基于球体层状介质模型的大地电磁正演

目前大地电磁测深法的一维正演理论,是基于平面波垂直入射水平层状介质的假设模型。但由于地球是一个球体,因此有必要研究基于球状介质模型的大地电磁正演理论。这里详细推导了基于球体层状介质模型的大地电磁正演公式,计算了若干理论模型。通过同基于水平层状介质模型的大地电磁正演结果对比,验证了正演公式的正确性。同时,指出当探测周期增加到上万秒时,阻抗相位会增大;而当探测周期增加到数十万秒时,视电阻率会减小。     

The Haraa Gol terrane in the western Hentiyn Mountains (northern Mongolia): geochemistry,geochronology, and geodynamics

According to geological, petrological, geochemical, and geochronological studies, the Haraa Gol terrane in the western Hentiyn Mts. is dominated by two rock assemblages of different ages, associated with the initiation and development of the island arcs and marginal spreading seas of the Mongol–Okhotsk Ocean. The Late Cambrian, Early Ordovician, and Middle Ordovician were marked by the effusion of basalt and basaltic andesite and the formation of gabbro and gabbro-dolerite in back-arc spreading basins. In the Late Silurian–Devonian, after a short pause, tectonomagmatic processes were activated, with the formation of differentiated island-arc volcanics, gabbro, and granitoids. Their absolute ⁴⁰Ar–³⁹Ar age is given in the paper. The model age of the T_Nd(DM) protolith of the Haraa Gol igneous rocks corresponds to the composition of the Mesoproterozoic juvenile crust.     

Ulvöspinel from xenoliths of contact-altered volcanic and volcanosedimentary rocks in nepheline syenites of the Khibiny and Lovozero plutons

Ulvöspinel is a typical accessory mineral of xenoliths of volcanic and volcanosedimentary rocks in alkaline syenites of the Khibiny and Lovozero plutons. Ulvöspinel forms homogeneous Cr- and V-rich grains in slightly altered olivine basalts, basaltic tuffs, and tuffites and is enriched in Mn and Si in the course of contact-metasomatic alteration of these rocks. The strongly reduced conditions of contact metamorphism controlled by ascending flows of hydrocarbon gases and hydrogen sulfide gave rise to the subsolidus decomposition of primary ulvöspinel and Ti-high magnetite with the formation of ilmenite lamellae and then, with decreasing redox potential, of the second-generation latticed ulvöspinel lamellae.     

Physical parameters and dynamical properties of the multiple system ι UMa (ADS 7114)

We analyze the physical parameters, orbital elements, and dynamic stability of the multiple system ?? UMa (HD 76644 = ADS 7114). We have used the positions from the WDS catalog and our own observations on the 6-m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences and the 1.5-m Russian-Turkish Telescope (Antalya, Turkey). We have obtained more precise orbital parameters of the subsystems, and spectral types, absolute magnitudes, and masses of the components. The primary has Sp = F0 V?CIV, M = 1.7 ± 0.1M _??, T _eff = 7260 ± 70 K, and log g = 4.30 ± 0.07. The companion in the close Aa subsystem is most likely a white dwarf with a mass of approximately 1.0 ± 0.3M _??. The spectral types and masses of the components in the BC subsystem are M3V, M4V and 0.35 ± 0.05M _??, 0.30 ± 0.05M _??, respectively. The total mass is 3.4 ± 0.4M _??. The Aa subsystem probably has an orbital period of 4470^d = 12.2^y and an eccentricity of approximately 0.6. The outer subsystem seems to have a period of approximately 2084 yrs and an eccentricity of approximately 0.9. We have carried out simulations using the stability criteria and shown that for all possible variations in the component parameters, the multiple system is unstable on a time scale of less than 10⁶ years with a probability exceeding 0.98. Possible reasons for this instability are discussed.     

Structural and magnetic microinhomogeneities in accessory spinel of the system Fe2+(Cr2–xFex3+)O4 from the Kytlym massif (Urals platinum-bearing belt)

The microstructure and magnetic properties of accessory Fe–Cr-spinels from the Kytlym massif of the Urals platinum-bearing belt were studied. Atypical Fe–Cr-spinels in the form of magnetic microareas in grains of primary nonmagnetic Fe–Cr-spinel have been revealed for the first time in the bed dunites of the Kytlym multiphase concentrically zoned massif, North Urals. These spinels are responsible for the magnetic properties of the dunites. It has been established that the microareas are separations in solid solution Fe²⁺(Cr_2–xFe_x³⁺)O₄, which are enriched in Fe^3 + and are probably an intermediate product of the transformation of primary accessory Fe-Cr-spinel during the formation of the dunite massif. These are magnetic microphases with particular chemical composition, cation distribution, and corresponding reversed crystal lattice, which determine the main magnetic properties of the microarea: the magnitude and direction of magnetization vector and Curie temperature. The formation of this earlier unknown type of magnetic Fe–Cr-spinel is probably conjugate with the formation and concentration of PGE mineralization in the bed dunites of the Kytlym platinum-bearing massif. The presence of such magnetization carriers in rocks and ores must be taken into account in geophysical research at the Urals chromite and platinum–chromite deposits.     

Mineralogy and Mineral Chemistry of the Cretaceous Duolong Gold‐Rich Porphyry Copper Deposit in the Bangongco Arc,Northern Tibet

The Early Cretaceous Duolong gold‐rich porphyry copper deposit is a newly discovered deposit with proven 5.38 Mt Cu resources of 0.72% Cu and 41 t gold of 0.23 g t^?1 in northern Tibet. Granodiorite porphyry and quartz diorite porphyrite are the main ore‐bearing porphyries. A wide range of hydrothermal alteration associated with these porphyries is divided into potassic, argillic and propylitic zones from the ore‐bearing porphyry center outward and upward. In the hydrothermal alteration zones, secondary albite (91.5–99.7% Ab) occurs along the rim of plagioclase phenocryst and fissures. Secondary K‐feldspar (75.1–96.9% Or) replaces plagioclase phenocryst and matrix or occurs in veinlets. Biotite occurs mainly as matrix and veinlet in addition to phenocryst in the potassic zone. The biotite are Mg‐rich and formed under a highly oxidized condition at temperatures ranging from 400°C to 430°C. All the biotites are absent in F, and have high Cl content (0.19–0.26%), with log (X_Cl/X_OH) values of ?2.74 to ?2.88 and IV (Cl) values of ?3.48 to ?3.35, suggesting a significant role of chloride complexes (CuCl₂^‐ and AuCl₂^‐) in transporting and precipitating copper and gold. Chlorites are present in all alteration zones and correspond mainly to pycnochlorite. They have similar Fe/(Fe+Mg), Mn/(Mn+Mg) ratios, and a formation temperature range of 280–360°C. However, the formation temperature of chlorite in the quartz‐gypsum‐carbonate‐chlorite vein is between 190°C and 220°C, indicating that it may have resulted from a later stage of hydrothermal activity. Fe³⁺/Fe²⁺ ratios of chlorites have negative correlation with Al^IV, suggesting oxygen fugacity of fluids increases with decreasing temperature. Apatite mineral inclusions in the biotite phenocrysts show high SO₃ content (0.44–0.82%) and high Cl content (1–1.37%), indicating the host magma had a high oxidation state and was enriched in S and Cl. The highest Cl content of apatite in the propylitic zone may have resulted from pressure decrease, and the lowest Cl content of apatite in the argillic zone may have been caused by a low Cl content in the fluids. The low concentration of SO₃ content in the hydrothermal apatite compared to the magmatic one may have resulted from the decrease of oxygen fugacity and S content in the hydrothermal fluid, which are caused by the abundant precipitation of magnetite.     

天然气藏He的累积模式及定年应用初探

天然气藏He的聚集存在一定的年代累积效应,借鉴相关地质模型,引入气藏特征参数,对外部壳源以及气藏原位产生的He进行量化,明确天然气藏中He累积量与时间的数学关系,进而建立了约束天然气藏形成时代的新方法——He定年模型。将该方法应用于四川盆地威远气田,估算威远震旦系天然气成藏定型的时间约为31Ma,对应渐新世,处于喜马拉雅运动中期。该结果与威远气田成藏过程的研究成果相吻合,表明天然气藏He的年代累积效应可以用于成藏时代的研究,所建立的He定年模型具有一定的实用性和应用潜力。     

东濮凹陷上古生界致密砂岩优质储层发育特征及主控因素

文章探讨了东濮凹陷上古生界砂岩优质储层形成的主控因素,为预测优质储层提供依据。文章以东濮凹陷庆古3井为主要研究对象,通过岩心观察、铸体薄片、XRD、核磁共振冻融法及三束离子抛光—场发射扫描电镜联用等综合分析,研究了东濮凹陷二叠系储层发育特征及控制因素。研究表明：东濮凹陷上古生界砂岩以岩屑长石和长石岩屑砂岩为主,孔隙度值介于0.2%~12.8%,渗透率值介于0.0016~5.7 mD,属于特低孔致密型储层。溶蚀残余粒间孔、粒内溶蚀孔、晶间孔是东濮凹陷主要发育的孔隙类型,储集空间都是次生成因,各层段几乎未见原生孔隙留存,裂缝相对不发育。次生孔隙主要由长石颗粒和岩屑（包括凝灰质）溶蚀形成,在石千峰组和下石盒子组储层中较为常见。优质储层受沉积相、岩性和成岩作用的控制,石千峰组砂岩属于内陆河流相沉积,砂体发育,是东濮凹陷上古生界最有利的储集层系,长石的溶蚀是石千峰组优质储层形成的主要控制因素。下石盒子组属于三角洲沉积,由于沉积时期火山作用,导致大量的凝灰质沉积,凝灰质蚀变形成的高岭石晶间孔是该层储层形成的重要机制。山西组主要三角洲沉积,也是主要成煤期,煤系酸性流体导致溶蚀,但强烈的石英次生加大使砂岩致密化。