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101.
带螺旋桨飞机模型风洞实验进行洞壁干扰修正时,必须考虑螺旋桨滑流的影响。运用等效动压对运八飞机带螺旋桨模型风洞实验才气进行洞壁干扰修正,分析洞壁对带螺旋桨飞机模型试验数据的影响,并与壁压信息修正方法进行了比较。两种修正方法的修正结果基本一致,壁压信息法能实际反映洞壁干扰影响,但壁压信息法需要进行准确的壁压测量,增加实验工作量;等效动压法是以经典的洞壁干扰修正公式为基础,考虑了螺旋桨滑流的影响,而且带 相似文献
102.
103.
基于合作目标和视觉的无人飞行器全天候自动着陆导引关键技术 总被引:3,自引:0,他引:3
GPS受他国控制和易受干扰对基于该导航系统的无人飞行器导航和着陆具有潜在危险,为了使其安全自动着陆,提出通过在着陆跑道(广场或公路)上预设具有受控发射红外光的地面合作目标,实现无人飞行器的视觉全天候自动精确着陆新技术。首先研究得到切实可行的工作过程;然后研制了合作目标,通过理论分析和实验得出,无论能见度高低,8~12 μm中远红外视觉系统探测到的合作目标图像质量远优于可见光视觉系统,研究得到合作目标和背景的温差在170~200 ℃时,成像效果最好。在识别研究中发现,基于传统的不变矩算法对合作目标的识别可靠性稍差,为了进一步准确地识别合作目标,又提出了基于方向链码的合作目标识别算法,该方法的耗时为不变距的96%,但是识别的可靠性比前者有显著提高。 相似文献
104.
105.
空间陀螺仪显式标定与隐式标定方法 总被引:1,自引:0,他引:1
针对航天器陀螺仪误差系数的标定问题,提出了显式与隐式两种标定方法。建立了显式标定与隐式标定方法的状态方程与测量方程,利用扩展Kalman滤波获得了陀螺仪误差系数的高精度估计,同时比较了显式标定与隐式标定的不同,仿真结果表明,在当前参数设置下,显式标定与隐式标定精度基本相同,两种方法得到的误差系数估计相对误差在10%以内,而隐式标定方法实现较为容易,但对航天器姿态测量精度较为敏感。 相似文献
106.
Kaixuan Ni Laura Baudis 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(12):2019-2023
The cryogenic dark matter search (CDMS) and XENON experiments aim to directly detect dark matter in the form of weakly interacting massive particles (WIMPs) via their elastic scattering on the target nuclei. The experiments use different techniques to suppress background event rates to the minimum, and at the same time, to achieve a high WIMP detection rate. The operation of cryogenic Ge and Si crystals of the CDMS-II experiment in the Soudan mine reported spectrum-weighted exposures of 34 (12) kg-d for the Ge (Si) targets after cuts, over the recoil energies 10–100 keV for a WIMP mass of 60 GeV/c2. It gives an upper limit (90% C.L.) of spin-independent WIMP-nucleon cross-section at 1.6 × 10−43 cm2 for a WIMP mass of 60 GeV/c2, starting to constrain predications in supersymmetry models. The two-phase xenon detector of the XENON10 experiment is currently taking data in the Gran Sasso underground lab and promising preliminary results were recently reported. Both experiments are expected to increase their WIMP sensitivity by a one order of magnitude in the scheduled science runs for 2007. 相似文献
107.
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
108.
Yang Zhang Binbin Ni Zheng Xiang Xianguo Zhang Xiaoxin Zhang Xudong Gu Song Fu Xing Cao Zhengyang Zou 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(9):2290-2300
We perform an L-shell dependent inter-satellite calibration of FengYun 3 medium energy electron measurements with POES measurements based on rough orbital conjunctions within 5?min?×?0.1?L?×?0.5 MLT. By comparing electron flux data between the U.S. Polar Orbiting Environmental Satellites (POES) and Chinese sun-synchronous satellites including FY-3B and FY-3C for a whole year of 2014, we attempt to remove less reliable data and evaluate systematic uncertainties associated with the FY-3B and FY-3C datasets, expecting to quantify the inter-satellite calibration factors for the 150–350?keV energy channel at L?=?2–7. Compared to the POES data, the FY-3B and FY-3C data generally exhibit a similar trend of electron flux variations but more or less underestimate them within a factor of 5 for the medium electron energy 150–350?keV channel. Good consistency in the flux conjunctions after the inter-calibration procedures gives us certain confidence to generalize our method to calibrate electron flux measurements from various satellite instruments. 相似文献
109.
110.
基于Internet的汽车检测线远程故障诊断系统 总被引:7,自引:0,他引:7
现代机动车安全性能检测线是综合了通信,电子,自动控制,信号处理和计算机等先进技术的复杂测控系统,因此需在其工作时适时地对其各种状态进行监测。基于Internet的机动车安全性能检测线远程监测系统的解决方案。本讨论了以Web数据库和Socket技术来实现本方案的具体步骤。 相似文献