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991.
针对航天器精确预测与健康管理的需求,将粒子群算法、模糊数学与支持向量机的优势相结合,提出了一种粒子群模糊支持向量机预测方法。针对某卫星南帆板输出电流参量的预测实例,设计了总平均绝对误差、总平均绝对百分比误差、总均方根误差三个预测结果评价指标,对不同步长情况下的预测结果进行了比较,证明了粒子群优化模糊支持向量机预测方法的有效性。通过对比粒子群优化模糊支持向量机模型、灰色粒子群神经网络优化模型、粒子群神经网络模型、灰色模型预测的总平均绝对百分比误差,结果证明粒子群优化模糊支持向量机的预测精度和效率较高,在航天器参量预测领域具有较好的应用前景。 相似文献
992.
针对卫星网络通信路径发生改变引起往返时延突变,导致现有的拥塞控制机制中超时重传时间估计不准确,并对拥塞窗口计算产生不利影响的问题,提出一种基于链路长度的带宽估计TCPW\|BLC算法。该算法通过计算通信链路长度合理调整拥塞窗口、慢启动阈值及超时重传定时器中相关参数的增益因子,使拥塞控制算法在往返时延突变情况下仍保持较高吞吐量,适应卫星网络动态环境特性。NS2仿真结果表明,TCPW\|BLC算法相比TCPW算法在卫星网络中吞吐量性能提高了2.8%,有效降低了时延突变给拥塞控制机制造成的不利影响。 相似文献
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996.
针对球面运动机构驱动方式问题,提出了一种新型的二自由度液压驱动球面运动关节机构,该机构利用超全周转动马达及舵叶摆动马达作为驱动,采用了滑轨支撑框架位置测量系统,可以实现超全周转动;给出了两驱动马达各自的油路设计方案,在机构的不同部位采取了合理的密封方法;由机构的工作原理推导了正逆运动学方程及速度雅可比矩阵,得出了机构的奇异位形;分析了机构的灵巧度性能指标,通过仿真得到了机构性能较优时的工作空间.该球形关节机构具有结构紧凑、运动精度高、负载大、并且能够实现全方位输出的特点. 相似文献
997.
Qiumin Dai Xiande Fang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
Solar radiation is one of the major factors that dominate the thermal behaviors of aerostats in the daytime and the primary energy source of high altitude long endurance aerostats. Therefore, it is necessary to propose an accurate model to predict the solar irradiances. A comprehensive review of the well-known solar radiation models is conducted to help develop the new model. Based on the analysis of the existing models and the available radiation data, the extensive computer tests of the regression and optimization are conducted, from which the new solar radiation model for direct and diffuse irradiances under clear sky conditions is proposed. The new model has excellent prediction accuracy. The coefficient of determination for direct radiation is 0.992, with the root mean square error (RMSE) of 16.9 W/m2 and the mean absolute error (MAE) of 2.2%. The coefficient of determination for diffuse radiation is 0.86, with RMSE = 8.7 W/m2 and MAE = 9.9%. Comparisons with the well-known existing models show that the new model is much more accurate than the best existing ones. 相似文献
998.
A direct performance comparison between the four-hole aero-ramp injector and single transverse injector in a dual-mode scramjet combustor was conducted. The mixing characteristics of two injectors were calculated by solving the three-dimensional (3-D) compressible Reynolds-averaged Navier-Stokes equations (RANS), with the help of the shear-stress-transport (SST) k-ω turbulence model. The numerical results show that the far field mixing efficiency of the aero-ramp injector is higher than that of the single transverse injector. High enthalpy vitiated air was heated to a total temperature of 1200K by hydrogen-oxygen combustion, entering the isolator entrance at a Mach number of 2.0. Non-reacting experimental conditions involved sonic injection of nitrogen to safely simulate ethylene injected into the combustor at a jet-to-free stream momentum flux ratio of 2.6. Schlieren photographs were obtained to analyze the shock structure around the injectors. Reacting test conditions involved sonic injection of ethylene at the jet-to-free stream momentum flux ratios ranging from 0.5 to 2.7. High speed camera was used to capture the flame structures in the near-field combustion. The experimental results show that the aero-ramp injector produce sustained combustion over a wider range of fuel-air ratios than the single transverse injector. At the identical jet-to-free stream momentum flux ratio, the aero-ramp has a larger isolator margin than the single transverse injector, demonstrating a better ability for avoiding overflows. However, the air specific impulse and total temperature recovery of two injectors, which are calculated by the one-dimensional (1-D) performance analysis code, are almost identical. 相似文献
999.
建立了带有太阳翼的挠性航天器的姿态动力学模型,应用改进的罗德里格参数来描述姿态运动学模型。针对挠性航天器模型参数不确定性和环境干扰等问题,提出了变论域自整定模糊比例积分微分(PID)控制方案,构建了计算简单并且可以达到控制精度的伸缩因子。基于Matlab/Simulink进行了仿真验证,结果表明,变论域自整定模糊PID 控制响应速度比传统PID控制、模糊PID控制快350s,且无超调,不仅能够使航天器完成对目标姿态的机动,而且能够有效地抑制挠性太阳翼的振动。 相似文献
1000.
Jun Niu Li-bin Weng Han-xian Fang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(3):1204-1213
Ionospheric sporadic E layer refers to localized thin irregularity with enhanced plasma density appearing in the height range of ionospheric E layer (~90–130?km). The much higher electron density in the sporadic E layer than the background ionosphere would cause sudden TEC enhancement in the occultation TEC profile. A wavelet decomposition and reconstruction method is applied to extract the TEC fluctuation in this paper, and then index is defined to represent the intensity of the sudden TEC enhancement. index is compared with sporadic E critical frequency () observed by the ionosonde. The results show a well linear correlation between them with mean correlation coefficient about 0.7. Thus, an empirical linear model is established to inverse the . The monthly/hourly mean values and global distribution of sporadic E intensity and occurrence ratio are calculated using this method based on the COSMIC occultation data from 2007 to 2011. The statistical analysis results indicate that it is feasible to inverse the based on the occultation TEC profile data and the inversion results can be applied to the long-term global variations of sporadic E investigations. 相似文献