Two years of INTEGRAL observation of the BHC IGR J17464-3213

On March 2003, IBIS, the γ-ray imager on board the INTEGRAL satellite, detected an outburst from a new source, IGR J17464-3213, that turned out to be an HEAO-1 transient, namely H1743-322. The spectral and temporal evolutions of the source were observed by INTEGRAL in different periods. Also RXTE observed the source for the first time on 2003 March 29 during a PCA Galactic bulge scan. The source flux decayed below the RXTE PCA sensitivity limit in November 2003, then in April 2004 it was again detected by INTEGRAL. On July 3, 2004 the source was again detected by RXTE/PCA at a 2–10 keV intensity of 16 mCrab and on July 7, reached 69 mCrab. Recently, a new outburst was observed on August 2005. We briefly summarise here the behaviour of the source observed by INTEGRAL from March 2003 to August 2005. The new outbursts of the source and the analysis of all the data collected (now public) give a global view of the spectral and time behaviour of this X-ray transient.     

Time-dependent thermal X-ray afterglows from GRBS

Time-dependent thermal X-ray spectra are calculated from physically plausible conditions around GRB. It is shown that account for time-dependent ionization processes strongly affects the observed spectra of hot rarefied plasma. These calculations may provide an alternative explanation to the observed X-ray lines of early GRBs afterglows (such as GRB 011211). Our technique will allow one to obtain independent constraints on the GRB collimation angle and on the clumpiness of circumstellar matter.     

Broad-band spectral properties of accreting X-ray binary pulsars

Broad-band spectra of accreting X-ray binary pulsars can be fitted by a phenomenological model composed of a power law with a high energy rollover above 10 keV, plus a blackbody component with a temperature of few hundred eV. While, at least qualitatively, the hard tail can be explained in terms of (inverse) Compton scattering, the origin of the soft component cannot find a unique explanation. Recently, a qualitative picture able to explain the overall broad-band spectrum of luminous X-ray pulsars was carried out by taking into account the effect of bulk Comptonization in the accretion column. After a review of these recent theoretical developments, I will present a case study of how different modeling of the continuum affect broad features, in particular the cyclotron resonance features in Vela X-1.     

CBERS-1卫星红外多光谱扫描仪扫描子系统

文章介绍了CBERS -1卫星红外多光谱扫描仪(IRMSS)关键部件扫描子系统研制与应用情况。     

三维图元的设计及其在遥测数据可视化中的应用

设计了接口良好、通用性强、运行速度快、视觉效果良好的三维图形元。以设计某型无人直升机三维图元为例进行了详细测试和实际应用 ,收到了满意效果。     

Sc在L10-TiAl金属间化合物中占位的理论研究

基于密度泛函理论,运用第一原理赝势平面波方法,采用CASTEP量子力学能量软件包研究了Sc占据Ti位与Sc占据A l位的超胞晶格常数、原子形成热、超胞总态密度与电子密度差分图,两种情况对比下,在L10-TiA l合金中,Sc优先占据Ti位,这一结论为进一步研究三元系TiA l-Sc合金提供了理论研究的基础。     

有机高分子絮凝剂处理高浊度原水效果和机理研究

本文研究了有机高分子絮凝剂ＰＡＭ、ＣＴＡＢ及它们的复配ＰＡＭ＋ＣＴＡＢ处理高浊度原水的最佳实验条件、絮凝性能、效果和机理，为有机高分子絮凝剂的选择和管式絮凝器的研制提供了理论依据。     

Cd1-xZnxS体系红外光谱及发射率特性

制备了Cd1-xZnxS三元系半导体材料。利用X射线衍射(XRD)对其结构进行了表征,结果表明实验所得样品均为纤锌矿结构。建立了Cd1-xZnxS混晶替位模型,根据所建模型和晶格振动理论,对Cd1-xZnxS红外光谱特性进行探讨。研究了Cd1-xZnxS三元系半导体材料红外发射率特性,Cd1-xZnxS在3~5μm波段的发射率远远低于8~14μm波段的发射率,这与材料的红外吸收机制和光谱特性有关;Cd1-xZnxS半导体材料的红外发射率随着烧结温度的提高而降低,这是由于温度升高,晶格畸变减小并逐渐趋近于完整晶格。     

高速列车绕流的数值模拟

给出了用低速N－S方程求解高速列车绕流的数值计算方法，采用显隐式结合的方法来加快收敛速度，基于该方法编制了计算软件系统Train3D，用该软件系统对高速列车外形的外流场进行了数值模拟，获得了该外形的空气动力特性和流场结构。     

Re对Ni3Al屈服强度及断裂强度影响的第一原理研究

为了满足航空发动机热端部件材料力学性能的不断提高,应用基于密度泛函理论的第一原理方法,研究了Re对Ni_3Al金属间化合物力学强度的影响。通过建立掺杂Re前后Ni_3Al的滑移模型和断裂模型,计算了晶胞的不稳定堆垛层错能γ_(US)和断裂能γ_C,进而判断Re对Ni_3Al屈服强度和断裂强度的影响。另外根据经验判据,γ_C/γ_(US)值可表征材料的韧脆性。计算结果表明,Re的掺杂增大了Ni_3Al [11■](111)和[1■0](111)两个滑移系下的γ_(US),使得滑移系不易开动,不易使Ni_3Al发生塑性变形,增大了Ni_3Al的屈服强度。Re增大了Ni_3Al在密排面处的断裂能,使得其不易在密排面发生断裂,增大了断裂强度。关于改善Ni_3Al的韧性,Re的掺杂对于密排面上不同滑移方向的影响具有一定的差别。此研究工作可为改善航空发动机单晶叶片的力学性能提供理论基础。