公差原则中相关要求的计算问题

关于公差原则中的相关要求的计算问题 ,本文提出了两种方法 :计算法和图解法。运用这两种方法可以简化此类问题的计算过程 ,准确求得计算结果。     

一种提高测量CCD成像系统MTF精度的数据处理方法

根据刃边图像的特点,采用中值滤波法、多剖线平均法以及局部滤波法对图像中的噪声进行前期处理,去噪效果好,使图像的有用信息损失小,提高了测量CCD成像系统调制传递函数的精度。实验表明,本文的数据处理方法能有效的提高测量CCD成像系统的传递函数的精度。     

航天器交会快速接近机动策略

对航天器交会接近段V-bar上保持点间的转移,单向(轨道径向或周向)推力机动的最短转移时间为半个轨道周期(对应双径向推力冲量)。若要求转移时间小于半个轨道周期,须采用双向(径向与周向联合)推力。为此,提出5种机动方案:1)起点双向冲量与终点双向冲量机动;2)途中双向连续推力机动;3)起点双向冲量与途中双向连续推力机动;4)途中双向连续推力与终点双向冲量机动;5)起点切向冲量与途中径向连续推力及终点切向冲量机动(即直线路径转移)。其中,方案1)(冲量机动)的速度增量最小,但轨迹视界角最大;方案5)(直线路径)的视界角最小(近似为零),但当转移时间T>0.292P(P为轨道周期)时,所需的速度增量较大。机动方案的选择应全面考虑转移轨迹安全性、速度增量需求、转移轨迹视界角,以及机动复杂程度等多方面因素。若视界角可满足总体设计要求,宜选择方案1);当T<0.292P时,也可考虑方案5)。     

定常基线卫星编队构形设计

采用动力学法研究了卫星编队的相对运动特性,根据星间相对基线的定义,仔细推导了星间相对基线与卫星编队构形参数之间的关系,并根据此关系定义了一种可以较好地反映星间相对基线运动稳定性的指标,即稳定度.在一个轨道周期内,分析了三种特殊卫星编队的最大水平基线和最大垂直基线在相同稳定度下的稳定时间.结果表明,这三种编队构形不能满足水平基线和垂直基线同时定常的要求.由此出发,重点研究了可以使星间相对基线定常的条件,并得出了相应的结论.水平基线定常的充要条件为三个约束关系式,垂直基线定常的充要条件为两个约束关系式.由此条件同时可知,两星编队无法满足水平基线和垂直基线同时定常的要求,因此,至少需要三星编队才可以达到此要求.最后,按照本文所得结论,设计了一个水平基线和垂直基线同时定常的三星编队.利用成熟软件对设计结果进行了分析,分析结果表明了本设计方法的正确性.     

The radiation environment in the ISS-USLab measured by ALTEA: Spectra and relative nuclear abundances in the polar,equatorial and SAA regions

We present here the energy spectra relative to different geomagnetic regions as measured by the ALTEA (Anomalous Long Term Effects on Astronauts) detector in the International Space Station – USLab from August 2006 to July 2007.     

Comparison between observed ionospheric foF2 and IRI-2001 predictions over periods of severe geomagnetic activities at Grahamstown,South Africa

The observed ionospheric F2 critical frequency (foF2) values over a South Africa mid-latitude station, Grahamstown, (geographic coordinates: 33.3°S, 26.5°E), were analysed and compared with International Reference Ionosphere (IRI) model, using the CCIR (Comite´ Consultatif International des Radio communications) and URSI (Union Radio-Scientifique Internationale) coefficients, during four geomagnetically disturbed days in the year 2000. These days are April 5, May 23, August 10 and September 15. The data were analysed for five days around the storm day. Comparisons between the IRI-2001 predicted foF2 values, using both CCIR and URSI coefficients and the observed values are shown with their root-mean-square error (RMSE) and the relative deviation module mean (rdmm) for the various storm periods. The CCIR option performed more accurately than the URSI option.     

Stochastic modelling considering ionospheric scintillation effects on GNSS relative and point positioning

Global Navigation Satellite Systems (GNSS), in particular the Global Positioning System (GPS), have been widely used for high accuracy geodetic positioning. The Least Squares functional models related to the GNSS observables have been more extensively studied than the corresponding stochastic models, given that the development of the latter is significantly more complex. As a result, a simplified stochastic model is often used in GNSS positioning, which assumes that all the GNSS observables are statistically independent and of the same quality, i.e. a similar variance is assigned indiscriminately to all of the measurements. However, the definition of the stochastic model may be approached from a more detailed perspective, considering specific effects affecting each observable individually, as for example the effects of ionospheric scintillation. These effects relate to phase and amplitude fluctuations in the satellites signals that occur due to diffraction on electron density irregularities in the ionosphere and are particularly relevant at equatorial and high latitude regions, especially during periods of high solar activity. As a consequence, degraded measurement quality and poorer positioning accuracy may result.     

基于杂波对消-自聚焦的多通道SAR-GMTI

对超高频(UHF)波段多通道合成孔径雷达(SAR)动目标检测技术进行研究,解决了长相干积累时间导致动目标在方位向散焦严重的问题。采用分块自聚焦技术对多通道SAR地面移动目标指示(GMTI)系统自适应杂波抑制后的SAR图像进行处理,改善杂波抑制后的SAR图像中动目标的聚焦情况,增强动目标与周围剩余杂波的对比度,进而提高恒虚警率(CFAR)检测的性能。与传统杂波抑制后直接进行CFAR检测方法相比较,该方法降低了检测虚警概率。实测数据处理结果显示动目标的信杂比明显提高,动目标方位向聚焦成功,证明了该方法的有效性。     

GPS P码并行矩阵式直接捕获方法

弱信号环境下,GPS信号中P码具有很强的抗模仿和抗欺骗能力。为了解决P码直接捕获技术中P码序列特性与无周期性,提出一种快速实现P码捕获的矩阵式直接捕获方法。在对直接平均法进行原理分析的基础上,研究了矩阵式频域直接捕获方法的模型,并对提出的P码捕获算法进行硬件系统设计和实现,在弱信号环境下对矩阵处理器进行实际测试。结果表明,与传统方法相比,算法能提高硬件效率,缩短捕获时间,提高数据处理效率。     

一种信道系数服从高斯分布的8PSK信号信噪比盲估计算法

信噪比（SNR,Signalto Noise Ratio）是衡量通信系统性能的重要指标。针对传统信噪比估计算法要求利用训练序列或一帧数据范周内信道系数恒定等问题,提出了一种8PSK信号在信道系数服从高斯分布的衰落信道下肯信噪比估计算法。该算法取接收信号实部或虚部数值运算构成中间观测量,理论分析8PSK信号经过衰落信道后...