企鹅珍珠贝游离珠培育技术的初步研究

2006 年 5 - 12 月,在广东省、湛江市、徐闻县芳华珍珠养殖场,采用贝龄 2 ～ 4 a 的企鹅珍珠贝作植核贝,以 1 ～ 3 a 贝作小片贝,进行游离珍珠培育试验.结果表明,植核母贝经 15 ～ 40 d 的术前处理,成活率为 95.33 % ～ 97.00 %;施术贝经过 6 个月培育后,吐核率为 63.00 % ～ 71.88 %,死亡率为 26.17 % ～ 35.00 %,成珠率为 1.95 % ～ 3.33 %.企鹅珍珠贝合适的植核母贝为 2 ～ 3 龄贝,小片贝为 1 ～ 2 龄贝.     

ICESat-2激光卫星与光学遥感影像融合水深测量

针对浅海测深的数据特点和应用需求,以我国南海甘泉岛为例,研究了利用ICESat-2(Ice,Cloud,and Land Elevation Satellite-2)激光卫星数据和光学遥感影像开展主被动融合水深测量的方法。首先通过信号点提取、水面/水底识别、水下点折射改正等步骤处理ICESat-2数据,获得水深值,随后以激光点作为控制,计算光学水深反演模型参数,最后由点及面地获取大范围高精度水深。实验表明,甘泉岛区域主被动融合测深中误差优于1.30m,基于激光卫星数据的主被动融合测深方法能够为浅水水深测量提供新手段。     

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.     

Matter-wave interference in an axial triple-well optical dipole trap

This paper proposes a scheme of axial triple-well optical dipole trap by employing a simple optical system composed of a circular cosine grating and a lens. Three optical wells separated averagely by ～37 μm were created when illuminating by a YAG laser with power 1 mW. These wells with average trapping depth ～0.5 μK and volume ～74 μm³ are suitable to trap and manipulate an atomic Bose--Einstein condensation (BEC). Due to a controllable grating implemented by a spatial light modulator, an evolution between a triple-well trap and a single-well one is achievable by adjusting the height of potential barrier between adjacent wells. Based on this novel triple-well potentials, the loading and splitting of BEC, as well as the interference between three freely expanding BECs, are also numerically stimulated within the framework of mean-field treatment. By fitting three cosine functions with three Gaussian envelopes to interference fringe, the information of relative phases among three condensates is extracted.     

南极树粉孢属真菌胞外多糖的分离纯化及结构表征

研究南极树粉孢属(Oidiodendron truncatum)真菌所产胞外多糖的理化性质和结构特征。采用阴离子交换柱层析和凝胶柱层析对南极树粉孢属(Oidiodendron truncatum)真菌胞外多糖进行了系统的分离纯化,从中得到4个均一的组分(AFW1,AFW2,AFS1和AFS2),并结合红外、气质及核磁等技术对它们的结构进行了解析。结果表明:AFW1和AFW2为中性多糖,AFS1和AFS2中含有少量的蛋白;AFW1和AFS1是由甘露糖、葡萄糖和半乳糖3种单糖组成的结构复杂的杂多糖;AFW2和AFS2则仅由葡萄糖组成,其中AFW2属线性(-1,6-葡聚糖,而AFS2属于C-3位有分支的α-1,6-葡聚糖。     

Ka波段毫米波云雷达对青藏高原东南缘降水回波的分析

利用丽江站新建的Ka波段毫米波云雷达获得的高时间分辨率的垂直观测资料,结合同址的地面自动气象站和雨滴谱的分钟数据、常规探空数据和附近C波段天气雷达的强度回波,分析了两次降水过程前后云雷达反射率因子Z、径向速度V_r、速度谱宽S_w的垂直变化规律。分析表明:在发生弱降水时,云雷达Z在垂直方向的变化不明显;但V_r、S_w值在0℃层稍低位置有一个明显的分界层(融化层),粒子通过融化层后V_r、S_w都是快速变大,这个变化主要是粒子的相态由固态变成液态引发的,可以通过V_r、S_w突变值的位置来识别0℃层亮带的高度。从C波段天气雷达回波强度、剖面图及云雷达位置的时间-高度图看,对毛毛雨和小雨的回波,强度和高度差异比较明显,毛毛雨比小雨回波高度低、强度弱,与云雷达相比C波段雷达对高一些的云观测不到,对距离较远的弱降水回波无法观测到;由于相同粒子对不同波长电磁波的散射不一样,造成两种雷达垂直方向观测到的Z变化不同。对比弱降水回波,云雷达在...     

云南热区≥10℃和≥18℃年积温及日数的分布规律研究

云南热区以其独特的自然地理条件,在我国热区的研究与开发中占有极其重要的地位。利用云南实测地面气温资料等,采用线性回归及残差分析等分析方法,分析了云南热区森林生态系统≥10℃积温及其日数、≥18℃积温等热量指标在不同地区的空间分布规律及原因。结果表明,云南热区不同区域≥10℃积温及其日数、≥18℃积温等热量指标都有明显的空间差异。根据这些划分热量带的基本指标,以及热区分布县市的最低海拔和增温或降温的效应,对其热区分布的海拔上限进行了估测,为准确确定云南热区分布的空间格局及各县市热带和南亚热带的热区范围及热区的主要特性提供了依据。     

浙江省衢州市上方镇重钙方解石矿工艺指标影响因素

重质碳酸钙的白度和色相值(Lab)是最重要的工业指标,但影响因素尚不清楚.本文通过扫描电镜、粉晶X射线衍射(XRD)和电感耦合等离子体发射光谱(ICP-OES)等分析手段,对浙江衢州上方镇的重钙方解矿石进行了研究,以期阐明重质碳酸钙白度和色相的影响因素.结果表明,矿石随研磨粒度的减小白度逐渐增加,在100～400目,白...     

杨山晚古生代沉积盆地成因类型及其与桐柏-大别造山带关系的探讨

杨山晚古生代沉积盆地位于桐柏-大别山北麓,它具有明显的前陆盆地沉积特点,由早期(D₂?—C₁)的复理石建造到晚期(C₁—P?)的磨拉石建造;古生物地理分析表明其与华北、扬子陆块都有密不可分的联系,其间不可能有古洋盆的存在,因而它应当是桐柏一大别造山带碰撞造山过程中形成的前陆盆地。杨山晚古生代前陆盆地的形成说明,扬子陆块和华北陆块的陆-陆碰撞起始于晚泥盆世之前(S₃—D₂),而桐柏-大别造山带中生代的构造事件则可能代表一次大规模陆内逆冲-推覆作用。