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.     

三维四向编织复合材料等效热特性数值分析和试验研究

 采用“米”字型枝状胞体有限元模型和试验方法对三维四向编织复合材料的整体等效热膨胀系数和等效热传导系数进行了分析并将计算结果和试验值进行了比较。研究表明枝状胞体模型能较为真实的反映三维四向编织复合材料的结构构形;有限元方法在分析热膨胀、热传导方面具有较好的精度;三维四向编织复合材料编织方向的热膨胀系数随着纤维体积比的增加而减小,随着编织角的增加而减小;热传导系数随着纤维体积比的增加而增大,随着编织角的增大而增大。     

刚性太阳电池阵基板的研究

文章简要地叙述碳纤维复合材料刚性太阳电池阵基板的结构设计,理论分析,模态试验和振动试验。理论分析和试验结果比较一致。通过试验还解决了基板各种复合材料的力学性能测试问题,取得了必要的数据。     

称重传感器的一种新的滞后补偿方法

通过对电阻应变式称重传感器在各种加载卸载情况下的滞后特性的分析,建立了其相应的数学模型,并初步探讨了一种可以通过程序在仪表中对传感器的重要指标-滞后进行补偿从而提高整个传感器的精度的方法.最后,对以上方法进行了验证性试验,证明了补偿方法的可行性.     

CONTROL STRUCTURE AND IMPLEMENTATION OF CELL CONTROL SYSTEM

在计算机集成制造系统（ＣＩＭＳ）的递阶控制结构中，单元控制系统起着重要作用。它上端联接车间控制系统和ＣＡＤ／ＣＡＰＰ／ＣＡＭ系统，下端联接生产设备，直接影响到生产的柔性和效率。该系统根据生产任务和目标，完成了生产计划调度、资源分配、监控设备运行等功能。文中主要讨论了系统的控制结构、系统功能和以下主要关键技术：客户／服务体系结构在生产控制和管理中的应用，单元生产计划和调度，ＤＮＣ接口以及生产中的随机事件处理。该系统已在应用中取得良好的经济效益。     

燃料电池电动车用隔离Boost全桥变换器的研究

针对燃料电池电动车辅助能源系统低压大功率、大升压比的特点,分析了几种隔离变换器方案,这几种方案均难以做到大功率应用。为此,提出了采用隔离Boost全桥变换器拓扑方案可有效地解决上述技术难点。文中介绍了该方案的原理,详细分析了控制系统,给出了数字化控制的实现方法和主电路关键参数的设计。为了验证上述方案的正确性,设计了5 kW,24 V输入300 V输出的隔离Boost全桥变换器。实验结果表明,系统具有良好的动态和静态性能,能有效地应用于电动汽车等领域。     

三块各向正交异性矩形板构成的卫星帆板在各种载荷下的横向弯曲

本文以三块各向正交异性矩形板组成的卫星帆板为研究对象,首次利用半解析方法研究了其横向弯曲的问题。就板间连接处复杂的边界条件,提出了与之对应的挠度函数形式。在此基础上采用相同形式的挠度函数求出了帆板在各种横向外载荷作用下的挠度,为解决多板连接结构的弯曲问题提供了一种有别于以往数值方法的新思路。     

含边界和损伤因素的纺织复合材料细观胞元模型

纺织复合材料的细观力学分析通常以胞元模型为基础,胞元边界条件的合理施加是获得精确分析结果的关键之一。本文以平面机织复合材料为例,讨论了细观胞元的选取和周期边界条件的施加方法,在此基础上建立了二维细观有限元模型,通过与全厚度模型分析结果的比较,研究了周期胞元模型的合理性,特别是边界效应和局部损伤等非周期因素对分析结果的影响,给出了这些因素下胞元边界条件的处理方法。     

高性能的标准单元库设计

从仿真和流片两个方面对标准单元库的验证方法进行了研究.在仿真方面,提出了采用静态时序分析工具和SPICE仿真工具对单元的估算值和仿真结果进行比较分析的方法来验证,同时还给出了具体的操作步骤实例.在流片验证中,提出了一种非常有效的电路结构.这种电路结构不但能够准确验证时序,还能极大地减少PAD数量;最重要的特点是:该电路能够完全避免PAD和非被测单元的引入带来的额外延迟,从而得到准确的被测单元延迟.     

What do Cosmogenic Isotopes Tell us About Past Solar Forcing of Climate?

In paleoclimate studies, cosmogenic isotopes are frequently used as proxy indicators of past variations in solar irradiance on centennial and millennial timescales. These isotopes are spallation products of galactic cosmic rays (GCRs) impacting Earth's atmosphere, which are deposited and stored in terrestrial reservoirs such as ice sheets, ocean sediments and tree trunks. On timescales shorter than the variations in the geomagnetic field, they are modulated by the heliosphere and thus they are, strictly speaking, an index of heliospheric variability rather than one of solar variability. Strong evidence of climate variations associated with the production (as opposed to the deposition) of these isotopes is emerging. This raises a vital question: do cosmic rays have a direct influence on climate or are they a good proxy indicator for another factor that does (such as the total or spectral solar irradiance)? The former possibility raises further questions about the possible growth of air ions generated by cosmic rays into cloud condensation nuclei and/or the modulation of the global thunderstorm electric circuit. The latter possibility requires new understanding about the required relationship between the heliospheric magnetic fields that scatter cosmic rays and the photospheric magnetic fields which modulate solar irradiance.