液体火箭发动机试验数据曲线绘制软件设计

利用Active X技术并结合Excel功能,开发出液体火箭发动机地面试验数据曲线绘制软件,重点介绍绘制软件程序的组成和功能,给出了关键部分的程序框图。软件可供试验数据分析时参考。     

空间材料科学实验中的X光三维成像仿真

用于空间材料科学研究的X射线观察设备已列入空间站材料科学实验规划,仿真实现X光三维成像的流程可为X射线观察设备的研制提供设计依据.仿真流程主要包括三个步骤：使用锥束X光照射被扫描对象并旋转对象,获取多角度下的投影影像;根据投影影像和几何信息重建扫描对象,获取对象空间点数据;将扫描对象三维显示出来.使用线衰减系数不同且相互重叠的多个椭球组成的三维Shepp-Logan模型对算法进行了仿真测试,仿真结果能很好地将模型重建并显示出来.     

MiniGUI在VxWorks中的应用及编程方法研究

VxWorks是风河公司设计开发的一种实时嵌入式操作系统,具有高可靠性和实时性。通常VxWorks不包含图形用户界面,这导致系统不易操作,为了实现图形用户界面,本文将MiniGUI应用在VxWorks中。首先本文对WindML、MiniGUI进行了介绍并对编程方法进行了研究和改进,然后实现了一个较复杂的图形用户界面。这种方法使系统易于操作,为VxWorks系统的应用带来了便利,而且不影响VxWorks系统的实时性能。另外对编程方法的改进可以提高图形用户界面的开发效率,便于代码的维护和二次开发。     

飞机技术出版物在飞机海外复装中的应用

以西锐SR2X飞机海外标准复装为例,初步探索了飞机技术出版物在通用飞机复装中的使用,明确了通用飞机复装的技术依据和作业流程,为未来通用飞机制造商或代理商复装飞机提供了工程经验。     

利用VB设计动态模拟MCS51中断系统的仿真平台

用VB编程软件设计——仿真单片机8051中断系统的响应过程，采用动态教学方法，实验演示和动手相结合，使教学变得活灵活现，栩栩如生。     

JPL Innovation Foundry

Space science missions are increasingly challenged today: in ambition, by increasingly sophisticated hypotheses tested; in development, by the increasing complexity of advanced technologies; in budgeting, by the decline of flagship-class mission opportunities; in management, by expectations for breakthrough science despite a risk-averse programmatic climate; and in planning, by increasing competition for scarce resources. How are the space-science missions of tomorrow being formulated? The paper describes the JPL Innovation Foundry, created in 2011, to respond to this evolving context. The Foundry integrates methods, tools, and experts that span the mission concept lifecycle. Grounded in JPL's heritage of missions, flight instruments, mission proposals, and concept innovation, the Foundry seeks to provide continuity of support and cost-effective, on-call access to the right domain experts at the right time, as science definition teams and Principal Investigators mature mission ideas from “cocktail napkin” to PDR. The Foundry blends JPL capabilities in proposal development and concurrent engineering, including Team X, with new approaches for open-ended concept exploration in earlier, cost-constrained phases, and with ongoing research and technology projects. It applies complexity and cost models, project-formulation lessons learned, and strategy analyses appropriate to each level of concept maturity. The Foundry is organizationally integrated with JPL formulation program offices; staffed by JPL's line organizations for engineering, science, and costing; and overseen by senior Laboratory leaders to assure experienced coordination and review. Incubation of each concept is tailored depending on its maturity and proposal history, and its highest-leverage modeling and analysis needs.     

基于话音／数据综合通信网络的空中交通管制中心之间的广域联接

话音／数据综合通信网络是民航中南地区传输雷达信号、话音移交信号、 Ａ Ｆ Ｔ Ｎ 信号、 Ｖ Ｈ Ｆ 信号等的广域网络。网络采用了目前先进的交换机、民航卫星网络、邮电 Ｄ Ｄ Ｎ 网络，把位于中南六省区的话音和数据信号进行集成传输，适应了空管业务的快速增长，提高了信号传输的可靠性，减少信号的延迟，节省了运行成本。     

LiXAlF6:xCe3+(X=Ca,Sr,Ba)的发光研究

光激励发光材料一直是人们竞争研究的对象。为在较短的时间内在发光中心存储更多的电子，要寻找一种荧光材料作为光激励发光材料的增感材料，使光激励发光材料敏化，从而提高光激励发光强度，这是提高激发光源利用率的最佳途径。通过对用紫外光源作激发源的光激励发光材料发光机理的研究，确定在紫外波段靠近短波方向的光可能使这种光激励发光材料敏化。Ce^3＋在氟化物体系中的发射通常位于紫外波段，对Ce^3＋掺杂浓度为x的LiXAlF6：xCe^3＋（X=Ca，Sr，Ba，x=0．002～0．012mol）一系列荧光材料作了研究，研究其发光是否在紫外波段，哪种基质更适合需要。采用高温固相法制备，研究该3种化合物的发射光谱及发射光谱随Ce^3＋掺杂浓度的变化。结果找到了最有可能作为用紫外光源作激发源的光激励发光材料的最佳Ce^3＋掺杂浓度的基质LiBaAlF6：xCe^3＋（x=0．010mol）。     

不完备轨道信息下的LEO轨道面内机动检测方法

针对某些因轨道信息不完整而无法直接外推的LEO轨道飞行器的机动检测问题,提出了一种基于轨道摄动影响的面内机动检测方法。该方法将半长轴和偏心率作为检测量,通过分析大气阻力摄动和J 2 项摄动对 LEO 飞行器轨道的影响,从而确定目标飞行器的轨道参数允许边界值,再通过和实际轨道参数进行比较来判定被检测数据点参数是否超出正常范围。最后,采用这种方法对X\|37B飞行器轨道数据进行了仿真验证,共检测出10个机动点,结果表明该方法可以较为准确地利用有限轨道信息检测目标的轨道机动情况。     

Hard X-ray observations of Cygnus X-1 with the MISO telescope

The black hole candidate Cygnus X-1 was observed in the hard X ray - soft γ ray energy range by the MISO telescope on two different occasions: in September 1979 and May 1980. We have measured two hard X-ray states of the source: in 1979 the observed spectrum confirms the superlow state measured in the same period by the HEAO-3 satellite, while in 1980 the MISO X-ray data are consistent with the so called low state of Cygnus X-1. In both occasions, no γ -ray excess has been observed above 200 KeV.