and its ability to handle low-quality input data through numerical testing. The final results from field data testing confirmed the feasibility and effectiveness of the proposed method.

获取可靠的低频地震数据对于有效减少全波形反演中的周期跳跃至关重要。然而,从野外数据中获取高信噪比的低频信息仍是一项挑战。减少周期跳跃的有效解决方案是利用神经网络合成的低频信息来获取低波数初始模型。之前使用监督学习方法重建合成低频数据的尝试已显示出可行性,但仅限于使用需要标记信息的合成数据进行训练。在这项研究中,我们采用了一种无监督学习方法,即循环一致性对抗网络(CycleGAN),来根据高频输入数据重建与大尺度特征相关的低频信息。与监督学习不同,CycleGAN 允许使用现场数据作为训练网络的输入,这与实际应用更为贴近。不过,这种方法在训练复杂性和潜在输出稳定性方面存在挑战。为了克服这些挑战,我们重建了一个适当的目标数据集,将高、中、低频成分结合在一起,并加入了额外的损失函数,以提高网络的输出性能。我们通过数值测试对该方法对目标数据集的灵敏度及其处理低质量输入数据的能力进行了定量评估。实地数据测试的最终结果证实了建议方法的可行性和有效性。
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引用次数: 0
Reconstruction of Nearshore Surface Gravity Wave Heights From Distributed Acoustic Sensing Data 根据分布式声学传感数据重建近岸表面重力波高度
IF 2.9 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-11-01 DOI: 10.1029/2024EA003589
Samuel Meulé, Julián Pelaez-Quiñones, Frédéric Bouchette, Anthony Sladen, Aurélien Ponte, Annika Maier, Itzhak Lior, Paschal Coyle

Distributed Acoustic Sensing (DAS) is a photonics technology converting seafloor telecommunications and optical fiber cables into dense arrays of strain sensors, allowing to monitor various oceanic physical processes. Yet, several applications are hindered by the limited knowledge of the transfer function between geophysical variables and DAS measurements. This study investigates the quantitative relationship between surface gravity DAS-recorded wave-generated strain signals along the seafloor and the pressure at a colocated sensor. A remarkable linear correlation is found over various sea conditions allowing us to reliably determine significant wave heights from DAS data. Utilizing linear wave potential theory, we derive an analytical transfer function linking cable deformation and wave kinematic parameters. This transfer function provides a first quantification of the effects related to surface gravity waves and fiber responses. Our results validate DAS's potential for real-time reconstruction of the surface gravity wave spectrum over extended coastal areas. It also enables the estimation of waves hydraulic parameters at depth without the need from offshore deployments.

分布式声学传感(DAS)是一种将海底电信和光纤电缆转换成密集应变传感器阵列的光子学技术,可用于监测各种海洋物理过程。然而,由于对地球物理变量与 DAS 测量之间传递函数的了解有限,一些应用受到了阻碍。本研究调查了沿海底的表面重力 DAS 记录波产生的应变信号与同位传感器压力之间的定量关系。在各种海况下都发现了明显的线性相关关系,使我们能够根据 DAS 数据可靠地确定显著波高。利用线性波势理论,我们推导出了连接电缆变形和波浪运动学参数的分析传递函数。该传递函数首次量化了与表面重力波和光纤响应相关的影响。我们的研究结果验证了 DAS 在实时重建沿海大范围表面重力波谱方面的潜力。它还可以估算波浪深度的水力参数,而无需进行海上部署。
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引用次数: 0
The Self-Calibrating Tilt Accelerometer: A Method for Observing Tilt and Correcting Drift With a Triaxial Accelerometer 自校准倾斜加速度计:使用三轴加速度计观测倾斜和校正漂移的方法
IF 2.9 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-10-31 DOI: 10.1029/2024EA003909
E. K. Fredrickson, W. S. D. Wilcock, M. J. Harrington, G. Cram, J. Tilley, D. Martin, J. Burnett

We present observations from two field deployments of a calibrated tiltmeter that we name the Self-Calibrating Tilt Accelerometer (SCTA). The tiltmeter is based upon a triaxial quartz crystal accelerometer; the horizontal channels measure tilt and are periodically rotated into the vertical to obtain a measurement of the acceleration of gravity. Changes in the measured total acceleration are ascribed to drift in the vertical channel and used as calibrations for removing that same drift from the tilt time series observed between calibrations. Changes in the span (sensitivity) of the accelerometer channels can also be measured by calibrating them pointing up and down. A 3-year test on the seafloor at Axial Seamount show that the calibrations are consistent with a linear-exponential model of drift to a RMS residual of ∼0.5 μg (μrad). The calibrated tilt time series was impacted by platform settling for the first 2 years, but after repositioning the tiltmeter, the calibrated observations were consistent for the final year with the tilt observed on a nearby LILY tiltmeter, within an assumed level of drift for the unconstrained LILY sensor. A separate 15-month test in a stable vault at Piñon Flat Observatory was complicated by seasonal temperature variations of >5°C; the calibrations are consistent with a linear-exponential model of drift to ∼2 μg RMS when temperature and temperature time-derivative dependence is included. Similarly, the calibrated tilt time series was impacted by thermal deformation of the SCTA assembly. A future test in a thermally and tectonically stable borehole will be required to assess the accuracy of the SCTA.

我们介绍了两次实地部署校准倾斜仪的观测结果,并将其命名为自校准倾斜加速度计(SCTA)。倾角仪以三轴石英晶体加速度计为基础;水平通道测量倾角,并定期旋转到垂直方向,以获得重力加速度的测量值。测得的总加速度的变化归因于垂直通道的漂移,并用作校准,以从校准之间观测到的倾斜时间序列中去除相同的漂移。加速度计通道跨度(灵敏度)的变化也可以通过上下校准来测量。在轴向海山海底进行的为期 3 年的测试表明,校准与漂移的线性-指数模型一致,均方根残差为 ∼ 0.5 μg(μrad)。校准后的倾角时间序列在头两年受到平台沉降的影响,但在重新定位倾角仪后,最后一年的校准观测结果与在附近的 LILY 倾角仪上观测到的倾角一致,在无约束 LILY 传感器的假定漂移水平范围内。在皮农平原天文台的稳定拱顶中进行的为期 15 个月的单独测试因 5°C 的季节性温度变化而变得复杂;如果将温度和温度时间衍生物依赖性包括在内,校准结果与漂移至 ∼2 μg RMS 的线性-指数模型一致。同样,校准的倾斜时间序列也受到 SCTA 组件热变形的影响。今后需要在热和构造稳定的钻孔中进行测试,以评估 SCTA 的准确性。
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引用次数: 0
A Rare Tropical Cyclone Associated With Southwest Monsoon Over the Northern Part of the South China Sea—Tropical Storm Maliksi 南海北部与西南季风有关的罕见热带气旋--热带风暴马立克斯
IF 2.9 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-10-30 DOI: 10.1029/2024EA003826
J. Y. He, P. W. Chan, C. W. Choy, P. Cheung, C. C. Lam, Y. H. He, C. K. Pan, K. K. Lai, H. Su, E. Z. Zhang, C. J. Sun, C. J. Huang

This study examines the characteristics and development of Tropical Storm Maliksi, which is a special case of tropical cyclone developed in the northwestern part of the South China Sea during a southwest monsoon outbreak. Detailed analyses were conducted using observational data and forecast products. Surface observations, radar wind profilers, aircraft data, and satellite products were used to evaluate Maliksi's wind structure, revealing multiple circulation centers and gale force winds. Vertical wind profiles, warm core structure, wind waves, and the influence of sea temperatures and salinity on Maliksi's intensification were investigated. Regarding forecasting, AI-based models outperformed conventional numerical weather prediction (NWP) models in predicting Maliksi's initial development, though both struggled to capture the persistence of strong winds as the system moved inland. High-resolution NWP simulations were employed to examine terrain-induced wind variability around Hong Kong International Airport, revealing the mountain wake effect and uneven wind and turbulence distribution. These findings provide insights into the challenges of forecasting and monitoring such tropical cyclones, and highlight the need for enhanced observational platforms and forecasting tools along coastlines vulnerable to these systems.

本研究探讨了热带风暴 "马立克斯 "的特征和发展情况。"马立克斯 "是西南季风爆发期间在南海西北部形成的一个热带气旋特例。研究利用观测数据和预报产品进行了详细分析。地面观测、雷达风廓线、飞机数据和卫星产品被用来评估 "马利克西 "的风结构,揭示了多个环流中心和大风。研究了垂直风廓线、暖核心结构、风浪以及海温和盐度对 "马利克西 "加强的影响。在预报方面,基于人工智能的模式在预测 "马利克西 "的初期发展方面优于传统的数值天气预报(NWP)模式,但两者都难以捕捉系统向内陆移动时强风的持续性。高分辨率的 NWP 模拟被用来研究香港国际机场周围由地形引起的风的变化,揭示了山区尾流效应以及风和湍流的不均匀分布。这些发现为预报和监测此类热带气旋所面临的挑战提供了启示,并强调了在易受此类系统影响的海岸线加强观测平台和预报工具的必要性。
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引用次数: 0
Improving Interpolating Accuracy of Weighted Mean Temperature by Using a Novel Lapse Rate Model in Compact VMF1 Product 在紧凑型 VMF1 产品中使用新的降温速率模型提高加权平均气温的插值精度
IF 2.9 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-10-30 DOI: 10.1029/2024EA003702
Peng Sun, Kefei Zhang, Dantong Zhu, Moufeng Wan, Ren Wang, Suqin Wu

In GNSS (Global Navigation Satellite Systems) meteorology, the accuracy of precipitable water vapor (PWV) retrieved from the tropospheric delay of GNSS signals is affected by the conversion factor. Compact VMF1 product (known as GGOS Atmosphere data) provides high-accuracy global grid-wise weighted mean temperature (Tm) values, which can be utilized to calculate the conversion factor. However, the Tm provided in the compact VMF1 data are solely ground surface values. To enhance the performance of compact VMF1 product, a new Tm lapse rate model for each grid point was developed for the purpose of reducing its surface Tm to the elevation of the GNSS site. Then the reduced Tm values over the neighboring grid points together with horizontal interpolation were used to obtain the interpolated Tm for the GNSS station. The sample data for the development of the new model were the Tm profiles obtained from ERA5 monthly averaged data spanning 2009–2018. To assess the model's performance, global radiosonde data at 504 radiosonde stations spanning 2019–2021 were employed. Results demonstrated that implementing the Tm lapse rate model significantly enhanced the accuracy of interpolating Tm values for GNSS stations with substantial height disparities from adjacent grid points, thereby improving PWV conversion accuracy. This indicates that employing the new Tm lapse rate model to adjust surface Tm data in the compact VMF1 product holds promise for enhancing its utility in GNSS meteorology.

在全球导航卫星系统(GNSS)气象学中,从全球导航卫星系统信号的对流层延迟中获取的可降水水汽(PWV)的准确性受到转换系数的影响。紧凑型 VMF1 产品(即全球全球观测系统大气数据)提供了高精度的全球网格加权平均温度(Tm)值,可用于计算转换系数。不过,紧凑型 VMF1 数据中提供的 Tm 值仅为地表值。为了提高紧凑型 VMF1 产品的性能,为每个网格点开发了一个新的 Tm 失效率模型,目的是将其地表 Tm 降低到全球导航卫星系统站点的海拔高度。然后,利用邻近网格点上的减小 Tm 值和水平插值法,获得全球导航卫星系统站点的插值 Tm。开发新模型的样本数据是从 2009-2018 年ERA5 月平均数据中获得的热量曲线。为评估该模型的性能,采用了 504 个无线电探空仪站的全球无线电探空仪数据,时间跨度为 2019-2021 年。结果表明,对于与相邻网格点高度差异较大的全球导航卫星系统站点,采用Tm失效率模型显著提高了Tm值的内插精度,从而提高了PWV转换精度。这表明,在紧凑型 VMF1 产品中采用新的 Tm 失效率模型来调整地表 Tm 数据,有望提高其在全球导航卫星系统气象学中的实用性。
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引用次数: 0
A Scalable, Cloud-Based Workflow for Spectrally-Attributed ICESat-2 Bathymetry With Application to Benthic Habitat Mapping Using Deep Learning 利用深度学习绘制底栖生物栖息地地图的可扩展、基于云的 ICESat-2 分光测深工作流程
IF 2.9 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-10-29 DOI: 10.1029/2024EA003735
Forrest Corcoran, Christopher E. Parrish, Lori A. Magruder, J. P. Swinski

Since the 2018 launch of NASA's ICESat-2 satellite, numerous studies have documented the bathymetric measurement capabilities of the space-based laser altimeter. However, a commonly identified limitation of ICESat-2 bathymetric point clouds is that they lack accompanying spectral reflectance attributes, or even intensity values, which have been found useful for benthic habitat mapping with airborne bathymetric lidar. We present a novel method for extracting bathymetry from ICESat-2 data and automatically adding spectral reflectance values from Sentinel-2 imagery to each detected bathymetric point. This method, which leverages the cloud computing systems Google Earth Engine and NASA's SlideRule Earth, is ideally suited for “big data” projects with ICESat-2 data products. To demonstrate the scalability of our workflow, we collected 3,500 ICESat-2 segments containing approximately 1.4 million spectrally-attributed bathymetric points. We then used this data set to facilitate training of a deep recurrent neural network for classifying benthic habitats at the ICESat-2 photon level. We trained two identical models, one with and one without the spectral attributes, to investigate the benefits of fusing ICESat-2 photons with Sentinel-2. The results show an improvement in model performance of 18 percentage points, based on F1 score. The procedures and source code are publicly available and will enhance the value of the new ICESat-2 bathymetry data product, ATL24, which is scheduled for release in Fall 2024. These procedures may also be applicable to data from NASA's upcoming CASALS mission.

自 2018 年美国国家航空航天局发射 ICESat-2 卫星以来,许多研究都记录了天基激光测高仪的测深能力。然而,ICESat-2测深点云普遍存在的一个局限性是缺乏相应的光谱反射属性,甚至缺乏强度值,而这些属性对于利用机载测深激光雷达绘制底栖生物栖息地图非常有用。我们提出了一种从 ICESat-2 数据中提取测深数据的新方法,并自动将 Sentinel-2 图像中的光谱反射率值添加到每个检测到的测深点上。该方法利用了云计算系统谷歌地球引擎和美国国家航空航天局的 SlideRule Earth,非常适合使用 ICESat-2 数据产品的 "大数据 "项目。为了证明我们工作流程的可扩展性,我们收集了 3,500 个 ICESat-2 片段,其中包含约 140 万个光谱归属水深测量点。然后,我们利用该数据集促进了深度递归神经网络的训练,以在 ICESat-2 光子水平上对海底栖息地进行分类。我们训练了两个相同的模型,一个包含光谱属性,另一个不包含光谱属性,以研究将 ICESat-2 光子与 Sentinel-2 融合的益处。结果显示,根据 F1 分数,模型性能提高了 18 个百分点。这些程序和源代码都是公开的,它们将提高 ICESat-2 的新测深数据产品 ATL24 的价值,该产品计划于 2024 年秋季发布。这些程序也可能适用于 NASA 即将执行的 CASALS 任务的数据。
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引用次数: 0
How to Find Accurate Terrain and Canopy Height GEDI Footprints in Temperate Forests and Grasslands? 如何在温带森林和草地中找到准确的地形和树冠高度 GEDI 脚印?
IF 2.9 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-10-25 DOI: 10.1029/2024EA003709
Vítězslav Moudrý, Jiří Prošek, Suzanne Marselis, Jana Marešová, Eliška Šárovcová, Kateřina Gdulová, Giorgi Kozhoridze, Michele Torresani, Duccio Rocchini, Anette Eltner, Xiao Liu, Markéta Potůčková, Adéla Šedová, Pablo Crespo-Peremarch, Jesús Torralba, Luis A. Ruiz, Michela Perrone, Olga Špatenková, Jan Wild

Filtering approaches on Global Ecosystem Dynamics Investigation (GEDI) data differ considerably across existing studies and it is yet unclear which method is the most effective. We conducted an in-depth analysis of GEDI's vertical accuracy in mapping terrain and canopy heights across three study sites in temperate forests and grasslands in Spain, California, and New Zealand. We started with unfiltered data (2,081,108 footprints) and describe a workflow for data filtering using Level 2A parameters and for geolocation error mitigation. We found that retaining observations with at least one detected mode eliminates noise more effectively than sensitivity. The accuracy of terrain and canopy height observations depended considerably on the number of modes, beam sensitivity, landcover, and terrain slope. In dense forests, a minimum sensitivity of 0.9 was required, while in areas with sparse vegetation, sensitivity of 0.5 sufficed. Sensitivity greater than 0.9 resulted in an overestimation of canopy height in grasslands, especially on steep slopes, where high sensitivity led to the detection of multiple modes. We suggest excluding observations with more than five modes in grasslands. We found that the most effective strategy for filtering low-quality observations was to combine the quality flag and difference from TanDEM-X, striking an optimal balance between eliminating poor-quality data and preserving a maximum number of high-quality observations. Positional shifts improved the accuracy of GEDI terrain estimates but not of vegetation height estimates. Our findings guide users to an easy way of processing of GEDI footprints, enabling the use of the most accurate data and leading to more reliable applications.

全球生态系统动力学调查(GEDI)数据的过滤方法在现有研究中差异很大,目前还不清楚哪种方法最有效。我们深入分析了 GEDI 在绘制西班牙、加利福尼亚和新西兰温带森林和草地三个研究地点的地形和树冠高度图时的垂直精度。我们从未经过滤的数据(2,081,108 个足迹)入手,描述了使用 2A 级参数进行数据过滤和减轻地理定位误差的工作流程。我们发现,保留至少一种检测模式的观测数据比灵敏度更有效地消除噪声。地形和树冠高度观测的准确性在很大程度上取决于模式数量、波束灵敏度、土地覆盖率和地形坡度。在茂密的森林中,最低灵敏度要求为 0.9,而在植被稀疏的地区,灵敏度为 0.5 即可。灵敏度大于 0.9 会导致高估草地的冠层高度,尤其是在陡坡上,高灵敏度会导致检测到多种模式。我们建议排除草地上超过五种模式的观测数据。我们发现,过滤低质量观测数据的最有效策略是将质量标志和 TanDEM-X 的差值结合起来,在剔除低质量数据和最大限度保留高质量观测数据之间取得最佳平衡。位置移动提高了 GEDI 地形估计的准确性,但没有提高植被高度估计的准确性。我们的研究结果为用户提供了处理 GEDI 脚印的简便方法,使他们能够使用最准确的数据,并带来更可靠的应用。
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引用次数: 0
Illuminating the Hierarchical Segmentation of Faults Through an Unsupervised Learning Approach Applied to Clouds of Earthquake Hypocenters 通过应用于地震中心云的无监督学习方法阐明断层的分层分割
IF 2.9 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-10-25 DOI: 10.1029/2023EA003267
E. Piegari, G. Camanni, M. Mercurio, W. Marzocchi

We propose a workflow for the recognition of the hierarchical segmentation of faults through earthquake hypocenter clustering without prior information. Our approach combines density-based clustering algorithms (DBSCAN and OPTICS), and principal component analysis (PCA). Given a spatial distribution of earthquake hypocenters, DBSCAN identifies first-order clusters, representing regions with the highest density of connected seismic events. Within each first-order cluster, OPTICS further identifies nested higher-order clusters, providing information on their number and size. PCA analysis is applied to first- and higher-order clusters to evaluate eigenvalues, allowing discrimination between seismicity associated with planar features and distributed seismicity that remains uncategorized. The identified planes are then geometrically characterized in terms of their location and orientation in the space, length, and height. This automated procedure operates within two spatial scales: the largest scale corresponds to the longest pattern of approximately equally dense earthquake clouds, while the smallest scale relates to earthquake location errors. By applying PCA analysis, a planar feature outputted from a first-order cluster can be interpreted as a fault surface while planes outputted after OPTICS can be interpreted as fault segments comprised within the fault surface. The evenness between the orientation of illuminated fault surfaces and fault segments, and that of the nodal planes of earthquake focal mechanisms calculated along the same faults, corroborates this interpretation. Our workflow has been successfully applied to earthquake hypocenter distributions from various seismically active areas (Italy, Taiwan, and California) associated with faults exhibiting diverse kinematics.

我们提出了一种工作流程,用于在没有先验信息的情况下,通过地震次中心聚类识别断层的分层分割。我们的方法结合了基于密度的聚类算法(DBSCAN 和 OPTICS)和主成分分析(PCA)。给定地震次中心的空间分布后,DBSCAN 会识别一阶聚类,代表连接地震事件密度最高的区域。在每个一阶群集内,OPTICS 进一步识别嵌套的高阶群集,提供有关其数量和规模的信息。对一阶和高阶震群进行 PCA 分析,以评估特征值,从而区分与平面特征相关的地震和未分类的分布式地震。然后,根据平面在空间中的位置和方向、长度和高度,对识别出的平面进行几何特征描述。这一自动程序在两个空间尺度内运行:最大尺度对应于近似等密度地震云的最长模式,而最小尺度则与地震位置误差有关。通过应用 PCA 分析,一阶聚类分析输出的平面特征可解释为断层面,而 OPTICS 后输出的平面可解释为断层面内的断层段。被照亮的断层面和断层段的方位与沿同一断层计算的地震焦点机制的节点平面的方位之间的均匀性证实了这一解释。我们的工作流程已成功应用于多个地震活跃地区(意大利、台湾和加利福尼亚)的地震震中分布,这些地区的断层具有不同的运动学特征。
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引用次数: 0
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