突片形状对气膜冷却效率的影响

气膜冷却广泛应用于航空发动机热端部件的热防护,为了提高气膜冷却效果,设计了3种突片型式,采用实验的方法对其冷却效果进行了对比研究,结果表明：突片的存在强化了气膜冷却效率,使得气膜冷却效率远高于无突片的气膜冷却效率。吹风比对不同突片作用有所不同,存在一最佳吹风比,但该值随着突片的型式变化。突片的堵塞比对气膜冷却效率有很大的影响,3种突片作用下的气膜冷却效率均随堵塞比的增加而增大。梯形突片的冷却效率明显优于三角形突片和椭圆突片。但突片亦增大了气膜孔的流动阻力,降低了流量系数。     

用CT值推导人体组织属性参数的方法及改进

蒙特卡罗方法是计算精度最高的人体组织剂量计算方法。常见的蒙特卡罗模拟程序,如M CNP,EG S4等都自带了各种介质的截面数据,而剂量计算的一个重要步骤就是得到人体组织的属性参数——质量密度和化学组成。本文主要介绍了两种根据医学影像CT值推导人体组织属性参数的方法——区间法和两分法,并经过分析比较认为两分法比区间法具有更高的精确度和可行性。同时,针对两分法存在的不足和缺陷,本文将CT值全范围划分为七段,根据两分法的假设条件假设每一段均由两种不同的人体组织混合而成。在每一段CT值范围内,人体组织的质量密度和化学组成通过对两种假定物质参数的拟合得到。结果说明该方法所得到的人体组织属性参数完全可以满足蒙特卡罗人体组织剂量计算的要求。     

关于农村老年人经济保障问题的思考

老人缺乏经济保障是造成农村养老纠纷事件多发的根本原因，作者在分析农村老人缺乏经济保障原因的基础上，对解决农村老人经济保障问题的途径进行了探讨。     

Influences of mass flow rate on heat and mass transfer performances of water sublimator combined with fluid loop

For spacecraft working in vacuum environment, sublimator is an effective heat rejection approach to reject system's peak heat load, and supplement spacecraft radiation heat rejection. For a spacecraft active fluid loop thermal control system combined with sublimator, waste heat generated from multi-point distributed heat sources could be collected by the fluid loop efficiently. However, the heat and mass transfer performances of the sublimator combined with fluid loop have not been adequately studied in previous research, especially for the influences of the heat load. Since work fluid mass flow rate is the main factor affecting heat load of the fluid loop, this context experimentally studied influences of the fluid loop mass flow rate on sublimator start-up transient characteristics, including heat transfer performances, response time, and work stability. Results indicated that the fluid loop mass flow rate affected the sublimator heat and mass transfer performances obviously, but the heat rejection ability is not always increase with the increasing of the fluid loop mass flow rate. In addition, we obtained the condition to judge whether there is a positive correlation between heat rejection ability and fluid loop mass flow rate.     

基于USB的数据存储设备开发方案

介绍一个基于USB的数据存储设备开发方案,系统采用PH ILIPS公司的ISP1160芯片来实现USB主机控制器。首先介绍USB的特点,然后详细讨论方案各功能模块的实现方法,最后说明方案应用和系统性能指标。     

卫星数据搜集系统(DCS)的技术现状与改进概念探索

对当前国际上流行的 DCS系统进行简介及评述 ,指出各自的优缺点 ,并提出多普勒频率补偿、自主计算开机时间和捷径点发报两种构想进行革新     

面向无人机的单芯片惯性测量组合

针对无人机对惯性测量组合的小尺寸、轻重量的需求,设计实现了芯体为1cm3的微小型单芯片的硅微惯性测量组合。论文提出了一种基于体硅深刻蚀—玻璃键合工艺的单芯片惯性测量组合结构,该结构集成了六个异构的单轴惯性器件,可实现运动载体的六自由度运动信息测量。单芯片惯性测量组合中的陀螺器件两个模态的的振动频率实现了较好的匹配,加速度计器件分辨率达到了0.93mg。测试结果表明该单芯片惯性测量组合有望实现高精度的惯性量测量,在无人机上有很好的应用前景。     

捷联惯性测量组合标定方案

本文介绍了惯性组合标定“6位置12点采样”的编排方案,可补偿测试设备调平、对北误差的影响,测试过程简单合理。此外介绍了对组合性能有特殊意义的ωｅ、ｇ自检及迭代求解方法,并以此作为求算标准偏差的依据。     

Statistical analysis of geomagnetic field variations during solar eclipses

We investigate the geomagnetic field variations recorded by INTERMAGNET geomagnetic observatories, which are observed while the Moon’s umbra or penumbra passed over them during a solar eclipse event. Though it is generally considered that the geomagnetic field can be modulated during solar eclipses, the effect of the solar eclipse on the observed geomagnetic field has proved subtle to be detected. Instead of exploring the geomagnetic field as a case study, we analyze 207 geomagnetic manifestations acquired by 100 geomagnetic observatories during 39 solar eclipses occurring from 1991 to 2016. As a result of examining a pattern of the geomagnetic field variation on average, we confirm that the effect can be seen over an interval of 180?min centered at the time of maximum eclipse on a site of a geomagnetic observatory. That is, demonstrate an increase in the Y component of the geomagnetic field and decreases in the X component and the total strength of the geomagnetic field. We also find that the effect can be overwhelmed, depending more sensitively on the level of daily geomagnetic events than on the level of solar activity and/or the phase of solar cycle. We have demonstrated it by dividing the whole data set into subsets based on parameters of the geomagnetic field, solar activity, and solar eclipses. It is suggested, therefore, that an evidence of the solar eclipse effect can be revealed even at the solar maximum, as long as the day of the solar eclipse is magnetically quiet.