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1.
国外航天侦察相机和测绘相机发展概况 总被引：5，自引：0，他引：5
航天侦察和测绘是战略武装必不可少的组成部分,航天侦察和测绘相机是对地观测卫星的有效载荷。 该文将简要介绍国外航天侦察和测绘相机发展概况、水平和发展趋势。 相似文献
2.
地基光电观测在同步轨道目标监测领域具有重要作用.为评估单站光电设备对同步轨道目标的实际测定轨能力,利用上海天文台佘山站1.56m望远镜,采用CCD漂移扫描光电技术,对3颗北斗同步卫星开展试验观测,基于卫星精密星历评估目标的测定轨外符精度.结果表明：同步轨道目标的天文定位在方位和俯仰方向上的外符精度均好于0.3\";在单圈次观测情况下,尽管轨道预报精度较低,约为数千米量级,但是观测弧段内定轨精度可优于百米;在多圈次观测情况下,轨道改进效果显著,定轨精度优于50m,外推至4d的轨道预报精度为百米量级.此外,定量评估了每晚不同观测时间跨度下同步轨道目标的测定轨精度,为单站光电设备实际应用提供了参考. 相似文献
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陀螺安装方式及相应的算法编排是稳定平台设计中的一项关键技术。针对机载对地观测用三轴稳定平台特点,提出了将方位陀螺安装在方位环上,俯仰陀螺和横滚陀螺安装在俯仰环上的陀螺安装方式。利用空间矢量分解理论分析了陀螺输出角速度信号的投影关系及电机控制信号的分配;基于稳定平台系统模型,对理想正交情况和考虑陀螺安装误差情况进行了仿真分析,验证了此种安装方式的可行性和优越性。分析表明,在同等条件下,所提出的安装方式减小了稳定平台的机械尺寸,降低了稳定平台的重量和功耗,实现了三维角速度的正交测量,简化了三轴解耦控制算法。研究结论可为其他三轴稳定平台结构设计和陀螺安装方式设计提供参考。 相似文献
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无轴承开关磁阻电机控制系统的设计与实现 总被引：17，自引：6，他引：11
介绍了无轴承开关磁阻电机的绕组结构和悬浮力原理,简要推导了数学模型。结合数学模型的复杂性详细分析了控制策略,根据控制策略设计了基于TMS320LF2407A的高速DSP芯片为核心控制器件的数模混合控制电路。样机实验结果不仅验证了理论分析的正确性,也表明了所设计控制电路的有效性和可靠性。 相似文献
7.
研究了状态不可测系统的变结构控制问题。构造了系统的状态观测器。为了分析系统的抖振,计入了传感器（测量装置）的动力学。在建立了由对象、观测器和传感器组成的系统的动力学方程之后,研究了滑动模态的稳定性及其特性,并用趋近律方法构造出了变结构控制,还给出了关于抖振的又一解释。 相似文献
8.
Xuemin Zhang Shufan Zhao Rui Song Dulin Zhai 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(11):3536-3544
The artificial low frequency (LF) signals recorded at topside ionosphere from DEMETER satellite were analyzed in this paper, and the typical diurnal and seasonal variations were illustrated around 162?kHz in electric field spectra. The larger power spectrum density (PSD) values in electric field at local nighttime and in winter season all demonstrate the correlation feature of lower plasma content to higher penetration of LF waves into ionosphere. Around Wenchuan earthquake, the comparison of signal-noise-ratio (SNR) values in electric field with each half month during January to May in 2008 and the same half month in May from 2005 to 2007 revealed their lowest values and small covering area around the preparation region of Wenchuan earthquake in 2008. Combined with other researches in VLF radio waves and geochemical observations from satellite, the interaction of ion accumulation and upward movement from gas-water release at surface might be a key factor to disturb the ionospheric plasma density, and then possibly leading to the decrease of low energy penetration of LF radio waves from the artificial transmitted source at ground. 相似文献
9.
T. Flohrer H. Krag H. Klinkrad T. Schildknecht 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
Under ESA contract an industrial consortium including Aboa Space Research Oy (ASRO), the Astronomical Institute of the University of Bern (AIUB), and the Dutch National Aerospace Laboratory (NLR), proposed the observation concept, developed a suitable sensor architecture, and assessed the performance of a space-based optical (SBO) telescope in 2005. The goal of the SBO study was to analyse how the existing knowledge gap in the space debris population in the millimetre and centimetre regime may be closed by means of a passive optical instrument. The SBO instrument was requested to provide statistical information on the space debris population in terms of number of objects and size distribution. The SBO instrument was considered to be a cost-efficient with 20 cm aperture and 6° field-of-view and having flexible integration requirements. It should be possible to integrate the SBO instrument easily as a secondary payload on satellites launched into low-Earth orbits (LEO), or into geostationary orbit (GEO). Thus the selected mission concept only allowed for fix-mounted telescopes, and the pointing direction could be requested freely. Since 2007 ESA focuses space surveillance and tracking activities in the Space Situational Awareness (SSA) preparatory program. Ground-based radars and optical telescopes are studied for the build-up and maintenance of a catalogue of objects. In this paper we analyse how the proposed SBO architecture could contribute to the space surveillance tasks survey and tracking. We assume that the SBO instrumentation is placed into a circular sun-synchronous orbit at 800 km altitude. We discuss the observation conditions of objects at higher altitude, and select an orbit close to the terminator plane. A pointing of the sensor orthogonal to the orbital plane with optimal elevation slightly in positive direction (0° and +5°) is found optimal for accessing the entire GEO regime within one day, implying a very good coverage of controlled objects in GEO, too. Simulations using ESA’s Program for Radar and Optical Observation Forecasting (PROOF) in the version 2005 and a GEO reference population extracted from DISCOS revealed that the proposed pointing scenario provides low phase angles together with low angular velocities of the objects crossing the field-of-view. Radiometric simulations show that the optimal exposure time is 1–2 s, and that spherical objects in GEO with a diameter of below 1 m can be detected. The GEO population can be covered under proper illumination nearly completely, but seasonal drops of the coverage are possible. Subsequent observations of objects are on average at least every 1.5 days, not exceeding 3 days at maximum. A single observation arc spans 3° to 5° on average. Using a simulation environment that connects PROOF to AIUB’s program system CelMech we verify the consistency of the initial orbit determination for five selected test objects on subsequent days as a function of realistic astrometric noise levels. The initial orbit determination is possible. We define requirements for a correlator process essential for catalogue build-up and maintenance. Each single observation should provide an astrometric accuracy of at least 1”–1.5” so that the initially determined orbits are consistent within a few hundred kilometres for the semi-major axis, 0.01 for the eccentricity, and 0.1° for the inclination. 相似文献
10.
任务分配是对地观测分布式卫星系统(Distributed Satellites System, DSS)自主协作运行过程中的一个重要环节. 针对任务分配中的约束满足问题(Constraint Satisfaction Problem, CSP), 以DSS完成任务总耗能最少为原则, 构建了任务分配问题的CSP模型, 并引入MAS理论中的合同网协议, 给出模型的求解算法, 通过仿真算例对模型和算法进行了验证. 相似文献