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CO2 Emissions Estimate From Mexico City Using Ground- and Space-Based Remote Sensing 利用地面和空间遥感估算墨西哥城的二氧化碳排放量
IF 3.8 2区 地球科学 Q2 METEOROLOGY & ATMOSPHERIC SCIENCES Pub Date : 2024-10-25 DOI: 10.1029/2024JD041297
Ke Che, Thomas Lauvaux, Noemie Taquet, Wolfgang Stremme, Yang Xu, Carlos Alberti, Morgan Lopez, Agustín García-Reynoso, Philippe Ciais, Yi Liu, Michel Ramonet, Michel Grutter
<p>The Mexico City Metropolitan Area (MCMA) stands as one of the most densely populated urban regions globally. To quantify the urban <span></span><math> <semantics> <mrow> <msub> <mtext>CO</mtext> <mn>2</mn> </msub> </mrow> <annotation> ${text{CO}}_{2}$</annotation> </semantics></math> emissions in the MCMA, we independently assimilated observations from a dense column-integrated Fourier transform infrared (FTIR) network and OCO-3 Snapshot Area Map observations between October 2020 and May 2021. Applying a computationally efficient analytical Bayesian inversion technique, we inverted for surface fluxes at high spatio-temporal resolutions (1-km and 1-hr). The fossil fuel (FF) emission estimates of 5.08 and 6.77 Gg<span></span><math> <semantics> <mrow> <msub> <mtext>CO</mtext> <mn>2</mn> </msub> </mrow> <annotation> ${text{CO}}_{2}$</annotation> </semantics></math>/hr reported by the global and local emission inventories were optimized to 4.85 and 5.51 Gg<span></span><math> <semantics> <mrow> <msub> <mtext>CO</mtext> <mn>2</mn> </msub> </mrow> <annotation> ${text{CO}}_{2}$</annotation> </semantics></math>/hr based on FTIR observations over this 7 month period, highlighting a convergence of posterior estimates. The modeled biogenic flux estimate of −0.14 Gg<span></span><math> <semantics> <mrow> <msub> <mtext>CO</mtext> <mn>2</mn> </msub> </mrow> <annotation> ${text{CO}}_{2}$</annotation> </semantics></math>/hr was improved to −0.33 to −0.27 Gg<span></span><math> <semantics> <mrow> <msub> <mtext>CO</mtext> <mn>2</mn> </msub> </mrow> <annotation> ${text{CO}}_{2}$</annotation> </semantics></math>/hr, respectively. It is worth noting that utilizing observations from three primary sites significantly enhanced the accuracy of estimates (13.6 <span></span><math> <semantics> <mrow> <mo>∼</mo> </mrow> <annotation> ${sim} $</annotation> </semantics></math> 29.2%) around the other four. Using FTIR posterior estimates can improve simulation with the OCO-3 data set. OCO-3 shows a similar decreasing trend
墨西哥城大都市区(MCMA)是全球人口最稠密的城市地区之一。为了量化墨西哥城都会区的城市 CO 2 ${text{CO}}_{2}$ 排放量,我们独立同化了 2020 年 10 月至 2021 年 5 月期间密集的列积分傅立叶变换红外(FTIR)网络观测数据和 OCO-3 快照区域图观测数据。我们采用计算高效的贝叶斯分析反演技术,对高时空分辨率(1 公里和 1 小时)的地表通量进行了反演。根据这7个月期间的傅立叶变换红外观测数据,全球和地方排放清单报告的化石燃料(FF)排放量估计值分别为5.08和6.77千兆克CO 2 ${text{CO}}_{2}$ /小时,优化后分别为4.85和5.51千兆克CO 2 ${text{CO}}_{2}$ /小时,凸显了后验估计值的趋同。模拟的生物通量估计值-0.14 千兆克 CO 2 ${text{CO}}_{2}$ /小时分别提高到-0.33 到-0.27 千兆克 CO 2 ${text{CO}}_{2}$ /小时。值得注意的是,利用三个主要观测点的观测数据大大提高了其他四个观测点的估计精度(13.6 ∼ ${sim} $ 29.2%)。使用傅立叶变换红外后验估计值可以改进对 OCO-3 数据集的模拟。OCO-3 显示了与 FTIR 相似的 FF 排放下降趋势(从 6.37 千兆克 CO 2 ${text{CO}}_{2}$ /小时下降到 6.36 和 5.04 千兆克 CO 2 ${text{CO}}_{2}$ /小时),但其生物源修正趋势不同,从 0.37 千兆克 CO 2 ${text{CO}}_{2}$ /小时变化到 0.48 千兆克 CO 2 ${text{CO}}_{2}$ /小时。主要原因是 OCO-3 的时间采样密度较低。将傅立叶变换红外反演时间与 OCO-3 的反演时间相一致,可以得到类似的傅立叶排放修正,但生物源排放的差异仍然存在,这可能是由于它们在农村地区的采样位置不同以及 X CO 2 ${text{CO}}_{2}$ 观测结果的差异造成的。我们的发现标志着向验证大都市地区的 OCO-3 和傅立叶变换反演结果迈出了重要一步。
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引用次数: 0
Contrasting Domestic and Global Impacts of Emission Reductions in China on Tropospheric Ozone 中国减排对对流层臭氧的国内和全球影响对比
IF 3.8 2区 地球科学 Q2 METEOROLOGY & ATMOSPHERIC SCIENCES Pub Date : 2024-10-25 DOI: 10.1029/2024JD041453
Han Han, Lin Zhang, Xiaolin Wang, Xiao Lu

Sustained near-surface ozone pollution despite stringent emission controls in China has drawn wide attention. However, how such rapid regional emission reductions affect global tropospheric ozone remains unexplored. Here, using an ensemble of measurements and global model simulations, we find Chinese emission reductions during 2013–2020 have increased domestic surface ozone; particularly in North China, they have decreased the global tropospheric ozone burden by 2.7 Tg (54% of China's anthropogenic contribution and 7% of global anthropogenic contribution in 2019) and ozone radiative forcing by 8.8 mW m−2 (64% of China's anthropogenic contribution and 9% of global anthropogenic contribution in 2019). Nitrogen oxides (NOx) associated nonlinear chemistry and height-dependent atmospheric transport patterns primarily cause the contrasting impacts. Future Chinese NOx emission controls would continue to decrease global tropospheric ozone, while regional surface ozone may still increase unless NOx reductions exceed ∼53% of the 2019 level. Our results reveal the substantial benefit of regional emission reductions in China on global tropospheric ozone mitigation.

尽管中国采取了严格的排放控制措施,但持续的近地表臭氧污染仍引起了广泛关注。然而,这种快速的区域减排如何影响全球对流层臭氧仍未得到探讨。在此,我们利用一系列测量数据和全球模型模拟,发现中国在 2013-2020 年期间的减排增加了国内地表臭氧;尤其是在华北地区,减排使全球对流层臭氧负荷减少了 2.7 Tg(占中国人为贡献的 54%,2019 年占全球人为贡献的 7%),臭氧辐射强迫减少了 8.8 mW m-2(占中国人为贡献的 64%,2019 年占全球人为贡献的 9%)。氮氧化物(NOx)相关的非线性化学性质和高度依赖性大气传输模式是造成对比影响的主要原因。未来中国的氮氧化物排放控制将继续减少全球对流层臭氧,而区域地表臭氧仍可能增加,除非氮氧化物减排量超过 2019 年水平的 53%。我们的研究结果揭示了中国区域减排对全球对流层臭氧减缓的巨大益处。
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引用次数: 0
Numerical Insights Into Gobi Wind-Blown Sand: Deriving a Saltation Flux Scheme 戈壁风吹沙的数值洞察:盐化通量方案的推导
IF 3.8 2区 地球科学 Q2 METEOROLOGY & ATMOSPHERIC SCIENCES Pub Date : 2024-10-25 DOI: 10.1029/2024JD041398
C. Zhang, Y. Wang, N. Huang, H. C. Dun

Dust emissions from land-air interaction in arid and semi-arid regions are crucial for predicting the global dust cycle. However, a comprehensive understanding of the complex physical mechanisms contributing to dust emissions from Gobi surfaces remains elusive. The expansive Gobi Desert, spanning northern China and Mongolia, significantly intensifies sandstorms in East Asia. Although researchers use models to study global dust transport, current models primarily depend on the aerodynamic roughness of the Gobi Desert. They often overlook the particle-bed collision processes unique to the Gobi bed surface, which differ significantly from those of desert surfaces, thus compromising the accuracy of global dust cycle simulations. In this article, we establish a numerical model for drift sand in the Gobi based on existing theoretical and experimental studies. The model accurately simulates the wind-blown sand in the Gobi and been used to investigate the saltation structure of sand transport. Simulations reveal an exponential decay of mass concentration with height, with an average attenuation rate of 0.00385 in the Gobi compared to 0.00806 in sandy deserts. The horizontal velocity of saltating particles increases with height following a power law. Through quantitative analysis of this structure, we present a saltation flux formula suitable for the Gobi.

干旱和半干旱地区陆气相互作用产生的尘埃排放对预测全球尘埃循环至关重要。然而,对导致戈壁表面沙尘排放的复杂物理机制的全面了解仍然遥不可及。横跨中国北部和蒙古的广袤戈壁滩极大地加剧了东亚地区的沙尘暴。尽管研究人员使用模型来研究全球沙尘传输,但目前的模型主要依赖于戈壁滩的空气动力学粗糙度。它们往往忽略了戈壁床面特有的颗粒-床面碰撞过程,而这一过程与沙漠表面的碰撞过程有很大不同,从而影响了全球沙尘循环模拟的准确性。本文在现有理论和实验研究的基础上,建立了戈壁流沙的数值模型。该模型准确地模拟了戈壁中的风吹流沙,并用于研究流沙传输的盐化结构。模拟结果表明,质量浓度随高度呈指数衰减,戈壁中的平均衰减率为 0.00385,而沙漠中的平均衰减率为 0.00806。盐化粒子的水平速度随高度增加,呈幂律上升。通过对这一结构的定量分析,我们提出了适合戈壁的盐化通量公式。
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引用次数: 0
Predictability of the 2020 Strong Vortex in the Antarctic Stratosphere and the Role of Ozone 2020 年南极平流层强漩涡的可预测性和臭氧的作用
IF 3.8 2区 地球科学 Q2 METEOROLOGY & ATMOSPHERIC SCIENCES Pub Date : 2024-10-24 DOI: 10.1029/2024JD040820
Eun-Pa Lim, Linjing Zhou, Griffith Young, S. Abhik, Irina Rudeva, Pandora Hope, Matthew C. Wheeler, Julie M. Arblaster, Harry H. Hendon, Gloria L. Manney, Seok-Woo Son, Jiyoung Oh, René D. Garreaud

The Antarctic vortex of October–December 2020 was the strongest on record in the satellite era for the season in the mid- to lower stratosphere. However, it was poorly predicted by the Australian Bureau of Meteorology's operational seasonal climate forecast system of that time, ACCESS-S1, even at a short lead time of a month. Using the current operational forecast system, ACCESS-S2, we have, therefore, tried to find a primary cause of the limited predictability of this event and conducted forecast sensitivity experiments to understand the potential role of ozone in the event and its associated anomalies of the Southern Annular Mode (SAM) and rainfall over south–eastern Australia and western Patagonia. Here, we show that the 2020 strong vortex event did not follow the canonical dynamical evolution seen in previous strong vortex events in spring but suddenly appeared as a result of the record-low upward propagating wave activity in September 2020. The ACCESS-S2 forecasts significantly underestimated the negative wave forcing in September even at zero lead time, irrespective of the ozone configuration, therefore falling short in predicting the record strength of the polar vortex in late spring 2020. Nevertheless, ACCESS-S2 with prescribed realistic ozone that had large anomalies in the Antarctic stratosphere significantly better predicted the strong vortex and the subsequent positive SAM and related rainfall anomalies over south–eastern Australia and western Patagonia in the austral summer of 2020–21. This highlights the potentially important role of ozone variations for seasonal climate forecasting as a source of long-lead predictability.

2020 年 10 月至 12 月的南极漩涡是卫星时代平流层中下层最强的季节。然而,澳大利亚气象局当时的季节性气候业务预报系统 ACCESS-S1 对其预测不佳,即使在一个月的短时间内也是如此。因此,我们利用当前的业务预报系统 ACCESS-S2,试图找到导致这一事件可预测性有限的主要原因,并进行了预报敏感性实验,以了解臭氧在这一事件中的潜在作用,以及与之相关的澳大利亚东南部和巴塔哥尼亚西部的南环流模式(SAM)和降雨异常。在这里,我们表明 2020 年的强涡旋事件并没有遵循以往春季强涡旋事件中的典型动力学演变过程,而是由于 2020 年 9 月创纪录的低向上传播波活动而突然出现的。ACCESS-S2 预测大大低估了 9 月份的负波动力,即使在零准备时间内也是如此,与臭氧配置无关,因此未能预测出 2020 年春末创纪录的极地涡旋强度。尽管如此,ACCESS-S2 在南极平流层有较大异常的情况下,使用规定的现实臭氧,明显更好地预测了 2020-21 年澳大利亚东南部和巴塔哥尼亚西部夏季的强漩涡以及随后的正 SAM 和相关降雨异常。这凸显了臭氧变化作为长期可预测性来源在季节性气候预测中的潜在重要作用。
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引用次数: 0
Aerosol Vertical Turbulent Mass Flux Retrievals Through Novel Remote Sensing Algorithm 通过新型遥感算法检索气溶胶垂直湍流质量通量
IF 3.8 2区 地球科学 Q2 METEOROLOGY & ATMOSPHERIC SCIENCES Pub Date : 2024-10-24 DOI: 10.1029/2023JD040322
Ajmal Rasheeda Satheesh, Markus D. Petters, Nicholas Meskhidze

Integrated measurements of aerosol, radiation, cloud, and turbulent transport in the planetary boundary layer (PBL) are essential for understanding and modeling climate and air quality. Here, we developed a new technique for the identification of convective turbulent regions and deriving the vertical distribution of aerosol turbulent mass fluxes within PBL. The algorithm uses retrievals from coherent Doppler lidars and a high spectral resolution lidar. The technique was applied to study particle mass fluxes over 2 months (November–December 2020) during the campaign conducted at the DOE Atmospheric Radiation Measurement Southern Great Plains (SGP) site in Lamont, Oklahoma. The algorithm developed here is capable of continuously deriving vertically resolved (curtains) aerosol mass fluxes. Our data analysis shows that at the site, the 30-min averaged fluxes at 135 m above the surface were mainly positive (upward) at ∼1 μg m−2 s−1, suggesting that the surface is the primary source of the particle mass supplied to the boundary layer at the SGP site. Analyses of the individual case studies have revealed that not all the derived fluxes can be linked to surface emissions. Both positive and negative values in a range of ±5 μg m−2 s−1 can be caused by convective thermals interacting between the residual layer and the mixed layer and by rotation of the horizontal wind with the height. Large erroneous negative fluxes can also be caused by drizzling/precipitating clouds. We anticipate that the application of the current technique will lead to a more realistic representation of aerosol mass budgets and bidirectional mixing rates.

行星边界层(PBL)中气溶胶、辐射、云和湍流传输的综合测量对于理解和模拟气候和空气质量至关重要。在此,我们开发了一种新技术,用于识别对流湍流区域,并推导出行星边界层内气溶胶湍流质量通量的垂直分布。该算法使用相干多普勒激光雷达和高光谱分辨率激光雷达的检索结果。在俄克拉荷马州拉蒙特的能源部大气辐射测量南部大平原(SGP)站点开展的活动中,该技术被用于研究为期两个月(2020 年 11 月至 12 月)的粒子质量通量。这里开发的算法能够连续得出垂直分辨(帘)气溶胶质量通量。我们的数据分析显示,在该站点,距地表 135 米处的 30 分钟平均通量主要为正值(向上),为 ∼1 μg m-2 s-1,这表明地表是 SGP 站点边界层颗粒质量的主要来源。对个别案例研究的分析表明,并非所有得出的通量都与地表排放有关。在 ±5 μg m-2 s-1 范围内的正值和负值都可能是由残余层和混合层之间相互作用的对流热气流以及水平风随高度旋转造成的。大量错误的负通量也可能是由细雨/沉淀云造成的。我们预计,当前技术的应用将使气溶胶质量预算和双向混合率得到更真实的呈现。
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引用次数: 0
Implementation of WRF-Urban Asymmetric Convective Model (UACM) for Simulating Urban Fog Over Delhi, India 实施 WRF-城市非对称对流模型(UACM)模拟印度德里上空的城市大雾
IF 3.8 2区 地球科学 Q2 METEOROLOGY & ATMOSPHERIC SCIENCES Pub Date : 2024-10-24 DOI: 10.1029/2024JD040760
Utkarsh Prakash Bhautmage, Sachin D. Ghude, Avinash N. Parde, Harsh G. Kamath, Narendra Gokul Dhangar, Jonathan Pleim, Michael Mau Fung Wong, Sandeep Wagh, Rakesh Kumar, Dev Niyogi, M. Rajeevan

Accurate fog prediction in densely urbanized cities poses a challenge due to the complex influence of urban morphology on meteorological conditions in the urban roughness sublayer. This study implemented a coupled WRF-Urban Asymmetric Convective Model (WRF-UACM) for Delhi, India, integrating explicit urban physics with Sentinel-updated USGS land-use and urban morphological parameters derived from the UT-GLOBUS dataset. When evaluated against the baseline Asymmetric Convective Model (WRF-BACM) using Winter Fog Experiment (WiFEX) data, WRF-UACM significantly improved urban meteorological variables such as diurnal variations in 10-m wind speed, 2-m air temperature (T2), and 2-m relative humidity (RH2) during a fog event. UACM also demonstrates improved accuracy in simulating temperature and significantly reducing biases for wind speed and daytime RH2 under clear sky conditions. UACM reproduced the nighttime urban heat island effect within the city, showing realistic diurnal heating and cooling patterns that are important for accurate fog onset and duration. UACM effectively predicts the onset, evolution, and dissipation of fog, aligning well with observed data and satellite imagery. Compared to WRF-BACM, WRF-UACM reduces the cold bias soon after sunset, thus improving the fog onset error by ∼3 hr. This study highlights the UACM's potential to improve fog prediction and its application in operational settings. With further investigation into different fog types, the UACM can provide crucial insights for preventive measures and reducing disruptions in urban areas.

由于城市形态对城市粗糙度子层气象条件的复杂影响,在城市化密集的城市中进行准确的雾预测是一项挑战。本研究针对印度德里实施了 WRF-城市非对称对流耦合模型(WRF-UACM),将显式城市物理学与哨兵更新的 USGS 土地利用和从 UT-GLOBUS 数据集获得的城市形态参数进行了整合。在使用冬季大雾实验(WiFEX)数据与基准非对称对流模型(WRF-BACM)进行评估时,WRF-UACM 显著改善了城市气象变量,如大雾事件中 10 米风速、2 米气温 (T2) 和 2 米相对湿度 (RH2) 的昼夜变化。UACM 还提高了模拟温度的精度,并显著减少了晴天条件下风速和白天相对湿度 RH2 的偏差。UACM 重现了城市中的夜间城市热岛效应,显示了逼真的昼夜加热和冷却模式,这对于准确预测雾的开始和持续时间非常重要。UACM 有效地预测了雾的开始、演变和消散,与观测数据和卫星图像非常吻合。与 WRF-BACM 相比,WRF-UACM 减少了日落后不久的冷偏差,从而将起雾误差提高了 3 小时。这项研究凸显了 UACM 在改善雾预测方面的潜力及其在业务环境中的应用。随着对不同类型雾的进一步研究,UACM 可为城市地区的预防措施和减少干扰提供重要见解。
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引用次数: 0
Continuous Initial Breakdown Development of In-Cloud Lightning Flashes 云内闪电的连续初始分解开发
IF 3.8 2区 地球科学 Q2 METEOROLOGY & ATMOSPHERIC SCIENCES Pub Date : 2024-10-24 DOI: 10.1029/2024JD041302
Yunjiao Pu, Steven A. Cummer

Using a 30–250 MHz VHF interferometer, we observed a previously unreported mode of initial lightning development inside thunderclouds. This mode is defined by continuous VHF radiation spanning several km within the first few milliseconds of lightning initiation. Following flash initiation through fast positive breakdown at high altitudes above 9 km, the VHF radiation front of upward negative streamers ascended continuously at a speed of ∼1.0 × 106 m/s, forming a continuous initial breakdown burst (CIBB) about 2 km in length. For the two CIBBs analyzed, the long and narrow CIBB channel was traversed by dart leaders that occurred later in the flash, indicating that the CIBB channel belongs to what becomes the main conducting leader channel. In contrast to classic initial breakdown pulses (IBPs) with sub-pulses superimposed on the rising edge, CIBBs produced a series of discrete, narrow LF pulses (<10 μs) with an average time interval of 0.20 and 0.14 ms, respectively. We speculate that a CIBB is a continuously developing negative streamer system in the high electric field region at high altitudes, with connections of internal plasma channels producing LF pulses. These results have implications for physical conditions conducive to the formation of a long and continuous negative streamer system.

利用 30-250 MHz 甚高频干涉仪,我们观测到了一种以前未曾报道过的雷云内部初始闪电发展模式。这种模式是指在闪电发生的最初几毫秒内,持续的甚高频辐射跨越数公里。在 9 千米以上的高空通过快速正击穿引发闪电后,向上的负流束的甚高频辐射前沿以 1.0 × 106 米/秒的速度持续上升,形成了约 2 千米长的持续初始击穿爆发(CIBB)。在分析的两个 CIBB 中,狭长的 CIBB 通道被闪光后期出现的飞镖头穿过,这表明 CIBB 通道属于成为主要传导头的通道。与上升沿上叠加有子脉冲的经典初始击穿脉冲(IBPs)不同,CIBBs产生了一系列离散、狭窄的低频脉冲(<10 μs),平均时间间隔分别为0.20和0.14毫秒。我们推测,在高海拔地区的高电场区域,CIBB 是一个持续发展的负流束系统,其内部等离子通道的连接产生低频脉冲。这些结果对有利于形成长而连续的负流束系统的物理条件具有影响。
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引用次数: 0
Anthropogenic Exacerbation in Dry-Hot Probability and Consequential Record-Shattering Droughts in the Middle and Lower Reaches of the Yangtze River 长江中下游干热概率的人为加剧和随之而来的破纪录干旱
IF 3.8 2区 地球科学 Q2 METEOROLOGY & ATMOSPHERIC SCIENCES Pub Date : 2024-10-24 DOI: 10.1029/2024JD041603
Shuyun Feng, Xihui Gu, Yansong Guan, Quan J. Wang, Yanhui Zheng, Lunche Wang, Xiang Zhang, Dongdong Kong

In the year 2019, the middle and lower reaches of the Yangtze River (MLRYR) experienced an unprecedented summer-autumn drought (SAD) driven by dry-hot conditions [high near-surface air temperatures (T) and low precipitation (P)], causing substantial agricultural and economic losses. However, the influence of anthropogenic climate change (ACC) on these dry-hot conditions and their impacts on SAD occurrences remains uncertain. Here, both observations and simulations show that an ACC-driven T increase led to the greater likelihood of dry-hot conditions from August to November 1901–2020 in MLRYR. Using the self-calibrating Palmer drought index (scPDSI) to assess SAD severity, we find an increasing likelihood of SAD occurrence (from 33.3% in 1901–2000 to 85.7% in 2001–2020) in MLRYR associated with more frequent dry-hot conditions. Under a business-as-usual scenario, future dry-hot association is projected to be stronger, with exceptional dry-hot conditions to increase by +10% per century. ACC-induced increase in dry-hot conditions would elevate the likelihood of SAD events like the 2019 event from 1.59% (1961–2020) to 17.82% (2041–2100). Therefore, effective measures are needed in MLRYR to adapt to increasing dry-hot conditions and associated SAD occurrences under anthropogenic warming.

2019 年,长江中下游地区在干热条件(近地面气温(T)高、降水量(P)少)的驱动下经历了前所未有的夏秋干旱(SAD),造成了巨大的农业和经济损失。然而,人为气候变化(ACC)对这些干热条件的影响及其对 SAD 发生的影响仍不确定。在此,观测和模拟结果表明,ACC 驱动的 T 升高导致 1901-2020 年 8 月至 11 月在 MLRYR 出现干热条件的可能性增大。利用自校准帕尔默干旱指数(scPDSI)来评估 SAD 的严重程度,我们发现在 MLRYR,SAD 发生的可能性越来越大(从 1901-2000 年的 33.3% 增加到 2001-2020 年的 85.7%),这与更频繁的干热条件有关。在 "一切照旧 "的情景下,预计未来干热关联将更强,特殊干热条件每百年将增加 +10%。ACC 引起的干热条件增加将使发生类似 2019 年 SAD 事件的可能性从 1.59%(1961-2020 年)增加到 17.82%(2041-2100 年)。因此,在人为气候变暖的情况下,需要采取有效的措施来适应日益增加的干热条件和相关的 SAD 事件。
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引用次数: 0
Aeolus Winds Improve Arctic Weather Prediction Aeolus 风改善了北极天气预报
IF 3.8 2区 地球科学 Q2 METEOROLOGY & ATMOSPHERIC SCIENCES Pub Date : 2024-10-24 DOI: 10.1029/2024JD041124
C.-C. Chou, P. J. Kushner, Z. Mariani

It has been proven that assimilating winds from the Aeolus global Doppler Wind Lidar (DWL) would enhance the predictive skill of weather forecast models. In this study, we use a series of observing system experiments to examine how currently assimilated “operational” wind products and Aeolus winds impact environment and climate change Canada's global forecast system over the data-sparse Arctic region. Aeolus winds improve the tropospheric wind and temperature forecasts by about 0.7%–0.9% of error reduction (a 15%–20% effect compared to the impact of operational wind products) while having little impact on specific humidity. In particular, Aeolus winds have an impact on forecasts of strong wind days on the wind and temperature fields that is double the impact for weaker wind days. On the other hand, the operational wind products do not show as large a discrepancy in impact between forecasts of disturbed and normal days. These findings suggest significant potential for global DWL observations to enhance severe weather prediction in polar regions.

事实证明,同化来自 Aeolus 全球多普勒风激光雷达(DWL)的风将提高天气预报模式的预测能力。在这项研究中,我们利用一系列观测系统实验来研究目前同化的 "业务 "风产品和 Aeolus 风如何影响加拿大在数据稀缺的北极地区的环境和气候变化全球预报系统。Aeolus 风改善了对流层风和温度预报,误差减少了约 0.7%-0.9%(与业务风产品的影响相比,效果为 15%-20%),而对具体湿度的影响很小。特别是,Aeolus 风对强风日风场和温度场预报的影响是弱风日的两倍。另一方面,业务风产品对扰动日和正常日预报的影响差异不大。这些发现表明,全球 DWL 观测在加强极地地区恶劣天气预报方面具有巨大潜力。
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引用次数: 0
Deciphering the Characteristics and Drivers of the Summer Monsoon Precipitation Extremes Over the Indian Himalayas 解读印度喜马拉雅山脉夏季季风极端降水的特征和驱动因素
IF 3.8 2区 地球科学 Q2 METEOROLOGY & ATMOSPHERIC SCIENCES Pub Date : 2024-10-23 DOI: 10.1029/2024JD042226
Rohtash Saini, Raju Attada

This study investigates the physical processes behind extreme precipitation events (EPEs) in the Himalayas, notorious for causing frequent floods and significant loss of life and property. Due to the presence of complex terrain, understanding the driving factors of these EPEs is challenging. Here, we decipher the precipitation characteristics and their driving factors responsible for the occurrence of EPEs in the Western Himalayas (WH) for the period 1979–2020. EPEs are defined as events exceeding the 99th percentile threshold. The extreme precipitation in the WH is contributed by both large-scale precipitation (accounting for 61%) and convective precipitation (39%). Moreover, 25.49% of EPEs in this region are directly associated with monsoon depressions. The presence of distinct upper-tropospheric gyres flanking the WH, along with a prominent zonal wave pattern, promotes a southward extension of the trough. This intensifies the low-level convergence of moisture-laden winds from the adjoining seas, resulting in substantial moisture availability for the EPEs. An omega-type blocking pattern emerges 4 days before EPEs, facilitating the intrusion of an extratropical cyclonic circulation. This circulation, characterized by its slow eastward and equatorward movement, leads to low-level moisture flux convergence and ascending motions, which in turn trigger the EPEs. This highlights the crucial role of extratropical signals in driving EPEs and implies that tropical-extratropical interactions play an important role in these EPEs. Furthermore, the shifting of the Intertropical Convergence Zone is strongly linked to the enhancement of the intensity of EPEs. Moreover, moisture budget analysis shows that EPEs over the WH are primarily driven by vertical advection, with the dynamic (thermodynamic) terms explaining 92% (8%) contribution. The intensified diabatic heating structure further enhances the convection, facilitating the development of deep convection which controls the local thermodynamics of these EREs. Lastly, our study demonstrated that most intensified and persistent EPEs over the Himalayas are found to be linked with Quasi-Resonance Amplification, which is driven by baroclinic waves with 5 and 8 zonal wave numbers that contribute to these EPEs.

喜马拉雅山的极端降水事件因频繁引发洪水和造成重大生命财产损失而臭名昭著,本研究调查了这些事件背后的物理过程。由于地形复杂,了解这些极端降水事件的驱动因素具有挑战性。在此,我们解读了 1979-2020 年间西喜马拉雅山(WH)发生 EPEs 的降水特征及其驱动因素。极端降水事件被定义为超过第 99 百分位数阈值的事件。大尺度降水(占 61%)和对流降水(占 39%)都是造成西喜马拉雅山极端降水的原因。此外,该地区 25.49% 的极端降水事件与季风低气压直接相关。WH两侧存在明显的上对流层回旋,加上显著的地带性波浪模式,促进了低槽向南延伸。这加强了来自邻近海域的含湿风的低空辐合,从而为 EPE 提供了大量水汽。欧米茄型阻塞模式在 EPE 出现前 4 天出现,促进了外热带气旋环流的侵入。该环流的特点是缓慢向东和向赤道移动,导致低层水汽通量汇聚和上升运动,进而引发 EPE。这凸显了外热带信号在驱动 EPEs 方面的关键作用,并意味着热带-外热带相互作用在这些 EPEs 中发挥了重要作用。此外,热带辐合带的移动与 EPEs 强度的增强密切相关。此外,水汽预算分析表明,WH 上的 EPEs 主要是由垂直平流驱动的,其中动力(热动力)项占 92%(8%)。强化的二重加热结构进一步增强了对流,促进了深层对流的发展,而深层对流控制了这些EREs的局部热力学。最后,我们的研究表明,喜马拉雅山脉上空的大多数强化和持续性 EPE 都与准共振放大有关,而准共振放大是由 5 和 8 级带状波数的气压波驱动的,它们对这些 EPE 起到了促进作用。
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Journal of Geophysical Research: Atmospheres
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