潍北凹陷孔店组二段页岩气资源潜力分析          下载免费PDF全文

彭文泉 《山东国土资源》2016,32(11)

潍北凹陷是昌潍坳陷的次一级凹陷盆地,也是胜利油田外围常规油气开采区。潍北凹陷孔店组二段发育了较厚的暗色泥页岩,是页岩气形成最有利层段,也是常规油气的生烃母岩。利用昌页参1井数据,结合以往资料,对潍北凹陷孔店组二段岩性特征,有机地球化学特征、矿物组成、泥页岩含气性特征等进行分析研究,认为孔店组二段上亚段下部和中亚段下部具备页岩气资源勘查开发潜力。  相似文献   

A permeability–porosity relationship for mudstones     

Yunlai Yang  Andrew C. Aplin 《Marine and Petroleum Geology》2010

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南堡凹陷4号构造带蛤坨断层特征与油气成藏关系   总被引：1，自引：0，他引：1  

张华文  周江羽  刘德志  刘国超  何雅娟 《海洋地质译丛》2010,(2):14-18,22

南堡凹陷4号构造带断裂发育,既发育沟通烃源岩的深断裂,也发育沟通浅层圈闭的次级断裂。综合利用地震、测井、岩性等资料分析断层的空间展布,计算蛤坨断层的生长指数和断层泥比率（SGR）,分析断层的活动性、封堵性,评价其输导性能,并结合其与烃源岩生排烃期的匹配关系研究断裂与油气运移、聚集的关系及控制规律。在典型油气藏剖面解剖的基础上,建立了4号构造带油气运聚成藏模式。  相似文献   

Towards a new standard model for black hole accretion     

Zdenka Kuncic  Geoffrey V. Bicknell 《Astrophysics and Space Science》2007,311(1-3):127-135

We briefly review recent developments in black hole accretion disk theory, emphasizing the vital role played by magnetohydrodynamic (MHD) stresses in transporting angular momentum. The apparent universality of accretion-related outflow phenomena is a strong indicator that large-scale MHD torques facilitate vertical transport of angular momentum. This leads to an enhanced overall rate of angular momentum transport and allows accretion of matter to proceed at an interesting rate. Furthermore, we argue that when vertical transport is important, the radial structure of the accretion disk is modified at small radii and this affects the disk emission spectrum. We present a simple model demonstrating how energetic, magnetically-driven outflows modify the emergent disk emission spectrum with respect to that predicted by standard accretion disk theory. A comparison of the predicted spectra against observations of quasar spectral energy distributions suggests that mass accretion rates inferred using the standard disk model may be severely underestimated.  相似文献   

黑洞熵可以量子化吗?     

汪定雄 《中国天文和天体物理学报》1991,(1)

在黑洞蒸发的最后阶段其残余质量为Planck质量的量级,因而所对应的黑洞熵为2πk_B量级,在Bekenstein工作的基础上作者导出在吸积物质的过程中黑洞的最小熵增为2πk_B,这一最小熵增又限制能参与吸积物质的黑洞的质量下限为Planck质量的量级,因而所对应的最小黑洞熵也为2πk_B这一量级。作者进一步指出:黑洞的最小熵及最小熵增不受引力常数G变化的影响,因此上述结论在极早期宇宙中也能成立,在上述分析的基础上作者提出一个猜想:黑洞熵可以量子化,其量子单位为2πk_B。  相似文献   

辽宁省中晚元古代—中生代页岩的化学元素丰度及其演化特征     

张耀华 《国土资源》1991,(3)

作者利用全省不同地质时代和不同地质构造单元内的页岩41种元素的分析数据,计算出辽宁省全域内的页岩元素丰度休系。同时探讨了元素从中、晚元古代至中生代的演化规律,指出Ca、Cd、Sb、As、Na、Mn、P、Sr的元素丰度随时间序列的演化不断增长,B、F、K、Rb、W、Mg则显示出降低的趋势。某些元素比值从老至新表现出明显的规律性变化,如Sr/Ba、Ca/Mg值的演化具有阶段性,K/Na、Th/U值的演化具有方向性,Al/Ti值的演化则具有周期性。  相似文献   

Why the fundamental plane of black hole activity is not simply a distance driven artifact     

A. Merloni  E. Krding  S. Heinz  S. Markoff  T. DiMatteo  H. Falcke 《New Astronomy》2006,11(8):567-576

The fundamental plane of black hole activity is a non-linear correlation among radio core luminosity, X-ray luminosity and mass of all accreting black holes, both of stellar mass and supermassive, found by Merloni et al. [Merloni, A., Heinz, S., di Matteo, T. 2003. MNRAS 345, 1057 (MHD03)] and, independently, by Falcke et al. [Falcke, H., Körding, E., Markoff, S., 2004. A& A 414, 895]. Here we further examine a number of statistical issues related to this correlation. In particular, we discuss the issue of sample selection and quantify the bias introduced by the effect of distance in two of the correlated quantities. We demonstrate that the fundamental plane relation cannot be a distance artifact, and that its non-linearity must represent an intrinsic characteristic of accreting black holes. We also discuss possible future observational strategies to improve our understanding of this correlation.  相似文献   

吸积盘谱讨论     

李家锦  樊军辉 《天文研究与技术》1993,(3)

本文用数值方法讨论了吸积盘谱与黑体谱的形状和谱指数。结果表明:对于吸积盘用F_v∝v~(1/3)作为其特征谱是不合适的;同时Frank等(1985)所得到的解析式F_v∝v~2也是不正确的。  相似文献   

鄂尔多斯盆地南部延长组长7油组页岩层系天然裂缝发育特征及主控因素     

李彦录  陆诗磊  夏东领  吕文雅  梁丰  唐磊  李睿琦  王磊飞 《地质科学》2022,57(1):73-87

利用地表露头、岩心、薄片和测井资料,对鄂尔多斯盆地南部长7油层组陆相页岩层系天然裂缝的成因类型、发育特征和主控因素进行研究。按地质成因,鄂尔多斯盆地南部长7油层组页岩层系的天然裂缝可以分为构造裂缝和成岩裂缝两大类,其中构造裂缝主要包括剪切裂缝和张性裂缝;成岩裂缝主要包括层理缝、页理缝和收缩裂缝。不同岩性中的天然裂缝发育情况明显不同,致密砂岩中以构造裂缝为主,层理缝仅在粉砂岩和局部细砂岩中发育;页岩和凝灰岩中页理缝、层理缝和构造裂缝均比较发育。不同类型的天然裂缝主控因素明显不同,构造裂缝的发育主要受岩性和岩石力学层层厚控制;砂岩中层理缝的发育主要受碳质纹层、粘土矿物转化程度等因素控制;凝灰岩中层理缝的发育主要受刚性玻屑脱玻化作用的控制;页岩中页理缝的发育主要受纹层、TOC含量和黄铁矿含量的控制。  相似文献   

Taphonomy of large marine vertebrates in the Upper Cretaceous (Cenomanian-Turonian) Tropic Shale of southern Utah     

《Cretaceous Research》2015

Sediments from the Upper Cretaceous (Cenomanian-Turonian) Tropic Shale were deposited along the western margin of the Western Interior Seaway, in present-day southern Utah. Marine vertebrates from this formation include plesiosaurs, mosasaurs, bony fish, sharks, and turtles. They are concentrated in the lower portion of the Tropic Shale, mostly between Bentonites B and D. Study of the taphonomic condition of these vertebrates has contributed to an understanding of how they were preserved as well as a detailed paleoenvironment for the Tropic Shale. Physical factors played the dominant role in their preservation, with robust and durable skeletal elements, such as teeth and vertebrae, being most common within the shale. Isolated bones and teeth are also relatively common within the formation, while complete and nearly complete skeletons are more rare. Biological factors played a less dominant role, with no evidence of epifaunal or infaunal activity preserved with any of the skeletal remains. In addition, scavenging marks (both bite and gnaw marks) are relatively uncommon, typically only being found on more complete specimens. A signature of post-burial alteration can be recognized as low levels of abrasion, weathering, and compression and high levels of fracturing of vertebrate skeletal material. Slightly higher levels of abrasion and weathering occur to the west, closer to the ancient shoreline, suggesting some pre-burial alteration. The preservation of marine vertebrates in the Tropic Shale suggests a low energy marine environment with some weak bottom currents and low levels of benthic oxygen. The substrate ranged from soft and soupy to firm, with moderate sedimentation rates resulting in relatively rapid burial.  相似文献