Solar Gamma-Ray Spectroscopy

Interactions of ions accelerated in solar flares produce gamma-ray lines and continuum and neutrons. These emissions contain a rich set of observables that provides information about both the accelerated ions and the environment where the ions are transported and interact. Ion interactions with the various nuclei present in the ambient medium produce gamma-ray lines at unique energies. How abundance information is extracted from the measurements is discussed and results from analyses of a number of solar flares are presented. The analyses indicate that the composition of the ambient gas where the ions interact (typically at chromospheric densities) is different from that of the photosphere and more like the composition of the corona, exhibiting low-FIP elemental enhancements that may vary from flare to flare. Evidence for increased Ne/O and the photospheric ³He abundance is also discussed.     

The Local Bubble and Interstellar Material Near the Sun

The properties of interstellar matter at the Sun are regulated by our location with respect to a void in the local matter distribution, known as the Local Bubble. The Local Bubble (LB) is bounded by associations of massive stars and fossil supernovae that have disrupted dense interstellar matter (ISM), driving low density intermediate velocity ISM into the void. The Sun appears to be located in one of these flows of low density material. This nearby interstellar matter, dubbed the Local Fluff, has a bulk velocity of ∼19 km s⁻¹ in the local standard of rest. The flow is coming from the direction of the gas and dust ring formed where the Loop I supernova remnant merges into the LB. Optical polarization data suggest that the local interstellar magnetic field lines are draped over the heliosphere. A longstanding discrepancy between the high thermal pressure of plasma filling the LB and low thermal pressures in the embedded Local Fluff cloudlets is partially mitigated when the ram pressure component parallel to the cloudlet flow direction is included.     

基于VXI总线的发动机综合调节器自动测试系统的研制

介绍了某型发动机综合调节器自动测试系统的研制情况,并重点讲述了在系统开发过程中所使用的几项关键技术。     

Stellar flares

Radio and X-ray observations of stellar flares provide the most direct probes of energy relaase particle acceleration, and energy transport on stars other than the Sun. In this review, the observational basis for our understanding of the flare phenomenon on other stars is briefly described and outstanding interpretive and theoretical issues are discussed. I shall confine my attention to objects which are solar-like, to the extent that they possess deep convective envelopes and display activity which is presumed to be magnetic in origin. These include pre-main sequence objects, classical flare stars, and close binaries. Future directions are briefly discussed.     

金属水反应水冲压发动机系统性能估算

使用金属／水反应燃料是推进水下超高速航行器的最佳途径，分析了单次注水和二次注水的铝／水反应燃料水冲压发动机系统，得出了燃料质量配比、燃烧室温度、燃烧室压强、系统有效推力、效率等关键技术性能指标。指出了二次注水系统的优越性并提出了一种二次注水系统的实施方案。分析结论与实际系统性能指标相吻合，证明了分析的正确性，可以为系统研究提供参考。     

基于数据库的CAPP系统研究

简述了航空产品基于数据库的CAPP的必要性,介绍这种CAPP的体系结构、数据流程和特点。论述以产品结构树为核心的用户化工艺文件信息模型、工艺文件的表达、面向产品或BOM的工艺设计方法、CAPP与PDM、MRPII之间的信息集成等关键技术。     

基于CATIA的装配工装数字化设计制造技术

介绍了沈飞公司在工装数字化设计制造领域的主要研究成果——基于CATIA的装配工装设计技术、装配工装数字化安装技术,及其在波音737-X尾段中的应用情况;指出了今后国内飞机装配工装设计及制造技术的发展趋势。     

基于BDS-2/BDS-3联合处理的北斗超快速钟差预报优化策略

针对北斗卫星导航系统(BDS)钟差预报产品无法满足高精度快速服务需求的现状，提出了一种基于BDS-2/BDS-3联合估计的超快速卫星钟差预报优化策略。区别于传统两步法预报模型，利用稀疏建模方法一步求解所有模型项，并通过BDS-2/BDS-3星间相关性实现了模型系数解的增强；为进一步降低模型残差的影响，基于残差序列时空相关性，利用半变异函数重构了模型估计的权阵。为验证提出的钟差预报模型，设计了12套对比方案，实验结果表明：基于稀疏建模的钟差模型参数一步估计可略微提高钟差预报精度；通过引入星间相关性对随机模型进行精化，钟差序列一步建模可分别将BDS-2与BDS-3卫星钟差18h预报精度提升28.6%与27.2%；基于半变异函数建模的模型残差相关性提取，可实现BDS-2与BDS-3预报钟差精度8.0%与11.1%的提升。因此，提出的优化策略对当前北斗超快速卫星钟差预报产品精化具有重要意义。     

基于客户／服务器体系的工程数据库管理系统

提出了一种基于客户／服务器结构的工程数据库管理系统。客户／服务器结构的总体思想是将所有共享数据放在共享的服务器数据库上，所有客户的临时数据放在客户方由客户独占，客户通过局域网（ＬＡＮ）向服务器申请所要的数据，服务器通过ＣｈｅｃｋＩｎ和ＣｈｅｃｋＯｕｔ机制向客户提供数据服务，并确保数据的一致性和完整性。文章讨论了如何在客户和服务器之间合理分配负荷，描述了客户／服务器体系的多级存贮结构和客户与服务器之间的数据通信．重点探讨了客户／服务器结构下的缓冲管理问题。系统的开发环境是ＳｕｎＯＳ，ＴＣＰ／ＩＰ协议，系统用Ｃ语言开发。