基于开环穿越频率的伪攻角反馈驾驶仪设计

分析伪攻角反馈过载驾驶仪的结构特点,在采用输出反馈形式的基础上,以开环穿越频率为性能指标、系统自振频率为变量,使用连续搜索法,将闭环极点配置在期望的位置;同时考虑到伺服特性,使用优化方法搜索根平面,完成了引入附加约束条件的极点配置设计。通过实例分析,该方法便捷有效,适用于驾驶仪的工程设计。     

Solar, geomagnetic and cosmic ray intensity changes, preceding the cyclone appearances around Mexico

Recently it has been suggested that there exist specific changes in the cosmic ray intensity and some solar and geomagnetic parameters during the days, preceding the hurricane appearances over the North Atlantic Ocean. To understand better these phenomena, data for all hurricanes born not only over the Atlantic but also over the Pacific waters in the last 55 years that hit the Mexican borders were elaborated. As basic hurricane parameters the maximum rotational velocity and the estimated total energy were used. To avoid any interference all hurricanes, overlapping the preceding ones with more than 20 days were not included. Then the behavior of the cosmic ray (CR) intensity, the sunspot (SS) numbers, and the geomagnetic parameters (AP) and (KP) in 35 days prior and 20 days after the cyclone start were investigated. The CR, SS, AP and KP showed much more intensive disturbances in the periods preceding and following the hurricane appearance. For SS this disturbance gradually increase with the hurricane strength. A characteristic peak in the CR intensity appears before the hurricane start. But its place varies between 5 and 20 days before that start. Specific changes were observed in the SS. For major hurricanes they begins sometimes more than 20 days in advance. The AP and the KP show series of bursts, spread over the whole period of 30 preceding days. The obtained results from the performed correlational analysis are enough interesting to motivate a further statistical analysis with more precise techniques: in particular a common periodicity of 30 years found in the number of tropical storms landing into Mexico, the averaged rotational wind velocity and the ACE must be studied in connection with the solar Hale cycle. Using coherence wavelet spectral analysis we present a comparative study between one terrestrial and one cosmophysical phenomena that presumable influence hurricanes development: African dust outbreaks versus cosmic rays for all North Atlantic tropical cyclones. It is shown that the cosmophysical influence cannot be considered as a negligible effect.     

On bandwidth of solar subsecond bursts in cm-range

The goal is to study parameters of drifting type III bursts, and find out the emission mechanism of these bursts and understand what factors affect instantaneous spectral bandwidth of these bursts.     

大迎角耦合运动非定常空气动力特性

采用某飞机大迎角大振幅运动风洞实验结果，分析了大迎角非定常空气动力的一些特性。结果表明，飞机机动飞行时多自由度运动的气动特性比单自由度运动复杂，耦合运动时的气动特性和两个单自由度运动的气动特性的叠加结果相比有一定差别。此外，旋转天平实验结果同本实验的结果相比差别较大。     

Estimation of Galactic Cosmic Ray exposure inside and outside the Earth’s magnetosphere during the recent solar minimum between solar cycles 23 and 24

The evidently low solar activity observed between solar cycles 23 and 24 during the years 2008–2010 led to a substantial increase in the Galactic Cosmic Ray (GCR) intensity in comparison with preceding solar minima. As the GCRs consist of highly-ionizing charged particles having the potential to cause biological damage, they are a subject of concern for manned missions to space. With the enhanced particle fluxes observed between 2008 and 2010, it is reasonable to assume that the radiation exposure from GCR must have also increased to unusually high levels. In this paper, the GCR exposure outside and inside the Earth’s magnetosphere is numerically calculated for time periods starting from 1970 to the end of 2011 in order to investigate the increase in dose levels during the years 2008–2010 in comparison with the last three solar minima. The dose rates were calculated in a water sphere, used as a surrogate for the human body, either unshielded or surrounded by aluminium shielding of 0.3, 10 or 40 g/cm².     

克服旋转飞行器螺旋运动的方法研究

旋转飞行器虽然具有内在稳定性，但在飞行过程中一些不确定因素会导致飞行器产生螺旋运动，而非理想的关于角动量矢量纯粹的旋转运动。结合旋转飞行器自身的特点，借鉴自旋卫生的被动章动阻尼的方法，提出了一种通过主动控制飞行器内部质量块的运动使得飞行器碑的惯量主轴发生偏移，惯量矩阵由原来的对称阵变为含有非零非对角元素的矩阵，从而改变飞行器的姿态角运动来克服螺旋运动的方法，这将有助于提高旋转飞行器的资态控制精度。以某型旋转飞行器为背景进行仿真研究，计算结果证实了该方法的有效性和可行性。     

TDRSS中用户星的星-星天线跟踪规律深入研究

应用坐标转换，得到用户星的星-星天线基本跟踪规律。针对几种情况，并考虑地球的隔断影响和天线的自身限制，对星一星天线的方位角和俯仰角表达式进行了修正和补充。最后，针对某用户星，应用Matlab进行数学仿真。结果表明，根据得出的跟踪规律，可以使用户星的星一星天线最大范围地跟踪中继卫星。     

边条翼作俯仰运动时翼面吹气的作用

在３ｍ低速风洞中通过测力与微丝显示方法，研究了在边条翼的边条和主翼上吹气对机翼作大攻角快速俯仰运动时空气动力特性的影响，同时还研究了在不同迎角下开始吹气的作用。结果表明，翼面吹气能有效提高机翼的非定常气动特性和缩小机翼的非定常气动特性迟滞回环，特别是在小迎角下开始吹气效果较好。     

两边角盒强度计算的工程方法研究

以大量角盒试验件的试验实测值为依托 ,对常用的角盒计算方法进行了较客观的评价 ,并在此基础上 ,提出了工程可用的简化计算方法 ,这个方法使用方便 ,且具有工程上可接受的精度 ,因此推荐使用     

升力式再入飞行器离轨制动研究

针对一种升力式再入飞行器———通用航空飞行器进行全球攻击时离轨推力的控制和相应的下降轨道特点,对其再入角的选择等关键技术进行了深入分析,最终得到了依据远地点半径和可施加的Δv的范围来确定最优离轨推力角和下降椭圆轨道的有工程意义的结论。在此基础上进一步分析了切线制动和非切线制动的再入轨道特点,同时依据已知条件得到了再入角的最佳控制范围。所得结论亦可用于一般升力式再入飞行器初步轨迹的设计。