天山托木尔峰地区青冰滩72号冰川表面运动速度特征研究

托木尔峰地区是天山最大的冰川分布区,是阿克苏地区主要水资源补给地.一直以来,该区冰川运动资料空白,严重阻碍了对冰川水资源现状及未来变化评估工作的开展.鉴于以上情况,中国科学院天山冰川站在2008年8月到2009年8月3次开展了对天山托木尔峰青冰滩72号冰川表面运动速度的观测,获得了冰川表面运动速度特征变化状况.结果表明:青冰滩72号冰川冰舌区域运动速度存在明显的消融季和非消融季的差异,消融季速度偏大.年均水平运动速度47.1m.a-1速度分布受局地地形因素影响明显.与天山乌鲁木齐河源1号冰川相比,该冰川运动速度明显偏大,消融季底部滑动显著,其运动特征更偏向海洋性冰川.

球状星团M79的自行测定和轨道运动

利用上海天文台相隔29年的两期天体测量底片,测量了球状星团M79的绝对自行,采用Harris给出的这个星团离开太阳的距离和视向速度数据,计算了星团当前的空间运动速度;根据银河系引力势模型,进一步计算了该星团在银河系中的轨道参数.还对利用自行数据所作的球状星团运动学研究的不确定性作了讨论.

Modeling of Bubble Motion in Two Dimensional Space

The equations of motion of a bubble, expanding adiabatically through an incompressible viscous fluid, are deduced when the centre of the bubble moves in a vertical plane in the presence of gravitational acceleration, acting vertically downwards. The non-linear equations of motion obtained are solved numerically for different values of the various parameters of the problem. The path traced by the centre of the bubble and velocity of the centre, the change of radius R with time, and the influence of the buoyancy force, which is experienced by the expanding bubble for different values of the gravitational acceleration on these quantities, are investigated. The radius R（t） of the bubble is found to vary periodically with time when the acceleration due to gravity is small. But when the acceleration due to gravity increases, this periodicity in the value of R（t） with t is lost. The influence of viscosity in determining the periodicity of the bubble motion is also investigated.