80.9MeV 16O+27Al能量耗散和核子交换的关系

用带ΔE-E望远镜系统的飞行时间系统测量了80.9MeV ¹⁶O+²⁷Al反应出射产物的三重微分截面d³σ/dA dZ dE.对该反应中所出现的能量耗散和核子交换的关系进行了讨论.     

19F+51V耗散反应同位素类弹碎片的截面涨落

采用飞行时间(TOF)加△E-E探测系统,在102.25-109.50MeV(能量步长为250keV)的¹⁹T+⁵¹V反应中,第一次给出了耗散碰撞同位素产物的激发函数,讨论了双核系统的能量相干宽度Γ与产物的质量数A和Γ与产物的中子过剩自由度N/Z的依赖关系.     

14N+58Ni和14N+64Ni深部非弹性反应产物同位素分布的差异

实验测得¹⁴N(93兆电子伏)+⁵⁸Ni、⁶⁴Ni深部非弹性反应产物同位素分布, 发现这两者存在系统性的差异.     

Neutron Spectroscopic Factors of ^7Li and Astrophysical ^6Li（n,γ）^7Li Reaction Rates

Angular distributions of the ^7Li（^6Li, ^6Li）^7Li elastic scattering and the ^7Li（^6Li, ^7Lig.s.）^6Li, ^7Li（^6Li, ^7Li0.48）^6Li transfer reactions at Ec.m. = 23.7 MeV are measured with the Q3D magnetic spectrograph. The optical potential of ^6Li ＋ ^7Li is obtained by fitting the elastic scattering differential cross sections. Based on the distorted wave Born approximation （DWBA） analysis, spectroscopic factors of ^7Li =^6Li n are determined to be 0.73 ± 0.05 and 0.90 ± 0.09 for the ground and first exited states in ^7Li, respectively. Using the spectroscopic factors, the cross sections of the ^6 Li（n, γ0,1）^7 Li direct neutron capture reactions and the astrophysical ^6Li（n, γ）^7 Li reaction rates are derived.     

北斗B1信号捕获跟踪算法的软件仿真研究

针对北斗B1频率的I支路信号,设计并实现了北斗软件接收机的基带处理部分。阐述了北斗B1频点信号的扩频体制和产生过程,并行码相位搜索捕获策略以及鉴相辅助跟踪环路,并设计了二阶数字环路滤波器,滤波器参数取ζ=0.707,B_n=25(Hz)。同时采用Matlab软件,仿真北斗中频数字信号,编码实现捕获跟踪算法,并分别通过对仿真信号和真实卫星信号的捕获跟踪,验证捕获跟踪算法的可行性,并提出锁频环辅助锁相环算法的改进思路。为进一步开展北斗软件接收机相关技术研究打下了基础。     

基于信噪比测量的欺骗干扰检测方法

在捕获北斗信号的过程中,接收机根据预先设定好的信号搜捕策略和门限值来捕获信号;欺骗干扰源通过产生虚假的相关峰和增加噪声基底,可以有效地干扰普通型北斗接收机正常的捕获工作;针对欺骗信号检测问题,在分析欺骗信号入侵对接收机噪声基底影响的基础上,提出了在捕获阶段利用信噪比(SNR)检测技术识别欺骗干扰信号的方法,并对其有效性进行了分析;仿真结果表明,采用该方法的接收机具有一定程度的欺骗干扰识别能力,为提高GNSS接收机抗干扰能力提供了有益的参考 。     

Impact parameter and beam energy dependence for azimuthal asymmetry of direct photons and free protons in intermediate energy heavy-ion collisions

Hard photon emitted from energetic heavy ion collisions is of very interesting since it does not experience the late-stage nuclear interaction, therefore it is useful to explore the early-stage information of matter phase. In this work, we have calculated the impact parameter and beam energy dependence for azimuthal asymmetry, characterized by directed transverse flow parameter F and elliptic asymmetry coeffcient v2, of direct photons and the corresponding free protons in intermediate energy heavy-ion collisions. It is further shown the anti-correlated azimuthal asymmetry between direct photons and free protons.     

Impact parameter and beam energy dependence for azimuthal asymmetry of direct photons and free protons in intermediate energy heavy-ion collisions

Hard photon emitted from energetic heavy ion collisions is of very interesting since it does not experience the late-stage nuclear interaction, therefore it is useful to explore the early-stage information of matter phase. In this work, we have calculated the impact parameter and beam energy dependence for azimuthal asymmetry, characterized by directed transverse flow parameter F and elliptic asymmetry coefficient v₂, of direct photons and the corresponding free protons in intermediate energy heavy-ion collisions. It is further shown the anti-correlated azimuthal asymmetry between direct photons and free protons.     

二代高温超导带材的机械特性研究进展

以 YBCO(YBa2Cu3 O7 -δ ) 为代表的二代高温超导带材因具有高临界转变温度、 高临界磁场和强载流能力,受到了国际学界高度关注, 在各个领域具有广泛的应用前景. 二代高温超导带材在绕制、 冷却和运行过程中会受到不同来源的外力作用, 且超导带材的韧性、 延展性较差, 因此其机械性能是影响安全性与设备运行可靠性的关键.本文基于二代超导带材各向异性的特点, 对超导带材轴向、 横向、 弯曲三个方向的静态机械性能及疲劳性能进行了介绍. 同时, 也对超导带材各方向机械性能的测试方法、 影响因素及机理进行了总结     

煤直接制甲烷系统的热力学分析

通过Ca基吸收剂的引入,将煤的气化反应、甲烷化反应和CO₂吸收反应集成在同一反应器内,形成煤直接制甲烷系统,可缩短传统煤制甲烷系统流程,提高转化效率。分析了热力学平衡状态下温度、压力、Ca/C比和H₂O/C比对气体产物产量的影响。结果表明降低反应温度和提高反应压力有利于甲烷的产生,而Ca/C比和H₂O/C比的选取存在最优值,得到了煤直接制甲烷体系较为适宜的反应条件为:500～700℃,5～10 MPa,Ca/C=0.5,H₂O/C=1。