电荷交换离子对栅极系统束流影响的数值研究

采用二维网格质点法(PIC)计算离子在离子发动机栅极系统中的运动, 通过在模型中添加离子和中性粒子电荷交换的Monte Carlo碰撞模块, 得到了电荷交换离子在栅极周围的分布及电荷交换离子的运动规律.计算结果表明:考虑电荷交换离子后, 屏栅极电流较不考虑电荷交换离子情况时增大了1.42%, 所受影响不大, 加速栅极电流由0增大到主束流电流的1.41%.模拟结果表明:加速栅极下游较远处产生的电荷交换离子, 是造成加速栅极下游面腐蚀及加速栅极电流的主要原因.      

重离子在生物组织中的阻止本领

根据中能重离子与靶物质相互作用的特点,将参数化的阻止本领计算方法进行了改进和推广,给出了计算重离子在人体组织及生物等效介质中阻止本领的方法。作为带电离子适形放疗的基础,计算了中能碳离子在肌肉、骨胳、脂肪、水及其他生物等效介质中的阻止本领,Bragg峰、射程等参量,并对计算方法的可靠性及在临床肿瘤治疗剂量控制方面的应用进行了分析。参数化的计算方法能满足实际应用的要求。     

重型运载火箭动力系统分析

讨论了两种载人登月的动力系统方案,分析了已有重型火箭动力系统的结构和基本参数,以满足载人登月的任务要求为前提,提出了重型火箭箭体结构和任务要求.从性能、经济性、技术难度、工作可靠性等方面综合考虑,提出重型火箭下面级的基本方案.提出了一套重型火箭动力系统,建立了一个运载火箭系列,并对其运载能力进行了计算.经综合分析,提出登月火箭可采用8 m直径的三级半结构,助推级、第一级和第二级均为推力5 000 kN量级富氧预燃室补燃循环液氧煤油发动机,第三级为2台50 t氢氧发动机.      

An update about recent developments of the PHITS code

PHITS (Particle and Heavy-Ion Transport code System) is a general-purpose three-dimensional Monte Carlo code, developed and maintained by RIST, JAEA and KEK in Japan together with Sihver et al. at Chalmers in Sweden. PHITS can deal with the transports of all varieties of hadrons and heavy ions with energies up to around 100 GeV/nucleon, and in this paper the current status of PHITS is presented. We introduce a relativistically covariant version of JQMD, called R-JQMD, that features an improved ground state initialization algorithm, and we will present the introduction of electron and photon transport in PHITS using EGS5, which have increased the energy region for the photon and energy transport from up to around 3 GeV to up to several hundred GeV depending on the atomic number of the target. We show how the accuracy in dose and fluence calculations can be improved by using tabulated cross sections. Benchmarking of shielding and irradiation effects of high energy protons in different materials relevant for shielding of accelerator facilities is also presented. In particular, we show that PHITS can be used for estimating the dose received by aircrews and personnel in space. In recent years, many countries have issued regulations or recommendations to set annual dose limitations for aircrews. Since estimation of cosmic-ray spectra in the atmosphere is an essential issue for the evaluation of aviation doses, we have calculated these spectra using PHITS. The accuracy of the atmospheric propagation simulation of cosmic-ray performed by PHITS has been well verified by experimental cosmic-ray spectra taken under various conditions. Based on a comprehensive analysis of the simulation results, an analytical model called “PARMA” has been proposed for instantaneously estimating the atmospheric cosmic-ray spectra below the altitude of 20 km. We have also performed preliminary simulations of long-term dose distribution measurements at the ISS performed with the joint ESA-FSA experiment MATROSHKA-R (MTR-R) led by the Russian Federation Institute of Biomedical Problems (IMBP) and the ESA supported experiment MATROSHKA (MTR), led by the German Aerospace Center (DLR). For the purpose of examining the applicability of PHITS to the shielding design in space, the absorbed doses in a tissue equivalent water phantom inside an imaginary space vessel has been estimated for different shielding materials of different thicknesses. The results confirm previous results which indicate that PHITS is a suitable tool when performing shielding design studies of spacecrafts.     

叶型厚度参数与压气机转子叶片颤振关联性研究

采用计算流体力学与结构动力学相结合的方法,数值模拟了大负荷弯掠扭组合叶片非定常粘性流场;通过对叶片表面非定常气动力及其所做非定常气动功的计算分析,采用能量法对叶片颤振与否进行预估判断。在气动设计满足设计要求的基础上,小范围调整大负荷弯掠扭组合叶片的最大厚度分布和最大厚度相对位置分布,并分别进行颤振预估计算。结果表明,最大厚度分布和最大厚度相对位置分布对颤振影响明显。在最大厚度相对位置分布相同的情况下,均匀减薄叶片,会使一阶动频减小,积累功率增大,颤振发生的可能性增大。研究结果对叶轮机颤振机理研究具有一定的参考意义。     

A census of high-energy observations of Galactic supernova remnants

We present the first public database of high-energy observations of all known Galactic supernova remnants (SNRs). In Section 1 we introduce the rationale for this work motivated primarily by studying particle acceleration in SNRs, and which aims at bridging the already existing census of Galactic SNRs (primarily made at radio wavelengths) with the ever-growing but diverse observations of these objects at high-energies (in the X-ray and γ$\gamma$-ray regimes). In Section 2 we show how users can browse the database using a dedicated web front–end (http://www.physics.umanitoba.ca/snr/SNRcat). In Section 3 we give some basic statistics about the records we have collected so far, which provides a summary of our current view of Galactic SNRs. Finally, in Section 4, we discuss some possible extensions of this work. We believe that this catalogue will be useful to both observers and theorists, and timely with the synergy in radio/high-energy SNR studies as well as the upcoming new high-energy missions. A feedback form provided on the website will allow users to provide comments or input, thus helping us keep the database up-to-date with the latest observations.     

载人火星和小行星探测任务初步分析

载人火星和小行星探测是未来深空探测的重要发展方向,以美国为代表的航天强国正在积极开展相关方案论证和技术攻关。由于任务规模庞大,受制于目前以化学推进为主的运输系统能力限制,要进行火星、小行星探测,必须发展重型运载火箭、轨道转移级等运载工具。从载人火星、小行星探测任务规划的角度出发,对总体任务进行了初步分析,提出了初步的系统方案。     

80C31微处理器单粒子效应敏感性地面试验研究

文章针对不同厂家的80C31微处理器,利用重离子、锎源模拟源进行单粒子效应地面试验研究。详细介绍了80C31微处理器单粒子效应试验原理、试验方法、试验系统的软硬件组成以及试验取得的结论。通过试验研究获得了80C31微处理器单粒子翻转和单粒子锁定特征参数。研究结果可为被测器件在卫星型号的使用提供技术参考依据。     

Radiative transitions in few-electron quasi-molecules

The review is aimed at the discussion of recent results on spectral profiles produced in collisions of few-electron atoms/ions. Calculations of spectral profiles produced by atom/ion collisions need some preliminary quantum-chemical information such as potential energy surfaces, dipole transition moments, etc. The main advantage of few-electron systems is that all input data can be obtained ab initio or analytically, thus the profiles calculated do not include any fit parameters. Two specific examples have been discussed. The first one deals with radiative transitions accompanying charge-exchange in collisions of one-electron ions with bare nuclei. The second example concerns radiative transitions produced by H⁻ + H collisions.     

太阳极区低日冕重离子的回旋波加热机制

采用电子、质子、氦核和另外一种微量离子代替氧离子的4组元模型分别计算了Fe^11 ,Mg^9 ,Mg^7 ,Ne^7 和Si^7 等微量离子的漂移速度和温度，并和SUMER的观测结果进行了比较。