化学-电喷双模推进系统的研究现状及展望

传统的化学推进和电推进拥有不同的特点及适用范围。化学推进可以产生毫牛级至牛级推力，相比于电推进，推力大，推力范围宽；电推进比冲高达上千秒，最小可以产生微牛级推力。但两种模式单独执行任务有一定的局限性，难以完成较为复杂的航天任务。化学推进与电推进相结合的双模推进系统，同时拥有高比冲和较宽的推力范围，为航天器提供了更高的任务灵活性，其中单组元液体火箭发动机 离子液体电喷推力器双模推进系统近年来受到广泛关注。简述了单组元 电喷双模推进系统的工作原理和特点，重点总结了国内外关于双模推进的研究现状，并对目前面临的问题与挑战进行分析。     

IC制造中平坦化技术的性能与分析

表面平整化技术是半导体工业的关键技术,在一定程度上制约着半导体芯片集成技术的发展,针对多层立体布线的IC全局平坦化技术,介绍了代表当今平整化技术及其未来的发展方向,其中一些技术会取代传统的CMP技术而成为IC产业的主导技术之一;叙述了超大规模集成电路(ULSI)的发展对全局平整化的具体要求;对传统的CMP技术的特点进行了分析;并论述了当今主流的IC平整化技术的原理、性能以及未来的发展方向。     

自由飞试验模型惯性矩的测定

作者根据多年来自由飞试验的实践,叙述了自由飞模型惯性矩的调试、计算、误差分析与处理的经验与方法。     

质量矩导弹的神经网络及自适应非线性控制

本文对质量矩控制导弹的动力学方程简化和控制系统的设计进行了研究。详细阐述了所提出的控制方法，介绍了径向基单隐层神经网络进行误差补偿的算法原理，用Lyapunov理论证明了所采用方法的稳定性。在给出了质量矩导弹的六自由度动力学方程和简化后的方程后，用所提出的方法设计控制系统。通过仿真分析，得出了本文所提出的方法具有较好的误差补偿能力的结论。     

A Novel Onboard-gateway-based Mechanism to Improve TCP Performance in Aeronautical Satellite Networks

The IP-based networks on aircraft serve to support Internet services via satellites. However, in aeronautical satellite hybrid net- works,the TCP protocol performance often deteriorates due to improper decreases and slow recovery of the congestion window. This paper proposes a window size determination and notification mechanism, onboard-gateway-based mechanism (OGBM), which is based on the onboard gateway in the networks on aircraft. A cross-layer approach is adopted by the onboard gateway to obtain the satellite link bandwidth information. And then, by the gateway, through changing the receiver’s advertised window field in ACK packets, TCP sources are notified of the window size of each TCP source calculated on the ground of bandwidth delay product and flow numbers. The mechanism is able to avoid improper changes of TCP window and serve multiple users. Simulation results show that the mechanism with the fairness index close to 1 improves TCP performance in aeronautical satellite networks.     

Galactic Wind: Mass Fractionation and Cosmic Ray Acceleration

The dynamical and chemical effects of the Galactic Wind are discussed. This wind is primarily driven by the pressure gradient of the Cosmic Rays. Assuming the latter to be accelerated in the Supernova Remnants of the disk which at the same time produce the Hot Interstellar Medium, it is argued that the gas removed by the wind is enriched in the nucleosynthesis products of Supernova explosions. Therefore the moderate mass loss through this wind should still be able to remove a substantial amount of metals, opening the way for stars to produce more metals than observed in the disk, by e.g. assuming a Salpeter-type stellar initial mass function beyond a few Solar masses. The wind also allows a global, physically appealing interpretation of Cosmic Ray propagation and escape from the Galaxy. In addition the spiral structure of the disk induces periodic pressure waves in the expanding wind that become a sawtooth shock wave train at large distances which can re-accelerate “knee” particles coming from the disk sources. This new Galactic Cosmic Ray component can reach energies of a few×10¹⁸ eV and may contribute to the juncture between the particles of Galactic and extragalactic origin in the observed overall Cosmic Ray spectrum.     

Progress in space weather predictions and applications

The methods of today’s predictions of space weather and effects are so much more advanced and yesterday’s statistical methods are now replaced by integrated knowledge-based neuro-computing models and MHD methods. Within the ESA Space Weather Programme Study a real-time forecast service has been developed for space weather and effects. This prototype is now being implemented for specific users. Today’s applications are not only so many more but also so much more advanced and user-oriented. A scientist needs real-time predictions of a global index as input for an MHD model calculating the radiation dose for EVAs. A power company system operator needs a prediction of the local value of a geomagnetically induced current. A science tourist needs to know whether or not aurora will occur. Soon we might even be able to predict the tropospheric climate changes and weather caused by the space weather.     

航电系统SCI环型互连的计算机仿真建模

研究可扩展一致性接口 SCI环型互连的计算机仿真问题。作为未来一代航电系统的首选技术 ,SCI互连系统性能的优劣直接影响到飞行器的质量 ,对其性能的评价因此显得尤为重要。文中按照计算机仿真建模的一般方法 ,从 SCI协议的基本原理出发 ,建立了接口和节点模型 ,解决了并发数据交互的仿真时序问题 ,给出了 SCI环型互连的系统仿真模型 ,并通过例子对仿真模型的有效性进行了验证     

一种具有较强泛化能力的神经网络模型研究与应用

分析了影响神经网络模型泛化能力的因素。以电解铝过程中氧化铝浓度的神经网络软测量为例 ,提出了利用先验知识确定网络结构 ,采用特定实验保证样本数量和质量 ,离线训练加在线学习修正模型等措施 ,改善神经网络模型的泛化能力。现场应用表明这些措施是有效的。这样建立的神经网络模型准确 ,泛化能力强 ,为实现过程的先进控制提供了可靠保障     

数据库开放对象的一般结构和操作

为了更精确地模拟客观世界，减少软件生成的复杂性，本文提出开放对象的数据模型，使其自身具有自组织、自我进化的能力，实质是面向对象＋人工智能＋数据库的一个模型。本文讨论了它的一般结构，开放对象的集合在子开放对象关系下构成有向图，并在对其加以适当限制做成偏序格的基础上，定义了一组开放对象的基本操作。