小黄鱼(Pseudosciaena polyactis)形态性状与体质量的相关性及通径分析

为了研究野生小黄鱼(Pseudosciaena polyactis)繁殖后代的形态性状对体质量的影响作用,以随机采集的729尾4.5月龄小黄鱼为研究对象,对每尾个体的体质量(g)和8个形态性状(cm):全长(X1)、体长(X2)、头长(X3)、躯干长(X4)、尾部长(X5)、尾柄长(X6)、尾柄高(X7)和体高(X8)进行准确测定,运用相关分析、多元回归分析和通径分析方法,分别计算性状间的相关系数、构建形态性状与体质量的多元回归方程,获得了通径系数和决定系数,进行了养殖小黄鱼的形态性状对体质量的影响研究。结果显示,8个形态性状与体质量的相关系数均达到极显著水平(P0.01);通径分析中,4个形态性状对体质量的通径系数达到极显著水平(P0.01),它们是影响体质量的重要指标,其中体长(通径系数:0.589)对体质量的直接影响最大。应用逐步多元回归分析建立了以体质量为因变量(Y),体长(X2)、躯干长(X4)、尾柄高(X7)和体高(X8)为自变量的回归方程:Y=–32.377+3.064X2–1.511X4+14.285X7+4.438X8。模型等式中形态性状与体质量的相关指数R2=0.927,说明所选性状是影响体质量的主要形态性状。以上分析结果为小黄鱼的选育测量指标的确定提供了理论依据。     

新一代区域海-气-浪耦合台风预报系统

依托国家重点基础研究（973）计划项目"上层海洋对台风的响应和调制机理研究",中国气象局上海台风研究所联合国家海洋局的相关单位,通过实施近海台风的外场观测科学试验、加强台风边界层（特别是海气相互作用）物理过程诊断分析及参数化方案等的研究,建立并改进了台风强度预报的海-气-浪耦合预报模式系统,并在此基础上发展了台风强度的集合预报技术,在历史典型台风个例和2016-2017年台汛期的业务化测试中表现出良好的预报性能。     

卫星导航欺骗干扰技术研究进展

在卫星导航应用越来越重视对抗与防护的背景下,梳理了卫星导航欺骗干扰技术的发展现状。讨论了欺骗干扰的原理和分类,介绍了欺骗干扰对接收机的影响、转发式欺骗干扰定位模型、新型渐变自同步欺骗干扰三个方向的研究进展,最后展望了卫星导航欺骗干扰技术下一步的发展方向。     

基于db7小波的活体浮游植物荧光识别分析技术研究

通过小波变换可对信号的不同频率成分进行分解,为弱信号特征提取提供了有效途径。通过db7小波对分属7个门32个属的43种浮游植物的三维荧光光谱进行分析,后经Bayes判别分析选择小波分解后的第三层尺度分量作为最佳荧光识别特征谱,并通过系统聚类法将最佳特征谱在不同的条件下聚类进而得到门、属上的标准谱库。基于此,运用多元线性回归辅以非负最小二乘法建立浮游植物三维荧光光谱识别技术。利用该技术对4128个单种浮游植物样品和636个混合浮游植物样品进行识别分析。单种浮游植物样品在属水平上的识别正确率为75%,门水平上的识别正确率为95%;浮游植物混合样品中的优势种在属水平上的识别正确率为83%,门水平上的识别正确率为91%。结果表明:该技术可以实现对浮游植物的快速准确识别。     

绿鳍马面鲀重复发育雄性生殖腺结构与发育组织学观察

采用常规石蜡切片、HE组织染色法研究了性成熟绿鳍马面鲀雄性生殖腺结构和发育组织学。结果表明,性成熟绿鳍马面鲀精巢从外形上明显分为上、下两段,上段为生精部,下段为贮精囊。生精部分为2支,呈黄色、长条状;生精部为典型的小叶型结构;精小叶间有间质(Leydig)细胞。其生精部的发育历程可分为重复发育Ⅲ期、精子形成Ⅳ期、精子成熟Ⅴ期和退化吸收Ⅵ期。贮精囊位于精巢的后方并通过壶腹与生精部相连,贮精囊为椭圆形,白色不分支,其组织结构与贮存精子功能相适应,由许多被结缔组织分开的管状囊腔组成;贮精囊组织学变化与生精部周期性的变化相关,又有相对的独立性,也有周期发育,可分为恢复期、生殖期和退化期。     

关于确保甘肃省祁连山生态保护红线落地并严守的科技支撑建议

祁连山是中国西部重要生态安全屏障,是国家重点生态功能区,其生态保护与治理一直受到国家、地方政府和当地居民高度关注。目前,在祁连山的生态保护工作中,缺乏对现状基础数据的全面掌握,区域经济发展与生态环境保护矛盾突出,生态环境综合监测系统不完备,生态补偿机制推进实施缺乏创新。在全面梳理祁连山目前存在的重大生态问题的基础上,提出了祁连山生态保护红线落地并严守的建议,包括加快开展祁连山综合科学考察、完善并落实开展生态补偿机制、探索以正面清单为导向的协调发展模式、促进生态安全与地方经济社会可持续发展相协调、进一步实施重大配套政策、完善保障支撑体系等。     

小叶锦鸡儿(Caragana microphylla)群落蒸散发模拟

基于2016、2017年生长季原位气象监测数据,利用Shuttleworth-Wallace(S-W)模型模拟了科尔沁沙地主要固沙植物小叶锦鸡儿(Caragana microphylla)群落的蒸散发,对蒸散组分进行了拆分,并利用涡度相关系统对模拟蒸散发值进行了验证。结果表明:2016、2017年生长季小叶锦鸡儿群落蒸散发量分别为345.4、325.2 mm,土壤蒸发量分别为93.8、83.8 mm,植被蒸腾量分别为251.6、241.4 mm,土壤蒸发占总蒸散发分别为27.2%、25.8%。30 min尺度上模拟值与实测值一致性较高,模拟精度大体表现为晴天>阴天>雨天。持续干旱和降水后,小叶锦鸡儿蒸腾耗水规律明显不同,持续干旱时期小叶锦鸡儿保持较低的蒸腾耗水,且具有明显的"午休"现象,连续降水后小叶锦鸡儿"午休"消失,蒸腾耗水增强。饱和水汽压差是影响小叶锦鸡儿蒸散发的主要因子。     

Methods Comparison for Microsatellite Marker Development： Different Isolation Methods, Different Yield Efficiency

Microsatellite markers have become one kind of the most important molecular tools used in various researches. A large number of microsatellite markers are required for the whole genome survey in the fields of molecular ecology, quantitative genetics and genomics. Therefore, it is extremely necessary to select several versatile, low-cost, efficient and time- and labor-saving methods to develop a large panel of microsatellite markers. In this study, we used Zhikong scallop (Chlamys farreri) as the target species to compare the efficiency of the five methods derived from three strategies for microsatellite marker development. The results showed that the strategy of constructing small insert genomic DNA library resulted in poor efficiency, while the microsatellite-enriched strategy highly improved the isolation efficiency. Although the mining public database strategy is time- and cost-saving, it is difficult to obtain a large number of microsatellite markers, mainly due to the limited sequence data of non-model species deposited in public databases. Based on the results in this study, we recommend two methods, microsatellite-enriched library construction method and FIASCO-colony hybridization method, for large-scale microsatellite marker development. Both methods were derived from the mi-crosatellite-enriched strategy. The experimental results obtained from Zhikong scallop also provide the reference for microsatellite marker development in other species with large genomes.     

Impacts of soil fauna on litter decomposition at different succession stages of wetland in Sanjiang Plain, China

Litter decomposition is the key process in nutrient recycling and energy flow. The present study examined the impacts of soil fauna on decomposition rates and nutrient fluxes at three succession stages of wetland in the Sanjiang Plain, China using different mesh litterbags. The results show that in each succession stage of wetland, soil fauna can obviously increase litter decomposition rates. The average contribution of whole soil fauna to litter mass loss was 35.35%. The more complex the soil fauna group, the more significant the role of soil fauna. The average loss of three types of litter in the 4mm mesh litterbags was 0.3–4.1 times that in 0.058mm ones. The decomposition function of soil fauna to litter mass changed with the wetland succession. The average contribution of soil fauna to litter loss firstly decreased from 34.96% (Carex lasiocapa) to 32.94% (Carex meyeriana), then increased to 38.16% (Calamagrostics angustifolia). The contributions of soil fauna to litter decomposition rates vary according to the litter substrata, soil fauna communities and seasons. Significant effects were respectively found in August and July on C. angustifolia and C. lasiocapa, while in June and August on C. meyeriana. Total carbon (TC), total nitrogen (TN) and total phosphorus (TP) contents and the C/N and C/P ratios of decaying litter can be influenced by soil fauna. At different wetland succession stages, the effects of soil fauna on nutrient elements also differ greatly, which shows the significant difference of influencing element types and degrees. Soil fauna communities strongly influenced the TC and TP concentrations of C. meyeriana litter, and TP content of C. lasiocapa. Our results indicate that soil fauna have important effects on litter decomposition and this influence will vary with the wetland succession and seasonal variation. Foundation item: Under the auspices of State Key Development Program for Basic Research of China (No. 2009CB421103), Key Program of National Natural Science Foundation of China (No. 40830535/D0101), Knowledge Innovation Programs of Chinese Academy of Sciences (No. KZCX2-YW-BR-16, KSCX2-YW-N-46-06)     

The 1978 outburst of the recurrent nova WZ Sagittae

We give the results of photographic observations of the recurrent nova WZ Sge during its 1978 outburst, between December 5 and 25, using the double astrograph of Beijing Observatory. We discuss the observed properties and calculate the total energy released during the outburst to be about 1.07 (+40) erg. We estimate that the next outburst will occur around the year 2011.