~(157)YB的形状共存和Vi_(13/2)带的结构演变

利用在束γ谱学技术,通过反应144Sm（16O,3n）研究了157Yb的高自旋态,其中16O束流的能量为90MeV.采用门套BGO（AC）HPGe探测器进行了长时间的γ-γ-t符合测量.基于γ-γ符合关系、γ射线的各向异性度和DCO系数的测量结果,首次建立了157Yb的高自旋能级纲图.围绕157Yb的能级纲图着重讨论了此核的形状共存和Vi13/2能带随着角动量增加的结构演变,另外还比较了N=87同中子素链的Vi13/2转动带结构的系统性.

~(157)Yb的形状共存研究(英文)

利用在束γ谱学方法 ,通过反应1 4 4 Sm( 1 6O ,3n) 1 57Yb研究了1 57Yb的激发态能级结构 .实验中使用的1 6O束流能量为 90MeV .基于实验得到的γ γ符合关系、γ射线的各向异性度和DCO系数 ,建议了1 57Yb的高自旋能级纲图 .1 57Yb的能级纲图主要由两串跃迁性质明显不同的级联能级组成 ,它们分别对应于νi1 3 2 转动带和单粒子激发态 .着重讨论了1 57Yb的形状共存和νi1 3 2 转动带随角动量的结构演化 .

~(153)Er, ~(157)Yb(EC+#beta#~+)衰变纲图的首次建立

用蒸发中子反应产生~(157)Tb和~(153)Er，收集活性样品，作x, #gamma# 单谱及符合谱测量，对~(157)Yb和~(153)Er的(EC+#beta#~+)衰变进行了研究，给出了~(157)Yb及~(153)Er的衰变纲图，其中~(157)Yb的衰变纲图包括25条新#gamma#射线，分析~(157)Yb的衰变纲图，~(153)Er的衰变纲图包括15条#gamma#射线，并指定出~(153)Er半衰变期值，该值与文献给出值符合得很好。指定了~(153)Er的衰变纲图中能级状况

缺中子同位素~(153)Er和~(157)Yb的（EC/β~+）衰变纲图

利用142Nd（16O，5n）153Er和147Sm（16O，6n）157Yb反应并藉助与氦喷嘴快速带传输装置和x(γ) γt-符合测量技术首次建立了153Er和157Yb的（EC/β+）衰变能级纲图。 对153Er的（EC/β+）衰变纲图的分析，得到结果有， 1） 辨认了256.7KeV和634.2KeV的二条低位能级分别为d3/2和d5/2的单质子态。因此，153H0的基态 的形状为球形。在同位素链Ho（Z=67）上，随着中子数的增加，奇质量数Ho核的基态核形状由球形过渡到变形发生在中子数86和88之间。 2） 位于1700.1KeV能级为三粒子态，具有[(πh11/2 νh9/2)1+ νf7/2] ， ， 的结构特征。 经对157Yb的（EC/β+）衰变纲图分析，得到结果有， 1） 发现了建立在157Tm基态上的Kπ= 转动带的带头部分。用可变转动惯量的三轴行变粒子转子模型对157Tm的转动能谱的计算结果表明，157Tm的基态Kπ= 转动带所对应的形变是三轴形变，相应的形变参数为ε2=0.23，ε4=0.01，γ=35°。给出了随着中子数的增加，奇质量数Tm（Z=69）核的基态核形状由球形过渡到非球形发生在中子数86和88之间。 2） 辨认了一条位于激发能为3502KeV的同质异能态，其寿命>40ns。

Comparative observation of Ar, Ar-H-2 and Ar-N-2 DC arc plasma jets and their arc root behaviour at reduced pressure

Results observed experimentally are presented, about the DC arc plasma jets and their arc-root behaviour generated at reduced gas pressure without or with an applied magnetic field. Pure argon, argon-hydrogen or argon- nitrogen mixture was used as the plasma-forming gas. A specially designed copper mirror was used for a better observation of the arc-root behaviour on the anode surface of the DC non-transferred arc plasma torch. It was found that in the cases without an applied magnetic field, the laminar plasma jets were stable and approximately axisymmetrical. The arc-root attachment on the anode surface was completely diffusive when argon was used as the plasma-forming gas, while the arc-root attachment often became constrictive when hydrogen or nitrogen was added into the argon. As an external magnetic field was applied, the arc root tended to rotate along the anode surface of the non-transferred arc plasma torch.

环状日冕瞬变的活塞驱动理论

本文用柱面活塞驱动过程模拟环状日冕瞬变现象。用特征线法数值研究在太阳引力作用下活塞的运动过程,得出了符合活塞运动条件及联结条件的等离子体密度分布、流速分布及激波特征。活塞驱动理论所得结果在形态、运动学、动力学及演化方面均与观测一致。

板块运动的模拟实验

本文较详细地分析了板块运动模拟实验的困难性.提出了用物质密度差代替温度差的实验方法,结合离心技术,研究了地幔对流对板块运动的作用,成功地再现了板块运动的流动图案。 通过对上涌流动微分方程组的分析,本文还建立了模拟实验中“模型”与“原型”之间的相似准则D_e=D_m。

Computation of turbulent-flow in a square duct - aspects of the secondary flow and its origin

A numerical study of turbulent flow in a straight duct of square cross-section is made. An order-of-magnitude analysis of the 3-D, time-averaged Navier-Stokes equations resulted in a parabolic form of the Navier-Stokes equations. The governing equations, expressed in terms of a new vector-potential formulation, are expanded as a multi-deck structure with each deck characterized by its dominant physical forces. The resulting equations are solved using a finite-element approach with a bicubic element representation on each cross-sectional plane. The numerical integration along the streamwise direction is carried out with finite-difference approximations until a fully-developed state is reached. The computed results agree well with other numerical studies and compare very favorably with the available experimental data. One important outcome of the current investigation is the interpretation analytically that the driving force of the secondary flow in a square duct comes mainly from the second-order terms of the difference in the gradients of the normal and transverse Reynolds stresses in the axial vorticity equation.

A discussion about a class of stress intensity factors and its verification

In this paper, new formulae of a class of stress intensity factors for an infinite plane with two collinear semi-infinite cracks are presented. The formulae differ from those gathered in several handbooks used all over the world. Some experiments and finite element calculations have been developed to verify the new formulae and the results have shown its reliability. Finally, the new formulae and the old are listed to show the differences between them.