排序方式： 共有23条查询结果，搜索用时 15 毫秒
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东海原甲藻cDNA文库构建及尝试性EST分析 总被引：2，自引：0，他引：2
东海原甲藻(Prorocentrumdonghaiense)是中国沿海频繁发生的大规模赤潮的原因种之一,大规模分离鉴定东海原甲藻功能基因是理解东海原甲藻赤潮形成过程和机理的重要基础。取对数生长期藻体,经微量总RNA抽提、cDNA合成、cDNA扩增和克隆等步骤,构建了东海原甲藻cDNA文库并进行了尝试性表达序列标签分析。从含有约5000个转化子的文库中随机取150个测序,获得126条EST序列。经网上BlastN及BlastX分析,共发现11个是已知功能的基因的标签。这些基因与东海原甲藻生长发育、物质转换和能量代谢相关。 相似文献
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Rui-Xiang Chang Cheng-Gang Shu Jin-Liang Hou Shanghai Astronomical Observatory Chinese Academy of Sciences Shanghai CAS-Peking University Joint Beijing Astronomical Center Beijing 《中国天文和天体物理学报》2002,2(3)
Based on a physical treatment of the star formation law similar to that given by Efstathiou, we have improved our two-component chemical evolution model for the Milky Way disk. Two gas infall rates are compared, one exponential, one Gaussian. It is shown that the star formation law adopted in this paper depends more strongly on the gas surface density than that in Chang et al. It has large effects on the history of star formation and gas evolution of the whole disk. In the solar neighborhood, the history of chemical evolution and star formation is not sensitive to whether the infall rate is Gaussian or exponential. For the same infall time scale, both forms predict the same behavior for the current properties of the Galactic disk. The model predictions do depend on whether or not the infall time scale varies with the radius, but current available observations cannot decide which case is the more realistic. Our results also show that it would be inadequate to describe the gradient evolution along the Gala 相似文献
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在实验室条件下,研究了温度对赤潮异弯藻生长速率、细胞体积和生化组成的影响。结果表明,赤潮异弯藻在10~30℃之间均能正常生长,25℃时生长速率最高,25℃为其最适生长温度;赤潮异弯藻的细胞体积随着温度的升高大致呈逐渐减小的趋势,10℃时细胞体积最大(823.89μm3),25℃时细胞体积最小(387.98μm3)。进一步分析表明,赤潮异弯藻生长速率与细胞体积(对数值)呈显著的负相关关系(P0.05)。在10~25℃之间,赤潮异弯藻单个细胞的碳、氮含量随着温度的升高呈逐渐减少的趋势,其单位体积细胞的碳、氮含量却呈单峰变化(15℃时结果为峰值)现象;叶绿素a含量在单个细胞和单位体积细胞两个层次上随温度的变化趋势一致,即其在整个温度区间内随着温度的升高均呈逐渐增加的趋势。赤潮异弯藻细胞C∶Chl a和N∶Chl a随着温度的升高呈先减小后增加的趋势,均在10℃时最大,在25℃时最小。 相似文献
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Seismic data processing typically deals with seismic wave reflections and neglects wave diffraction that affect the resolution. As a general rule, wave diffractions are treated as noise in seismic data processing. However, wave diffractions generally originate from geological structures, such as fractures, karst caves, and faults. The wave diffraction energy is much weaker than that of the reflections. Therefore, even if wave diffractions can be traced back to their origin, their energy is masked by that of the reflections. Separating and imaging diffractions and reflections can improve the imaging accuracy of diffractive targets. Based on the geometrical differences between reflections and diffractions on the plane-wave record; that is, reflections are quasi-linear and diffractions are quasi-hyperbolic, we use plane-wave prediction filtering to separate the wave diffractions. First, we estimate the local slope of the seismic event using planewave destruction filtering and, then, we predict and extract the wave reflections based on the local slope. Thus, we obtain the diffracted wavefield by directly subtracting the reflected wavefield from the entire wavefield. Finally, we image the diffracted wavefield and obtain high-resolution diffractive target results. 2D SEG salt model data suggest that the plane-wave prediction filtering eliminates the phase reversal in the plane-wave destruction filtering and maintains the original wavefield phase, improving the accuracy of imaging heterogeneous objects. 相似文献
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Rui-Xiang Xie Min Wang Yi-Hua YanNational Astronomical Observatories Yunnan Observatory Chinese Academy of Sciences Kunming National Astronomical Observatories Chinese Academy of Sciences Beijing 《中国天文和天体物理学报》2005,(1)
A rare Type I-like noise storm was observed with the solar radio spectrometers (1.0-2.0 GHz and 2.60-3.8 GHz) at National Astronomical Observatories of China (NAOC) on September 23, 1998. We concentrate on checking the Type I-like noise storm occurred in the decay phase of a Type Ⅳ radio burst. This noise storm consists of many Type I bursts and isolated Type Ⅲ or Type Ⅲ pair bursts. It has a bandwidth of ≤0.5 GHz. The duration of each Type I burst is of the order of 100-300 ms. The total duration is greater than 11 minutes. The circular polarization 相似文献
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通过对目前生态动力学模型的总结和综合，以生态系统中氮、磷营养盐循环为主线，建立了适用于海洋围隔浮游生态系统的多变量的营养盐迁移-转化动力学模型。该模型包括浮游植物、浮游动物、溶解无机态营养盐、溶解有机态营养盐和生物碎屑5个模块，涉及溶解无机氮、磷酸盐、溶解有机氮、溶解有机磷、浮游植物、浮游动物和生物碎屑7个状态变量。利用2002年8月末莱州湾围隔生态实验数据进行了模型的验证工作，成功地模拟了富加营养盐条件下围隔浮游生态系统中氮、磷营养盐生物化学迁移-转化过程，并通过灵敏度分析探讨了模型主要状态变量对参数改变的灵敏程度。 相似文献
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