Petrogenesis of the Az Zabirah south zone bauxite ore deposits,central northern Saudi Arabia     

Al-Mutairi  Abdulaziz N.  Galmed  Mahmoud A.  Aldamegh  Khaled S. 《Arabian Journal of Geosciences》2015,8(4):2327-2339

Arabian Journal of Geosciences - The bauxite ore deposits are mainly found around the Az Zabirah area in the central northern part of Saudi Arabia. The age of the Az Zabirah bauxites was suggested...  相似文献   

Carbonate inclusions in Lower Cretaceous picrites from the Hončova hůrka Hill (Czech Republic,Outer Western Carpathians): Evidence for primary magmatic carbonates?     

Kamil Kropáč  Zdeněk Dolníček  David Buriánek  Tomáš Urubek  Vlastimil Mašek 《International Journal of Earth Sciences》2015,104(5):1299-1315

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The Momentum 4-Vector Imparted by Gravitational Waves in Bianchi-Type Metrics     

Ali Havare  Murat Korunur  Mustafa Salti 《Astrophysics and Space Science》2006,301(1-4):43-46

Considering the Møller, Weinberg and Qadir-Sharif's definitions in general relativity, we find the momentum 4-vector of the closed universe based on the Bianchi-type metrics. The momentum 4-vector (due to matter plus fields) is found to be zero. This result supports the viewpoints of Albrow and Tryon and extends the previous works by Cooperstock–Israelit, Rosen, Johri et al., Banerjee–Sen and Vargas who investigated the problem of the energy in Friedmann–Robertson–Walker universe and Salt?-Havare who studied the problem of the energy-momentum of the viscous Kasner-type space-times.  相似文献   

Geoelectrical and Hydrogeochemical Studies for Delineating Ground-Water Contamination Due to Salt-Water Intrusion in the Northern Part of the Nile Delta, Egypt   总被引：3，自引：0，他引：3  

Abdel-Azim M. Ebraheem  Mahmoud M. Senosy  Kamal A. Dahab 《Ground water》1997,35(2):216-222

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Temperature variations of one well-known UV ceti type flare star     

Farouk M. Mahmoud 《Astrophysics and Space Science》1995,234(1):107-123

Temperature variations of the flare star, EV Lac, at its quiet-state luminosity were computed from its colour indices,B - V, which were measured in Johnson's system, these daily temperature changes are the essential reason of the short-term behaviour appearance in the flare star which is due to the presence of active region(s) causing a temperature difference of a few hundred degrees from the photosphere. A correlation between the annual mean of temperature variations of the flare star at its quiet-state and the annual rate of some physical parameters of the flare star at its active-state was detected. This correlation can interpret the occurrence of the long-term behaviour of the flare star at its quiescent-state as found by Mavridiset al. (1982).  相似文献   

A kinematical approach to dark energy studies     

David Rapetti  Steven W. Allen  Mustafa A. Amin  Roger D. Blandford 《Monthly notices of the Royal Astronomical Society》2007,375(4):1510-1520

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Erratum     

Khalid J. Fahmi 《Natural Hazards》1984,2(2):199

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Structure of magnetogasdynamic weak shock waves     

M. A. Khidr  S. S. Elghabaty  M. A. A. Mahmoud 《Astrophysics and Space Science》1987,136(2):379-391

The problem of the detailed structure of magnetogasdynamic shock waves is investigated. It is assumed that the flow takes place under normal magnetic fieldH ₀ and the conductivity of the medium is considered infinite. An approximate analytical solution of the nonlinear differential equations describing the phenomena is obtained. The suggested analytical results in this paper are in good agreement with the previous numerical computations for the thickness and the velocity distribution inside the transition region. In addition, the enthalpy distribution inside the shock front is predicted.  相似文献   

Energy–Momentum In The Viscous Kasner-Type Universe In Teleparallel Gravity     

Mustafa?SaltiEmail author 《Astrophysics and Space Science》2005,299(2):159-166

Using the teleparallel gravity versions of the Einstein and Landau–Lifshitz’s energy and/or momentum complexes, I obtain the energy and momentum of the universe in viscous Kasner-type cosmological models. The energy and momentum components (due to matter plus field) are found to be zero and this agree with a previous work of Rosen and Johri et al., who investigated the problem of the energy in Friedmann–Robertson–Walker (FRW) universe. The result that the total energy and momentum components of the universe in these models is zero same as Bergmann–Thomson’s energy–momentum and props the viewpoint of Tryon. Rosen found that the energy of the FRW space–time is zero, which agrees with the studies of Tryon. PACs Numbers: 04.20.-q; 04.50.+h An erratum to this article is available at .  相似文献   

Energy Of The Universe In Bianchi-Type I Models In MØLler’S Tetrad Theory Of Gravity     

Oktay?Aydo?duEmail author  Mustafa?Salti 《Astrophysics and Space Science》2005,299(3):227-232

In this paper, using the energy definition in MØller’s tetrad theory of gravity we calculate the total energy of the universe in Bianchi-type I cosmological models which includes both the matter and gravitational fields. The total energy is found to be zero and this result agrees with a previous works of Banerjee and Sen who investigated this problem using the general relativity version of the Einstein energy-momentum complex and Xulu who investigated same problem using the general relativity versions of the Landau and lifshitz, Papapetrou and Weinberg’s energy-momentum complexes. The result that total energy of the universe in Bianchi-type I universes is zero supports the viewpoint of Tryon.  相似文献