环境减灾-1B卫星遥感数据在干旱监测中的应用

以2010-2011年发生在山东省的秋、冬、春三季连旱为例,介绍了环境减灾-1B（HJ-1B）卫星遥感数据在干旱监测中的应用。获取了山东省干旱发展顶峰时段的HJ-1B卫星采集的多光谱和热红外遥感影像,利用ENVI 4.7遥感数据处理平台对山东全省的归一化植被指数和地面温度进行了反演,在此基础上计算了山东全省的植被供水指数,并据此将山东省的干旱情况划分为5级,对该干旱监测结果进行了分析。为了验证结论的可靠性,将干旱监测结果与全国降水距平百分率进行了对比,对比结果表明两者一致性较好。文章提供了HJ-1B卫星遥感数据在干旱监测方面的一个实例,其监测结果为相关减灾部门的救灾工作提供了重要的参考,同时也为HJ-1B卫星遥感数据在干旱监测方面的业务化运营提供了一个通用的方法。     

实验室条件下IRMSS遥感器MTF与遥感图像参数的相关分析设计与性能评估

调制传递函数MTF(ModuleTransferFunction)在物理光学理论中 ,是光学系统成像性能的综合评价指标。遥感器MTF的性能变化会导致遥感图像的质量变化 ,遥感图像质量的变化则导致描述遥感图像的参数的变化。文章以CBERS - 1的 0 2星IRMSS遥感器为例 ,在实验室条件下模拟遥感器在轨运行的成像过程并获得图像数据 ,MTF可通过专业仪器直接测量 ,然后再进行MTF与遥感图像参数的相关分析 ,从而确定出与MTF相关性最强的图像参数。文章的相关分析采用SPSS统计分析软件完成     

考虑燃料均衡的卫星编队队形重构技术

在卫星编队队形重构过程中,如何在实现编队整体燃料消耗较少的同时使得各子卫星燃料消耗均衡,能够有效地提高卫星编队整体的寿命。提出了一种基于虚拟中心位置可变的卫星编队队形重构新方法。该方法以虚拟中心位置为寻优变量,以首末脉冲时刻可优化的双脉冲规划作为单星轨道机动策略,将编队队形重构问题转化为混合0-1数学规划问题。仿真结果表明,该优化算法在实现整体燃料次优的同时,兼顾了各星当前的燃料剩余水平,实现了各子卫星的燃料均衡。     

FCD1软脆光学镜片的高效研磨加工

针对FCD1软脆光学镜片高效高成品率的精密加工问题,本研究提出了一种使用复合结合剂金刚石丸片的精研加工技术,其金刚石丸片研具采用了金属、树脂和添加剂等复合结合剂。在精研过程中,丸片表层金刚石磨粒对工件的切深一致性避免了工件表面易出现的深划痕,可有效减少后道抛光工序加工时间,从而提高FCD1软脆光学镜片的生产效率和成品率。     

一种适于动态环境的盲多用户检测算法

比较两种盲多用户检测算法在动态环境中的收敛性能,并通过计算机进行模拟仿真。其中一种是能随输入信号矢量变化而变化的变步长最小输出能量盲算法;另一种是既保持最小输出能量检测器的全局收敛性,又具有最小均方误差检测器高输出信干比优点的判决反馈变步长盲算法。利用前者在动态强干扰下收敛快及后者在稳态时输出信干比高的优势,将二者结合起来应用到动态环境中,提高系统性能,同时抑制多址干扰和窄带干扰。     

CBERS-1卫星红外多光谱扫描仪扫描子系统

文章介绍了CBERS -1卫星红外多光谱扫描仪(IRMSS)关键部件扫描子系统研制与应用情况。     

嫦娥一号月球探测卫星研制综述

嫦娥一号卫星是我国第一个月球探测卫星,将实现对月球的环绕探测。嫦娥一号卫星的研制和发射是我国深空探测活动的开端,在我国航天史上将成为继人造卫星和载人航天后的第三个里程碑。与近地卫星相比,嫦娥一号卫星面临更复杂的控制过程和环境,因此,嫦娥一号卫星必须突破一系列的关键技术,实现既定的任务目标。文章介绍了嫦娥一号卫星的任务目标、主要技术方案和研制过程;概要性地说明了嫦娥一号卫星的研制过程。     

战术导弹控制系统滚动回路的一种设计方法

结合近程战术地地导弹控制系统滚动回路的设计，讨论了整个设计过程中的设计思路和设计方法。针对导弹的弹体滚动运动参数在较大范围内变化的特点，将回路校正网络设计为变参数校正网络。设计中，使用ＩＥＡＳ语言编程对滚动回路单通道和控制回路三通道进行计算机仿真，经多次协调设计，结果令人满意。给出了部分仿真结果。     

The effect of neglecting VLBI reference station clock offsets on UT1 estimates

Very Long Baseline Interferometry (VLBI) allows to monitor universal time (UT1) by conducting regular international experiments. Such dedicated observation networks are equipped with different hardware components, which require different processing strategies when the data are correlated. As the timing units at each stations are usually offset with respect to universal time (UTC) this effect should be considered during correlation processing. Thus, it is investigated how neglecting of these offsets theoretically impacts the estimation of UT1. Three different strategies for the proper handling of the timing offset will be discussed and their advantages/drawbacks will be pointed out. Moreover, it is studied how neglecting of these timing offsets affects UT1 time-series and how such a missing correction can be applied a posteriori. Although the discussed effect is for most of the UT1 experiments smaller than the formal error of the estimates, it is important to consider station clock offsets properly in next-generation VLBI systems, which are expected to improve accuracy of results by about one order of magnitude.     

Spatial heterogeneity in the radiogenic activity of the lunar interior: Inferences from CHACE and LLRI on Chandrayaan-1

In the past, clues on the potential radiogenic activity of the lunar interior have been obtained from the isotopic composition of noble gases like Argon. Excess Argon (40) relative to Argon (36), as compared to the solar wind composition, is generally ascribed to the radiogenic activity of the lunar interior. Almost all the previous estimates were based on, ‘on-the-spot’ measurements from the landing sites. Relative concentration of the isotopes of ⁴⁰Ar and ³⁶Ar along a meridian by the Chandra’s Altitudinal Composition Explorer (CHACE) experiment, on the Moon Impact Probe (MIP) of India’s first mission to Moon, has independently yielded clues on the possible spatial heterogeneity in the radiogenic activity of the lunar interior in addition to providing indicative ‘antiquity’ of the lunar surface along the ground track over the near side of the moon. These results are shown to broadly corroborate the independent topography measurements by the Lunar Laser Ranging Instrument (LLRI) in the main orbiter Chandrayaan-1. The unique combination of these experiments provided high spatial resolution data while indicating the possible close linkages between the lunar interior and the lunar ambience.