RS-GIS based morphometrical and geological multi-criteria approach to the landslide susceptibility mapping in Gish River Basin,West Bengal,India

Darjeeling Himalaya is one of the several mountainous areas of India which is often suffered from landslide hazards. In this paper, a multi criteria evaluation is applied using 16 morphometric indicators, geology and lineaments to identify the areas vulnerable in respect to drainage and relief conditions. As both drainage and relief parameters exert strong influences on landslide intensity, both the diversity maps are integrated for final landslide susceptibility mapping. The obtained results show that 20.17?sq.?km (7.61%) area within the basin is highly susceptible for landslides, where average drainage density is 3.78?km/sq.?km, relative relief is greater than 408?m and slope is greater than 12°. The validation result shows that very high landslide susceptible zone is associated with very high frequency of landslide occurrence. Beside this, ROC curve also suggests good predicted rate (86.60%) for the model. So, the proposed method can be applied for predicting landslide susceptible zone.     

某型飞机桨叶平衡孔的喷丸强化技术分析

对飞机铝合金桨叶平衡孔的喷丸强化可以有效提高桨叶的疲劳强度。但在强化过程中必须对喷丸时间、喷丸强度、丸料、覆盖率等因素进行精确控制及优化，以确保达到理想的强化效果，保障飞行安全。     

超宽带螺旋天线的小型化设计

介绍一种新型的螺旋结构天线,将平面等角螺旋天线与锥面螺旋天线结合起来,采用渐变式的巴伦平衡馈电。相比传统的平面螺旋天线,针对同样频带宽度的天线设计,这种混合型螺旋天线体积更小。利用Ansoft HFSS电磁场仿真软件对天线进行建模和仿真计算,并结合仿真结果实际制作了该螺旋天线,给出了实测结果,表明天线可以在工程实际中应用。     

极大似然法在飞机极曲线辨识中的应用

介绍了利用极大似然法辨识飞机极曲线的基本原理。通过仿真研究及对实测飞行试验数据的处理，表明该方法能够辨识出光滑的非线性飞机极曲线，算法具有良好的收敛性及结果的唯一性，并且可方便地推广应用于工程中其它类型的非线性曲线辨识问题。     

Analysis Approach to Durability Based on Material Initial Fatigue Quality and S-N Curve

Based on probabilistic fracture mechanics approach, a new concept of material initial fatigue quality (MIFQ) is developed. Then, the relation between S-N curve and crack propagation curve is studied. From the study, a new durability analysis method is presented. In this method, S-N curve is used to determine crack growth rate under constant amplitude loading and evaluate the effects of different factors on durability and then the structural durability is analyzed. The tests and analyses indicate that this method has lower dependence on testing, and higher accuracy, reliability and generality and is convenient for application.     

火箭橇水刹车戽斗入水运动的阻力预测

火箭橇水刹车戽斗作为火箭橇高速试验的减速装置,附加质量较大,运行速度快,在利用水的冲击作用减速时,承受很大的载荷。为了确保火箭橇水刹车戽斗的安全,同时达到预期的减速效果,对火箭橇水刹车戽斗的运动情况进行数值仿真分析。借助Abaqus中的流固耦合技术,通过CEL方法对火箭橇水刹车戽斗入水运动情况进行分析,得到火箭橇水刹车戽斗在多种不同运动情况下的阻力曲线,并根据流体阻力理论计算公式,拟合出该火箭橇水戽斗入水的流体阻力计算公式。利用该公式可对该火箭橇水刹车戽斗在不同速度、不同初始水位高度下所受的阻力进行预测。     

基于逐次升阶的翼型参数化与气动优化方法研究

研究了基本Bezier样条曲线的特性,对比了不同阶次Bezier曲线对超临界翼型的几何描述能力以及由几何偏差带来的气动性能的偏差。利用Bezier曲线的特性提出逐次升阶的翼型参数化方法,结合改进的粒子群优化算法,建立了逐步扩展设计空间的气动优化设计方法,兼顾设计空间和优化效率,很好地解决了设计质量和设计效率之间的矛盾。最后通过典型翼型的优化设计,对比了文中方法与传统Hicks-Henne型函数方法,验证了文中方法的可行性和高效性。     

凸曲线的求长问题

本文给出并证明了凸函数的一个新的性质（文中引理及其证明），依此证明了凸曲线是可以求出长度的曲线（文中定理及其证明）及凸函数是可以积分的函数。     

河南省金融产业竞争力评价与对策

以河南省为研究重点，选取了31个省份作为对照样本，这用主成分和因子分析法对各个区域的金融产业竞争力进行计量分析和排序，结果认为，东部地区金融产业竞争力仍然保持着绝对优势地位，中部六省中，河南省的金融产业竞争力发挥着龙头作用，被划入我国区域金融产业发展的前三个梯度内，表现出良好的发展态势。在对金融产业竞争力的模糊曲线分析后认为，影响金融产业竞争力提高的八个分力，依其重要程度依次为经济力、科技力、文化力、开放力、设施力、劳动力、聚集力和环境力，均对其产生正向贡献。因此，提高河南省金融产业竞争力，主要应从以下方面入手：（1）促进河南省经济的继续增长，努力提高人均可支配收入水平。（2）做好对内对外开放，尤其是针对不同区域有针对性地扩大对外开放与区际开放。（3）完善对外金融交往基础设施，加强政府的监管效率。（4）拓展河南金融业的发展空间，充分发挥其就业效应。（5）进一步加大科技成果的转化。（6）加强区域向心吸引力，促进产业集聚。（7）加强文化建设，完善金融生态环境。     

The variability of the proton cosmic ray flux on the Sun’s way around the galactic center

The discovery of direct evidences for the acceleration of high energetic particles at the shell supernova remnant RXJ1713.7-3946 underlined the need to calculate the cosmic ray (CR) distribution in the Galaxy on a spatial grid fine enough to resolve the changes in the CR density due to these kind of objects. It was shown before by Büsching et al. [Büsching, I., Kopp, A., Pohl, M., Schlickeiser, R., Perrot, C., Grenier, I. Cosmic-ray propagation properties for an origin in supernova remnants. ApJ 619, 314–326, 2005] that the discrete nature (both in space and time) of super novae (SN) as sources of Galactic CR leads to CR spectra changing in space and time, resulting in a range of possible CR spectra at a given location in the Galaxy. As the most frequent SN types Ib and II are found within spiral arms, one can expect a significant difference of the range of possible spectra in and outside spiral arms. We investigate the variability of the local interstellar CR proton spectrum during the motion of the Sun in and out of spiral arms in its journey around the Galactic center. Using the code described by Büsching et al. [Büsching, I., Kopp, A., Pohl, M., Schlickeiser, R., Perrot, C., Grenier, I. Cosmic-ray propagation properties for an origin in supernova remnants. ApJ 619, 314–326, 2005], the proton CR density in the Galaxy is calculated with high spatial and temporal resolution (75 pc in galactocentric radius r and azimuth φ at the position of the Sun and 20 pc in z (perpendicular to the galactic plane), with a time step of 1 kyr), assuming stochastically distributed point sources with a probability distribution that resembles the spiral structure of our Galaxy. We find the averaged CR flux outside the spiral arm to be about 50% of that inside a spiral arm. We further find spatial and temporal variations of the CR flux inside spiral arms.