Residual oil as a tool in migration and filling history analysis of petroleum reservoirs,Ghazal Field,Saudi Arabia     

Khaled R. Arouri  Salah H. Al-Saleh  Ziyad M. Al-Hilal 《Organic Geochemistry》2009,40(5):617-627

Stepwise extraction and molecular analysis of non-recoverable oil from intact reservoir core plugs is used to provide constraints on the accumulation history of petroleum in the Permo-Carboniferous Unayzah reservoirs at the Ghazal Field, Saudi Arabia. When integrated with existing tools such as oil geochemistry, gas geochemistry, stable carbon isotopes, fluid inclusions and thermal modeling, the sequential extraction approach helped decode a previously unrecognized component of the hydrocarbon accumulation history. In particular, it indicates that the region received early petroleum charges that were less mature than currently produced light oil and gas condensates, possibly from the prolific Early Silurian Qusaiba shale source rock and other sources. This has significant implications for prospecting for additional oil, particularly in the north/northwest of the Ghazal region where paleo-oil accumulations may have been displaced or spilled. The lower portion of the Unayzah reservoir (Unayzah-C) remained water-wet during early filling of the upper reservoir unit (Unayzah-A) and appears to have been filled only by a late oil charge. Anomalous molecular and carbon isotopic behavior of residual oil extracts from the uppermost segment of the Unayzah reservoir, where the free oil (first of the sequential extracts) is less mature (0.95% Rc) and isotopically lighter (δ¹³C?31.15‰) than the adsorbed oil (last sequential extract, 1.05% Rc; δ¹³C?29.65‰), suggests a late oil contribution or bitumen contamination from the overlying Khuff Formation.  相似文献   

Exchange of gravitational energy during a collision of galaxies     

K. Shankara Sastry  Saleh Mohamed Alladin 《Astrophysics and Space Science》1970,7(2):261-271

The problem of the change in internal energy of a colliding galaxy due to tidal effects is considered, assuming that the galaxies may be regarded as spherical stellar systems whose over-all structure remains unchanged during the collision and that the stars move in circular orbits. The numerical estimates thus made for the energy gained by the stars during the collision are compared with those derived on the basis of the assumption that the motions of the stars may be neglected during the encounter (the impulsive approximation) to test the adequacy of the latter approximation. If the two galaxies are of 10¹¹ M , of radii 10 kpc and of mass distribution that of a polytrope of indexn=4; and if the relative distance and velocity at their closest approach are taken as 2 kpc and 1000 km/sec respectively, the mass of escaping stars from a galaxy is estimated to be roughly 4% of the total mass of the galaxy and the total increase in the internal energy of a galaxy during the collision due to the tidal acceleration of all its stars is equal in magnitude to approximately 25% of its initial internal energy, about one-fifth of which is associated with the escaping stars.  相似文献   

The dynamics of head-on collisions of spherical stellar systems     

K. S. V. S. Narasimhan  Saleh Mohammed Alladin 《Astrophysics and Space Science》1986,128(2):307-317

Energy changes in a head-on collision between two unequal Plummer model stellar systems (galaxies) are studied analytically under the impulsive approximation. The variation of the disruptive effects within and the mass escape from systems widely differing in mass and scalelength ratios are determined and some physical implications regarding the dynamical stability of the systems undergoing head-on collisions are indicated. It is found that if two systems differ considerably in size, both systems generally survive the collision if (i) the mass of the bigger is greater than about six times the mass of the smaller and (ii) the density of the smaller is more than about twenty-five times the entity of the bigger system, when the velocity at minimum separation is equal to the parabolic velocity of escape.  相似文献   

Integration of RADARSAT and GIS modelling for estimating future Red River flood risk   总被引：1，自引：0，他引：1  

Michael Stephen Chubey  Salah Hathout 《GeoJournal》2004,59(3):237-246

A new geomatics-based approach for flood prediction was developed and used to model the magnitude and spatial extent of a future Red River flood in southern Manitoba. This approach combines the statistical modelling capabilities of Markov (non-spatial) analysis and logistic regression (spatial) within a geographic information system (GIS) environment, utilizing modelling inputs derived from remotely sensed RADARSAT imagery and other digital geographic data. The 1997 Red River flood was the second largest in recorded history, and the largest for which accurate data are available. The results indicate: (i) a flood “one time interval-in terms of 3 days time unit measurement- larger in area” than the 1997 flood is expected to affect 17.6% more land (an additional 47.6 km²) within the study area compared to 1997 levels based on Markovian probability derived from observations from the 1997 event; and (ii) the majority of this excess flooding will take place on agricultural land; no additional communities are expected to be at risk. Quantitative assessment verified the capability of this modelling approach for producing statistically significant results. The methodology used in this research would be easily transferable to other areas, and may provide the basis for a viable alternative to conventional hydrologic-based flood prediction approaches This revised version was published online in August 2006 with corrections to the Cover Date.  相似文献   

Soil moisture retrievals from biangular L-band passive microwave observations     

Wigneron  J.-P. Calvet  J.-C. de Rosnay  P. Kerr  Y. Waldteufel  P. Saleh  K. Escorihuela  M.J. Kruszewski  A. 《Geoscience and Remote Sensing Letters, IEEE》2004,1(4):277-281

A simple approach for correcting the effect of vegetation in the estimation of soil moisture (w/sub S/) from L-band passive microwave observations is presented in this study. The approach is based on statistical relationships, calibrated from simulated datasets, which requires only two observations made at distinct incidence angles (/spl theta//sub 1/,/spl theta//sub 2/). A sensitivity study was carried out, and best retrieval remote sensing configurations, in terms of polarization and couple of incidence angles (/spl theta//sub 1/,/spl theta//sub 2/), were investigated. Best estimations of w/sub S/ could be made at H polarization, for /spl theta//sub 1/ varying between 15/spl deg/ and 30/spl deg/, and with a difference (/spl theta//sub 2/-/spl theta//sub 1/) larger than 30/spl deg/. The method was tested against two experimental datasets acquired over crop fields (soybean and wheat). The average accuracy in the soil moisture retrievals during the whole crop cycle was found to be about 0.05 m/sup 3//m/sup 3/ for both crops.  相似文献   

Sustainable development and international cooperation in the Eastern Nile Basin     

Salah El-Din Amer  Yacob Arsano  Atta El-Battahani  Osman El-Tom Hamad  Magdy Abd El-Moenim Hefny  Imeru Tamrat  Simon A. Mason 《Aquatic Sciences - Research Across Boundaries》2005,67(1):3-14

  相似文献   

An intercomparison between the GSWM, UARS, and ground based radar observations: a case-study in January 1993     

S. E. Palo  M. E. Hagan  C. E. Meek  R. A. Vincent  M. D. Burrage  C. McLandress  S. J. Franke  W. E. Ward  R. R. Clark  P. Hoffmann  R. Johnson  D. Kürschner  A. H. Manson  D. Murphy  T. Nakamura  Yu. I. Portnyagin  J. E. Salah  R. Schminder  W. Singer  T. Tsuda  T. S. Virdi  Q. Zhou 《Annales Geophysicae》1997,15(9):1123-1141

The Global-Scale Wave Model (GSWM) is a steady-state two-dimensional linearized model capable of simulating the solar tides and planetary waves. In an effort to understand the capabilities and limitations of the GSWM throughout the upper mesosphere and thermosphere a comparative analysis with observational data is presented. A majority of the observational data used in this study was collected during the World Day campaign which ran from 20 January to 30 January 1993. During this campaign data from 18 ground-based observational sites across the globe and two instruments located on the UARS spacecraft were analyzed. Comparisons of these data with the simulations from the GSWM indicate that the GSWM results are in reasonable agreement with the observations. However, there are a number of cases where the agreement is not particularly good. One such instance is for the semidiurnal tide in the northern hemisphere, where the GSWM estimates may exceed observations by 50%. Through a number of numerical simulations, it appears that this discrepancy may be due to the eddy diffusivity profiles used by the GSWM. Other differences relating to the diurnal tide and the quasi-two-day wave are presented and discussed. Additionally, a discussion on the biases and aliasing difficulties which may arise in the observational data is alos presented.  相似文献   

Ground-water quality of the Nile west bank related to soil characteristics and geological setting     

A. Saleh  F. M. Al-Ruwiah  M. Shehata 《Journal of Arid Environments》2001,49(4):761

The objective of this study is to outline how the ground-water quality is affected by geological factors, soil characteristics and subsurface structure. The results of 25 ground-water samples, and 30 soil samples of which 10 soil samples analysed chemically provide the basis of this study. Procedures to interpret water quality data are based on a combined use of the traditional graphical methods, ratios of Na⁺/Cl⁻and Ca²⁺/Mg²⁺, multivariate geostatistical methods and computation of the saturation indices (SI) of minerals. The results of soil analyses show that the grain size ranges from very coarse sand to clayey loams, and from well sorted and extremely poorly sorted. The soil salinity increases in old alluvial plains and decreases in the dissected wadis of limestone plateaux, while vertical distribution decreases with depth. It is found that the ground-water is supersaturated with respect to calcite and dolomite, and undersaturated with respect to gypsum. Calculated values of P_CO2for the ground-water samples range from 2×10⁻⁴to 7×10⁻³with a mean value of 3×10⁻³(atm.). This indicates that the ground-water becomes charged with CO₂during infiltration processes.  相似文献   

Les minéralisations ferrifères du Sahara Algerien: le gisement de fer oolithique de Mecheri Abdelaziz (bassin de Tindouf)     

Salah Guerrak  Jean Jacques Chauvel 《Mineralium Deposita》1985,20(4):249-259

Résumé Le gisement de fer oolithique de Mecheri Abdelaziz (Famennien terminal du bassin de Tindouf), présente des caractères morphologiques et sédimentologiques qui permettent de penser que la minéralisation s'est mise en place dans des édifices deltaïques progradants.La minéralisation est complexe et comprend trois paragenèses principales; maghémite-magnétite, bavalite-hématite, bavalite-magnétite et quatre faciès types: faciès microconglomératique (FMC), faciès à oolithes dispersées dans une matrice détritique (FOD), faciès à oolithes dispersées dans une matrice non détritique (FOND) et faciès à oolithes jointives, cimentées (FOC).Les caractères des oolithes et de la mésostase montrent que les corps minéralisés résultent de l'accumulation d'oolithes, développées essentiellement par concrétionnement intrasédimentaire et ayant subi, avant le dépôt définitif, des phases alternantes d'oolithisation et de remise en suspension.Sur l'ensemble du gisement, les teneurs moyennes sont les suivantes: Fe total: 43,49%; SiO₂=13,66%; P₂O₅=2,31%; CaO=5,35%.En ce qui concerne la source du fer, il semble que la mise en place du minerai soit liée aux importantes réserves de quartzites ferrugineux situées dans le Précambrien du socle Réguibat, dont le stock métal initial a subi des remobilisations successives.

---

The Mecheri Abdelaziz oolitic iron deposit (late Famennian of Tindouf Basin) shows morphological and sedimentological features of prograding deltaic sequences.The mineralization is complex and allows the recognition of 3 types of paragenesis: maghemite-magnetite, bavalite-hematite, bavalite-magnetite; and 4 types of facies: microconglomerate facies, oolites dispersed in a matrix with detritic elements, oolites dispersed in a matrix without detritic elements and oolites with cement.The comparison of oolites and matrix suggests that the orebodies are the result of oolites deposition, developed by intrasedimentary processes and before the final deposition, by alternating phases of oolitization and suspension.For the whole ore deposit, the main composition is: total Fe=43.49%; SiO₂=13.66%; P₂O₅=2.31%; CaO=5.35%.The major portion of iron was probably provided by continental leaching of the very important iron formations of the Precambrien Reguibat shield.

  相似文献   

Geologic relationships and mineralization of peralkaline/alkaline granite-syenite of the Zargat Na''am ring complex, Southeastern Desert, Egypt     

Gehad M. Saleh 《中国地球化学学报》2006,25(2)

The Zargat Na'am ring complex crops out 90 km NW of Shalatin City in the Southeastern Desert of Egypt. The ring complex forms a prominent ridge standing high above the surrounding mafic-ultramafic hills. It is cut by two sets of joints and faults which strike predominantly NNW-SSE and E-W,and is injected by dikes, porphyritic alkaline syenites, and felsite porphyries. It consists of alkali syenites, alkali quartz syenites, and peralkaline arfvedsonite-bearing granitic and pegmatitic dikes and sills.The complex is characterized locally by extreme enrichments in REEs, wolframite and rare, high field strength metals (HFSM), such as Zr and Nb. The highest concentrations ( 1.5 wt% Zr, 0.25 wt% Nb,0.6 wt% ∑REEs) occur in aegirine-albite aplites that formed around arfvedsonite pegmatites. Quartzhosted melt inclusions in arfvedsonite granite and pegmatite provide unequivocal evidence that the peralkaline compositions and rare metal enrichments are primary magmatic features. Glass inclusions in quartz crystals also have high concentrations of incompatible trace elements including Nb (750 × 10-6), Zr (2500 × 10-6) and REEs (1450 × 10-6). The REEs, Nb and Zr compositions of the aegirine-albite aplites plot along the same linear enrichment trends as the melt inclusions, and Y/Ho ratios mostly display unfractionated, near-chondritic values. The chemical and textural features of the aegirine-albite aplites are apparently resultant from rapid crystallization after volatile loss from a residual peralkaline granitic melt similar in composition to the melt inclusions.  相似文献