关于多普勒频率转换成距离变化率公式的讨论

利用多普勒效应原理对雷达测速的转换公式进行了讨论，指出在飞行器高精度轨道测量中，现行的测速转换公式存在较大的误差；给出了新的包含二阶项的测速转换公式，并导出了一个简便实用的直接在测量数据上进行该项误差修正的方法，同时进行了误差特性分析。实际计算表明：轨道测量数据进行二次修正后，匹配程度明显优于修正前。     

利用林胶茶人工群落减弱台风对橡胶林破坏机理的风洞模拟试验研究

本文研究台风登陆时（中性大层结）胶茶人工群落内部及上部风速的变化，湍流结构的变化及阻力的变化，来分析判断基减弱台风破坏的机理，评定最佳防风效果的林胶茶人工群落方案。试验研究证明台风吹向胶茶人工群落，台风越过和穿过林带，由于气流与树冠，枝叶的冲击与摩作用，使台风风速大大降低，使动能大大损失，使原来动能强和湍流弱的较大尺度旋涡的台风，变成旋涡尺度较小的动能弱湍流强的湍流，湍流能量的增强反映了风速递减率     

1:10人-椅模型上肢的跨-超音速风洞实验

 本文介绍了1:10人椅模型上肢跨-超音速风洞实验的结果。测量了Ma=0.5～2.04和攻角10°～20°范围内上肢的阻力和侧向力。获得了在握扶手和拉中央环两种姿态下手臂的气动力特性。比较了穿衣袖与不穿衣袖两种状态下手臂的气动力数据。实验结果为确定人体上肢对高速气流吹袭的耐久限度和设计防护措施提供了重要的气动力数据。     

InSb磁敏电阻角位移传感器的研究

简单分析了InSb磁敏电阻的工作原理，讨论了利用偏置磁场作用于半桥磁敏电阻构成转动速度及位移传感器的测试原理；针对半导体材料对温度十分敏感的特点，提出了利用浮动零点跟踪技术测试齿轮转速的方法，并对其优缺点进行了讨论。     

碘化钾类稳定剂在化学镀Ni-P工艺中的应用

在合理选择化学Ni-P合金配方和工艺条件的前提下，采用对比试验比较了几种稳定剂对化学镀Ni-P合金镀液及镀层性能的影响，选取合适的工艺参数，采取正交试验方案，研究了KI与其他稳定剂复配时的性能变化规律，探讨了KI的稳定机理。结果表明，备稳定剂之间有的相互兼容、相互促进，有的则相互抵触、相互削弱对方的作用。复合稳定剂综合性能的提高程度明显优于单稳定剂，获得了复合稳定剂KI与Pb（Ac）2质量浓度分别为8g／m^3和1．2g／m^3匹配的最佳工艺参数。     

关于刚体转动的角速度和角加速度的讨论

在理论力学教学中，平面运动刚体的转动与基点无关的证明过于简单，本利用矢量代数的知识，证明平面运动刚体的角度与角加速度与基点的选择无关。     

六喷管超音速引射器性能的理论分析和实验研究

对某一定尺寸的六喷管超音速引射器进行气动性能的实验研究。结果表明：随着主次流压比Ｐ＊ｐ／Ｐ＊ｓ增加，引射系数及修正引射系数下降；当引射系数增加时，混合管动量修正系数Ｋｍ下降，但主喷管流量系数μ变化不大。对上述工况进行理论计算的结果与实验数据符合良好。     

双圆柱斜向排列时旋涡脱落频率的实验研究

本研究用热线风速仪测量了斜向排列双圆柱的尾迹,并分析了尾迹中某些特征点上的速度频谱,从旋涡脱落频率的规律来研究双圆柱绕流相互之间的干扰。当两圆柱间距较远时,速度振荡的频率与单圆柱卡门涡街的频率相接近,随着两圆柱间距的接近,前、后圆柱各有其不同的旋涡脱落频率,且都不同于单圆柱旋涡脱落的频率。特别是当两圆柱处于某一相对位置时,出现双峰值的功率谱,其中一个峰值的频率大大地高于另一个峰值对应的频率,而且这两个峰值谁主谁副是不确定的,呈现出不稳定流动的特性。     

Orientations of LASCO Halo CMEs and their connection to the flux rope structure of interplanetary CMEs

Coronal mass ejections (CMEs) observed near the Sun via LASCO coronographic imaging are the most important solar drivers of geomagnetic storms. ICMEs, their interplanetary, near-Earth counterparts, can be detected in situ, for example, by the Wind and ACE spacecraft. An ICME usually exhibits a complex structure that very often includes a magnetic cloud (MC). They can be commonly modelled as magnetic flux ropes and there is observational evidence to expect that the orientation of a halo CME elongation corresponds to the orientation of the flux rope. In this study, we compare orientations of elongated CME halos and the corresponding MCs, measured by Wind and ACE spacecraft. We characterize the MC structures by using the Grad–Shafranov reconstruction technique and three MC fitting methods to obtain their axis directions. The CME tilt angles and MC fitted axis angles were compared without taking into account handedness of the underlying flux rope field and the polarity of its axial field. We report that for about 64% of CME–MC events, we found a good correspondence between the orientation angles implying that for the majority of interplanetary ejecta their orientations do not change significantly (less than 45 deg rotation) while travelling from the Sun to the near-Earth environment.     

Coronal mass ejection detection using wavelets,curvelets and ridgelets: Applications for space weather monitoring

Coronal mass ejections (CMEs) are large-scale eruptions of plasma and magnetic field that can produce adverse space weather at Earth and other locations in the Heliosphere. Due to the intrinsic multiscale nature of features in coronagraph images, wavelet and multiscale image processing techniques are well suited to enhancing the visibility of CMEs and suppressing noise. However, wavelets are better suited to identifying point-like features, such as noise or background stars, than to enhancing the visibility of the curved form of a typical CME front. Higher order multiscale techniques, such as ridgelets and curvelets, were therefore explored to characterise the morphology (width, curvature) and kinematics (position, velocity, acceleration) of CMEs. Curvelets in particular were found to be well suited to characterising CME properties in a self-consistent manner. Curvelets are thus likely to be of benefit to autonomous monitoring of CME properties for space weather applications.