The exceptional Herbig Ae star HD 101412: The first detection of resolved magnetically split lines and the presence of chemical spots in a Herbig star

In our previous search for magnetic fields in Herbig Ae stars, we pointed out that HD 101412 possesses the strongest magnetic field among the Herbig Ae stars and hence is of special interest for follow‐up studies of magnetism among young pre‐main‐sequence stars. We obtained high‐resolution, high signal‐to‐noise UVES and a few lower quality HARPS spectra revealing the presence of resolved magnetically split lines. HD 101412 is the first Herbig Ae star for which the rotational Doppler effect was found to be small in comparison to the magnetic splitting and several spectral lines observed in unpolarized light at high dispersion are resolved into magnetically split components. The measured mean magnetic field modulus varies from 2.5 to 3.5kG, while the mean quadratic field was found to vary in the range of 3.5 to 4.8 kG. To determine the period of variations, we used radial velocity, equivalent width, line width, and line asymmetry measurements of variable spectral lines of several elements, as well as magnetic field measurements. The period determination was done using the Lomb‐Scargle method. The most pronounced variability was detected for spectral lines of He I and the iron peak elements, whereas the spectral lines of CNO elements are only slightly variable. From spectral variations and magnetic field measurements we derived a potential rotation period P_rot = 13.86 d, which has to be proven in future studies with a larger number of observations. It is the first time that the presence of element spots is detected on the surface of a Herbig Ae/Be star. Our previous study of Herbig Ae stars revealed a trend towards stronger magnetic fields for younger Herbig Ae stars, confirmed by statistical tests. This is in contrast to a few other (non‐statistical) studies claiming that magnetic Herbig Ae stars are progenitors of the magnetic Ap stars. New developments in MHD theory show that the measured magnetic field strengths are compatible with a current‐driven instability of toroidal fields generated by differential rotation in the stellar interior. This explanation for magnetic intermediate‐mass stars could be an alternative to a frozen‐in fossil field (© 2010 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

南京—仪征地区新近纪地层层序及时代讨论

上世纪70年代以来，由于雨花台组与其他砂砾层之间接触关系未被发现，南京—仪征地区新近纪地层层序及时代一直存在着争议。笔者对仪征大仪集新仪1孔剖面进行了重新整理划分，新近纪各地层叠置关系明显，同时结合其他剖面及岩相古地理分析，在前人工作的基础上，对新近纪地层层序及时代进行了讨论。该地区新近纪地层层序为中新世中期的洞玄观组(N1d)、中新世晚期的六合组(N1l)黄岗组(N1h)及上新世的雨花台组(N2γ)以及非正式岩石地层单位方山玄武岩(fb)。雨花台组沉积是位于六合组之上的另一套砂砾层，其沉积时代为上新世晚期。     

草湖地区侏罗系层序地层及沉积体系特征

基于测录井资料对比,结合区域构造演化特征,将草湖凹陷侏罗系划分为两个三级层序J-SQ1与J-SQ2。J-SQ1时期气候温暖潮湿,层序发育完整的上升半旋回和下降半旋回沉积,发育辫状河体系和湖泊体系;J-SQ2时期气候逐渐转为炎热半干旱,层序发育不完整,只发育上升半旋回沉积,主要由氧化型湖泊体系构成,发育滨浅湖砂滩、泥滩互层沉积。其中,J-SQ1早期辫状河河道砂体叠置厚度大,储层物性好,上覆中厚层湖相泥岩沉积,是本区有利的储集层段。     

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一类非线性二阶奇异初值问题的正解

在简单的假定下。建立了一类非线性二阶奇异初值问题C^1[0,1]正解存在的充分必要条件，我们的奇异问题在有奇性。     

Sequences Characterization of Microsatellite DNA Sequences in Pacific Abalone(Haliotis discus hannai)

1 Introduction Microsatellites or simple sequence repeats (SSRs) are tandemly repeated motifs of one to six bases found in all prokaryotic and eukaryotic genomes analysed to date (Zane et al., 2002). Due to their hyper-variable and co-dominant nature, relatively high abundance and random distribution in the genome, microsatellites are among the most efficient class of molecular markers. Such repeats display high polymorphism because of variation in repeat length and can be rapidly analysed t…     

无碰撞区跳频/时序列理论界与设计

跳频(时)序列分析与设计是跳频(时)扩频通信系统的核心技术.无碰撞区跳频序列是近年新出现的一个研究方向,现已成为通信领域的研究热点.对无碰撞区跳频序列的理论界及其设计进行深入研究,导出无碰撞区跳频序列的一些本质属性;讨论无碰撞区跳频序列集周期汉明相关函数的理论界,揭示几个理论界之间的关系,给出这些理论界等价的条件.提出最优无碰撞区跳频序列的一般构造方法.利用该构造方法,可以产生任意长度的最优无碰撞区跳频序列集.并且,任意一个最优无碰撞区跳频序列集,都可以由一般构造方法产生.     

尼日尔Agadem区块古近系层序地层及沉积体系研究

古近系是尼日尔Termit坳陷Agadem区块目前油气勘探的主要目的层位,但研究区目前整体勘探程度低,对古近系有利沉积相带及砂体的展布没有系统的认识,这些都极大制约了进一步的油气勘探。因此在研究区古近系开展层序地层和沉积体系的研究,预测有利砂体分布具有重要的理论及实践意义。文章以层序地层学及沉积学理论为指导,依据录井、测井及地震等资料,运用准层序组叠加样式、ΔlogR、地震反射终止关系及地震时频分析等方法,在Agadem区块古近系识别出2个二级层序界面、4个三级层序界面,将古近系划分为1个二级层序、5个三级层序（ESQ1-ESQ5）。在建立的层序地层格架内,综合岩心相、测井相及地震相特征分析了Agadem区块古近系的沉积环境,认为古近系层序ESQ1-ESQ3沉积时主要发育三角洲湖泊沉积体系,层序ESQ4-ESQ5沉积时主要为湖泊相沉积。在层序格架内沉积体系综合研究的基础上建立起本区古近系的两种沉积模式：层序ESQ1-ESQ3的拗陷期沉积模式及层序ESQ4-ESQ5的断陷期沉积模式。     

基于测井曲线的小波变换定量层序地层单元划分

盆地中沉积地层具有明显的旋回性,对应不同的测井曲线特征,可以用它来进行层序地层划分。为降低在一个视觉层次上划分地层的人为主观性,使得层序地层单元的划分更加科学,将一维的测井曲线运用小波变换技术拓展为二维时频域,将不同时间( 深度) 尺度的沉积旋回清晰地展现出来。以梅河盆地钻井为例,选取a 值在0. 25 ～ 0. 5 amax区间利用小波时频能量图识别三—五级层序地层学单元特征明显。在小波时频能量图中,层序顶底高能量向中部减弱,进而划分出三级层序界面; 层序内部能量从向大尺度转移--向小尺度转移--趋于稳定--向大尺度转移,反映了体系域从低水位--水进－高水位--水退的垂向变化过程; 其内部每个小的能量团又可以看作是一个准层序。由此建立应用小波变换划分层序地层单元的模型,为层序地层学的定量划分提供了一种新手段。     

2017年九寨沟7.0级地震断层破裂尺度初步研究

本文利用2017年九寨沟7.0级地震的余震序列数据,结合震源机制解确定的地震断层面,研究了地震断层的破裂尺度。基于余震序列在断层面上的投影,分析直接余震和间接余震以及不同起始震级条件下余震区的长度和震源深度分布,估算了地震断层破裂面的破裂长度和破裂深度,并探讨了地震断层破裂对地震烈度分布的影响。研究结果显示,九寨沟7.0级地震断层的破裂长度约33—35km,破裂深度约23—26km;地震断层破裂对Ⅷ度区分布有明显的控制作用,地震断层破裂长度接近Ⅷ度区的长度。