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Dust Storms Forward Trajectories and Influence Range over the Mu Us Desert
HU Wenjie, MA Li, WU Xiuqin, ZHANG Kebin
Acta Scientiarum Naturalium Universitatis Pekinensis    2021, 57 (6): 1161-1171.   DOI: 10.13209/j.0479-8023.2021.089
Abstract703)   HTML    PDF(pc) (4567KB)(189)       Save
Based on meteorological data, MODIS remote sensing image data and NCEP reanalysis data, the forward trajectories of dust storms in different seasons at different altitudes (500, 1000, and 1500 m) over the Mu Us Desert from 2000 to 2019 were simulated by HYSPLIT model, and was compared with the dust information identified by remote sensing image to determine the influence range of dust storm in the Mu Us Desert. The results show that: 1) In the past 20 years, the number of dust storms in the Mu Us Desert decreased slowly, with 143 dust storms months and 387 dust storms days. Since 2004, the frequency of dust storms has gradually decreased. 2) Seasonal climatic conditions have great influence on the moving path of dust storms in the Mu Us Desert. The frequency of dust storms is higher in spring and lowest in autumn. 3) The main areas affected by dust storms in the Mu Us Desert include northern Shaanxi Province, northern Shanxi Province, northern and central Hebei Province, northern and central Shandong Province, Beijing, Tianjin, eastern Inner Mongolia Autonomous Region and Northeast Three Provinces. The affected areas abroad include North Korea, North Japan and the border between Russia and China. The affected sea areas include Bohai Sea, Northern Yellow Sea and sea of Japan Northwest. The comparison between remote sensing image and HYSPLIT model provides an effective tool to verify and enhance the understanding of dust transport, diffusion and deposition process, so as to provide scientific reference for disaster prevention and mitigation decision-making and sand source control.
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The Implementation about The Method of Low-bound Velocity Spectrum Reduce Errors in MRR Retrieval
HE Siyuan;LIU Xiaoyang1;SUN Dali;ZHANG Ke;ZUO Quan
Acta Scientiarum Naturalium Universitatis Pekinensis    DOI: 10.13209/j.0479-8023.2014.174
Local Regularity for the Linear Second-Order Parabolic Equation in Nondivergence Form
YAO Fengping,ZHANG Kejing
Acta Scientiarum Naturalium Universitatis Pekinensis   
Abstract683)            Save
By developing the method of Acerbi et al, the authors obtain local regularity in Orlicz spaces for the linear second-order parabolic equations with small BMO coefficients in nondivergence form. Such regularity estimates can be applied to the study of the existence of solutions in W2,1p.
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The Discovery and Its Significance of Late Quaternary Involution in the Area of Lower Reach of Qingshuihe River, Ningxia, China
ZHANG Ke,LIU Kaiyu,YANG Jingchun
Acta Scientiarum Naturalium Universitatis Pekinensis   
Abstract804)            Save
In the lake-face strata located in the lower reach of the Qingshuihe River, Ningxia with the latitude of 37.4° N and the elevation about 1230m, involution dated in late period of late Quaternary was discovered, which indicates that the south limit of permafrost had once expanded approximately to the latitude of 37.4° N in that time in Ningxia and that the annual mean temperature was 8~9℃ lower than today. Because the intensive tectonic uplift in the northeast margin of Tibetan Plateau and cold and dry weather in the last glacial maximum, the Qingshuihe River was so blocked that along the margin of the blocked-lake the involution was developed.
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The Neotectonic Movements of Enkai Fault Zone in Guangdong Province
ZHANG Ke,CHEN Guoneng,DENG Ruru
Acta Scientiarum Naturalium Universitatis Pekinensis   
Abstract1112)            Save
Enkai fault zone is one of the important fault zones along the coast area of southeast China. The fault zone with the length of about 160km is mainly constituted by three approximately parallel NE faults (F1 and F2 incline to NW and F3 incline to SE). In Tertiary the faults moved in a way of normal faulting. However, at the end of Tertiary or early Quaternary, the faults turned to be compressive ones by WNW-ESE strong horizontal force, resulting in compressive deformation along the whole fault zone. Probably because of weakening of the WNW-ESE compressive stress from middle Pleistocene and because of weakening tendency of compressive stress from the south to the north along the southeastern coast of China, compressive stress in the south segments of the fault zone is strong enough to make the faults move in a way of reverse faulting and form reverse faulting landform while compressive stress in the north segments of the fault zone is so weak compared to isostacy force as to make the fault blocks restart isostacy uplift, move in a way of normal faulting and form normal faulting landform. Because of the approximate equilibrium between isostacy and horizontal compressive force in the middle segments of the fault zone, the faults have kept relatively steady state, resulting in weak contrast landform. In about late Pleistocene, a series of NW faults in the fault zone came into being or reactivated. On one hand, these NW faults, due to small angle between their strike and main compressing stress axis, have relatively small friction stress on the fault surfaces so that they could be moved more easily and often offset NE faults, forming obstacles to the strike slip of NE faults. On the other hand, the movements of NW faults release some strain energy so that they weaken compressive stress on the NE fault surfaces. Both of them reduce the activity of NE faults.
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