Decay of Magnetic Field Irregularities Observed by Ulysses

We study the solar cycle, radial, and latitudinal dependence of the characteristics of magnetic field irregularities in the Heliosphere. The frequency of magnetic field discontinuities is determined, using high time resolution magnetic field observations by Ulysses, covering the time interval from 1992 to 2000. The quasi-linear scattering mean free path of particles is also calculated. These investigations aim at understanding/exploring transport properties of energetic charged particles in the Heliosphere. We find that the travel time of solar wind plasma from the Sun to the observer is the key parameter of the process, by controling the decay of the irregularities. This revised version was published online in August 2006 with corrections to the Cover Date.     

The Heliospheric Magnetic Field at Solar Maximum: Ulysses Observations

At solar maximum, the large-scale structure of the heliospheric magnetic field (HMF) reflects the complexity of the Sun's coronal magnetic fields. The corona is characterised by mostly closed magnetic structures and short-lived, small coronal holes. The axis of the Sun's dipole field is close to the solar equator; there are also important contributions from the higher order terms. This complex and variable coronal magnetic configuration leads to a much increased variability in the HMF on all time scales, at all latitudes. The transition from solar minimum to solar maximum conditions, as reflected in the HMF, is described, as observed by Ulysses during its passage to high southern heliolatitudes. The magnetic signatures associated with the interaction regions generated by short-lived fast solar wind streams are presented, together with the highly disordered period in mid-1999 when there was a considerable reorganisation in coronal structures. The magnetic sector structure at high heliolatitudes shows, from mid-1999, a recognisable two-sector structure, corresponding to a highly inclined Heliospheric Current Sheet. A preliminary investigation of the radial component of the magnetic field indicates that it remains, on average, constant as a function of heliolatitude. Intervals of highly Alfvénic fluctuations in the rarefaction regions trailing the interaction regions have been, even if intermittently, identified even close to solar maximum. This revised version was published online in August 2006 with corrections to the Cover Date.     

试建立基于检测振动加速度信号的设备故障部位诊断模型

往复式压缩机、内燃机等复杂设备,一旦出现故障,诊断的首要任务是要判断它们的故障部位。以检测振动加速度信号取代传统的耳听手摸的经验方法是这类设备诊断的一个趋势。尝试着提出了基于检测振动加速度信号的设备故障部位诊断模型--单特征模型和多特征集成模型。通过在往复式压缩机和内燃机上的实例验证表明,提出的单特征模型和多特征集成模型具有一定的可行性,其中多特征集成模型比单特征模型更有效。     

The Freja wave and plasma density experiment

The Wave Experiment, F4, on the Swedish/German satelliteFreja, is designed to measure the electric wave fields up to 4 MHz, the magnetic wave fields up to 16 kHz and the plasma density and its relative variations up to 2 kHz. Six wave signals and four density probe signals can be measured simultaneously. The wave forms of all signals are transmitted to ground without any analysis onboard. The limited TM allocation does not allow continuous sampling of the wave signals, so normally the measurements are made in snapshots of various lengths dependent on sampling frequency, etc. Continuous sampling can be made for shorter time periods by using a 6 Mbyte memory as a buffer.     

Summary of quantitative interpretation of IMAGE far ultraviolet auroral data

Direct imaging of the magnetosphere by instruments on the IMAGE spacecraft is supplemented by simultaneous observations of the global aurora in three far ultraviolet (FUV) wavelength bands. The purpose of the multi-wavelength imaging is to study the global auroral particle and energy input from the magnetosphere into the atmosphere. This paper describes the method for quantitative interpretation of FUV measurements. The Wide-Band Imaging Camera (WIC) provides broad band ultraviolet images of the aurora with maximum spatial resolution by imaging the nitrogen lines and bands between 140 and 180 nm wavelength. The Spectrographic Imager (SI), a dual wavelength monochromatic instrument, images both Doppler-shifted Lyman-α emissions produced by precipitating protons, in the SI-12 channel and OI 135.6 nm emissions in the SI-13 channel. From the SI-12 Doppler shifted Lyman-α images it is possible to obtain the precipitating proton flux provided assumptions are made regarding the mean energy of the protons. Knowledge of the proton (flux and energy) component allows the calculation of the contribution produced by protons in the WIC and SI-13 instruments. Comparison of the corrected WIC and SI-13 signals provides a measure of the electron mean energy, which can then be used to determine the electron energy flux. To accomplish this, reliable emission modeling and instrument calibrations are required. In-flight calibration using early-type stars was used to validate the pre-flight laboratory calibrations and determine long-term trends in sensitivity. In general, very reasonable agreement is found between in-situ measurements and remote quantitative determinations.     

电弧加热器驻点烧蚀/侵蚀试验技术

介绍了在电弧加热器试验设备上进行复合材料烧蚀/侵蚀试验技术,通过改进电弧加热试验设备和粒子播发系统,将石墨粒子均匀注入到高压混合室中,与高温空气混合后经过超声速粒子加速喷管形成烧蚀/侵蚀试验流场,对驻点模型进行试验,同时建立了相应流场参数的测试、计算方法。并对C/C和含钨C/C防热复合材料的抗粒子侵蚀性能进行了初步研究。结果显示有粒子流场的均匀性和重复性较好,能满足材料的烧蚀/侵蚀考核试验要求,且含钨C/C材料的抗粒子侵蚀性能高于C/C材料。     

航天器管路数字化制造技术与实践

文章介绍了航天器管路实现全过程数字化制造的解决方案,对管路坐标转换及数据提取、数控弯管及回弹补偿的仿真、装配仿真和管路快速检测等关键技术进行了分析,并提出了具体的解决方案。结合航天器管路研制需求,将管路数字化制造技术应用于实践,实现了管路生产不再依赖安装现场取样,航天器管路生产与总装分离,管路以产品化形式交付。     

空间碎片失效概率分析软件标准的校验

空间碎片失效概率分析软件是“空间碎片防护设计软件包”的重要组成部分。文章简单介绍了失效概率分析软件的组成结构,并根据国际标准对失效概率分析软件进行详细校验。     

INTESPACE试验中心为阿里安娜-V型火箭而进行的改造

文章介绍了法国宇航环境工程试验中心(INTESPACE)为满足阿里安娜-V的需要所准备进行的一系列改造.这些工作主要有:增建一个适合大型容器用的空气锁,保持厅内连续的10万级洁净度,建立一个紧凑试验区域,建造一面强效吸波墙,扩展振动设备能力以及改造原热真空设备.这些工作计划于2001年初全部完成.改造工作的完成将保证INTESPACE在独立的欧洲试验中心中继续处于领先地位.     

一种FMCWSAR成像的副瓣抑制方法

调频连续波合成孔径雷达（FMCwSAR）是一种新近提出来的成像雷达体制,它结合调频连续波与合成孔径成像技术,具有体积小、质量轻、成本低、分辨率高等一系列优点。在FMCWSAR成像中,由于副瓣可形成倍增的噪声,并与附近散射体产生干涉,因此,系统响应具有低副瓣是非常重要的。研究了泰勒加权对副瓣的抑制能力,并与其他加权方法进行了比较,之后给出仿真结果,证明了该方法能有效抑制FMCWSAR成像的副瓣。