重复使用航天器发展趋势及若干思考

重复使用航天器具有快速、低成本的特性,是自由进出空间的重要技术途径之一。自从２0世纪50年代重复使用航天器的概念被提出以来,历经７０多年,重复使用航天器的研制取得了很大的进步,积累了丰富的经验和教训。基于国内外发展情况,梳理了重复使用航天器的技术路线,深入分析了其发展趋势,从设计、制造、试验、运行维护4个方面探讨了重复使用航天器的特点和难点,并提出了未来重复使用航天器发展的若干思考与建议。     

玻璃熔窑计算机控制的现状和展望

玻璃熔制是一个非常复杂的物理变化、化学反应过程，为了获得高质量的玻璃制品，必须要稳定熔窑热工制度，即习惯上称的“四大稳”。为此整个熔制过程控制分为五个系统：窑温控制系统、窑压控制系统、玻璃液面控制系统、燃烧控制系统以及火焰换向控制系统。目前，自动控制技术对提高玻璃熔窑热效率、降低能耗和稳定生产过程的作用，已充分被人们所认识。本文介绍了玻璃熔窑自动控制的现状，归纳并分析了四大类中小规模计算机控制系统在玻璃行业的应用现状，并对玻璃熔密计算机控制的发展方向。提出了一些看法。     

舰载直升机的研究现状与发展趋势

从舰载直升机的发展历史出发,首先给出了舰载直升机的主要使命和任务,并对国外先进舰载直升机主要机型进行梳理和分析,总结了国外舰载直升机的特点;然后,从舰载直升机使用特殊性考虑,详细阐述了其使用环境特点,提出了舰载直升机应具有的特殊要求,即良好的环境适应性和舰机适配性,同时分析给出了舰载直升机的指标要求;最后,通过对舰载直升机发展趋势的探究,提出了国内舰载直升机的发展建议.     

Mapping seasonal trends of electron temperature in the topside ionosphere based on DEMETER data

The diurnal, seasonal and latitudinal variations of the electron temperature in the Earth‘s topside ionosphere during relatively low solar activity period of 2005 – 2008 are investigated. In order to examine seasonal variations and morphology of the topside ionospheric plasma temperature, CNES micro-satellite DEMETER ISL data are used. Presented study is oriented on the dataset gathered in 2005 and 2008. Within conducted analysis, global maps of electron temperature for months of equinoxes and solstices have been developed. Furthermore, simultaneous studies on two-dimensional time series based on DEMETER measurements and predictions obtained with the IRI-2012 model supply examination of the topside ionosphere during recent deep solar minimum. Comparison with the IRI-2012 model reveals discrepancies between data and prediction, that are especially prominent during the periods of very low solar activity.     

美国空军未来的装备与技术——2010"技术地平线"报告分析

介绍了美国空军2010年发布的"技术地平线"的出台背景、主要内容.并根据该研究报告浅析了美国空军未来的装备与技术趋向.     

On the long-term variability of the heliosphere–magnetosphere environment

Annual means of measured and reconstructed solar, heliospheric, and magnetospheric parameters are used to infer solar activity signatures at the Hale and Gleissberg cycles timescales. Available open solar flux, modulation strength, cosmic ray flux, total solar irradiance data, reconstructed back to 1700, solar wind parameters (speed and density) and the magnitude of the heliospheric magnetic field at 1 AU, reconstructed back to 1870, as well as the time series of geomagnetic activity indices (aa, IDV, IHV), going back to 1870, have been considered. Simple filtering procedures (successive 11-, 22-, and 88-year running averages and differences between them) and scaling by the standard deviation from the average value for the common interval covered by the data show that the long-discussed variation in the 20th century (a pronounced increase since ∼1900, followed by a depression in the ‘60s and a new, slower, increase) seen in the 11-year averages of parameters such as geomagnetic activity indices and reconstructed heliospheric magnetic field strength, solar wind speed, open solar flux, is a result of the superposition in data of solar activity signatures at Hale and Gleissberg cycles timescales. The Hale and Gleissberg signals were characterized and similarities and differences in the temporal behavior of the analyzed parameters at these timescales are discussed. The similarities in the studied parameters point to a common pacing source, the solar dynamo.     

一种应用于空间碎片演化模型的碰撞概率算法

针对碰撞概率算法Cube模型参数影响空间碎片演化模型的仿真结果问题进行了深入分析与研究，并将原Cube算法进行改进，由此提出I-Cube模型。经过多次蒙特卡洛仿真结果验证，I-Cube模型对演化过程中空间碎片碰撞概率的计算更为准确合理，空间碎片长期演化模型的结果不再依赖于自身碰撞概率算法的相关参数，提高了空间碎片长期演化模型的稳定性与可信度。     

Long-term photometric signature study of two GEO satellites

Geostationary earth orbit satellites have been extensively used for unique high-orbit stationary characteristics. Long-term precise investigation is an important issue in the observation of GEO satellites, since it can provide valuable information on the satellites’ operation state, discrimination and early warning analysis. Ground-based optical-electronic devices play a significant role in the observation. 4-month photometric signature variation of two satellites is presented based on the successive observations using the 1.56-meter telescope of Shanghai Astronomical Observatory (SHAO). It can be concluded that the long-term brightness change mainly results from the sun declination angle and regular orbit maneuver. Moreover, the solar panel offsets of the two satellites are analyzed and found to be approximately 4 degrees. Estimation of photometric accuracy reaches 0.15 mag for the application of CCD drift-scan optical-electronic technique.     

美国深空测控通信技术动向分析

文章详细介绍了美国深空测控通信技术的发展动向,并对其未来规划进行了较为详细的综述和分析。     

Analytical long-term evolution and perturbation compensation models for BeiDou MEO satellites

The current paper establishes the analytical models of the long-term evolution and perturbation compensation strategy for Medium Earth Orbits(MEO)shallow-resonant navigation constellation,with application to the Chinese Bei Dou Navigation Satellite System(BDS).The long-term perturbation model for the relative motion is developed based on the Hamiltonian model,and the long-term evolution law is analyzed.The relationship between the control boundary of the constellation and the offset of the orbital elements is analyzed,and a general analytical method for calculating the offset of the orbit elements is proposed.The analytical model is further improved when the luni-solar perturbations are included.The long-term evolutions of the BDS MEO constellation within 10 years are illustrated,and the effectiveness of the proposed analytical perturbation compensation calculation approach is compared with the traditional numerical results.We found the fundamental reason for the nonlinear variations of the relative longitude of ascending node and the mean argument of latitude is the long-periodic variations of the orbital inclination due to the luni-solar perturbations.The proposed analytical approach can avoid the numerical iterations,and reveal the essential relationship between the orbital element offsets and the secular drifts of the constellation configuration.Moreover,there is no need for maintaining the BDS MEO constellation within 10 years while using the perturbation compensation method.