重磁异常正反演计算在煤田中的应用   总被引：1，自引：0，他引：1  

张作新  姜鹏里 《中国煤田地质》1998,10(1):64-65

以海拉尔盆地呼和湖研究区为例,对重磁异常进行正、反演计算,求取各个主要地层组、段顶界面埋深。Ｐａｒｋｅｒ正、反演计算方法,兼有频率域里计算速度快,空间域计算准确的优点。该方法是重磁异常定量解释中有利工具,在平面解释中各层深度值连续性加强,适于煤田地质、油田地质普查阶段、高精度重磁勘探,定量解释、为后期钻探提供参考数据。  相似文献   

镜质组反射率Ro抑制及其校正研究     

李贤庆  钟宁宁 《中国煤田地质》1998,10(4):35-38

采用有机岩石学与有机地球化学相结合的分析方法,对新疆三塘湖盆地塘参３井自然演化剖面烃源岩样品进行了较详细的研究,  相似文献   

西湖凹陷西次凹古近系花港组—平湖组深层油气成藏过程          下载免费PDF全文

刘春锋  蒋一鸣  李宁  郭小波  马剑  张武  熊志武 《地质学报》2024,98(1):231-246

西湖凹陷西次凹古近系花港组和平湖组深层油气资源丰富，是东海陆架盆地勘探开发新领域，受储层差异致密化影响，油气成藏机理复杂。为了厘清西次凹深层油气成藏过程，本文通过流体包裹体岩相学特征、显微测温、激光拉曼光谱、包裹体所含油气地球化学等实验分析，结合构造演化、地层埋藏史、热史等，开展了系统的储层特征、油气成藏期次、成藏过程研究。结果表明，花港组深层（>4000 m）和平湖组储层均已致密化，溶蚀孔隙是主要的储集孔隙类型；花港组和平湖组均发育两期油气包裹体，早期含油包裹体较多，晚期以天然气包裹体为主，成藏时间分别为龙井运动期和冲绳运动期，以晚期天然气成藏最为关键。包裹体中油气地球化学特征类似，反映生烃母质以高等植物生源为主，低等生物为辅，与平湖组煤系烃源岩特征一致。冲绳运动叠加平湖组生气增压是晚期天然气成藏的主要动力，此时H10段及以上储层未致密化。根据储层致密化与成藏时序匹配关系可将西次凹M构造深层油气藏类型划分为常规型、先成藏后致密型、先致密后成藏型和边成藏边致密型4种。本文成果可为研究区下一步致密砂岩气的勘探开发部署提供重要的理论依据。  相似文献   

Eruption of an Active-Region Filament Driven by an Emerging Bipole     

Yun-Chun Jiang  Yuan-Deng Shen  Jing-Xiu Wang National Astronomical Observatories / Yunnan Observatory  Chinese Academy of Sciences  Kunming  National Astronomical Observatories  Chinese Academy of Sciences  Beijing 《中国天文和天体物理学报》2007,7(1):129-140

1 INTRODUCTION Filaments are cool, dense material suspended in the hot, tenuous corona. It is widely accepted that the global magnetic field surrounding the filaments plays a key role in their formation, structure and stability (Tandberg-Hanssen1995). Fil…  相似文献   

Populations of Bright X-ray Sources in the Starburst Galaxies NGC 4038/4039     

Xi-Wei Liu Xiang-Dong Li 《中国天文和天体物理学报》2007,7(3):389-396

Assuming a naive star formation history, we construct synthetic X-ray source pop- ulations, using a population synthesis code, for comparison with the observed X-ray lumi- nosity function (XLF) of the interacting galaxies NGC 4038/4039. We have included high- and intermediate-mass X-ray binaries, young rotation-powered pulsars and fallback disk-fed black holes in modeling the bright X-ray sources detected. We find that the majority of the X-ray sources are likely to be intermediate-mass X-ray binaries, but for typical binary evolu- tion parameters, the predicted XLF seems to be steeper than observed. We note that the shape of the XLFs depends critically on the existence of XLF break for young populations, and suggest super-Eddington accretion luminosities or the existence of intermediate-mass black holes to account for the high luminosity end and the slope of the XLF in NGC 4038/4039.  相似文献   

Evidence of the Link between Broad Emission Line Regions and Accretion Disks in Active Galactic Nuclei     

Yun Xu    Xin-Wu Cao Shanghai Astronomical Observatory  Chinese Academy of Sciences  Shanghai  Graduate School of Chinese Academy of Sciences  Beijing 《中国天文和天体物理学报》2007,7(1):63-70

1 INTRODUCTION Most bright active galactic nuclei (AGNs) exhibit broad emission lines, with full width at half maximum (FWHM ≥ 103 km s?1) (Peterson et al. 1999). Some type 1 AGNs could have very broad emission lines (FWHM≥ 20 000 km s?1). Type 2 AGNs s…  相似文献   

Seven-frequency VLBI Observations of the GHz-Peaked-Spectrum Source OQ 208     

Wen-Feng Luo Jun Yang Lang Cui Xiang Liu Zhi-Qiang Shen 《中国天文和天体物理学报》2007,7(5):611-619

We present quasi-simultaneous VLBI images of the GHz-Peaked-Spectrum radio source OQ 208 obtained with the Very Long Baseline Array at 1.4,1.7,2.3,5.0,8.4,15.4GHz and the European VLBI Network at 6.7 GHz.The low frequency(1.4,1.7 and 2.3GHz)ob- servations reveal a weak and extended steep-spectrum component at about 30mas away at position angle-110°,which may be a remnant emission.The radio structure of OQ 208 con- sists of two mini-lobes at 5.0,6.7,8.4 and 15.4 GHz.Our spectral analysis further confirms that the southwest lobe undergoes free-free absorption and finds that the free-free absorption is stronger in the inner region.By fitting the 8.4 GHz images from 1994 to 2005,we obtain a separation speed of 0.031±0.006 mas yr~(-1)between the two mini-lobes.This indicates a jet proper motion of 0.105±0.020 c and a kinematic age of 219±42 yr for the radio source.  相似文献   

准噶尔盆地南部下侏罗统三工河组沉积体系及其控制因素     

焦国华  张卫平  谢利华  王军  周晋科  汪云海 《古地理学报》2023,(3):628-647

下侏罗统三工河组是准噶尔盆地南部地区(南缘和腹部)的主要生产层段，但物源、沉积相类型、沉积体系分布演化及控制因素一直存在争议。综合运用露头、录井、岩心、测井及地震资料等，研究三工河组四级层序格架下物源、沉积体系类型、分布演化及控制因素。结果表明：物源变化、古地貌演化、构造和古气候条件共同控制了准噶尔盆地南缘及腹部早侏罗世沉积环境格局及充填过程。准噶尔盆地早侏罗世处于相对稳定的构造环境，古气候相对湿润。准噶尔盆地南缘东段及腹部形成了宽缓的大面积汇水区，发育来自西部扎伊尔山、哈拉阿拉特山、东部克拉美丽山的毯式浅水辫状河三角洲，来自天山造山带的毯式浅水扇三角洲和毯式浅水辫状河三角洲2种沉积环境，可划分为5大沉积体系；准噶尔盆地南缘西段为小而陡的汇水区，南侧发育来自天山的吉尔伯特式浅水扇三角洲，北侧发育来自扎伊尔山的吉尔伯特式浅水辫状河三角洲2种沉积环境，可划分为2大沉积体系；受古气候、沉积基准面和沉积作用的控制，三工河组二段1砂组为低位体系域，沉积基准面低，三角洲向湖延伸较远，砂体分布最广，向湖粒度变细；三工河组二段2砂组为湖侵体系域，三工河组一段为高位体系域，三角洲分布范围次之；三工河组三...  相似文献   

A Model for Contact Binary Systems     

Han-Feng Song Run-Qian Huang Shao-Lan Bi 《中国天文和天体物理学报》2007,7(4):539-550

A model for contact binary systems is presented, which incorporates the following special features: a) The energy exchange between the components is based on the understand-ing that the energy exchange is due to the release of potential, kinetic and thermal energies of the exchanged mass. b) A special form of mass and angular momentum loss occurring in contact binaries is losses via the outer Lagrangian point. c) The effects of spin, orbital rota-tion and tidal action on the stellar structure as well as the effect of meridian circulation on the mixing of the chemical elements are considered. d) The model is valid not only for low-mass contact binaries but also for high-mass contact binaries. For illustration, we used the model to trace the evolution of a massive binary system consisting of one 12M and one 5M star. The result shows that the start and end of the contact stage fall within the semi-detached phase during which the primary continually transfers mass to the secondary. The time span of the contact stage is short and the mass transfer rate is very large. Therefore, the contact stage can be regarded as a special part of the semi-detached phase with a large mass transfer rate. Both mass loss through the outer Lagrangian point and oscillation between contact and semi-contact states can occur during the contact phase, and the effective temperatures of the primary and the secondary are almost equal.  相似文献   

The Origin and Acceleration of ~3He and Heavy Ions in the 2000 July 14 Event     

Gui-Ping Wu  Guang-Li Huang  Yu-Hua Tang  Yu Dai Department of Physics  Southeast University  Nanjing  Purple Mountain Observatory  Chinese Academy of Sciences  Nanjing Department of Astronomy  Nanjing University  Nanjing 《中国天文和天体物理学报》2007,7(1):141-147

1INTRODUCTIONEnrichment of3He and heavy ions(i.e.,Ne,Mg,Si and Fe),characteristic of impulsive?ares,have beenstudied for more than three decades.It is found that they are generally associated with nonthermal energeticelectron-rich events(Reames et al.1988;Reames1999and references therein;Ho et al.2001;Wang et al.2006)and are related to the peculiar ratio of charge to mass(Mazur et al.1996;Reames1999).Althoughthe abundance of3He ions is not correlated with the abundance of heavy ions,s…  相似文献