No major thermal event on the mid-Cretaceous Côte d'Ivoire–Ghana Transform Margin     

T. Wagner  & T. Pletsch 《地学学报》2001,13(3):165-171

Transient mid-Cretaceous thermal uplift induced by lateral heating from passing oceanic lithosphere is often invoked as a mechanism for the formation of the Côte d'Ivoire–Ghana basement ridge in the Equatorial Atlantic. This heating event should have affected mid-Cretaceous sedimentary rocks along the ridge. However, organic maturity and clay mineral data on the thermal evolution of these rocks suggest that burial temperatures did not exceed 80 °C and that palaeo–geothermal gradients are not anomalous. Optical petrography and the stratigraphic pattern of temperature-sensitive parameters indicate that higher palaeotemperature estimates are related to admixtures of preheated, detrital organic and inorganic matter. Erosion brought the sediments to their present shallow burial depths. Lack of evidence for significant thermal alteration implies that either thermal exchange between oceanic and continental lithosphere along the Côte d'Ivoire–Ghana Transform Margin was negligible, or that lateral heating by oceanic lithosphere was not strong enough to affect the sedimentary cover of the basement ridge.  相似文献   

Spectral variations of DY Cen     

Sunetra Giridhar  N. Kameswara Rao  David L. Lambert 《Journal of Astrophysics and Astronomy》1996,17(1-2):23-40

Two high resolution spectra of the hot RCrB star DY Cen in the red region are compared. The photospheric absorption lines show a radial velocity variation of 12 kms-1 between 1989 July and 1992 May. Emission components to some CII lines present in 1989 are almost entirely absent in 1992. Nebular forbidden lines of [OI], [NII] and [SII] appear unchanged from 1989 to 1992  相似文献   

Aquitard Distribution In A Northern Reach Of The Miami Valley Aquifer,Ohio, USA: Part 1. Three-Dimensional Geostatistical Evaluation Of Physical Heterogeneity     

Robert W. Ritzi  David F. Dominic  Kenneth W. Kausch 《Hydrogeology Journal》1996,4(2):12-24

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Tracer budgets in the warm water sphere     

JAMES C. MCWILLIAMS  GOKHAN DANABASOGLU  PETER R. GENT 《地球，A辑:动力气象学与海洋学》1996,48(1):179-192

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Astrometry from space: GAIA and planet detection     

S. Casertano  M. G. Lattanzi  M. A. C. Perryman  A. Spagna 《Astrophysics and Space Science》1996,241(1):89-104

The proposed baseline GAIA mission will be able to detect the astrometric signature of Jupiter-size planets around of the order of a million stars, using either global or narrow-angle astrometry. If the mission can realize the higher astrometric accuracy that photon statistics allows for bright stars, lower-mass planets (from Earth size to ten times larger) can be found around ten to a few hundred stars.  相似文献   

Statistical parameterization of inverse problems     

V. Yu. Terebizh 《Astrophysics and Space Science》1992,193(2):269-288

Image restoration, computerized tomography, and other similar problems are considered as a unified class of stochastic inverse problems. The conventional approach to these problems that proceeds from some integral or functional equations suffers from three main shortcomings: (i) subjectivity, (ii) inability to account for the inner (radiational) noise, and (iii) inability to include the fundamental concept of the natural limit of solution accuracy. A general approach is developed, the Statistical Parameterization of Inverse Problems (SPIPR), that takes into account both the inner and external random noise and gives an explicit form of the above-mentioned natural limit. Applications of the SPIPR to various problems show that the maximum likelihood method as the concrete way to obtain an object estimate has practically limiting efficiency.Two new fields of applications of the SPIPR are outlined along with the image restoration problem: the elimination of blurring due to atmosphere turbulence and reconstruction of an object structure in the computerized tomography. The expressions for the main distribution function in all these problems are found. The corresponding real examples and model cases are considered as well.  相似文献   

Comment on ‘coupling versus uncoupling in soil consolidation’     

Giuseppe Gambolati  R. W. Lewis  B. A. Schrefler  L. Simoni 《国际地质力学数值与分析法杂志》1992,16(11):833-837

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Rayleigh-Taylor instability of a plasma with finite ion Larmor radius effects     

P. Donald Ariel 《Astrophysics and Space Science》1992,196(1):153-166

The stability of an infinitely conducting plasma of variable density has been investigated taking into account the finiteness of the ion Larmor radius. The perturbations propagating along the ambient magnetic field are considered. It is established that, in general,n ² is necessarily real, wheren is the growth rate of disturbance, thus ruling out the possibility of overstability or damped oscillations. The solution is shown to be characterized by a variational principle, which provides the basis for obtaining an approximate solution of the problem. Two density distributions are considered: (i) a continuously stratified plasma layer and (ii) two semi-infinitely extending plasmas of constant densities separated by a horizontal interface. In both cases it has been shown that for the said disturbances the stability criterion remains unaffected by the inclusion of finite Larmor radius effects, though the amplified motion is strongly inhibited due to their inclusion.  相似文献   

Influence of viscous dissipation on a hydromagnetic field     

Th. I. Lekas  G. A. Georgantopoulos 《Astrophysics and Space Science》1992,191(2):299-305

The effect of a transverse magnetic field and of the viscosity diffusion on the free-convection flow of an electrically-conducting incompressible fluid past a uniformally accelerated vertical plate is discussed. A finite difference method has been used to obtain a numerical solution. The influence of the various parameters on the flow field is discussed.  相似文献   

Analytical and numerical analysis of the generalized Shkarofsky function     

N. M. Temme  A. E. Sumner  S. S. Sazhin 《Astrophysics and Space Science》1992,194(2):173-196

The main analytical properties of the generalized Shkarofsky function and a numerical code for its computation are discussed. The results of a numerical analysis are compared with the results of an asymptotic analysis for parameter values relevant to the problem of whistler-mode propagation in the Earth's magnetosphere. This comparison allows us to specify the range of applicability of different approximations to the generalized Shkarofsky function, which have been used for the analysis of relativistic effects on whistler-mode propagation and instability.  相似文献