Radial velocity searches for other planetary systems:Current status and future prospects

Measurement of variations in the radial velocities of stars due to the reflex orbital motion of the star around the planetary-system barycenter constitutes a powerful method of searching for substellar or planetary mass companions. After several years of patient data acquisition, radial-velocity searches for planetary systems around other stars are now beginning to bear fruit. In late 1995 and early 1996, three candidate systems were announced with Jovian-mass planets around solar-type stars. The current paradigm for low-mass star formation suggests that planetary systems should be able to form in the circumstellar disks surrounding young stellar objects. These newly discovered systems, and other discoveries which will soon follow them, will test critically our understanding of the processes of star- and planet-formation. We review the techniques used in these radial-velocity searches and their results to date. We then discuss planned improvements in the surveys, and the prospects for the next 20 years.     

Elastic properties of granulite facies rocks of Mahabalipuram, Tamil Nadu, India

Compressional and shear wave velocities and attenuation measurements have been carried out in some of the borehole samples of acidic, basic and intermediate granulites of Mahabalipuram, Tamil Nadu, India. The results have been obtained at ambient conditions using ‘time-of-flight’ pulse transmission technique at 1.0 MHz frequency. The results show linear relationships between velocity and density, and velocity and attenuation properties of the rocks. The acidic granulites show lower velocities and higher attenuation than the intermediate and basic granulites. The average values of the Poisson’s ratio of acidic, intermediate and basic granulites have been found to be 0.210, 0.241 and 0.279 respectively. The variations in velocities and attenuation in these low porosity crystalline rocks are found to be strongly influenced by their mineral composition. The laboratory velocity data (extrapolated to high pressure) of the present study and the published field velocity data from deep seismic sounding studies indicate that these granulite facies rocks may belong to mid-crustal depths only.     

Effect of protection against wind according to the variation porosity of wind fence

This study examines shelter effect against the wind by using wind fence with various porosities and distance. The shelter effect of wind fence was investigated by a wind tunnel test. Flow characteristics of velocities and turbulences behind wind fence were measured using a hot-wire anemometer. This was done by varying the porosity by 0, 20, and 40% of the wind fence. The wind fence distance ranged from 1H to 9H. In addition, the overall characterization of the wind fence was investigated by measuring a total of 28 points on the wind fence, which forms a lattice structure on it with 7 points in the lateral direction and 4 points in the vertical direction. The results indicate that the degree of the turbulence is lowered and the velocity of the wind is decreased when porosity of 40% is used at a distance of 4H–7H. The effectiveness of the wind fence depends on the porosity and distance. Porosity of 20% proved to be effective for the protection area of 1H–3H, while that of 40% was effective for the protection area of 4H–6H.     

Properties of the lithosphere-asthenosphere system in Europe with a view toward earth conductivity

Over the past 20 years the study ofP- andS-wave velocities in the upper mantle of the Mediterranean area and continental Europe has been the subject of intensive research work. We present a summary of results based on the inversion of available surface-wave dispersion data andP-wave trave time observations. For areas characterized by different tectonic settings and very large lateral variations, a discussion is made about structural models based on seismological, geothermal and electrical conductivity data.     

硬化粗质地基冻土层的速度参数与卓越周期的关系

本文给出了对共振现象出现概率的理论分析与实验数据间关系的思考。样品取自位于半空间的硬化粗质冻土地基,包括石质冻层。参考从三个场地14次地震记录的纵、横波速求得的土层相对频率特征,进行了对其共振频率的评估。纵、横波速在前贝加尔和后贝加尔地区的粗质冻土层中随湿度和温度而变化。将这些概括化的速度值与一个共振频率和纵、横波度之间的关系式结合起来,用于评估被调查土层的纵、横波速的概率值。结果显示,通过综合在实验室尺度获得的速度值和现场测量获得的速度值的数据,则利用地震记录波来确定在松散土层内传播速度的概率值是可能的。     

Groundwater Renewal in the Middle Odra River Catchment Based on Flow Model and Isotopic Data – the Lubin Głogów Copper Region,Poland

In the area of intense mining within the Lubin Głogów Copper Region the investigation of groundwater renewal was made according to two methods: a numerical flow model and isotopic analysis. The results of model simulations show that within the shallow aquifer the groundwater renewal is quick and mostly depends on infiltration within the recharge zones. An average time of groundwater flow between recharge and discharge areas in the representative part of the entire system has been obtained as 130 years. The content of isotopes was determined in samples collected as well from the mine excavations as from water intakes. The measurements were done on 17 samples. Results of isotopic studies indicate that the relationship of δD – δ18O in groundwater gathers along the established local meteoric water line (MWL) δD = 7.58 δ18O + 4.45. Deep groundwaters that create an inflow to the mines were formed by infiltration in Holocene with reference to two of total four mines and probably in Eopleistocene in another two.     

古地磁欧拉极及对华北地块的应用

本文详细讨论了古地磁欧拉最佳小圆拟合法的基本原理和实际方法，并提出了提高拟合速度和优度的措施，同时利用此方法对前人取得的华北地块中石炭世至晚侏罗世这一时间的古地磁视极移曲线进行了最佳小圆拟合。