Transient outburst mechanisms in Supergiant Fast X-ray Transients

The recent discovery of a new class of recurrent and fast X-ray transient sources, the Supergiant Fast X-ray Transients, poses interesting questions on the possible mechanisms responsible for their transient X-ray emission. The association with blue supergiants, the spectral properties similar to those of accreting pulsars and the detection, in a few cases, of X-ray pulsations, confirm that these transients are High Mass X-ray Binaries. I review the different mechanisms proposed to explain their transient outbursts and the link to persistent wind accretors. I discuss the different models in light of the new observational results coming from an on-going monitoring campaign of four Supergiant Fast X-ray Transients with Swift.     

利用金刚石微颗粒进行微米级加工的研究

为确立用金刚石微颗粒对硬脆性材料进行微加工的技术基础,在进行了螺旋切入方式的运动学和力学模式的解析后,对用金刚石微颗粒进行磨削微加工的最佳条件进行了探讨。在此基础之上,用电镀有金刚石微颗粒的工具和螺旋切入磨削方式,成功地实现了对玻璃、硅片等各种各样的硬脆性材料的100μm尺度的高精度加工。     

测控资源调度管理系统的构造与实现

针对我国航天测控实际问题的特点和现状,基于知识发现提出了测控资源动态调度算法的框架,在此基础上,基于数据仓库建立了测控资源动态调度管理系统的体系结构,并采用面向对象(Ob ject-O riented,O-O)技术,分析和设计了测控资源动态调度管理系统,最后阐明了该系统的优点。实际应用表明,该方法使我国“一网管多星”的效率得到极大的提高。     

TC4钛合金侧铣加工表面形貌分析及工艺参数优化

TC4钛合金是 1种典型的不易加工材料,其切削加工表面质量很难控制。为实现面向侧铣加工表面形貌的切削工艺参数优选,开展了 TC4钛合金侧铣加工实验研究。首先,探究了加工表面微观缺陷特征及其形成机制;然后,采用粗糙度参数 Ra和 Sa对铣削表面形貌进行定量表征,并分析了切削速度、进给量和切削深度对表面粗糙度参数的影响;最后,基于遗传算法(Genetic Algorithm,GA)对铣削工艺参数进行了优化。研究发现,加工表面微观缺陷主要有进给刀痕等固有缺陷和黏附颗粒等随机缺陷。铣削表面粗糙度随主轴转速的增大先减小后增大;随径向切深的增大先增大后减小;随进给量先增大后减小。在主轴转速 n = 1 093 r/min、径向切深 ae = 0.2 mm、每转进给量 f = 0.06 mm/r的条件下可以获得较小的表面粗糙度。     

球头模具铣刀刀刃和前刀面成形的研究

提出了一种使球头模具铣刀具有良好切削性能,可以大大改善球顶点及其附近处切削条件的刀刃构造形式和前刀面形状;根据包络原理详细分析和研究了成形这种球头铣刀刀刃及前刀面的磨削（或铣削）系统的合理运动方式,并导出了各运动间的函数关系;给出了一计算实例。     

星座通信系统测控模式探讨

立足星座通信系统的测控观点,基于卫星自主管理和采用新的伪码扩频测控体制,探讨简化地面测控管理所必需完成的大量复杂跟踪测量与控制任务的可行性,研究星座通信系统测控管理的操作设想。     

卫星通用测控模拟器设计与实现

介绍了一种适用于不同型号、不同环境的卫星通用测控模拟器的设计实现方法和应用现状及发展前景。该设备在70MHz以下完全采用了数字化处理,可通过连接某一频段内上／下变频器实现射频通用测控模拟器。     

我国航天测控通信系统配置CCSDS SLE业务方案设计

介绍了CCSDS SL正业务的具体内容,提出了在我国航天测控系统中采用CCSDS标准的SLE传输协议实现国际联网的设想,并给出了前向遥控SLE业务的配置方案。     

The Milky Way 3-Helium Abundance

We are making precise determinations of the abundance of the light isotope of helium, ³He. The ³He abundance in Milky Way sources impacts stellar evolution, chemical evolution, and cosmology. The abundance of ³He is derived from measurements of the hyperfine transition of ³He⁺ which has a rest wavelength of 3.46 cm (8.665 GHz). As with all the light elements, the present interstellar ³He abundance results from a combination of Big Bang Nucleosynthesis (BBNS) and stellar nucleosynthesis. We are measuring the ³He abundance in Milky Way H ii regions and planetary nebulae (PNe). The source sample is currently comprised of 60 H ii regions and 12 PNe. H ii regions are examples of zero-age objects that are young relative to the age of the Galaxy. Therefore their abundances chronicle the results of billions of years of Galactic chemical evolution. PNe probe material that has been ejected from low-mass (M≤ 2M _⊙) to intermediate-mass (M∼2–5M _⊙) stars to be further processed by future stellar generations. Because the Milky Way ISM is optically thin at centimeter wavelengths, our source sample probes a larger volume of the Galactic disk than does any other light element tracer of Galactic chemical evolution. The sources in our sample possess a wide range of physical properties (including object type, size, temperature, excitation, etc.). The ³He abundances we derive have led to what has been called “The ³He Problem”.