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941.
视觉辅助遥操作在卫星在轨自维护中的应用 总被引:1,自引:0,他引:1
为了克服时延对空间机器人遥操作的影响,提出了利用视觉技术辅助遥操作进行卫星自维护的方法.针对遥操作数据传输滞后的问题,设计并实现了一种基于视觉的共享控制策略,该策略将维护任务分为自由空间控制与自主视觉伺服控制.在自由空间控制阶段,通过3D图形预测仿真以及实时反馈的视频流,提高了遥操作者的视觉临场感.在自主控制阶段,采用冗余特征视觉伺服控制,克服了系统对标定精度的依赖性,从而提高了整个系统的智能化程度.最后,通过对典型的卫星维护任务实例的分析,验证了该方法的有效性. 相似文献
942.
An approach to inversion of the lunar regolith layer thickness by using multi-channel brightness temperature observation in passive microwave remote sensing is developed. To first make simulation of brightness temperature from the lunar layered media, the lunar regolith layer thickness (d) is proposed being constructed by available lunar DEM (digital elevation mapping) and on site measurements. The physical temperature distribution (T) over the lunar surface is also empirically assumed as a monotonic function of the latitude. Optical albedo of the lunar nearside from the telescopic observation is employed to construct the spatial distribution of the FeO+TiO2 content (S) in the lunar regolith layer. A statistic relationship between the DEM and S of the lunar nearside is further extended to construction of S of the lunar farside. Thus, the dielectric permittivity (ε) of global lunar regolith layer can then be determined. Based on all these conditions (d,T,ε), brightness temperature of the lunar regolith layer in passive microwave remote sensing, which is planned for China's Chang-E lunar project, is numerically simulated by a parallel layering model using the strong fluctuation theory of random media.Then, taking these simulations with random noise as observations, an inversion method of the lunar regolith layer thickness is developed by using three- or two-channels brightness temperatures. When the S is low, and the four channels brightness temperatures in China's Chang-E project are well distinguishable, the regolith layer thickness and physical temperature of the underlying lunar rock media can be inverted by the three-channels approach. When the S becomes high that the brightness temperature at high frequency channels such as 19.35, 37 GHz are saturated, the regolith layer thickness is alternatively inverted only by the two-channels approach.Numerical simulation and inversion approach in this paper make an evaluation of the performance for lunar passive microwave remote sensing, and for future data calibration and validation. 相似文献
943.
基于自校正模糊神经控制的无刷直流传动系统 总被引:1,自引:0,他引:1
范正翘 《北京航空航天大学学报》1998,24(5):529-532
提出了一种自校正模糊神经网络控制器(SCFNNC)来实现无刷直流电动机起动、调速、制动等各运行阶段的性能指标.该SCFNNC是采用调整系统增益参数的方法完成较完善的控制规则的.重点研究了系统自校正增益参数的确定方法,模糊控制器的设计,人工神经网络实现模糊控制规则的方法等.自校正增益参数是根据系统对超调量、转速稳态误差、动态速降的期望值来确定的.设计模糊控制器时是根据系统的性能指标,确定出合适的模糊控制规则表,用于训练神经网络.为使系统的性能达到最佳,采用了自校正模糊神经控制、开关控制和比例控制相结合的复合控制方法,通过数学仿真证实配备SCFNNC的系统具有优良的动、静态特性,及较强的鲁棒性. 相似文献
944.
945.
介绍了用人工神经网络算法确定待复原颅面的软组织厚度及颅面特征点的方法。在计算机辅助颅面复原过程中,通常只能根据颅骨上少数特征点及其所在部位的法向软组织厚度的统计值进行运算。由于现有统计值指标涵盖的年龄较宽泛,导致复原结果缺乏个性。在测定待复原颅骨骨龄的基础上,通过神经网络训练,确定软组织厚度随年龄的变化规律,较精确地计算出与拟复原对象的骨龄相适应的特征点软组织厚度值,并用最小二乘法及曲面法线原理建立数学模型,计算出颅面特征点。最后用基于Delaunay三角剖分的wavelet插值法复原出面貌雏形。 相似文献
946.
航空发动机的放气活门调节规律是一个较为复杂的控制过程。依据大量QAR数据,采用数学分析的方法初步探索了PW4077D型发动机2.5级放气活门开度控制规律。通过对大量数据的统计分析可知,放气活门开度与低压转子转速N1关系最为密切。首先通过数据解码和修正得到各航班标准状态下的N1值;采用非线性回归的数理统计方法分段拟合,得到2.5级放气活门开度与N1的数学模型。经检验,该模型在一定范围内良好地反映了该型发动机2.5级放气活门开度大小的调节规律。 相似文献
947.
王奇利 《西安航空技术高等专科学校学报》2010,28(1)
实验教学是学生获得知识和能力训练的重要途径,工程力学实验是工科院校学生的一门技术基础课。尝试利用现代网络技术和3Dmax软件,结合我校的力学实验课教学,开发一套基于网络的工程力学实验教学系统,作为对理论教学和实验室教学的补充,取得很好效果。 相似文献
948.
E.G. Cordaro E. Olivares D. Galvez D. Salazar-Aravena D. Laroze 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
We present the results of three years of continuous operations and the principal characteristics of our new 3He neutron monitors installed in the Chilean Network of Cosmic-Ray Observatories. During the years 2004 and 2005, we began the construction of this International Geophysical Year (IGY)-type 3He neutron monitor, with the intention of replacing the older proportional tubes of the BF3. These new monitors are installed in stations at locations ranging from the near-equatorial zone to the Antarctic zone. As a reference system, we used our own BF3 neutron monitors and previously complemented the collected data with a Monte Carlo simulation for the proton-yield function response of the Putre neutron monitor. Herein, we present for the first time the data obtained from our new high-mountain observatory located in the Altiplanic zone. 相似文献
949.
B.G.B. Solheim 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
The European Modular Cultivation System (EMCS) on the ISS allows long-term biological experiments, e.g. on plants. Video cameras provide near real-time 2D images from these experiments. A method to obtain 3D coordinates and stereoscopic images from these 2D images has been developed and is described in this paper. The procedure was developed to enhance the data output of the MULTIGEN-1 experiment in 2007. One of the main objectives of the experiment was to study growth movements of the Arabidopsis plants and the effect of gravity on these. 3D data were important during parts of the experiment and the paper presents the method developed to acquire 3D data, the accuracy of the data, limitations to the technique and ways to improve the accuracy. Sequences of 3D data obtained from the MULTIGEN-1 experiment are used to illustrate the potential of this newfound capability of the EMCS. In the experiment setup, a positional depth accuracy of about ±0.4 mm for relative object distances and an absolute depth accuracy of about ±1.4 mm for time dependent phenomena was reached. The ability to both view biological specimens in 3D as well as obtaining quantitative 3D data added greatly to the scientific output of the MULTIGEN-1 experiment. The uses of the technique to other researchers and their experiments are discussed. 相似文献
950.
Xiao Xiao Yang Chen 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(3):416-423
We present the preliminary results of a Chandra X-ray study of N132D, a young shell-like supernova remnant (SNR) in the Large Magellanic Cloud. The equivalent width maps of emissions from O, Ne, Mg, Si, and S are provided. Spatially resolved spectral analysis for the small-scale regions were tentatively performed. X-ray spectra of the interior can be described with a single-thermal model. The faint interior regions have lower density, higher temperature above 1 keV than that of bright interior regions. The X-ray spectra along the shell can be phenomenally fitted with either a double-vpshock model or a vpshock + powerlaw model. If the non-thermal component is true, N132D would be listed as another X-ray synchrotron SNR. 相似文献