冀豫浙中小企业集群中的创业机制实证研究   总被引：3，自引：0，他引：3  

杨静文  朱宪辰 《地域研究与开发》2005,24(2):34-37

理论和实证研究表明,企业集群中存在比较完善的创业机制;另一方面,正是由于创业机制的存在,企业集群才能够得以发育成长。文章通过对冀豫浙3个中小企业集群实地调研分析,证实了企业集群发育过程中创业机制的存在以及创业机制对企业集群发育成长的重要作用。认为建立健全创业机制是促进企业集群发育、成长和升级的有效方法。  相似文献   

斑尾复鰕虎鱼群体的形态学比较   总被引：3，自引：0，他引：3  

高天翔  孙希福  宋娜 《中国海洋大学学报(自然科学版)》2009,39(1)

对采自丹东、大连、东营、青岛、赣榆、舟山、厦门7个斑尾复鰕虎鱼群体的可量性状和可数性状进行了主成分分析、聚类分析、判别分析和单因子方差分析.主成分分析和聚类分析结果显示东营和赣榆群体为一组,而其它群体为另一组.2组差异极为显著.主成分分析构建了4个主成分,其贡献率分别为41.30%,8.92%,8.08%和7.31%,累计贡献率为65.60%.第一主成分主要受尾柄长/尾柄高、体高/体长、头长/体长和吻至背鳍起点/体长的影响.判别分析也可将两组群体分开,东营和赣榆组与另一组没有误判,对于样本所属海域的判别,其中东营为100%,最低为青岛群体66.7%,综合判别率为85.5%;选取贡献较大的14个特征值建立判别公式,利用判别公式计算各群体的差别准确率为62.1%～100%.对形态特征参数进行单因子方差分析,计算差异系数,根据Mayr等提出的75%规则,认为两组群体已达到亚种水平,而两组群体内的形态差异为种内不同群体间的差异.  相似文献   

NGC 1624 (OCl 403, Cr 53) – A very young open cluster     

S. Sujatha  G. S. D. Babu 《Astrophysics and Space Science》2006,305(4):399-410

We present the first CCD photometric UBVRI observations of the not-so-well-studied open cluster NGC 1624 (OCl 403, Cr 53; α₂₀₀₀ = 04 h 40 m 36 s; δ₂₀₀₀ = + 50^˚ 27^′ 42″ Trumpler class = I 2 p N). This cluster was observed on 01 February 2004 with the 2 m Himalayan Chandra Telescope at Hanle using a LN2 cooled 2k × 2k CCD. The cluster presents differential reddening with E(B-V) values ranging from 0.70 to 0.90 mag, which could be attributed to the presence of the HII region wherein the cluster is embedded. It is found to be at a distance of 6.025 ± 0.5 kpc and the age of this cluster is estimated to be ∼3.98 × 10⁶ years. In view of these parameters, it can be considered as a young enough cluster located in the direction of the Perseus constellation with the galactic coordinates of l = 155^˚.35 and b = + 02 ^˚.58. Thus it could also be used as a suitable candidate for tracing the Outer Perseus spiral arm of our Galaxy. The initial mass function slope is derived as 1.65 ± 0.25 by applying the corrections for field star contamination and data incompleteness. This is in good agreement with the Salpeter value within the limits of errors.  相似文献   

Variability of sediment diatom assemblages in an upland,wind-stressed lake (Loch Fleet,Galloway, S.W. Scotland)     

N. J. Anderson 《Journal of Paleolimnology》1990,4(1):43-59

The variability of diatom distribution in an acidified, upland wind-stressed lake (Loch Fleet, Galloway, S. W. Scotland) was assessed by analysis of 28 surface sediment samples and 11 cores. Correspondence analysis (CA) and cluster analysis were used to illustrate the variability of the surface sediment and core samples. There was reasonable uniformity of taxa in most of the surface sediment samples, although 7 samples, as indicated by both CA and cluster analyses were atypical. Most cores recorded clearly the acidification of the lake, although percentages of individual taxa varied up to 20% between cores. Two cores had old, preacidification diatom assemblages (of indeterminate age) close to the sediment surface. These old sediments were probably the source of the re-worked diatoms found in the atypical surface sediment assemblages. Diatom trends, as CA ordinations and pH profiles, were less variable than the surface sediment assemblages. It is argued that non-uniform sediment accumulation rates and diatom deposition cause variability in surface sediment diatom samples. This variability may be reduced in core profiles by homogenization during further resuspension/deposition cycles and burial. Cores, and the associated time component they offer, may be useful in assessing the variability of surface sediment assemblages.  相似文献   

A multivariate statistical study of copper mineralization in the central section of Mosaboni Mine, Eastern Singhbhum, India     

A. K. Saha  S. N. Sarkar  Swapna Basu  Dhruba Ganguly 《Mathematical Geology》1986,18(2):215-235

A multivariate statistical analysis was carried out with log-transformed values of Cu, Ni, Co, Pb, Zn, Ag, Cr, Mn, Ca, and Sr in several sets of samples collected across the mineralized base metal zone in sheared soda granite, feldspathic schist, and chlorite schist from the central section of Mosaboni Mine of the famous Singhbhum Copper Belt of eastern India. Linear correlation coefficient matrices of two sets of ore samples (>0.5% Cu)—one from levels 18 and 21 and the other from levels 25 and 28—indicate two well-defined and distinct clusters comprising Cu, Ni, Co, Pb, and Zn on one hand and Ca, Sr, and Mn on the other. Varimax-rotatedR-mode factor analysis of two above-noted sample sets, taken along with available geologic information, indicates that over 80% of the variability in data matrices for 9–10 elements can be accounted for by four distinct processes: (a) an early phase of copper mineralization which apparently replaced Mn, Ca, and Sr in the host rock; (b) a silicate-cum-oxide phase of crystallization/recrystallization of host rock; (c) remobilization of sulfide-forming ore elements (Cu, Ni, Co, Pb, and Zn); and (d) a phase of mineralization of Ag which appears to have replaced Cr, Ca and Cu. Process (c) was quantitatively most important. Factor score studies are suggestive of preferred introduction of Ni, Co, Pb, and Zn along central parts of preexisting copper-mineralized zones.  相似文献   

恒星形成区GGD12-15的近红外观测     

房敏  姚永强 《天文学报》2004,45(1):1-15

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．  相似文献   

Interpreting the colour–magnitude diagrams of open star clusters through numerical simulations     

Jasonjot Singh Kalirai  Monica Tosi 《Monthly notices of the Royal Astronomical Society》2004,351(2):649-662

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Numerical simulations of the Hyades dynamics and the nature of the moving Hyades cluster     

Ya. O. Chumak  A. S. Rastorguev  S. J. Aarseth 《Astronomy Letters》2005,31(5):308-314

We present our numerical simulations of the dynamical evolution of the Hyades open cluster. The simulations were performed usinga modified NBODY6 algorithm that included tidal forces and a realistic orbit of the cluster in a gravitational field described by the Miyamoto-Nagai potential. Our goal was to study the nature of movingclu sters. We show that the stars that were earlier cluster members could be later identified within a sphere of 50 pc in diameter around the Sun. The number of such stars for the chosen initial mass and virial radius of the cluster does not exceed ten. The maximum space velocity of these stars relative to the core of the current cluster does not exceed 3 km s^?1. Our numerical simulations confirm the assumption that some of the moving clusters near the Sun could consist of stars that have escaped from open clusters in the course of their dynamical evolution.  相似文献   

疏散星团M11的研究：1.自行测定与成员研究     

束成钢  赵君亮  田凯平 《天文学报》1996,37(3):294-302

本文利用中国科学院上海天文台４０厘米双筒天体照相仪所拍摄得的１０对底片（历元差１６─７０年），经ＰＤＳ测量仪测量，共确定了疏散星团Ｍｌｌ天区８７２颗恒星的相对自行，其中８５％以上恒星的自行测定精度好于±０″．１／百年．利用所测得的相对自行和新的数学模型，确定了不同星等组恒星的分布参数并计算了团中心距ｒ≤２５＇内７８５颗恒星的成员概率，其中成员概率大于０．７的恒星共有５４１颗．详细的讨论表明，新方法不仅在理论上更为严格，实用上也是可行的，可以使星团成员确定取得更为合理的结果．  相似文献   

应用灰色聚类分析部署地质找矿工作     

燕长海 《河南国土资源》1995,(1)

本文以汝阳南部铅锌矿成矿预测勘查过程中预测出的３２个含矿单元为例，阐述了如何用灰色系统理论中的灰色聚类分析方法定量地划分预测靶区类别，合理、客观地部署铅锌矿地质找矿工作，取得了令人满意的结果。  相似文献