金属零件切削加工中刀具前角的合理选用原则

分析了金属零件切削加工中刀具前角大小对加工过程中切削力、刀具耐用度、切削温度等方面的影响,提出了合理前角的概念,给出了工作中合理选用前角的原则。     

考虑侧风情况下的无人机自主导航控制技术研究

随着无人机应用范围的扩大,要求无人机能精确跟踪预定航线.介绍了无人机侧向导航控制律、切换准则和控制参数的限定;分析了侧风对无人机自主飞行时姿态的影响,以及在一种常用侧向控制律下形成侧风偏差的原因,给出了解决的办法.Matlab软件数字仿真的结果对比表明了控制系统抗侧风偏差的有效性.     

旋成体大迎角分离流的Euler方程数值模拟

用三维Euler方程计算旋成体的大迎角绕流,我们发现:亚声速自由流时,计算得到的是无分离流动,与实际的分离流不相符合,因而计算的法向力大大小于有分离的实验值;而当自由流为超声速,且横向自由流M数较高时,由于背风表面出现激波,无粘Euler方程的数值计算能自动捕捉到背风面上的分离涡,计算法向力与实验值接近。为了对亚声速自由流用Euler方程数值模拟大迎角旋成体背风面上分离涡,根据问题的物理图像,在假设的分离线上,提出强加Kutta条件的方法,成功地计算出有分离流动,使计算的法向力与实验值接近。     

Interplanetary Physics Research in China： 2006-2008

This brief report summarized the latest advances of the interplanetary physics research in China during the period of 2006-2007,made independently by Chinese space physicists and through international collaboration.The report covers all aspects of the interplanetary physics,including theoretical studies,numerical simulation and data analysis.     

Gnevyshev gap, Forbush decreases, ICMEs and solar wind electric field: relationships

We have studied annual frequency distribution of the Forbush decreases for three solar cycles (20, 21, 22); most are associated with the fast ICMEs and SSCs. The frequency varies in step with the solar cycle but the distribution has a notable gap embedded in it, near the maximum of the cycle leading to two peaks in Forbush decreases per cycle. We show that the gap coincides with the epoch of solar polar field reversal. There is an indication of an odd/even cycle effect in the frequency distribution of Forbush decreases and the associated SSCs. We find that two peaks in Forbush decrease and SSC distributions are separated by the Gnevyshev gap; second peaks occur well before the onset of the high-speed streams in the descending phase of a cycle which do not cause Forbush decreases but do contribute to a peak in the geomagnetic activity index Ap. We compare Forbush decrease and SSC distributions with the corresponding distribution of the solar wind electric field and find that a large amplitude of the electric field of itself does not cause a Forbush decrease to occur unless it is also associated with a fast ICME/SSC.     

Relativistic solar protons in the ground level event of 23 February 1956: New study

In this study we applied again to the outstanding solar particle event of 23 February 1956, the largest one in the entire history of observations of solar cosmic rays. Due to significant improvement of the analysis/modeling techniques and new understanding of physical processes in the solar atmosphere and interplanetary space, a possibility arises to interpret the old data in the light of modern concept of multiple particle acceleration at/near the Sun. In our new analysis the data of available then neutron monitors and muon telescopes are used. The technique of the analysis includes: (a) calculation of asymptotic cones of ground-based detectors; (b) modeling of cosmic ray detector responses at variable parameters of the flux of solar relativistic protons; (c) determination of primary solar proton parameters outside magnetosphere by comparison of computed responses with observations. Certain evidence was obtained that the flux of relativistic solar protons consisted of two distinct components: prompt and delayed ones. The prompt component with exponential energy spectrum caused a giant impulse-like increase at a number of European cosmic ray stations. The delayed component had a power-law spectrum and was a cause of gradual increase at cosmic ray stations in the North American region. A numerical simulation of the proton acceleration in the vicinity of the magnetic reconnection region brings to the proton spectrum with exponential dependence on energy. This agrees with observational data for the prompt component. It is also shown that the huge increase in ∼5000% on neutron monitors was due to the prompt component only with the exponential proton spectrum. The power-law spectrum of comparable intensity gave considerably smaller effect.     

Spectroscopic observations of coronal waves and coronal mass ejections

It is common to use imaging instruments such as EUV and X-ray imagers and coronagraphs to study large-scale phenomena such as coronal mass ejections and coronal waves. Although high resolution spectroscopy is generally limited to a small field of view, its importance in understanding global phenomena should not be under-estimated. I will review current spectroscopic observations of large-scale dynamic phenomena such as global coronal waves and coronal mass ejections. The aim is to determine plasma parameters such as flows, temperatures and densities to obtain a physical understanding of these phenomena.     

关于螺旋桨桨叶有利迎角的探讨

通过桨叶的性质角与迎角关系的数学模型,对桨叶有利迎角进行了分析研究。当桨叶迎角和桨叶性质角变化时,桨叶极线图和桨叶总空气动力向拉力轴靠近或离开,由此找出桨叶的最有利状态。通过分析得出,桨叶迎角接近桨叶临界迎角时最有利。最后通过桨叶极线图和桨叶总空气动力方向变化的模型实验验证了此结论的正确性。     

三维编织工艺参数对复合材料拉伸性能的影响

通过一系列的实验比较和分析研究 ,客观地评价了三维编织工艺参数对复合材料拉伸性能的影响。实验结果表明 :三维编织复合材料具有良好的力学性能 ,纤维表面编织角、纤维体积分数和纤维束细度对复合材料拉伸性能有较大的影响     

先进的大面积太阳电池阵电性能测试系统

介绍一种先进的大面积太阳电池阵电性能测试系统 ,它可用于卫星的太阳电池帆板电性能的测试 ,也可用于地面或其他领域中使用的太阳电池阵或单个太阳电池的测试。其主要特点在于 :脉冲光源使光强达一个太阳常数 ,在直径 5m的测试面上 ,光照不均匀性± 3% ,计算机控制 ,测试过程完全自动化 ,多脉冲测试功能可解决太阳电池响应慢的问题。介绍了该系统在国内外的使用及发展情况及在我国空间太阳电池阵的测试中的应用。