共查询到20条相似文献,搜索用时 62 毫秒
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介绍了基于TFT-LCD的动态星模拟器的工作原理及星点位置误差的计算方法。利用经纬仪对动态星模拟器显示的网格星点进行测量,计算了各星点的位置误差及修正系数。对网格上星点的修正系数进行分区处理,并利用Matlab软件对各分区的修正系数进行曲线拟合,得到修正系数关于星点位置(方位或俯仰)坐标的方程。结果表明,修正后星点的位置误差均小于35″,满足动态星模拟器的设计要求。 相似文献
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高能碰撞末态粒子在相空间的动力学分布存在着非均匀因素的影响,通过对这种非均匀因素影响的研究,引入了修正系数,和到了拟事修正曲线的判据,给出了计算修正系数的方法。 相似文献
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对不良导体导热系数测量原理的修正 总被引:11,自引:0,他引:11
对稳态法测量原理进行了较深入的探讨,指出了用稳态法测定非金属材料导热系数的不足之处,并作了一定的修正,从而推出了计算导热系数的新公式。通过测定结果,验证了修正后的导热系数计算公式的正确性和合理性。 相似文献
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采用密度矩阵方法描述了两模反向耦合.在两模反向耦合情况下,用随机畸变的功率耦合系数(即模混合系数)对密度矩阵运动方程作了修正,并获得了修正后方程的精确解析解的表达式. 相似文献
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提出了一种基于场景的红外图像非均匀性校正算法。该算法结合了两点定标校正算法和基于场景的改进的恒定统计算法,将两点校正算法的校正系数作为恒定统计算法的系数初值,并引入阈值进行运动状态检测,对运动场景和非运动场景分别进行系数更新。实验表明,该算法可以实现对红外图像非均匀性的校正,对于本文实验中的视频图像,在100帧时算法收敛,其收敛时间优于其他传统基于场景的非均匀性校正算法,并一定程度上抑制了"鬼影"现象。 相似文献
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Minas K. Balyan 《Journal of synchrotron radiation》2014,21(2):449-451
Taking into account background correction and using Fourier analysis, a numerical method of an object image correction using an X‐ray dynamical diffraction Fraunhofer hologram is presented. An example of the image correction of a cylindrical beryllium wire is considered. A background correction of second‐order iteration leads to an almost precise reconstruction of the real part of the amplitude transmission coefficient and improves the imaginary part compared with that without a background correction. Using Fourier analysis of the reconstructed transmission coefficient, non‐physical oscillations can be avoided. This method can be applied for the determination of the complex amplitude transmission coefficient of amplitude as well as phase objects, and can be used in X‐ray microscopy. 相似文献
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Timoshenko's theory of vibrating beams requires a shear correction factor to correctly take into account the effects of shear deformation for different beam cross-sections. This correction is crucial for a precise determination of the shear modulus from the resonant frequencies. Hutchinson's beam theory is used to derive a new shear correction coefficient for anisotropic materials. A comparison is made with other shear coefficients for anisotropic materials published in the literature. Computer-simulated spectra are used to validate the new anisotropic shear correction coefficient. 相似文献
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基于529单元自适应光学(AO)系统,分析了变形镜到哈特曼波前传感器的斜率响应矩阵的稀疏特性、波前复原中迭代矩阵的稀疏特性.在变形镜驱动器间距不变的条件下,研究了驱动器交连值对斜率响应矩阵稀疏度、迭代矩阵稀疏度以及AO系统校正能力的影响.研究表明,斜率响应矩阵和迭代矩阵的稀疏度随交连值的增大而减小;交连值过大或者过小都会影响AO系统的稳定性和校正能力.最后,综合斜率响应矩阵和迭代矩阵的稀疏度、系统稳定性和校正能力,给出了交连值的合理取值范围. 相似文献
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Magnetic resonance fingerprinting (MRF) pulse sequences often employ spiral trajectories for data readout. Spiral k-space acquisitions are vulnerable to blurring in the spatial domain in the presence of static field off-resonance. This work describes a blurring correction algorithm for use in spiral MRF and demonstrates its effectiveness in phantom and in vivo experiments. Results show that image quality of T1 and T2 parametric maps is improved by application of this correction. This MRF correction has negligible effect on the concordance correlation coefficient and improves coefficient of variation in regions of off-resonance relative to uncorrected measurements. 相似文献
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Recently, there has been much attention devoted to resolving the quantum corrections to the BekensteinHawking black hole entropy. In particular, many researchers have expressed a vested interest in the coefficient of the logarithmic term of the black hole entropy correction term. In this paper, we calculate the correction value of the black hole entropy by utilizing the generalized uncertainty principle and obtain the correction term caused by the generalized uncertainty principle. Because in our calculation we think that the Bekenstein-Hawking area theorem is still valid after considering the generalized uncertainty principle, we derive that the coefficient of the logarithmic term of the black hole entropy correction term is positive. This result is different from the known result at present. Our method is valid not only for four-dimensional spacetimes but also for higher-dimensional spacetimes. In the whole process, the physics idea is clear and calculation is simple. It offers a new way for studying the entropy correction of the complicated spacetime. 相似文献