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21.
后随X射线望远镜(follow-up X-ray telescope, FXT)是爱因斯坦探针卫星的主要载荷之一.为了获取高信噪比的数据,实现对观测天体的高精度定位, FXT使用Wolter-Ⅰ型X射线聚焦光学系统,该系统一直是X射线空间天文观测中的重要设备.根据Wolter-Ⅰ型的聚焦原理,结合实际的加工特点,利用蒙特卡罗模拟算法对影响光学成像质量的几个关键参量,如表面粗糙度、面形误差进行了模拟,结合模拟结果对各参量的作用效果进行了分析.之后利用PANTER实验室提供的聚焦镜性能测试结果对模拟方法进行了验证,同时对面形误差参量进行了限制.最终聚焦镜结构热控件半能量宽度(half energy width, HEW)模拟与实测结果基本一致.该模拟过程可以很有效地应用于聚焦镜加工工艺的摸索,为FXT的聚焦镜测试和标定工作提供参考.结合实测标定数据,该模拟方法生成的有效面积、渐晕和点扩散函数等可用于在轨观测标定数据库.  相似文献   
22.
High spin states of the odd-A 87Sr were populated by the fusion-evaporation reaction 82Se(9Be, 4n) 87Sr at a beam energy of 46 MeV. Excited levels of 87Sr have been extended up to an excitation energy of 7.4 MeV at spin 31/2ħ. The coupling of a g9/2 neutron hole to the yrast states of the 88Sr core can account for the low-lying states in 87Sr. The structure of the higher spin states is discussed by analogy with those of the neighboring odd-A N=49 isotones and possible configurations are proposed.  相似文献   
23.
The Low Energy X-ray Telescope is one of the main payloads on the Hard X-ray Modulation Telescope satellite.Swept charge devices(SCDs)are selected as detectors for the Low Energy X-ray Telescope.As SCDs are sensitive to proton irradiation,irradiation tests were carried out on the HI-13 accelerator at the China Institute of Atomic Energy.The beam energy was measured to be 10 MeV at the SCD.The proton fluence delivered to the SCD was 3×108protons/cm2over two hours.By comparing the performance before and after irradiation,it is concluded that proton irradiation affects both the dark current and the charge transfer inefficiency of the SCD.The energy resolution of the proton-irradiated SCD is 212 eV@5.9 keV at-60?C,while it before irradiated is 134 eV.Moreover,better performance can be reached by lowering the operating temperature of the SCD in orbit.  相似文献   
24.
Readout noise is a critical parameter for characterizing the performance of charge-coupled devices (CCDs), which can be greatly reduced by the correlated double sampling (CDS) circuit. However, a conventional CDS circuit inevitably introduces new noise since it consists of several active analog components such as operational amplifiers. This paper proposes a digital CDS circuit technique, which transforms the pre-amplified CCD signal into a train of digital presentations by a high-speed data acquisition card directly without the noisy CDS circuit, then implements the digital CDS algorithm through a numerical method. A readout noise of 3.3 e- and an energy resolution of 121 eV@5.9 keV can be achieved via the digital CDS technique.  相似文献   
25.
通过融合蒸发反应144Nd(19F,5n)E=108, 112MeV对双奇核158Tm的高自旋态进行了研究. 扩展了原已建立的带结构, 并建立了2条新转动带. 获得了γ射线的相对强度和耦合带的B(M1)/B(E2)比值.观测到了πh11/2⊙νi13/2组态带的旋称反转点. 对新建立的转动带进行了自旋-宇称以及组态的讨论.  相似文献   
26.
在稀土区奇奇核πh1/2×vi13/2转动带中,系统地观测到随转动频率或角动量增加,B(M1)/B(E2)曲线表现出所谓parabola-1ike形状,即在增加到某一转动频率或自旋后,B(M1)/B(E2)比值快速增强。基于推转模型和粒子转子模型关于奇奇核二准粒子转动带磁偶极约化跃迁几率的描述,对稀土区双奇核的这一行为进行了讨论。指出该现象的发生与vi13/2准中子转动顺排特性密切相关。B(M1)/B(E2)比值在接近第二带交叉(即BC准中子对顺排)的较高频率处的增强效果,可以理解为主要来源于带交叉引起的波函数中混合四准粒子成分的结果。通过对B(M1)/B(E2)比值的增强效果发生在较低频率处的分析,对稀土区奇奇核πh1/2×vi13/2带角动量耦合图像有了进一步认识。It is systematically observed that the B(M1)/B(E2) plots with the increasing of rotational frequency, behaves as a so called parabola like shape in the π h11/2 νi13/2 bands of rare earth doubly odd nuclei (i.e., the B(M1)/B(E2) ratios increase rapidly after a certain rotational frequency). Such a phenomenon is discussed based on the formula of magnetic dipole reduced transition probability deduced from the Cranking Shell Model and Particle Rotor Model respectively. It is pointed out that, the occurrence of this behavior is closely related to the alignment nature of the νi 13/2 quasineutron. The increasing of B(M1)/B(E2) occurring at large frequency approaching the second BC crossing can be understood as mainly resulted from the mixing of wave function with the 4 quasiparticle band caused by the band crossing. Insight into the angular momentum coupling scheme between the quasiparticles and collective core in the πh11/2 νi 13/2 structures of rare earth doubly odd nuclei is gained by analyzing the increasing behavior of B(M1)/B(E2) ratios occurring at low rotational frequency.  相似文献   
27.
利用95MeV的19F束轰击116Sn靶,采用11台反康普顿BGO-HPGe探测器对蒸发剩余核退激发射的γ射线进行γ-γ符合测量.通过对多普勒展宽峰的形状分析测定了131Ce和131Pr高自旋态的寿命.根据寿命数据提取的跃迁四极矩显示,在带交叉区发生形状变化.通过与相邻偶-偶核芯130Ce的比较表明,价中子对核芯形状变化的影响大于价质子的影响.  相似文献   
28.
用熔合蒸发反应 58Ni(2 3Na,3p) (Ein=70 Me V)和 58Ni(2 8Si,α4p) (Ein=1 30 Me V)研究了78Kr的高自旋态 ,用美国劳伦斯伯克利国家实验室的γ球测量了实验中产生的瞬时符合事件,对新发现的一个负宇称带用多普勒位移衰减法对 1 0 0 4 ke V(1 0 -→ 8-)和 873ke V(8-→ 6-)作了多普勒展宽谱线形状测量 .得到了负宇称带 1 0 -态能级的寿命τ=(2 .2± 0 .3) ps,8-态能级的寿命τ=(1 .6± 0 .2 ) ps.故可知此负宇称带呈现长椭形变 ,与正宇称带的扁椭形变形状共存. Doppler shift attenuation lifetime measurements were performed in the 58 Ni( 23 Na,3p) reaction at 70 MeV and 58 Ni( 28 Si, α4p) reaction at 130 MeV. By analyzing the Doppler broadened line shapes of the 1 004 keV(10 -→8 -) negative parity transition in coincidence with depopulating transitions, the lifetime of the 10 - state has been deduced as τ =(2.2±0.3) ps. A similar analysis of 873 keV(8 -→6 -)transition gave values of τ =(1.6±0.2)...  相似文献   
29.
High-spin states of 160Tm have been studied through the 146Nd(19F, 5n) reaction at a beam energy of 102 MeV. The previously known πh11/2⊙νi13/2 yrast band and πh11/2⊙νh9/2 side band are confirmed, and several low-lying levels are observed. A 4-quasiparticle band feeding into the yrast band based on the πg7/2⊙νh9/2⊙νi13/22 is suggested. Other two bands are observed and assigned to be based on the πd3/2⊙νi13/2 and πg7/2⊙νi13/2 configurations, respectively.  相似文献   
30.
The level structures of 93 Mo are investigated using Large Scale Shell Model calculations,and reasonable agreement is obtained between the experimental and calculated values.The calculated results show that the lower-lying states are mainly dominated by proton excitations from the If5/2,2 p3/2,and 2 p1/2 orbitals into the higher orbitals across the Z=38 or Z=40 subshell closure.For the higher-spin states,multi-particle excitations,including the excitation of 2 d5/2 neutrons across the N=56 subshell closure into the high-j intruder 1 h11/2 orbital,are essential.Moreover,the previously unknown spin-parity assignments of the six higher excited states in 93 Mo are inferred from the shell model calculations.  相似文献   
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