栉孔扇贝(♀)×虾夷扇贝(♂)子一代杂种优势的SRAP分析

采用新型的分子标记技术(Sequence-related amplified polymorphism,简称SRAP)对栉孔扇贝(Chlamys farreri)(♀)×虾夷扇贝(Patinopecten yessoensis)(♂)子一代及其双亲的遗传变异进行分析.从不同的引物组合中筛选出9对条带清晰、多态性丰富的组合,9对引物共产生了121条扩增带,其中多态性条带107条,平均每对引物组合产生11.89条多态标记.Shannon信息指数I分别为0.299 9、0.218 9、0.334 3,Nei's基因多样性指数h分别是0.196 4、0.141 1、0.218 9,栉孔扇贝与杂交后代的遗传距离是0.107 4,虾夷扇贝与杂交后代的遗传距离是0.228 7,聚类分析也显示了这一特点.从变异贡献率来看,3个群体的总变异中,有37.31%的变异来源于群体间,62.69%的变异来源于个体间.     

The spectroscopic period of the Cepheid SU Cassiopeiae

The spectroscopic period of the short periodic Cepheid SU Cas was determined from the radial velocity measurements by ABT, GIEREN and HÄUPL. The calculated period is 1.949312 days. Radial velocity differences between measurements by GIEREN and HÄUPL are explained as velocity zero point of the used spectrographs. The zero point of the Tautenburg Coudé spectrograph was determined by measuring the radial velocity standard star ϵ Leo. The difference to the standard value was -0.7 km/s. No significant differences are found between the spectroscopic period and light curve of SU Cas in the last 35 years.     

Photometric Follow-up Transit (Primary Eclipse) Observations of WASP-43 b and TrES-3b and A Study on Their Transit Timing Variations

Two photometric follow-up transit (primary eclipse) observations on WASP-43 b and four observations on TrES-3 b are performed using the Xuyi Near-Earth Object Survey Telescope. After differential photometry and light curve analysis, the physical parameters of the two systems are obtained and are in good match with the literature. Combining with transit data from a lot of literature, the residuals (O ? C) of transit observations of both systems are fitted with the linear and quadratic functions. With the linear fitting, the periods and transit timing variations (TTVs) of the planets are obtained, and no obvious periodic TTV signal is found in both systems after an analysis. The maximum mass of a perturbing planet located at the 1:2 mean motion resonance (MMR) for WASP-43 b and TrES-3 b is estimated to be 1.826 and 1.504 Earth mass, respectively. By quadratic fitting, it is confirmed that WASP-43 b may have a long-term TTV which means an orbital decay. The decay rate is shown to be P? = (?0.005248 ± 0.001714) s·yr^?1, and compared with the previous results. Based on this, the lower limit of the stellar tidal quality parameter of WASP-43 is calculated to be ${Q^{\prime }}_{*}\ge 1.5\times {10}^5$, and the remaining lifetimes of the planets are presented for the different ${Q^{\prime }}_{*}$ values of the two systems, correspondingly.     

Research and Test of Real-time Search Algorithm of Fast Radio Bursts Based on GPU Acceleration

In order to satisfy the research need of Nanshan 25 m radio telescope of Xinjiang Astronomical Observatory (XAO) and study the key technology of the planned QiTai radio Telescope (QTT), on the basis of the original CPU (Central Processing Unit)-based real-time search algorithm of FRBs (Fast Radio Bursts), we have studied the GPU (Graphics Processing Unit)-based real-time search algorithm of FRBs, and built the corresponding real-time search system of FRBs. We have made the comparison and analysis on the GPU system and CPU system, the test result shows that under a given searching accuracy, the speed of the GPU-accelerated algorithm is improved by 35–45 times compared with that of the CPU algorithm.     

Low-energy Lunar Trajectories with Lunar Flybystwo

The low-energy lunar trajectories with lunar flybys are investigated based on the Sun-Earth-Moon bicircular problem (BCP). The characteristics of the distribution of trajectories in the phase space are summarized. Using the invariant manifolds in the BCP system, the low-energy lunar trajectories with lunar flybys are sought. Then, take time as an augmented dimension in the phase space of a nonautonomous system, we present the state space map and reveal the distribution of these lunar trajectories in the phase space. Consequently, we find that the low-energy lunar trajectories exist as families, and that the every moment in the Sun-Earth-Moon synodic period can be the departure date. Finally, we analyse the velocity increment, transfer duration, and system energy for the different trajectory families, and obtain the velocity-impulse optimal family and the transfer-duration optimal family, respectively.     

柱撑蛭石吸附去除废水中重金属离子的实验研究

分别利用有机柱化剂十二烷基磺酸钠(SDS)和无机柱化剂聚羟基铝(HA)对蛭石进行柱撑制得十二烷基磺酸钠柱撑蛭石(SDS-V erm icu lite)和聚羟基铝柱撑蛭石(HA-V erm icu lite),并通过XRD、红外光谱、ZETA电位等表征手段对柱撑蛭石进行表征,同时针对柱撑蛭石对Cu2 ,Cd2 ,C r3 3种重金属离子的吸附进行研究,结果表明:吸附去除率受反应时间、重金属离子的初始浓度、pH值等因素的影响,经柱撑后的蛭石对重金属离子吸附的吸附性能比蛭石原矿要强。柱撑蛭石吸附3种重金属离子的动力学吸附过程可用E lov icb方程和双常数方程进行较好的拟合。     

The behaviour of dissolved organic material,iron and manganese in estuarine mixing

Fractionation by ultra-filtration of the dissolved organic material (DOM) in the River Beaulieu, with typical concentrations of dissolved organic carbon (DOC) of 7–8 mg C/l, showed it to be mainly in the nominal molecular weight range of 10³–10⁵, with 16–23% of the total DOC in the fraction > 10⁵. The molecular weight distribution of DOM in the more alkaline River Test (average DOC, 2 mg C/l) was similar. In the River Beaulieu water, containing 136–314 βg Fe/l in ‘dissolved’ forms, 90% or more of this Fe was in the nominal molecular weight fraction > 10⁵. Experiments showed that DOM of nominal molecular weight <10⁵ could stabilize Fe(III) in ‘dissolved’ forms. The concentrations of ‘dissolved’ Fe in the river water probably reflect the presence of colloidal Fe stabilized by organic material and this process may influence the apparent molecular weight of the DOM. Dissolved. Mn (100–136 βg/l) in the River Beaulieu was mainly in true solution, probably as Mn(II), with some 30% in forms of molecular weight greater than ca 10⁴.During mi xing in the Beaulieu Estuary, DOC and dissolved Mn behave essentially conservatively. This contrasts with the removal of a large fraction of the dissolved Fe (Holliday and LISS, 1976, Est. Coastal Mar. Sci. 4, 349–353). Concentrations of lattice-held Fe and Mn in suspended particulate material were essentially uniform in the estuary, at 3.2 and 0.012%, respectively, whereas the non-lattice held fractions decreased markedly with increase in salinity. For Mn the decrease was linear and could be most simply accounted for by the physical mixing of riverborne and marine participates, although the possibility that some desorption occurs is not excluded. The non-linear decrease in the concentration of non-lattice held Fe in particulates reflected the more complex situation in which physical mixing is accompanied by removal of material from the ‘dissolved’ fraction.     

东北地区前中生代构造演化及其与晚中生代盆地发育的关系

摘　 要　 东北地区前中生代构造演化可大致分为如下阶段：（1） 中、新元古代阶段;（2） 早古 生代加里东阶段;（3） 泥盆纪—早石炭世早华力西阶段;（4） 晚石炭世—三叠纪晚华力西—印 支阶段。多旋回构造演化使该区形成由多期褶皱带和多中间或边缘地块组成的 “镶嵌构造 区”‚并为晚中生代大型含油气盆地的发育奠定了基础。     

浙江雷甸淡水无光珠中球文石的首次确认

球文石（Vaterite)是CaCO3很不稳定的同质多象变体，在自然界里很少出现，通过光学显微镜在淡水无光珠中发现球文石尚属首次，本文研究了淡水无光珠内球文石的显微特征、X射线粉晶衍射特征及显微红外光谱特征，研究结果表明淡水无光珍珠内球文石粉晶衍射由强至弱五个强峰的d值为0.3266,0.2723,0.3553,0.1811,0.2057nm；其红外光谱特征波数为1489，1450,1420,1087,1050,876,830,762,743cm^-1。球文石的存在是影响淡水珍珠品质的主要内在因素之一。     

有机酸对长石溶解度影响的热力学研究

为明确认识有机酸（草酸、醋酸）对长石溶解度及储层次生孔隙发育的影响，本文利用热力学方法，计算了不同温度、酸度下钾长石在含有醋酸根0.05mol/L、草酸0.0055mol/L的溶液中的溶解度及草酸和醋酸对溶液酸度的影响，计算的结果表明醒酸根与铝的络合作用只发生在偏酸性的溶液体系中，并且随温度升高要求酸度增加，实际的络合能力降低，醋酸根的络合作用对长石溶解度的增加作用极及有限，最高时不足一倍；但醋酸能有效地缓冲溶液酸度，从而提高长石溶解度。草酸根与铝的络合作用发生在弱碱性至酸性条件下，温度升高，络合能力增加，络合效应对长石溶解度，草酸根上铝的络合作用发生在弱碱性至酸性条件下，温度升高，络合能力增加，络合效应对长石溶出量的增加最多可达2个数量级以上，草酸的浓度太低无法通过缓冲溶液在较高的酸度下来促进长石的溶解，草酸和醒酸能否促进储层次生孔隙的发育取决于盆地流体的酸度及组成流体的缓冲体系。