并网逆变器闭环控制带宽对死区效应的抑制

阐述了死区效应的产生机理及其在开环控制下对逆变器输出基波电压的影响和死区谐波频谱分布情况。在此基础上,通过闭环传递函数带宽分析,定量地分析了闭环系统对死区效应的抑制作用以及控制带宽大小对抑制死区效应效果的关系。以单电流闭环控制的LCL滤波并网逆变器系统为例,进行闭环控制带宽对死区效应抑制的仿真验证。最后,在一台250kW三相并网逆变器上进行实验验证。仿真和实验结果证明了理论分析的正确性。     

一种热平衡等温机制的新型热防护及相关技术

给出了一种适用于高超声速飞行器热防护的新概念——疏导式热防护,其基本理论是利用热平衡等温机制,使防热层趋于一等温体,实现热负载平衡。针对这一概念,进行了较为系统的研究,包括原理、分析方法、实现疏导式热防护的关键技术。研究结果表明,疏导式热防护技术可有效地减少高热流区的温度和热应力,是一种有效的非烧蚀热防护技术。     

FL-8风洞旋转天平试验支架干扰研究（英文）

给出了FL-8风洞进行旋转天平试验支架干扰研究的情况,对试验方法、设备和试验结果进行了介绍。为了实现圆弧形滑轨与模型支杆的支撑和变角功能,特别设计了新型的变角支杆。试验结果表明：支架干扰对纵横向气动力的影响规律是不同的,对纵向结果的影响是与旋转方向无关的,而对横向结果的影响在正反旋转时是相反的。尾撑和背撑试验结果经过支架干扰修正后向相同的值靠近,说明支架干扰修正的结果是合理的,提高了试验结果的准度。     

Φ5m立式风洞旋转天平试验装置研制

Φ5m立式风洞旋转天平试验装置是为开展飞机尾旋特性研究而研制的重要基础设备,主要用于测定模型在绕风轴以不同速率作等速旋转状态下的气动特性,为飞机尾旋特性的分析和预测提供必要的气动参数。该装置采用双立柱弧形轨结构形式,采用网络一体化试验管理和控制模式,不但能够开展旋转天平试验,而且还具备动导数试验、大迎角试验、旋转/振荡耦合试验等功能。主要介绍旋转天平试验装置系统组成和设计,分析了引导性试验结果,最后给出了结论。     

Harmonic analysis of the ionospheric electron densities retrieved from FORMOSAT-3/COSMIC radio occultation measurements

In order to investigate the regular variations of the ionosphere, the least-squares harmonic estimation is applied to the time series of ionospheric electron densities derived from about five years of Global Positioning System radio occultation observations by FORMOSAT-3/COSMIC satellites. The analysis is done for different latitudes and altitudes in the region of Iran. The least-squares harmonic estimation is found to be a powerful tool for the frequency analysis of the completely unevenly spaced time series of radio occultation measurements. Although the obtained results are slightly different from the exact expected cycles (i.e. annual and diurnal components with their Fourier decompositions, and the 27-day period) due to the low horizontal resolution of radio occultation measurements, high vertical resolution of the observations enables us to detect not only the total electron content variations but also periodic patterns of electron densities at different altitudes of the ionosphere. The dominant diurnal and annual signals together with their Fourier series decompositions are obtained, which are consistent with the previous analyses on the total electron content. In the equatorial anomaly band, the annual component is weaker than its Fourier decomposition periods. In particular, the semiannual period dominates the annual component, indicating the relationship between the semiannual variation of the electron densities and the ionospheric equatorial anomaly. From detection of the phases of the components, it is revealed that the annual signal generally has its maximum value in summers at high altitudes, and in the winters at low altitudes. This is probably due to the higher [O/N₂] ratios in winter than in the summer in the lower ionosphere. Furthermore, the semiannual component mostly peaks around solstices or about a month before/after them.     

测量气体活塞式压力计有效面积时气柱差的误差分析

目前多采用起始平衡法测量气体活塞有效面积,起始平衡法是用一定的小砝码来消除两活塞参考面液（气）体的高度差所产生的压力,即认为液（气）柱所产生的压力是不变的。但由于气体的可压缩性,气体密度随压力变化而变化,这就造成了气柱高度虽然不变,而气柱所产生的压力却是变化的,从而产生测量误差。本文就此问题进行分析,力求使气体活塞式压力计的量值传递更准确。     

高超声速飞行器相关的摩擦阻力直接测量技术

摩擦阻力是高超声速飞行器气动力的重要组成部分,也是制约高超声速飞行器发展的重要因素,因而对摩擦阻力的准确测量就显得尤为重要.简要介绍了近年国内外与高超声速相关的摩擦阻力直接测量技术的发展状况,同时对中国航天空气动力技术研究院自行研制的两套摩擦阻力测量装置作了介绍,并指出应变式摩阻天平技术是测量摩擦阻力的有效途径之一.文中给出了这两种结构形式摩阻天平的静校结果及其在高超声速风洞中的试验结果,并对结果进行了讨论.     

供电系统的干扰模式及抑制措施

供电系统的电磁干扰主要由发电机噪声、整流谐波、开关频率和它的谐波,以及在开关转换中高速电流和电压的瞬变所引起,这些干扰可通过传导和辐射的方式直接影响交流电网和用电设备。所以,本文所要讨论的主要问题就是电磁干扰的解决方法。     

两种小力值校准装置研究

介绍了小力值校准的应用现状和需求;详述了两种结构的小力值校准装置的技术指标、工作原理、结构设计;最后给出了小力值校准装置的部分比对试验数据。     

Lunar gravity field modeling critical analysis and challenges

This paper summarizes and provides a critical analysis of the historical developments of lunar gravitational models from the earliest use of ground based tracking systems of the Lunar Orbiter to the Lunar Prospector mission. This encompasses a comprehensive and critical analysis of the various methods used in the estimation of the gravity coefficients and the processing of large batches of diverse measurements and data types. It has been shown that weakness exists in the current models of the lunar gravity field, which is primarily due to the lack of far side lunar tracking data information, which makes the lunar potential modeling difficult but expected to be overcome as data from SELENE satellite-to-satellite tracking becomes available. Comparisons of various lunar models reveal an agreement in the low order coefficients of the spherical harmonics. However, substantial differences in the models exist in the higher-order harmonics. A numerical comparison has been presented showing the performance of all the contemporary lunar gravitational models used within the astrodynamics community and available in public domain. Improvements to the current models are part of a continuing process and the recent model improvements and future possibilities in lunar gravity modeling are discussed. A brief review of the recent missions has been presented. It is hoped that this critical review will benefit the researchers by presenting the historical as well as state of the art in this field.