弱太阳闪烁对深空通信的影响

行星聚合和太阳闪烁是影响深空通信的重要因素. 分析了行星聚合和太阳闪烁的物理特性, 建立了弱太阳闪烁条件下深空通信信道的Rician 模型, 并得出了当Rician 因子大于10 dB 时近似为高斯信道的结论. 对弱太阳闪烁下X 波段和Ka 波段的通信性能进行了仿真, 这对建立可靠的深空通信链路具有十分重要的意义.      

Possible influence of solar extreme events and related geomagnetic disturbances on human cardio-vascular state: Results of collaborative Bulgarian–Azerbaijani studies

This collaborative study is based on the analysis and comparison of results of coordinated experimental investigations conducted in Bulgaria and Azerbaijan for revealing a possible influence of solar activity changes and related geomagnetic activity variations on the human cardio-vascular state. Arterial blood pressure and heart rate of 86 healthy volunteers were measured on working days during a period of comparatively high solar and geomagnetic activity (2799 measurements in autumn 2001 and spring 2002) in Sofia. Daily experimental investigations of parameters of cardio-vascular health state were performed in Azerbaijan with a permanent group of examined persons. Heart rate and electrocardiograms were digitally registered (in total 1532 records) for seven functionally healthy persons on working days and Saturdays, in the Laboratory of Heliobiology at the Medical Center INAM in Baku, from 15.07.2006 to 13.11.2007. Obtained digital recordings were subjected to medical, statistical and spectral analyses. Special attention was paid to effects of solar extreme events, particularly those of November 2001 and December 2006. The statistical method of the analysis of variance (ANOVA) and post hoc analysis were applied to check the significance of the influence of geomagnetic activity on the cardio-vascular parameters under consideration. Results revealed statistically significant increments for the mean systolic and diastolic blood pressure values of the group with geomagnetic activity increase. Arterial blood pressure values started increasing two days prior to geomagnetic storms and kept their high values up to two days after the storms. Heart rate reaction was ambiguous and not significant for healthy persons examined (for both groups) under conditions with geomagnetic activity changes. It is concluded that heart rate for healthy persons at middle latitudes can be considered as a more stable physiological parameter which is not so sensitive to environmental changes while the dynamics of arterial blood pressure reveals a compensatory reaction of the human organism for adaptation.     

Thermal neutrons’ response to the GLEs

Thermal neutrons’ flux near the Earth’s crust is very sensitive regarding different processes and phenomena both in the near-Earth space and in the Earth’s crust by reason of the dual nature of the thermal neutron flux. Its first source is associated with high-energy particles of cosmic rays penetrating into the Earth’s atmosphere and interacting with its elements. The second source originates from the radioactive gases contained in the Earth’s crust. So the contributions of these two sources are specified by the Earth’s crust conditions and its movements, on one hand and variations of high-energy particles flux near the Earth.     

X-ray, γ-emission and energetic particles in near-Earth space as measured by CORONAS-F satellite: From maximum to minimum of the last solar cycle

The Russian solar observatory CORONAS-F was launched into a circular orbit on July 31, 2001 and operated until December 12, 2005. Two main aims of this experiment were: (1) simultaneous study of solar hard X-ray and γ-ray emission and charged solar energetic particles, (2) detailed investigation of how solar energetic particles influence the near-Earth space environment. The CORONAS-F satellite orbit allows one to measure both solar energetic particle dynamics and variations of the solar particle boundary penetration as well as relativistic electrons of the Earth’s outer radiation belt during and after magnetic storms. We have found that significant enhancements of relativistic electron flux in the outer radiation belt were observed not only during strong magnetic storms near solar maximum but also after weak storms caused by high speed solar wind streams. Relativistic electrons of the Earth’s outer radiation belt cause volumetric ionization in the microcircuits of spacecraft causing them to malfunction, and solar energetic particles form an important source of radiation damage in near-Earth space. Therefore, the present results and future research in relativistic electron flux dynamics are very important.     

SMESE: A SMall Explorer for Solar Eruptions

The SMall Explorer for Solar Eruptions (SMESE) mission is a microsatellite proposed by France and China. The payload of SMESE consists of three packages: LYOT (a Lyman imager and a Lyman coronagraph), DESIR (an Infra-Red Telescope working at 35–80 and 100–250 μm), and HEBS (a High-Energy Burst Spectrometer working in X- and γ-rays).

The status of research on flares and coronal mass ejections is briefly reviewed in the context of on-going missions such as SOHO, TRACE and RHESSI. The scientific objectives and the profile of the mission are described. With a launch around 2012–2013, SMESE will provide a unique tool for detecting and understanding eruptions (flares and coronal mass ejections) close to the maximum phase of activity.     

充气太阳能帆板展开动力学数值模拟预报

充气太阳能帆板是一种通过气体驱动支撑管展开的新型太阳能帆板。首先简要介绍其研究进展，然后针对充气展开支撑管，提出了分段式充气体积控制模型，基于LS—DYNA模拟了空间环境下Z型折叠充气太阳能帆板在支撑管无约束与有轴向约束控制时的展开过程，分析了支撑管每折叠段的气压变化，上横板的动力学特性以及基板的平面外振动，预报了展开过程中支撑管与基板的接触碰撞，并通过悬吊式展开试验验证了计算结果。结果表明，本文计算能够预报充气太阳能帆板在空间展开的动力学特性。     

利用太阳帆定点探测器在地一月系共线平动点附近的探讨

共线平动点附近的运动仅仅是条件稳定的,探测器的轨道需要经过控制才能维持在其附近.以地-月系11点和12点附近大振幅晕轨道的控制为例,探讨了太阳帆在定点这类探测器中的应用.首先,考虑了月球轨道的偏心率和太阳辐射的影响,给出了太阳帆对日定向的探测器轨道的低阶分析解,并在此基础上构造了在太阳系真实引力模型下一段时间内维持在共线平动点附近的拟周期轨道.然后,给出了两种利用太阳帆的控制方案,一是固定面质比而改变太阳帆法线的方向,另一是固定太阳帆对日定向而改变面质比,并对两种方案分别作了数值模拟.最后,文章探讨了测控误差及地、月影对轨道控制的影响.     

某型机座舱照明系统分析与改进

深入分析了某型机座舱照明"左明右暗"产生原因,进行了改进技术方案论证。根据飞机现状,提出了改进座舱照明效果最优技术方案。     

纹影技术中光源的选择与设计方法

在纹影技术应用过程中,纹影光源的性能一定程度上决定了拍摄结果的优劣.不同种类的光源,得到的拍摄效果不同,对于某种特定拍摄需求,光源的选择和设计也不同.如何选择和设计合适的纹影光源,对于最终拍摄结果的好坏至关重要.结合纹影技术在工程实际中的应用,分析了不同被测对象对光源的需求,总结了几种常见光源的应用情况及其特点,提供了一种光源参数设计的方法.在实验室典型超声速自由射流流场测量中,对卤钨灯、氙灯和激光3种纹影光源的应用进行了对比分析.所提出的纹影光源的选择与设计方法,具有一定的工程实验参考价值.     

基于光纤延迟的光脉冲有源复制器

根据高速光脉冲测量系统应用的需求,提出了使用循环式光纤光脉冲有源复制器实现模拟短脉冲信号的低噪音、低失真复制的一种方法.针对有源复制器中半导体光放大器(SOA)带来的放大自发辐射(ASE)光噪声与非线性失真,建立了SOA的计算模型,并对光脉冲在复制器中的循环传输性能进行了仿真和分析.仿真结果证明了使用外加直流光注入方法抑制波形失真的有源复制器方案是可行的,同时为合理选择注入直流光功率及环内损耗等参数,实现复制器的优化设计提供了依据.