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981.
Yuan Lian Mark I. Richardson Claire E. Newman Christopher Lee Anthony D. Toigo Michael A. Mischna Jean-Michel Campin 《Icarus》2012,218(2):1043-1070
We investigate the ability of modern general circulation models (GCMs) to simulate transport in the martian atmosphere using measurements of argon as a proxy for the transport processes. Argon provides the simplest measure of transport as it is a noble gas with no sinks or sources on seasonal timescales. Variations in argon result solely from ‘freeze distillation’, as the atmosphere condenses at the winter poles, and from atmospheric transport. Comparison of all previously published models when rescaled to a common definition of the argon enhancement factor (EF) suggest that models generally do a poor job in predicting the peak enhancement in southern winter over the winter pole – the time when the capability of the model transport approaches are most severely tested. Despite observed peak EF values of ~6, previously published model predictions peaked at EF values of only 2–3. We introduce a new GCM that provides a better treatment of mass conservation within the dynamical core, includes more sophisticated tracer transport approaches, and utilizes a cube–sphere grid structure thus avoiding the grid-point convergence problem at the pole that exists for most current Mars GCMs. We describe this model – the Ashima Research/Massachusetts Institute of Technology Mars General Circulation Model (Ashima/MIT Mars GCM) and use it to demonstrate the significant sensitivity of peak EF to the choices of transport approach for both tracers and heat. We obtain a peak EF of 4.75 which, while over 50% higher than any prior model, remains well short of the observed value. We show that the polar EF value in winter is primarily determined by the competition between two processes: (1) mean meridional import of lower-latitude air not enriched in argon and (2) the leakage of enriched argon out of the polar column by eddies in the lowest atmospheric levels. We suggest possibilities for improving GCM representation of the CO2 cycle and the general circulation that may further improve the simulation of the argon cycle. We conclude that current GCMs may be insufficient for detailed simulation of transport-sensitive problems like the water cycle and potentially also the dust cycle. 相似文献
982.
GlobeLand30数据已被广泛应用于生态、环境、气候等研究领域,对其进行精度验证是保证GlobeLand30产品推广应用的首要前提.本文提出了一种基于众源地理数据的GlobeLand30人造地表精度验证方法:首先利用随机抽样的方法布设样本点,其次应用LDA(latent Dirichlet allocation)主题模型计算众源数据文档的地表覆盖主题,最后通过构建样本点与GlobeLand30数据产品之间的混淆矩阵,以实现人造地表数据的精度验证.研究区域为我国27个省级行政区,众源地理数据选用POI数据,对本文提出的方法进行了实例验证.结果表明:2000年和2010年的人造地表总体精度分别为87.63%和88.81%,这与GlobeLand30人造地表第三方评价精度86.97%相近,验证了本文方法的有效性. 相似文献
983.
984.
The safety of offshore pipeline has drawn a great deal of attention during deepwater installation due to the combined actions of high external pressure, axial tension, and bending moment. Meanwhile, the pipeline configuration has a remarkable effect on the structural behaviour of the tube. The special studies focus on the deepwater S-lay technique in the present paper. The stiffened catenary theory is applied to establish the static equilibrium governing differential equation of a pipe element, and the solution equations of the total pipeline configuration from a lay-barge over a stinger to the seabed are derived. The numerical iteration method for solving pipeline configuration is described in detail, and the corresponding program is developed to conduct the analysis of effects of various parameters such as laying water depth, pipe diameter, thickness of concrete weighted coating layer, stinger length, control strain, and axial tension on pipeline configuration. The results show that the laying water depth, the submerged weight of the pipe, and the axial tension are the critical factors influencing pipeline configuration. In addition, geometrical parameters of the stinger such as length, radius, and shape have an important effect on the pipe-laying capacity of the vessel. The validity of the program is further verified by means of a comparison with results obtained from the commercial finite element software OFFPIPE. 相似文献
985.
薛丁 《地震地磁观测与研究》2021,42(z1):112-113
1 研究背景
地震预报中测震学指标广泛应用于地震异常分析.顾瑾平等(2001)研究了多项指标综合预测概率,得出综合概率值在0.5以上时,对应地震率80%,测震学指标有其物理意义,若出现高综合概率值时应关注.2020年7月12日,在河北省唐山市古冶区发生MS 5.1后期强余震(39.78°N,118.44°E),震中位于1976年唐山MS 7.8大地震余震分布区内,是近几年华北地区一次显著的地震事件.基于意义相互独立的多种测震学指标0—1化异常(指标值超出2倍方差为1,反之为0)合成信息的全时空扫描预测方法,定量分析该地震的异常时空特征,对地震进行预测研究,可为中强地震的时间、地点判定提供一种新的数值预测依据. 相似文献
986.
Topography effects on the vertical vibration responses of pile group are revealed though numerical analysis and model tests.First,a series of model tests with different topography of ground and bedrock are conducted.The results indicate that displacement amplitude of the pile head in sloping ground topography is larger than in horizontal ground.Differential displacement at various positions of the pile cap is observed in non-horizontal topography.Afterwards,a numerical algorithm is employed to further explore the essential response characteristics in group piles of different topography configurations,which has been verified by the test results.The lengths of the exposed and frictional segment,together with the thickness of the subsoil layer,are the dominant factors which cause non-axisymmetric vibration at the pile cap. 相似文献
987.
黄河中游砒砂岩地区长川流域土地利用变化分析 总被引:2,自引:0,他引:2
根据1976年的Landsat-MSS影像数据以及1987年和2000年的Landsat-TM影像数据,应用遥感和地理信息系统手段以及转移矩阵和景观空间格局指数分析方法,对地处黄河中游砒砂岩地区的内蒙古准格尔旗长川流域土地利用及其变化进行研究。结果表明:1)研究区内分布最多的土地利用类型是灌木林地、草地和难利用地,该三个土地利用类型的面积占研究区域总面积75%;2)从1976~2000年期间,虽然乔木和灌木林地的面积明显增加,但同时也存在林地和草地向难利用土地、沙地和农地的转变过程。与此同时水域亦明显减少;3)水土保持生物措施的实施、农田开垦和降雨量偏少可能是导致研究区土地利用变化的主要原因。 相似文献
988.
研究近地小天体的探测机会搜索问题.针对交会型探测任务,通过结合变分理论和状态转移矩阵推导了性能指标关于可调参数的解析偏导数,然后在搜索空间中随机生成初始点,并从这些初始点出发利用解析偏导数寻优,从而得到搜索空间内对应潜在发射机会的全部局部极小值点.此方法既在一定程度上保持了传统搜索方法全局搜索的特点,又克服了传统搜索方法的盲目性,因此计算速度获得很大提高.此外该方法可以对探测机会的搜索精度进行有效地控制. 相似文献
989.
990.
Zongjun Ning M. D. Ding K. P. Qiu H. Li Y. N. Su C. Fang 《Astrophysics and Space Science》2008,315(1-4):45-51
We present multi-wavelength observations of a complicated solar eruption event to associate with an X1.2 flare and a Coronal Mass Ejection (CME) on 2003 October 26. The soft X-ray profile shows a possibility for occurrence of two flares with peaks around 06:20 and 07:00 UT. According to our observations, there are many evidences to show that they are corresponding to two energy releases. The first one produces type II, type III, moving type IV continua, a decimetric burst (DCIM) and strong emissions at Hα, 195 and 1600 Å; While the second energy release only produces a group of RS-III bursts, DCIM and Hα emissions. It appears that the first energy release is associated with a CME, while the second CME is quiet. Such observational difference between two energy releases is found indicating two magnetic reconnection processes occurrence with different plasma situation. 相似文献