Concept of wireless sensor network for future in-situ exploration of lunar ice using wireless impedance sensor

It is known that a wireless sensor network uses some sort of sensors to detect a physical quantity of interest, in general. The wireless sensor network is a potential tool for exploring the difficult-to-access area on the earth and the concept may be extended to space applications in future. Recently, lunar water has been detected by a few lunar missions using remote sensing techniques. The lunar water is expected to be in the form of ice at very low temperatures of permanently dark regions on the moon. To support the remote observations and also to find out potential ice bearing sites on the moon, in-situ measurement of the lunar ice is essential. However, a rover may not be able to reach the permanently shadowed regions due to terrain irregularity. One possibility to access such areas is to use a wireless sensor network on the lunar surface.     

缝式处理机匣轴向位置对压气机特性影响的机理

对轴向倾斜缝处理机匣轴向位置的改变如何影响轴流压气机性能进行了研究.试验与数值结果均表明三个轴向位置的处理机匣均扩宽压气机的稳定工作范围,轴向位置不变时扩稳效果最好,轴向位置后移时效果最差.同时轴向位置前移或后移使压气机等熵效率损害程度降低.通过详细地分析压气机内部流场表明:处理机匣轴向位置后移使叶顶机匣约1/3的轴向...     

霍尔推力器等离子体磁鞘特性

为进一步研究霍尔推力器壁面二次电子发射对发动机性能的影响,建立流体模型数值模拟了霍尔推力器磁化二次电子等离子体的鞘层特性,采用Sagdeev势的方法得到了鞘层的玻姆判据,以这个判据为鞘层边界条件数值讨论了磁场、二次电子发射以及不同等离子体对推力器等离子体鞘层结构的影响。结果表明,磁场和二次电子发射系数的增加都将使鞘层中粒子密度增加,鞘层电势升高,鞘层厚度减小;对于氩和氙二种等离子体,氙等离子体产生的鞘层势垒高,粒子密度大,鞘层厚度增加。这些结果直接影响推力器的电子传导机制及性能。     

基于制导信息的一维波束可控随机脉位脉冲多普勒引信技术研究

针对空空导弹引信的任务特点,综合采用了基于制导信息的起爆控制算法技术、自适应调整天线波束倾角技术、基于频域信号处理的数字信号处理技术设计了总体技术方案.仿真分析和试验表明,系统实现了对作战飞机、导弹等不同类型目标的智能探测,提高了对目标的探测灵敏度和抗干扰能力.     

基于FSK的测斜系统电路设计

本文重点阐述了测斜系统井下仪器数据采集单元和数据发送单元电路的设计及井上仪器解调电路的设计，给出了具体的电路设计结果及元器件参数。     

用于压力传感器校准的高低温试验箱设计

基于压力传感器在高低温环境下的校准需求,设计了一种专用高低温试验箱。其控制温度范围可达到-120℃[KG-*4]~[KG-*7]500℃。提出了高低温试验箱的总体方案,介绍了宽温区温度的实现方法以及高温和低温系统不兼容的解决方法和控制流程。试验验证结果显示,高低温试验箱达到了实现宽温区温度的目的,满足设计指标要求。     

A Fast Global Node Selection Algorithm for Bearings-only Target Localization

In the target tracking, the nodes aggregate their observations of the directions of arrival of the target. The network then uses an extended Kalman filter （EKF） to combine the measurements from multiple snapshots to track the target. In order to rapidly select the best subset of nodes to localize the target with the minimum mean square position error and low power consumption, this paper proposes a simple algorithm, which uses the location information of the target and the network. The lower botmd of localization error is utilized according to the distances between the target and the selected active nodes. Furthermore, the direction likelihoods of the active nodes is predicted by way of the node/target bearing distributing relationships.     

基于Visual Basic6.0的功率传感器自动校准系统

从硬件组成和软件设计两方面介绍了功率传感器自动校准系统.着重介绍了该系统的软件设计思路,并就其特点进行说明.该自动校准系统在Visual Basic 6.0环境下完成编程,完整地实现了登录、设备信患登记、测试、报告文件输出及查询功能,使用简便、性能可靠且人机交互良好.     

MEMS惯性器件及系统发展研究综述

将MEMS惯性系统分为ISA、IMU和INS三级,分别介绍了国内外的研究概况,并对MEMS INS的发展趋势进行了讨论,供广大惯性导航研究人员参考。     

Gravitational wave detection on the Moon and the moons of Mars

The Moon and the moons of Mars should be extremely quiet seismically and could therefore become sensitive gravitational wave detectors, if instrumented properly. Highly sensitive displacement sensors could be deployed on these planetary bodies to monitor the motion induced by gravitational waves. A superconducting displacement sensor with a 10-kg test mass cooled to 2 K will have an intrinsic instrument noise of 10⁻¹⁶ m Hz^−1/2. These sensors could be tuned to the lowest two quadrupole modes of the body or operated as a wideband detector below its fundamental mode. An interesting frequency range is 0.1–1 Hz, which will be missed by both the ground detectors on the Earth and LISA and would be the best window for searching for stochastic background gravitational waves. Phobos and Deimos have their lowest quadrupole modes at 0.2–0.3 Hz and could offer a sensitivity h_min ? 10⁻²² Hz^−1/2 within their resonance peaks, which is within two orders of magnitude from the goal of the Big Bang Observer (BBO). The lunar and Martian moon detectors would detect many interesting foreground sources in a new frequency window and could serve as a valuable precursor for BBO.