柴达木盆地石炭系烃源岩和煤岩生物标志物特征及其地球化学意义   总被引：34，自引：7，他引：27  

孟仟祥  房嬛  徐永昌  沈平 《沉积学报》2004,22(4):729-736

采自柴达木盆地东北部石炭系烃源岩和煤岩的生物标志化合物研究表明,研究样品的有机质演化已达高成熟阶段,其母质来源以水生生物为主,同时有较丰富的陆源物质输入。除煤岩的沉积古环境较氧化且经历过较强的降解过程外,其余样品的沉积古环境均属于较还原环境,沉积介质为咸水环境,有机质总体丰度高。因此该区石炭系海陆交互相含煤沉积是一套较一般侏罗系为好的烃源岩系,有较好的生烃潜力。  相似文献   

AzTEC millimetre survey of the COSMOS field – I. Data reduction and source catalogue     

K. S. Scott  J. E. Austermann  T. A. Perera  G. W. Wilson  I. Aretxaga  J. J. Bock  D. H. Hughes  Y. Kang  S. Kim  P. D. Mauskopf  D. B. Sanders  N. Scoville  M. S. Yun 《Monthly notices of the Royal Astronomical Society》2008,385(4):2225-2238

We present a 1.1 mm wavelength imaging survey covering 0.3 deg² in the COSMOS field. These data, obtained with the AzTEC continuum camera on the James Clerk Maxwell Telescope, were centred on a prominent large-scale structure overdensity which includes a rich X-ray cluster at z ≈ 0.73. A total of 50 mm-galaxy candidates, with a significance ranging from 3.5 to 8.5σ, are extracted from the central 0.15 deg² area which has a uniform sensitivity of ∼1.3 mJy beam⁻¹. 16 sources are detected with S/N ≥ 4.5, where the expected false-detection rate is zero, of which a surprisingly large number (9) have intrinsic (deboosted) fluxes ≥5 mJy at 1.1 mm. Assuming the emission is dominated by radiation from dust, heated by a massive population of young, optically obscured stars, then these bright AzTEC sources have far-infrared luminosities  >6 × 10¹² L_⊙  and star formation rates  >1100 M_⊙ yr⁻¹  . Two of these nine bright AzTEC sources are found towards the extreme peripheral region of the X-ray cluster, whilst the remainder are distributed across the larger scale overdensity. We describe the AzTEC data reduction pipeline, the source-extraction algorithm, and the characterization of the source catalogue, including the completeness, flux deboosting correction, false-detection rate and the source positional uncertainty, through an extensive set of Monte Carlo simulations. We conclude with a preliminary comparison, via a stacked analysis, of the overlapping MIPS 24-μm data and radio data with this AzTEC map of the COSMOS field.  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   

Correlated Radio-Optical Variations on Intraday Timescales     

Shan-Jie Qian 《中国天文和天体物理学报》2008,8(2):219-229

Correlated radio-optical variations on intraday timescales have been observed (e.g. In BLO 0716 714) and such radio intraday variability is suggested to have an intrinsic ori- gin. Recently, multi-wavelength observations, simultaneous at radio, mm-submm, optical and hard X-rays, of 0716 714, show that during a period of intraday/interday variations at ra- dio and mm wavelengths, the apparent brightness temperature of the source exceeded the Compton-limit (～1012 K) by 2--4 orders of magnitude, but no Compton catastrophe (or no high luminosity of inverse-Compton radiation) was detected. It is also found that the intra- day/interday variations at mm-submm wavelengths are consistent with the evolutionary be- havior of a standard synchrotron source and for the intraday/interday variations at centimeter wavelengths opacity effects can play a significant role, which is consistent with the interpreta- tion suggested previously by Qian et al. Thus the apparent high brightness temperatures may probably be explained in terms of Doppler boosting effects due to bulk relativistic motion of the source. We will argue a scenario to simulate the correlations between the radio and optical variations on intraday timescales observed in BLO 0716 714 in terms of a relativistic shock propagating through a jet with a dual structure.  相似文献   

A Photometric Study of the W UMa-Type Contact Binary RZ Corn     

Jia-Jia He  Sheng-Bang Qian 《中国天文和天体物理学报》2008,8(4)

We present results of CCD photometric observations of the short-period W UMatype contact binary system, RZ Com. The light curve of the binary has changed from Wsubtype to A-subtype from 1998 to 2003, then back to W-subtype in 2004. An analysis was carried out using the 2003 version of the Wilson-Devinney code. It is confirmed that RZ Com is a low-degree, overcontact f = 20.1% (±7.4%) binary system with a high inclination of i = 81.°40 (±0.°40), and a mass ratio q = 2.351 (±0.031). Combining four newly determined times of light minimum with others in the literature, the variations in orbital period is examined. A small-amplitude oscillation (A=0.0065d), with a period of 41.5 year, is discovered superimposed on a long-term increase at rate dP/dt = +3.97×10-8d yr-1. The period oscillation can be explained either by the light-time effect due to the presence of an unseen third body, or by cycles of magnetic activity on the components. Combining our photometric solution with the spectroscopic elements obtained by Mclean & Hilditch, the absolute dimensions of RZ Com are: M1 = 1.14 (+0.19)Mo, M2 = 0.50 (-4-0.09)Mo, R1= 1.12 (±0.01)R⊙, R2 = 0.78 (±0.01)R⊙ and A = 2.41 (±0.02)R⊙.  相似文献   

华南地区锡多金属矿床空间数据统计分析   总被引：1，自引：1，他引：0  

李林  罗郧 《地质科技情报》2004,23(2):94-98

基于MAPGIS系统平台空间分析方法的特点, 以华南地区的锡多金属矿床为空间分析对象,对锡多金属矿床的分布态势及有利成矿地层、构造、岩浆岩等要素的相关对象属性进行了统计分析, 初步总结出华南地区燕山期和晋宁期岩浆岩、泥盆系和侏罗系地层及NE向或NEE向断裂带等有利因素的叠加复合部位是寻找锡多金属矿床的有利成矿条件组合标志, 为成矿预测及相关区域找矿工作的部署提供了量化依据.  相似文献   

城市地下空间开发利用容量评估的基础研究   总被引：10，自引：1，他引：9  

吴立新  姜云  梁越  徐磊  陈学习  祝文君 《地理与地理信息科学》2004,20(4):44-47

该文探讨了城市地下空间开发利用容量评估的必要性,容量评估研究的基本内容及其关键技术。指出当前城市地下空间容量评估基础研究包括指标体系、评估模型、评估平台与评估示范四方面。城市地下空间容量评估研究不仅有利于城市地下空间的合理利用和有序开发,也有利于引导城市地面设施的合理布局与科学规划,对保障现代城市的可持续发展具有重要意义。  相似文献   

藏北昂吾地区超基性岩的蛇纹石化和磁铁矿化过程及影响因素     

李静超  赵涛  刘治博  林赟  邵华胜  袁国礼  宋扬 《岩石学报》2019,35(7):2158-2172

班公湖-怒江缝合带广泛分布超基性岩及蛇纹石化超基性岩,已有研究表明它们与区域成矿关系密切,其蛇纹石化过程使一些元素活化并具有一定的成矿潜力。位于班-怒带中段的昂吾地区蛇纹石化超基性岩主要矿物成分有橄榄石、单斜辉石、铬铁矿、利蛇纹石、磁铁矿和绿泥石等,原岩恢复表明该超基性岩为单辉橄榄岩。镜下鉴定、背散射电子图像、能谱成分分析和电子探针分析结果显示单辉橄榄岩的蛇纹石化及蚀变过程可分为三个阶段:(Ⅰ)以形成相对富铁蛇纹石(Mg#=75～88)为主,基本无磁铁矿析出;(Ⅱ)形成相对富镁的蛇纹石(Mg# 90),析出磁铁矿;(Ⅲ)蛇纹石进一步蚀变成绿泥石。热力学模拟及多组分矿物相平衡图表明,在蛇纹石化过程中,昂吾地区超基性岩中的辉石脱硅致使反应体系SiO_2活度升高,限制了磁铁矿的生成。同时也发现,在利蛇纹石稳定存在的温度区间内(100～300℃),本研究的蛇纹石化体系温度倾向高值区,不利于磁铁矿的析出。进而探讨了原岩成分、反应体系SiO_2活度及温度等因素对蛇纹石化过程中磁铁矿析出的影响。本研究有助于理解班-怒带内超基性岩的蛇纹石化过程及磁铁矿化机制。  相似文献   

西准萨吾尔山一带吉木乃组地层时代厘定及意义     

支倩  李永军  段丰浩 《地质论评》2019,65(Z1):135-135

正"吉木乃组"由新疆地质局区测大队与中国地质科学院地质研究所1974年创建,创名地为吉木乃县哈尔加乌西南萨尔布拉克沟,原称之为萨尔布拉克组。后因名称与柯坪地区奥陶系组名相同,将其更名为吉木乃组,时代置于早石炭世(新疆维吾尔自治区地质矿产局,1993)。新疆地质矿产局地质矿产研究所(1991)将该组时代定为中石炭世(石炭纪三分法)。1998年新疆地矿局第四地质大队在萨吾尔山  相似文献   

郯庐断裂带(安徽段)对地表水系空间分布形态的影响研究          下载免费PDF全文

钱家忠  卫佳佳  姜琼  郑勇  赵卫东 《地质科学》2019,54(2):398-410

为了研究郯庐断裂带(安徽段)构造活动对其周边地表水系形态及其发育特征的影响,本文基于DEM数据,利用GIS空间分析功能并结合郯庐断裂带构造运动特征,对郯庐断裂带(安徽段)周边水系的几何分布特征进行研究。研究表明:郯庐断裂带(安徽段)在不同地质历史时期对区内地表水系产生错动影响。受郯庐断裂三叠纪到白垩纪期间左旋走滑运动影响,两条二级水系在大别山区自西北向东南流经郯庐主干断裂及次级断裂时与断裂呈近似直角相交并发生左旋错动。大别山地区的皖河流域与华阳河流域水系受郯庐断裂第四纪以来逆右行平移运动影响流向由东南向同步大幅度拐向南西,表现为右旋扭错;巢湖流域水系受五河—合肥断裂和石门山断裂影响也出现了右旋位错。此外,受郯庐断裂带构造运动形成的合肥盆地和地堑式嘉山盆地的影响,池河的主河道沿合肥盆地东侧的沉降带和石门山断裂与嘉庐断裂之间的嘉山盆地发育。  相似文献