一种简易的曲面隐藏线消去法

本文介绍一种简易的曲面隐藏线消去法。先将曲面上各网点分成可见与不可见两类,然后根据线与线相关性,判断各网格线段的可见性,最后只显示或绘制所有的可见网格线段,得到消隐后的曲面立体图形,本法比较简易,调用方便,通用性较强,不管曲面是根据什么方法构作的,只要顺序输入两个方向的网点数及所有网点的坐标值,调用本子程序,一般均能进行曲面消隐。     

Numerical Simulations of the Warm-Hot Intergalactic Medium

In this paper we review the current predictions of numerical simulations for the origin and observability of the warm hot intergalactic medium (WHIM), the diffuse gas that contains up to 50 per cent of the baryons at z∼0. During structure formation, gravitational accretion shocks emerging from collapsing regions gradually heat the intergalactic medium (IGM) to temperatures in the range T∼10⁵–10⁷ K. The WHIM is predicted to radiate most of its energy in the ultraviolet (UV) and X-ray bands and to contribute a significant fraction of the soft X-ray background emission. While O vi and C iv absorption systems arising in the cooler fraction of the WHIM with T∼10⁵–10^5.5 K are seen in FUSE and Hubble Space Telescope observations, models agree that current X-ray telescopes such as Chandra and XMM-Newton do not have enough sensitivity to detect the hotter WHIM. However, future missions such as Constellation-X and XEUS might be able to detect both emission lines and absorption systems from highly ionised atoms such as O vii, O viii and Fe xvii.     

CBERS-02星红外数据系统正反扫描行配准方法研究

CBERS-02星搭载的有效载荷有一台是红外多光谱扫描仪(IRMSS),它是摆扫式的相机,与推扫式的CCD相机成像方式不同。摆扫式IRMSS相机的几何校正处理对比推扫式相机更为复杂,特别是正反扫描行之间,容易出现不配准、有缝隙或叠加等问题。文章根据IRMSS成像的机理,对CBERS-02星IRMSS图像存在的扫描行不配准问题进行了改进,达到了良好的效果。     

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.     

Semi-analytic Solution of Steady Temperature Fields During Thin Plate Welding

Usually, it is very difficult to find out an analytical solution to thermal conduction problems during high temperature welding. Therefore, as an important numerical approach, the method of lines (MOLs) is introduced to solve the temperature field characterized by high gradients. The basic idea of the method is to semi-discretize the governing equation of the problem into a system of ordinary dif-ferential equations (ODEs) defined on discrete lines by means of the finite difference method, by which the thermal boundary condition with high gradients are directly embodied in formulation. Thus the temperature field can be obtained by solving the ODEs. As a numeri-cal example, the variation of an axisymmetrical temperature field along the plate thickness can be obtained.     

Observation of Transition Region Fine Structures with Soho/Sumer

We present a preliminary analysis of two quiet Sun transition region areas observed with the SOHO/SUMER spectrometer, using lines from oxygen, nitrogen and silicon. The average quiet Sun physical parameters are studied as a function of line intensity. Systematic variations of line position and width with increasing intensity are found. A large number of small-scale active points have been observed, and preliminary analysis of the physical properties and dynamics of these active features is presented. A jet-like structure, found in an active point, is also investigated and its velocity along the line of sight determined. This revised version was published online in June 2006 with corrections to the Cover Date.     

分散剂对玻璃纤维浆料分散性的影响

研究了切棉方式、玻璃纤维长度、分散剂种类和含量对玻璃纤维浆料分散性的影响。结果表明:切

棉后的浆料分散程度明显高于未切棉的;浆料中所含纤维成团所占面积百分数由72.6%降到2.4%。长方形棉块

经打浆后形成的浆料纤维较正方形的更为分散。玻璃纤维越长则越难分散,适宜的纤维分散长度为10 ~12 mm。

浆料所含纤维为0.2wt%时,羟乙基纤维素、羟丙基甲基纤维素、六偏磷酸钠的最佳加入量分别为0． 008wt%、0.

012wt%和0.04wt%,所对应的浆料吸光度分别为0.344、0.703 和0.663 A。沉降实验显示添加六偏磷酸钠的浆料

分散性最好,浆料沉降高度最低、沉降速率最慢,羟丙基甲基纤维素次之,羟乙基纤维素最差。

     

某小型离心压气机气动设计

针对无人机动力装置的需求,为某小推力的涡轮喷气发动机进行了单级离心压气机的气动设计.所用的压气机设计方法为:从一维的热力计算出发来进行流道结构设计,以二维通流计算为基础,通过调整各排叶片的环量分布,来获得所要求的气动性能,并通过叶片任意造型最终生成与通流计算结果较为一致的三维叶型,最后通过三维计算流体动力学(CFD)计算来分析气动设计的性能结果.最终设计出的离心压气机在设计点的各项性能参数均达到了设计要求,并且在各个转速下压气机的特性线比较平缓,压气机有较为宽广的稳定工作范围.