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Forest Impacts on Peak Runoff Revealed by Accounting for the Effects of Climate 考虑气候影响的森林对峰值径流的影响
IF 5.2 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-03-16 DOI: 10.1029/2025gl121139
Shaozhen Liu, James W. Kirchner, Louise J. Slater, Marius G. Floriancic, Ilja van Meerveld, Wouter R. Berghuijs
Land cover affects the runoff response of catchments. However, such land-cover effects remain difficult to decipher because experimental studies are site-specific, while large-sample analyses are often confounded by climate gradients that obscure the role of land cover. Site-to-site comparisons that ignore differences in antecedent wetness may overestimate runoff responses in forested catchments because they are typically found in humid climates. Here we quantify runoff responses to unit precipitation inputs and examine how they vary across 252 U.S. catchments with different land covers and forest fractions. For comparable antecedent wetness conditions (as quantified by antecedent streamflow), peak runoff responses decline as forest cover increases, with peak responses in forested catchments being 16%–63% lower than in catchments dominated by cropland or grassland. By accounting for climate-driven differences among catchments, our approach isolates the influences of land cover on reducing peak flows, which are often masked by climate in large-sample analyses.
土地覆盖影响流域径流响应。然而,这样的土地覆盖效应仍然难以破译,因为实验研究是特定地点的,而大样本分析经常被气候梯度混淆,而气候梯度模糊了土地覆盖的作用。忽略先前湿度差异的点对点比较可能会高估森林流域的径流响应,因为它们通常存在于潮湿的气候中。在这里,我们量化了径流对单位降水输入的响应,并研究了它们在美国252个不同土地覆盖和森林部分的集水区中的变化。对于可比的先前湿度条件(通过先前的溪流流量量化),峰值径流响应随着森林覆盖的增加而下降,森林流域的峰值响应比农田或草地为主的流域低16%-63%。通过考虑气候驱动的集水区差异,我们的方法隔离了土地覆盖对减少峰值流量的影响,这在大样本分析中经常被气候所掩盖。
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引用次数: 0
Frictional Heterogeneity Governs Slip Partitioning and Seismic Hazard in the 2023 Turkey Earthquake Doublet 2023年土耳其地震双峰的摩擦非均质性控制滑动分配和地震危险性
IF 5.2 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-03-15 DOI: 10.1029/2025gl119502
Jianlong Chen, Peizhen Zhang, Xin Qiao, Zicheng Huang, Lejun Lu
Quantifying fault frictional properties is fundamental to understanding slip behavior and seismic hazard. We analyze 2 years of Sentinel-1 SAR data following the 2023 Turkey earthquake doublet using Independent Component Analysis-enhanced Small Baseline Subset-InSAR, to resolve postseismic deformation and invert for afterslip on the East Anatolian and Çardak faults. Within a rate-and-state framework, we estimate the friction parameter <span data-altimg="/cms/asset/fd8e17c4-d7e8-4832-8d71-7a1b328d5200/grl72251-math-0001.png"></span><mjx-container ctxtmenu_counter="85" ctxtmenu_oldtabindex="1" jax="CHTML" role="application" sre-explorer- style="font-size: 103%; position: relative;" tabindex="0"><mjx-math aria-hidden="true" location="graphic/grl72251-math-0001.png"><mjx-semantics><mjx-mrow data-semantic-children="4" data-semantic-content="0,5" data-semantic- data-semantic-role="leftright" data-semantic-speech="left parenthesis a minus b right parenthesis" data-semantic-type="fenced"><mjx-mo data-semantic- data-semantic-operator="fenced" data-semantic-parent="6" data-semantic-role="open" data-semantic-type="fence" style="margin-left: 0.056em; margin-right: 0.056em;"><mjx-c></mjx-c></mjx-mo><mjx-mrow data-semantic-children="1,3" data-semantic-content="2" data-semantic- data-semantic-parent="6" data-semantic-role="subtraction" data-semantic-type="infixop"><mjx-mi data-semantic-annotation="clearspeak:simple" data-semantic-font="italic" data-semantic- data-semantic-parent="4" data-semantic-role="latinletter" data-semantic-type="identifier"><mjx-c></mjx-c></mjx-mi><mjx-mo data-semantic- data-semantic-operator="infixop,−" data-semantic-parent="4" data-semantic-role="subtraction" data-semantic-type="operator" rspace="4" space="4"><mjx-c></mjx-c></mjx-mo><mjx-mi data-semantic-annotation="clearspeak:simple" data-semantic-font="italic" data-semantic- data-semantic-parent="4" data-semantic-role="latinletter" data-semantic-type="identifier"><mjx-c></mjx-c></mjx-mi></mjx-mrow><mjx-mo data-semantic- data-semantic-operator="fenced" data-semantic-parent="6" data-semantic-role="close" data-semantic-type="fence" style="margin-left: 0.056em; margin-right: 0.056em;"><mjx-c></mjx-c></mjx-mo></mjx-mrow></mjx-semantics></mjx-math><mjx-assistive-mml display="inline" unselectable="on"><math altimg="urn:x-wiley:00948276:media:grl72251:grl72251-math-0001" display="inline" location="graphic/grl72251-math-0001.png" xmlns="http://www.w3.org/1998/Math/MathML"><semantics><mrow data-semantic-="" data-semantic-children="4" data-semantic-content="0,5" data-semantic-role="leftright" data-semantic-speech="left parenthesis a minus b right parenthesis" data-semantic-type="fenced"><mo data-semantic-="" data-semantic-operator="fenced" data-semantic-parent="6" data-semantic-role="open" data-semantic-type="fence" stretchy="false">(</mo><mrow data-semantic-="" data-semantic-children="1,3" data-semantic-content="2" data-semantic-parent="6" data-semantic-role="subtraction" data-semantic-type="in
量化断层的摩擦特性是理解滑动行为和地震危险性的基础。利用独立分量分析增强的小基线子集insar分析了2023年土耳其地震后2年的Sentinel-1 SAR数据,以解决东安纳托利亚断层和Çardak断层的震后变形和反演。在速率-状态框架内,我们估计了震后稳定区域的摩擦参数(a-b)$ (a-b)$ (R2 > 0.9),表明余震主要发生在高a-b$ a-b$速度增强区域,而同震破裂和余震集中在低a-b$ a-b$区域或邻近的不稳定斑块附近。深度相关的滑动分配表明受摩擦非均质性调节的脆性-韧性转变,深部后滑向东偏移和滑动行为的分割突出了震后变形的复杂性。p trge段a-b$ a-b$值升高表明断裂传播受到速度强化区域的限制。这些结果表明,摩擦非均质性可能控制滑动划分,并为大陆断层系统的地震危险性评估提供定量约束。
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引用次数: 0
Coral δ13C Reveals Little Ice Age Dimming of Tropical Surface Shortwave Radiation Not Captured by Climate Models 珊瑚δ13C揭示了没有被气候模式捕获的热带表面短波辐射的小冰河时期变暗
IF 5.2 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-03-14 DOI: 10.1029/2026gl121885
Guangchao Deng, Huimin Guo, Xuefei Chen, Jian-xin Zhao, Gangjian Wei, Wenfeng Deng
Tropical low-cloud feedback is the largest source of uncertainty in climate sensitivity, yet multi-century records of surface shortwave radiation are scarce. We calibrate Porites coral δ13C against satellite photosynthetically available radiation (PAR) and reconstruct monthly PAR for the northern South China Sea during the Medieval Climate Anomaly (1129–1264 CE) and the Little Ice Age (1631–1771 CE). After correcting for the Suess effect and propagating errors via Monte Carlo resampling techniques, annual PAR during the Little-Ice-Age is ∼22% lower and seasonality slightly weaker. The dimming aligns with regional proxies for cooler, wetter conditions and is best explained by brighter low clouds, likely boosted by volcanic aerosol–cloud interactions. CMIP6/PMIP4 past1000 simulations, however, yield <0.2% change over the same interval, indicating that current models understate volcanic microphysics and tropical low-cloud sensitivity. The coral PAR record thus provides a quantitative pre-industrial target for evaluating tropical cloud processes and reducing uncertainty in equilibrium climate sensitivity.
热带低云反馈是气候敏感性中最大的不确定性来源,然而多世纪的地表短波辐射记录却很少。本文利用卫星光合有效辐射(PAR)对Porites珊瑚的δ13C进行了校正,重建了中世纪气候异常(1129-1264 CE)和小冰期(1631-1771 CE)期间南海北部的PAR。在通过蒙特卡罗重采样技术校正了苏斯效应和传播误差后,小冰期的年PAR降低了约22%,季节性也稍弱。这种变暗与较冷、较湿的区域条件相一致,最好的解释是较亮的低空云层,可能是由火山气溶胶与云的相互作用推动的。然而,CMIP6/PMIP4过去1000次的模拟在相同的时间间隔内产生了0.2%的变化,这表明目前的模式低估了火山微物理和热带低云的敏感性。因此,珊瑚PAR记录为评估热带云过程和减少平衡气候敏感性的不确定性提供了定量的工业化前目标。
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引用次数: 0
Influence of Tibetan Plateau Snow Cover on ENSO Variability via the Dust-Iron Fertilization 青藏高原积雪通过尘铁施肥对ENSO变率的影响
IF 5.2 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-03-14 DOI: 10.1029/2025gl120206
Chao Zhang, Anmin Duan, Thomas J. Browning, Yuxin Xie, Eric P. Achterberg
The El Niño–Southern Oscillation (ENSO) and Tibetan Plateau, as key drivers of Earth's climate system, exert bidirectional controls that complicate causal attribution. Here, we integrate satellite-derived Tibetan Plateau snow cover (TPSC) with causal inference to establish TPSC-ENSO conversion factor. Using this factor, we estimate that TPSC anomalies contribute 24.8% (6.4%–44.1%) of September ENSO variability. Notably, TPSC-modulated biogeochemical processes are as influential as equatorial zonal wind mechanisms, constituting an additional ENSO driver. Reduced TPSC intensifies the Tibetan Plateau heat source, driving ascendant easterly anomalies. This accelerates the tropical easterly jet, transporting more Saharan dust to the tropical Pacific. Dust-iron fertilization stimulates phytoplankton accumulation across iron-limited central-eastern Equatorial Pacific, reducing solar irradiance penetration depth, lowering upper ocean heat content by 21% (7%–29%), and promoting La Niña development. Conversely, high TPSC favors El Niño development. These findings quantify TPSC's impact on ENSO variability, unveiling a biogeochemical pathway linking dust-iron fertilization to ocean energetics.
厄尔尼诺Niño-Southern涛动(ENSO)和青藏高原作为地球气候系统的主要驱动因素,发挥着双向控制作用,使因果归因复杂化。本文将卫星反演的青藏高原积雪(TPSC)与因果推断相结合,建立了TPSC- enso转换因子。利用这一因子,我们估计TPSC异常对9月份ENSO变率的贡献为24.8%(6.4%-44.1%)。值得注意的是,tpsc调节的生物地球化学过程与赤道纬向风机制一样有影响力,构成了额外的ENSO驱动因素。TPSC的减少强化了青藏高原热源,驱动上升偏东异常。这加速了热带偏东气流,将更多的撒哈拉沙尘输送到热带太平洋。尘铁施肥刺激了铁限制的赤道太平洋中东部浮游植物的积累,降低了太阳辐照度的穿透深度,使上层海洋热含量降低了21%(7%-29%),促进了La Niña的发展。相反,高TPSC有利于El Niño的发展。这些发现量化了TPSC对ENSO变异性的影响,揭示了将尘铁施肥与海洋能量学联系起来的生物地球化学途径。
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引用次数: 0
An Arctic Sea Ice Energy Budget for the Last Interglacial 末次间冰期的北极海冰能量收支
IF 5.2 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-03-14 DOI: 10.1029/2025gl120781
M. Pollock, R. Diamond, H. Heorton, L. C. Sime, D. Schroeder, C. Brierley
With ongoing anthropogenic warming, the Arctic is increasingly dominated by thin, first-year sea ice. Understanding the ice–ocean–atmosphere interactions in warmer climates is therefore essential. We analyze the Arctic sea-ice energy budget in nine CMIP6-PMIP4 lig127k simulations of the Last Interglacial warm Arctic. All models show reduced Last Interglacial summer sea ice, but with substantial inter-model spread. We demonstrate that this arises from differences in surface energy anomalies, which are highly correlated with sea ice area anomalies (r2${mathrm{r}}^{2}$ of 74%). Ice–albedo feedbacks dominate this response: reduced ice cover exposes more open ocean, enhances shortwave absorption, and warms the upper ocean. This heat is released in autumn, delaying sea-ice regrowth. Although modern warming is driven by longwave forcing, our results highlight that shortwave absorption from reduced albedo is a key driver of summer sea-ice loss, underscoring the need for accurate representation of surface heat-balance processes in future Arctic projections.
随着持续的人为变暖,北极越来越多地被薄的新生海冰所主宰。因此,了解温暖气候下的冰-海洋-大气相互作用是至关重要的。利用9次CMIP6-PMIP4 lig127k模拟分析了末次间冰期暖北极的海冰能量收支。所有模式均显示末次间冰期夏季海冰减少,但模式间扩展较大。我们证明这是由于地表能量异常的差异引起的,地表能量异常与海冰面积异常高度相关(r2${ mathm {r}}^{2}$ = 74%)。冰反照率反馈主导了这一反应:冰盖的减少使更开阔的海洋暴露出来,增强了短波的吸收,并使上层海洋变暖。这些热量在秋天被释放,延缓了海冰的再生。尽管现代变暖是由长波强迫驱动的,但我们的研究结果强调,反照率降低引起的短波吸收是夏季海冰损失的关键驱动因素,这强调了在未来北极预测中准确表示地表热平衡过程的必要性。
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引用次数: 0
Steady Collapse of Uranus' Exosphere After 1998 to the Present Decade 天王星外逸层的稳定坍缩从1998年到现在的十年
IF 5.2 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-03-14 DOI: 10.1029/2025gl120292
D. Bhattacharyya, J. T. Clarke, P. Stephenson, T. Koskinen, J.-Y. Chaufray, L. Moore, H. Melin
Uranus' thermospheric temperature decreased from ∼800K in 1986 to ∼450K in 2022 as determined from observations of H3+ and H2 infrared emissions. Spitzer 2007 lower atmosphere observations do not emulate this cooling trend. Here we show that the atomic H Lyman ⍺ emission from the disk of Uranus observed by HST from 2011 to 2022 are not consistent with radiative transfer models based on a constant atmospheric structure retrieved from the Voyager 2 flyby of 1986. Instead, the optical depth of the H column matching the Uranus Lyman ⍺ disk brightness decreased after 1998, consistent with the long-term cooling trend. This decrease is irrespective of auroral activity. While the origin of the cooling is poorly understood, it indicates that the density and extent of the Uranssian exosphere changes on a time scale of years impacting the atmospheric structure, the magnetospheric proton source, and exospheric drag on the inner rings.
根据对H3+和H2红外辐射的观测,天王星的热层温度从1986年的~ 800K下降到2022年的~ 450K。斯皮策2007年的低层大气观测没有模拟这种冷却趋势。本文表明,2011年至2022年HST观测到的天王星盘的H Lyman原子发射与基于1986年旅行者2号飞掠获得的恒定大气结构的辐射传输模型不一致。相反,与天王星莱曼盘亮度匹配的H柱的光学深度在1998年后下降,与长期冷却趋势一致。这种减少与极光活动无关。虽然冷却的起源尚不清楚,但它表明,乌兰系外逸层的密度和范围以年为时间尺度变化,影响大气结构、磁层质子源和外逸层对内环的阻力。
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引用次数: 0
Holistic Retrieval of Absolute Coseismic Displacement Fields From Single Interferograms via Physics-Aware GANs 基于物理感知gan的单干涉图绝对同震位移场整体检索
IF 5.2 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-03-13 DOI: 10.1029/2025gl121419
Chuanhua Zhu, Jiaqiao Gan, Zuqi Lan, Chisheng Wang
The efficacy of rapid seismic response is fundamentally constrained by the sequential, multi-step nature of conventional InSAR processing, where error propagation and reliance on auxiliary data hinder automation. Here, we present a holistic framework using Physics-Aware Generative Adversarial Networks (GANs) to directly retrieve absolute coseismic displacement fields from single, noisy interferograms. By synthesizing the distinct spectral signatures of tectonic deformation against stratified and turbulent atmosphere, orbital ramps, and topographic residuals, our model achieves end-to-end signal extraction. This approach effectively bypasses adaptive filtering, external error corrections, and the fragile phase unwrapping step. Validation against 18 real-world earthquakes confirms the robust removal of segmentation artifacts. Crucially, comparison with GPS data from the 2016 Amatrice earthquake demonstrates high physical fidelity (>69 within 1σ) without post-processing. This self-contained paradigm eliminates manual intervention, establishing a new standard for instantaneous, automated, post-event situational awareness.
传统InSAR处理的顺序、多步骤特性从根本上限制了快速地震响应的有效性,其中误差传播和对辅助数据的依赖阻碍了自动化。在这里,我们提出了一个使用物理感知生成对抗网络(gan)的整体框架,以直接从单个噪声干涉图中检索绝对同震位移场。通过综合构造形变对层状和湍流大气、轨道斜坡和地形残差的独特光谱特征,我们的模型实现了端到端的信号提取。这种方法有效地绕过了自适应滤波、外部错误校正和脆弱的相位展开步骤。对18次真实地震的验证证实了分割伪影的鲁棒去除。至关重要的是,与2016年阿马特里切地震的GPS数据相比,未经后处理的物理保真度很高(1σ内>;69)。这种自包含的模式消除了人工干预,为即时、自动化、事件后的态势感知建立了新的标准。
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引用次数: 0
Thank You to Our 2025 Peer Reviewers 感谢我们的2025位同行评审
IF 5.2 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-03-13 DOI: 10.1029/2026gl122706
Kristopher Karnauskas, Anantha Aiyyer, Suzana Camargo, Fabio Capitanio, Peter Chi, Sloan Coats, Sylvia Dee, Christine Dow, Sarah Feakins, Robinson Fulweiler, Valier Galy, Neil Ganju, Alessandra Giannini, Yu Gu, Jianping Guo, Christian Huber, Valeriy Ivanov, Gregory Johnson, Monika Korte, Sujay Kumar, Soléne Lejosne, Kevin Lewis, Huixin Liu, Gudrun Magnusdottir, Mathieu Morlighem, Yuichi Otsuka, Paola Passalacqua, Christina Patricola-DiRosario, Germán Prieto, Bo Qiu, Lynn Russell, Kanako Seki, Hui Su, Daoyuan Sun, Hari Viswanathan, Guiling Wang, Kaicun Wang, Angelicque White, Quentin Williams, Lei Zhang, Zhaoru Zhang
<p>On behalf of the journal, AGU, and the scientific community, the editors of Geophysical Research Letters would like to sincerely thank those who reviewed manuscripts in 2025. The hours reading and commenting on manuscripts not only improve the manuscripts but also increase the scientific rigor of future research in the field. We greatly appreciate the assistance of the reviewers in advancing open science, which is a key objective of AGU's data policy. We particularly appreciate the timely reviews in light of the demands imposed by the rapid review process at Geophysical Research Letters. We received 5,930 submissions in 2025, and 6,036 reviewers contributed to their evaluation by providing 10,970 reviews in total. We deeply appreciate their contributions. Individuals in <i>italics</i> provided three or more reviews for GRL during the year.</p><p>A. Jayakumar</p><p>A. Karp</p><p>A. Petrukovich</p><p>Aakash Sane</p><p>Aaron Ashley</p><p><i>Aaron Breneman</i></p><p><i>Aaron Donohoe</i></p><p>Aaron Hendry</p><p>Aaron Hill</p><p>Aaron Johnson</p><p>Aaron Levine</p><p>Aaron Match</p><p>Aaron Mohammed</p><p>Aaron Naeger</p><p>Aaron Wech</p><p>Abby Hutson</p><p>Abdallah Zaki</p><p>Abdelhaq Hamza</p><p>Abdulamid Fakoya</p><p>Abhijit Das</p><p>Abhik Santra</p><p>Abhinav Gupta</p><p>Abhishek Rajhans</p><p>Abhishek Savita</p><p><i>Abigail Azari</i></p><p>Abigail Langston</p><p>Abigail Lute</p><p>Abigail Swann</p><p>Abigail Whittington</p><p><i>Abigail Williams</i></p><p>Abraham Emond</p><p>Abram Jacobson</p><p>Acacia Pepler</p><p>Adam Blaker</p><p><i>Adam Burnett</i></p><p>Adam Clark</p><p>Adam Forte</p><p>Adam Masters</p><p><i>Adam Povey</i></p><p>Adam Scaife</p><p>Adam Schreiner-McGraw</p><p>Adam Smith</p><p>Adam Sobel</p><p>Adam Sokol</p><p>Addison Rice</p><p><i>Adele Igel</i></p><p>Adeline Montlaur</p><p>Ademe Mekonnen</p><p>Adeyemi Adebiyi</p><p>Adina Pusok</p><p>Aditya Gusman</p><p>Aditya Khuller</p><p><i>Adrià Barbeta</i></p><p>Adrian Burd</p><p>Adrián Flores Orozco</p><p>Adrian Grocott</p><p><i>Adrian Harpold</i></p><p>Adrian Martin</p><p>Adrian Matthews</p><p>Adrian Muxworthy</p><p>Adrian Sheppard</p><p>Adrian Tasistro-Hart</p><p>Adrian Tompkins</p><p>Adriano Gualandi</p><p>Adrianus Reniers</p><p>Adrienne Marshall</p><p>Advik Eswaran</p><p>Agnès Borbon</p><p>Agnes Kontny</p><p>Agnes Lim</p><p>Agnese Marcato</p><p>Agniv Sengupta</p><p>Agus Santoso</p><p>Agust Gudmundsson</p><p>Ahmad Ghassemi</p><p>Ahmad Lalti</p><p>Ahmed Elkouk</p><p>Aibing Li</p><p>Aidan Blaser</p><p>Aiguo Dai</p><p>Aihui Wang</p><p>Aiko Voigt</p><p>Aimée Slangen</p><p>Aimin Du</p><p>Aislinn Fox</p><p>Aitaro Kato</p><p><i>Aixue Hu</i></p><p>Ajay Kumar</p><p><i>Ajay Raghavendra</i></p><p>Akash Koppa</p><p><i>Akira Kuwano-Yoshida</i></p><p>Akira Oka</p><p>Akira Yamazaki</p><p>Akiyoshi Wada</p><p>Akshay Deoras</p><p><i>Akshaya Nikumbh</i></p><p>Ala Aldahan</p><p>Alain Pietroniro</p><p>
《地球物理研究快报》的编辑谨代表杂志、AGU和科学界衷心感谢2025年审稿人员。对稿件的阅读和评论不仅提高了稿件的质量,而且增加了该领域未来研究的科学严谨性。我们非常感谢审稿人在推进开放科学方面的帮助,这是AGU数据政策的一个关键目标。鉴于《地球物理研究快报》快速审查过程的要求,我们特别感谢及时的审查。2025年共收到投稿5930篇,评审人员6036人,共提供评审10970篇。我们对他们的贡献深表感谢。以斜体字表示的个人在年内为GRL提供了三次或更多的审查。JayakumarA。KarpA。彼得鲁科维奇哈卡什SaneAaron ashleyaaaron BrenemanAaron DonohoeAaron hendryaaaron HillAaron JohnsonAaron leineaaron matchaon MohammedAaron NaegerAaron WechAbby HutsonAbdallah ZakiAbdelhaq hamzaabdelhaq hamzahamid FakoyaAbhijit dasabhihik SantraAbhinav古普塔abhishek RajhansAbhishek SavitaAbigail AzariAbigail langston阿比盖尔LuteAbigail SwannAbigail whittington阿比盖尔WilliamsAbraham EmondAbram JacobsonAcacia pepler亚当布莱克亚当伯内特亚当克拉克亚当亚当forte亚当大师亚当PoveyAdam ScaifeAdamSchreiner-McGrawAdam SmithAdam SobelAdam SokolAddison RiceAdele IgelAdeline montlauademe MekonnenAdeyemi AdebiyiAdina PusokAditya GusmanAditya khullradrionbarbetaadrian BurdAdrián弗洛雷斯·奥罗兹科阿德里安·格罗柯特·阿德里安·哈波德里安·马丁·阿德里安·马修斯·穆克斯沃斯·阿德里安·谢普帕德里安·塔斯特罗-哈特·托普金·德里亚诺·瓜兰迪亚·阿德里安·雷尼厄斯·萨德里安·马歇尔·阿德里安·埃斯瓦拉纳·阿格尼斯·孔蒂尼·阿格尼斯·利马涅斯·马卡托纳·阿格尼·森古普塔·圣托索·阿古斯特·古德蒙森·艾哈迈德·加塞米·艾哈迈德·拉尔蒂艾哈迈德ElkoukAibing LiAidan BlaserAiguo DaiAihui WangAiko voigtaiamachixue HuAjay KumarAjay raghavendraakakpaakira kuwano - yoshidaakakpaakakshaya nikumhala aldahashaya niumhala aldahashaya niumhala aldahaya PietroniroAlan CondronAlan FoxAlan Ley CooperAlan LiuAlan RempelAlan RhoadesAlan RobockAlan SeltzerAlan WoodlandAlba Rodriguez PadillaAlba ZapponeAlberto ArdidAldo fiori亚历克·达列克·彼得纳亚历克·桑切斯-弗兰克·桑切斯·桑切斯-里奥萨里克·佩德罗·阿列克谢TitovAleksi NummelinAlena MalyarenkoAlessandra BorghiAlessandra MarzadriAlessandro battaghialessandro LenciAlessandro SavazziAlessandro SilvanoAlessandro TengattiniAlessio BozzoAlex BradleyAlex BrisbourneAlex collinex CopleyAlex GonzalezAlex HaberlieAlex HoffmannAlex HutkoAlex MegannAlex RinehartAlex SheremetAlex VermeulenAlex wyatsander beereralexandbernealexandchernyshovalexandergottliealexandanderhageralexandkostskialexander MarshakAlexander MassaAlexander亚历山大·雷日科,亚历山大·西姆,亚历山大·索洛维,亚历山大·斯托,亚历山大·孙,亚历山大·特纳,亚历山大·维克,亚历山大·耶茨,亚历山德拉·奥德塞,亚历山大·亚历山大·福格,亚历山大·奥德塞,亚历山大·亚历山德拉·海特,亚历山德拉·拉莫斯-瓦莱,亚历山大·巴尔博尼,亚历山大·卡斯塔格,亚历山大·贡塞特,亚历山大·普洛维德,亚历山大·波尔,亚历山大·霍恩,亚历山大·波利迪,亚历山大·卡尔佩奇科,亚历克西斯·奥尔塔克西,赫里西维奇,亚历山德拉·卡佩奇科,阿列克谢·卡佩奇科,阿列克谢·卡佩奇科,阿列克谢·卡尔佩奇科,阿列克谢·卡尔佩奇科,阿列克谢·马丁内斯,加西亚·阿尔弗雷多·普拉奇,阿里·贝朗吉阿里Hasan SiddiquiAli SulaimanAlia al - hajana LesnekAliakbar HassanpouryouzbandAlice barthe alice portalalalice RenAlice TurnerAlice-Agnes GabrielAllison HoAllison michaelallison PeaseAllison steinallison allison WingAlvaro de la CámaraAlvise AranyossyAlyssa stansfield damadelis QuesadaAmala MahadevanAman BasuAmanda GiangAmani reddyamury deheqamber walshineia gromeelia sheevenellamilcar JuarezAmir AzarnivandAmir CaspiAmir KhanAmir Ouyed HernandezAmir SouriAmit patraamitabl NagAmol KishoreAmrapalliGaranaikAmy BowerAmy LiuAmy SimonAna BastosAna bolbolvarana EliasAna Maria Restrepo AcevedoAnam KhanAnant ParekhAnantha AiyyerAnass El aouniananastasia PiliourasAnatoly StreltsovAnders jorgensenandrr<s:1> NiemeijerAndre RevilAndrea BoehnischAndrea fassbenderanda
{"title":"Thank You to Our 2025 Peer Reviewers","authors":"Kristopher Karnauskas, Anantha Aiyyer, Suzana Camargo, Fabio Capitanio, Peter Chi, Sloan Coats, Sylvia Dee, Christine Dow, Sarah Feakins, Robinson Fulweiler, Valier Galy, Neil Ganju, Alessandra Giannini, Yu Gu, Jianping Guo, Christian Huber, Valeriy Ivanov, Gregory Johnson, Monika Korte, Sujay Kumar, Soléne Lejosne, Kevin Lewis, Huixin Liu, Gudrun Magnusdottir, Mathieu Morlighem, Yuichi Otsuka, Paola Passalacqua, Christina Patricola-DiRosario, Germán Prieto, Bo Qiu, Lynn Russell, Kanako Seki, Hui Su, Daoyuan Sun, Hari Viswanathan, Guiling Wang, Kaicun Wang, Angelicque White, Quentin Williams, Lei Zhang, Zhaoru Zhang","doi":"10.1029/2026gl122706","DOIUrl":"https://doi.org/10.1029/2026gl122706","url":null,"abstract":"&lt;p&gt;On behalf of the journal, AGU, and the scientific community, the editors of Geophysical Research Letters would like to sincerely thank those who reviewed manuscripts in 2025. The hours reading and commenting on manuscripts not only improve the manuscripts but also increase the scientific rigor of future research in the field. We greatly appreciate the assistance of the reviewers in advancing open science, which is a key objective of AGU's data policy. We particularly appreciate the timely reviews in light of the demands imposed by the rapid review process at Geophysical Research Letters. We received 5,930 submissions in 2025, and 6,036 reviewers contributed to their evaluation by providing 10,970 reviews in total. We deeply appreciate their contributions. Individuals in &lt;i&gt;italics&lt;/i&gt; provided three or more reviews for GRL during the year.&lt;/p&gt;\u0000&lt;p&gt;A. Jayakumar&lt;/p&gt;\u0000&lt;p&gt;A. Karp&lt;/p&gt;\u0000&lt;p&gt;A. Petrukovich&lt;/p&gt;\u0000&lt;p&gt;Aakash Sane&lt;/p&gt;\u0000&lt;p&gt;Aaron Ashley&lt;/p&gt;\u0000&lt;p&gt;&lt;i&gt;Aaron Breneman&lt;/i&gt;&lt;/p&gt;\u0000&lt;p&gt;&lt;i&gt;Aaron Donohoe&lt;/i&gt;&lt;/p&gt;\u0000&lt;p&gt;Aaron Hendry&lt;/p&gt;\u0000&lt;p&gt;Aaron Hill&lt;/p&gt;\u0000&lt;p&gt;Aaron Johnson&lt;/p&gt;\u0000&lt;p&gt;Aaron Levine&lt;/p&gt;\u0000&lt;p&gt;Aaron Match&lt;/p&gt;\u0000&lt;p&gt;Aaron Mohammed&lt;/p&gt;\u0000&lt;p&gt;Aaron Naeger&lt;/p&gt;\u0000&lt;p&gt;Aaron Wech&lt;/p&gt;\u0000&lt;p&gt;Abby Hutson&lt;/p&gt;\u0000&lt;p&gt;Abdallah Zaki&lt;/p&gt;\u0000&lt;p&gt;Abdelhaq Hamza&lt;/p&gt;\u0000&lt;p&gt;Abdulamid Fakoya&lt;/p&gt;\u0000&lt;p&gt;Abhijit Das&lt;/p&gt;\u0000&lt;p&gt;Abhik Santra&lt;/p&gt;\u0000&lt;p&gt;Abhinav Gupta&lt;/p&gt;\u0000&lt;p&gt;Abhishek Rajhans&lt;/p&gt;\u0000&lt;p&gt;Abhishek Savita&lt;/p&gt;\u0000&lt;p&gt;&lt;i&gt;Abigail Azari&lt;/i&gt;&lt;/p&gt;\u0000&lt;p&gt;Abigail Langston&lt;/p&gt;\u0000&lt;p&gt;Abigail Lute&lt;/p&gt;\u0000&lt;p&gt;Abigail Swann&lt;/p&gt;\u0000&lt;p&gt;Abigail Whittington&lt;/p&gt;\u0000&lt;p&gt;&lt;i&gt;Abigail Williams&lt;/i&gt;&lt;/p&gt;\u0000&lt;p&gt;Abraham Emond&lt;/p&gt;\u0000&lt;p&gt;Abram Jacobson&lt;/p&gt;\u0000&lt;p&gt;Acacia Pepler&lt;/p&gt;\u0000&lt;p&gt;Adam Blaker&lt;/p&gt;\u0000&lt;p&gt;&lt;i&gt;Adam Burnett&lt;/i&gt;&lt;/p&gt;\u0000&lt;p&gt;Adam Clark&lt;/p&gt;\u0000&lt;p&gt;Adam Forte&lt;/p&gt;\u0000&lt;p&gt;Adam Masters&lt;/p&gt;\u0000&lt;p&gt;&lt;i&gt;Adam Povey&lt;/i&gt;&lt;/p&gt;\u0000&lt;p&gt;Adam Scaife&lt;/p&gt;\u0000&lt;p&gt;Adam Schreiner-McGraw&lt;/p&gt;\u0000&lt;p&gt;Adam Smith&lt;/p&gt;\u0000&lt;p&gt;Adam Sobel&lt;/p&gt;\u0000&lt;p&gt;Adam Sokol&lt;/p&gt;\u0000&lt;p&gt;Addison Rice&lt;/p&gt;\u0000&lt;p&gt;&lt;i&gt;Adele Igel&lt;/i&gt;&lt;/p&gt;\u0000&lt;p&gt;Adeline Montlaur&lt;/p&gt;\u0000&lt;p&gt;Ademe Mekonnen&lt;/p&gt;\u0000&lt;p&gt;Adeyemi Adebiyi&lt;/p&gt;\u0000&lt;p&gt;Adina Pusok&lt;/p&gt;\u0000&lt;p&gt;Aditya Gusman&lt;/p&gt;\u0000&lt;p&gt;Aditya Khuller&lt;/p&gt;\u0000&lt;p&gt;&lt;i&gt;Adrià Barbeta&lt;/i&gt;&lt;/p&gt;\u0000&lt;p&gt;Adrian Burd&lt;/p&gt;\u0000&lt;p&gt;Adrián Flores Orozco&lt;/p&gt;\u0000&lt;p&gt;Adrian Grocott&lt;/p&gt;\u0000&lt;p&gt;&lt;i&gt;Adrian Harpold&lt;/i&gt;&lt;/p&gt;\u0000&lt;p&gt;Adrian Martin&lt;/p&gt;\u0000&lt;p&gt;Adrian Matthews&lt;/p&gt;\u0000&lt;p&gt;Adrian Muxworthy&lt;/p&gt;\u0000&lt;p&gt;Adrian Sheppard&lt;/p&gt;\u0000&lt;p&gt;Adrian Tasistro-Hart&lt;/p&gt;\u0000&lt;p&gt;Adrian Tompkins&lt;/p&gt;\u0000&lt;p&gt;Adriano Gualandi&lt;/p&gt;\u0000&lt;p&gt;Adrianus Reniers&lt;/p&gt;\u0000&lt;p&gt;Adrienne Marshall&lt;/p&gt;\u0000&lt;p&gt;Advik Eswaran&lt;/p&gt;\u0000&lt;p&gt;Agnès Borbon&lt;/p&gt;\u0000&lt;p&gt;Agnes Kontny&lt;/p&gt;\u0000&lt;p&gt;Agnes Lim&lt;/p&gt;\u0000&lt;p&gt;Agnese Marcato&lt;/p&gt;\u0000&lt;p&gt;Agniv Sengupta&lt;/p&gt;\u0000&lt;p&gt;Agus Santoso&lt;/p&gt;\u0000&lt;p&gt;Agust Gudmundsson&lt;/p&gt;\u0000&lt;p&gt;Ahmad Ghassemi&lt;/p&gt;\u0000&lt;p&gt;Ahmad Lalti&lt;/p&gt;\u0000&lt;p&gt;Ahmed Elkouk&lt;/p&gt;\u0000&lt;p&gt;Aibing Li&lt;/p&gt;\u0000&lt;p&gt;Aidan Blaser&lt;/p&gt;\u0000&lt;p&gt;Aiguo Dai&lt;/p&gt;\u0000&lt;p&gt;Aihui Wang&lt;/p&gt;\u0000&lt;p&gt;Aiko Voigt&lt;/p&gt;\u0000&lt;p&gt;Aimée Slangen&lt;/p&gt;\u0000&lt;p&gt;Aimin Du&lt;/p&gt;\u0000&lt;p&gt;Aislinn Fox&lt;/p&gt;\u0000&lt;p&gt;Aitaro Kato&lt;/p&gt;\u0000&lt;p&gt;&lt;i&gt;Aixue Hu&lt;/i&gt;&lt;/p&gt;\u0000&lt;p&gt;Ajay Kumar&lt;/p&gt;\u0000&lt;p&gt;&lt;i&gt;Ajay Raghavendra&lt;/i&gt;&lt;/p&gt;\u0000&lt;p&gt;Akash Koppa&lt;/p&gt;\u0000&lt;p&gt;&lt;i&gt;Akira Kuwano-Yoshida&lt;/i&gt;&lt;/p&gt;\u0000&lt;p&gt;Akira Oka&lt;/p&gt;\u0000&lt;p&gt;Akira Yamazaki&lt;/p&gt;\u0000&lt;p&gt;Akiyoshi Wada&lt;/p&gt;\u0000&lt;p&gt;Akshay Deoras&lt;/p&gt;\u0000&lt;p&gt;&lt;i&gt;Akshaya Nikumbh&lt;/i&gt;&lt;/p&gt;\u0000&lt;p&gt;Ala Aldahan&lt;/p&gt;\u0000&lt;p&gt;Alain Pietroniro&lt;/p&gt;\u0000&lt;p&gt;","PeriodicalId":12523,"journal":{"name":"Geophysical Research Letters","volume":"54 1","pages":""},"PeriodicalIF":5.2,"publicationDate":"2026-03-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"147462135","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Inverse Grading Emerges From Particle-Scale Migration Under Seasonal Freeze-Thaw Forcing: Evidence From Multi-Year Monitoring and Physical Modeling 季节性冻融强迫下颗粒尺度迁移产生逆级配:来自多年监测和物理模拟的证据
IF 5.2 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-03-13 DOI: 10.1029/2025gl119590
Weibo Li, Qinglu Deng, Limin Zhang, Pengju An, Xingwei Ren, Xuexue Su, Ruiqiang Bai, Jiren Xie, Li Zeng, Kun Fang
Inverse grading, where coarse particles overlay finer materials, is common on talus slopes, yet its progressive formation under realistic conditions is rarely quantified. We integrate multi-year field observations with controlled freeze-thaw experiments to elucidate the processes driving particle migration that result in inverse grading and slope creep. Data from a talus slope in Northeast China show spatially varied downslope movements (2.0–19 mm/a), seasonal uplift during freezing, and net subsidence upon thawing. Laboratory models reveal systematic sorting: small particles move downward and downslope through expanded pores, while large particles shift and rotate with minimal descent. This vertical mobility contrast (small vs. large displaced by factors of 11–15) results in inverse grading over time. Depth-dependent displacement shows differential deformation, with surface layers moving more than deeper layers. Our findings demonstrate that seasonal particle-scale variations consistently drive talus restructuring, linking granular dynamics to landscape deformation and enhancing risk assessments in cold regions.
逆级配,即粗颗粒覆盖较细的材料,在距骨斜坡上很常见,但其在现实条件下的渐进形成很少被量化。我们将多年的现场观测与控制冻融实验相结合,以阐明驱动颗粒迁移的过程,从而导致反级配和边坡蠕变。东北某坡面数据显示,坡面下移(2.0 ~ 19 mm/a)、冻结期季节性抬升和融化期净沉降具有明显的空间差异。实验室模型显示了系统的分选:小颗粒通过膨胀的孔隙向下和下坡移动,而大颗粒则以最小的下降移动和旋转。这种垂直迁移率的对比(小与大的11-15倍位移)导致了随时间的反向分级。随深度变化的位移表现出不同的变形,表层的位移大于深层。我们的研究结果表明,季节性的颗粒尺度变化持续地驱动着距骨重构,将颗粒动力学与景观变形联系起来,并加强了寒冷地区的风险评估。
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引用次数: 0
Data-Driven Exploration of Tropical Cyclone's Controllability 数据驱动的热带气旋可控性研究
IF 5.2 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-03-13 DOI: 10.1029/2025gl120393
Yohei Sawada, Masashi Minamide, Yuyue Yan, Kazumune Hashimoto, Le Duc
Although the chaotic nature of the atmosphere may enable efficient control of tropical cyclones (TCs) via small-scale perturbations, few studies have proposed data-driven optimization methods to identify such perturbations. Here, we apply the recently proposed Ensemble Kalman Control (EnKC) to a TC simulation. We show that EnKC finds small-scale perturbations that mitigate TC. An EnKC-estimated reduction in surface water vapor, located approximately 250 km from the TC center, suppresses convective activity and latent heat release in the eye wall, leading to a reduction of TC intensity. To advance the discovery of feasible TC mitigation strategies, we discuss the potential of this data-driven method for leveraging chaos, as well as its remaining challenges.
虽然大气的混沌性质可以通过小尺度扰动有效地控制热带气旋,但很少有研究提出数据驱动的优化方法来识别这种扰动。在这里,我们将最近提出的集成卡尔曼控制(EnKC)应用于TC仿真。我们发现EnKC发现小尺度的扰动可以减轻TC。据enkc估计,距离TC中心约250公里处的地表水汽减少,抑制了眼壁的对流活动和潜热释放,导致TC强度降低。为了促进发现可行的TC缓解策略,我们讨论了这种数据驱动方法在利用混乱方面的潜力,以及它仍然存在的挑战。
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引用次数: 0
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Geophysical Research Letters
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