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451.
Kewei Xi Xiaoya Wang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(12):4054-4065
The ionospheric error affects the accuracy of the Global Navigation Satellite Systems observation and precise orbit determination. Usually, only the first order ionospheric error is considered, which can be eliminated by the ionospheric-free linear combination observation. But the remaining higher order ionospheric error will affect the accuracy of observations and their applications. In this paper, the influence of the higher order ionospheric error have been studied by using the International Geomagnetic Reference Field 13 and the Global Ionosphere Maps model produced by the Center for Orbit Determination in Europe. Focus on ionospheric error, the experiment of paper at doy 302 in 2019, which show that the second order ionospheric error impacting BeiDou Navigation Satellite System (BDS) B1I and B3I observation is 6.3569 mm and 11.8484 mm, respectively. Whereas, the third order ionospheric error impacting BDS B1I and B3I observation is 0.1734 mm and 0.3977 mm, respectively. Due to the current measurement accuracy of BDS carrier-phase observation can reach 2 mm, the influence of high order ionospheric error on observation should be considered. For BDS precise orbit determination, the orbit overlapping results are indicated that its orbit accuracy can be improved approximately 5 mm with the higher order ionospheric error correction, which is also in agreement with the results of Satellite Laser Ranging in this work. 相似文献
452.
Mode shape has become a hotspot of vibration-based damage detection in plates.Two-dimensional(2D)modal curvature(MC2D),derived from mode shapes,is a prevailing physical quantity used to indicate damage.Unfortunately,the physical mechanism of MC2 Dfor characterizing damage in plates has not been clarified to date.In contrast,one-dimensional(1D)modal curvature(MC1D)has explicit physical mechanism to portray damage in beams.Unresolved physical mechanism of MC2 Dseverely hampers its applications for damage identification in plates.To address this deficiency,the clarification mechanism of MC2 Dis investigated to identify damage.With the clarified mechanism,numerical and experimental cases are used to demonstrate the effectiveness of MC2 Din detecting damage in plates. 相似文献
453.
454.
双旋流器单头部模型燃烧室冷态流场试验 总被引:10,自引:3,他引:7
利用PIV(Particle image velocimetry)技术对双轴向反旋旋流器、单头部、矩形模型燃烧室内的冷态流场进行了试验研究.分析了燃烧室的纵向截面、横向截面上的流场结构以及旋流器参数对回流区尺寸的影响.研究结果表明:双旋流燃烧室的流场为不规则的结构,中心轴上下两个涡不对称,各主燃孔气流穿透深度也不相同,流场中存在流向涡;减小一级旋流器流通面积、旋流数,或增大二级旋流器的旋流数,可增大回流区的尺寸,而增大二级旋流器流通面积,回流区的尺寸会减小. 相似文献
455.
窄线宽单频单偏振环行腔掺铒光纤激光器 总被引:3,自引:1,他引:2
为了获得稳定的窄线宽单频单偏振掺铒光纤激光器输出,对采用饱和吸收体的环行腔结构掺铒光纤激光器进行了研究.实验中采用未抽运掺铒光纤作为饱和吸收体形成窄带滤波器,并选用高反射率的光纤光栅作为波长选择元件,同时采用具有高消光比的保偏环行器来获得单偏振激光.窄线宽单频单偏振环行腔掺铒光纤激光器的峰值波长可以通过拉伸光纤光栅进行调谐,调谐的范围为1548~1552nm.当抽运功率为275mW时获得的输出最大功率55.4mW.通过采用光纤延迟自外差法的线宽测试技术测量出该环行腔掺铒光纤激光器的20dB线宽为3kHz,光纤激光器的输出光偏振态长时间稳定在偏振度99.9%.这种窄线宽单频单偏振掺铒光纤激光器可以作为相干激光雷达的稳定信号源. 相似文献
456.
短光纤延时自外差法测量窄线宽激光器线宽 总被引:4,自引:2,他引:2
从理论上分析推导了移频延时自外差法测量激光器线宽的基本原理,并采用延时自外差法数学模型,编写了仿真程序.借助此分析结果,通过对两台已知线宽的窄线宽激光器的实际测量数据,与仿真结果对比,验证了模型的正确性.在此基础上,提出了短光纤延时自外差法,采用该方法可以在延时光纤长度远小于6倍的激光器相干长度时,消除延时自外差法因为延时时间不够导致测量精度的大幅度下降这一缺陷,为工程上实现精确测量窄线宽激光器线宽提供了行之有效的方法. 相似文献
457.
458.
介绍了一种利用激光测距仪测距、CCD光学经纬仪测角对动态的舰载雷达天线进行定位的雷达标校方法。探讨了对动态目标的定位原理,给出了真值测量的数学模型,论证了方位标的设计原则,分析了雷达标校的精度。 相似文献
459.
S.M. Kopeikin E. Pavlis D. Pavlis V.A. Brumberg A. Escapa J. Getino A. Gusev J. Müller W.-T. Ni N. Petrova 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,42(8):1378-1390
Lunar laser ranging (LLR) measurements are crucial for advanced exploration of the laws of fundamental gravitational physics and geophysics as well as for future human and robotic missions to the Moon. The corner-cube reflectors (CCR) currently on the Moon require no power and still work perfectly since their installation during the project Apollo era. Current LLR technology allows us to measure distances to the Moon with a precision approaching 1 mm. As NASA pursues the vision of taking humans back to the Moon, new, more precise laser ranging applications will be demanded, including continuous tracking from more sites on Earth, placing new CCR arrays on the Moon, and possibly installing other devices such as transponders, etc. for multiple scientific and technical purposes. Since this effort involves humans in space, then in all situations the accuracy, fidelity, and robustness of the measurements, their adequate interpretation, and any products based on them, are of utmost importance. Successful achievement of this goal strongly demands further significant improvement of the theoretical model of the orbital and rotational dynamics of the Earth–Moon system. This model should inevitably be based on the theory of general relativity, fully incorporate the relevant geophysical processes, lunar librations, tides, and should rely upon the most recent standards and recommendations of the IAU for data analysis. This paper discusses methods and problems in developing such a mathematical model. The model will take into account all the classical and relativistic effects in the orbital and rotational motion of the Moon and Earth at the sub-centimeter level. The model is supposed to be implemented as a part of the computer code underlying NASA Goddard’s orbital analysis and geophysical parameter estimation package GEODYN and the ephemeris package PMOE 2003 of the Purple Mountain Observatory. The new model will allow us to navigate a spacecraft precisely to a location on the Moon. It will also greatly improve our understanding of the structure of the lunar interior and the nature of the physical interaction at the core–mantle interface layer. The new theory and upcoming millimeter LLR will give us the means to perform one of the most precise fundamental tests of general relativity in the solar system. 相似文献
460.
文章介绍了航天器用热控镀铝薄膜材料的激光打孔设备研制,设备调试及应用,并介绍了镀铝薄膜材料打孔后的存放方法. 相似文献