2017年春夏季西北太平洋浮游植物的区域差异及其与不同水团的关系   总被引：2，自引：0，他引：2  

林更铭  陈杨航  黄奖  王彦国  叶又茵  杨清良 《海洋学报(英文版)》2020,39(6):107-118

The West Pacific Ocean is considered as the provenance center of global marine life and has the highest species diversity of numerous marine taxa. The phytoplankton, as the primary producer at the base of the food chain,effects on climate change, fish resources as well as the entire ecosystem. However, there are few large-scale surveys covering several currents with different hydrographic characteristics. This study aimed to explore the relationships between the spatio-temporal variation in phytoplankton community structure and different water masses. A total of 630 water samples and 90 net samples of phytoplankton were collected at 45 stations in the Northwest Pacific Ocean(21.0°–42.0°N, 118.0°–156.0°E) during spring and summer 2017. A total of 281 phytoplankton taxa(5 μm) belonging to 61 genera were identified in the study area. The distribution pattern of the phytoplankton community differed significantly both spatially and temporally. The average abundances of phytoplankton in spring and summer were 797.07×10~2 cells/L and 84.94×10~2 cells/L, respectively. Whether in spring or summer, the maximum abundance always appeared in the northern transition region affected by the Oyashio Current, where nutrients were abundant and diatoms dominated the phytoplankton community;whereas the phytoplankton abundance was very low in the oligotrophic Kuroshio region, and the proportion of dinoflagellates in total abundance increased significantly. The horizontal distribution of phytoplankton abundance increased from low to high latitudes, which was consistent with the trend of nutrient distributions, but contrary to that of water temperature and salinity. In the northern area affected by the Oyashio Current, the phytoplankton abundance was mainly concentrated in the upper 30 m of water column, while the maximum abundance often occurred at depths of 50–75 m in the south-central area affected by the Kuroshio Current.Pearson correlation and redundancy analysis(RDA) showed that phytoplankton abundance was significant negatively correlated with temperature and salinity, but positively correlated with nutrient concentration. The phytoplankton community structure was mainly determined by nutrient availability, especially the N:P ratio.  相似文献   

长江口表层沉积物中正构烷烃的高分辨分布特征及有机碳来源解析     

王春禹  姚鹏  赵彬 《海洋学报》2020,42(10):1-13

于2014年3月对长江口及邻近海域的表层沉积物进行了高分辨率采样，分析了沉积物粒级组成、比表面积、总有机碳含量及其稳定碳同位素组成(δ13C)、正构烷烃及其相关分子指标，讨论了此区域沉积有机碳和正构烷烃的高分辨分布特征，并结合基于主成分分析?蒙特卡洛模拟的三端元混合模型，对沉积有机碳的来源进行了定量解析。结果表明，长江口及其邻近海域表层沉积物中总有机碳含量为0.45%±0.16%，近岸泥质区总有机碳含量较高，外海砂质区含量较低。总正构烷烃(C₁₄?C₃₅)的绝对含量和相对于总有机碳的含量分别为(1.42±0.73) μg/g和(0.34±0.21) mg/g。泥质区以长链正构烷烃占优势，具有较强的奇碳优势；砂质区以短链正构烷烃占优势，且具有一定的偶碳优势。长江输入、老黄河口输入、闽浙沿岸小型河流输入和水动力分选等因素制约了正构烷烃的输运和分布特征。模型结果显示此区域沉积有机碳来自海源、土壤和高等植物的混合输入，其中以海源为主，其贡献为42.70%±18.18%，由陆地向外海贡献逐渐升高，其次是土壤和高等植物，其贡献分别为28.99%±15.37%和28.31%±17.12%。在水动力分选作用的影响下，两种陆源有机碳在入海之后的输运过程中存在明显的分异，土壤有机碳主要与细颗粒物结合，并沿闽浙沿岸向南输运，而高等植物来源有机碳则在长江口存在东北方向的输运。  相似文献   

长江三角洲蓝图重绘的基础科学问题:进展与未来研究     

汪亚平  贾建军  杨阳  周亮  冯威  高建华  魏稳  李占海  史本伟  高抒 《海洋科学》2019,43(10):2-12

在全球气候变化和人类活动影响加剧的背景下,作为河口海岸重要子系统的三角洲正在发生快速变化。长江三角洲地处长江入东海交汇处,是中国最重要的经济核心区之一,对邻近区域乃至整个长江经济带经济社会发展都起着重要作用。由于全球变暖、海面上升和强烈人类活动引发了三角洲系统状态转换,因此以往基于恒定系统状态而获得的有关长江三角洲的认识已不能满足未来需求,迫切需要对未来海面变化、极端事件、流域与河口工程影响下的三角洲物质循环条件、物理过程、地貌冲淤演化、源-汇格局调整等科学问题进行深入研究。在三角洲系统行为、未来演化趋势的预测能力建设中,应重视从海面到海底的综合立体观测系统的发展,以获取关键数据;基于三角洲系统的时、空演化特征,建立三角洲本征态和衍生态的谱系理论。未来需针对系统状态转换而调整原先的经济社会发展模式,以便保护自然资源、重建生态系统,更好地支撑长江经济带发展,重绘长江三角洲发展蓝图。  相似文献   

Size and spatial distribution of loess slides on the Chinese Loess Plateau     

Haijun Qiu  Sheng Hu  Xingang Wang  Dongdong Yang  Yanqian Pei  Shuyue Ma 《自然地理学》2020,41(2):126-144

ABSTRACT

The size and spatial distribution of loess slides are important for estimating the yield of eroded materials and determining the landslide risk. While previous studies have investigated landslide size distributions, the spatial distribution pattern of landslides at different spatial scales is poorly understood. The results indicate that the loess slide distribution exhibits a power-law scaling across a range of the size distribution. The mean landslide size and size distribution in the different geomorphic types are different. The double Pareto and inverse gamma functions can coincide well with the empirical probability distribution of the loess slide areas and can quantitatively reveal the rollover location, maximum probability, and scaling exponents. The frequency of loess slides increases with mean monthly precipitation. Moreover, point distance analysis showed that > 80% of landslides are located < 3 km from other loess slides. We found that the loess slides at the two study sites (Zhidan and Luochuan County) in northern Shaanxi Province, China show a significant clustered distribution. Furthermore, analysis results of the correlated fractal dimension show that the landslides exhibit a dispersed distribution at smaller spatial scales and a clustered distribution at larger spatial scales.  相似文献   

More than two hundred and fifty thousand spectroscopic binary or variable star candidates discovered by LAMOST     

Sheng-Bang Qian  Xiang-Dong Shi  Li-Ying Zhu  Lin-Jia Li  Jia Zhang  Er-Gang Zhao  Zhong-Tao Han  Xiao Zhou  Xiao-Hui Fang  Wen-Ping Liao 《天文和天体物理学研究(英文版)》2019,(5)

About 786.4 thousand stars were observed by LAMOST twice or more during the first stage of its spectroscopic survey. The radial velocity differences for about 256 thousand targets are larger than10 km s~(-1) and they are possible spectroscopic binary or variable candidates(SBVCs). It is shown that most SBVCs are slightly metal poorer than the Sun. There are two peaks in the temperature distribution of SBVCs around 5760 K and 4870 K, while there are three peaks in the distribution of the gravitational acceleration at 2.461, 4.171 and 4.621 cm s~(-2). The locations of SBVCs on the [Fe/H]-T, [Fe/H]-log g, log g-T and H-R diagrams are investigated. It is found that the detected SBVCs could be classified into four groups. The first group has higher log g～4.621 and lower T ～ 4870 K which are mainly cool red dwarf binaries. The second group of SBVCs has logg around 4.171 cm s~(-2) that includes binaries and pulsating stars such as δSet and γ Dor variables. The gravitational accelerations of the third group of SBVCs are higher and some of them are below the zero-age main sequence. They may be contact binaries in which the primary components are losing energy to the secondaries in the common envelopes and are at a special stellar evolutionary stage.The last group is composed of giants or supergiants with log g around 2.461 cm s~(-2) that may be evolved pulsating stars. One target(C134624.29+333921.2) is confirmed as an eclipsing binary with a period of 0.65 days. A preliminary analysis suggests that it is a detached binary with a mass ratio of 0.46. The primary fills its critical Roche lobe by about 89%, indicating that mass transfer will occur between the two components.  相似文献   

A PCA approach to stellar abundances I. testing of the method validity     

Wei He  Gang Zhao 《天文和天体物理学研究(英文版)》2019,(10)

The derivation of element abundances of stars is a key step in detailed spectroscopic analysis. A spectroscopic method may suffer from errors associated with model simplifications. We have developed a new method of deriving the various element abundances of stars based on the calibration established from a group of standard stars. We perform principal component analysis(PCA) on a homogeneous library of stellar spectra, and then use machine learning to calibrate the relationship between principal components and element abundances. By testing with spectral libraries S4 N and MILES, we find that our procedure provides good consistency when spectra from a homogeneous set of observations are used, and it could be expanded to stars with quite a wide range of stellar parameters, with both dwarfs and giants. Moreover, we discuss the four key factors that have a significant impact on the results of derived element abundances,including the resolution of the spectra, wavelength range, the signal-to-noise ratio(S/N) of spectra and the number of principal components adopted.  相似文献   

中国土地行政复议案件时空格局演变及宏观驱动机制     

宋洋  朱道林  张立新  杜挺  张晖 《地理科学》2019,39(11):1749-1756

基于2000~2015年中国省（市、区）土地行政复议案件数量、案由与复议结果等数据,定量探究中国土地行政复议案件的分布特征、格局演变与宏观驱动机制。研究表明：中国年度土地行政复议案件数量整体呈连续增加态势,行政相对人复议成功率先下降后上升。土地行政复议案件的空间分布与中国宏观人口-经济格局基本匹配,整体具有东南多西北少的分异特征,以中部主要省份为核心,经历了先向东部沿海、后向西北与西南地区蔓延的演进过程。中国土地行政复议案件的时空格局演变由经济发展水平、城市化水平、产业结构升级、城市建成区面积、土地财政收入状况、土地市场化水平、区位条件等因素共同驱动。  相似文献   

基于线粒体COI和16S rRNA基因的中国沿海相手蟹系统发育研究   总被引：2，自引：0，他引：2  

徐岩  潘红平  阎冰  高霆炜  吴斌  杨明柳 《海洋学报》2019,41(8):63-71

相手蟹科的诸多种类因其形态极其相似成为方蟹总科分类中疑问较多的一个类群。通过对中国沿海相手蟹线粒体COI和16S rRNA基因序列进行分子系统发育分析，结果表明14种相手蟹COI和16S rRNA基因序列之间差异分别为5.7%～14.5%和1.5%～12.1%，均达到了种间差异水平。构建的系统发育树显示，14种相手蟹分别为独立有效物种，但分属于拟相手蟹属和近相手蟹属的4种拟相手蟹和3种近相手蟹，没有分别形成2个独立的支系，而是混合聚成一大支系。而属于螳臂相手蟹属的无齿螳臂相手蟹则首先与属于中相手蟹属的中华中相手蟹聚成一支，再与红螯螳臂相手蟹聚为一大支，表现出与形态分类的不一致。错综复杂的分子系统关系预示着相手蟹类为多系起源，也表明它们之间的种间关系乃至于属间关系尚有诸多问题有待进一步厘定。  相似文献   

IU Cancri:a solar-type contact binary with mass transfer     

Hui-Yu Yuan  Hai-Feng Dai  Yuan-Gui Yang 《天文和天体物理学研究(英文版)》2019,(6)

We present new CCD photometry of the solar-type contact binary IU Cnc, which was observed from November 2017 to March 2018 with three small telescopes in China. BV light curves imply that IU Cnc is a W-type contact binary with total eclipses. The photometric solution indicates that the mass ratio and fill-out factor are q = 4.104 ± 0.004 and f = 30.2% ± 0.3%, respectively. From all available light minimum times, the orbital period may increase at a rate of dP/dt = +6.93(4) × 10~(-7) d yr~(-1), which may result from mass transfer from the secondary component to the primary one. With mass transferring,IU Cnc may evolve from a contact configuration into a semi-detached configuration.  相似文献   

苯并（a）芘诱导下岩虫CYP基因的表达特征     

李婉娟  赵欢  Ba Fuyang  李绍娟  孙秀鹏  杨大佐  周一兵 《海洋学报(英文版)》2019,38(6):46-53

Rapid amplification of cDNA ends(RACE) and real-time polymerase chain reaction(RT-PCR) were carried out to analyze the CYP4 gene expression in polychaete Marphysa sanguinea exposed to benzo[a]pyrene(BaP) in this study. The full length of MsCYP4 cDNA was 2 470 bp, and it encoded 512 amino acids. The deduced amino acid sequence showed 47% identity with CYP4 F from frog Xenopus tropicalis and shared high homology with other known CYP4 sequences. To analyse the role of CYP4 in protecting M. sanguinea from BaP exposure, three BaP groups were established: 0.5, 5 and 50 μg/L. Polychaetes were sampled after 3, 7 and 12 d. At 0.5 μg/L, the effect of BaP on MsCYP4 gene expression increased with time prolonged. MsCYP4 gene expression curve showed Ushaped trend with time in 5 and 50 μg/L BaP groups. Therefore, MsCYP4 gene may play an important role in maintaining the balance of cellular metabolism and protecting M. sanguinea from BaP toxicity.  相似文献