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1.
Summary The Aguablanca Ni-Cu-(PGE) magmatic sulphide deposit is associated with a magmatic breccia located in the northern part of the Aguablanca gabbro (SW, Iberia). Three types of ores are present: semi-massive, disseminated, and chalcopyrite-rich veined ore. The principal ore minerals are pyrrhotite, pentlandite and chalcopyrite. A relatively abundant platinum-group mineral (PGM) assemblage is present and includes merenskyite, melonite, michenerite, moncheite and sperrylite. Moreover, concentrations of base and precious metals and micro-PIXE analyses were obtained for the three ore-types. The mineralogy and the mantle-normalised chalcophile element profiles strongly suggest that semi-massive ore represents mss crystallisation, whereas the disseminated ore represents an unfractionated sulphide liquid and the chalcopyrite-rich veined ore a Cu-rich sulphide liquid. Palladium-bearing minerals occur commonly enclosed within sulphides, indicating a magmatic origin rather than hydrothermal. The occurrences and the composition of these minerals suggest that Pd was initially dissolved in the sulphides and subsequently exsolved at low temperatures to form bismutotellurides. Negative Pt and Au anomalies in the mantle-normalised chalcophile element profiles, a lack of Cu-S correlation and textural observations (such as sperrylite losing its euhedral shape when in contact with altered minerals) suggest partial remobilisation of Pt, Au and Cu by postmagmatic hydrothermal fluids after the sulphide crystallisation. Authors’ addresses: R. Pi?a, L. Ortega, R. Lunar, Departamento de Cristalografía y Mineralogía, Facultad de Geología, Universidad Complutense de Madrid, ES-28040 Madrid, Spain; F. Gervilla, Facultad de Ciencias, Instituto Andaluz de Ciencias de la Tierra, Universidad de Granada-CSIC, Avda. Fuentenueva, s/n, ES-18002 Granada, Spain  相似文献   
2.
Soupy and mousse-like fabrics are disturbance sedimentary features that result from the dissociation of gas hydrate, a process that releases water. During the core retrieval process, soupy and mousse-like fabrics are produced in the gas hydrate-bearing sediments due to changes in pressure and temperature conditions. Therefore, the identification of soupy and mousse-like fabrics can be used as a proxy for the presence of gas hydrate in addition to other evidence, such as pore water freshening or anomalously cool temperature. We present here grain-size results, mineralogical composition and magnetic susceptibility data of soupy and mousse-like samples from the southern Hydrate Ridge (Cascadia accretionary complex) acquired during Leg 204 of the Ocean Drilling Program. In order to study the relationship between sedimentary texture and the presence of gas hydrates, we have compared these results with the main textural and compositional data available from the same area. Most of the disturbed analyzed samples from the summit and the western flank of southern Hydrate Ridge show a mean grain size coarser than the average mean grain size of the hemipelagic samples from the same area. The depositional features of the sediments are not recognised due to disturbance. However, their granulometric statistical parameters and distribution curves, and magnetic susceptibility logs indicate that they correspond to a turbidite facies. These results suggest that gas hydrates in the southern Hydrate Ridge could form preferentially in coarser grain-size layers that could act as conduits feeding gas from below the BSR. Two samples from the uppermost metres near the seafloor at the summit of the southern Hydrate Ridge show a finer mean grain-size value than the average of hemipelagic samples. They were located where the highest amount of gas hydrates was detected, suggesting that in this area the availability of methane gas was high enough to generate gas hydrates, even within low-permeability layers. The mineralogical composition of the soupy and mousse-like sediments does not show any specific characteristic with respect to the other samples from the southern Hydrate Ridge.  相似文献   
3.
The main goal of this paper is to show that the elliptic restricted three-body problem has ejection-collision orbits when the mass parameter µ is small enough. We make use of the blow up techniques. Moreover, we describe the global flow of the elliptic problem when µ = 0 taking into account the singularities due to collision and to infinity.  相似文献   
4.
Periodic orbits in the Stormer problem are studied using the symmetry lines of the Poincaré map introduced by De Vogelaere. Many known facts are explained by mean of these lines. The dynamics of four special symmetry lines when the Stormer parameter 1 changes is presented, and we obtain a clear global view of the structure of the simple periodic orbits and their bifurcations, including the asymmetrical ones. New asymmetrical multiple periodic orbits are obtained.  相似文献   
5.
用混合和扩散云室对大气冰核浓度的观测分析   总被引:3,自引:0,他引:3  
杨绍忠  王祥国  游来光  皮家雄 《气象》2004,30(12):39-43
继1963年用混合云室对春季冰核浓度观测之后,1994~1996年,在同季节、同地点用混合和静力扩散云室又做了同步观测。对取得的资料进行整理分析,得出了凝华核浓度在不同天气背景下占总冰核浓度的百分比,两种云室测值的对应关系;分析了扩散云室的容积效应及冰核浓度随气压、能见度等气象因子的变化。  相似文献   
6.
7.
Wang  Minfang  Zhang  Xubo  Guo  Xiaonan  Pi  Daohui  Yang  Meijun 《Mineralogy and Petrology》2018,112(1):85-103
Mineralogy and Petrology - Electron probe microanalysis (EPMA) results are reported for newly identified silver–bearing minerals from the Xinhua deposit, Yunkaidashan area, South China. The...  相似文献   
8.
9.
洞庭湖区第四纪气候变化的初步探讨   总被引:14,自引:0,他引:14  
探讨了洞庭湖区第四纪以来的气候变化,初步得出以下规律:更新世气候变化剧烈,气候组合暖湿(温湿)与冷干;全新世气候转为温凉,主要气候组合为温湿与凉干;历史时期气候主要仍温湿与凉干交替,但15 世纪以来出现短暂的温干与凉温期;15世纪以来,气候波动频繁,有愈来愈不稳定的趋向,进入20世纪,旱涝灾害更加。在全球变暖的背景下,预计该区未来气候趋向于暖湿,但不排除暖干的可能性。  相似文献   
10.
论三峡工程对洞庭湖区土壤潜育化和沼泽化的影响   总被引:1,自引:0,他引:1  
皮建高 《湖南地质》1995,14(1):58-60
三峡工程完工后,在坝下长江水位抬高的季节里,顶托洞庭湖的排泄,使东、西洞庭湖地段地表、地下水位相应抬高,对这些地区土壤的潜育化和沼泽化有明显影响,农业部门应引起重视。  相似文献   
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