基于BICMOS电流控制型多路输出电源的研制

介绍一种适用于低压、宽范围供电的多路输出DC/DC变换器,在功率电路中使用无损耗箝位电路实现了变压器磁芯的复位,控制电路使用第三代BICOMS电流控制型PWM,简化了电路设计、降低了噪声敏感度,给出了多路输出电源中变压器和耦合电感的工程设计的详细过程,同时分析了多路输出耦合电感对负载交叉调节性能的影响.研制的变换器输入电压范围8V-40VDC,输出5V/3A、±15V/0.5A、 10V/0.5A.     

失谐周期压电复合材料结构中的波动局部化研究

考虑力电耦合效应的影响,研究了层状失谐周期压电复合材料结构中的波动局部化问题。根据界面上力电连续条件,推导了结构中相邻单胞间的传递矩阵。以力场和电场变量为状态向量,给出了结构中局部化因子的表达式。作为算例,计算了结构中的波动局部化因子。计算结果表明,压电陶瓷的压电效应对周期压电复合材料的波动局部化特性有显著影响,压电常数越大局部化因子值越大,结构的局部化程度越强;结构的失谐度越大,频率通带区间内的局部化因子值越大,局部化程度越强。分析结果对于周期压电复合材料结构的优化设计和振动控制具有理论参考价值。     

Solar Irradiance Variability Since 1978

Since November 1978 a set of total solar irradiance (TSI) measurements from space is available, yielding a time series of more than 25 years. Presently, there are three TSI composites available, called PMOD, ACRIM and IRMB, which are all constructed from the same original data, but use different procedures to correct for sensitivity changes. The PMOD composite is the only one which also corrects the early HF data for degradation. The results from the detailed analysis of the VIRGO radiometry allow a good understanding of the effects influencing the long-term behaviour of classical radiometers in space. Thus, a re-analysis of the behaviour of HF/NIMBUS-7 and ACRIM-I/SMM was indicated. For the former the situation is complicated by the fact that there are no in-flight means to determine changes due to exposure to solar radiation by comparison with a less exposed radiometer on the same spacecraft. The geometry and optical property of the cavity of HF is, however, very similar to the PMO6-type radiometers, so the behaviour of the PMO6V radiometers on VIRGO can be used as a model. ACRIM-I had to be revised mainly due to a henceforth undetected early increase and a more detailed analysis of its degradation. The results are not only important for solar radiometry from space, but they also provide a more reliable TSI during cycle 21. The differences between the revised PMOD composite and the ACRIM and IRMB are discussed by comparison with a TSI reconstruction from Kitt-Peak magnetograms. As the PMOD composite is the only one which has reliable data for cycle 21, the behaviour of the three solar cycles can now be compared and the similarities and differences discussed.     

Global Response of Martian Plasma Environment to an Interplanetary Structure: From Ena and Plasma Observations at Mars

As a part of the global plasma environment study of Mars and its response to the solar wind, we have analyzed a peculiar case of the subsolar energetic neutral atom (ENA) jet observed on June 7, 2004 by the Neutral Particle Detector (NPD) on board the Mars Express satellite. The “subsolar ENA jet” is generated by the interaction between the solar wind and the Martian exosphere, and is one of the most intense sources of ENA flux observed in the vicinity of Mars. On June 7, 2004 (orbit 485 of Mars Express), the NPD observed a very intense subsolar ENA jet, which then abruptly decreased within ∼10 sec followed by quasi-periodic (∼1 min) flux variations. Simultaneously, the plasma sensors detected a solar wind structure, which was most likely an interplanetary shock surface. The abrupt decrease of the ENA flux and the quasi-periodic flux variations can be understood in the framework of the global response of the Martian plasma obstacle to the interplanetary shock. The generation region of the subsolar ENA jet was pushed towards the planet by the interplanetary shock; and therefore, Mars Express went out of the ENA jet region. Associated global vibrations of the Martian plasma obstacle may have been the cause of the quasi-periodic flux variations of the ENA flux at the spacecraft location.     

原子氧对Kapton／Al薄膜性能影响研究

模拟空间环境下原子氧辐照条件,通过采用固定的原子氧束流密度进行不同时间辐照试验,研究了温控涂层材料Kapton/Al薄膜的质量损失、光学性能、表面形貌和表面粗糙度的演化规律.试验结果表明,原子氧对材料的剥蚀量与原子氧的作用时间成正比例关系.材料辐照后太阳吸收率发生明显变化,而辐射率几乎不发生变化.辐照后试样表面的粗糙度,是影响太阳吸收率变化主要因素.随着辐照时间的增长,材料表面粗糙度增加,导致太阳吸收率增大.     

直升机桨叶刚柔耦合特性及计算方法分析

为了研究桨叶刚柔耦合特性,采用中等变形梁模型处理桨叶弹性变形,分别采用小转角和有限转角两种方法处理桨叶绕铰的刚性运动。以桨叶扬起下坠碰撞问题为研究对象。计算分析表明:(1)弹性桨叶存在较明显的刚性运动和弹性变形耦合;(2)挥舞角较小时,两种处理方法计算结果一致,均与试验数据吻合较好;(3)挥舞角较大时,刚柔耦合增强,两种处理方法的计算值差别较为明显;(4)桨叶弯曲刚度对桨叶刚柔耦合特性有较明显影响,刚度越小,耦合越强;(5)桨叶如果比较柔软,小转角处理方法计算值相对有限转角处理方法,相位滞后、幅值增加均较为明显,计算桨叶动响应时需引起注意。      

Solar and Solar-Wind Composition Results from the Genesis Mission

The Genesis mission returned samples of solar wind to Earth in September 2004 for ground-based analyses of solar-wind composition, particularly for isotope ratios. Substrates, consisting mostly of high-purity semiconductor materials, were exposed to the solar wind at L1 from December 2001 to April 2004. In addition to a bulk sample of the solar wind, separate samples of coronal hole (CH), interstream (IS), and coronal mass ejection material were obtained. Although many substrates were broken upon landing due to the failure to deploy the parachute, a number of results have been obtained, and most of the primary science objectives will likely be met. These objectives include He, Ne, Ar, Kr, and Xe isotope ratios in the bulk solar wind and in different solar-wind regimes, and ¹⁵N/¹⁴N and ¹⁸O/¹⁷O/¹⁶O to high precision. The greatest successes to date have been with the noble gases. Light noble gases from bulk solar wind and separate solar-wind regime samples have now been analyzed. Helium results show clear evidence of isotopic fractionation between CH and IS samples, consistent with simplistic Coulomb drag theory predictions of fractionation between the photosphere and different solar-wind regimes, though fractionation by wave heating is also a possible explanation. Neon results from closed system stepped etching of bulk metallic glass have revealed the nature of isotopic fractionation as a function of depth, which in lunar samples have for years deceptively suggested the presence of an additional, energetic component in solar wind trapped in lunar grains and meteorites. Isotope ratios of the heavy noble gases, nitrogen, and oxygen are in the process of being measured.     

利用模拟试验研究APC预测准则的适应性

使用多种飞机系统构型的人机耦合(APC)振荡地面模拟试验数据,研究各种Ⅰ类、Ⅱ类APC预测准则的适用性,通过对比分析试验中试飞员评分结果和各种准则计算结果,得到APC预测准则与试飞员APC趋势评分的符合率。研究结果表明,现有的APC预测准则并非预想的那样有效,进而针对APC预测准则和模拟试验提出改进建议。     

航天器太阳电池阵驱动装置的新进展

通常长寿命三轴稳定卫星都采用帆板式太阳电池阵进行能源供应,并使用太阳电池阵驱动装置使电池阵对日定向。国际上从20世纪60年代开始,不断开发研制太阳电池阵驱动装置,以满足在大功率、小型化、适应恶劣环境等方面的特殊需求,经过几代的发展,取得了长足的进步。根据国内收集的相关信息和资料,通过介绍国际该领域的发展及对应需求的典型产品,尝试分析该领域中相应的应用、研究的重点及发展的方向。