Ion Temperatures as Observed in a Solar Coronal Hole

From the widths of the extreme ultraviolet (EUV) lines measured by the SUMER instrument on SOHO, it was found previously (Tu et al. 1998) that the average temperature of Ne⁺⁷, at heights (relative to h₀) above the southern solar limb from 17″ to 64″, ranges between 1.3 and 5 × 10⁶ K and of Ne⁺⁶ between 1 and 4 × 10⁶ K. For mass-per-charge numbers greater than 4 the temperatures of the ions increase slightly with increasing mass-per-charge, while the thermal speed reveals no clear trend. We present a new data set with exposure times much longer than the ones in the previous study. The results obtained from line width analysis of Fe XII (1242 Å), Mg X (1249 Å), Mg VIII (772 Å) Ne VIII (770 Å), and Si VIII (1445 Å) support our previous study. In this case, the trend of increasing temperature begins at a mass-per-charge number of 3. A qualitative explanation based on ion-cyclotron-resonance heating within linear kinetic theory is suggested.     

一种IC测试系统的可靠性分析与改进设计

美国ＧＲ系列ＩＣ测试系统采用磁带机作为系统程序的输入设备,由于磁带机故障率较高,因此使用中经常发生程序输入失败的现象,严重影响了该测试系统的可靠性,本文在对ＧＲ１７３２Ｍ型测试系统的组成结构进入深入分析的基础上,应用在线仿真器对主处理器进行实时仿真,跟踪了引导程序的执行流程和系统磁带的输入过程,提出了用ＰＣ微机代替磁带机,通过ＲＳ－２３２串行接口传送所有软件,本文详细阐述了改进设计方法,改进成功后     

High energy cosmic-ray nuclei results on Ulysses: 2. Effects of a recurrent high-speed stream from the southern polar coronal hole

Since June 1992 the Kiel Electron Telescope on board ULYSSES measures 26-day variations of the order of 6% in the fluxes of high energy H and He. In May 1993 ULYSSES entered into the unipolar region of the southern polar coronal hole, but continued to observe similar effects: increases in the MeV proton channels due to acceleration near the shocks of the corotating interaction region and decreases in the intensity of galactic nuclei associated with the same region. Amplitude variations are presented for different magnetic rigidities and the effects are discussed in view of corotating shock development in a 3-dimensional heliospheric structure.     

轴流压气机进口小总压径向畸变对失速颤振的影响

对进口流场畸变失速颤振的影响进行了实验研究。实验结果表明:小的叶尖径向畸变能抑制颤振的发作。对此现象用三维变形激盘法进行了计算。计算结果与实验符合。      

新型筛选教练机发展趋势

阐述了我国发展新型筛选教练机的必要性;对国内外筛选训练概况进行了跟踪,总结了目前国内外主要的几型筛选教练机性能特点,在此基础上对筛选教练机的发展趋势进行了分析与预测;结合发展趋势,总结了新型筛选教练机的特点,从而提出了发展新型筛选教练机发展思路.     

不同力学边界下梯度功能材料板稳态热应力

用有限元法研究了由ZrO2和Ti-6Al-4V组成的梯度功能材料板的稳态热应力问题，检验了研究方法的正确性，给出了不同力学边界条件下该材料板的稳态热应力场分布。结果表明：无限自由长板内的热应力最小；当无限长板只能伸长、不能弯曲时，板内稳态拉应力最大，比无限自由长板时板内最大拉应力增大6．1倍；当无限长板的伸长、弯曲受限时，板内的压应力最大，比无限自由长板时板内最大压应力增大12．0倍；此外，材料组分形状分布系数M、对流换热系数、环境介质温度和孔隙度的变化对不同力学边界条件下该材料板稳态热应力场的影响显著。此结果为该材料的设计和应用提供了准确的理论计算依据。     

航空电子WDM光网络可靠性建模

为了构建先进综合化航空电子系统的统一网络,提出了基于WDM （Wave-length Division Multiplexing）光网络的航电骨干网与外接边缘网互连方式的航电统一网络,并采用多跳ShuffleNet网络作为航电光骨干网的模型.针对综合化航电网络的可靠性问题,建立了基于航电任务与任务路径的可靠性建模方法,给出了保证任务执行成功的可靠度计算公式.以ShuffleNet航电光骨干网作为建模实例,通过对航电任务可靠度的分析计算,得到了系统任务的执行时间、网络规模、任务路径的跳数对系统可靠度影响最大,而同等条件下光纤链路的复用波长数对任务可靠度影响不明显的结论.仿真结果显示,基于任务的可靠性建模与计算方法可以为航电系统的可靠性分析提供理论基础.     

低速翼型近场尾流及其后缘边界层流动特性之热线测量结果

本文对低速翼型近场尾流及其后缘边界层流动中的有关参数(如平均流速(?),雷诺应力(?))的测量方法,实验设备,实验结果分析等作了简要叙述。对测量中需严格控制的有关问题也进行了讨论。实验结果表明本文采用的测量方法是可行的。     

Augmented Empirical Models of Plasmaspheric Density and Electric Field Using IMAGE and CLUSTER Data

Empirical models for the plasma densities in the inner magnetosphere, including plasmasphere and polar magnetosphere, have been in the past derived from in situ measurements. Such empirical models, however, are still in their initial phase compared to magnetospheric magnetic field models. Recent studies using data from CRRES, Polar, and Image have significantly improved empirical models for inner-magnetospheric plasma and mass densities. Comprehensive electric field models in the magnetosphere have been developed using radar and in situ observations at low altitude orbits. To use these models at high altitudes one needs to rely strongly on the assumption of equipotential magnetic field lines. Direct measurements of the electric field by the Cluster mission have been used to derive an equatorial electric field model in which reliance on the equipotential assumption is less. In this paper we review the recent progress in developing empirical models of plasma densities and electric fields in the inner magnetosphere with emphasis on the achievements from the Image and Cluster missions. Recent results from other satellites are also discussed when they are relevant.     

新型整星隔振平台的被动隔振性能及星箭耦合特性分析

针对卫星的隔振要求,提出一种新型半主动整星隔振平台,采用磁流变(MR)阻尼器作为半主动作动器。为增加平台的横向转动刚度,提出一种套筒式防摇结构。建立新型整星隔振系统的详细有限元(FE)模型,对隔振系统进行基础随机激励下的响应分析和隔振平台的振级落差分析,并建立星箭系统的详细有限元模型,分析星箭结合后对整星隔振性能的影响情况,以及加入新型隔振平台后对火箭动态特性的影响。结果表明:新型整星隔振平台具有优良的被动隔振性能;火箭的动态特性对新型隔振系统的性能有一定影响,但当火箭和隔振平台结合处的刚度较大时,影响较小;加入新型隔振平台后,在火箭点火时到一级分离时,火箭整体的动态特性无明显变化。