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Occurrence of Rare Lightning Events During Hurricane Nicholas (2021) “尼古拉斯”飓风期间罕见闪电事件的发生(2021年)
IF 2.9 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-12-21 DOI: 10.1029/2024EA003733
Timothy Logan, Jacob Hale, Sydney Butler, Brendan Lawrence, Samuel Gardner

Hurricane Nicholas was classified as a Category 1 tropical cyclone (TC) at 0000 UTC on 14 September 2021 and made landfall along the upper Texas Gulf Coast at 0530 UTC with maximum sustained winds of 33 m s−1. Much of the electrical activity during Nicholas was monitored by the Houston Lightning Mapping Array (HLMA) network. Thunderstorm activity developed in the rainband at 1700 UTC on 13 September, diminished by 2030 UTC, and re-intensified after 2200 UTC. At 2004 UTC (13 September), a curved megaflash (∼220 km) was observed by the HLMA in the stratiform precipitation region of the outer rainband. By 0130 UTC on 14 September 2021, vigorous storm cells developed in the eastern eyewall region and propagated cyclonically to the western eyewall region. At least four “jet-like” transient luminous events (TLEs) were observed by the HLMA emanating from a storm cell in the western eyewall region between 0230 and 0300 UTC with VHF source points ranging from 30 to 45 km in altitude. Moreover, the TLEs occurred within a region of strong wind shear, upper-level graupel-ice crystal collisions (∼15 km), and strong cloud top divergence. Charge analysis of the thunderstorm activity during Nicholas revealed an overall normal dipole structure, while the megaflash and TLE cases exhibited inverted dipole charge structures. Dissipation of the upper-level screening charge layer resulting from cloud top divergence likely played a role in the observed TLE VHF sources escaping to altitudes exceeding 30 km.

飓风尼古拉斯于2021年9月14日0000世界时被列为一级热带气旋,并于0530世界时沿德克萨斯州墨西哥湾沿岸登陆,最大持续风速为33米/秒。“尼古拉斯”期间的大部分电活动由休斯敦闪电测绘阵列(HLMA)网络监测。雷暴活动在9月13日1700世界时在雨带发展,到2030世界时减弱,2200世界时后再次增强。在2004 UTC(9月13日),HLMA在外层雨带的层状降水区观测到一个弯曲的巨型闪光(~ 220公里)。到2021年9月14日0130 UTC,东部眼壁区发展出强烈的风暴单体,并以气旋方式向西部眼壁区传播。在0230 - 0300 UTC期间,hma在西眼壁区域的一个风暴单体观测到至少4个“喷射状”瞬变发光事件(TLEs), VHF源点高度在30 - 45 km之间。此外,TLEs发生在强风切变、上层霰-冰晶碰撞(~ 15 km)和强云顶辐散的区域内。尼古拉斯雷暴期间的电荷分析显示整体上为正常的偶极子结构,而巨闪和TLE则表现为反向的偶极子电荷结构。在观测到的TLE VHF源逃逸到超过30 km高度的过程中,由云顶散度引起的上层屏蔽电荷层耗散可能起了一定作用。
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引用次数: 0
Seasonal Cycle in Sea Level Across the Coastal Zone 沿海地区海平面的季节周期
IF 2.9 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-12-20 DOI: 10.1029/2024EA003978
Rui M. Ponte, Michael Schindelegger
<p>Data from tide gauges and satellite altimeters are used to provide an up-to-date assessment of the mean seasonal cycle in sea level (<span></span><math> <semantics> <mrow> <mi>ζ</mi> </mrow> <annotation> $zeta $</annotation> </semantics></math>) over most of the global coastal ocean. The tide gauge records, where available, depict a <span></span><math> <semantics> <mrow> <mi>ζ</mi> </mrow> <annotation> $zeta $</annotation> </semantics></math> seasonal cycle with complex spatial structure along and across continental boundaries, and an annual oscillation dominating over semiannual variability, except in a few regions (e.g., the northwestern Gulf of Mexico). Comparisons between tide gauge and altimeter data reveal substantial root-mean-square differences and only slight improvements in agreement when using along-track data optimized for coastal applications. Quantification of the uncertainty in the altimeter products, inferred from comparing gridded and along-track estimates, indicate that differences to tide gauges partly reflect short-scale features of the seasonal cycle in proximity to the coasts. We additionally probe the <span></span><math> <semantics> <mrow> <mi>ζ</mi> </mrow> <annotation> $zeta $</annotation> </semantics></math> seasonal budget using satellite gravimetry-based manometric estimates and steric terms calculated from the World Ocean Atlas 2023. Focusing on global median values, the sum of the estimated steric and manometric harmonics can explain <span></span><math> <semantics> <mrow> <mo>∼</mo> </mrow> <annotation> ${sim} $</annotation> </semantics></math> 65% (respectively 40%) of the annual (semiannual) variance in the coastal <span></span><math> <semantics> <mrow> <mi>ζ</mi> </mrow> <annotation> $zeta $</annotation> </semantics></math> observations. We identify several regions, for example, the Australian seaboard, where the seasonal <span></span><math> <semantics> <mrow> <mi>ζ</mi> </mrow> <annotation> $zeta $</annotation> </semantics></math> budget is not closed and illustrate that such analysis is mainly limited by the coarse spatial resolution of present satellite-derived mass change products. For most regions with a sufficiently tight budget closure, we find that although the importance of the manometric term generally increases with decreasing water depth, steric contributions are non-negligible nea
来自潮汐计和卫星高度计的数据被用来提供全球大部分沿海海洋海平面平均季节周期的最新评估(ζ $zeta $)。在现有的验潮仪记录中,描述了一个ζ $zeta $季节周期,具有沿大陆边界和跨大陆边界的复杂空间结构,除了少数地区(如墨西哥湾西北部)外,一年一次的振荡占主导地位,而不是半年一次的变化。潮汐计和高度计数据之间的比较揭示了显著的均方根差异,当使用针对沿海应用优化的沿轨数据时,一致性仅略有改善。对高度计产品的不确定性进行量化,通过比较格网估算和沿迹估算推断,表明与潮汐测量仪的差异部分反映了海岸附近季节周期的短尺度特征。我们还使用基于卫星重力的压力估计和2023年世界海洋地图集计算的立体项来探测ζ $zeta $季节预算。关注全局中值,估计的空间谐波和压力谐波的总和可以解释~ ${sim} $ 65% (respectively 40%) of the annual (semiannual) variance in the coastal ζ $zeta $ observations. We identify several regions, for example, the Australian seaboard, where the seasonal ζ $zeta $ budget is not closed and illustrate that such analysis is mainly limited by the coarse spatial resolution of present satellite-derived mass change products. For most regions with a sufficiently tight budget closure, we find that although the importance of the manometric term generally increases with decreasing water depth, steric contributions are non-negligible near coastlines, especially at the annual frequency.
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引用次数: 0
Trends of Summer Lake Surface Water Temperature on the Tibetan Plateau and Their Response to Climate Change 青藏高原夏季湖泊地表水温变化趋势及其对气候变化的响应
IF 2.9 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-12-18 DOI: 10.1029/2024EA003910
Yi Shi, Anning Huang, Yang Wu,  Lazhu, Lijuan Wen

The Tibetan Plateau (TP) is covered by numerous lakes, and lake surface water temperature (LSWT) is an essential indicator of climate change, while few observations hinder our understanding of LSWT variation and its causes over TP. This study aims to simulate the summer LSWT long-term trends of 81 TP lakes during 1980–2018 and quantify the impacts and contributions of atmospheric variables. Results show that TP lakes warmed with 0.32°C decade−1 on average. Northern TP lakes warmed faster than the southern ones (0.44 vs. 0.16°C decade−1) due to stronger trends of atmospheric variables and higher sensitive of colder lakes to atmospheric changes. 55 (67.9%) lakes of the total lakes studied in current work warmed slower than air due to weakened shortwave radiation (SW). Attribution analysis suggests that the air warming and wetting over TP dominate lakes' warming. Regarding synthesis contributions, air warming contributed 79.3%, with increased surface air temperature (SAT) and downward longwave radiation (LW) accounting for 41.6% and 37.7%, respectively, and air wetting indicated by increased surface specific humidity (SSH) contributed 39.0%, followed by a positive contribution (16.8%) from declined wind speed (WS). The negative contribution (−35.1%) from weakened SW nearly counterbalances the positive effects of increased LW. 55.1% of the total synthesis contribution arises from the cross contribution through interactions among atmospheric variables and is mainly reflected in SAT and SSH, accounting for 26.8% and 24.8%, respectively. The findings enhance understanding of climate change impacts on lake systems and offer insights for lake resource management.

青藏高原湖泊覆盖面积大,湖泊地表温度是气候变化的重要指标,但观测资料较少,阻碍了我们对青藏高原地表温度变化及其原因的认识。本研究旨在模拟1980—2018年81个TP湖泊夏季LSWT的长期趋势,量化大气变量的影响和贡献。结果表明,青藏高原湖泊平均升温幅度为0.32°C。由于大气变量的变化趋势更强,较冷湖泊对大气变化的敏感性更高,北部TP湖泊比南部湖泊升温更快(0.44 vs 0.16°C 10−1)。由于短波辐射减弱(SW↓),目前研究的湖泊中有55个(67.9%)湖泊的升温速度比空气慢。归因分析表明,青藏高原上空的空气增暖和湿润主导了湖泊增暖。在综合贡献中,空气增温贡献占79.3%,其中地表气温(SAT)升高和向下长波辐射(LW↓)分别占41.6%和37.7%,地表比湿度(SSH)增加所表现的空气润湿贡献占39.0%,其次是风速(WS)下降的正贡献(16.8%)。减弱的SW↓的负贡献(- 35.1%)几乎抵消了增加的LW↓的正影响。总合成贡献的55.1%来自于大气变量间相互作用的交叉贡献,主要体现在SAT和SSH,分别占26.8%和24.8%。这一发现增强了对气候变化对湖泊系统影响的认识,并为湖泊资源管理提供了见解。
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引用次数: 0
Changing Extreme Precipitation Patterns in Nepal Over 1971–2015 1971-2015 年尼泊尔极端降水模式的变化
IF 2.9 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-12-15 DOI: 10.1029/2024EA003563
Yinxue Luo, Lang Wang, Chenxi Hu, Lu Hao, Ge Sun

This paper provides a comprehensive and comparative analysis of extreme precipitation patterns from 1971 to 2015 in Nepal, a data scarce, but “hot spot” region in global climate change. We compare in-situ observations and gridded precipitation data from the Asian Precipitation Highly Resolved Observational Data Integration Toward Evaluation of Water Resources (APHRODITE). Using 11 precipitation indices, we show that high-intensity (RX1day, R95pTOT, R99pTOT) and frequency-related indices (R10 mm, R20 mm) have decreased but annual maximum consecutive dry and wet days have increased. Observations affirm these trends found by the APHRODITE, but show smaller magnitudes likely due to differences in measurements at locations made below the 3,000 m elevation line. Spatially, the relatively dry western region has become wetter, and the relatively wet eastern region has become drier post-2003. The weakening of the South Asia Monsoon circulation, particularly assessed by the Webster and Yang Monsoon Index, correlates strongly with extreme precipitation indices. Changes in upper-level jet and associated lower-level monsoon trough are identified as critical factors influencing the extreme precipitation trend post-2003. This study is the first to confirm the efficacy of APHRODITE in providing spatial and temporal precipitation patterns in a data-limited region. We conclude that monsoon weakened circulations and changes in regional wind fields play dominant roles in the long-term temporal and spatial trends of extreme precipitation in Nepal. The reduced precipitation extremes in the wet eastern region may somewhat lessen severe flooding and erosion, but the drier western region may face heightened risks in precipitation-related hazards in Nepal.

本文对尼泊尔1971 - 2015年的极端降水模式进行了综合对比分析,尼泊尔是全球气候变化的一个数据稀缺的“热点”地区。我们比较了亚洲降水高分辨率观测数据整合对水资源评价(APHRODITE)的现场观测和网格降水数据。利用11个降水指数分析,高强度(RX1day、R95pTOT、R99pTOT)和频率相关指数(R10 mm、R20 mm)均有所减少,年最大连续干湿日数增加。观测证实了阿芙罗狄蒂号发现的这些趋势,但显示出较小的震级,可能是由于在海拔3000米以下的地点测量的差异。从空间上看,2003年后相对干燥的西部地区变湿润,相对湿润的东部地区变干燥。南亚季风环流的减弱,特别是由韦伯斯特和杨季风指数评估的减弱,与极端降水指数密切相关。高层急流和低层风槽的变化是影响2003年以后极端降水趋势的关键因素。这项研究首次证实了APHRODITE在数据有限的区域内提供时空降水模式的有效性。季风减弱环流和区域风场变化在尼泊尔极端降水的长期时空变化趋势中起主导作用。在潮湿的东部地区,极端降水的减少可能会在一定程度上减轻严重的洪水和侵蚀,但在尼泊尔,干旱的西部地区可能面临与降水有关的灾害的高风险。
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引用次数: 0
InSAR Observations of Construction-Induced Coastal Subsidence on Miami's Barrier Islands, Florida InSAR 对佛罗里达州迈阿密壁垒岛施工引起的海岸沉降的观测结果
IF 2.9 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-12-13 DOI: 10.1029/2024EA003852
Farzaneh Aziz Zanjani, Falk Amelung, Andreas Piter, Khaled Sobhan, Amin Tavakkoliestahbanati, Gregor P. Eberli, Mahmud Haghshenas Haghighi, Mahdi Motagh, Pietro Milillo, Sara Mirzaee, Antonio Nanni, Esber Andiroglu

This study utilizes Interferometric Synthetic Aperture Radar (InSAR) to examine subsidence along the coastal strip of the Miami barrier islands from 2016 to 2023. Using Sentinel-1 data, we document vertical displacements ranging from 2 to 8 cm, affecting a total of 35 coastal buildings and their vicinity. About half of the subsiding structures are younger than 2014 and at the majority of them subsidence decays with time. This correlation suggests that the subsidence is related to construction activities. In northern and central Sunny Isles Beach, where 23% of coastal structures were built during the last decade, nearly 70% are experiencing subsidence. The majority of the older subsiding structures show sudden onset or sudden acceleration of subsidence, suggesting that this is due to construction activities in their vicinity; we have identified subsidence at distance of 200 m, possibly up to 320 m, from construction sites. We attribute the observed subsidence to load-induced, prolonged creep deformation of the sandy layers within the limestone, which is accelerated, if not instigated, by construction activities. Distant subsidence from a construction site could indicate extended sandy deposits. Anthropogenic and natural groundwater movements could also be driving the creep deformation. This study demonstrates that high-rise construction on karstic barrier islands can induce creep deformation in sandy layer within the limestone succession persisting for a decade or longer. It showcases the potential of InSAR technology for monitoring both building settlement and structural stability.

本研究利用干涉合成孔径雷达(InSAR)研究了2016年至2023年迈阿密堰洲岛沿海地带的沉降情况。利用Sentinel-1数据,我们记录了垂直位移范围从2到8厘米,总共影响了35座沿海建筑物及其附近地区。大约一半的沉降构造比2014年更年轻,其中大多数沉降随时间而衰减。这种相关性表明下沉与建筑活动有关。在阳光岛海滩的北部和中部,23%的海岸建筑是在过去十年中建造的,近70%的建筑正在下沉。大多数老旧沉降构造表现为突然开始或突然加速沉降,表明这是由于其附近的建筑活动所致;我们已经确定了距离建筑工地200米,可能高达320米的下沉。我们将观测到的下沉归因于荷载引起的石灰岩内砂层的长期蠕变变形,如果不是由建筑活动引起的话,这种变形是加速的。建筑工地远处的下沉可能表明有大面积的沙质沉积物。人为和自然的地下水运动也可能导致蠕变变形。研究表明,喀斯特堰洲岛上的高层建筑可引起持续10年或更长时间的灰岩演替中的砂层蠕变。它展示了InSAR技术在监测建筑物沉降和结构稳定性方面的潜力。
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引用次数: 0
Long Period Seismology on Titan in the Presence of a Methane Clathrate Lid 甲烷包合物盖存在下土卫六上的长周期地震学
IF 2.9 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-12-07 DOI: 10.1029/2024EA003703
Andrea S. Bryant, Mark P. Panning, Angela G. Marusiak

Previous 1-D spherically symmetric seismic modeling studies have shown that in the presence of a clathrate lid on Titan significant thermal profile differences result, particularly in comparison to a pure water ice shell. In turn, these thermal differences would lead to notable changes in the waveform amplitudes and seismic phase arrival times. In this study we investigate the feasibility of using surface waves dispersion to explore the structure of Titan's ice shell. We investigate the ability to measure and observe the frequency-dependent signals (0.003–0.100 Hz) and their utility in being able to detect existence of a methane-clathrate lid. We find that we are unlikely to resolve the clathrate-lid's existence using long-period techniques, and this could be a limitation for studying very thick ice shells (> ${ >} approx $ 20 km) of icy ocean worlds. We did resolve the frequency range of flexural waves transitioning to a Stoneley wave (mode) in the fundamental mode, and see a Rayleigh wave in the first overtone for a 100 km ice shell on Titan for a simulated quake.

之前的一维球对称地震建模研究表明,泰坦上存在笼形物盖时,会产生显著的热剖面差异,特别是与纯水冰壳相比。反过来,这些温差会导致波形幅度和地震相位到达时间的显著变化。在这项研究中,我们探讨了利用表面波色散来探索土卫六冰壳结构的可行性。我们研究了测量和观察频率相关信号(0.003-0.100 Hz)的能力及其在能够检测甲烷包合物盖的存在方面的效用。我们发现,我们不太可能用长周期技术来解决笼形盖子的存在,这可能是研究非常厚的冰壳的一个限制。≈${>;} 约$ 20公里)的冰海洋世界。我们确实在基模中解析了弯曲波过渡到斯通利波(模式)的频率范围,并在模拟地震的土卫六上100公里冰壳的第一泛音中发现了瑞利波。
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引用次数: 0
Moisture Sources and Atmospheric Circulation Patterns for Extreme Rainfall Event Over North China Plain From 29 July to 2 August 2023 2023年7月29日- 8月2日华北平原极端降水事件的水汽源和大气环流特征
IF 2.9 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-12-07 DOI: 10.1029/2024EA003956
Hui Guo, Wanting Hu, Chen Yang, Fang Wan

Two years following the extreme rainfall event in Henan Province in July 2021, North China was struck by another significant rainfall episode in late July and early August 2023 (the “23.7” event). This recent event, surpassed only by the August 1963 deluge in Henan province, precipitated extensive disasters across the Beijing-Tianjin-Hebei region (BTH) over the North China Plain. Understanding the mechanisms underlying such extreme precipitation events, including moisture sources and atmospheric circulation patterns, in the context of synoptic-scale systems is crucial for accurate predictions and effective disaster mitigation in the future. To achieve this, this study utilized a vertically integrated water vapor transport method and a Water Accounting model to investigate the moisture sources and pathways of the “23.7” event. A systematic analysis of circulation patterns was also conducted based on the ERA5 reanalysis. The results showed that the western North Pacific and Indian Ocean contributed 38.1% and 18.6%, respectively, to the extreme rainfall over the BTH region. Additionally, terrestrial moisture sources contributed 16.59%, playing a significant role in the event. The stable and moisture-laden air was transported to the BTH due to the influence of binary tropical cyclones “Doksuri” and “Khanun,” as well as the western Pacific subtropical high-pressure system. Convergence and updraft dynamics trigger convective processes modulated by vortices and topography. The findings of this study help to build a deeper understanding of the formation processes and mechanisms behind such heavy rainfall, which provides insights for model predictions of similar high-impact low-frequency extreme rainfall events.

继2021年7月河南省极端降雨事件两年后,2023年7月下旬和8月上旬,华北地区又发生了一次重大降雨事件(“23.7”事件)。最近发生的这一事件,仅次于1963年8月发生在河南省的洪水,在华北平原的京津冀地区(BTH)引发了广泛的灾害。在天气尺度系统的背景下,了解这些极端降水事件背后的机制,包括水分来源和大气环流模式,对于未来准确预测和有效减轻灾害至关重要。为此,本研究利用垂直一体化水汽输送法和水分核算模型对“23.7”事件的水汽源和水汽通道进行了研究。在ERA5再分析的基础上,对环流模式进行了系统分析。结果表明,北太平洋西部和印度洋对BTH地区极端降水的贡献率分别为38.1%和18.6%。此外,陆地水汽源贡献了16.59%,在此次事件中发挥了重要作用。受双热带气旋“Doksuri”和“Khanun”的影响,以及西太平洋副热带高压系统的影响,稳定且富含水分的空气被输送到BTH。辐合和上升气流动力学触发由涡旋和地形调制的对流过程。这项研究的发现有助于更深入地了解这种强降雨背后的形成过程和机制,这为类似高影响低频极端降雨事件的模型预测提供了见解。
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引用次数: 0
An Improved Pattern Informatics Method for Extracting Ionospheric Disturbances Related to Seismicity Based on CSES Data: A Case Study of the Mw7.3 Maduo Earthquake 基于CSES数据的电离层扰动提取改进模式信息学方法——以Mw7.3玛多地震为例
IF 2.9 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-12-06 DOI: 10.1029/2024EA003687
Weixi Tian, Yongxian Zhang, Changhui Ju, Shengfeng Zhang, Maoning Feng, Fengli Liu

The exploration of multi-layer coupling mechanisms between earthquakes and the ionosphere is crucial for utilizing ionospheric precursors in earthquake prediction. A significant research task involves continuously tracking the spatio-temporal changes in ionospheric parameters, acquiring comprehensive seismic anomaly information, and capturing “deterministic” precursor anomalies. Based on data from the China Seismo-Electromagnetic Satellite (CSES), we enhance the Pattern Informatics (PI) Method and propose an Improved Pattern Informatics (IPI) Method. The IPI method enables the calculation of the spatio-temporal dynamics of electron density anomalies detected by the CSES satellite. The seismic signals in the electron density during earthquake on 2021 at Maduo are investigated in this work. The results show that: (a) Compared to original electron density images, the IPI method-derived models extract distinct electron density anomaly signals, regardless of the data whether are collected during descending (daytime) or ascending (nighttime) orbits, or across different time scales of change window. (b) The electron density anomalies appear about 40 days prior to the Maduo Mw7.3 earthquake. The evolution of these anomalies follows a pattern of appearance, persistence, disappearance, re-emergence, and final disappearance. Moreover, the evolution trends of the IPI hotspot images at daytime and nighttime are similar. These results suggest that the IPI method can capture the spatio-temporal trends of ionospheric parameters and effectively extract electronic precursors related to strong earthquakes.

探索地震与电离层的多层耦合机制是利用电离层前兆进行地震预报的关键。持续跟踪电离层参数的时空变化,获取全面的地震异常信息,捕捉“确定性”前兆异常,是一个重要的研究任务。基于中国地震电磁卫星(CSES)数据,对模式信息学(PI)方法进行了改进,提出了一种改进的模式信息学(IPI)方法。IPI方法可以计算CSES卫星探测到的电子密度异常的时空动态。本文研究了2021年玛多地震期间电子密度的地震信号。结果表明:(a)与原始电子密度图像相比,IPI方法衍生的模型无论在下降(白天)或上升(夜间)轨道上收集数据,还是在不同的变化窗口时间尺度上收集数据,都能提取出明显的电子密度异常信号。(b)电子密度异常出现在麻多Mw7.3地震前40天左右。这些异常的演变遵循出现、持续、消失、重新出现和最终消失的模式。此外,IPI热点图像在白天和夜间的演变趋势相似。这些结果表明,IPI方法可以捕捉电离层参数的时空变化趋势,有效地提取与强震有关的电子前兆。
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引用次数: 0
Tropical Cyclone Wind Field Reconstruction for Hazard Estimation via Bayesian Hierarchical Modeling With Neural Network 基于神经网络贝叶斯分层建模的热带气旋风场重建
IF 2.9 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-12-06 DOI: 10.1029/2024EA003678
C. Yang, J. Xu

Tropical cyclones (TCs) are one of the biggest threats to life and property around the world. Accurate estimation of TC wind hazard requires estimation of catastrophic TCs having a very long return period spanning up to thousands of years. Since reliable TC data are available only for recently decades, stochastic modeling and simulation turned out to be an effective approach to achieve more stable hazard estimates. In common practice, hundreds of thousands of synthetic TCs are generated first, then wind fields are reconstructed along synthetic TC tracks for hazard estimation. A Bayesian hierarchical modeling approach to the reconstruction of TC wind field is proposed. A modified Rankine vortex is adopted as the wind field model, of which the four free parameters are modeled simultaneously through a multi-output neural network as a latent process of the wind field. The four parameters are finally represented, spatially and temporally, by a set of neural network weights, The Bayesian model averaging technique is used for parameter estimation and wind field reconstruction, based on a ensemble of maximum a posteriori estimates of the set of weights. Together with previously proposed algorithm for synthetic TC simulation, a two-stage scheme for TC wind hazard estimation has been formed, which is based on best-track data only and thus is highly consistent. Application of this scheme to the offshore waters in the western North Pacific basin shows inspiring performance and great flexibility for various purposes of TC wind hazard estimation.

热带气旋(tc)是世界各地生命和财产的最大威胁之一。对TC风害的准确估计需要对灾难性TC进行估计,这些TC具有很长的重现期,长达数千年。由于可靠的TC数据仅在最近几十年才可用,因此随机建模和模拟被证明是实现更稳定的危害估计的有效方法。在通常的实践中,首先产生数十万个合成TC,然后沿着合成TC轨道重建风场以进行危害估计。提出了一种用于TC风场重建的贝叶斯分层建模方法。采用改进的Rankine涡旋作为风场模型,通过多输出神经网络将四个自由参数作为风场的潜在过程同时建模。最后用一组神经网络权值在空间和时间上表示这四个参数。基于权值集的最大后验估计集合,采用贝叶斯模型平均技术进行参数估计和风场重建。结合前人提出的TC综合模拟算法,形成了一种仅基于最优轨迹数据的两阶段TC风害估计方案,具有较高的一致性。将该方案应用于北太平洋西部海盆近海海域,对各种目的的TC风害估算显示出令人鼓舞的效果和极大的灵活性。
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引用次数: 0
Hollows on Mercury: A Comprehensive Analysis of Spatial Patterns and Their Relationship to Craters and Structures 水星上的空洞:空间模式的综合分析及其与陨石坑和结构的关系
IF 2.9 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-12-05 DOI: 10.1029/2024EA003854
Barbara De Toffoli, Valentina Galluzzi, Matteo Massironi, Sebastien Besse, Gene Walter Schmidt, Oceane Barraud, Salvatore Buoninfante, Pasquale Palumbo

Hollows on Mercury are small (hundreds of meters - few kilometers), shallow (tens of meters), irregular depressions typically found in clusters, often associated with impact craters, and likely formed by the loss of volatile materials. While their exact formation process remains debated, various hypotheses suggest sublimation or space weathering. In this study, we analyzed the global distribution of hollows, exploring their spatial patterns and relationships with key geological features. Our findings challenge the idea that hollows arise from a single volatile-rich surface layer, suggesting instead that volatiles are dispersed throughout the crust. Hollows show no correlation with specific geological units or elevations, indicating no singular volatile source. Moreover, the transitory nature of hollows is suggested as they are rare in older, degraded craters but common in younger ones or older craters with deep-seated features, hinting at a link to the reworking of materials through impacts or volcano-tectonic activity.

水星上的空洞很小(几百米-几公里),浅(几十米),不规则的洼地通常在星系团中发现,通常与撞击坑有关,可能是由于挥发性物质的损失而形成的。虽然它们确切的形成过程仍有争议,但各种假说认为是升华或空间风化。本研究分析了全球凹陷的分布,探讨了其空间格局及其与关键地质特征的关系。我们的发现挑战了空穴起源于单一挥发物丰富的表层的观点,表明挥发物分散在整个地壳中。空洞与特定的地质单元或海拔没有相关性,表明没有单一的挥发源。此外,空洞的短暂性表明,它们在较老的、退化的陨石坑中很少见,但在较年轻的陨石坑或具有深层特征的较老的陨石坑中很常见,这暗示了通过撞击或火山构造活动对物质进行再加工的联系。
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Earth and Space Science
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