基于i860XP和Transputer的异构型多处理器系统

新出现的RISC微处理器提供了超计算能力，采用i860XP超标量微处理器来增强已存在的Transputer系统的性能是一种切实可行的办法，它们构造了一种异构型多处理器系统。本文给出了该系统的设计和性能分析。     

On mid-term periodicities of high-latitude solar activity

The mid-term periodicities of polar faculae are studied separately for the total disk, northern and southern hemispheres of the Sun for a time interval from 1951 August to 1998 December. Apart from the 11-year Schwabe cycle which is the fundamental period and is found in all of the three time series, the following prominent results are found: (1) the rotational periodicity of solar activity at high latitudes is approximately from 28 to 32 days; (2) a large number of quasi-periods appearing in low-latitude solar activity (annual variation, 1.3–1.7 years, quasi-biennial oscillation, and 4–5 years) also exist in polar faculae; (3) the periodicities on both hemispheres are not identical.     

Model of a fluxtube with a twisted magnetic field in the stratified solar atmosphere

We build a single vertical straight magnetic fluxtube spanning the solar photosphere and the transition region which does not expand with height. We assume that the fluxtube containing twisted magnetic fields is in magnetohydrostatic equilibrium within a realistic stratified atmosphere subject to solar gravity. Incorporating specific forms of current density and gas pressure in the Grad–Shafranov equation, we solve the magnetic flux function, and find it to be separable with a Coulomb wave function in radial direction while the vertical part of the solution decreases exponentially. We employ improved fluxtube boundary conditions and take a realistic ambient external pressure for the photosphere to transition region, to derive a family of solutions for reasonable values of the fluxtube radius and magnetic field strength at the base of the axis that are the free parameters in our model. We find that our model estimates are consistent with the magnetic field strength and the radii of Magnetic bright points (MBPs) as estimated from observations. We also derive thermodynamic quantities inside the fluxtube.     

Interstellar scintillation,ISS, and intrinsic variability of radio AGN

We investigate the relationship between the 5 GHz interstellar scintillation (ISS) and the 15 GHz intrinsic variability of the compact, radio-selected active galactic nuclei (AGN) common to the Microarcsecond Scintillation-Induced Variability (MASIV) Survey and the Owens Valley Radio Observatory blazar flux density monitoring program. As part of this investigation, we also re-examine the reported intrinsic nature of the February 1990 VLA observations of the blazar S5 0716+714. We are also examining the presence of IDV/ISS in the Owens Valley 15 GHz flux density monitoring data. We find a significant relationship between the Owens Valley 15 GHz modulation index and the MASIV modulation index. We also discuss the implications of these findings for RadioAstron.     

Interpretation of the SOHO/UVCS observations of two CME-driven shocks

We report on the analysis of two fast CME-driven shocks observed with the UltraViolet Coronagraph Spectrometer (UVCS) on board the Solar and Heliospheric Observatory (SOHO). The first event, detected on 2002 March 22 at 4.1 R_⊙ with the UVCS slit placed in correspondence with the flank of the expanding CME surface, represents the highest UV detection of a shock obtained so far with the UVCS instrument in the corona. The second one, detected on 2002 July 23 at 1.6 R_⊙ with the UVCS slit placed in correspondence with the front of the expanding CME surface, shows an anomalous deficiency of ion heating with respect to what observed in previous CME/shocks observed by UVCS, possibly reflecting the effect of different coronal plasma conditions over the solar cycle. From the two different sets of observations we derived an estimate for the shock compression ratio X, which turns out to be X = 2.4 ± 0.2 and X = 2.2 ± 0.1, respectively, for the first and second event. Comparison between the two events provides complementary perspectives on the dynamical evolution of CME-driven shocks.     

The investigation of powerful solar flares characteristics by analysis of excited states of C and various neutrons capture lines

Accelerated energetic particles in solar flares produced nuclear γ-lines in interactions with ambient solar atmosphere. Analysis of intensity of ratios between various γ-lines allows us to make estimations of abundance of elements, parameters of surrounding media and other solar characteristics. In this article we discuss the flux ratio between two lines from excited states of ¹²C (f_15.11/f_4.44) and our results of preliminary calculation of intensity ratio between two neutron capture lines at ³He and ¹H (f_20.58/f_2.223). In particular we consider the opportunity to obtain n(³He)/n(¹H) ratio during solar flares and using high-energy gamma-emission studying, based on the satellite data. Possible interpretation of spectral features observed during the January 20, 2005 solar flare is discussed. Preliminary analysis of energy spectrum in the band of 2–21 MeV gives n(³He)/n(¹H) ∼ 8 × 10⁻⁴ for January 20, 2005 solar flare.     

Composite profile of the Fe Kα spectral line emitted from a binary system of supermassive black holes

We used a model of a relativistic accretion disk around a supermassive black hole (SMBH), based on ray-tracing method in the Kerr metric, to study the variations of the composite Fe Kα line emitted from two accretion disks around SMBHs in a binary system. We assumed that the orbit of such a binary is approximately Keplerian, and simulated the composite line shapes for different orbital elements, accretion disk parameters and mass ratios of the components. The obtained results show that, if observed in the spectra of some SMBH binaries during their different orbital phases, such composite Fe Kα line profiles could be used to constrain the orbits and several properties of such SMBH binaries.     

民航机场飞机排放浓度分布模型

按照国际民航组织规定的起飞着陆循环过程,简化飞机在机场起飞降落的活动路线,在原有飞机排放污染物排放指数(EI)计算的基础上,再结合飞机起飞降落过程的燃油流量(F),计算出进近、滑行、起飞、爬升四段路线的排放污染强度.基于高斯点源扩散公式,对其进行积分得线源扩散模型,再对线源扩散模型中的参数进行修正,建立了民航机场飞机排放浓度模型.     

静基座捷联惯性组合加速度计高阶误差项显著性分析

在标定捷联惯组加速度计时,一般采用多位置试验,但是目前并未对多位置试验所能标定出的误差系数数量和标定结果的有效性进行分析,本文针对这一问题展开了研究.首先,阐述了带有高次误差项的捷联惯组加速度计误差模型.然后,针对一般6位置标定方法无法完成这一模型标定的缺陷,提出了一种18位置标定方法.进行标定后,运用显著性分析方法,对误差模型本身和其中的参数的有效性进行了分析.最后,通过重复进行去除最不显著项、再标定、显著性检验等步骤,获得了试验室条件下所能标定的捷联惯组加速度计组合误差模型.     

压电智能结构的实验研究

在复合材料表层铺设压电元件，利用压电元件能够实现力学量和电学量之间相互转化的独特性能，可将其用作传感器和驱动器，赋予材料和结构传感及动作的能力。本研究的压电材料采用锆钛酸铅压电陶瓷，基体材料采用玻璃纤维－环氧树脂复合材料，与外部信号采集和控制系统结合，构成了智能结构实验系统。本文对这一系统的损伤诊断和损伤主动控制功能进行了实验研究。该结构一方面可对冲击、过载等可能造成损伤的原因进行监测，并诊断裂缝、连接松动等损伤的产生和位置，另一方面还可自适应地驱动结构中的压电驱动器，改善结构应力状态，防止损伤的扩展。