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71.
本文用化学沉积法和电化学沉积法制备太阳能电池用半导体薄膜硫化镉(CdS),对成膜的影响因素进行了测试。结果表明,化学沉积CdS质量较好,沉积速度较慢,受pH的影响较大,且水浴容器壁上沉积有大量的CdS膜。电化学沉积CdS的电流密度在0.5~2.5 m A/cm 2 的范围内,沉积速度快,材料消耗少,但是对电流密度过于敏感,成膜参数难以控制。  相似文献   
72.
基于SAGWO算法的UCAVs动态协同任务分配   总被引:1,自引:2,他引:1  
通过分析无人作战飞机(UCAV)优势概率和任务联合威胁以及定义任务时间,建立了以目标价值毁伤、编队损耗代价和时间消耗为性能指标的多无人作战飞机(UCAVs)多约束动态任务分配数学模型,采用改进的灰狼优化(GWO)算法对数学模型进行求解;针对基本GWO算法求解早熟的缺点,给出了自适应调整策略和跳出局部最优策略,引入了二次曲线控制方法;对UCAVs动态协同任务分配特点,设计了目标任务序列编码方式,提出了基于自适应GWO(SAGWO)算法的UCAVs多目标动态任务分配方法。从静态与动态2种情况分别对该方法进行仿真验证;仿真结果表明,该方法是有效的,相比较于其他算法,其优化过程快速精准。   相似文献   
73.
传统的标准太阳电池标定方法分为高空标定与地面标定,地面标定方法已纳入国际标准。地面标定由于操作简便、标定结果较为精准目前被广泛应用。太阳电池标定结果准确与否对航天器电源系统姿态敏感期、地面环境模拟的设计具有重要意义。本文对太阳电池地面标定方法展开研究,根据国家标准中地面标定方法原理研制了便携式、高准确度的地面标定测试设备,包括准直孔、太阳电池托盘、太阳跟踪器等标定装置,使地面标定过程简易化,对航天用太阳电池地面标定有着重要意义。  相似文献   
74.
空间实验室大面积太阳电池阵技术研究   总被引:3,自引:0,他引:3  
介绍了空间实验室大面积太阳电池阵的方案构型,并进行了模态分析、热结构耦合分析和动力学仿真分析。生产出了全尺寸的集成演示样机,进行了展开试验、主展开机构的模态试验,以及半刚性太阳电池板和二自由度驱动机构的振动试验。计算和试验结果表明,技术方案是可行的。  相似文献   
75.
表面再结晶对定向凝固高温合金高周疲劳行为的影响   总被引:1,自引:0,他引:1  
采用悬臂旋转弯曲试验,研究定向凝固DZ4合金在喷丸预变形及热处理后产生的再结晶层对高周疲劳寿命的影响.结果表明,DZ4合金经过一定程度的预变形,在随后的高温热处理后表面会产生一定厚度的再结晶;再结晶层对DZ4合金高周疲劳寿命有一定影响;在一定喷丸强度范围内,随喷丸强度增加,疲劳寿命先减小后增大.  相似文献   
76.
地球同步轨道(GEO)卫星在轨的主要环境干扰力矩为太阳光压力矩和重力梯度力矩,干扰力矩的累积效应表现为飞轮转速的变化,需要通过外力矩进行角动量卸载避免飞轮饱和。由于GEO磁场极弱,卫星无法使用磁力矩卸载,只能通过喷气卸载,而喷气将对卫星轨道产生影响,因此需要尽可能延长卸载周期。针对配置双对称太阳电池阵GEO卫星的角动量管控需求,首先建立卫星在惯性空间中角动量积累模型,并映射到卫星本体系中,得到本体系中的角动量变化规律。通过飞轮在轨转速遥测数据,精确辨识获取环境干扰力矩特征参数,获得真实可靠的干扰模型。以角动量卸载周期最长为原则,基于在轨环境干扰模型制定角动量管控策略,并准确预估下次角动量卸载时间。经在轨数据处理与分析表明:提出的角动量管控策略,可有效将飞轮的角动量卸载周期提升为原来的2倍,有效提升卫星在轨应用效能,具有实际工程意义。  相似文献   
77.
针对传统脉冲重复间隔(PRI)分选算法在估计PRI方面存在的不足,提出了一种对PRI周期信号的周期进行精确估计的算法。该算法首先从待分选脉冲序列中提取出属于一部雷达的脉冲样本,然后利用同余方程的余数周期性质对该雷达脉冲序列的PRI进行精确的估计。相对于传统的PRI估计算法,该算法有效地消除了TOA量化误差对PRI估计造成的影响,可以精确地估计出雷达脉冲序列的准确 PRI数值,从而能够更好地满足信号分选算法的处理需求。理论推导及仿真实验均表明了该算法的有效性。  相似文献   
78.
A database of electron temperature (Te) measurements comprising of most of the available satellite measurements in the topside ionosphere is used for studying the solar activity variations of the electron temperature Te at different latitudes, altitudes, local times and seasons. The Te data are grouped into three levels of solar activity (low, medium, high) at four altitude ranges, for day and night, and for equinox and solstices. We find that in general Te changes with solar activity are small and comparable in magnitude with seasonal changes but much smaller than the changes with altitude, latitude, and from day to night. In all cases, except at low altitude during daytime, Te increases with increasing solar activity. But this increase is not linear as assumed in most empirical Te models but requires at least a parabolic approximation. At 550 km during daytime negative as well as positive correlation is found with solar activity. Our global data base allows to quantify the latitude range and seasonal conditions for which these correlations occur. A negative correlation with solar activity is found in the invdip latitude range from 20 to 55 degrees during equinox and from 20 degrees onward during winter. In the low latitude (20 to −20 degrees invdip) F-region there is almost no change with solar activity during solstice and a positive correlation during equinox. A positive correlation is also observed during summer from 30 degrees onward.  相似文献   
79.
The descent of sunspot cycle 23 to an unprecedented minimum of long duration in 2006–2009 led to a prolonged galactic cosmic ray (GCR) recovery to the highest level observed in the instrumental era for a variety of energetic charged particle species on Earth, over a wide range of rigidities. The remarkable GCR increase measured by several ground-based, balloon-borne, and detectors on a satellite is described and discussed. It is accompanied by a decrease in solar wind velocity and interplanetary magnetic field at 1 a.u., reaching the lowest values since measurements of the solar wind began in October 1963; the solar polar field strength (μT) measured at the Wilcox Solar Observatory (WSO) is also significantly reduced compared to prior cycles since the start of the program in 1976, the polar field in the northern hemisphere reversed in June 2012 and again in February 2014, that in the southern hemisphere reversed in July 2013. If updates of WSO data confirm the second reversal in northern solar hemisphere, it would pose a serious challenge to the Dynamo Theory. The long-term change in solar behavior may have begun in 1992, perhaps earlier. The physical underpinnings of these solar changes need to be understood and their effect on GCR modulation processes clarified. The study discusses the recent phenomena in the context of GCR modulation since 1900. These happenings affected our empirical predictions for the key parameters for the next two sunspot cycles (they may be progressively less active than sunspot cycle 24) but it enhanced support for our prediction that solar activity is descending into a Dalton-like grand minimum in the middle of the twentyfirst century, reducing the frequency of the coronal mass ejections; they determine the space weather affecting the quality of life on Earth, radiation dose for hardware and human activities in space as well as the frequency of large Forbush decreases at 1 a.u.  相似文献   
80.
Remote sensing scientists work under assumptions that should not be taken for granted and should, therefore, be challenged. These assumptions include the following:1. Space, especially Low Earth Orbit (LEO), will always be available to governmental and commercial space entities that launch Earth remote sensing missions.2. Space launches are benign with respect to environmental impacts.3. Minimization of Type 1 error, which provides increased confidence in the experimental outcome, is the best way to assess the significance of environmental change.4. Large-area remote sensing investigations, i.e. national, continental, global studies, are best done from space.5. National space missions should trump international, cooperative space missions to ensure national control and distribution of the data products.At best, all of these points are arguable, and in some cases, they're wrong. Development of observational space systems that are compatible with sustainability principles should be a primary concern when Earth remote sensing space systems are envisioned, designed, and launched. The discussion is based on the hypothesis that reducing the environmental impacts of the data acquisition step, which is at the very beginning of the information stream leading to decision and action, will enhance coherence in the information stream and strengthen the capacity of measurement processes to meet their stated functional goal, i.e. sustainable management of Earth resources. We suggest that unconventional points of view should be adopted and when appropriate, remedial measures considered that could help to reduce the environmental footprint of space remote sensing and of Earth observation and monitoring systems in general. This article discusses these five assumptions in the context of sustainable management of Earth's resources. Taking each assumption in turn, we find the following:(1) Space debris may limit access to Low Earth Orbit over the next decades.(2) Relatively speaking, given that they're rare event, space launches may be benign, but study is merited on upper stratospheric and exospheric layers given the chemical activity associated with rocket combustion by-products.(3) Minimization of Type II error should be considered in situations where minimization of Type I error greatly hampers or precludes our ability to correct the environmental condition being studied.(4) In certain situations, airborne collects may be less expensive and more environmentally benign, and comparative studies should be done to determine which path is wisest.(5) International cooperation and data sharing will reduce instrument and launch costs and mission redundancy. Given fiscal concerns of most of the major space agencies – e.g. NASA, ESA, CNES – it seems prudent to combine resources.  相似文献   
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