冲绳日本绒螯蟹线粒体DNA 12S rRNA序列的研究

采集日本冲绳源河川和边野古川的日本绒螯蟹样品 ,参考果蝇与蚤状氵蚤线粒体 DNA12 Sr RNA基因片段序列进行了其相同片段的引物设计、PCR扩增及序列测定。结果表明冲绳两河川 4只日本绒螯蟹的碱基序列完全相同 ,为 4 58bp,其 A、T、G、C含量分别为 16 0 bp(34.94 % )、 179bp(39.0 8% )、4 9bp(10 .70 % )、70 bp(15.2 8% ) ,同果蝇与蚤状氵蚤相同基因片段的序列含量相似。     

DFT对Rb+水合团簇及其相关性质的分析

运用密度泛函理论(DFT)在ωB97XD/gen (O、H元素Aug-cc-PVDZ; Rb元素Lanl2DZ)基组水平上研究了[Rb(H_2O)_n]~+(n=1～12)水合团簇的结构和光谱学性质。研究结果表明,通过分析气相和液相中的稳定能以及水合团簇可知,稳定构型出现在8配位的团簇中。第一配位层水分子数为8时形成Rb~+第一近似饱和水合层。此外,拉曼光谱显示[Rb(H_2O)_n]~+(n=1～12)水合团簇中O-H伸缩振动峰随着水分子数增加发生移动和加宽,Rb~+发生水合时,O-H对称和非对称伸缩振动发生红移,随着水合数的增多,频率蓝移。此外,文中对拉曼光谱中O-H振动的频率位置结合团簇结构进行了说明。     

CCD astrometric observations of 2017 VR12, Camillo and Midas

We have observed three near-Earth objects(NEOs), 2017 VR12, Camillo and Midas, during 2018.The observations were made with the 1-m telescope, operated by Yunnan Observatories, over two nights.Their precise astrometric positions are derived from 989 CCD observations. The theoretical positions of asteroids are retrieved from the Jet Propulsion Laboratory(JPL) Horizons System and Institut de M′ecanique C′eleste et de Calcul des ′Eph′em′erides(IMCCE). The positions of three asteroids are measured with respect to stars in the Gaia DR2 star catalog. For 2017 VR12, the means(O-C) of right ascension and declination are -0.090′′and-0.623′′respectively based on the published JPL ephemeris, but the corresponding means(O-C) are 3.122′′and-0.636′′based on the published IMCCE ephemeris. The great difference in declination could be explained by several factors.(1) The degraded CCD images caused by the fast apparent motion of the objects lead to a reduction in positioning accuracy.(2) The poor timing system may introduce systematic errors, especially in the high speed direction.(3) The asteroid may be perturbed by Earth when it approaches the Earth too closely. These astrometric results demonstrate that the centroid centering method can reduce the dispersion of non-Gaussian images as compared with the PSF modeling method.For Camillo and Midas, the astrometric results are consistent based on the two ephemerides. Implementing a high-precision timing system, and analyzing some astronomical effects and geometric distortions in CCD images should be carefully considered in future works.     

Effects of pulsed nutrient inputs on phytoplankton assemblage structure and blooms in an enclosed coastal area

The response of phytoplankton assemblage structure to terrestrial nutrient inputs was examined for the Gulf of Kalloni in the Northern Aegean Sea, a productive semi-enclosed coastal marine ecosystem. The study was focused on a typical annual cycle, and emphasis was placed on the comparative analysis between blooms developing after significant nutrient inputs from the watershed, and naturally occurring blooms. Baseline information was collected on a monthly basis from a network of stations located in the oligotrophic open sea and the interior and more productive part of the embayment. Intensive sampling was also carried out along a gradient in the vicinity of a river which was the most important source of freshwater and nutrient input for the Gulf. Phytoplankton assemblage structure was analyzed from 188 samples using diversity indices (Shannon and Average Taxonomic Distinctness), multivariate plotting methods (NMDS), multivariate statistics (PERMANOVA), and canonical correspondence analysis (CCA). Three characteristic assemblages were recognized: (1) an autumn assemblage developed under nutrient depleted conditions, having low diversity due to the dominance of two small diatoms, (2) a winter bloom of the potentially toxic species Pseudo-nitzschia calliantha occurring immediately after a nutrient peak and characterized by very low diversity, and (3) a naturally occurring early summer bloom of centric diatoms with relatively high diversity. The results of the study support the view that moderate nutrient inputs may have a beneficial effect on the functioning of coastal ecosystems, stimulating the taxonomic diversity through the growth of different taxonomic groups and taxa. On the other hand, a sudden pulse of high nutrient concentrations may greatly affect the natural succession of organisms, have a negative effect on the diversity through the dominance of a single species, and can increase the possibility of a harmful algal bloom development.     

日本(虫寻)和底栖短桨蟹线粒体DNA 12SrRNA基因序列的初步研究

以相应引物对日本和底栖短桨蟹的线粒体 DNA1 2 S r RNA基因片段进行了 PCR扩增和序列测定 ,分析比较了 2种间序列差异。结果表明 :日本 1 2 S r RNA基因片段长度为 41 4 bp,底栖短桨蟹为 41 5bp,2种的 A,T,G,C含量分别为 1 51 bp(36.47% ) ,1 53bp(36.96% ) ,43bp(1 0 .39% ) ,67bp(1 6.1 8% )和 1 50 bp(36.1 4 % ) ,1 55bp(37.35% ) ,44bp(1 0 .60 % ) ,66bp(1 5.90 % )。 2种间共出现了 3个碱基的缺失 /插入和 38bp的序列差异 ,其碱基转换与碱基颠换比约为 2 .1 7。     

On the nature of the Galactic nebula We 1–12

In 1977, Weinberger published a list of 12 new extended possible planetary nebulae (PNe). Whereas, because of their characteristic morphology and/or the presence of a blue central star, almost all of them could easily be suspected to be genuine planetary nebulae, one object (No. 12) captivated because of its unusually bright central star. This find prompted Kaler & Feibelman to question the PN nature of this object (We 1–12) on the basis of IUE spectra. A definite conclusion could, however, not be drawn by them; thus, until now, the real nature of We 1–12 remained unsolved. For the first time, a spectral investigation of both the central star and the nebula is presented in this paper. It definitely shows that this intriguing object is an (isolated) H  ii region and its central star, as previously assumed, is an early B star which serves as the ionizing source. We 1–12, a part of which is coincident with a weak IRAS point source, is at a distance of 2–2.6 kpc and is reddened by E ( B − V )=0.6–0.8 mag.     

恒星形成区GGD12-15的近红外观测

给出恒星形成区GGD12-15的宽波段JHK和窄波段H2v=1-0S(1)近红外成像观测．观测图像揭示了致密的年轻红外星团和与红外源成协的红外星云，并发现了以H2发射结表征的星团外流活动．大多数红外点源在光学波段不可见；对76颗红外点源的JHK′测光结果显示，有32颗具有红外超，其中5颗表现原恒星特征，表明分子云中的恒星形成活动很活跃．以B8光谱型作为大质量星分界，由色星等图估计出大质量星所占星团比例为-10％～26％．GGD12—15星团的K′星等分布的峰值位于15.0mag，并在13．0mag-16．0mag平坦分布；[H—K′]色分布的峰值出现在-0．7mag，在此以上更红的星团成分占70％．在GGD12-15区新发现的氢分子发射结集中在星团中心领域，其空间分布明显与剧烈的恒星形成活动相关；有5个发射结位于分子外流的中心区域，暗示其激发可能与分子外流同源．     

Reform of Teacher Education: An Opportunity for Geographers

Abstract

This paper focuses on the context and major efforts designed to reform teacher education in the nation's universities. An overview of systems governing and impacting teacher education is provided, with focus on the issues and conflicting forces that form the context within which teacher education-and geography education—find themselves. The paper concludes with a discussion of general trends in education reform and renewal and leadership opportunities open to geographers.     

由地基微波辐射计测量得到的北京地区水汽特性的初步分析

首先对比分析了三种测量水汽技术(地基微波辐射计、探空、GPS)之间的差异, 得到地基微波辐射计与探空的差值为0.281cm, GPS与探空的差值为0.728 cm, 地基微波辐射计与GPS的差值为0.322 cm。接着就地基12通道微波辐射计测量得到的水汽总量 (简称PWV), 分析了北京地区水汽在四个季节中的日变化特征。秋季日变化差为0.162 cm, 冬季日变化差为0.130 cm, 春季日变化差为0.229 cm, 夏季日变化差为0.276 cm。另外, 北京地区四个季节中水汽最大值/最小值出现频率最高的时间段呈现一定的特征。即四个季节中在北京时间00:00到00:59和23:00到23:59这两个时间段中, 水汽出现最大值/最小值的概率较其他时间段都高, 其中冬季在北京时间10:00到10:59之间出现最小值的概率最高。水汽总量PWV每小时变化率在四个季节中都存在这样的现象: 出现正的水汽总量PWV每小时变化率的百分比与出现负的水汽总量PWV每小时变化率的百分比相当, 几乎都为50%。最后就水汽与温度相关性做了分析, 分别得到四个季节中各个小时水汽与温度的相关系数, 结果显示各个小时水汽与温度的相关性在四个季节中, 除了夏季从北京时间09:00到22:00为负相关外, 其他时间段内都为正相关。而且各个小时水汽与温度的相关系数都按照秋、春、 冬、夏的顺序递减。