长江口盐度梯度下不同形态碳的分布、来源与混合行为   总被引：1，自引：0，他引：1  

叶君  姚鹏  徐亚宏  王金鹏  赵彬 《海洋学报》2019,41(4):15-26

河口碳的生物地球化学过程是全球碳循环的重要组成。通过测定溶解无机碳（DIC）及其稳定同位素丰度（δ13C_DIC），溶解有机碳（DOC），有色溶解有机物（CDOM），颗粒有机碳（POC）及其稳定同位素丰度（δ13C_POC）与元素比值（N/C）及相关指标，研究了2014年7月长江口盐度梯度下不同形态碳的分布、来源和混合行为。结果表明，DIC浓度、DOC浓度、POC含量分别为1 583.2~1 739.6 μmol/L，128.4~369.4 μmol/L和51.2~530.8 μmol/L，这些不同形态碳及CDOM的荧光组分的分布模式相似，均是从口内到口外，整体呈现先增大后减小的趋势，并与盐度呈现非保守混合行为。添加作用主要发生在在口门处最大浑浊带附近。与含量相反，从口内到口外，δ13C_DIC和δ13C_POC均呈现逐渐减小再增大的趋势，在口门附近达到最低值，分别为-9.7‰和-26.7‰。在口门附近不同形态碳含量上升及δ13C_DIC、δ13C_POC的降低可能主要与沉积物再悬浮及微生物作用有关。基于蒙特卡洛模拟的三端元混合模型的结果显示，河口内外POC来源变化明显，口内POC以陆源有机碳贡献为主，平均为62.3%，口外海源贡献逐渐增加。CDOM相关参数结果表明长江口CDOM主要来自陆源输入，海源及人类活动等也对其产生影响。  相似文献   

内蒙古中东部上侏罗统满克头鄂博组划分及时代          下载免费PDF全文

张永清 《地球科学》2021,46(1):162-171

内蒙古自治区中东部满克头鄂博组以流纹质火山碎屑岩为主夹山间湖盆相陆相碎屑岩及少量流纹岩或英安岩.沉积岩中产叶肢介Magumbonia paramecia,Nestoria reticulate,N.xishunjingensis,N.cf.pissoui,Lioestheria sp.;双壳类Ferganoconcha curta,F.subcentralis,F.elongate;植物:Ginkgoites sp.,Cladophlebis sp.,Lycopodites sp.,Baiera gracilis,Phoenicopsis sp.化石.岩石化学SiO₂71.47%~75.96%,Ai₂O₃12.50%~14.18%,K₂O 3.84%~4.98%,Na₂O 3.22%~4.14%,ALK 7.84%~9.12%,K₂O>Na₂O,显示高硅高碱特征;微量元素组成上以富集Rb、K、Th、U、La和LREE,亏损Ba、Nb、Sr、P和Ti为特征;稀土元素ΣREE=47.116×10-6~176.78×10-6,轻重稀土分溜明显,分溜系数（La/Yb）_N为4.79~25.56,δEu为0.05~0.61,为中等铕负异常.4个样品在logδ-logτ图解上全部落入造山带山花岗岩区、Rb-Y+Nb图解上落在火山弧花岗岩区、Nb-Y图解上全部落入火山弧花岗岩同碰撞花岗岩区;在阿巴嘎旗-扎鲁特旗-巴林右旗一带采集了4个锆石LA-MC-IC-MS同位素,年龄值分别为138.89±0.93 Ma、137.70±1.40 Ma、147.70±1.20 Ma和137.27±0.96 Ma,将满克头鄂博组的时代置于晚侏罗世-早白垩世.   相似文献   

Chandra observations of neutron stars: an overview     

M. C. Weisskopf  M. Karovska  G. G. Pavlov  V. E. Zavlin  T. Clarke 《Astrophysics and Space Science》2007,308(1-4):151-160

We present an overview of Chandra X-ray Observatory observations of neutron stars. The outstanding spatial and spectral resolution of this great observatory have allowed for observations of unprecedented clarity and accuracy. Many of these observations have provided new insights into neutron star physics. We present an admittedly biased and overly brief review of these observations, highlighting some new discoveries made possible by the Observatory’s unique capabilities. This includes our analysis of recent multiwavelength observations of the putative pulsar and its pulsar-wind nebula in the IC443 SNR.   相似文献   

分布式社区口腔医疗信息管理系统设计   总被引：3，自引：1，他引：2  

谢明元  刘福祥  郭在华  刘维成 《成都信息工程学院学报》2004,19(1):7-11

利用SQL Server和VB设计分布式社区口腔医疗信息管理系统,建立牙科电子病历,实现远程医疗信息共享和IC卡一卡通服务,改善口腔医疗服务水平.  相似文献   

Kinematics and stellar populations of the dwarf elliptical galaxy IC 3653     

I. V. Chilingarian  P. Prugniel  O. K. Sil'chenko  V. L. Afanasiev 《Monthly notices of the Royal Astronomical Society》2007,376(3):1033-1046

We present the first 3D observations of a diffuse elliptical galaxy (dE). The good quality data (S/N up to 40) reveal the kinematical signature of an embedded stellar disc, reminiscent of what is commonly observed in elliptical galaxies, though similarity of their origins is questionable. Colour map built from Hubble Space Telescope Advanced Camera for Surveys (ACS) images confirms the presence of this disc. Its characteristic scale (about 3 arcsec =250 pc) is about a half of galaxy's effective radius, and its metallicity is 0.1–0.2 dex larger than the underlying population. Fitting the spectra with synthetic single stellar populations (SSP), we found an SSP-equivalent age of 5 Gyr and nearly solar metallicity [Fe/H]  =−0.06  dex. We checked that these determinations are consistent with those based on Lick indices, but have smaller error bars. The kinematical discovery of a stellar disc in dE gives additional support to an evolutionary link from dwarf irregular galaxies due to stripping of the gas against the intracluster medium.  相似文献   

SN 1998A: explosion of a blue supergiant     

A. Pastorello  E. Baron  D. Branch  L. Zampieri  M. Turatto  M. Ramina  S. Benetti  E. Cappellaro  M. Salvo  F. Patat  A. Piemonte  J. Sollerman  B. Leibundgut  G. Altavilla 《Monthly notices of the Royal Astronomical Society》2005,360(3):950-962

We present spectroscopic and photometric observations of the peculiar Type II supernova (SN) 1998A. The light curves and spectra closely resemble those of SN 1987A, suggesting that the SN 1998A progenitor exploded when it was a compact blue supergiant. However, the comparison with SN 1987A also highlights some important differences: SN 1998A is more luminous and the spectra show bluer continua and larger expansion velocities at all epochs. These observational properties indicate that the explosion of SN 1998A is more energetic than SN 1987A and more typical of Type II supernovae. Comparing the observational data with simulations, we deduce that the progenitor of SN 1998A was a massive star  (∼25 M_⊙)  with a small pre-supernova radius  (≲6 × 10¹² cm)  . The Ba  ii lines, unusually strong in SN 1987A and some faint II-P events, are almost normal in the case of SN 1998A, indicating that the temperature plays a key role in determining their strength.  相似文献   

ATCA H i observations of the peculiar galaxy IC 2554     

Bärbel Koribalski  Scott Gordon  Keith Jones 《Monthly notices of the Royal Astronomical Society》2003,339(4):1203-1222

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产业集群与浦东集成电路产业建设   总被引：1，自引：0，他引：1  

王琳  王琛  曾刚 《世界地理研究》2005,14(1):23-27

产业集群的形成是现代经济发展中的一个非常重要的现象。浦东集成电路产业集群是“国家集成电路产业基地”的核心，产业集群的形成对浦东集成电路产业提高竞争力具有重要的意义。本文分析了浦东集成电路产业集群的发展现状。指出目前浦东集成电路产业集群的建设还处于一个初步阶段，无论是企业间，还是企业与高校、科研机构或者其他组织机构间的创新合作交流都十分有限，从而在一定程度上抑制了集成电路产业整体学习能力和竞争力的提高。文章针对这些问题，从产业链、区域性产业发展政策、环境配套设施建设等方面提出了加强浦东集成电路产业集群建设的对策建议。  相似文献   

狭缝系统与伊利石结晶度Kuebler指数的测定及相关问题讨论   总被引：4，自引：0，他引：4  

王河锦  徐庆生 《地质论评》2000,46(6):588-593

根据实验结果,衍射峰半高宽随接收狭缝增大而呈二次工线线性增大。扫描速度与扫描步长的确定应遵守Ｗａｎｇ（１９９４）提出的关系式,并确定在相对误差小于〈５％的范围内。固定样品条件,选定最优实验条件下使用国际标样标定系统偏差是伊利石结晶测量中必不可少的重要步骤。不固定样品条件和实验条件,同一样品的伊利石工值将因条件的变化而不同;固定样品和实验条件而不使用国际标样标定系统偏差,则无法与他人数据进行对比,其  相似文献   

New observations of the only supernova remnant in the galaxy IC 1613     

T. A. Lozinskaya  N. Yu. Podorvanyuk 《Astronomy Letters》2009,35(6):375-383

We present new results of our kinematic study of the supernova remnant S8 in the galaxy IC 1613. Based on our observations at the 6-m Special Astrophysical Observatory telescope with the two-dimensional MPFS spectrograph and the SCORPIO focal reducer in the mode of a scanning Fabry-Perot interferometer, we have determined the expansion velocity of the bright optical nebula. Analysis of the 21-cm VLA radio observations for the galaxy confirms our previously suggested model for a supernova explosion in a cavity surrounded by a dense HI shell and a collision of S8 with the shell wall.  相似文献