多螺旋桨太阳能无人机横航向操稳特性研究

首先分析了大型高空长航时太阳能无人机由于超大展弦比和高效多螺旋桨带来的航向阻尼增量和航向操纵导数,接着分析了由此带来的横航向动态特性变化,并结合多螺旋桨的操纵特性,提出了多桨航向控制方法,最后进行了仿真验证.结果表明,分布式多桨布局对提高该类无人机的横航向稳定性有较大作用,以多桨的转速变化量最小为目标的最优化航向控制分配方法对超长航时飞行很有利.     

发动机高压两级涡轮盘联合低循环疲劳寿命试验

以某型发动机高压两级涡轮盘为研究对象,通过有限元计算得到试验载荷系数,组装和调试了全尺寸联合试验件,完成了低循环疲劳试验,得到了以传动臂销钉孔为定寿部位的两级涡轮盘低循环疲劳寿命。两级涡轮盘联合低循环疲劳试验在国内尚属首次,相对于单盘低循环疲劳试验,更加符合发动机实际工作状态,将传动臂销钉孔作为两级涡轮盘的定寿部位更为合理。该联合试验为外场涡轮盘重新定寿提供了依据。     

变循环发动机模态转换数值模拟

对双外涵变循环发动机的模态转换过程进行了研究,设计了变循环发动机模态转换方案,确立了模态转换时的多部件调节规律,采用稳态模型对模态转换进行了数值模拟.结果表明,所设计的模态转换方案可行,能够使变循环发动机的涵道比发生明显改变,并有效提高了发动机在部分推力时的空气流量,与设计参数相同的常规涡扇发动机相比,其安装耗油率明显降低.      

The Modulation of Galactic Cosmic Rays in the Heliosphere: Theory and Models

Almost all theoretical and numerical models for the modulation of cosmic ray in the heliosphere are based on Parker's transport equation which contains all the important basic physical processes. The relative importance of the various mechanisms is however not established and may vary significantly over 22 years. The simultaneous measurements of solar wind parameters, heliospheric magnetic field properties and cosmic rays over a wide range of energies and positions in the heliosphere have brought the realization that modulation is much more complicated than what the original drift models predicted. In the process the sophistication of models based on solving Parker's equation has increased by orders of magnitude. A short review of the global modulation of cosmic rays is given from a theoretical and modelling point of view.     

布雷顿和卡诺热机循环性能比较(Ⅱ)定常态流变温热源循环

研究定常态变温热源热机循环性能，导出内可逆卡诺热机和布雷顿热机的最佳功率、效率关系和最大功率及相应的效率界限，并对这两种热机循环的最优性能进行了比较。理论分析表明，在相同的边界条件和热效率下，布雷顿循环的功率可以高于卡诺循环的功率，极限情况下前者是后者的两倍。对于变温热源条件，布雷顿循环主要受益于其工质与热源间有较佳的匹配。所得结果对热机工作参数和工质的最优选择有一定指导意义。     

一种定向凝固高温合金低周疲劳性能的研究

研究了同成分合金在定向凝固（ＤＳ）和普通铸造（ＣＣ）状态下７６０℃的低周疲劳性能。结果表明，ＤＳ合金的疲劳寿命比ＣＣ合金在应力控制条件下高２倍左右，而在应变控制条件下可提高寿命２０倍左右。ＣＣ合金的疲劳裂纹往往萌生在与表面相连的晶界或某些缺陷（如孔洞）上，由外向内沿晶界扩展。而ＤＳ合金裂纹则起源于纵向晶界的横段或预开裂的碳化物，并沿枝晶间穿枝干扩展。     

Energetic particles at high latitudes

We review work on diffusion coefficients of energetic particles with an attempt to extract implications on their behaviour at high latitudes. In the ecliptic plane results from solar energetic particle propagation between the Sun and about 5 AU can be described by an effective radial mean free path _r which is approximately constant as a function of distancer. When particle propagation in three dimensions in the heliosphere is considered it is not sufficient to consider _r only. Jovian electrons can be used as probes to determine the parameters of three-dimensional diffusion. In the polar regions diffusion is dominated by its parallel component. Some predictions how should vary with latitude are discussed. For different choices of this variation we present expectations for intensity-time profiles of solar particle events during the Ulysses polar passages.     

应力集中对GH2036合金低周疲劳—蠕变性能的影响

在对光滑试件和缺口试件进行高温疲劳－蠕变实验的基础上,分析了应力集中对ＧＨ２０３６合金低周疲劳－蠕变特性的影响。结果表明缺口试件的循环寿命远远低于光滑试件的循环寿命。将应变范围划分方法和改进的Ｎｅｕｂｅｒ原理相结合,得到了缺口部位高温低周疲劳－蠕变寿命估测的方法。用该方法估算ＧＨ２０３６合金的寿命并与实测寿命结果进行比较,证明此方法的预测效果良好。     

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.