河北蔚县盆地晚上新世以来沉积古环境演化分析     

张亚光  马梦玲  周明兴  贠杰  高尚  何立  赵力颖  李广栋  鲁艳明 《地质论评》2023,69(Z1):37-39

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Phosphorus speciation in surface sediments of a hypertrophic lake,Southwestern China: insights from fractionation and 31P NMR     

Zhang  Runyu  Wang  Liying  Wu  Fengchang 《中国地球化学学报》2015,34(2):167-176

Acta Geochimica - Phosphorus (P) species in surface sediments from a shallow, hypertrophic lake, Lake Dianchi, China, were investigated by P fractionation and 31P nuclear magnetic resonance (NMR)...  相似文献   

Characteristics and Main Controlling Factors of Tight Oil Reservoir in the Jimsar Sag of Junggar Basin   总被引：1，自引：0，他引：1  

BAO Haijuan  HE Wenjun  FEI Liying  JIA Xiyu  ZHENG Menglin  YANG Haibo  GGUO Xuguang 《《地质学报》英文版》2015,89(Z1):182-183

<正>1 Introduction Jimsar sag covers about 1278 km2 in the south of the eastern uplift of Junggar basin.It is a half graben depression area in which the west,south and north is controlled by faults(Fig.1),and is tilting uplift to the east.It deposited Permian,Triassic,Jurassic,the Cretaceous and Cenozoic strata chronologically.The thickness of Lucaogou Formation is about 200 m to 350 m,it is the  相似文献   

中南部非洲的地质构造演化与矿产分布规律          下载免费PDF全文

刘晓阳  王杰  余金杰  王丽瑛  修群业  贺福清  任军平 《地质找矿论丛》2015,30(S1):1-12

中南部非洲优势矿产资源有金、铜、铁、铬、金刚石,锰、铀、镍、钒、钴、铂、锑的储量也居世界前列。主要的矿产集中分布于前寒武纪地体内,中南部非洲前寒武纪地体的形成演化决定了矿产的种类和主要成矿类型。文章总结了中南部非洲的地质构造演化以及其主要矿产资源的成矿类型和分布规律,并划分成矿区带至三级。探讨了部分主要成矿区带的成矿规律:太古宙的矿产主要与花岗-绿岩地体有关;古元古代的矿产主要分布于陆缘盆地,与岩浆作用有关;中元古代的矿产主要与岩浆作用有关,次为沉积变质作用;新元古代的矿产主要与沉积变质作用有关,次为岩浆作用。  相似文献   

中南部非洲纳米比亚三级成矿区带划分          下载免费PDF全文

王丽瑛  董卫宏  屠立鹏  刘晓阳 《地质找矿论丛》2015,30(S1):53-59

纳米比亚矿产资源丰富,是非洲第四大矿产国,现已发现矿产30多种,主要生产金刚石、铀、铜、金、银、铅、锌等,其外汇收入的一半以上来自矿产品。文章在查阅文献资料的基础上,详细研究了该国区域成矿地质背景、矿产资源分布特征,结合成矿理论和成矿规律研究的新成果,对纳米比亚成矿规律进行了研究,提出三级成矿区带划分方案,全区共划分8个Ⅲ级成矿区带,对进一步圈定重要找矿远景区提供了依据。  相似文献   

Photometric Studies of Twelve Deep, Low-mass Ratio Overcontact Binary Systems     

Qian Shengbang  Yang Yuangui  Zhu Liying  He Jiajia  Yuan Jingzhao 《Astrophysics and Space Science》2006,304(1-4):25-28

The formations of the blue straggler stars and the FK Com-type stars are unsolved problems in stellar astrophysics. One of the possibilities for their formations is from the coalescence of W UMa-type overcontact binary systems. Therefore, deep (f > 50%), low-mass ratio (q < 0.25) overcontact binary stars are a very important source to understand the phenomena of Blue Straggler/FK Com-type stars. Recently, 12 W UMa-type binary stars, FG Hya, GR Vir, IK Per, TV Mus, CU Tau, V857 Her, V410 Aur, XY Boo, SX CrV, QX And, GSC 619-232, and AH Cnc, were investigated photometrically. Apart from TV Mus, XY boo, and GSC 619-232, new observations of the other 9 binaries were obtained. Complete light curves of the 10 systems, FG Hya, GR Vir, IK Per, TV Mus, CU Tau, V857 Her, GSC 619-232, V410 Aur, XY Boo, and AH Cnc, were analyzed with the 2003 version of the W-D code. It is shown that all of those systems are deep (f > 50%), low-mass ratio (q < 0.25) overcontact binary stars. We found that the system GSC 619-232 has the highest degree of overcontact (f = 93.4%). The derived photometric mass ratio of V857 Her, q = 0.0653, indicates that it is the lowest-mass ratio system among W UMa-type binaries.Of the 12 sample stars, long-term period changes of 11 systems were found. About 58% (seven) of the sample binaries show cyclic period oscillation. No cyclic period changes were discovered for the other 5 systems, which may be caused by the short observational time interval or by insufficient observations. Therefore, we think that all W UMa-type binary stars may contain cyclic period variations. By considering the long-term period changes (both increase and decrease) of those binary stars, we proposed two evolutionary scenarios evolving from deep, low-mass ratio overcontact binaries into Blue Straggler/FK Com-type stars.  相似文献   

邯郸市可吸入颗粒物的污染现状及相关气象条件分析   总被引：3，自引：1，他引：2  

张海霞  董占强  杨玲珠  王丽英  李敏 《气象与环境科学》2009,32(Z1)

利用邯郸市区4个代表站2006年逐时可吸入颗粒物PM10浓度监测资料和邯郸市观测站地面气象要素的逐时观测资料,分析了邯郸市主要空气污染物--PM10的时空分布特征,结果表明:PM10平均浓度采暖期明显大于非采暖期;日变化规律为上午浓度最高,夜间次之,下午浓度最低,采暖期为双峰双谷型,非采暖期为一峰一谷型;弱风、低温和潮湿的气象条件有利于可吸入颗粒物的积累,增加PM10浓度.  相似文献   

基于欧洲中心细网格预报资料和观测资料的浙江省春夏降水性质分类指标     

王霁吟  陈懿妮  孙长  王丽颖  俞佩 《气候与环境研究》2018,23(5):543-550

利用浙江省2004~2013年3~8月Micaps（气象信息综合分析处理系统）地面填图数据和T-logP数据研究杭州、衢州和台州三市的阵雨和雷雨个例,同时选取能表征雷雨并能区分阵雨与雷雨的气象预报因子:对流有效位能、850 hPa与500 hPa的温差、K指数、地面2 m温度,用临近探空的分析方法和决策树的分类方法初步建立了一个适用于浙江省春夏季降水性质分类指标。利用欧洲中心（ECMWF）细网格预报资料,对历史样本和2016年春、夏季分别作了检验。结果表明:除去有降水预报误差个例后,指标TS（Threat Score）评分超过0.53,雷雨阵雨综合命中率达到71%,空报率阵雨（10%）小于雷雨（43%）,在不同地区和季节稍有区别;同时对浙江省2016年春夏两次典型大范围阵雨雷雨过程进行预报,效果很好。此方法不仅可以依据预报数据在短期内做出精细化降水性质分类预报,在中长期预报上也有表现力。  相似文献   

一次强降水过程的热量和水汽收支分析     

王爱君  宋晓辉  田秀霞  王丽英  李菊香 《气象与环境科学》2010,33(Z1)

利用NCEP/NCAR每日4次全球再分析1°×1°网格资料,计算了2007年7月18日河北南部暴雨过程的水汽通量、视热源(Q1)和视水汽汇(Q2),分析了降水区热量和水汽收支的变化,并探讨了其垂直分布特征.结果表明:本次暴雨过程是由沿低涡切变线相继生成并强烈发展的中尺度对流云团造成的;当有强对流发生并伴有强降水时,就会有强的视热源Q1和视水汽汇Q2出现,且与强降水区基本对应,对流层上半部的相对冷层为暴雨区上空积云对流提供了极为有利的热力不稳定条件.  相似文献   

XUV Photometer System (XPS): Improved Solar Irradiance Algorithm Using CHIANTI Spectral Models     

Thomas N. Woods  Phillip C. Chamberlin  W. K. Peterson  R. R. Meier  Phil G. Richards  Douglas J. Strickland  Gang Lu  Liying Qian  Stanley C. Solomon  B. A. Iijima  A. J. Mannucci  B. T. Tsurutani 《Solar physics》2008,250(2):235-267

Solar soft X-ray (XUV) radiation is highly variable on all time scales and strongly affects Earth’s ionosphere and upper atmosphere; consequently, the solar XUV irradiance is important for atmospheric studies and for space weather applications. Although there have been several recent measurements of the solar XUV irradiance, detailed understanding of the solar XUV irradiance, especially its variability during flares, has been hampered by the broad bands measured in the XUV range. In particular, the simple conversion of the XUV photometer signal into irradiance, in which a static solar spectrum is assumed, overestimates the flare variations by more than a factor of two as compared to the atmospheric response to the flares. To address this deficiency in the simple conversion, an improved algorithm using CHIANTI spectral models has been developed to process the XUV Photometer System (XPS) measurements with its broadband photometers. Model spectra representative of quiet Sun, active region, and flares are combined to match the signals from the XPS and produce spectra from 0.1 to 40 nm in 0.1-nm intervals for the XPS Level 4 data product. The two XPS instruments are aboard NASA’s Solar Radiation and Climate Experiment (SORCE) and Thermosphere, Ionosphere, Mesosphere, Energetics, and Dynamics (TIMED) satellites. In addition, the XPS responsivities have been updated for the latest XPS data processing version. The new XPS results are consistent with daily variations from the previous simple conversion technique used for XPS and are also consistent with spectral measurements made at wavelengths longer than 27 nm. Most importantly, the XPS flare variations are reduced by factors of 2 – 4 at wavelengths shorter than 14 nm and are more consistent, for the first time, with atmospheric response to solar flares. Along with the details of the new XPS algorithm, several comparisons to dayglow and photoelectron measurements and model results are also presented to help verify the accuracy of the new XUV irradiance spectra.  相似文献