四维超混沌射频隐身跳频通信设计方法

为提高飞行器通信系统的抗截获性能,提出了一种基于四维超混沌系统的射频隐身跳频通信设计方法。该方法构建了四维超混沌系统,扩展了系统解空间,有效增加了系统复杂度,并通过引入周期性扰动措施,解决了有限精度带来的短周期现象。在四维超混沌系统的基础上,利用超混沌系统生成的双通道超混沌序列,实现了跳频通信系统的频率序列和周期序列联合不确定设计方法。仿真结果表明：四维超混沌系统与传统混沌系统相比,其复杂度最优,在相同有限精度条件下,超混沌系统的周期性明显减弱。另外,基于四维超混沌设计的跳频系统,其截获概率优于常规跳频系统,具有较好的射频隐身性能。     

固体火箭发动机推进剂/衬层界面贮存性能研究进展

针对固体火箭发动机推进剂/衬层界面,从性能失效、组分迁移、表征方法和在线监测四方面综述了界面贮存性能研究进展。首先,从界面脱粘和裂纹扩展两方面讨论界面贮存性能失效,提出有必要探索准确获取界面性能参数的方法和发动机层次的界面裂纹扩展试验方法,以完善发动机界面性能失效分析体系。其次,分析增塑剂和安定剂等不同组分的迁移机理,认为分子动力学模拟能降低组分迁移机理研究的成本。如能进一步与组分迁移抑制的工程经验相结合,建立完整的界面组分迁移模拟和评价体系,对组分迁移机理研究具有重要意义。再次,从宏观、细观和微观多个层次讨论了界面贮存性能的表征问题,提出应构建“宏观-细观-微观”的跨尺度综合表征体系,由浅入深,从不同尺度和不同特性全面表征界面贮存性能。最后,分析了实现界面贮存性能在线监测的主要技术途径,指出集成化、微型化和适应性是界面在线监测需要攻克的关键技术。     

三叉杆式万向联轴器采用调心轴承时的运动分析

分析了三叉杆式万向联轴器采用调心轴承时输出转角和输入转角之间的关系式,并得出这种联轴器为准等角速传动万向联轴器的结论;讨论了轴偏转角大小对输出输入转角差值的影响,分析表明,这种联轴器中转角差值的变化周期是输入轴自转周期的3倍。     

科学评价党史，正确处理历史遗留问题——论邓小平指导党史研究的基本原则

本文系统阐述了邓小平同志指导党史研究、正确处理历史遗留问题的六大原则：“向前看”原则;“宜粗不宜细”原则;“有错必纠”原则;客观性原则;分析个人责任与分析复杂背景相结合的原则;总结成功经验与汲取失败教训相结合的原则。文章深入分析了上述原则的内涵、要求及其意义。     

Massive stars: Setting the stage

The paper gives a summary of the situation mid-1993 of theory and observations regarding massive stars. I describe: stellar mass loss and its implications, pre-main-sequence evolution, the main sequence, problems of atmospheric instability, Luminous Blue Supergiants, Yellow Hypergiants, Wolf-Rayet stars and supernovae.     

Detectors for infrared heterodyne mixing and detection

Conclusion For wavelengths < 50m fast and sensitive detectors are available. For wavelengths > 50m the available detectors are far from ideal. Research and development of far infrared detectors for the mixing purpose are highly recommended.     

A Discrete Method for Parameter Identification in Linear Systems with Transport Lags

Linear dynamical systems with transport lags are characterized by linear differential-difference equations. The task of identifying unknown parameters in such systems from the input-output data is difficult due to mathematical complications associated with differentialdifference equations. This paper presents a method which solves the identification problem. The method is digitally oriented and shows how a continuous-time system can be identified by discrete techniques. The solution is based on Kalman's least square method. The identification procedure essentially involves two steps: 1) discretizing the continuous system via finite difference approximation, and 2) estimating the parameters through the identification of the resulting discrete model. Experimental results have verified the validity of the proposed method.     

Eye light flashes on the Mir space station

The phenomenon of light flashes (LF) in eyes for people in space has been investigated onboard Mir. Data on particles hitting the eye have been collected with the SilEye detectors, and correlated with human observations. It is found that a nucleus in the radiation environment of Mir has roughly a 1% probability to cause an LF, whereas the proton probability is almost three orders of magnitude less. As a function of LET, the LF probability increases above 10 keV/micrometer, reaching about 5% at around 50 keV/micrometer.     

Study of cosmic rays and light flashes on board Space Station MIR: the SilEye experiment.

The SilEye experiment aims to study the cause and processes related to the anomalous Light Flashes (LF) perceived by astronauts in orbit and their relation with Cosmic Rays. These observations will be also useful in the study of the long duration manned space flight environment. Two PC-driven silicon detector telescopes have been built and placed aboard Space Station MIR. SilEye-1 was launched in 1995 and provided particles track and LF information; the data gathered indicate a linear dependence of FLF(Hz) ( 4 2) 10(3) 5.3 1.7 10(4) Fpart(Hz) if South Atlantic Anomaly fluxes are not included. Even though higher statistic is required, this is an indication that heavy ion interactions with the eye are the main LF cause. To improve quality and quantity of measurements, a second apparatus, SilEye-2, was placed on MIR in 1997, and started work from August 1998. This instrument provides energetic information, which allows nuclear identification in selected energy ranges; we present preliminary measurements of the radiation field inside MIR performed with SilEye-2 detector in June 1998.