A rope-shaped solar filament and a IIIb flare

On September 14–18, 2000, a medium-small solar active region was observed at Ganyu Station of Purple Mountain Observatory. Its spots were not large, but it had a peculiar active filament. On Sep.16, a flare of importance III_b with rather intense geophysical effects was produced. Our computation of the magnetic structure of the active region reveals that the rope-shaped filament was concerned with a low magnetic arc close to magnetic neutral line. An intense shear of magnetic field occurred near magnetic rope. The QSL analysis shows that a 3-D magnetic reconnection might appear in the vicinity of filament, and this can be used to interpret the formation of a large flare.     

Experimental research on reservoir sensitivity to stress and impacts on productivity in Kela 2 Gas Field

Kela 2 Gas Field, with high formation pressure (74.35MPa), high pressure coefficient (2.022) and difficulty of potential test and evaluation, is the largest integrated proved dry gas reservoir in China so far and the principal source for West-East Gas Development Project. In order to correctly evaluate the elastic-plastic deformation of rocks caused by the pressure decline during production, some researches, as the experiment on reservoir sensitivity to stress of gas filed with abnormal high pressure, are made. By testing the rock mechanic properties, porosities and permeabilities at different temperature and pressure of 342 core samples from 5 wells in this area, the variations of petro-physical properties at changing pressure are analyzed, and the applicable inspection relationship is concluded. The average productivity curve with the reservoir sensitivity to stress is plotted on the basis of the research, integrated with the field-wide productivity equation. The knowledge lays a foundation for the gas well productivity evaluation in the field and the gas field development plan, and provides effective techniques and measures for basic research on the development of similar gas fields.     

华北地台北缘花岗岩—绿岩型金矿田及盲矿体的找矿模型

花岗岩—绿岩型金矿田的找矿模型地质上是富镁铁质绿岩、韧性剪切带与重熔岩体的三体一位;物探上位于航磁高背景场的负磁异常带边缘,矿田晕分散流异常规模大、强度高,有明显的浓集中心。隐伏矿床、盲矿体的找矿模型地质上是韧性剪切带、退变质带及脆性断裂带的三体一位;物探上呈现高极化率、低电阻、位于磁异常边缘的“一高一低一边”模型;化探原生晕上呈现As、sb、F、Ag、Bi、W的找矿模型。     

山东省泰安市大汶口盆地岩盐矿地质特征及开发煮义

大汶口盆地岩盐矿均为第四系所覆盖,钻孔揭露,除第四系外,主要为古近系官庄群大汶口组.大汶口盆地主要是由南留断裂所控制.岩盐矿是大汶口盆地盐类矿床的主体.矿层多而集中,厚度大而变化小,品位高而稳定.矿层延展面积约45km2,其平面形态为一个椭圆形,在空间上整个含盐段似一个向北缓倾的大透镜体.矿石自然类型有3种,即块状岩盐(灰白盐)、含杂质岩盐(杂色盐)和脉状岩盐,其中以块状岩盐为主,含杂质岩盐次之,脉状岩盐不具有工业意义.该矿床地质条件好、埋藏深度适宜,外部建设条件好,该矿床具备大规模开发的条件,矿业开发可促进当地的经济发展.当地政府有关部门已在着手工作,推动该岩盐矿规模开发进程.     

经受住汶川8．0级地震考验的RSDA-1采集器

RSDA-1地震数据采集器是四川省地震局水库地震研究所于2006年7月～2007年6月研制出的新产品,2007年8月用于瓦屋山水库地震台网的4个台站和紫坪铺水库地震台网的庙子坪地震台。庙子坪地震台位于汶川8．0级地震震中区15km的极震区。截止2008年8月,历时一年并经受住汶川8．0级地震考验的RSDA-1采集器总体运行良好。本文从运行情况、事件定位和“平坦限幅”等3方面说明RSDA-1采集器在两个水库地震台网的运行情况。     

Air–sea interaction over ocean fronts and eddies

Air–sea interaction at ocean fronts and eddies exhibits positive correlation between sea surface temperature (SST), wind speed, and heat fluxes out of the ocean, indicating that the ocean is forcing the atmosphere. This contrasts with larger scale climate modes where the negative correlations suggest that the atmosphere is driving the system. This paper examines the physical processes that lie behind the interaction of sharp SST gradients and the overlying marine atmospheric boundary layer and deeper atmosphere, using high resolution satellite data, field data and numerical models. The importance of different physical mechanisms of atmospheric response to SST gradients, such as the effect of surface stability variations on momentum transfer, pressure gradients, secondary circulations and cloud cover will be assessed. The atmospheric response is known to create small-scale wind stress curl and divergence anomalies, and a discussion of the feedback of these features onto the ocean will also be presented. These processes will be compared and contrasted for different regions such as the Equatorial Front in the Eastern Pacific, and oceanic fronts in mid-latitudes such as the Gulf Stream, Kuroshio, and Agulhas Return Current.     

Observation and Research of the Transits of Extrasolar Planets

In order to make more accurate estimates of the physical parameters of extrasolar planets, the observation and research on the phenomena of transits of the 7 known stars with the planetary systems TrES-1, TrES-3, XO-2, WASP-1, WASP-2, WASP-3 and HAT-P-7 are carried out with the 1-m reflecting telescope at Shandong University Weihai Astronomical Observatory/Weihai Municipal Astronomical Observatory. The fundamental conditions of the observation and data processing are introduced, and the transit light curves as well as the parameters of some planets derived from them are given. At the same time, when the results are summarized and analyzed, the prospects for the more in-depth and detailed researches which will be further carried out are also described.     

Feasibility of Re-injecting the Production Effluent from Alkali–Surfactant–Polymer Flooding Systems Back into a Reservoir to Further Improve Oil Recovery

Natural Resources Research - Alkali–surfactant–polymer (ASP)-produced effluent contains polymer, alkali and surfactant, and it has higher content of suspended oil droplets and suspended...