UTEVA树脂分离纯化珊瑚中铀、钍的改进研究     

汤震宇  瞿建国  张安余  李秀保  杜金洲 《海洋学报》2022,44(2):11-20

珊瑚是记录海洋环境变化信息的载体之一,测定其U/Ca比值可重建海水温度或测定Th/U同位素比值可计算年龄重建海平面高度等.准确测定珊瑚中U、Th含量及同位素比值是提取所记载的海洋环境变化信息的前提,其难点在于高Ca基体分离和痕量U、Th富集纯化.基于此,本研究拟采用UTEVA树脂改进了一步富集分离珊瑚中U、Th的前处理...  相似文献   

WATER　RESOURCES　TRANSFORMATION　AND　WATER　QUALITY　VARIATION　IN　THE　URUMQI　RIVER　BASIN     

曲耀光  骆鸿珍 《中国地理科学(英文版)》1995,5(4):325-335

ＷＡＴＥＲＲＥＳＯＵＲＣＥＳＴＲＡＮＳＦＯＲＭＡＴＩＯＮＡＮＤＷＡＴＥＲＱＵＡＬＩＴＹＶＡＲＩＡＴＩＯＮＩＮＴＨＥＵＲＵＭＱＩＲＩＶＥＲＢＡＳＩＮＱｕＹａｏｇｕａｎｇ（曲耀光）；ＬｕｏＨｏｎｇｚｈｅｎ（骆鸿珍）（ＬａｎｚｈｏｕＩｎｓｔｉｔｕｔｅｏｆＧ...  相似文献   

Cultivation of marine sponges   总被引：3，自引：0，他引：3  

曲翊 张卫李华  虞星炬 《中国海洋湖沼学报》2005,23(2):194-198

Sponges are the most primitive of multicellular animals, and are major pharmaceutical sources of marine secondary metabolites. A wide variety of new compounds have been isolated from sponges. In order to produce sufficient amounts of the compounds of the needed, it is necessary to obtain large amount of sponges.The production of sponge biomass has become a focus of marine biotechnology.  相似文献   

论浙江安吉矿产资源开发保护规划与区域经济的可持续发展     

任荣富  曲卫 《浙江国土资源》2002,18(1):90-95

安吉县矿产资源开发利用与保护规划工作在我省开展比较早 ,规划的组织实施在国发经济建设和社会发展中已发挥出较好的作用。在参与安吉地区农业生态环境地质调查过程中 ,结合资源环境的调查评价 ,在整顿矿业秩序 ,改善和修复矿山生态环境 ,矿山地质灾害调查防治等方面做了些尝试。本文就资源环境的开发保护 ,矿业经济与区域经济可持续发展方面作些探讨 ,对于正在进行或将要进行规划和实施规划的地区具一定借鉴意义  相似文献   

First Results from SWAN Lyman α solar wind mapper on SOHO     

J. L. Bertaux  E. Quémerais  R. Lallement  E. Kyrölä  W. Schmidt  T. Summanen  J. P. Goutail  M. Berthé  J. Costa  T. Holzer 《Solar physics》1997,175(2):737-770

After one year of almost flawless operation on board the SOHO spacecraft poised at L1 Lagrange point, we report the main features of SWAN observations. SWAN is mainly dedicated to the monitoring of the latitude distribution of the solar wind by the Lα method. Maps of sky Lα emissions were recorded througout the year. The region of maximum emission, located in the upwind hemisphere, deviates strongly from the pattern that could be expected from a solar wind constant with latitude. It is divided into two lobes by a depression aligned with the solar equatorial plane called the Lyα groove already noted in 1976 Prognoz data. The north lobe is much brighter than the south lobe. These two characteristics can be explained qualitatively by an enhanced ionization along the neutral sheet where the slow solar wind is concentrated, which results from the higher low-latitude solar wind mass flux as measured by Ulysses. The groove is the direct imprint on the sky of the enhanced carving by the slow solar wind, at this time of solar minimum, when the tilt angle of the neutral sheet is small. The question is still pending to predict what will happen with the ascending phase of the solar cycle. Observations of comets are briefly mentioned, with the ability of SWAN to monitor the H₂O production of many comets. Operations of the instrument are briefly described, including some instrumental problems which could be solved by software modifications sent to the instrument. Supplementary material to this paper is available in electronic form at http://dx.doi.org/10.1023/A:1004979605559  相似文献   

Magneto-induced Line Broadening of Magneto-sensitive Lines in Solar Magnetized Atmospheres     

Zhong-Quan Qu  Shuai Wang  Cheng-Lin Xu  XiaoYu Zhang  Ming-Guo Sun  Chun-Lan Jin National Astronomical Observatories/Yunnan Astronomical Observatory  Chinese Academy of Sciences  Kunming  zqqu@vip.km.net Graduate School of the Chinese Academy of Sciences  Beijing 《中国天文和天体物理学报》2005,5(4):426-432

We analyze the spectral line broadening of those magneto-sensitive lines in solar magnetized atmospheres. The broadening at the line wings is due to the increase of the effective width of energy levels involved in Zeeman splitting, and the broadening at the line core also originated in Zeeman splitting under the condition that the Zeeman components are mixed. Therefore, the magnetoinduced or Zeeman broadening take effects on the whole line. The observed Stokes parameter data in a sunspot and outside it acquired by Solar Stokes Spectrum Telescope (S3T) are analyzed for the demonstration of this mechanism, and the Zeeman broadening rates are calculated for FeI6302.5 under some assumptions. Our result shows that the broadening is increased as the magnetic field strength becomes stronger, but the rate of increase at the line core is decreased as the field strength increases, while the rate at the wing does not show such an obvious regularity. The broadening is more effective in the line core than in the wings.  相似文献   

宽甸北部早元古宙铅锌矿地质特征及成因讨论     

曲亚军  王文清 《国土资源》1989,(3)

辽宁宽甸北部早元古宙铅锌矿位于辽东青城子—吉林荒沟山—朝鲜检德铅锌矿带上。赋存于辽东优、冒地槽的过渡带,靠近优地槽一侧的碳酸盐岩建造中。矿体受岩相、岩性控制明显,属层控矿床。吕梁构造旋回的变质变形作用对矿带的改造不明显。矿带的同位素特征表明,张家堡子铅锌矿形成于封闭盆地环境,矿质来源于大陆边缘深部液态矿源层;而高丽墓子铅锌矿带则形成于正常海洋环境,表现了明显的原始沉积矿床的特点。  相似文献   

致密星的X射线辐射时延现象     

屈进禄  宋黎明  吴枚  李年福 《天文学进展》2002,20(2):144-157

能谱仅反映了高能天体辐射的部分性质，而高能X射线辐射的时变可以反映致密天体的动态性质。因此，在构造高能辐射的理论模型时，既要考虑X辐射的能谱性质，也要考虑其时变性质。特别对高能天体X辐射的快速光变，一般认为其发生在致密天体附近，致密天体快速光变的研究可以揭示出致密天体附近的物理性质，因此，时变可以对X辐射模型给以很强的限制。X射线源不同能量光子到达观测者的时间差称为X射线辐射的时延。介绍了高能X辐射时变中的时延分析方法及其最新发展，综述了致密双星系统中黑洞侯选林和中子星的时延现象，并简单介绍了为解释这些现象所发展的模型，以及时延对模型的限制。  相似文献   

Wind tunnel simulation experiment and investigation on the electrification of sandstorms     

QU Jianjun  YAN Muhong  DONG Guangrong  ZHANG Hongfa  ZU Ruiping  TUO Wanquan  ZHAO Aiguo  XlAO Zhenghua  LI Fang & YANG Bao Key Laboratory of Desert  Desertification  Cold  Arid Regions Environmental  Engineering Research Institute  Shapotou Desert Research  Experiment Station  Chinese Academy of Sciences  Lanzhou  China 《中国科学D辑(英文版)》2004,47(6):529-539

~~Wind tunnel simulation experiment and investigation on the electrification of sandstorms~~  相似文献   

Features of clay minerals in the YSDP102 core on the continental shelf of the southeast Yellow Sea     

JIANGXuejun QUGaosheng LIShaoquan 《中国海洋大学学报(英文版)》2004,3(2):201-207

Ninety-eight clay mineral samples from the YSDP102 core were analyzed by x-ray diffractometer to study the four clay minerals: illite, chlorite, kaolinite and smectite. Twenty-eight samples had been analyzed on the laser particle-siz eanalyzer to reveal the particle features of the sediments. Distribution of the clay minerals and the particle characteristics in the YSDP102 core show that the core experienced three different depositional periods and formed three different sedimentary intervals due to different sediment sources and different depositional environments. Features of the clay minerals and the heavy minerals in the YSDP102 core indicate that coarse-grained sediments and fine-grained sediments result from different sources. The Yellow Sea Warm Current has greatly influenced the sedimentary framework of this region since the current‘s formation.  相似文献