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41.
基于长江流域148个气象站1980—2017年的蒸发皿观测数据,将旋转经验正交函数(REOF)和模糊C均值聚类(FCM)相结合,对流域蒸发皿蒸发量(PE)进行分区,然后运用Modified Mann-Kendall检验和多元逐步回归等方法,分析各子区域PE的变化特征并识别其主要影响因子。结果表明:1) REOF的前4个空间模态显示流域PE存在5个主要的异常敏感区,基于这4个空间模态,流域PE在空间上可划分为9个子区域。2)在年尺度上,各区PE呈不同程度的增加趋势,其中中部盆地区上升速率最大(111.28 mm/10 a),西部高原区上升速率最小(12.5 mm/10 a);而在季节尺度上,秋、冬季流域PE呈显著上升趋势,春、夏季PE的变化具有明显的区域差异性,部分地区PE为下降趋势。3)影响PE变化的主要因子因地而异,但大多子区域的PE变化与平均气温和饱和水汽压差的变化显著相关。 相似文献
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smail Hakk
zler 《Ocean Engineering》2008,35(1):17-27
The beach profile and sediment transport are very important factors in the design of coastal structures, and the beach profile is mainly affected by a number of parameters, such as wave height and period, beach slope, and the material properties of the bed. In this study, considering wave height (H0=6.5, 11.5, 16, 20, 23, 26 and 30 cm), wave period (T=1.46 and 2.03 s), beach slope (m=1/10 and 1/15) and mean sediment diameter (d50=0.18, 0.26, 0.33 and 0.40 mm), an experimental investigation of coastal erosion profile (storm profile) was carried out in a wave flume using regular waves, and geometric characteristics of erosion profile were determined by the resultant erosion profile. Dimensional and non-dimensional equations were obtained by using linear and non-linear regression methods through the experimental data and were compared with previously developed equations in the literature. The results have shown that the experimental data fitted well to the proposed equations with respect to the previously developed equations. 相似文献
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本文采用中国沿海地区13个探空站2010~2014年实测地表温度Ts与平均温度Tm数据,利用傅里叶级数分析法精化中国沿海地区Tm模型,并将2015年探空站实测Tm数据与精化模型进行对比检验。结果表明,精化模型在Tm探测方面具有更高的计算精度,其计算大气可降水量的误差概率分布趋近于正态分布,具有较强的稳定性。 相似文献
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Achieving a reliable and accurate numerical prediction of the self-propulsion performance of a ship is still an open problem that poses some relevant issues. Several CFD methods, ranging from boundary element methods (BEM) to higher-fidelity viscous Reynolds averaged Navier–Stokes (RANS) based solvers, can be used to accurately analyze the separate problems, i.e. the open water propeller and the hull calm water resistance. However, when the fully-coupled self-propulsion problem is considered, i.e. the hull advancing at uniform speed propelled by its own propulsion system, several complexities rise up. Typical flow simplifications adopted to speed-up the simulations of the single analysis (hull and propeller separately) lose their validity requiring a more complex solver to tackle the fully-coupled problem. The complexity rises up further when considering a maneuver condition. This aspect increases the computational burden and, consequently, the required time which becomes prohibitive in a preliminary ship design stage.The majority of the simplified methods proposed in literature to include propeller effects, without directly solve the propeller flow, in a high-fidelity viscous solver are not able to provide all the commonly required self-propulsion coefficients. In this work, a new method to enrich the results from a body force based approach is proposed and investigated, with the aim to reduce as much as possible the computational burden without losing any useful result. This procedure is tested for validation on the KCS hull form in self-propulsion and maneuver conditions. 相似文献
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高分辨率光学遥感场景分类的深度度量学习方法 总被引:1,自引:1,他引:0
针对高分辨率光学遥感影像场景具有同类型内部差异大、不同类型间相似度高导致部分场景识别困难的问题,本文提出了一种深度度量学习方法。首先在深度学习模型的特征输出层上为每类预设聚类中心,其次基于欧氏距离方法设计均值中心度量损失项,最后联合交叉熵损失项以及权重与偏置正则项构成模型的损失函数。该方法的目标是在特征空间上使同类型特征聚集并扩大类型间的距离以提高分类准确率。试验结果表明,本文方法有效地提升了分类准确率。在RSSCN7、UC Merced和NWPU-RESISC45数据集上,与现有方法相比,分类准确率分别提高了1.46%、1.09%和2.51%。 相似文献
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Dong Li 《天文和天体物理学研究(英文版)》2019,(5):43-52
Magnetic reconnection is thought to be a key process in most solar eruptions. Thanks to highresolution observations and simulations, the studied scale of the reconnection process has become smaller and smaller. Spectroscopic observations show that the reconnection site can be very small, which always exhibits a bright core and two extended wings with fast speeds, i.e., transition-region explosive events.In this paper, using the PLUTO code, we perform a 2-D magnetohydrodynamic simulation to investigate small-scale reconnection in double current sheets. Based on our simulation results, such as the line-of-sight velocity, number density and plasma temperature, we can synthesize the line profile of SiIV 1402.77? which is a well known emission line used to study transition-region explosive events on the Sun. The synthetic line profile of Si IV 1402.77? is complex with a bright core and two broad wings which can extend to nearly 200 km s-1. Our simulation results suggest that the transition-region explosive events on the Sun are produced by plasmoid instability during small-scale magnetic reconnection. 相似文献
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