轴系回转轴线指向误差测量方法

回转轴线指向误差是扫描机构的重要性能指标之一,对遥感成像质量有明显影响。针对回转轴线无法直接精确测量的问题,提出了基于平面反射镜、电子自准直仪的测量系统。在详细分析平面反射镜法线与回转轴线间关系的基础上,对测得的镜面法线指向数据进行傅里叶级数展开,通过零次项去除和一次谐波分量误差分离处理,得到真实的回转轴线指向误差。利用该方法对某扫描轴系实物进行了测量,结果表明:该方法测得的回转轴线误差为39″,满足系统的指标要求,相对于常规处理方法在精度和准确度上有所提高。     

高速弹载平台相参积累研究

针对高速弹载平台加速度大相参积累效果变差需进行加速度补偿的问题，研究了信号波长和积累时间与加速度之间的关系，推导了利用多普勒谱宽计算加速度的公式，提出短时间积累使用弹载惯导设备输出加速度值进行补偿、长时间积累使用惯导数据与多普勒谱宽测量加速度相结合的加速度补偿方法。仿真验证了该方法的有效性。     

飞行模拟器动力学控制的研究

针对如何获取运动平台的实时加速度和在精确跟踪加速度的同时限制位移,建立了系统动力学模型以计算加速度,使用虚拟弹簧法限制位移。在Matlab环境下,搭建了整个伺服控制系统。仿真结果表明,控制系统在保证平台位移不脱离限制区域的基础上,实现了加速度的精确跟踪。     

对直升机齿轮齿根应力分布规律的研究

本文不但指出并纠正传统齿轮齿根应力分析中的错误及不妥，而且还提出一组可确定直升机齿根剖面上正应力、剪应力以及主应力等分布规律的解析表达式。     

Diffusive shock acceleration at interplanetary perpendicular shock waves: Influence of the large scale structure of turbulence on the maximum particle energy

We calculate the maximum energy that a particle can obtain at perpendicular interplanetary shock waves by the mechanism of diffusive shock acceleration. The influence of the energy range spectral index of the two-dimensional modes of the interplanetary turbulence is explored. We show that changes in this parameter lead to energies that differ in at least one order of magnitude. Therefore, the large scale structure of the turbulence is a key input if the maximum particle energy is calculated.     

冲击加速度校准中低通滤波器的应用

介绍了在冲击加速度校准中,为了抑制电、机械等干扰和噪声对冲击加速度测量结果的影响,采用二阶巴特沃斯型低通滤波器,通过时间序列翻转、二次滤波等方式,实现零相移的低通滤波效果。并比较不同截止频率下,低通滤波器对衰减程度不同的冲击加速度波形产生的峰值偏差,给出不同加速度波形下,低通滤波器截止频率选择应注意的问题。     

Thermodynamic features of aircraft diagonal gas turbines

An effect of the Coriolis forces on the process of gas expansion in the turbine stage is considered. Expressions for efficiency with regard for the radial flow passage are derived. The calculation results and statistical data on the geometric parameters of diagonal stages are presented.     

Study of the 28 October 2003 and 20 January 2005 solar flares by means of 2.223 MeV gamma-emission line

By the data on intensity-time profiles of the neutron capture line of 2.223 MeV we have studied some characteristics of two solar flares, 28 October 2003 and 20 January 2005 (INTEGRAL and CORONAS-F observations, respectively). The SINP code was applied making allowance for the main processes of neutron interactions and deceleration in the solar plasma, character of neutron source, losses of neutrons and density model of the solar atmosphere. Comparison of the computed time profiles of 2.223 MeV line with observed ones for the flare of 28 October 2003 confirms the results obtained earlier for three other flares. Namely, the effect of density enhancement (EDE) in the sub-flare region, as well as the variations (hardening) of accelerated particle spectrum in the course of the event have been confirmed. The usual modeling procedure by the SINP code, however, seems to be inapplicable to the event of 20 January 2005. Possible causes of density enhancements during some flares and peculiarities of the 20 January 2005 flare are discussed.     

斜爆轰波的波角和法向速度-曲率关系初探

为研究斜劈诱导斜爆轰波的波阵面弯曲效应，以期为斜爆轰的不稳定性及其演化规律提供新的见解，基于加权本质无振荡（WENO）格式空间离散和附加Runge-Kutta方法时间离散的求解器，针对不同的化学反应参数（释热量、放热速率和化学反应区参考长度）条件，开展斜爆轰波的数值计算研究。结果表明斜爆轰波沿波阵面的波角变化可分为3个区域：区域I，波角平滑减小；区域II，波角跃升后衰减；区域III，波角有规律振荡。波阵面法向速度-曲率关系在区域I呈现准垂直直线变化趋势，并伴随着爆轰波强度的不断衰减；在区域III则呈现出"D"形曲线，即由极曲线段、光滑水平变化段和拟线性变化段组成，为类胞格结构的周期性演变；区域II可认为是以上两个区域特征的耦合。不同的化学反应参数对斜爆轰波波阵面的弯曲效应影响存在较大差别。     

Optimal steering law of refractive sail

The interaction between electromagnetic waves and matter is the working principle of a photon-propelled spacecraft, which extracts momentum from the solar radiation to obtain a propulsive acceleration. An example is offered by solar sails, which use a thin membrane to reflect the impinging photons. The solar radiation momentum may actually be transferred to matter by means of various optical phenomena, such as absorption, emission, or refraction. This paper deals with the novel concept of a refractive sail, through which the Sun’s light is refracted by crossing a film made of polymeric micro-prisms. The main feature of a refractive sail is to give a large transverse component of thrust even when the sail nominal plane is orthogonal to the Sun-spacecraft line. Starting from the recent literature results, this paper proposes a semi-analytical thrust model that estimates the characteristics of the propulsive acceleration vector as a function of the sail attitude angles. Such a mathematical model is then used to analyze a simplified Earth-Mars and Earth-Venus interplanetary transfer within an optimal framework.