东营凹陷现今大规模超压系统整体分布特征及主控因素

东营凹陷为超压富烃凹陷, 钻井揭示该凹陷现今大规模超压系统出现在始新统沙三-四段烃源岩层系.根据大量的钻杆测试(DST)数据, 实测沙三-四段砂岩异常高压的深度范围约在2 200~4 400 m, 剩余压力约为4~40 MPa, 压力系数为1.2~1.99.根据钻井和测井以及地震速度资料解释, 超压带钻井泥浆密度明显增加, 超压泥岩层具有偏离正常趋势的异常高声波时差测井响应和异常低地震层速度响应特征.综合解释超压系统顶界面埋深在2 200~2 900 m, 对应地温在90~120 ℃; 超压顶界面深度随着烃源岩层系顶界埋深的增加而增加.超压系统范围内烃源岩层系样品镜质体反射率(R_o)分布在0.5%~1.2%, 沙三中、下亚段-沙四上亚段成熟烃源岩(R_o为0.5%~1.2%)及其生油作用控制了超压分布的主体区域, 佐证了东营凹陷现今大规模超压发育区与烃源岩生油增压有成因联系; 成熟烃源岩的累积厚度、埋深及热成熟度是超压系统整体分布特征和超压发育幅度的主控因素; 断裂系统和输导性砂体对东营凹陷沙三-四段烃源岩层系中发育的大规模超压系统的分布特征和结构变化具有重要影响.      

云南滇池流域强烈灌溉条件下西芹大棚土壤水分动态特征

利用TRIME-T3型TDR仪土壤含水量测量系统和WM-1型负压计系统现场监测了强烈灌溉条件下整个作物生长期西芹大棚土壤水分、土壤负压(基质势)的动态变化;研究表明,不同深度土壤含水量受强烈灌溉的影响程度不同,0.3 m深度处受影响最大,1.0,2.0 m深度处受影响最小;受灌溉的影响,0.3,0.6,1.0 m深度处负压有所波动,其中0.3 m深度处负压的波动幅度最大;2.0 m深度处的土壤一直处于"饱和-非饱和"两种状态的转换之中;在地下水埋深为2.0 m左右,且上部土层的渗透性较差(饱和渗透系数仅为0.04 m/d)的情况下,地下水水位受灌溉的影响极小.     

多种剥蚀厚度恢复方法在内蒙古雅布赖盆地侏罗系和白垩系中的应用及其地质意义

剥蚀厚度恢复是进行盆地埋藏史、热演化史、油气成藏等定量分析的基础。文中利用镜质体反射率法、流体包裹体法、声波时差法和地层厚度趋势法等多种方法,恢复了内蒙古雅布赖盆地侏罗系和白垩系剥蚀厚度。计算结果表明,侏罗系和白垩系总剥蚀厚度为1610.9~2177.0,m;在流体包裹体法和地层厚度趋势法约束下,恢复的侏罗系剥蚀厚度为930.2~1395.3,m,白垩系剥蚀厚度为0~612.1,m。雅布赖盆地侏罗系剥蚀厚度“北大南小”,白垩系剥蚀厚度“南大北小”,反映盆地改造强度具有晚侏罗世南弱北强、早白垩世南强北弱的特征。大规模隆升剥蚀,导致地层温度下降、烃源岩遭到破坏,一定程度上制约着雅布赖盆地的烃源岩成熟演化以及油气生成。     

台北凹陷葡北—葡萄沟地区七克台组低幅度构造特征与油气成藏分析

从低幅度构造识别的影响因素出发,采用地震正演模拟技术对吐哈盆地台北凹陷葡北—葡萄沟地区侏罗系七克台组低幅度构造特征进行分析,并以主要成藏期七克台组古地貌特征和沉积相分布特征进行低幅度构造成藏模式分析。研究表明:葡北—葡萄沟地区侏罗系七克台组低幅度构造识别受其埋藏深度和上覆地层平均速度的控制和影响,埋藏较浅且平均速度较小是低幅度构造易于识别的重要特征;该区火焰山断裂和七克台组上部泥岩控制着低幅度构造的垂向运移,缓坡带断裂结合七克台上部的泥岩盖层控制着葡北地区低幅度构造侧向运移+垂向运移的成藏模式。     

The diagenetic history of some septarian concretions from the Kimmeridge Clay, England

ABSTRACT
Large septarian concretions from the Kimmeridge Clay, up to 1.2 m in diameter, have centres comprising anhedral calcite microspar passing into margins of radiating fibrous calcite microspar, with a pyrite-rich zone at the transition. Septarian veins formed and were lined with brown calcite synchronously with fibrous matrix growth, with white calcite precipitated in septarian cavities after concretion growth ceased. Septarian veins, filled only with white calcite, formed later, at the same time as the outermost calcite microspar crystals were enlarged.
The concretions were buried in the Late Jurassic to about 130 m, and in the Late Cretaceous to about 550 m, with uplift between. Oxygen isotopes show that the concretion grew throughout the first burial, with septarian veins forming from about 30 m depth onwards. Later septarian veins formed between about 200 and 500 m during the second burial.
Carbon isotopes show that the compact inner matrix grew in the sulphate reduction zone, the end of which is marked by the pyrite-enriched zone. Dissolving shells, and possibly minor methanogenic carbonate, slowly diluted sulphate reduction-zone carbonate during deeper burial. During early concretion growth, Mg and Sr were depleted in the pore water. During later stages of the first burial, Mg, Sr, Mn and Fe all increased, especially after concretion growth ceased. During the second burial, Fe, Mn and Mg decreased as calcite precipitated, implying relatively closed systems for these elements.
Synchronous formation of septarian fractures and fibrous calcite matrix shows that the Kimmeridge Clay became overpressured during the later stages of both burials.     

Some effects of compaction and geological time on the pore parameters of argillaceous rocks

Graphical statistics have been applied to the pore-size distribution curves of argillaceous rocks to characterize the changes in pore parameters that result from compaction and geological time. The most striking characteristic of recently deposited sediment is the high variability in mean pore size and in the sorting and skewness of the pore system. The mean pore size ranges from 15 to 980 nm, sorting ranges from very well sorted to poorly sorted, and skewness varies from systems in which small pores predominate over large ones to systems in which large pores predominate. This high variability in pore structure represents the many environmental and mineral-related variables that affect the pore system of newly deposited sediment. The mean pore size of shales decreases with increasing compaction and approaches a limiting value of about 3·5 nm at depth. Within a geological time span of 50 m.y. and/or depth of burial of about 1200 m, most sediments have reached an irreversible, well sorted pore-size distribution. Early diagenetic processes apparently affect the skewness of pore systems more than compaction, such that within about 50 m.y. the pore system is negatively skewed, with small pores predominating over large. Sediments buried to a depth of 500 m or less exhibit a porosity range of 40--85%; below 500 m, porosity decreases linearly with burial depth. No correlation exists between the surface area of shale pore systems and depth of burial, geological age, and the pore parameters mean pore size, sorting, and skewness.     

Carbonate diagenesis of the upper Jurassic successions in the west of Binalud — Eastern Alborz (NE Iran)

The upper Jurassic carbonate settings in Iran are widely exposed in north and northeastern parts. Five stratigraphic columns were selected in the north eastern Iran. Their thickness ranges from 330 to 500 m. The various diagenetic processes identified include, micritization, cementation, compaction (physical and chemical), dissolution, neomorphism, pyritization, hematitization, silicification and dolomitization, which affected these carbonates. Elemental and stable isotopes analysis indicated that these deposits have undergone both meteoric and burial diagenesis in a relatively open system with moderate water-rock interaction. The positive trend between trace elements and oxygen isotope depletion also support these burial conditions. Lighter δ^l8O values of the dolomite samples may be related to an increase in temperature during the burial, which correspond to coarser euhedral crystals. Relatively higher δ¹⁸O values in finer dolomite crystals indicate their formation at lower burial depths relative to coarser crystals. Petrographic evidences such as coarse euhedral crystals with bright and dull zonation prove this interpretation. Chert nodules also have lighter ¹⁸O values relative to carbonate host rock, thus indicating the influence of burial diagenetic processes in their formation. The average environmental palaeotemperature was estimated to be 26°C on the basis of oxygen isotope values of less altered lime-mudstones.     

川西岷江河谷典型大型—巨型古滑坡特征物探解译分析

在遥感解译、野外调查的基础上,采用高密度电法和电阻率测深法,并结合钻探对川西岷江河谷发育的尕米寺滑坡、俄寨村滑坡、格机寨滑坡等典型大型—巨型古滑坡的空间结构进行了勘探分析,有效确定了古滑坡的空间结构和滑带特征,并认为古滑坡的滑动面多具有高低阻相间的不稳定电性层,且滑坡前缘多位于不稳定电性层变薄收敛的地方。其中,俄寨村滑坡高低阻相间的不稳定电性层厚约0~45 m,为滑坡堆积层,古滑动面紧贴基岩面,滑动面平均埋深约30 m,弱风化基岩面埋深约5.6~61 m,强风化层厚约为3~12 m;尕米寺滑坡高低阻相间的不稳定电性层厚约2.5~43 m,为滑坡堆积层,沿剖面古滑动面平均埋深约35 m,在滑坡中部存在一圈闭的低阻异常体,推测为古河道,并与钻探结果相吻合,其埋深约56~96 m,弱风化基岩面埋深13.3~100 m,强风化及岩溶综合层厚一般约为5~20 m。基于古滑坡的地球物理勘探数据和解译结果,统计分析了川西岷江河谷地区大型—巨型古滑坡空间岩土体的地球物理物性参数,对指导该区滑坡调查分析具有重要的指导意义。     

祁南矿东风井冻结温度场时空演化规律分析

以安徽祁南矿东风井冻结法凿井为工程背景,以多圈管冻结的不同土性表土层为研究对象,基于冻结孔实际成孔位置,应用有限元软件COMSOL Multiphysics分别建立埋深218 m钙质黏土层位、埋深225 m细砂层位和埋深259 m砂质黏土层位3个不同土性、不同埋深的冻结温度场数值计算模型,并结合现场实测数据,分层计算分析了其冻结壁温度场时空演化规律,结果表明：在相同冻结条件下,埋深225 m细砂层位冻结壁有效平均温度比埋深259 m砂质黏土层位和埋深218 m钙质黏土层位分别低0.09～0.72℃和0.44～1.95℃,埋深225 m细砂层位平均有效厚度比埋深259 m砂质黏土层位和埋深218 m钙质黏土层位分别厚0.17～0.38 m和0.29～0.47 m;现场实测与数值计算均表明,各个层位冻结壁开挖时,其平均温度均低于–15℃,有效厚度均大于6.2 m,200 m以下深部表土层井帮温度低于–4℃,满足施工要求,冻结壁强度和稳定性均处于安全状态;冻结孔沿径向将冻结温度场划分为3个区域(A区、B区、C区),B区在冻结孔冷量叠加的影响下降温速度最快,A区降温速度适中,C区距离冻结管较远...     

Surface history of lunar soil and soil columns

Measurements of cosmic ray track densities are presented for soil samples from Apollo 15, 16 and 17. Median track densities are used to infer total effective exposure times within ~15 cm of the lunar surface. Minimum track densities are used to derive the time of the last impact-produced rearrangement of soil grains. For samples from near various craters ages are derived of 40 m.y. for St. George, 6 (±3) m.y. for S. Ray, 25–90 m.y. for Plum, and 20–35 m.y. for Shorty. The material of 15003. the Apollo 15 deep core at depths of 120–160 cm, is inferred to have been deposited at an average rate of ≥0.35 cm/m.y. The Apollo 16 core at 41–47 cm depths. 60007, appears to be well mixed and was covered up by deposition at 0.3 cm/m.y. for the next few m.y. after its deposition.     

潞安矿区构造－热演化特征

通过对潞安矿区区域地质背景研究,在镜质体反射率测试分析的基础上,对研究区多个井田含煤地层的埋藏史及其热史进行了恢复。结果表明,早三叠世-侏罗纪,研究区构造运动强烈,埋深增大至3 500 m左右,经历较高古地温（120~135℃）,热流达到第一个峰值（76~89 mW/m2）;侏罗纪晚期-早白垩世,受燕山期火山运动及深层侵入岩影响,研究区含煤地层温度骤升至160~180℃并伴随出第二个古热流峰值（90~99 mW/m2）。通过比对,认为沁水盆地东南缘潞安矿区所处构造-热演化程度较沁水盆地中部偏高。      

高速铁路大断面黄土隧道深浅埋分界深度研究

郑州-西安铁路客运专线穿越西部黄土分布的主要地区,该线含大量单洞双线隧道,其开挖面积大于160 m2,跨度大于15 m,属于超大断面隧道。由于黄土的特殊性质以及开挖跨度与断面的增大,隧道围岩压力随埋深的变化尚不清楚,目前对该类型隧道的深、浅埋分界深度界定认识不统一。通过郑西线12座隧道地表裂缝与埋深关系的现场调查,初步确定了大断面黄土隧道的深、浅埋分界范围,指出小于11 m可作为超浅埋,40～60 m为浅埋与深埋分界深度,大于60 m为深埋;基于裂缝调查,按剪切滑移破坏极限状态理论对以上分界范围进行了理论分析与验证;精心设计现场试验,在浅、深埋等地段布置17个量测断面进行围岩-初期支护间接触压力的量测,发现实测围岩压力与界定的深浅埋计算结果吻合良好,表明所给深、浅埋界定范围正确。     

雄安新区白洋淀湿地地表水和地下水转化关系及其对芦苇分布的影响

查明地表水和地下水作用关系对湿地生态保护与修复具有重要意义。采用地表水和地下水位监测、氢氧稳定同位素分析、湖床沉积物温度示踪等方法,研究了白洋淀渗漏对周边浅层地下水的影响范围和深度,评价了地表水垂向渗漏速率,并探讨了芦苇分布面积和地表水位以及地下水位埋深的关系。结果表明：白洋淀渗漏受地质结构和水力梯度等因素影响,对浅层地下水垂向上影响深度为20 m,水平向上影响范围存在较大空间变异。周边浅层地下水的补给来源为大气降雨和地表水,其中地表水渗漏的补给比例为0~90.5%。淀区渗漏速率0.01~0.59 mm/d,和含水层埋深关系密切,埋深越小,越有利于地表水渗漏。1976-2020年,白洋淀芦苇分布面积和地表水位关系密切。当地表水位为6.3~6.8 m时,芦苇分布面积最大,在水位小于6.3 m条件下芦苇面积随着水位增高而增加,大于6.8 m条件下随着水位增高而减少。芦苇台地下水位埋深和地表水位显著相关,在2020年4-9月芦苇生长期,除雨季前期外多数时段台地地下水埋深均适宜芦苇发育,建议在雨季前期实施生态补水,通过降低台地地下水位埋深促进芦苇生长发育。研究结果可为白洋淀生态补水、渗漏防治和生态保护提供参考。     

Stable and clumped isotopes in desert carbonate spring and lake deposits reveal palaeohydrology: A case study of the Lower Jurassic Navajo Sandstone,south‐western USA

Carbon, oxygen and clumped isotope (Δ₄₇) values were measured from lacustrine and tufa (spring)‐mound carbonate deposits in the Lower Jurassic Navajo Sandstone of southern Utah and northern Arizona in order to understand the palaeohydrology. These carbonate deposits are enriched in both ¹⁸O and ¹³C across the basin from east to west; neither isotope is strongly sensitive to the carbonate facies. However, ¹⁸O is enriched in lake carbonate deposits compared to the associated spring mounds. This is consistent with evaporation of the spring waters as they exited the mounds and were retained in interdune lakes. Clumped isotopes (Δ₄₇) exhibit minor systematic differences between lake and tufa‐mound temperatures, suggesting that the rate of carbonate formation under ambient conditions was moderate. These clumped isotope values imply palaeotemperature elevated beyond reasonable surface temperatures (54 to 86°C), which indicates limited bond reordering at estimated burial depths of ca 4 to 5 km, consistent with independent estimates of sediment thickness and burial depth gradients across the basin. Although clumped isotopes do not provide surface temperature information in this case, they still provide useful burial information and support interpretations of the evolution of groundwater locally. The findings of this study significantly extend the utility of combining stable isotope and clumped isotope methods into aeolian environments.     

Meganodular anhydritization: a new mechanism of gypsum to anhydrite conversion (Palaeogene–Neogene,Ebro Basin,North‐east Spain)

A number of Palaeogene to Early Neogene gypsum units are located along the southern margins of the Ebro Basin (North‐east Spain). These marginal units, of Eocene to Lower Miocene age, formed and accumulated deposits of Ca sulphates (gypsum and anhydrite) in small, shallow saline lakes of low ionic concentration. The lakes were fed mainly by ground water from deep regional aquifers whose recharge areas were located in the mountain chains bounding the basin, and these aquifers recycled and delivered Ca sulphate and Na chloride from Mesozoic evaporites (Triassic and Lower Jurassic). In outcrop, the marginal sulphate units are largely secondary gypsum after anhydrite and exhibit meganodules (from 0·5 to >5 m across) and large irregular masses. In the sub‐surface these meganodules and masses are mostly made of anhydrite, which replaced the original primary gypsum. The isotopic composition (11·1 to 17·4‰ for δ¹⁸O_VSMOW; 10·7 to 15·3‰ for δ³⁴S_VCDT) of secondary gypsum in this meganodular facies indicates that the precursor anhydrite derived from in situ replacement of an initial primary gypsum. As a result of ascending circulation of deep regional fluid flows through the gypsum units near the basin margins, the gypsum was partly altered to anhydrite within burial conditions from shallow to moderate depths (from some metres to a few hundred metres?). At such depths, the temperatures and solute contents of these regional flows exceeded those of the ground water today. These palaeoflows became anhydritizing solutions and partly altered the subsiding gypsum units before they became totally transformed by deep burial anhydritization. The characteristics of the meganodular anhydritization (for example, size and geometry of the meganodules and irregular masses, spatial arrangement, relations with the associated lithologies and the depositional cycles, presence of an enterolithic vein complex and palaeogeographic distribution) are compared with those of the anhydritization generated both in a sabkha setting or under deep burial conditions, and a number of fundamental differences are highlighted.     

Quaternary exhumation history of the NE Tibetan Plateau revealed by peculiar distributions of polycyclic aromatic hydrocarbons in core extracts from the Sanhu depression,eastern Qaidam basin

Reworked organic matter (ROM) has been frequently encountered in fresh organic matter (FOM) in young sedimentary basins. Our study reports an ROM-dominated sequence from 21 borehole cores of the Late Pliocene–Quaternary strata in the Sanhu depression of the eastern Qaidam basin in northwestern China. Reworked organic matter occurrence is confirmed by Rock-Eval pyrolysis results, high Ro values, and reversed polyaromatic hydrocarbon (PAH) maturity trends showing elevated maturities. Rock–source correlation using molecular fingerprints of biomarkers shows ROM was derived from Jurassic freshwater lacustrine source rocks dominated by terrestrial input, contrasting the immature Quaternary FOM developed in anoxic, saline lacustrine facies. The ROM provenance is traced northward to the southern Qilian Mountains. Maximum burial depths of ROM prior to erosion have been inferred by a burial depth–Rc (calculated vitrinite reflectance) correlation. Two chronological boundaries (1.83 Ma and 3.12 Ma) displaying distinct biomarker fingerprints are obtained from a previously reported chronological framework in the study area. Accordingly, an eroded thickness of 1214 m and an average erosion rate of 94 cm/ka of the ROM provenance areas during this temporal interval are derived. Our study has illustrated the potential value of geochemical compositions of ROM with constrained provenances in investigating the exhumation history of a mountain.     

四川盆地川中地区中下侏罗统砂岩储层异常致密成因机理

四川盆地川中地区中下侏罗统砂岩储层现今埋藏深度一般在1 500～3 000 m,但砂岩致密化程度异常偏高,其平均孔隙度小于5%,平均渗透率小于1×10-3μm2,为典型的超低孔、超低渗储层。岩石显微镜下成岩作用特征及压实与胶结作用的减孔强度统计结果显示,强压实作用（包括压溶作用）是导致砂岩储层异常致密的主要原因。利用砂...     

Stable isotope evidence for multiple fluid regimes during carbonate cementation of the Upper Tertiary Hazeva Formation, Dead Sea Graben, southern Israel

Stable carbon- and oxygen-isotope compositions of calcite and dolomite cements have been used to understand porewater evolution in the Upper Tertiary Hazeva Formation within the Dead Sea Graben, southern Israel. Sandstone samples were obtained from four boreholes in three tectonic blocks of the graben over depths of 253–6448 m, a variation that largely reflects differential subsidence of individual fault-bounded blocks. Early carbonate cements dominate diagenesis. Calcite occurs at <1600 m, but was replaced by dolomite at greater depths. Dolomite at 1600–2700 m is Fe-poor (<0.8 mol% FeCO₃), and at 4700–6200 m, Fe-rich (0.5–7.2 mol% FeCO₃). Magnesite, anhydrite and halite are the final diagenetic phases. Calcite has positively correlated δ¹⁸O (+21‰ to +25‰) and δ¹³C (−6‰ to −2‰) values that generally decrease with depth. Dolomite has a wider variation in δ¹⁸O (+18‰ to +30‰) and δ¹³C (−8‰ to −1‰) values, which also generally are lower with increasing depth. However, the δ¹³C and δ¹⁸O values of dolomite from the uppermost 400 m of the Hazeva Formation in the Sedom Deep-1 borehole are anomalous in spanning the entire range of stable carbon and oxygen isotopic compositions over this relatively small interval.The decreasing dolomite δ¹³C values likely indicate an increased contribution of carbon from organic sources with increasing depth. Except for the uppermost 400 m, Hazeva Formation dolomite in the Sedom Deep-1 borehole has stable carbon-isotope compositions that imply initial dolomitization at much shallower levels, prior to the preferential subsidence of this tectonic block. The oxygen isotopic compositions of the calcite cement are best explained by equilibration at present burial temperatures (≤55 °C) with porewater of meteoric origin. Its δ¹⁸O values increased from −5‰ at the shallowest depths to 0‰ at 1600 m. The dolomite oxygen isotopic compositions also reflect equilibration at present burial temperatures with porewaters ranging from 0‰ at 1600 m to +7‰ at 3600 m (100 °C). In the deepest fault block (Sedom Deep-1 borehole), however, increasingly Fe-rich dolomite has (re)equilibrated with porewater whose δ¹⁸O values decreased from +9‰ at 4750 m (120 °C) to +1‰ to +2‰ by 6200 m (150 °C).Much of the dolomite likely formed at relatively shallow depths from saline brines derived from precursors to the Dead Sea. These infiltrated the Hazeva Formation, mixing with and largely displacing meteoric water, and dolomitizing calcite. Rock–water ratios tended to be high during these processes. However, the upper 400 m of the Hazeva Formation in the deepest fault block were likely deposited during its rapid tectonic subsidence, and largely escaped the initial style of dolomitization pervasive elsewhere in the study area. These sediments were also capped by evaporites. This relatively thin interval likely became a preferential conduit for brines that escaped underlying and overlying strata, including the Fe-rich, lower ¹⁸O fluids (evolved seawater?) present in the deepest part of the graben. These rocks present the most promising target for the passage and accumulation of hydrocarbons in the study area.     

天津滨海地区晚新生代地层自然固结与地面沉降研究

天津滨海地区地处渤海湾西岸,晚新生代沉积了巨厚的松散沉积物。地下水位下降、地层自然固结、地表载荷的加速增长等复合因素造成了严重的地面沉降。利用在天津滨海新区塘沽地区施工的一眼1 226 m全取芯钻孔,通过原状样品测试分析,系统研究了晚新生代土层的物理力学性质、黏性土固结特征,并结合欠固结黏性土层沉降量计算等方法阐述了土层固结状态空间特征,探讨了土层固结特征与地面沉降的相关关系。结果表明：该地区0～100 m深度土层具有低天然密度、高孔隙比、高含水率、高压缩性等特点,表现出软土的性质,在地表荷载增大的情况下,易发生地面沉降;100～550 m的黏性土大都处于超固结和微超固结状态,主要是由于过去地下水的大量开采造成的;550 m以下的黏性土多为正常固结,局部存在欠固结黏性土夹层。钻孔中存在合计约218 m的欠固结黏性土夹层,这些欠固结黏性土夹层在自重应力下的最终沉降量为1 985 mm,沉降量最大的土层对应于第1、6含水组,分别达614 mm和665 mm,这一沉降过程完成所需时间为数十年甚至上百年。     

准噶尔盆地腹部侏罗系超压特征和测井响应以及成因

准噶尔盆地腹部地区深层钻井揭示侏罗系发育异常高压系统.根据26口井的67个钻杆测试(DST) 和电缆测试(MDT) 数据, 实测砂岩异常高压揭示深度约在4470~6160m, 剩余压力约为11~57MPa, 压力系数为1.24~2.07, 砂岩段超压实测值主要分布在侏罗系, 少数出现在白垩系底部与侏罗系邻近地层, 1个超压实测值位于下三叠统, 实测超压砂岩样品的孔隙度和渗透率范围分别为3.20%~16.00%和0.02×10-3~14.40×10-3μm2;根据钻井、测井和测试资料的综合解释, 埋深在4430~6650m的深部侏罗系流体超压带, 钻井泥浆密度明显增加, 泥页岩和砂岩共同具有相对于正常趋势的异常高声波时差和低视电阻率测井响应特征; 超压系统顶界埋深可能不浅于4400m (地温约104℃), 有些钻井超压顶界可深达约6000m (地温约140℃), 且超压带顶界深度随侏罗系埋深的增加而增大; 钻井揭示的侏罗系超压带烃源岩镜质体反射率(R_o, %) 约为0.7%~1.3%, 超压带分布深度受控于侏罗系成熟烃源岩层的埋深且两者深度分布的变化具有相关性; 研究认为腹部地区已被充分压实的侏罗系异常高压成因主要与其含煤岩系干酪根热演化及油气共生有关, 即生烃增压; 物理模拟实验表明, 由于高孔隙流体压力可导致岩石骨架颗粒间有效应力的减小, 从而直接引起通过岩石的声波速度降低, 即出现高声波时差响应; 在超压地层温度条件下, 高压液态水的电离常数可能明显增加, 从而减小地层电阻率, 进一步开展此种现象的相关探索性研究可望对超压带低电阻率异常的原因给出新的解释.