Initial results from the ISEE-1 and -2 plasma wave investigation

In this paper we present an initial survey of results from the plasma wave experiments on the ISEE-1 and -2 spacecraft which are in nearly identical orbits passing through the Earth's magnetosphere at radial distances out to about 22.5R_e. Essentially every crossing of the Earth's bow shock can be associated with an intense burst of electrostatic and whistler-mode turbulence at the shock, with substantial wave intensities in both the upstream and downstream regions. Usually the electric and magnetic field spectrum at the shock are quite similar for both spacecraft, although small differences in the detailed structure are sometimes apparent upstream and downstream of the shock, probably due to changes in the motion of the shock or propagation effects. Upstream of the shock emissions are often observed at both the fundamental, f_-^p, and second harmonic, 2f_p^-, of the electron plasma frequency. In the magnetosphere high resolution spectrograms of the electric field show an extremely complex distribution of plasma and radio emissions, with numerous resonance and cutoff effects. Electron density profiles can be obtained from emissions near the local electron plasma frequency. Comparisons of high resolution spectrograms of whistler-mode emissions such as chorus detected by the two spacecraft usually show a good overall similarity but marked differences in detailed structure on time scales less than one minute. Other types of locally generated waves, such as the (n+1/2)f_-^gelectron cyclotron waves, show a better correspondence between the two spacecraft. High resolution spectrograms of kilometric radio emissions are also presented which show an extremely complex frequency-time structure with many closely spaced narrow-band emissions.     

Spatial distribution and orbital properties of interplanetary dust at high latitudes

Although the interplanetary dust cloud is assumed to be mainly concentrated in the ecliptic plane, there is a component of dust particles on highly inclined orbits that forms the out-of-ecliptic distribution. The ULYSSES mission for the first time makes this component accessible to in-situ, detection. Evidence for this dust component is also provided from the analysis of the Zodiacal light brightness and especially from the spherical shape of the solar F — corona. An obvious source for an out-of-ecliptic dust population is the activity of comets on high eccentric, highly inclined orbits. We discuss the dynamical conditions of particles under the influence of the radiation pressure when released from the comet and discuss their input to the dust cloud based on brightness analysis and in-situ results.     

飞翼布局飞机起降阶段纵向大迎角气动增稳研究

针对某中等展弦比高速飞翼布局飞机,利用CFD计算方法,研究了一套新型舵面组合对飞机起降任务阶段纵向气动力特性的影响,并对该飞翼布局飞机不同舵面组合进行了数值模拟.仿真结果表明,采用该舵面组合在飞机的起降阶段可以有效改善其纵向气动力特性和操稳特性.     

巨磁电阻材料(La1-xGdx)2/3Ca1/3MnO3的制备工艺及其结构研究

采用固相反应法制备巨磁电阻材料(La1-xGdx)2/3Ca1/3MnO3和La1-xZnxMnO3.La2/3Ca1/3MnO3样品在1200～1400 ℃等五个不同温度下烧结12h;(La1-xGdx)2/3Ca1/3MnO3(x=0.2,0.4,0.6,0.8,1.0)样品系列在1350℃下分别烧结12h和24h,另外样品La1-xZnxMnO3(x=0.1,0.5,0.9)系列在1350℃下烧结24h.利用X射线衍射(XRD)和扫描电镜(SEM)对各样品晶体结构和表面微观结构进行了研究.X射线衍射结果表明,所有样品晶体结构基本不变,保持钙钛矿结构(空间群为Pnma),但随着掺杂量的增加,样品(La1-xGdx)2/3Ca1/3MnO3和La1-xZnxMnO3系列的晶格常数和晶胞体积发生了变化,并且产生了杂质相,导致对结构很敏感的这些材料的磁电性能发生变化.扫描电镜结果表明,样品La2/3Ca1/3MnO3在1400℃时烧结效果最好.     

Latitude-associated differences in the Low Energy Charged Particle activity at Voyagers 1 and 2 during 1991 to early 1994

The Low Energy Charged Particle (LECP) instruments on Voyagers 1 (V1) and 2 (V2) measure the differential in energy fluxes and anisotropies of low energy ions30 keV and electrons20 keV differential in energy ion composition200 keV/nuc, and the integral rates of cosmic ray protons>70 MeV (Krimigiset al., 1977). We discuss shock-accelerated ions and latitude-associated differences between V1 and V2 during 1991 to April 1994.     

热处理制度对1Cr16CO5Ni2Mo1WVNbN钢组织和性能的影响

通过试验研究了不同热处理制度对1Cr16CO5Ni2Mo1WVNbN钢的金相组织、室温拉伸、冲击性能的影响。得出结论：随淬火温度升高,回火温度降低,合金的室温冲击韧性降低,而室温拉伸强度略有升高;淬火介质对室温力学性能以及金相显微组织的影响不明显;淬火保温时间和回火保温时间对合金的室温冲击韧性和室温拉伸性能影响不大。因此合金的最佳热处理工艺参数为：1100oC×90min,油冷＋680℃×3h,空冷。     

CFM56-5B发动机修后过早出现燃烧室和一级低压涡轮导向器损伤分析

发动机热端部件的损伤易造成提前下发、增加维护成本、诱发不安全事件,本文针对CFM56-5B发动机修后过早出现燃烧室和一级低压涡轮导向器损伤的现象进行了调查分析,并提出相应的工程解决方案和应对维护措施。