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21.
基于有效准则矢量生成的成像调度方法 总被引:3,自引:0,他引:3
进行高效成像调度是卫星控制的一项重要任务。通过将成像需求序列对应为有向图中的成像路径,结合成像调度问题特点,基于多个优化准则使用支配关系对成像路径质量进行综合评价,提出有效准则矢量生成算法。利用成像有向图的拓扑特性,基于时间顺序顶点选择策略进行顶点标记更新,生成出有向图中所有的有效准则矢量及每个准则矢量对应的一条Pareto优化路径。实验结果表明,获得的有效准则矢量数目小,算法可以在较短时间内得到多条具有代表性的优化成像路径,满足卫星成像调度的时间和性能要求。 相似文献
22.
提出了一种适用于大距离徒动高分辨率星载合成孔径雷达 (SAR)精确成像的改进Chirp Scaling(CS)成像处理算法 ,以及实现单视图象斑点噪声抑制的基于目标检测的增强无偏最大后验概率 (TDRGMAP)方法。采用这种高精度成像处理方法和单视图像斑点噪声抑制方法 ,可以实现星载 SAR高空间分辨率和高辐射分辨率的雷达图像。 相似文献
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New design simulation for a high-altitude dual-balloon system to extend lifetime and improve floating performance 总被引:1,自引:0,他引:1
This paper presents a comprehensive simulation for a high-altitude dual-balloon system which consists of zero- and super-pressure balloons. Preliminary calculations were established to describe the basic concept of the new integrated system. A mathematical model was investigated to simulate the ascending and floating processes which considered the atmospheric conditions and thermodynamic variations. Based on the simulation, results showed that the floating altitude stability between daytime and nighttime was improved. This integrated system supports higher floating altitude levels than those of ordinary balloons and extends the lifetime of floating balloon systems. Moreover, results demonstrated that the integrated system was lighter than ordinary balloons, saving useful weight for effective payload. Furthermore, exploiting the advantages of both kinds of balloons while avoiding the difficulties was a significant goal in the current design to promote the floating performance of high-altitude balloons technology. 相似文献
25.
Due to the deficiencies in the conventional multiple-receiver localization systems based on direction of arrival(DOA) such as system complexity of interferometer or array and amplitude/phase unbalance between multiple receiving channels and constraint on antenna configuration,a new radiated source localization method using the changing rate of phase difference(CRPD)measured by a long baseline interferometer(LBI) only is studied. To solve the strictly nonlinear problem, a two-stage closed-form solution is proposed. In the first stage, the DOA and its changing rate are estimated from the CRPD of each observer by the pseudolinear least square(PLS) method,and then in the second stage, the source position and velocity are found by another PLS minimization. The bias of the algorithm caused by the correlation between the measurement matrix and the noise in the second stage is analyzed. To reduce this bias, an instrumental variable(IV) method is derived. A weighted IV estimator is given in order to reduce the estimation variance. The proposed method does not need any initial guess and the computation is small. The Cramer–Rao lower bound(CRLB) and mean square error(MSE) are also analyzed. Simulation results show that the proposed method can be close to the CRLB with moderate Gaussian measurement noise. 相似文献
26.
中国深空网首次△DOR联合测轨试验分析 总被引:1,自引:0,他引:1
通过分析中国深空网首次△DOR(Delta Differential One way Ranging,双差分单向测距)联合测轨试验的干涉测量事后数据,重点从观测量随机精度、闭合时延等方面讨论了国内深空网与国内VLBI(Very Long Baseline Interferometry,甚长基线干涉测量)观测网、国内深空网与国际深空网的联合干涉处理情况,并与ESOC(European Space Operation Center,欧洲空间操作中心)数据处理结果进行了比对.试验结果表明:我国深空网已具备独立或联合开展深空探测器导航测轨的系统支持能力;深空站系统具备高速率数据接收、采集、记录、传输能力,采集数据处理精度优于1 ns;深空网干涉测量信号处理中心具备多体制信号的干涉处理分析能力,其分析精度与ESOC处理精度差异在0.1 ns量级. 相似文献
27.
长配管、高落差空调系统的计算机仿真与试验研究 总被引:1,自引:0,他引:1
空调系统在长配管、高落差情况下其运行性能和可靠性会受到影响。建立数学模型预测长配管、高落差空调系统的性能,可以提供给用户准确的性能资料,指导用户合理安装空调器,提高产品的可靠性。 相似文献
28.
Arastou Zarei Reza Shah-Hosseini Sadegh Ranjbar Mahdi Hasanlou 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(12):3979-3993
In recent years, land surface temperature (LST) has become critical in environmental studies and earth science. Remote sensing technology enables spatiotemporal monitoring of this parameter on large scales. This parameter can be estimated by satellite images with at least one thermal band. Sentinel-3 SLSTR data provide LST products with a spatial resolution of 1 km. In this research, direct and indirect validation procedures were employed to evaluate the Sentinel-3 SLSTR LST products over the study area in different seasons from 2018 to 2019. The validation method was based on the absolute (direct) evaluation of this product with field data and comparison (indirect) evaluation with the MODIS LST product and the estimated LST using the non-linear split-window (NSW) algorithm. Also, two emissivity estimation methods, (1) NDVI thresholding method (NDVI-THM) and (2) classification-based emissivity method (CBEM), were used to estimate the LST using the NSW method according to the two thermal bands of Sentinel-3 images. Then, the accuracy of these methods in estimating LST was evaluated using field data and temporal changes of vegetation, which the NDVI-THM method generated better results. For indirect evaluation between the Sentinel-3 LST product, MODIS LST product, and LST estimated using NSW, four filters based on spatial and temporal separates between pairs of pixels and pixel quality were used to ensure the accuracy and consistency of the compared pairs of a pixel. In general, the accuracy results of the LST products of MODIS and Sentinel-3, and LST estimated using NSW showed a similar trend for LST changes during the seasons. With respect to the two absolute and comparative validations for the Sentinel-3 LST products, summer with the highest values of bias (?1.24 K), standard deviation (StDv = 2.66 K), and RMSE (2.43 K), and winter with the lowest ones (bias of 0.14 K, StDv of 1.13 K, and RMSE of 1.12 K) provided the worst and best results for the seasons in the period of 2018–2019, respectively. According to both absolute and comparative evaluation results, the Sentinel-3 SLSTR LST products provided reliable results for all seasons on a large temporal and spatial scale over our studied area. 相似文献
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In order for future imaging spacecraft to meet higher resolution imaging capability, it will be necessary to build large space telescopes with primary mirror diameters that range from 10 m to 20 m and do so with nanometer surface accuracy. Due to launch vehicle mass and volume constraints, these mirrors have to be deployable and lightweight, such as segmented mirrors using active optics to correct mirror surfaces with closed loop control. As a part of this work, system identification tests revealed that dynamic disturbances inherent in a laboratory environment are significant enough to degrade the optical performance of the telescope. Research was performed at the Naval Postgraduate School to identify the vibration modes most affecting the optical performance and evaluate different techniques to increase damping of those modes. Based on this work, tuned mass dampers (TMDs) were selected because of their simplicity in implementation and effectiveness in targeting specific modes. The selected damping mechanism was an eddy current damper where the damping and frequency of the damper could be easily changed. System identification of segments was performed to derive TMD specifications. Several configurations of the damper were evaluated, including the number and placement of TMDs, damping constant, and targeted structural modes. The final configuration consisted of two dampers located at the edge of each segment and resulted in 80% reduction in vibrations. The WFE for the system without dampers was 1.5 waves, with one TMD the WFE was 0.9 waves, and with two TMDs the WFE was 0.25 waves. This paper provides details of some of the work done in this area and includes theoretical predictions for optimum damping which were experimentally verified on a large aperture segmented system. 相似文献