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A Physically Consistent Particle Size Distribution Modeling of the Microphysics of Precipitation for Weather and Climate Models 用于天气和气候模式的降水微物理的物理一致粒度分布模拟
IF 5.2 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-02-11 DOI: 10.1029/2025gl118545
Francisco J. Tapiador, Kyuhee Shin, Livia J. Leganés, Kyo-Sun Lim, Gabriela Juárez, Wonbae Bang, Andrés Navarro, Raúl Martín, Sun-Young Park, GyuWon Lee
The probability density function of drops is difficult to model. Current approaches make assumptions that are often problematic, as they allow negative values for the mean of the distribution. While the statistical goodness of fit of those models might be reasonable for precipitation radar estimation, the situation is unsatisfactory if a fully consistent physical modeling of precipitation across scales is desired. This is the case of weather and climate models. This paper discusses a model that satisfies mathematical and physical consistency. The model can be seamlessly integrated into the parameterizations of the microphysics of precipitation and is tested on an extensive disdrometer data set. Comparison with existing models shows that the new method has substantial practical and theoretical advantages. The research has implications in elucidating the role of clouds in the climate sensitivity of climate models.
水滴的概率密度函数很难建模。目前的方法所做的假设往往是有问题的,因为它们允许分布的平均值为负值。虽然这些模型的统计拟合优度对于降水雷达估计可能是合理的,但如果需要跨尺度降水的完全一致的物理模拟,情况就不令人满意了。这就是天气和气候模型的情况。本文讨论了一个满足数学和物理一致性的模型。该模型可以无缝地集成到降水微物理的参数化中,并在大量的分差仪数据集上进行了测试。与现有模型的比较表明,新方法具有很大的实用和理论优势。该研究有助于阐明云在气候模式的气候敏感性中的作用。
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引用次数: 0
Antarctic Meltwater Accelerates Southern Ocean Evolution Under Projected Atmospheric Warming 在预估的大气变暖下,南极融水加速了南大洋的演变
IF 5.2 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-02-11 DOI: 10.1029/2025gl119952
Irena Vaňková, Matthew Hoffman, Xylar Asay-Davis, Carolyn Branecky Begeman, Darin Comeau, Stephen F. Price, Jonathan Wolfe
Increasing basal meltwater from Antarctic ice shelves may impact the Southern Ocean properties that feed back on the rate of melting. We investigate this feedback in a high-emissions scenario using an Earth-system model with interactive ice-shelf basal melting, an improvement on previous studies that did not have the capability to evolve melt rates and the ocean state self-consistently. We find that when interactive melt increases, it primarily accelerates the evolution of a spatial pattern of continental shelf warming and cooling that is initiated by freshening and sea-ice formation decline due to projected atmospheric warming. The competition between enhanced warming at depth from reduced ventilation and enhanced continental shelf cooling from reduced dense water export leads to net ${sim} $35% reduction in ice-shelf meltwater input into the Southern Ocean over the 21st century. Omitting this feedback introduces a bias in the timing of projected ocean-melt-driven ice loss from Antarctica.
来自南极冰架的基底融水的增加可能会影响南大洋的性质,这些性质对融化速度有反馈作用。我们使用具有相互作用的冰架基底融化的地球系统模型在高排放情景下研究了这种反馈,这是对以前的研究的改进,这些研究没有能力自一致地演变融化速率和海洋状态。我们发现,当相互作用融化增加时,它主要加速了大陆架增温和降温的空间格局的演变,这种格局是由预估的大气变暖导致的新生和海冰形成减少所引发的。由于通风减少导致的深度增温和稠密水输出减少导致的大陆架降温之间的竞争,导致21世纪进入南大洋的冰架融水净减少约35%。忽略这一反馈会在预测由海洋融化引起的南极冰损失的时间上造成偏差。
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引用次数: 0
High-Precision Aftershock Distribution Highlights the Complex Fault Geometry of the 2024 Mw 7.5 Noto Peninsula Earthquake 高精度余震分布凸显了2024年诺托半岛7.5 Mw地震的复杂断层几何形状
IF 5.2 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-02-11 DOI: 10.1029/2025gl118413
Hidenobu Takahashi, Yasuhira Aoyagi, Keisuke Yoshida, Haruo Kimura, Eiji Kurashimo, Shinichi Sakai
We deployed 30 temporary seismic stations around the source region of the 2024 Mw 7.5 Noto Peninsula earthquake to investigate the relationship between mainshock rupture and fault geometry. Using machine learning techniques, we detected and precisely located 46,252 aftershocks, revealing several fault planes corresponding to active faults ruptured during the mainshock. Two subparallel landward-dipping planar structures were identified near the mainshock hypocenter, converging westward to the Wajima-Oki segment. This geometry suggests that complex rupture episodes near the hypocenter resulted from successive ruptures on adjacent fault planes rather than slip on a single plane. At the western edge of the 2024 rupture area, aftershocks extend close to but rarely occur on the fault that ruptured during the 2007 Mw 6.7 earthquake, suggesting that the 2024 earthquake did not re-rupture the same faults of the 2007 earthquake.
我们在2024年诺托半岛7.5 Mw地震的震源区周围部署了30个临时地震台站,以研究主震破裂与断层几何形状之间的关系。利用机器学习技术,我们检测并精确定位了46,252次余震,揭示了主震期间活动断层破裂的几个断层面。在主震震源附近发现了两个近平行的向陆倾平面构造,向西汇聚到和岛-冲段。这种几何形状表明,震源附近的复杂破裂事件是由相邻断层面的连续破裂造成的,而不是单一断层面的滑动。在2024年断裂带的西部边缘,余震向2007年Mw 6.7地震破裂的断层附近延伸,但很少发生,这表明2024年地震没有再次破裂2007年地震的同一断层。
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引用次数: 0
Diverging Spring Warming and Growing Season Shifts Across Eurasia and North America Under Future Climate 在未来气候下欧亚大陆和北美的春季暖季和生长期变化
IF 4.6 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-02-11 DOI: 10.1029/2025GL120295
Shuzhen Hu, Lu Wang, Tianjun Zhou, Pang-Chi Hsu, Xiaolong Chen

Springtime warming over Northern Mid-High-latitude Land profoundly affects plant life cycles and water resources, yet large model uncertainty limits climate risk assessment. Here, we develop a novel emergent constraint that targets the key uncertainty source—model divergence in surface-albedo feedback linked to historical snowmelt sensitivity. This approach halves the spread of projected warming and reveals a pronounced geographical asymmetry. Under the high-emission scenario (SSP5-8.5), current climate models underestimate end-of-century warming over Eurasia by 0.80°C but overestimate it over North America by 0.44°C. These refined projections substantially alter ecological outcomes: the start of the growing season is predicted to advance by about 18 days in Eurasia and 8 days in North America, representing a 3-day greater advance and 1-day delay compared with original estimates. Our findings offer a more reliable basis for assessing climate change impacts on ecosystems and water resources and highlight the urgency of region-specific adaptation strategies.

北部中高纬度地区春季变暖深刻影响植物生命周期和水资源,但较大的模式不确定性限制了气候风险评估。在这里,我们开发了一个新的紧急约束,目标是与历史融雪敏感性相关的地表反照率反馈中的关键不确定性源模型发散。这种方法将预估变暖的范围减半,并显示出明显的地理不对称性。在高排放情景(SSP5-8.5)下,目前的气候模式将欧亚大陆的世纪末变暖低估了0.80℃,而将北美的世纪末变暖高估了0.44℃。这些改进后的预测结果大大改变了生态结果:预计欧亚大陆和北美的生长期开始时间分别提前约18天和8天,与最初的估计相比,提前了3天,推迟了1天。我们的研究结果为评估气候变化对生态系统和水资源的影响提供了更可靠的基础,并强调了制定特定区域适应战略的紧迫性。
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引用次数: 0
Tide-Modulated Ocean-to-Earth Energy Conversion Quantified With Coastal Fiber Sensing 潮汐调制海洋到地球的能量转换量化与海岸光纤传感
IF 5.2 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-02-11 DOI: 10.1029/2025gl120302
Justin Yen-Ting Ko, Kun-Chi Ho, Chun-Hung Lin, Hsin-Hua Huang, Ho-Han Hsu, Chen-Fen Huang, Hao Kuo-Chen, Hou-Sheng Cheng, Yao Hsu, En-Shi Wu, Hsi-An Chen, Yu-Fang Ma, Hung-Yi Wu, Po-Yin Lin, Yu-Hsian Chen, Wei-Jong Tien, Bo-Yu Siao, Hui-Yu Wu
Quantifying how incident ocean waves transfer energy into seismic surface waves along the nearshore is essential for understanding coastal hazards and Earth–ocean coupling, yet time-resolved in situ estimates have been scarce. Here we use a beach-deployed distributed acoustic sensing array co-located with an ocean-bottom node to directly measure the conversion efficiency from wave impacts to Rayleigh-type ground motion at 4–12 Hz. Frequency–wavenumber analysis, beamforming, and local back-projection consistently locate sources along a fixed, wave-breaking coastal segment, while particle-motion ellipticity confirms the Rayleigh character. Calibrating distributed acoustic sensing strain to ground velocity and combining nearshore wave energetics yields an energy-conversion efficiency on the order of 10−6. The efficiency is strongly modulated by tide, with high-tide conditions enhancing coupling even though the source region remains stationary. Our results establish a quantitative benchmark for dynamic ocean-to-Earth energy transfer at the land–sea interface and provide a generalizable framework for coastal monitoring using existing fiber infrastructure.
量化入射海浪如何沿近岸将能量转化为地震表面波对于了解海岸灾害和地球-海洋耦合至关重要,但时间分辨的原位估计很少。在这里,我们使用海滩部署的分布式声传感阵列与海底节点共同定位,直接测量从波浪冲击到4-12 Hz瑞利型地面运动的转换效率。频率波数分析、波束形成和局部反向投影一致地沿固定的破碎海岸段定位源,而粒子运动椭圆性证实了瑞利特征。将分布式声传感应变与地面速度校准,并结合近岸波能量学,可以得到10−6量级的能量转换效率。效率受潮汐的强烈调制,即使源区保持平稳,高潮条件也会增强耦合。我们的研究结果为陆地-海洋界面的动态海洋-地球能量转移建立了定量基准,并为利用现有光纤基础设施进行沿海监测提供了一个可推广的框架。
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引用次数: 0
Early to Mid-Holocene Cool Temperature-Induced Drought in Asian Interior 早至中全新世亚洲内陆的低温干旱
IF 5.2 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-02-11 DOI: 10.1029/2025gl121126
Jiawei Jiang, Huanye Wang, Hu Liu, Guoqiang Chu, Weiguo Liu, Sergey Krivonogov, Zhonghui Liu
Hydroclimatic variations in mid-latitude Asia during the early to mid-Holocene and associated mechanisms remain disputed, hampering our understanding of atmospheric circulation controls on regional climatic changes. We report Holocene alkenone records from two Siberian lakes, documenting lake temperature and hydrological changes, and synthesize records from mid-latitude Asia to address regional hydroclimatic variability. Relatively dry conditions occurred in westerlies-dominated regions and extended to marginal monsoon regions before ∼6,000 a BP, followed by wetting transitions during ∼6,000–5,000 a BP, despite contrasting temperature variations between two regions. We suggest that early to mid-Holocene drought in mid-latitude Asian interior appears to be associated with enhanced anticyclonic system over mid-high latitude Eurasian continent, induced by prevailing cold airmasses, which extended its hydrological control to marginal monsoon regions. Our findings explain the spatial heterogeneity of hydrological changes in mid-latitude Asia, and opposite temperature-moisture associations within westerlies-dominated and marginal monsoon regions during the early to mid-Holocene.
全新世早期至中期亚洲中纬度地区的水文气候变化及其相关机制仍存在争议,阻碍了我们对大气环流控制区域气候变化的认识。我们报告了两个西伯利亚湖泊的全新世烯烃记录,记录了湖泊温度和水文变化,并综合了亚洲中纬度地区的记录,以解决区域水文气候变率问题。在~ 6000 a BP之前,相对干燥的条件发生在西风带为主的地区,并扩展到边缘季风区,随后在~ 6000 - 5000 a BP期间发生湿润转变,尽管两个地区之间的温度变化存在差异。我们认为,早至中全新世亚洲内陆地区的干旱可能与中高纬度欧亚大陆的反气旋系统增强有关,该系统由盛行的冷气团引起,并将其水文控制扩展到边缘季风区。我们的研究结果解释了全新世早期至中期亚洲中纬度地区水文变化的空间异质性,以及西风带和边缘季风区相反的温度-湿度关联。
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引用次数: 0
Why Firn Quakes 为什么会发生地震
IF 4.6 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-02-11 DOI: 10.1029/2025GL120644
A. Voigtländer, B. Gee

Snow dampens sounds, but anecdotal reports concisely describe audible propagating collapse events—firnquakes—in Antarctic and Arctic snowfields. We propose combining granular and continuum mechanics to form a testable theory for conditioning, triggering, and propagation of firnquakes consistent with scarce data. A central condition for collapse events is unconsolidated firn at depth. As firn grains compact, stresses are transmitted along force chains which carry the overburden and transition into a continuous medium by pressure sintering. This granular legacy creates solid-like supports of denser layers that keep the material below unconsolidated. Dynamic amplification triggers local brittle failure of the supports, which induces a cascade of collapse propagation. Using bulk density from ice cores as proxy for stiffness, we find the flexural wave speed by collapsing supports matches the recorded firnquake velocities on the order of 100 m/s. Our theory is to be tested in firn sheets and other compacting granular materials.

雪会抑制声音,但坊间报道简洁地描述了在南极和北极雪原中传播的崩塌事件——地震。我们建议结合颗粒力学和连续介质力学,形成一个与稀缺数据一致的地震条件、触发和传播的可测试理论。塌陷事件的一个中心条件是深度未固结的坚固性。当坚硬晶粒压实时,应力沿着力链传递,力链携带覆岩,并通过压力烧结转变为连续介质。这种颗粒状的遗产形成了致密层的固体状支撑,使下面的材料保持不固结。动力放大触发了支护的局部脆性破坏,引发了一连串的破坏传播。利用冰芯的体积密度作为刚度的代表,我们发现坍塌支架的弯曲波速与记录的地震速度相匹配,大约为100米/秒。我们的理论将在钢板和其他压实颗粒材料中进行试验。
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引用次数: 0
New Cretaceous Paleomagnetic and Geochronologic Data From the Antarctic Peninsula: Constraints on the Pre-Opening Tectonic Evolution of the Drake Passage 南极半岛新白垩世古地磁和地质年代学资料:对德雷克海峡开放前构造演化的制约
IF 5.2 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-02-11 DOI: 10.1029/2025gl120389
Liang Gao, Xinwei Hu, Mengwei Zhang, Xiaoqian Guo, Junling Pei, Zhenyu Yang, Yue Zhao
Reconstructing oroclinal orogens along the Fuegian Andes-northern Antarctic Peninsula provides critical constraints on the pre-opening tectonic evolution of the Drake Passage, although such efforts are limited by a lack of reliable Cretaceous paleomagnetic and geochronological data. Here, we present new paleomagnetic, 40Ar/39Ar, and apatite U-Pb geochronological data to reconstruct the oroclinal bending of this belt. Our results reveal that oroclinal bending in the northern Antarctic Peninsula (∼67°–63°S) and the Fuegian Andes both occurred at ∼100–90 Ma, mainly driven by compression from the northward-moving Antarctic Peninsula and southeastward-moving Cordillera Darwin Metamorphic Complex. We propose that the orocline Drake Passage boundary primarily formed during this period. This oroclinal weak zone served as a fundamental prerequisite in opening the Drake Passage, facilitating the separation of the Fuegian Andes and Antarctic Peninsula.
重建沿fugegian Andes-northern Antarctic Peninsula的造山带为研究Drake通道打开前的构造演化提供了关键的约束条件,尽管这种努力受到缺乏可靠的白垩纪古地磁和地质年代学数据的限制。在此,我们利用新的古地磁、40Ar/39Ar和磷灰石U-Pb年代学数据来重建该带的造山带弯曲。我们的研究结果表明,南极半岛北部(~ 67°-63°S)和fugeian Andes都发生在~ 100-90 Ma,主要由向北移动的南极半岛和东南移动的Cordillera Darwin变质杂岩的压缩驱动。我们认为,这一时期形成了主要的欧斜德雷克海峡边界。这个斜顶弱带是打开德雷克海峡的基本先决条件,促进了斐济安第斯山脉和南极半岛的分离。
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引用次数: 0
Seasonal to Interannual Cross-Scale Energy Transfer Variability: Observational Insight From the Santa Barbara Channel 季节到年际跨尺度能量传输变率:来自圣巴巴拉海峡的观测见解
IF 4.6 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-02-11 DOI: 10.1029/2025GL117885
Sara Taylor, Andrew F. Thompson, Luke Kachelein, Patrice Klein

Kinetic energy (KE) transfer between spatial scales contributes to the ocean's energy budget by linking scales of KE supply and KE dissipation. Numerical simulations have indicated that for scales smaller than the baroclinic deformation radius, cross-scale KE transfer has complex spatial and temporal variability, modulated by mixed layer properties, fronts, and eddies. Here, over a decade of upper-ocean surface velocity data, collected from high-frequency radar within the Santa Barbara Channel, are used to estimate cross-scale KE transfer. The transfer of KE across 7 km has strong seasonal and interannual variations linked to energy exchange with the atmosphere. This study observationally confirms (a) the importance of the surface divergence field in determining the direction of the KE transfer and (b) the equi-partitioning of KE transfer between divergent and straining motions. The temporal variability in KE transfer suggests that surface forcing influences the long-term redistribution of energy between scales.

动能在空间尺度上的传递通过连接动能供给和动能耗散的尺度,对海洋的能量收支有贡献。数值模拟结果表明,在小于斜压变形半径的尺度上,跨尺度KE传输具有复杂的时空变异性,受混合层性质、锋面和涡旋的调制。在这里,使用从圣巴巴拉海峡内的高频雷达收集的十多年的上层海洋表面速度数据来估计跨尺度的KE传输。在与大气的能量交换过程中,穿越7 km的能量转移具有强烈的季节和年际变化。该研究通过观测证实了(a)表面散度场在确定KE传递方向方面的重要性,以及(b) KE传递在发散运动和应变运动之间的均匀分配。能量转移的时间变异性表明,地表强迫影响尺度间能量的长期再分配。
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引用次数: 0
Martian Atmospheric Loss Through Foreshock Transient Events 火星大气损失通过前震瞬态事件
IF 5.2 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2026-02-11 DOI: 10.1029/2025gl120618
Alexandros C. Cooke-Politikos, Sergey Shuvalov, Yaxue Dong, Yi Qi, David A. Brain, Jasper S. Halekas
At Mars, the MAVEN spacecraft has made observations of Hot Flow Anomalies (HFAs) in the foreshock. Due to the bow shock's proximity to the planet, it is theorized that HFAs contribute to atmospheric escape at Mars through the excavation of ionospheric ions. A case study investigates one HFA observation, with parameters suggesting a novel mechanism for planetary ion extraction. The event is further characterized by elevated number densities of <span data-altimg="/cms/asset/1a45c7bf-c36a-4bab-b8fb-e19131ab5516/grl72041-math-0001.png"></span><mjx-container ctxtmenu_counter="133" ctxtmenu_oldtabindex="1" jax="CHTML" role="application" sre-explorer- style="font-size: 103%; position: relative;" tabindex="0"><mjx-math aria-hidden="true" location="graphic/grl72041-math-0001.png"><mjx-semantics><mjx-mrow><mjx-mrow><mjx-msup data-semantic-children="0,1" data-semantic- data-semantic-role="latinletter" data-semantic-speech="normal upper O Superscript plus" data-semantic-type="superscript"><mjx-mi data-semantic-annotation="clearspeak:simple" data-semantic-font="normal" data-semantic- data-semantic-parent="2" data-semantic-role="latinletter" data-semantic-type="identifier"><mjx-c></mjx-c></mjx-mi><mjx-script style="vertical-align: 0.363em;"><mjx-mo data-semantic- data-semantic-parent="2" data-semantic-role="addition" data-semantic-type="operator" size="s"><mjx-c></mjx-c></mjx-mo></mjx-script></mjx-msup></mjx-mrow></mjx-mrow></mjx-semantics></mjx-math><mjx-assistive-mml display="inline" unselectable="on"><math altimg="urn:x-wiley:00948276:media:grl72041:grl72041-math-0001" display="inline" location="graphic/grl72041-math-0001.png" xmlns="http://www.w3.org/1998/Math/MathML"><semantics><mrow><mrow><msup data-semantic-="" data-semantic-children="0,1" data-semantic-role="latinletter" data-semantic-speech="normal upper O Superscript plus" data-semantic-type="superscript"><mi data-semantic-="" data-semantic-annotation="clearspeak:simple" data-semantic-font="normal" data-semantic-parent="2" data-semantic-role="latinletter" data-semantic-type="identifier" mathvariant="normal">O</mi><mo data-semantic-="" data-semantic-parent="2" data-semantic-role="addition" data-semantic-type="operator">+</mo></msup></mrow></mrow>${mathrm{O}}^{+}$</annotation></semantics></math></mjx-assistive-mml></mjx-container> and <span data-altimg="/cms/asset/3f883c89-45a8-4785-94e5-474c2fc4584c/grl72041-math-0002.png"></span><mjx-container ctxtmenu_counter="134" ctxtmenu_oldtabindex="1" jax="CHTML" role="application" sre-explorer- style="font-size: 103%; position: relative;" tabindex="0"><mjx-math aria-hidden="true" location="graphic/grl72041-math-0002.png"><mjx-semantics><mjx-mrow><mjx-mrow><mjx-msubsup data-semantic-children="0,1,2" data-semantic-collapsed="(4 (3 0 1) 2)" data-semantic- data-semantic-role="latinletter" data-semantic-speech="normal upper O 2 Superscript plus" data-semantic-type="subsup"><mjx-mi data-semantic-annotation="clearspeak:simple" data-semantic-font="normal" data-semanti
在火星上,MAVEN宇宙飞船观测到了前震中的热流异常(hfa)。由于弓形激波靠近火星,理论上hfa通过挖掘电离层离子有助于火星的大气逃逸。一个案例研究调查了一次HFA观测,其参数表明行星离子提取的新机制。该事件的进一步特征是在电流片交叉之前观察到的O+${mathrm{O}}^{+}$和O2+${mathrm{O}}_{2}^{+}$离子的数量密度升高。对一组91个事件进行了统计研究,使火星上HFA的频率估计为1次/天。该事件的估计离子逸出率约为火星标称条件下典型离子逸出率的9%。对进一步事件的计算表明,名义条件的逃逸率在1%到9%之间。这代表了对整体逃逸的适度贡献,突出了一条潜在的未被探索的途径。
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Geophysical Research Letters
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