某型号姿控动力系统气体减压阀性能测试系统设计

围绕某型号姿控动力系统减压阀性能测试需求,提出一种基于PC104总线测试架构的设计方案。详细阐述了减压阀性能测试原理、硬件设计方案和软件开发思路,着重介绍了软件开发需求、总体架构、用户程序开发思路和软件设计关键技术等。实际应用表明,该系统操作简单、携带方便,测试精度优于0.2%,控制定时精度优于1 ms,满足减压阀性能测试要求。     

激波管中测量JP-10点火延时的吸附问题研究

在JP-10点火延时的激波管实验中,JP-10在激波管壁的吸附导致气相浓度的不确定是测量结果分散的主要原因之一.利用精确测定的吸附曲线确定了实验时JP-10真实的气相浓度,解决了高碳数碳氢燃料点火延时激波管实验时管壁吸附影响燃料气相浓度确定的困难.实验显示JP-10的吸附符合Langmuir吸附等温关系.     

ATC3000航空地图制作软件及其关键技术分析

针对ATC3000空管自动化系统的运行要求以及飞行管制区现场实际工作的需要,介绍了ATC3000航空地图制作软件的关键技术。文中分析了该软件的结构以及在Windows系统中使用Delphi开发的具体实现技术。     

Anomalous Cosmic Rays and Solar Modulation

We review aspects of anomalous cosmic rays (ACRs) that bear on the solar modulation of energetic particles in the heliosphere. We show that the latitudinal and radial gradients of these particles exhibit a 22-year periodicity in concert with the reversal of the Sun's magnetic field. The power-law index of the low energy portion of the energy spectrum of ACRs at the shock in 1996 appears to be -1.3, suggesting that the strength of the solar wind termination shock at the helioequatorial plane is relatively weak, with s 2.8. The rigidity dependence of the perpendicular interplanetary mean free path in the outer heliosphere for particles with rigidities between 0.2 and 0.7 GV varies approximately as R2, where R is particle rigidity. There is evidence that ACR oxygen is primarily multiply charged above 20 MeV/nuc and primarily singly-charged below 16 MeV/nuc. The location of the termination shock was at 65 AU in 1987 and 85 AU in 1994.     

The Geology of Mercury: The View Prior to the MESSENGER Mission

Mariner 10 and Earth-based observations have revealed Mercury, the innermost of the terrestrial planetary bodies, to be an exciting laboratory for the study of Solar System geological processes. Mercury is characterized by a lunar-like surface, a global magnetic field, and an interior dominated by an iron core having a radius at least three-quarters of the radius of the planet. The 45% of the surface imaged by Mariner 10 reveals some distinctive differences from the Moon, however, with major contractional fault scarps and huge expanses of moderate-albedo Cayley-like smooth plains of uncertain origin. Our current image coverage of Mercury is comparable to that of telescopic photographs of the Earth’s Moon prior to the launch of Sputnik in 1957. We have no photographic images of one-half of the surface, the resolution of the images we do have is generally poor (∼1 km), and as with many lunar telescopic photographs, much of the available surface of Mercury is distorted by foreshortening due to viewing geometry, or poorly suited for geological analysis and impact-crater counting for age determinations because of high-Sun illumination conditions. Currently available topographic information is also very limited. Nonetheless, Mercury is a geological laboratory that represents (1) a planet where the presence of a huge iron core may be due to impact stripping of the crust and upper mantle, or alternatively, where formation of a huge core may have resulted in a residual mantle and crust of potentially unusual composition and structure; (2) a planet with an internal chemical and mechanical structure that provides new insights into planetary thermal history and the relative roles of conduction and convection in planetary heat loss; (3) a one-tectonic-plate planet where constraints on major interior processes can be deduced from the geology of the global tectonic system; (4) a planet where volcanic resurfacing may not have played a significant role in planetary history and internally generated volcanic resurfacing may have ceased at ∼3.8 Ga; (5) a planet where impact craters can be used to disentangle the fundamental roles of gravity and mean impactor velocity in determining impact crater morphology and morphometry; (6) an environment where global impact crater counts can test fundamental concepts of the distribution of impactor populations in space and time; (7) an extreme environment in which highly radar-reflective polar deposits, much more extensive than those on the Moon, can be better understood; (8) an extreme environment in which the basic processes of space weathering can be further deduced; and (9) a potential end-member in terrestrial planetary body geological evolution in which the relationships of internal and surface evolution can be clearly assessed from both a tectonic and volcanic point of view. In the half-century since the launch of Sputnik, more than 30 spacecraft have been sent to the Moon, yet only now is a second spacecraft en route to Mercury. The MESSENGER mission will address key questions about the geologic evolution of Mercury; the depth and breadth of the MESSENGER data will permit the confident reconstruction of the geological history and thermal evolution of Mercury using new imaging, topography, chemistry, mineralogy, gravity, magnetic, and environmental data.     

不同中间层合金对IC10合金的连接

采用B或Zr作为降熔元素分别配制不同中间层合金,并对IC10合金进行连接.分析不同状态下焊缝组织.结果表明,含B中间层合金连接IC10时,保温时间较长可以达到等温凝固,而含Zr中间层合金在本试验条件下表现为钎焊过程.     

16Co14Ni10Cr2Mo钢力学性能与应力腐蚀行为

研究了１６Ｃｏ１４Ｎｉ１０Ｃｒ２Ｍｏ钢不同温度回火５ｈ强度、冲击韧性、断裂韧性和应力腐蚀性能（在３．５％ＮａＣｌ水溶液中）。在５１０℃回火可以获得较高的强度，最高的断裂韧性及抗应力腐蚀性能，此时Ｋ＿（ＩＳＣＣ）可达，Ｋ＿（ＩＣ）为，屈服强度为１５８０ＭＰａ。应力腐蚀性能（ＳＣＣ）的改善主要与在较高温度回火，使Ｍｏ＿２Ｃ共格造成的应力下降，位错亚结构的恢复及碳化物的粗化，并导致氢的偏聚下降有关。     

含C,Cr,Mo的Fe—10Ni—14Co钢的微观组织

用TEM对两种含碳量的高钴镍钢的微观组织进行了研究。结果表明,各状态试样组织中孪晶的出现,淬火温度、冷却速度的影响是次要的,与合金中的合金元素镍、铬、铜有更密切的关系。淬火+510℃回火5小时组织中除在淬火过程中形成的薄膜状残余奥氏体外,还存在穿板条及沿板条的呈片状或颗粒状的逆转变奥氏体,组织中的合金碳化物鉴定为Mo_2C。     

基于备件保障概率的备件库存限额确定方法

鉴于目前装备研制早期信息较少,备件需求确定方法与战备完好性指标相脱节,备件需求的不确定性较大,通过建立装备完好率、可用度、平均故障停机时间与备件保障概率之间的关系,确定满足完好率的区间要求的装备系统备件保障概率。运用Delphi法对装备分系统和LRU的备件保障概率进行分配,进而确定相应的备件库存限额标准。最后,结合实例验证了分析方法的可行性与合理性。     

多线程异地备份发动机数据软件设计与应用

通过开发发动机信息管理系统后台数据的异地备份软件,介绍了以Delphi 10 Seattle为开发工具,应用Indy组件,多线程方式实现客户端向服务器端发送备份指令,完成数据的备份、加密压缩以及向异地客户端推送数据,以客户端完成压缩数据的接收结束异地传输,同时服务器端实时向不同客户端发送执行过程信息.因发动机数据量较大,备份和传输时间较长,在异地客户端采用同步进度条显示.软件设计采用TCP可靠传输,提高数据传输的安全性.