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41.
Understanding and characterising movement and area-use patterns of fishes within estuaries, as well as understanding the degree of connectivity between estuaries and the marine environment, can provide important insights into a species’ ecology, which is fundamental for effective management and conservation. Mark-and-recapture data obtained from the 082 TAG FISH Project, a dart-tagging programme, were used to describe movement patterns of juvenile leervis Lichia amia in the permanently open Swartkops Estuary, South Africa, as well as the degree of connectivity with the adjacent marine environment. A total of 628 juvenile leervis were tagged from 2008 to 2015, of which 77 fish (12.3%) were recaptured, with juveniles comprising 85.7% of all measured recaptures. The majority of recaptures (75.3%) were made within the Swartkops Estuary, indicating estuarine philopatry, with 23.4% having moved less than 1 km, revealing site fidelity, but most (51.9%) displaying estuarine roaming. A smaller portion of recaptures (27.7%) had dispersed to other habitats; 16 (20.8%) displayed multiple-habitat connectivity, while only 3 (3.9%) had undertaken long-distance movements (>100 km) and were recaptured up to 825 km northeast of the Swartkops Estuary. Lichia amia that had moved greater distances were characterised by a greater mean size and age at the time of recapture. This study provides valuable information on the philopatry and dispersal of juvenile L. amia.  相似文献   
42.
风成沙波纹脊线提取与应用计算   总被引:2,自引:1,他引:1  
李猛  董治宝  张正偲 《中国沙漠》2014,34(2):312-317
风成沙波纹是沙质地表在风力作用下形成的最小地貌单元,对研究风沙的起动过程和运动过程极其重要,同时,沙波纹形态特征的研究为了解大尺度范围风沙地貌形态演变提供理论基础。然而由于风成沙波纹尺度较小,形成速度较快,导致对其形态特征的观测比较困难。近些年,随着计算机图形学的迅猛发展,数字图像处理方法得到了较大发展,使得测量和计算更加便捷。本文基于高清相机拍摄的风成沙波纹图像,借助于Matlab平台,采用数字图像处理技术,对沙波纹脊线进行提取,并应用于沙波纹形态参数计算。本文选取腾格里沙漠东南缘的沙波纹进行验证分析,得到风成沙波纹波长的正态分布规律,沙波纹的波长随时间逐渐增长,在40 min的时间范围内,波长由不足1 cm逐步发展到接近10 cm。最后,采用数字图像处理方法,计算了沙波纹脊线长度和波长。采用数字图像处理方法,波长等数据更易于获取和统计,数据采集效率大大提高,为风成沙波纹的研究提供了新的方法。  相似文献   
43.
Seabed mapping, spatially referenced trapping, and mark‐recapture methods have all been useful tools in ecological studies of lobsters and other benthic animals. Here we integrate the three methods to evaluate local population dynamics and movements of American lobsters, Homarus americanus, in coastal fishing grounds in Maine, United States. The study was conducted on five study areas of different size, and used two different sampling protocols. At one site (1 km2 in area) we used a monthly mark‐recapture sampling interval over a 6‐month period, only tagging a subsample of the catch. At four smaller sites (0.3 km2) we used a shorter‐term approach, sampling at 3–4‐day intervals for a 2‐week duration, tagging the entire catch. Tagging data were analysed with a modified Jolly‐Seber model adapted for continuous sampling to estimate population abundance, gains (immigration), and losses (emigration and mortality). Side‐scan sonar surveys of the seabed combined with diver‐based population surveys, stratified by substrate type, provided an independent comparison to mark‐recapture‐based estimates of abundance over the same areas. Spatial referencing of trap catch also allowed us to relate catch rates and lobster movements directly to seabed features. The longer‐term tagging data on the larger study area provided abundance estimates that were more consistent with the diver observations, and estimates of gains and losses statistically more robust, than those derived from the shorter‐term effort on the smaller sites. The flux of lobsters followed the well known seasonal movements on these fishing grounds, with gains and losses from the larger study area ranging over 1000 individuals per day, and an estimated mid‐summer peak density of >65 000 lobsters per km2 (individuals >50 mm carapace length). This approach may lend itself to broader application with the American lobster.  相似文献   
44.
月球线性构造分类体系研究   总被引:1,自引:0,他引:1  
罗林  刘建忠  张莉  籍进柱  郭弟均  刘敬稳 《岩石学报》2017,33(10):3285-3301
月球线性构造是月球科学研究中的重要组成部分,建立月球线性构造分类体系是月球地质图编研的关键。前人对月球线性构造的分类研究主要基于月表的形貌特征,划分的线性构造类型参差不齐,尚未形成一个公认的、规范的、具有普适性的线性构造分类体系,以至于分类结果的可对比性差、参考性和易操作性较低,不利于月球线性构造纲要图的编制。并且月球线性构造的概念混乱、术语不统一,存在"同物异名、同词异义、异词同义、涵义不明"的现象,不利于全球性的统一制图和成果的展示及使用。鉴于此,本文采用多指标组合的分类方法,以成因机制和形貌特征作为主要指标,兼顾物质组成,再结合线性构造形成的动力学机制,建立了符合月球动力学演化背景的、统一规范的线性构造类型划分的新方案,避免了单以形貌特征为依据来分类出现的混乱状态,具有较好的科学性和可操作性。将月球的线性构造类型划分为:内动力地质作用形成的线性构造,包括皱脊、月溪、地堑、断裂;外动力地质作用形成的线性构造,包括坑缘断裂和坑底断裂,以及多成因机制、多动力来源作用形成的特殊类型如坑链等。在此基础上,并利用多源遥感数据建立了易于判别且具有代表性的线性构造识别标志,可为全月球线性构造的统一制图提供识别依据。  相似文献   
45.
基岩标是指在覆盖有松散地层的区域内为更准确测定地面沉降量,穿过覆盖层埋设在稳定基岩卜的标杆直通地面,经过保护处理作为相对稳定的基岩水准点。具有标孔要求高、基岩面判层准确、标杆安装要求高等特点。通过浙江省宁波市2座基岩标施工的实践,探讨了确保基岩标质量的关键技术和控制措施,对实际施工有一定的参考作用。  相似文献   
46.
Granule ripples are found mainly in four regions of the Kumtagh Desert in China; they are characterized by an asymmetrical shape, with gentle lower slopes on both sides and abrupt crests. The ripples tend to be oriented perpendicular to the prevailing winds, except when they form near obstacles such as yardangs. The wavelengths (λ) range between 0·31 m and 26 m and heights (h) range from 0·015 m to 1 m. The relationship between wavelength and height can be described by a simple linear function, and the mean ripple index (λ/h) is about 20·4 for the study sites. The sediments are poorly sorted, with negative to very negative skewness at lee and stoss slopes and between‐ripple troughs, which confirms the ‘poured in’ and ‘shadow’ appearance described by previous researchers. The bimodal or trimodal distributions of grains (with modes of ?1·16φ, ?0·5φ and 3·16φ) and the enrichment of coarse particles at the ripple surface (with coarse granule contents ranging between 5·2% and 62·1%) indicate that the underlying layer is the original sediment source and that the granule ripples resist erosional processes. Although the impact of saltating particles and, consequently, the creep and reptation of coarse grains are responsible for granule ripple initiation at a micro‐scale, however, the characteristics of local sediments, wind regimes and topographical obstacles, as well as the feedbacks among bedform and airflow, more strongly affect the development and alignment of granule ripples at a macro‐scale.  相似文献   
47.
在收集前人及野外采集资料基础上,利用薄片鉴定、岩石密度分析,对冀北坳陷中新元古界雾迷山组的岩石类型与特征、沉积相标志、剖面相研究了其沉积相类型。结果认为研究区属于典型的陆表海碳酸盐台地沉积环境,根据岩性及叠层石特征可细分为潮下、潮间和潮上带。其中一、二段由近35个小型韵律层组成了一个完整的由海侵到海退的沉积序列,具有自潮下至潮间再至潮上的潮坪相为主的沉积样式,为典型的雾迷山韵律沉积。第三段小型叠层石只见于三段的下部,而从第12层开始出现大型叠层石。第四段灰质白云岩中含沥青质块体,层理一般平直,或微波状,有时可见斜层理和波痕,为潮间带一潮下带沉积。  相似文献   
48.
利用MapGIS组件(COM)技术,在Visual Basic环境中编写了等值线图极值标注程序.程序首先利用MapGIS组件技术构造了含有物化探数据的点工作区,然后读入MapGIS等值线区文件(.wp).通过对闭合区的弧段数目的判断,挑选出包含极值点的MapGIS区实体.通过点对极值区的相交分析,提取出极值区内的数据.对提取的数据求取极值,并用该极值与圈闭它的等值线高程值进行比较,确定极值是极大值还是极小值,最后形成极值标泣点文件(.wt),从而完成了等值线平面图极值的标注.  相似文献   
49.
风沙物理学中两个焦点问题研究现状与未来研究思路刍议   总被引:4,自引:2,他引:2  
丁国栋 《中国沙漠》2008,28(3):395-398
风沙物理学经过数十年的发展与完善,可以说基本上自成体系。但由于学科的起步较晚,加之现象的复杂性,目前仍有很多重要的理论问题没能彻底解决,至少还未达成共识,成为学术界长期以来争论的焦点,从而影响了学科的继续发展。对“沙粒起动机制”和“风成沙纹的形成机理”两个焦点问题在进行研究现状剖析的基础上,浅析未来研究思路。提出沙粒起动主要驱动力是驻点升力的观点,以空气动力学理论为基础的沙粒起动机制研究将是未来该领域的发展趋势;关于沙纹的形成,认为沙粒粒径的不均匀性以及所导致的非平衡运动是前提和基础,风沙流运动过程中类似左右沙丘运动的蚀积转换规律是使沙纹能够维持其稳定形态的必要条件,而沙纹有规律、整齐划一的分布与排列可能与背风面气流小尺度的涡流有关。  相似文献   
50.
An experimental investigation on the initiation and development of bed forms on a bed of fine silica sand was conducted under alluvial flow conditions in a laboratory flume with a diverging channel. The main aims of the study were to assess: i) the steepness of bed forms in the transition stage of development; and ii) the threshold height of wavelets (ηt) that triggered the start of ripple development. Detailed bed profile measurements were carried out using an acoustic Doppler probe, traversed longitudinally over the sediment bed at various experimentation times. The bed form dimensions were extracted from such bed profile records and analysed for the wavelet, transition and equilibrium stages. It was found that the steepness of ripples in the transition and equilibrium stages were similar, confirming predictions of previous mathematical model simulations. A lognormal distribution fitted the wavelet length data. The wavelet threshold height was estimated as ηt ≈ 7 mm, or ηt≈ 80 in wall units. Such a height magnitude suggested that ripple development could be triggered by the wavelets reaching the outer flow zone of a turbulent boundary layer. The ηt value obtained corresponded generally to the intersection point between two predictive equations for bed form dimensions. A formulation was developed to predict ηt as a function of the sediment grain size, which was confirmed for the fine sand used in this study.  相似文献   
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