几种海藻粗多糖的理化性质及结构特征分析     

侯萍  马军  陈燕  裴志胜  赵静  叶细鹏  姜芳燕  黄海 《热带海洋学报》2018,37(2):55-62

主要采用傅里叶红外光谱(fourier transform infrared spectroscopy, FTIR)、气相色谱(gas chromatography, GC)和凝胶渗透色谱(gel permeation chromatography, GPC)方法对5种海藻粗多糖的单糖组成、官能团、分子量进行了初步分析。结果显示5种海藻粗多糖均含有木糖和岩藻糖, 其中南方团扇藻多糖含有较为丰富的山梨糖, 属于大分子量均一性多糖, 而孔石莼多糖分子量分布较宽, 均一性较差。红外光谱分析结果表明, 5种粗多糖均为酸性多糖, 棒叶蕨藻、琼枝麒麟菜和匍枝马尾藻多糖具有明显的硫酸基团吸收峰, 琼枝麒麟菜多糖存在呋喃糖和吡喃糖, 并且吡喃糖苷键可能存在β和α两种类型。明胶氯化钡实验结果指出南方团扇藻多糖的硫酸基团含量为38.43%(±2.38%), 明显高于其他几种海藻多糖, 而棒叶蕨藻多糖的硫酸基团含量最低, 仅为8.92%(±1.04%)。  相似文献   

Submarine landslides on the north continental slope of the South China Sea     

Weiwei Wang  Dawei Wang  Shiguo Wu  David Völker  Hongliu Zeng  Guanqiang Cai  Qingping Li 《中国海洋大学学报(英文版)》2018,17(1):83-100

Recent and paleo-submarine landslides are widely distributed within strata in deep-water areas along continental slopes, uplifts, and carbonate platforms on the north continental margin of the South China Sea (SCS). In this paper, high-resolution 3D seismic data and multibeam data based on seismic sedimentology and geomorphology are employed to assist in identifying submarine landslides. In addition, deposition models are proposed that are based on specific geological structures and features, and which illustrate the local stress field over entire submarine landslides in deep-water areas of the SCS. The SCS is one of the largest fluvial sediment sinks in enclosed or semi-enclosed marginal seas worldwide. It therefore provides a set of preconditions for the formation of submarine landslides, including rapid sediment accumulation, formation of gas hydrates, and fluid overpressure. A new concept involving temporal and spatial analyses is tested to construct a relationship between submarine landslides and different time scale trigger mechanisms, and three mechanisms are discussed in the context of spatial scale and temporal frequency: evolution of slope gradient and overpressure, global environmental changes, and tectonic events. Submarine landslides that are triggered by tectonic events are the largest but occur less frequently, while submarine landslides triggered by the combination of slope gradient and over-pressure evolution are the smallest but most frequently occurring events. In summary, analysis shows that the formation of submarine landslides is a complex process involving the operation of different factors on various time scales.  相似文献   

[已撤稿] 三亚珊瑚礁珊瑚藻种类及其空间特征与环境因子的关系     

雷新明  黄晖  练健生  张浴阳  杨剑辉 《热带海洋学报》2019,38(3):79-88

珊瑚藻是珊瑚礁生态系统中重要的功能性群体。2010年通过水肺潜水分析了三亚珊瑚礁区的珊瑚藻种类组成和丰度, 以及群落空间特征与环境因子的关系。共鉴定出3科10属25种珊瑚藻, 其中珊瑚藻科占优势地位。三亚珊瑚礁区的珊瑚藻优势种分别为叉节藻Amphiroa ephedraea、拟中叶藻Mesophyllum simulans、串胞新角石藻Neogoniolithon fosliei、中叶藻M. mesomorphum、圆锥呼叶藻Pneophyllum conicum、孔石藻Porolithon onkodes和布氏水石藻Hydrolithon boergesenii。基于多元统计的分析结果, 将调查采样站位分为近岸型和离岸型2个主要集群, 其中近岸型的珊瑚藻种类以浊度、沉积速率(0~63μm)和悬浮物耐受种类为主, 离岸型则以光依赖-沉积物敏感种类为主。以珊瑚藻种类组成和丰度为基础的群落相似性分析结果表明, 其空间变异处于显著性水平。生物与非生物变量的相关分析结果表明, 最佳两变量组合(浊度和盐度)显著影响三亚珊瑚礁区2种类型调查站位中的珊瑚藻集合。在同一个研究站位, 因受干扰程度不同, 深水处的珊瑚藻的覆盖率比浅水处高。分析结果表明, 在三亚独特的珊瑚礁区中, 自然或人为的物理干扰因素都对调节珊瑚藻群落结构非常重要。  相似文献   

海南岛沿岸海域砗磲资源调查及保护前景展望   总被引：1，自引：0，他引：1  

崔丹  王辉  刘君  陈家炜  刘合露  张海滨 《海洋通报》2019,38(5):527-532

砗磲是珊瑚礁海域的重要贝类之一,对维护珊瑚礁生态系统平衡起着重要作用。然而,近年来海洋的大力开发和利用给我国沿海砗磲资源造成严重威胁。本研究通过截线样带法对海南岛沿岸海域砗磲的种类和分布进行实地调查,结果表明,海南岛沿岸海域砗磲覆盖度呈现南北差异,东南沿岸海域砗磲覆盖度明显高于西北沿岸海域,这种差异可能是由自然因素和人为因素共同造成。调查海域共发现3种砗磲:诺亚砗磲(Tridacna noae)最多,占砗磲样品总数的58.6%;其次是番红砗磲(T. crocea),占34.3%;鳞砗磲(T. squamosa)最少,仅占7.1%。海洋管理部门应该加强对砗磲多样性的保护力度,合理开发和可持续利用并重,从而有效保护砗磲、珊瑚礁乃至海洋生态系统。  相似文献   

Apsidal precession of the outer solar planetary orbits due to the pioneer anomaly     

《New Astronomy》2017

Despite the now common position that the Pioneer anomaly is not a real gravitational effect but an effect due to the on-board thermal recoil forces – for curiosity’s sake, we here take the suggestion of Nyambuya (2015) where it has been assumed that the Pioneer anomaly – can, in-principle, be attributed to a gravitational effect due to these spacecrafts accreting some material from a rarefied Interplanetary Medium (IPM) in the domain where the Pioneer anomaly has manifested [20 AU ≲ r ≲ 70 AU]. If this assumption is correct, then, the expected Pioneer acceleration of these spacecrafts maybe much smaller than the Pioneer acceleration to cause as noticeable apsidal precession of the outer Solar planets Uranus, Neptune and Pluto, thus making it difficult to rule-out a gravitational origin of the Pioneer anomaly.  相似文献   

The Gaia Data Release 1 parallaxes and the distance scale of Galactic planetary nebulae     

《New Astronomy》2017

In this paper we gauge the potentiality of Gaia in the distance scale calibration of planetary nebulae (PNe) by assessing the impact of DR1 parallaxes of central stars of Galactic PNe (CSPNe) against known physical relations. For selected PNe targets with state-of-the-art data on angular sizes and fluxes, we derive the distance-dependent parameters of the classical distance scales, i.e., physical radii and ionized masses, from DR1 parallaxes; we propagate the uncertainties in the estimated quantities and evaluate their statistical properties in the presence of large relative parallax errors; we populate the statistical distance scale diagrams with this sample and discuss its significance in light of existing data and current calibrations. We glean from DR1 parallaxes 8 CSPNe with S/N> 1. We show that this set of potential calibrators doubles the number of extant trigonometric parallaxes (from HST and ground-based), and increases by two orders of magnitude the domain of physical parameters probed previously. We then use the combined sample of suitable trigonometric parallaxes to fit the physical-radius-to-surface-brightness relation. This distance scale calibration, although preliminary, appears solid on statistical grounds, and suggestive of new PNe physics. With the tenfold improvement in PNe number statistics and astrometric accuracy expected from future Gaia releases the new distance scale, already very intriguing, will be definitively constrained.  相似文献   

Orbital variations and outbursts of the unusual variable star V1129 Centauri     

《New Astronomy》2017

The variable star V1129 Cen is classified in the GCVS as being of β Lyr type. Unusual for such stars, it exhibits outbursts roughly once a year, lasting for ∼ 40 days. For this reason, a relationship to the dwarf novae has been suspected. Here, for the first time a detailed analysis of the light curve of the system is presented. Based on observations with high time resolution obtained at the Observatório do Pico dos Dias and on the long term ASAS light curve the orbital variations of the system are studied. They are dominated by ellipsoidal variations and partial eclipses of a probably slightly evolved F2 star in a binary with an orbital period of 21^h 26^m. Comparison with the characteristics of dwarf novae show that the observational properties of V1129 Cen can be explained if it is just another dwarf novae, albeit with an unusually bright and early type mass donor which outshines the accretion disk and the mass gainer to a degree that many normal photometric and spectroscopic hallmarks of cataclysmic variables remain undetected.  相似文献   

Background mortality rates for recovering populations of Acropora cytherea in the Chagos Archipelago,central Indian Ocean     

《Marine environmental research》2013

This study quantified background rates of mortality for Acropora cytherea in the Chagos Archipelago. Despite low levels of anthropogenic disturbance, 27.5% (149/541) of A. cytherea colonies exhibited some level of partial mortality, and 9.0% (49/541) of colonies had recent injuries. A total of 15.3% of the overall surface area of physically intact A. cytherea colonies was dead. Observed mortality was partly attributable to overtopping and/or self-shading among colonies. There were also low-densities of Acanthaster planci apparent at some study sites. However, most of the recent mortality recorded was associated with isolated infestations of the coral crab, Cymo melanodactylus. A. cytherea is a relatively fast growing coral and these levels of mortality may be biologically unimportant. However, few studies have measured background rates of coral mortality, especially in the absence of direct human disturbances. These data are important for assessing the impacts of increasing disturbances, especially in projecting likely recovery.  相似文献   

珠江口水域浮游生态系统中磷的循环及其效应评估   总被引：1，自引：0，他引：1       下载免费PDF全文

刘胜  李涛  王桂芬  曹文熙  宋星宇  张建林  尹建强  黄良民 《热带海洋学报》2010,29(1):42-45

根据现场调查和室内试验工作, 计算珠江口水域浮游植物有效光合作用水体体积, 同时研究浮游动物摄食行为对磷再生的补偿作用, 进而对该水域磷的生物利用状况进行初步评估。分析珠江口2002—2003年的数据发现, 珠江口水域浮游植物有效进行光合作用水体的体积存在季节性变化, 枯水期约为9.7×104m3, 而丰水期约为6.6×104m3。该水域总初级生产量在枯水期约为36kg.d-1, 在丰水期约为31kg.d-1, 呈现枯水期大于丰水期的特点。浮游动物的摄食作用可促进水体中磷的再生, 这部分磷可满足浮游植物生长对磷需求的1.5%—15.6%, 并呈现丰水期大于枯水期的特点。浮游动物摄食作用直接释放的量远大于其自身生理周转释放的量。  相似文献   

2015年夏季海南岛东部沿岸物理结构及浮游植物群落     

刘素敏  宏波  王桂芬  王卫强  谢强  倪泽楷  喻琉  江会常  龙桐  徐洪周 《海洋学报(英文版)》2020,39(11):103-114

琼东上升流（EHU）是南海北部最强劲的上升流系统之一。它的水动力过程已经被很多研究所揭示，但是它的浮游植物群落依然不清楚。通过利用卫星遥感数据和2015年上升流季节的航次数据，我们首次阐明了琼东上升流区域（EHU）和其临近区域雷州半岛东部上升流区（ELPU）浮游植物生物量和群落的空间结构。在夏季季风的驱动下，我们在琼东沿岸发现了一个显著的低温高盐冷舌。由于雷州半岛东部大陆架宽广平缓，ELPU比EHU相对较弱。在EHU,由于受潮汐和风浪混合的影响，高溶解氧浓度 (>6.0 mg/l)几乎从表层延伸到30米深度。其次，低溶解氧的海水(<6.0 mg/l, 缺氧)被上升流从底层抽吸到上层。ELPU和EHU相比有更差的DO状况，在EHU，底层DO浓度由于大量的消耗，浓度甚至低于3.5 mg/l。在EHU，浮游植物生物量最大值出现在30米水层而不是在表层，约为1.5 mg/m³。这表明了上升流对于浮游植物生长和DO分布的影响范围。由于营养物质输入丰富， ELPU处的浮游植物生物量比EHU高很多。在EHU处，浮游植物生物量最大值可以达到4.0 mg/m³。浮游植物生物量在EHU和ELPU的沿岸区域则降低到了大约0.2~0.3 mg/m³，而这个值与远海接近。在EHU的近岸，浮游植物群落结构被硅藻所主宰，大约占了浮游植物生物量的50%。原核生物（大约40%）、绿藻（大约20%）、原绿球藻（大约20%）组成了EHU的近岸的主要群落。在ELPU,硅藻大约占了浮游植物生物量的80%，其次是绿藻，这表明与EHU相比，这个区域是一个相对不同的生态系统。  相似文献