我国海洋保护地现状、问题及发展对策

随着我国海洋经济的不断发展,沿海地区的海洋环境和生态系统面临的压力不断加剧。海洋保护地作为海洋生态环境管理的有效手段,近30年来被广泛应用于海洋生物多样性和生态系统保护,取得了显著的成就和效果。文章通过对我国海洋保护地的建设情况进行系统研究,阐述了海洋保护地的发展现状和管理体制,重点剖析了海洋保护地管理和建设过程中面临的缺乏顶层设计、管理能力和管护条件弱、管理人才和资金少、空间发展不平衡等问题,在建设以国家公园为主体的自然保护地体系的新形势下,为我国海洋保护地的发展提出了健全海洋保护地管理制度体系、构建海洋保护地网络体系、加强海洋保护地管理能力建设和加强海洋保护地宣传教育等对策建议。     

非滑动式与滑动式拉格朗日插值法在BDS精密星历内插中的比较分析

在高精度卫星定位数据处理中,对精密星历内插处理是一项基础工作。利用拉格朗日多项式插值法,从三方面对北斗导航系统精密星历进行了内插精度分析,分别是非滑动式拉格朗日插值法在不同插值阶数下的插值精度,滑动式拉格朗日插值法在不同插值阶数下的插值精度,以及非滑动式和滑动式拉格朗日插值法在同一插值阶数下的插值精度。算例结果表明,如果将插值阶数作为横坐标,且向右为正,插值精度为纵坐标,向上为正,那么非滑动式拉格朗日插值法的插值精度与插值阶数呈现一个开口向下的抛物线关系;滑动式拉格朗日插值法的插值阶数高于7后,插值精度处于稳定且高的状态,插值误差最大值为1. 1 mm左右,均方差在0. 4 mm左右;在同一插值阶数下,滑动式拉格朗日插值法的精度高于非滑动式拉格朗日插值法的精度。     

Scaling-laws of Radio Spike Bursts and Their Constraints on New Solar Radio Telescopestwo

Radio observation is one of important methods in solar physics and space science. Sometimes, it is almost the sole approach to observe the physical processes such as the acceleration, emission, and propagation of non-thermal energetic particles, etc. So far, more than 100 solar radio telescopes have been built in the world, including solar radiometers, dynamic spectrometers, and radioheliographs. Some of them have been closed after the fulfillment of their primary scientific objectives, or for their malfunctions, and thus replaced by other advanced instruments. At the same time, based on some new technologies and scientific ideas, various kinds of new and much more complicated solar radio telescopes are being constructed by solar radio astronomers and space scientists, such as the American E-OVSA and the solar radio observing system under the framework of Chinese Meridian Project II, etc. When we plan to develop a new solar radio telescope, it is crucial to design the most suitable technical parameters, e.g., the observing frequency range and bandwidth, temporal resolution, frequency resolution, spatial resolution, polarization degree, and dynamic range. Then, how do we select a rational set of these parameters? The long-term observation and study revealed that a large strong solar radio burst is frequently composed of a series of small bursts with different time scales. Among them, the radio spike burst is the smallest one with the shortest lifetime, the narrowest bandwidth, and the smallest source region. Solar radio spikes are considered to be related to a single magnetic energy release process, and can be regarded as an elementary burst in solar flares. It is a basic requirement for the new solar radio telescope to observe and discriminate these solar radio spike bursts, even though the temporal and spatial scales of radio spike bursts actually vary with the observing frequency. This paper presents the scaling laws of the lifetime and bandwidth of solar radio spike bursts with respect to the observing frequency, which provide some constraints for the new solar radio telescopes, and help us to select the rational telescope parameters. Besides, we propose a spectrum-image combination mode as the best observation mode for the next-generation solar radio telescopes with high temporal, spectral, and spatial resolutions, which may have an important significance for revealing the physical essence of the various non-thermal processes in violent solar eruptions.     

山东省上古生界页岩气资源潜力评价

以山东省上古生界海陆过渡相富有机质泥页岩为研究对象,对泥页岩的沉积环境、厚度及分布、有机质类型及含量、有机质演化程度等资料进行分析,认为石炭-二叠纪山西组和太原组泥页岩发育厚度大而稳定,有机质类型以Ⅲ型为主,镜质体反射率一般在0.7%~1.7%之间,有机碳含量一般在1.5%~9.0%之间,是页岩气主要富集层位。以含气量不小于0.5m3/t、镜质体反射率不小于0.5%、有机碳含量平均不小于2.0%等为资源量评价标准,建立有机碳含量与含气量关系模型,估算山东省上古生界页岩气潜在地质资源总量为5 736.75×108 m~3,明确了具有勘查价值的区域有鲁西南含煤区、黄河北含煤区、阳谷-茌平含煤区和临清坳陷,为山东省上古生界页岩气下一步勘查指明了方向。     

Origin of ore-forming fluids in Qinggouzi stibnite deposit,NE China:Constraints from fluid inclusions and H-O-S isotopes

The Qinggouzi stibnite deposit is located in Huashan Town, Jilin Province, in the northeastern margin of North China Craton(NCC). It is controlled by fault structures, hosted within structurally controlled felsic dykes, predominantly surrounded by phyllite, schist and quartzite. This study presents the results of fluid inclusions studies, intending to determine the source of the fluid responsible for ore-formation, hence exploring its metallogenesis. The aqueous biphase inclusions are identified in the stibnite-bearing quartz veins of the deposit. Moreover, aqueous biphase inclusions are further classified into(1) biphase liquid-rich inclusions(1 a) and(2) biphase gas-rich inclusions(1 b) depending upon liquid to gas ratio trapped within the fluid inclusions. Homogenization temperatures for(1 a) and(1 b) range between 114.8℃ to 422℃ and 128.3℃ to 267.5℃, respectively. 1 a and 1 b have salinities of 0.18% to 16.14% NaCl_(eqv) and 1.22% to 12.88% NaCl_(eqv), and density range from 0.43 to 1.02 g/cm~3 and 0.81 to 0.98 g/cm~3, respectively. Sulfur isotopic analysis indicates δ~(34)S_(V-CDT) from 4.4×10~(-3) to 6.5×10~(-3), with an average of 5.2×10~(-3), whereas H isotopes values on δD_(V-SMOW) standard are-100.8×10~(-3) and-107.5×10~(-3), while O isotopes data on δ~(18)O_(V-SMOW) standard range between 20.1×10~(-3) and 20.4×10~(-3). Fluid inclusions study, combining with sulfur and H-O isotopic data reveal that the ore-forming fluids originated from deep source and were subsequently contaminated by meteoric water. Hydrostatic pressure calculation shows that the minimum and maximum pressures are 11.65 and 42.33 MPa, and relevant depths of deposit are estimated to be 1.16 and 4.23 km. Finally, we inferred that Qinggouzi stibnite deposit is a medium-low temperature, low salinity hydrothermal deposit, which is formed by deep source and later contaminated by meteoric water, and is classified as epizonal deposit in terms of orogenic series.     

安徽省酷热天气分析及预报指标

基于安徽省1961-2017年逐日地面最高气温资料,采用Mann-Kendall法对安徽省高温天气事件进行突变分析,发现安徽省2000年后高温事件明显增加。为分析安徽省酷热天气特征和产生机理,文中挑选了35~37℃高温天气个例对比分析。结果发现:1)500 hPa西太平洋副高位置和850 hPa气温对酷热天气预报的指示性最好。2)受西太平洋副热带高压不同位置控制,安徽省增温机制不同:当为高压中心控制时,太阳辐射在增温过程中起决定性作用,安徽省易出现酷热天气;当高压中心位于海上,脊线位于安徽省附近时,安徽省高温强度较弱。通过酷热天气个例研究和合成平均分析,文中总结了安徽省酷热天气预报指标。     

北太平洋冬季西部发展型天气尺度涡旋对平均流的影响

在中纬度北太平洋大气强斜压区,存在频繁的天气尺度涡旋活动,通过水分、动量和能量输送维持大气环流。为了进一步研究天气尺度涡旋发生发展与大尺度环流之间的联系,利用1981—2013年再分析资料,筛选出西部发展型天气尺度涡旋114个偏强日和87个偏弱日,给出了西部发展型天气尺度涡旋异常导致的动力和热力强迫的变化,同时从能量转换的角度分析了西部发展型天气尺度涡旋与平均流之间的相互作用,并探讨了其与西太平洋遥相关型的关系。结果表明:西部发展型天气尺度涡旋通过动力强迫和热力强迫影响平均流,其中动力强迫主要造成北太平洋中纬度上空的西风气流加速并向北移动;热力强迫的作用则是减弱中纬度大气斜压性。同时,强西部发展型天气尺度涡旋有利于西北太平洋上空对流层低层斜压有效位能向扰动动能的转化增大和扰动动能向平均流的转化增大,有利于中纬度地区对流层高层平均流向扰动动能的转化增大。此外,西部发展型天气尺度涡旋通过与平均流的作用,对维持西太平洋遥相关型的负位相有一定影响。     

适应数值模式垂直坐标的GPS掩星反演资料稀疏化方案

GPS掩星反演大气温湿资料具有高垂直分辨率、高精度、受云和降水影响小等优点,针对GRAPES同化预报系统,发展设计了一种既考虑预报模式高度-地形追随垂直坐标不均匀分层特点,又结合掩星反演资料特性的新适应性垂直稀疏化方案。通过个例试验和批量试验,探索了该适应性稀疏化方案对分析预报质量的影响。试验结果表明:选取合适的稀疏参数,新稀疏化方案的GPS掩星反演资料对背景场的调整更加有效,分析场质量更高;位势高度、比湿、温度和风场等预报场的均方根误差均更小;适应性稀疏化方案对改善台风路径预报具有积极作用。批量试验则进一步证实了适应性稀疏化方案对分析场质量有明显的改善作用。     

不同光质对坛紫菜果孢子和壳孢子萌发的影响

本研究探究了白、蓝、红、绿光4种光质对坛紫菜(Pyropia haitanensis)果孢子和壳孢子萌发的影响。结果表明,与白光相比,用绿光培养时,果孢子萌发管分枝形成速度、萌发管生长速度,以及壳孢子的细胞分裂速度均相对较快,用红光与蓝光培养时则相对较慢。不同光质对坛紫菜果孢子和壳孢子的存活率无显著影响,但能造成萌发体色泽呈现明显差异。刚从孢子囊释放出来的两种孢子均呈黄褐色,经白光培养的两种孢子以及蓝光培养的果孢子,其萌发体颜色加深至鲜红色,蓝光培养的壳孢子萌发体颜色加深尤为明显,最终呈深紫红色,而红光和绿光培养的两种孢子颜色变浅,最终呈浅黄褐色。研究表明,绿光培养可能不利于坛紫菜孢子萌发过程的色素积累,但有利于孢子萌发及萌发体的生长。     

河南省现代服务业集聚特征及影响因素分析

现代服务业是伴随着科技发展而出现的一种新兴产业,对区域产业结构优化升级、促进经济发展等方面日趋重要。采用空间基尼系数、区位熵分析、EG指数和面板回归等方法,对2007—2017年河南省现代服务业集聚特征及影响因素进行分析,得出以下结论：①河南省现代服务业总体及其8个分行业集聚程度较高,其中科学研究和技术服务业集聚程度最高,教育最低;②河南省现代服务业总体及其8个分行业专业化水平较低,其中郑州市专业化水平最高,并在金融业,文化、体育和娱乐业2个行业表现出较强的集聚优势;③河南省现代服务业总体及其8个分行业空间集聚结构较差,发展还不成熟;④经济发展水平对河南省现代服务业发展影响最大,交通条件、资本支持、信息化水平和人力资本对现代服务业发展具有不同程度的促进作用,工业化水平、政府行为对其产生显著的负影响。