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从世界古生界油气保存条件看我国海相盆地的勘探潜力 总被引:1,自引:2,他引:1
世界含油气盆地的统计数据表明,保存条件对于古生界油气有着压倒一切的重要性。首先是盆地的保存,其次是油气系统的保存。高保存的古生代盆地在形成后基本上未发生构造逆转和岩浆侵入或溢出,在中、新生代沉积和侵蚀作用大体处于平衡,因而盆地实体较完整,一般均上覆有相当厚度的中、新生界。中保存盆地虽经一定程度的构造逆转,但古生界层序的基本格局仍然存在,而且在中、新生代再次接受了一定厚度的沉积,因而仍有可观的产油气潜力。低保存盆地多已发生强烈构造逆转和广泛岩浆活动,盆地实体比较破碎或已全面出露,其含油气性大大下降。油气系统的保存主要涉及油气生成、聚集后大地构造作用的强度和区域封盖层的有效性。我国古生代海相盆地的油气保存条件具有西优东差和北强南弱的特点,其中塔里木、鄂尔多斯和四川盆地大体属于中保存盆地,而中、下扬子和滇黔桂等地区似已进入低保存状态。中保存的三大盆地已分别有可观的油气发现,而且仍有进一步勘探的潜力。对于低保存的南方海相分布区,则需作深入分析。从国外此类盆地的勘探经验看,寻找构造逆转程度较低的区域或次级构造单元,也许是我国南方海相领域获得油气发现的关键,但所发现的可能以小油气田为主。 相似文献
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Melchiorri A Ade PA de Bernardis P Bock JJ Borrill J Boscaleri A Crill BP De Troia G Farese P Ferreira PG Ganga K de Gasperis G Giacometti M Hristov VV Jaffe AH Lange AE Masi S Mauskopf PD Miglio L Netterfield CB Pascale E Piacentini F Romeo G Ruhl JE Vittorio N 《The Astrophysical journal》2000,536(2):L63-L66
We use the angular power spectrum of the cosmic microwave background, measured during the North American test flight of the Boomerang experiment, to constrain the geometry of the universe. Within the class of cold dark matter models, we find that the overall fractional energy density of the universe Omega is constrained to be 0.85=Omega=1.25 at the 68% confidence level. Combined with the COBE measurement, the data on degree scales from the Microwave Anisotropy Telescope in Chile, and the high-redshift supernovae data, we obtain new constraints on the fractional matter density and the cosmological constant. 相似文献
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Modern ground water characterization and remediation projects routinely require calibration and inverse analysis of large three-dimensional numerical models of complex hydrogeological systems. Hydrogeologic complexity can be prompted by various aquifer characteristics including complicated spatial hydrostratigraphy and aquifer recharge from infiltration through an unsaturated zone. To keep the numerical models computationally efficient, compromises are frequently made in the model development, particularly, about resolution of the computational grid and numerical representation of the governing flow equation. The compromise is required so that the model can be used in calibration, parameter estimation, performance assessment, and analysis of sensitivity and uncertainty in model predictions. However, grid properties and resolution as well as applied computational schemes can have large effects on forward-model predictions and on inverse parameter estimates. We investigate these effects for a series of one- and two-dimensional synthetic cases representing saturated and variably saturated flow problems. We show that "conformable" grids, despite neglecting terms in the numerical formulation, can lead to accurate solutions of problems with complex hydrostratigraphy. Our analysis also demonstrates that, despite slower computer run times and higher memory requirements for a given problem size, the control volume finite-element method showed an advantage over finite-difference techniques in accuracy of parameter estimation for a given grid resolution for most of the test problems. 相似文献
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油气田微磁异常成因及性质研究的近期进展 总被引:1,自引:0,他引:1
微磁测量是80年代出现的一种成功的非常规油气勘探方法,它所检测的是与油气渗漏相关的次生磁性矿化作用。近期的大量研究表明,油气田上方的微磁乒常具有复杂多样的成因:(1)从烃类获得代谢能的硫酸盐还原茵的作用;(2)烃类的微生物降解作用;(3)硫化环境中形成的磁黄铁矿;(4)泥质岩中富铁粘土的自生菱铁矿化;(5)与油气源岩露头或油气藏渗漏有关的自燃变质带。此外,烃类在陆相红层中的磁效应可以受到赤铁矿溶离的干扰,使其磁化强度出现数量级的下降。 相似文献
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