藏北羌塘盆地双湖地区油气成藏条件

藏北双湖地区油气显示有中侏罗统布曲组的隆鄂尼碳酸盐岩古油藏、充填于夏里组石膏孔洞里的沥青和夏里组砂岩夹层中的油页岩。布曲组及索瓦组中的生油岩有机碳含量普遍较高,生油能力大。油页岩的氯仿沥青“A”高达25255×10-6,有机碳含量28.8%,但总烃含量在40%～50%左右,OEP值分别为0.7和0.8,显示有机质演化处于低成熟阶段。有机质中既有Ⅰ型酐酪根,也有Ⅲ型酐酪根。有机质形成环境既有浅海陆棚相开阔型水体环境,也有半封闭型泻湖相等沉积环境。该地区可划分出4套生、储、盖组合,以第一套组合(由曲色组和布曲组组成)为最好。     

褐藻酸降解菌的产酶条件研究

以海带病烂处分离到的别单胞菌属（Alkteromonas)的褐藻酸降解菌菌株A1为研究对象，在该菌的产酶条件进行了研究。结果表明，产酶的最适温度20℃，褐藻酸钠浓度（质量分数）0．5％－0．6％，pH7.5，盐度15，氮源为（NH4)2SO4，培养时间72h。     

水平螺旋槽管壁面液膜传热特性的研究

对管式高效传热传质元件的工程应用进行理论探讨,根据水平螺旋槽管壁面液膜的形成机理及传热特性,通过建立单组分流体的物理和数学模型,得到了液膜速度和厚度解析解,并分析了在蒸发、冷凝时水平螺槽管的表面几何形状对液膜厚度分布的影响。结果表明：液膜的厚度主要受表面张力和槽道表面几何形状的影响,在槽道内弯处较厚,而在槽道起始处较薄,冷凝时与蒸发时相比液膜厚度更薄,液膜分布更均匀。相对于光滑直管,水平螺旋槽管壁面液膜具有更均匀的厚度分布,具有更好的传热传质性能。     

The Formation and Circulation of the Intermediate Water in the Japan Sea

In order to clarify the formation and circulation of the Japan/East Sea Intermediate Water (JESIW) and the Upper portion of the Japan Sea Proper Water (UJSPW), numerical experiments have been carried out using a 3-D ocean circulation model. The UJSPW is formed in the region southeast off Vladivostok between 41°N and 42°N west of 136°E. Taking the coastal orography near Vladivostok into account, the formation of the UJSPW results from the deep water convection in winter which is generated by the orchestration of fresh water supplied from the Amur River and saline water from the Tsushima Warm Current under very cold conditions. The UJSPW formed is advected by the current at depth near the bottom of the convection and penetrates into the layer below the JESIW. The origin of the JESIW is the low salinity coastal water along the Russian coast originated by the fresh water from the Amur River. The coastal low salinity water is advected by the current system in the northwestern Japan Sea and penetrates into the subsurface below the Tsushima Warm Current region forming a subsurface salinity minimum layer. This revised version was published online in August 2006 with corrections to the Cover Date.     

Dynamics and Variability of Terra Nova Bay Polynya

Abstract. We present a process study on the dynamics and variability of the Terra Nova Bay polynya in the western sector of the Ross Sea. The air-sea heat exchange is known to be particularly large in polynya during the winter, when differences between air and sea temperatures are large. We apply a 1-D model (Pease, 1987; Van Woert, 1999a, 1999b), which is modified in the latent heat parameterisation in order to account for time-dependent relative humidity and cloud coverage. Furthermore, the Ice Collection Depth is correlated linearly with a variable wind speed. The model is forced with two different meteorological data sets: the operational analysis of the European Center for Medium Range Weather Forecasts atmospheric data set and the meteorological parameters measured by an Automatic Weather Station located on the coast of Terra Nova Bay. The results are compared in terms of polynya extension, ice, and High Salinity Shelf Water production. According to the two different wind velocities, the results obtained from the different data sets clearly differ. Qualitatively, however, the results are in good agreement.     

铁山港湾水下动力地貌特征及其成因

探讨了铁山港湾的潮间浅滩、潮流冲刷深槽、潮流沙脊、水下拦门浅滩、水下岸坡和海底平原等水下动力地貌的形态特征及其成因,并结合沉积物的粒度、碎屑重矿物的分布特征,阐述了泥沙来源及运移趋势。     

井下双向流动阀防漏失技术在埕岛油田的应用

埕岛油田位于渤海西南部极浅一浅海地区,是一个大型潜山披覆构造油田。随着埕岛油田开采力度加强,地层亏空十分严重,作业过程中的地层漏失是困绕埕岛油田油层保护的一大难题。据此介绍了胜利油田海上埕岛油田油层保护的一项新技术——井下双向流动阀防漏失技术的应用情况,阐述了井下双向流动阀的结构、原理以及应用后对油层保护所起到的作用。     

南太平洋辐合带(SPCZ)的特征分析

根据热带西太平洋卫星云图资料及流场特征分析,讨论了南太平洋辐合带(SPCZ)的演变特征和形成机理。提出SPCZ是反映西太暖池同东太冷舌海气耦合系统以及暖池大气同相邻陆区大气间相互作用的重要特征。主要表现为在12～2月的热带西太平洋上的NW/SE辐合带,其形成原因主要应归因于西太暖池本身,以及暖池与东太赤道冷水舌强度与相对位置改变引发的Walker环流位置与走向的变动,另外,新几内亚岛及澳洲大陆也有重要影响。     

三肇凹陷葡萄花油层高分辨率层序地层划分及沉积特征研究

应用高分辨率层序地层学理论,通过对各级基准面旋回的沉积动力学分析,依据１０口井岩心和１２５６口井测井资料,把松辽盆地三肇凹陷葡萄花油层划分为１个长期基准面旋回、２个中期基准面旋回、１２个短期基准面旋回,提出了葡萄花油层南部为同沉积构造抬升控制的中部缺失而非底部缺失的层序地层新格架。通过对短期基准面旋回内储层沉积特征、单砂体展布规律的研究,认为葡萄花油层主要储层水下河道砂体比原认识更连续,且延伸较远, 分流平原、内前缘相带南移达３６ｋｍ,这对深入认识该区油藏类型、聚油规律、特别是高含水期剩余油挖潜具有重要意义,对指导整个松辽盆地北部岩性油气藏勘探与开发具有重大影响。     

Studies of ultracompact H ii regions — II. High-resolution radio continuum and methanol maser survey

High spatial resolution radio continuum and 6.67-GHz methanol spectral line data are presented for methanol masers previously detected by Walsh et al. (1997). Methanol maser and/or radio continuum emission is found in 364 cases towards IRAS -selected regions. For those sources with methanol maser emission, relative positions have been obtained to an accuracy of typically 0.05 arcsec, with absolute positions accurate to around 1 arcsec. Maps of selected sources are provided. The intensity of the maser emission does not seem to depend on the presence of a continuum source. The coincidence of water and methanol maser positions in some regions suggests there is overlap in the requirements for methanol and water maser emission to be observable. However, there is a striking difference between the general proximity of methanol and water masers to both cometary and irregularly shaped ultracompact (UC) H  ii regions, indicating that, in other cases, there must be differing environments conducive to stimulating their emission. We show that the methanol maser is most likely present before an observable UC H  ii region is formed around a massive star and is quickly destroyed as the UC H  ii region evolves. There are 36 out of 97 maser sites that are linearly extended. The hypothesis that the maser emission is found in a circumstellar disc is not inconsistent with these 36 maser sites, but is unlikely. It cannot, however, account for all other maser sites. An alternative model which uses shocks to create the masing spots can more readily reproduce the maser spot distributions.