慢车抽真空状态转速摆动故障排除方法研究

以某型发动机慢车抽真空状态转速摆动故障为研究对象，对故障发生机理进行分析，制定相应的排故策略，并通过具体案例验证了排故措施的有效性。     

MHD modeling of the outer heliosphere: Achievements and challenges

An overview is presented of magnetic-field-related effects in the solar wind (SW) interaction with the local interstellar medium (LISM) and the different theoretical approaches used in their investigation. We discuss the possibility that the interstellar magnetic field (ISMF) introduces north–south and east–west asymmetries of the heliosphere, which might explain observational data obtained by the Voyager 1 and Voyager 2 spacecraft. The SW–LISM interaction parameters that are responsible for the deflection of the interstellar neutral hydrogen flow from the direction of propagation of neutral helium in the inner heliosheath are outlined. The possibility of a strong ISMF, which increases the heliospheric asymmetry and the H–He flow deflection, is discussed. The effect of the combination of a slow-fast solar wind during solar minimum over the Sun’s 11-year activity cycle is illustrated. The consequences of a tilt between the Sun’s magnetic and rotational axes are analyzed. Band-like areas of an increased magnetic field distribution in the outer heliosheath are sought in order to discover regions of possible 2–3 kHz radio emission.     

时序信号设计的一种新方法

文章结合高速时序工作的特点，从实现的角度提出了一种利用软件调整时序的新方法。在可编程逻辑器件中，利用数字时钟管理器（DCM），通过模块化和增量式设计思想达到对高速时序信号的精确调节。最终实现了一个20MHz速率的时序控制，调节精度达到100ps。     

NPU-WA系列风力机翼型设计与风洞实验

针对兆瓦级大型风力机,研究发展了以具有更优良高雷诺数和高升力气动性能为特点的NPU-WA翼型族,风洞实验表明,该翼型族达到了在高雷诺数、高升力条件下实现高升阻比和外侧翼型对粗糙度不敏感的主要设计要求,为我国自主研发大型风力机提供了可以实际使用的翼型几何数据和雷诺数范围内1.0×106～5.0×106的风洞实验数据。     

大迎角耦合运动非定常空气动力特性

采用某飞机大迎角大振幅运动风洞实验结果，分析了大迎角非定常空气动力的一些特性。结果表明，飞机机动飞行时多自由度运动的气动特性比单自由度运动复杂，耦合运动时的气动特性和两个单自由度运动的气动特性的叠加结果相比有一定差别。此外，旋转天平实验结果同本实验的结果相比差别较大。     

固态染料敏化太阳能电池用聚苯胺-乙炔黑空穴导体的制备

以粘土状的聚苯胺-乙炔黑导电材料为空穴导体,制备了固态染料敏化太阳能电池.研究结果表明,将乙炔黑颗粒加入到聚苯胺电解质中,可明显提高该固态染料敏化太阳能电池的光电转换效率.这是由于加入的乙炔黑不仅可以提高聚苯胺电解质的空穴迁移率,改善其可润湿性,而且加强了电解质与光阳极以及对电极之间的界面接触性.最后,加入50%乙炔黑的聚苯胺电解质的电池光电转换效率达到了液态电池的48%.因此,聚苯胺-乙炔黑复合电解质可以作为有效的空穴导体材料,应用到固态染料敏化太阳能电池中.     

Is there an instrumental drift in the counting rate of some high latitude neutron monitors?

For the last six decades the neutron monitors have provided a continuous string of very reliable data to the heliophysics community. Although neutron monitors are not the primary source of data for the galactic cosmic rays, these data serve as a baseline reference for the data collected by the detectors on board the satellites and deep space probes, far away from earth orbit. The pressure corrected hourly data are available from the World Data Centers. These data have been used to derive deep insights pertaining to the electromagnetic states of the heliosphere and the modes of transport of energetic charged particles in the tangled interplanetary magnetic fields. We present evidence that some of the high latitude neutron monitors are undergoing long-term drifts in their baselines. In particular, we argue that there is no physical basis to justify the observed long-term downward trend in the baseline of the South Pole neutron monitor. The real reason may have to do with its maintenance at a distant location with challenging logistics and an improper normalization of its data after the 26 months break in the 1970s.     

Compressible Aspects of Slow Solar Wind Formation

Recently we have shown how the slow solar wind can be formed within a coronal helmet streamer. The solar wind is modeled by a "wake-neutral" sheet, whose subsequent linear and nonlinear evolution provides clues to the development of the wind. In this paper we describe the first results of our extension of this model to the compressible regime. In particular, we show that traveling density enhancements are formed, similar to those observed by LASCO. The compressible equations are solved by an extension to MHD of the SPECLS algorithm. This revised version was published online in June 2006 with corrections to the Cover Date.     

Anomalous Cosmic Rays and Solar Modulation

We review aspects of anomalous cosmic rays (ACRs) that bear on the solar modulation of energetic particles in the heliosphere. We show that the latitudinal and radial gradients of these particles exhibit a 22-year periodicity in concert with the reversal of the Sun's magnetic field. The power-law index of the low energy portion of the energy spectrum of ACRs at the shock in 1996 appears to be -1.3, suggesting that the strength of the solar wind termination shock at the helioequatorial plane is relatively weak, with s 2.8. The rigidity dependence of the perpendicular interplanetary mean free path in the outer heliosphere for particles with rigidities between 0.2 and 0.7 GV varies approximately as R2, where R is particle rigidity. There is evidence that ACR oxygen is primarily multiply charged above 20 MeV/nuc and primarily singly-charged below 16 MeV/nuc. The location of the termination shock was at 65 AU in 1987 and 85 AU in 1994.     

一种新Turbo码交织器的VHDL设计

介绍了Turbo码和交织技术，分析了几种常用交织算法的特点。根据组合交织器的设计思路，提出了隔行写入螺旋式交织方案。利用硬件描述语言（VHDL）编程设计了这种交织器的电路，并给出了仿真结果。