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针对石南31井区储层岩性多变、油气水关系复杂等问题,按不同岩性识别油气层、水层和干层,据油气不同测井响应特征进一步识别油层和气层.将储层划分为细砂岩、中粗砂岩和砂砾岩3类,识别储层流体性质,分析油藏分布特征,指出油层、隔夹层平面分布特征,探讨油气水层分布规律.结果表明,石南31井区主要有4个油藏.储层所含流体有油、水和气,中北部细砂岩储层为纯油层,南部中粗砂岩储层为水层.气层从南到北分布于全区,主要位于油藏北部和东部局部区域,为今后解释工作具很好指导意义. 相似文献
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Fourteen acoustic Doppler current profilers (ADCPs) were deployed on the shelf and slope for 1 year just west of the DeSoto Canyon in the Northeastern Gulf of Mexico by the Naval Research Laboratory (NRL) as part of its Slope to Shelf Energetics and Exchange Dynamics (SEED) project. The winter and spring observations are discussed here in regards to the low-frequency current variability and its relation to wind and eddy forcing. Empirical orthogonal function (EOF) analyses showed that two modes described most of the current variability. Wind-forced variability of the along-shelf flow was the main contributor in Mode 1 while eddies contributed much of the variability in Mode 2. Wind-stress controlled currents on the shelf and slope at time scales of about a week. On longer time scales, variations in the currents on both the outer shelf and slope appear to be related to seasonal variations in the time-cumulated wind stress curl. Winds were dominant in driving the along-shelf transports, particularly along the slope. However, the effective wind stress component was found to be aligned with the west Florida shelf direction rather than the local shelf direction. Eddy intrusions, which were more numerous in winter and spring than in summer and fall, and winds were found to contribute significantly to cross-shelf exchange processes. 相似文献
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通过对环境标准样进行31P-NMR测试,研究了磷的化学结构与化学位移的关系.结果表明:无机正磷酸盐(PO43-)化学位移在6.412×10-6,焦磷酸盐的化学位移在-4.353×10-6;多聚磷的化学位移分布特点是:主链末端磷化学位移在-3.53×10-6至-4.40×10-6之间,中间磷在-18.159×10-6至-20.246×10-6之间,有机磷中单酯和二醑的化学位移分别在4.3540×10-6至6.3652×10-6和-0.107×10-6至2.195×10-6之间,部分二脂不稳定,会降解为单脂;膦酸盐的化学位移在18.670×10-6至21.460×10-6之间,磷酸肌酸位于-0.380×10-6,有机多聚磷中α-P的化学位移在-8.833×10-6至-9.449×10-6之间,由于偶合作用产生P峰的裂分,P峰的偶合符合核磁中n 1的规则.结构环境影响31P的化学位移值的偏移. 相似文献
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Jun Ma ;Richard de Grijs ;Zhou Fan ;Soo-Chang Rey ;Zhen-Yu Wu ;Xu Zhou ;Jiang-Hua Wu ;Zhao-Ji Jiang ;Jian-Sheng Chen ;Kyungsook Lee ;Sangmo Tony Sohn 《天体物理学报》2009,(6):641-652
Mayall Ⅱ = G1 is one of the most luminous globular clusters （GCs） in M31. Here, we determine its age and mass by comparing multicolor photometry with theoretical stellar population synthesis models. Based on far- and near-ultraviolet GALEX photometry, broad-band UBVRI, and infrared JHKs 2MASS data, we construct the most extensive spectral energy distribution of G 1 to date, spanning the wavelength range from 1538 to 20 000A. A quantitative comparison with a variety of simple stellar population （SSP） models yields a mean age which is consistent with G1 being among the oldest building blocks of M31 and having formed within ～1.7 Gyr after the Big Bang. Irrespective of the SSP model or stellar initial mass function adopted, the resulting mass estimates （of order 10^7M⊙） indicate that GI is one of the most massive GCs in the Local Group. However, we speculate that the cluster＇s exceptionally high mass suggests that it may not be a genuine GC. Our results also suggest that G1 may contain, on average, （1.65±0.63） × 10^2L⊙ far-ultraviolet-bright, hot, extreme horizontal-branch stars, depending on the adopted SSP model. In addition, we demonstrate that extensive multi-passband photometry coupled with SSP analysis enables one to obtain age estimates for old SSPs that have similar accuracies as those from integrated spectroscopy or resolved stellar photometry, provided that some of the free parameters can be constrained independently. 相似文献
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