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951.
952.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2020,65(1):650-662
Multipath effects on code observables account for one of the major error sources in high-accuracy Global Positioning System (GPS)-based positioning, atmosphere sounding and timing applications. The multipath hemispherical model (MHM) represents one of the most widely used methods of mitigating code multipath effects by taking advantage of their spatial repeatability. The use of MHM usually assumes that the receiver code biases (RCBs) are time-invariant; however, this assumption is not always valid, as RCBs and linear combinations thereof (differential code biases, for instance) have long been found to be time-varying over a period of one day. In this contribution, we propose an extended multipath hemispherical model (EMHM) that is capable of mitigating the code multipath effects in the presence of time-varying RCBs. Consequently, the proposed EMHM has two advantages. First, the EMHM gives rise to code multipath corrections with improved reliability because it addresses the intraday variability of RCBs. Second, more interestingly, the EMHM allows easy and effective calibration of short-term temporal variations, if any, in the RCB on each frequency. These advantages are hopeful to benefit GPS code-related applications. 相似文献
953.
针对红外搜索跟踪系统(IRST)双机协同被动探测定位作战使用中,机动目标建模与实际运动失配造成定位误差偏大的问题,研究了一种基于曲线模型的自适应滤波新方法。该方法改进了传统方法根据方向角估计转弯率以及基于帧间插分线加速度估计切向加速度的思路,将转弯率及线加速度联合作为状态变量进行了状态扩维,并推导了扩维后的过程噪声协方差表达式,在缓解传统两层滤波结构带来的计算量大问题外,也提高了切向加速度的估计精度。另外基于反正切函数的值域,结合方向角在四象限间的转移关系,优化了方向角的设计。通过IRST双机协同仿真实例,验证了所提方法对机动目标的适应性更强、目标定位精度更高。 相似文献
954.
Hussain J. Nasiha Palanisamy Shanmugam Ranganathan Sundaravadivelu 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(11):3473-3488
A robust method has been developed for estimating sediment settling velocity (ws) from high resolution optical remote sensing data in estuarine, coastal and harbor waters. This method estimates settling velocity as a function of the drag coefficient (Cd), Reynolds number (Re), grain size (D50), specific gravity (ΔSG) and grain shape (in terms of the Corey Shape Factor – CSF). These parameters were derived from the particulate inherent optical properties such as backscattering (bbp), beam attenuation (cp), suspended sediment concentration and turbidity using Landsat 8 OLI and HICO data. Preliminary results for the Gulf of Cambay in the eastern Arabian Sea and Yangtze river estuary in the East China Sea, showed that satellite-retrieved settling velocities (m?s?1) varied from very low values in clear oceanic waters, intermediate values in coastal waters, to very high values in river plumes and sediment-laden coastal waters. The remote sensing retrievals of sediment properties and their settling velocities were generally consistent with the field and laboratory results, which indicate that the proposed methodology will have important implications in various coastal engineering, environmental and management studies. 相似文献
955.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2020,65(8):2018-2035
The Faculty of Mathematics, Physics and Informatics of Comenius University in Bratislava, Slovakia (FMPI) operates its own 0.7-m Newtonian telescope (AGO70) dedicated to the space surveillance tracking and research, with an emphasis on space debris. The observation planning focuses on objects on geosynchronous (GEO), eccentric (GTO and Molniya) and global navigation satellite system (GNSS) orbits. To verify the system’s capabilities, we conducted an observation campaign in 2017, 2018 and 2019 focused on astrometric and photometric measurements. In last two years we have built up a light curve catalogue of space debris which is now freely available for the scientific community. We report periodic signals extracted from more than 285 light curves of 226 individual objects. We constructed phase diagrams for 153 light curves for which we obtained apparent amplitudes. 相似文献
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957.
为了降低弹载星惯组合(Stellar-INS)飞行中段对调姿观星的要求,提高星惯组合姿态精度,提出了大视场(LFOV)星惯组合深度融合导航方法。小视场(NFOV)星敏感器输出星矢量为主,大视场星敏感器可同时输出姿态和星矢量信息,分别推导了基于星敏感器输出姿态和星矢量信息的观测方程,分析了星矢量和姿态观测方法之间的关联性。建立了包含星惯安装误差、陀螺误差以及初始平台误差角的星惯组合全误差项模型,基于线性卡尔曼滤波给出了深度融合导航方法。开展了数学仿真验证,分析了不同调姿观星路径约束下,大/小视场星惯组合性能差异。结果表明,大视场星惯组合深度融合导航方法不仅可以降低调姿观星约束要求,还可以实现组合姿态性能提升。 相似文献
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959.
960.
步进电机转速稳定度的测定与分析 总被引:2,自引:0,他引:2
在分析低速扫描中步进电机转速质量影响的基础上,介绍了用光电编码器测量转速稳定度的方法以及判定标准,并讨论了不同条件下步距角、惯性负载和微步距驱动对步进电机转速稳定度的影响。 相似文献