高浓度NO对小新月菱形藻生长影响的初步研究

以小新月菱形藻为实验对象,从化学角度研究了加入高浓度一氧化氮(nitric oxide,NO)对其生长的影响。结果表明:(1)一次性加入不同浓度NO时,1.4μmol/L NO对微藻生长有促进作用;7,14,28和42μmol/L的NO对微藻生长起抑制作用,并且NO浓度越大,抑制作用越明显。(2)每天一次加入不同浓度NO时,1.4~42μmol/L的NO对微藻生长起不同程度的抑制作用,且微藻生长周期缩短。藻的生长曲线由S型变成峰型;加入42μmol/L NO,在100 h内完全抑制了微藻的生长。(3)通过进一步检测外加NO在藻液中的浓度变化,结果表明采用2种不同加入方式时,1.4μmol/L NO对藻生长分别起促进和抑制作用,这是由于NO的不断衰变造成的。     

Binary Star Fractions from the LAMOST DR4

Stellar systems composed of single, double, triple or higher-order systems are rightfully regarded as the fundamental building blocks of the Milky Way. Binary stars play an important role in formation and evolution of the Galaxy. Through comparing the radial velocity variations from multiepoch observations, we analyze the binary fraction of dwarf stars observed with LAMOST. Effects of different model assumptions, such as orbital period distributions on the estimate of binary fractions,are investigated. The results based on log-normal distribution of orbital periods reproduce the previous complete analyses better than the power-law distribution. We find that the binary fraction increases with Teff and decreases with [Fe/H]. We first investigate the relation between α-elements and binary fraction in such a large sample as provided by LAMOST. The old stars with high [α/Fe] dominate with a higher binary fraction than young stars with low [α/Fe]. At the same mass, earlier forming stars possess a higher binary fraction than newly forming ones, which may be related with evolution of the Galaxy.     

Multi-scale Tomography for Crustal <Emphasis Type="Italic">P</Emphasis> and <Emphasis Type="Italic">S</Emphasis> Velocities in Southern California

Seismic tomography is a viable tool in building depth-velocity models in the presence of strong lateral velocity variations. In this study 3-D P- and S-velocity models for the crust of southern California are constrained using more than 1,000,000 P-wave first arrivals and 130,000 S-wave arrivals from local earthquakes. To cope with the uneven distribution of raypaths, a multi-scale tomography is applied with overlapping model cells of different sizes. Within the 300 × 480 × 39 km³ model volume, the smallest cell size is 10 × 10 × 3 km³. During the iterations of velocity updating, earthquake hypocenters are determined using both P and S arrivals, and full 3-D ray tracing is implemented. Except near the edges and in the lower crust, the resultant models are robust according to various tests on the effects of reference models, resolution and signal-to-noise ratio. The tomographic velocities at shallow depths correlate very well with the regional geology of southern California. In the upper crust the P-wave and S-wave models exhibit slow velocities in major sedimentary basins and fast velocities in areas of crystalline rocks. Mid-crustal low velocity zones are present under the Coso Range, San Gabriel Mountains, and a large portion of the Mojave Desert. P- and S-velocity patterns maintain their similarity in the lower crust though the models are less reliable there.     

2015年3月新不列颠MS7.4地震震源及邻区构造应力场特征

2015年3月30日至5月15日,巴布亚新几内亚-新不列颠地区发生了一系列地震.为研究该地区的构造应力环境及孕震背景,本文基于Global CMT目录,对新不列颠区域浅部进行构造应力场反演,拟得到高精度的应力图像.反演结果显示：（1）沿着南、北俾斯麦块体边界的区域构造应力场呈走滑体系,最大主压应力轴方位呈SWW-NEE向.（2）所罗门海的NW和NE走向的海沟处于压缩状态,所罗门海块体向新不列颠和所罗门群岛俯冲的板块弯曲部分是局部拉张.（3）受俯冲带的北向推挤,南俾斯麦板块顺时针旋转的挤压,太平洋板块向西部运动汇聚作用,新不列颠岛东北部与新爱尔兰岛南部交汇区域呈现明显非均匀应力状态.（4）此次地震序列的大多数走滑型和逆冲型地震,可能是所罗门海块体俯冲运动,和南俾斯麦块体与太平洋板块的近EW向挤压作用共同引发.     

杭州湾北部实测波浪特征

为了解杭州湾北部波浪特性,利用杭州湾北部一年实测波浪资料,统计分析该地区的波参数变化特征,运用回归分析获得波参数之间的相关关系,并用谱参数及波谱形态分析了实测波浪频谱的变化特性。结果表明,与杭州湾南部海域波浪特性明显不同之处是热带气旋对本观测水域波浪的影响强度大于冬季季风的影响强度,较大波浪主要由热带气旋引起,并且路径相似的热带气旋在杭州湾南、北部测点引起的最大波浪其参数较为接近。研究水域常浪向分布在东东北至东南向,强浪向主要分布在东东北方向。研究成果可为河口海湾相关工程的设计建造和沿海防灾减灾提供重要参考。     

三峡地区上地壳结构的远震虚震源反射地震成像

远震虚震源反射成像方法利用远震初至波在台网之下地表与地下界面间形成的反射波(PPdp震相)波形资料进行台网地区地震反射结构研究.此方法先用台网各台站的平均初至波形求取震源信号,再用该震源信号与各道地震记录作反褶积从而取得反射剖面.本文介绍了远震虚震源反射成像的基本原理和实现步骤,并以三峡地区的观测资料为例,得到三峡库首区上地壳的反射地震剖面.成像剖面中解释出的四川盆地和秭归盆地的底界面位置和形态与地表地质观测和大地构造背景吻合.为验证虚震源成像的能力,本文使用弹性波正演模拟合成地震数据,经过处理实际资料一样的步骤获得虚震源成像结果.正演模拟表明,叠加多个远震的反射地震剖面可以有效地改善成像的信噪比和连续性;虚震源成像需要选择特定的震源频率范围,以减轻高频噪音以及低频造成的成像问题.在研究上地壳结构时,建议在不适合主动源采集和缺乏低频信号的地区尝试远震虚震源方法.     

An Analysis of the Condensation Temperature of Elements of Extrasolar Planetary Systems

Using high signal-to-noise ratio spectra of extrasolar planet-hosting stars, we obtained the atmospheric parameters, accurate metallicities and the differential abundance for 15 elements (C, O, Na, Mg, Al, Si, S, Ca, Sc, Ti, V, Cr, Mn, Ni and Ba). In a search for possible signatures of metal-rich material accreting onto the parent stars, we found that , for a given element, there is no significant trend of increasing [X/H] with increasing condensation temperature Tc. In our sample of planet-harboring stars, the volatile and refractory elements behave similarly, and we can not confirm if there exists any significant dependence on the condensation temperature Tc.     

Dispersion splitting of Rayleigh waves in layered azimuthally anisotropic media

Rayleigh wave dispersion can be induced in an anisotropic medium or a layered isotropic medium. For a layered azimuthally anisotropic structure, traditional wave equation of layered structure can be modified to describe the dispersion behavior of Rayleigh waves. Numerical stimulation results show that for layered azimuthal anisotropy both the dispersion velocities and anisotropic parameters depend principally on anisotropic S-wave velocities. The splitting S-wave velocities may produce dispersion splitting of Rayleigh waves. Such dispersion splitting appears noticeable at azimuthal angle 45°. This feature was confirmed by the measured results of a field test. The fundamental mode splits into two branches at azimuthal angle 45° to the symmetry axis for some frequencies, and along the same direction the difference of splitting-phase velocities of the fundamental model reaches the maximum. Dispersion splitting of Rayleigh waves was firstly displayed for anisotropy study in dispersion image by means of multichannel analysis of surface waves, the image of which provides a new window for studying the anisotropic property of media.     

浅谈地震剖面的假象识别

假象识别是正确解释地震剖面的前提,也是描述地震成像保真度(精准度)的主要标准之一.本文通过分析反射地震剖面实例,对几种常见的、易被误解的地震成像假象的特征进行了分类阐述,提出基于成因识别地震成像假象的思路.从地震剖面成像过程来看,假象的成因包括信号误判、成像畸变和波速模型误差这三个主要因素.许多不易被识别的假象起源于地震数据处理成像过程中对信号的误判,犹如“张冠李戴”;成像畸变假象的根源包括成像照明度、资料频宽和方法假设等方面的缺陷,造成抹痕等成像结果畸变假象;当地震波速度模型误差较大时,地震成像结果不仅会出现成像位置错误,还可能在波阻抗不连续点出现散射拖尾假象.因此,衡量地震成像精准度的标准应包括成像结果的分辨率、位置准确度和假象识别三个要素.这些要素相互影响,因此应该根据研究目标和实际情况,综合评判地震成像中假象的影响.