寻找金伯利岩的合理工作程序

通过实例简要概括了金伯利岩体上物探异常的特点,重点论述了使用综合地球物理方法的原则,并提出了寻找金伯利岩的合理工作程序。     

河北沧州地区第四纪地下水~(36)Cl示踪

通过对华北平原沧州地区第四纪地下水中宇宙成因核素3 6Cl进行的测定 ,其浅层咸水的3 6Cl Cl值为5 7× 10 - 1 5,证实了该区浅层地下水的盐化成因主要是蒸发浓缩所造成。该区深层地下水中大气成因的3 6Cl所占的份额为 33%～ 30 %,系由上覆咸水下移所致。     

疏散星团NGC2244天区恒星的绝对自行研究

利用上海天文台相隔35年的两期照相底片资料,测定了疏散星团NGC2244所在天区55’×55’范围内495颗恒星基于Tycho-2星表的位置和绝对自行,并对自行精度作了初步分析。     

Is IRAS 03134 + 5958 a Herbig-Haro object?

The source IRAS 03134 + 5958 identified by Iyengar & Verma (1984) on the Palomar Observatory Sky Survey (POSS) prints with a nonstellar optical object with [P – R]≃ 5.3 ± 1.5 is near the edge of Lynds dark cloud No. 1384 and is either embedded in or behind the cloud. The galactic latitude of this source (b ^II = 2‡.3), its positionvis-a-vis the Lynds dark cloud, its nonstellar appearance, high [P – R] colour and its far-infrared spectrum, all suggest the possibility of its being a Herbig-Haro (HH) object. To test this possibility we undertook measurements of its proper motion and variability (two of the characteristic properties of HH objects). These yield μ_a = (3.6 ± 2.3) arcsec/century and μ_δ= (−1.2 ± 2.0) arcsec/century for its proper motion. The source reveals large variation in brightness between 1950 and 1954. Optical line studies of the source are required to confirm its classification as an HH object.     

球状星团NGC4147的绝对自行和颜色星等图

本文以上海天文台佘山40厘米折射望远镜于1958年拍摄的3张照相底片为第一期,印度Kavalur的234米VainuBappu望远镜于1996年用CCD拍摄的4幅图像为第二期,使用Brosche等1985年发表的球状星团NGC4147天区42颗恒星的位置和绝对自行作为参考架,用中心重叠法进行天体测量归算,得到了这个星团中心附近11'×11'天区内到B＝17.6为止115颗恒星的位置和绝对自行,利用这些自行对成员概率作了估计.本文还给出了用VainuBappu望远镜CCD测光结果得到的这个星因水平文和巨星支恒星V与B-V．V－R和V－I颜色星等图,并对这些颜色星等图和团自行作了讨论,得到这个星团的赤经方向绝对自行为-2.82±0.49mas／yr,赤纬方向绝对自行为2.37±0.43mas／yr.     

疏散星团NGC6530天区的恒星自行和成员概率

利用上海天文台的照相底片资料,确定了疏散星团NGC6530天区364颗恒星的自行和成员概率,并对有关自行测定的方法、结果和精度等问题作了较为详细的介绍和讨论。使用的底片历元差为87年,全部恒星自行中误差的均方根值为1．09mas/a。     

福建泉州湾贝类养殖容量评估

通过对泉州湾叶绿素a、初级生产力、生态效率、浮游植物有机碳含量、养殖贝类有机碳含量及其含壳重与鲜组织重比值、潮间带和潮下带及吊养区附着滤食性动物现存量等的调查和检测,应用营养动态模型、沿岸能流模型估算贝类生态容量及扣除野生滤食性动物现存量来估算贝类养殖容量。还采用方建光模型估算贝类养殖容量,并采用统计分析法估算贝类及其各品种的适养面积。3种模型估算的贝类养殖容量分别为43 171t、220 991×104个,46 388 t、237 464×104个,44 049t、225 490×104个。贝类适养总面积为2 878hm2,其中牡蛎Ostrea1 349hm2,缢蛏Sinoncvacula con-stricta1 268 hm2,菲律宾蛤仔Ruditapes philippinarum117hm2,翡翠贻贝Perna viridis144hm2。1999年实际养殖面积2 615 hm2,尚有263 hm2可扩大养殖面积。还讨论了模型的实用性等问题。     

河北舍女寺油田女12—女20断块孔二段沉积微相与油气聚集关系研究

黄骅坳陷南部舍女寺油田的古近系孔店组是在断陷盆地的快速充填过程中形成的典型的河流—三角洲沉积。根据取芯井段的取芯和测井资料分析,把剖面结构、砂体几何形态、沉积构造等微相特征进行描述和分析,划分出水下分流河道、河口坝、席状砂等储层沉积微相类型。研究表明,舍女寺地区沉积微相不仅控制储集层的分布,而且控制油气聚集。研究区中较大厚度的油层分布在水下分流河道的中心部位,即该区沉积微相带的主体部位起着油层控制作用。在复杂断块高含水开发中后期,微突起、微断层、微断鼻等圈闭和储集层的有利配置区,尤其是中心微相带与有利的微构造部位叠合区将是有利高产井区。     

Proper motion measurements in the HH 46/47 outflow

Proper motion measurements have been carried out for the HH 46/47 outflow system. The results of these measurements and some implications for the physics of the outflow and its modelling are discussed.     

Determination of the Proper Motions and Membership of the Globular Cluster M3 and of its Orbit in the Galaxy

We examine 14 plates of the globular cluster M3 (NGC 5272) taken with the 40 cm refractor at the Sheshan station of Shanghai Astronomical Observatory. The plates span over a period of about 77 years. The positions and absolute proper motions of eight stars in the Hipparcos Catalogue and of 49 stars in the Tycho-2 Catalogue are used as the reference frame. The astrometric reduction is made with the central overlapping principle. The absolute proper motions of 534 stars in a region of about 100' × 100' around the cluster are measured. With the new proper motion data the membership probabilities of the stars are determined. The average absolute proper motion obtained for the cluster is -0.06@0.30 mas yr-1 in R.A. and -2.6@0.30 mas yr-1 in Decl. By combining this result with the known distance and radial velocity of the cluster, we also obtained the Galactic orbit of M3 for a chosen three-component Galactic potential.