Iron Regulation of Wetland Vegetation Performance Through Synchronous Effects on Phosphorus Acquisition Efficiency

Iron-rich groundwater flowing into wetlands is a worldwide environmental pollution phenomenon that is closely associated with the stability of wetland ecosystems. Combined with high phosphorus(P) loading from agricultural runoff, the prediction of the evolution of wetland vegetation affected by compound contamination is particularly urgent. We tested the effects of anaerobic iron-rich groundwater discharge in a freshwater marsh by simulating the effect of three levels of eutrophic water on native plants(Glyceria spiculosa(Fr. Schmidt.) Rosh.). The management of wetland vegetation with 1–20 mg/L Fe input is an efficient method to promote the growth of plants, which showed an optimum response under a 0.10 mg/L P surface water environment. Iron-rich groundwater strongly affects the changes in ecological niches of some wetland plant species and the dominant species. In addition, when the P concentration in a natural body of water is too high, the governance effect of eutrophication might not be as expected. Under iron-rich groundwater conditions, the δ~(13)C values of organs were more depleted, which can partially explain the differences in δ~(13)C in the soil profile. Conversely, the carbon isotope composition of soil organic carbon is indicative of past changes in vegetation. The results of our experiments confirm that iron-rich groundwater discharge has the potential to affect vegetation composition through toxicity modification in eutrophic environments.     

Tail Emission from a Ring-like Jet: Its Application to Shallow Decays of Early Afterglows and GRB 050709

Similar to the case of pulsars the magnetic axis and the spin axis of gamma-ray burst sources may not lie on the same line. This may cause the formation of a ring-like jet due to collimation of the processing magnetic axis. We analyze the tail emission from such a jet, and find that it has a shallow decay phase with a temporal index of -1/2 if the Lorentz factor of the ejecta is not very high, which is consistent with the shallow decay phase of some early X-ray afterglow detected by Swift. The ring-like jet has a tail cusp with sharp rising and very sharp decay. This effect can provide an explanation for the re-brightening and sharp decay of the X-ray afterglow of GRB 050709.     

A new lunar absolute control point: established by images from the landing camera on Chang'e-3

The establishment of a lunar control network is one of the core tasks in selenodesy, in which defining an absolute control point on the Moon is the most important step. However, up to now, the number of absolute control points has been very sparse. These absolute control points have mainly been lunar laser ranging retroreflectors, whose geographical location can be observed by observations on Earth and also identified in high resolution lunar satellite images. The Chang'e-3(CE-3) probe successfully landed on the Moon, and its geographical location has been monitored by an observing station on Earth. Since its positional accuracy is expected to reach the meter level, the CE-3 landing site can become a new high precision absolute control point. We use a sequence of images taken from the landing camera, as well as satellite images taken by CE-1 and CE-2, to identify the location of the CE-3 lander. With its geographical location known, the CE-3 landing site can be established as a new absolute control point, which will effectively expand the current area of the lunar absolute control network by 22%, and can greatly facilitate future research in the field of lunar surveying and mapping, as well as selenodesy.     

Data processing and initial results from the CE-3 Extreme Ultraviolet Camera

The Extreme Ultraviolet Camera(EUVC) onboard the Chang'e-3(CE-3)lander is used to observe the structure and dynamics of Earth's plasmasphere from the Moon. By detecting the resonance line emission of helium ions(He+) at 30.4 nm, the EUVC images the entire plasmasphere with a time resolution of 10 min and a spatial resolution of about 0.1 Earth radius(RE) in a single frame. We first present details about the data processing from EUVC and the data acquisition in the commissioning phase, and then report some initial results, which reflect the basic features of the plasmasphere well. The photon count and emission intensity of EUVC are consistent with previous observations and models, which indicate that the EUVC works normally and can provide high quality data for future studies.     

On the intrinsic shape of the gamma-ray spectrum for Fermi blazars

The curvature of the γ-ray spectrum in blazars may reflect the intrinsic distribution of emitting electrons, which will further give some information on the possible acceleration and cooling processes in the emitting region. The γ-ray spectra of Fermi blazars are normally fitted either by a single power-law(PL) or a log-normal(call Logarithmic Parabola, LP) form. The possible reason for this difference is not clear. We statistically explore this issue based on the different observational properties of 1419 Fermi blazars in the 3 LAC Clean Sample. We find that the γ-ray flux(100 Me V–100 Ge V) and variability index follow bimodal distributions for PL and LP blazars, where the γ-ray flux and variability index show a positive correlation. However, the distributions of γ-ray luminosity and redshift follow a unimodal distribution. Our results suggest that the bimodal distribution of γ-ray fluxes for LP and PL blazars may not be intrinsic and all blazars may have an intrinsically curved γ-ray spectrum, and the PL spectrum is just caused by the fitting effect due to less photons.     

Faint field galaxies: an explanation of the faint blue excessusing number evolution models

Pure luminosity evolution models for galaxies provide an unacceptable fit to the redshifts and colors of faint galaxies. In this paper we demonstrate, using HST morphological number counts derived both from the I ₈₁₄-band of WFPC2 in the Medium Deep Survey (MDS) and the Hubble Deep Field (HDF) and from the H _1.6-band of NICMOS, and ground-based spectroscopic data of the Hawaii Deep Field and the Canada-France Redshift Survey, that number evolution is necessary for galaxies, regardless of whether the cosmic geometry is flat, open, or Λ-dominated. Furthermore, we show that the number evolution is small at redshifts of z<1, but large at z>1, and that this conclusion is valid for all the three cosmological models under consideration. If the universe is open or Λ-dominated, the models, which are subject to the constraint of the conservation of the comoving mass density of galaxies, naturally predict a population of star-forming galaxies with the redshift distribution peaking at z=2∼ 3, which seems to be consistent with the recent findings from Lyman-break photometric selection techniques. If the cosmological model is flat, however, the conservation of the comoving mass density is invalid. Hence, in order to account for the steep slope of B-band number counts at faint magnitudes in the flat universe, such a star-forming galaxy population has to be introduced ad hoc into the modelling alongside the merger assumption. This revised version was published online in July 2006 with corrections to the Cover Date.     

长江漫滩区深大异形基坑施工对紧邻特大型桥梁影响及变形控制研究

随着地下空间资源的开发利用,越来越多深基坑呈现出开挖深、规模大、形状不规则等特点,其支护结构设计复杂,施工难度大,具有明显的空间效应。本文以南京地铁某基坑工程为例,分析基坑施工对邻近桥梁的影响。其场区位于长江下游漫滩相二元结构地层分布地段,上部软土层厚度大,下部承压含水层地下水位高、水量丰富,地质条件复杂,该基坑为典型的深大异形基坑,距离某大桥的双曲拱引桥仅为7. 2 m,由于之前桥梁已遭受其他地下工程施工产生的较大变形,所以后续工程对其影响变形控制要求极高。为此,该车站基坑支护结构设计基于地下空间实际功能采用设置分隔墙分区开挖及MJS超深工法墙综合变形控制方案。本文通过有限元数值模拟计算,开展复杂环境下基坑开挖引起的围护结构及桥梁桩基的变形预测分析,计算结果显示,该深大狭长异形基坑开挖对邻近桥梁沉降变形影响显著,通过设置分隔墙分区开挖及MJS工法墙进行变形控制,能够较好地控制基坑的空间效应,减少“长边效应”、“异形效应”等对桥梁沉降变形的影响。通过现场基坑开挖过程实际监测结果,验证这一综合变形控制方案的可行性。该研究成果对于类似复杂地质条件下深大狭长异形基坑的支护及施工设计具有很好的借鉴意义。     

牛心山花岗岩岩体特征及其与成矿的关系

本文较系统地阐述了牛心山花岗岩岩体的地质特征及岩体的成因,并结合华尖金矿区地质矿化特征,探讨了花岗岩体在时间、空间及岩浆演化方面与成矿的关系。     

江西萍乡杨家湾2号洞哺乳动物化石及其时代探讨

2015年11月和2016年10月先后对杨家湾2号洞化石点进行发掘。目前已出土哺乳动物化石1000多件,主要为单个牙齿化石,骨骼较少且较为破碎。初步鉴定出31个哺乳动物属种,其中偶蹄类数量最为丰富,野猪所占比例最大;灵长类和食肉类较为丰富;啮齿类、长鼻类及奇蹄类较少;尚未发现食虫类和翼手类。大部分属种为现生类群,少量灭绝属种如巴氏大熊猫、东方剑齿象及华南巨貘等。从动物群组成来看,该动物群与杨家湾1号洞、湖南道县福岩洞等动物群较为相似,属于我国南方典型的晚更新世大熊猫-剑齿象动物群,但是其所包含的动物属种相对后两个化石点都较少,尤其是小哺乳动物属种单调。杨家湾2号洞的堆积物颗粒比1号洞的较粗,且含较多角砾,缺少红色粘土;据初步判断,该洞的堆积物是由洞口进入。动物群组合指示该地区晚更新世气候较为温暖湿润。

     

早全新世白令海北部陆坡沉积环境快速变化

理解增暖背景下海洋环境的演化过程是海洋学和气候学一项重要的研究内容。在地质时期,地球经历了多次增暖时段（包括早全新世）,这为认识海洋环境演化过程提供了重要参考。早全新世全球气候经历了快速增暖,并伴随着冰原融化和海平面快速上升,对包括白令海在内的高纬边缘海的沉积过程和海洋环境产生显著影响。白令海发育宽阔的大陆架,毗邻北美大陆,接受来自育空河、阿纳德尔河和库斯科维姆河物质的供给。目前我们对白令海如何响应早全新世气候的认识还存在明显不足。本研究对位于白令海北部陆坡LV63-19-3岩心沉积物中陆源碎屑组份进行了高分辨率调查,结合沉积年龄模型,研究了早中全新世（距今11.7～5.5 ka）白令海北部陆坡陆源沉积演化过程。研究结果显示,在距今11.5～11 ka,白令海北部陆坡沉积速率高达392.9 cm/ka,在距今约9.7 ka以后降至17.2 cm/ka。在距今11～10.7 ka,发现一层厚约40 cm的暗色纹层状沉积层。在高沉积速率时段,沉积物平均粒径较细,距今9 ka以来平均粒径逐渐增大。主微量元素分析结果表明,陆源碎屑沉积物母岩性质以长英质沉积物为主,并存在少量火山碎屑源贡献。白令海北部陆坡高沉积速率事件对应于冰原融水脉冲（MWP）-1B事件（距今11.4～11.1 ka）,并导致白令海陆坡硅质生产力勃发。在距今11～10.7 ka研究区春夏季海冰覆盖增加抑制表层水体氧供给,夏、秋季持续冰川融水和高表层生产力进一步加剧了水体层化和海洋内部消耗,共同促进了纹层状沉积层的形成。距今9 ka以来白令海季节性海冰活动增强,但是陆源碎屑物质质量累积速率则逐渐减小,表明随着海平面上升,供给到研究区的陆源物质减少。我们认为早全新世白令海北部陆坡沉积环境快速变化是海平面、冰融水脉冲事件和季节性海冰活动共同作用的结果,实际上受高纬日射量、北美大陆冰原融化和全球气候变化控制。