UVCS/SOHO Observations of H I Lyman Alpha Line Profiles in Coronal Holes at Heliocentric Heights Above 3.0 R⊙

The Ultraviolet Coronagraph Spectrometer (UVCS) on the Solar and Heliospheric Observatory (SOHO) has been used to measure spectral line profiles for H I Lyα in the south polar coronal hole at projected heliocentric heights from 3.5 to 6.0 R_⊙ during 1998 January 5–11. Observations from 1.5 to 2.5 R_⊙ were made for comparison. The H I Lyα profile is the only one observable with UVCS above 3.5 R_⊙ in coronal holes. Within this region the outflowing coronal plasma becomes nearly collisionless and the ionization balance is believed to become frozen. In this paper, the 1/e half widths of the coronal velocity distributions are provided for the observed heights. The velocity distributions include all motions contributing to the velocities along the line of sight (LOS). The observations have been corrected for instrumental effects and interplanetary H I Lyα. The half widths were found to increase with projected heliographic height from 1.5 to 2.5 R_⊙ and decrease with height from 3.5 to 5 R_⊙. This revised version was published online in June 2006 with corrections to the Cover Date.     

Crab脉冲星标准脉冲轮廓更新对计时精度的改进

对于脉冲星试验01星的两年实测数据，针对蟹状星云脉冲星星历经历了多次更新的特点，提出了更新标准脉冲轮廓进行X射线计时的改进方法。以一系列观测时长为实测数据分组，再采用改进后的方法进行计时分析并与改进前的结果进行对比。通过对比改进前后的计时结果，发现改进方法得到的计时残差的均方根(root mean square, RMS)平均降低了14.2%，定位精度平均提高了14.4%，估计原子钟相对频率偏差的精度平均提高了26.2%，体现了改进方法处理经历多次星历更新的Crab脉冲星观测数据的合理性和优越性。此外，改进方法对脉冲星试验01星两年观测数据的稳定度σz没有量级上的改进，说明改进方法对Crab脉冲星时间稳定度的影响不大。     

Be／X射线双星LSI＋61°303的光谱研究

给出了１９９２－１９９５年Ｂｅ／Ｘ射线双星ＬＳＩ＋６１°３０３每年的光谱观测结果，分析了光谱发射线轮廓及其变化，观测显示Ｈβ发射线轮廓具有典型的气壳吸收，表明观测视线与Ｂｅ星赤道平面平行，同时发现Ｈα发射线参数发等值宽度和双峰强度之比也具有类似射电流量的周期性变化，但其变化与射电玫光学光度的变化不同，因此认为此变化可能与中子星周期的吸积盘及其轨道交食有关。     

潜入喷管背壁区熔渣溢流沉积实验研究

利用X射线诊断系统，观察了固体火箭发动机热试车条件下潜入喷管壁区熔渣粒子的溢流过程。得到了实验条件下的潜入喷管背壁区熔渣生成沉积数据和图像，分析探讨了喷管潜入深度、喷管部面积对背壁熔渣生成和溢流过程的影响，为发动机的设计提供了实验依据。     

显微拉曼光谱在物品鉴别上的应用

根据拉曼散射的基本原理 ,利用拉曼光谱仪 ,可以对物质进行简单而科学的分析。显微拉曼分析技术的发展为鉴别某些物品的真伪提供了一种新的手段。文章介绍了一些茶饮料和水晶饰品的显微拉曼鉴别实例。     

Imaging diagnostics of solar non-thermal particles

Non-thermal hard X-ray, gamma-ray and radio emission are the most direct signatures of the presence of energetic particles in the solar atmosphere. This paper lays emphasis on hard X-ray and radio imaging data, obtained during and outside flares, which reveal the sites where particles interact with the ambient medium. These observations, which provide more or less direct information on the topology and dynamics of the magnetic structures in which particles are accelerated and propagate, are discussed in the framework of the statistical flare scenario.     

Optical and X-ray aspects of quasars

We review the present knowledge on the cosmological evolution of quasars, by discussing some of the recent results obtained from studies of optically selected objects. Despite the fast development of prism survey tecniques, the color selection still appears to be the best tecnique for constructing the complete samples which are necessary for statistical studies. It is shown, however, that even the best available complete samples of quasars selected on the basis of ultraviolet excess (z < 2.2) are not sufficient to univocally determine the “correct” evolutionary model. Moreover, some preliminary results suggest that the evolution law derived from quasars with m_B<20 and z<2.2 can not be extrapolated to fainter magnitudes and higher redshifts. On the basis of what is known today about the optical and X-ray properties of quasars, we then discuss some of teh possible results, relevant to cosmology, which can be achieved with future coordinated optical and X-ray observations of quasars.     

304奥氏体不锈钢喷丸引起的组织转变和两相残余应力测定

采用X射线衍射技术研究了304奥氏体不锈钢喷丸过程所引起的组织结构变化以及两相组织中每相的残余应力。试验结果表明,喷丸强化可使亚稳态304奥氏体材料表面发生γ→α转变,在相同的喷丸强度下转变量与喷丸弹丸种类规格关系很大,而且与喷丸时间有关;表面两相组织γ和α相各自的残余应力可采用X射线衍射应力仪进行测定,两相的残余应力数值相差很大。     

Zn-5Al-xMn(x=0，0.1，0.2，0.3)合金的铸态组织与耐蚀性能

采用SEM、EDS、电化学测试等方法研究了热浸镀用Zn-5Al-xMn(x=0,0.1,0.2,0.3)合金的铸态组织与耐蚀性能。结果表明:在Zn-5Al合金中加入少量的Mn显著抑制了粗大初生β-Zn相的生成,当Mn含量为0.2%时,初生β-Zn相最少,共晶组织占比最高。试验合金的自腐蚀电位随着Mn含量的提高而增大,自腐蚀电流密度先减小后增大。Zn-5Al-0.2Mn合金自腐蚀电流最小为1.403μA/cm~2,其高频阻抗和低频扩散阻抗均最大。Zn-5Al合金中初生β-Zn相优先腐蚀,Zn-5Al-0.2Mn合金因初生β-Zn相较少,发生均匀性腐蚀,其腐蚀产物在Zn-5Al-xMn合金中最致密。