Pro/E二次开发技术在导弹设计中的应用

为了提高导弹快速设计的效率以及降低设计人员的工作量,以VC++6.0为开发环境,充分利用Pro/E基于骨架模型的参数化建模、变量化和单一数据库等技术,研究基于Pro/TOOLKIT异步模式的Pro/E二次开发技术,实现了应用软件与Pro/E之间的数据通信以及数据共享,从而保证了飞行器的外形及其相关参数能够快速、自动地更新,进而驱动各个学科自动分析.最后通过工程实例,验证了该方法的有效性和系统的可行性,结果表明此方法是可行的.     

嫦娥工程技术发展路线

月球是距离地球最近的天体,以其独特的空间位置、广阔的科学探索前景,成为人类地外天体探测和资源利用的首选目标和持续选择。简要总结世界各主要航天大国的探月发展历程和后续计划,详细介绍了我国探月工程(嫦娥工程)"绕""落""回"三步走的发展思路和技术路线,分析了后续的发展方向,提出了2030年前月球机器人科研站任务设想。     

Parameterized Regional Ionospheric Model and a comparison of its results with experimental data and IRI representations

We describe a Parameterized Regional Ionospheric Model (PARIM) to calculate the spatial and temporal variations of the ionospheric electron density/plasma frequency over the Brazilian sector. The ionospheric plasma frequency values as calculated from an enhanced Sheffield University Plasmasphere–Ionosphere Model (SUPIM) were used to construct the model. PARIM is a time-independent 3D regional model (altitude, longitude/local time, latitude) used to reproduce SUPIM plasma frequencies for geomagnetic quiet condition, for any day of the year and for low to moderately high solar activity. The procedure to obtain the modeled representation uses finite Fourier series so that all plasma frequency dependencies can be represented by Fourier coefficients. PARIM presents very good results, except for the F region peak height (hmF2) near the geomagnetic equator during times of occurrence of the F₃ layer. The plasma frequency calculated by IRI from E region to bottomside of the F region present latitudinal discontinuities during morning and evening times for both solar minimum and solar maximum conditions. Both the results of PARIM and the IRI for the E region peak density show excellent agreement with the observational values obtained during the conjugate point equatorial experiment (COPEX) campaign. The IRI representations significantly underestimate the foF2 and hmF2 compared to the observational results over the COPEX sites, mainly during the evening–nighttime period.     

23Co14Ni12Cr3Mo超高强度钢DCB试样在3.5%NaCl溶液中的应力腐蚀开裂行为

23Co14Ni12Cr3Mo超高强度钢具有优异的强韧性配合,逐步取代现役的超高强度钢,被广泛地应用于起落架等航空关键承力构件中。研究了23Co14Ni12Cr3Mo超高强度钢的应力腐蚀开裂(SCC)行为,对该材料的安全可靠应用具有重要的意义。采用双悬臂(DCB)试样研究了23Co14Ni12Cr3Mo超高强度钢在3.5%NaCl溶液中的SCC分叉行为,为该材料在航空航天领域安全可靠地使用提供了理论数据。采用扫描电子显微镜(SEM)对试验开裂后的断口形貌进行了表征,采用X射线电子衍射技术(XRD)结合能谱(EDS)技术对腐蚀产物进行分析。结果表明应力腐蚀裂纹扩展分叉,断口形貌在裂纹扩展前期、中期和后期分别为穿晶(TG)形貌、穿晶伴随沿晶(IG)形貌并含有二次微裂纹以及沿晶脆性断裂。该超高强度钢腐蚀产物主要包括Fe、Cr、Co的氧化物,结合Co、Cr、Ni、Mo在应力腐蚀过程中的变化,讨论了裂纹扩展分叉机理。     

热开关热管在月面探测光学设备中的应用

在月面-180~+90℃的极端高低温环境下,月面探测光学设备的月昼远距离散热和月夜保温矛盾异常突出。针对设备热耗的传输、排散,以及月夜生存时的热能存留问题,利用热管工质的汽、液、固相变特性,提出一种无源热开关热管作为设备和散热面间长距离传热手段,即依据设备温度指标选择具有合适凝固点和传热能力的工质,当月昼工作期间通过热管内工质两相传热实现热量的高效收集和传输,到月夜期间冻结热管内全部工质,完全切断热管与散热面间的两相传热,维持设备温度。地面试验和在轨飞行数据表明,热开关热管凝固点附近热导比达30以上。热管工作时,7℃时传热能力大于15W,传热温差小于4℃,且能够适应着陆器±15°的倾斜,确保了嫦娥三号着陆器月基光学望远镜在轨的高性能工作。     

空间核电源系统整流装置设计

为满足我国未来深空探测、星表基地等空间任务电源系统的需求,针对空间核电源系统,为解决高压高频输入导致高谐波输出的问题,本文提出了利用12脉波整流器来实现交直流变换.在本文的拓扑结构中,重点研究三相三绕组隔离型变压器、三抽头平衡电抗器及LLC谐振变换器的参数设计.通过三相三绕组隔离型变压器产生30°相位差的两组电压,进而...     

Comparison Structure Forms Between Isogrid and Orthogrid of C/ E CompositeTrellis Wound Structure Based on Calculation of Load Carrying

This paper calculated load carrying of isogrid and orthogrid of carbon epoxy composite trellis wound
structure (C/ E CTWS) using non linear finite element method. Based on the analysis, test cases were designed and
tests of axial compression were carried. Analysis result and test result fit well. In order to be used in the project, this
kind of structure cut out repairing was calculated. The method presented in this paper has been proved and can be used
to solve complicated engineering problems. According to calculations and experimental results combined with applica
tion, a principle of choosing wound structure is obtained and principle could be applied to engineering.
     

卫星导航有源接收天线噪声温度测量

卫星导航有源接收天线的噪声温度是导航接收系统的关键技术指标之一。针对卫星导航有源天线总体噪声温度无法测量的问题，研制了两台口面型噪声源，口面噪声源主要由辐射体、辐射体物理温度控制和温度测量仪等组成。两个口面噪声源在L和S波段分别提供高低温标准噪声温度，采用Y系数测量方法测量有源接收天线的总体天线噪声温度。测量了某卫星导航有源天线的总噪声温度，在(1.19～1.29) GHz的频率范围内，中心频率1.24 GHz上噪声温度测量结果为206 K，但是在1.266 GHz频率点上噪声温度测量大于4 000 K，说明天线与滤波器之间、滤波器与放大器之间存在设计问题或其它问题，体现出测量有源天线噪声温度的必要性。