窄分布纳米级HMX的制备及粒度分析

通过撞击法成功地制备了窄分布的纳米级HMX。实验结果表明，分散剂1和分散剂2能改善HMX的粒度分布。在分散剂1存在的条件下，用撞击法可制备出粒度分布较窄的纳米HMX颗粒，其d50分别为70．1nm和68．9nm，分布范围分别为0．9nm和1．4nm。     

The Role of Magnetic Reconnection in CME Acceleration

Observations carried out from the coronagraphs on board space missions (LASCO/SOHO, Solar Maximum and Skylab) and ground-based facilities (HAO/Mauna Loa Observatory) show that coronal mass ejections (CMEs) can be classified into two classes based on their kinematics evolution. These two classes of CMEs are so-called fast and slow CMEs. The fast CME starts with a high initial speed that remains more or less constant; it is also called the constant-speed CME. On the other hand, the slow CME starts with a low initial speed, but shows a gradual acceleration; it is also called the accelerated and slow CME. Low and Zhang [Astrophys. J. 564, L53–L56, 2002] suggested that these two classes of CMEs could be a result of a difference in the initial topology of the magnetic fields associated with the underlying quiescent prominences. A normal prominence magnetic field topology will lead to a fast CME, while an inverse quiescent prominence results in a slow CME, because of the nature of the magnetic reconnection processes. In a recent study given by Wu et al. [Solar Phys. 225, 157–175, 2004], it was shown that an inverse quiescent prominence magnetic topology also could produce a fast CME. In this study, we perform a numerical MHD simulation for CMEs occurring in both normal and inverse quiescent prominence magnetic topology. This study demonstrates three major physical processes responsible for destabilization of these two types of prominence magnetic field topologies that can launch CMEs. These three initiation processes are identical to those used by Wu et al. [Solar Phys. 225, 157–175, 2004]. The simulations show that both fast and slow CMEs can be initiated from these two different types of magnetic topologies. However, the normal quiescent prominence magnetic topology does show the possibility for launching a reconnection island (or secondary O-line) that might be thought of as a “CME’’.     

200km/h动力分散型电动旅客列车组车体表面压力分布试验研究

阐述了对我国首列200km/h动力分散型电动旅客列车组(先锋号列车)车体表面压力分布测试情况,对测量结果进行了较为详细的分析,最后用流场计算软件CFX对先锋号列车周围流场进行了数值模拟计算,并将计算结果与测量结果进行了对比,两者有较好的一致性。该研究结果可为空调装置及电器设备冷却风道进排风口位置的选取提供科学依据。     

Evolution of binaries with chemically peculiar primaries

The chemically peculiar (CP) stars are classified into subgroups based on the type of peculiarities. A significant fraction of these are known to be binaries. The faster evolution of the massive component leads to a white dwarf or a neutron star. Further evolution of the binary is analysed taking into consideration, the orbital parameters, effect of magnetic field, spectroscopic peculiarities and finally the statistics of CP binaries and Low Mass X-ray Binaries (LMXB).

The possible consequences of the evolution to lead to the formation of Magnetic Cataclysmic Variables (MCV) and LMXB are discussed.     

Orbital evolution studies of two HMXB pulsars

High mass X-ray binary (HMXB) pulsars are of two types, persistent and transient. 4U1538−52 is a persistent HMXB whose orbit was previously measured to be circular but the RXTE observations revealed an eccentric orbit. We observed this system with RXTE-PCA in August 2003 and our timing analysis supports the eccentric orbit of the system. However, we do not find any evidence for orbital evolution.

Rotational and tidal interactions between the stars of a closed binary system result in apsidal motion which can be measured in systems with eccentric orbit. 4U0115+63 is a Be-transient HMXB whose eccentric orbit was well-determined during its 1978 outburst. We report preliminary results from analysis of data obtained during the 1999 outburst of this source with the RXTE-PCA.     

正态-复合非时齐Poisson过程模型结构可靠性当量正态设计

讨论强度R～N（μ_R，_R），应力｛S（t），t∈［0，T］｝为非时齐Poisson过程模型结构可靠性当量正态设计。获得应力在设计基准期［0，T］内的最大值概率分布及统计参数估计；正态－复合非时齐Poisson过程模型结构可靠度及结构可靠性当量正态设计表达式。     

Properties of Interplanetary Coronal Mass Ejections

Interplanetary coronal mass ejections (ICMEs) originating from closed field regions on the Sun are the most energetic phenomenon in the heliosphere. They cause intense geomagnetic storms and drive fast mode shocks that accelerate charged particles. ICMEs are the interplanetary manifestations of CMEs typically remote-sensed by coronagraphs. This paper summarizes the observational properties of ICMEs with reference to the ordinary solar wind and the progenitor CMEs.     

侧链基团和填料对硅橡胶材料耐烧蚀性能的影响

为了研究侧链基团和填料对硅橡胶材料耐烧蚀性能的影响,选用具有苯环和多面体低聚倍半硅氧烷(POSS)这2种侧链基团的硅橡胶基体,以及Mg(OH)2、蒙脱石、Fe2O3和短切碳纤维(1 mm)这4种填料,利用马弗炉等温烧蚀和动态热失重TG法研究不同侧链基团和填料样品的耐烧蚀机制。结果表明:苯环和POSS基团的引入使得基体初始分解温度分别提高了79 ºC和9 ºC,质量损失率分别降低了19.4%和12.0%。以Mg(OH)2 25 g(每100 g硅橡胶)、蒙脱石4 g和Fe2O3 6 g作为硅橡胶复合材料进行填料时,其质量烧蚀率为0.008 g/s,相比纯橡胶基体降低了86.8%。在以上配方中继续引入5 g碳纤维,使其质量烧蚀率降低至0.004 g/s。残炭层的微观形貌显示,短切碳纤维形成的三维骨架结构是提高硅橡胶材料耐烧蚀性能的关键。     

综合运输中理想运力分配模型

本文对综合运输中各种运输方式的理想运力进行了理论上的探讨,希望能引起交通运输的主管部门的重视,并在实践中积极地实践,从而来检验理论的正确性.     

调控收入差别,缩小收入差距

全面建设小康社会是党的十六大确立的奋斗目标.全面建设小康社会要求我们重视收入分配,当前收入分配的改革重点应放在缩小收入差距上,通过收入分配的市场公平和社会公平来促进全面建设小康社会.