四川盆地震旦系灯影组葡萄状白云岩成因

四川盆地震旦系灯影组发育巨厚的白云岩,其中灯影组二段和四段发育大量具有各种形态的葡萄状白云岩,其直径最长可达75cm,有的平行于层面,有的穿层。剖面资料表明,葡萄状白云岩发育多期等厚环边胶结物,中部残留大量未充填的不规则洞穴,这成为与岩溶喀斯特作用相关的地下溶蚀作用的证据。围岩泥晶白云石为早期海水中原生结晶的产物,后来的胶结物可划分为4期: (1)自泥晶化白云石(部分样品中可见)作为最早的一期胶结物,由于各种生物化学作用和生物作用的影响而紧贴着围岩发育;(2)第2期胶结物纤维状白云石可能为海水中直接沉淀的产物,经历后期成岩作用后,具有完全有序的结构,晶胞参数接近理想值;(3)细—中晶白云石为第3期胶结物,包含纤维状白云石溶蚀残余,形成于构造抬升之后的近地表大气淡水环境;(4)第4期胶结物中—粗晶白云石为埋藏环境下直接结晶的产物,充填了孔洞中心,残留部分未充填孔洞。灯影组受到了岩溶喀斯特作用、胶结作用以及白云石化作用等成岩作用的影响,其中与葡萄状白云岩有关的岩溶喀斯特作用对于灯影组储集层的发育至关重要。对灯影组葡萄状白云岩的研究,不仅有助于深入探讨灯影组储集层成因和演化及灯影组白云岩的成因,而且有助于指导四川盆地前寒武系油气勘探。     

A three-layered spectral model with application to wind-induced motion in the presence of stratification and a bottom slope

The main features of a new three-dimensional spectral model for the motion of a stratified sea are described. The model is applied to determine wind-induced elevations and currents over an idealised shelf-edge slope during the summer season of thermal stratification. A wind stress field spanning the slope is applied in the form of a rectangular pulse through time, the direction of the stress being parallel to the shelf edge. It is shown that strong vertical motion occurs near the top of the slope in the wind region; inertial currents are excited. Outside the wind region, long-period waves trapped over the slope and propagating along it may be identified.     

A shallow seismic refraction study of the Versailles cryptoexplosion structure,central Kentucky

Abstract— The Versailles cryptoexplosion structure, located in central Kentucky, contains a partially brecciated central uplift and a boundary marked by arcuate faulting. Seismic refraction data were used to divide the structure into distinct units on the basis of velocity. A zone of brecciated material shows a decrease in velocity compared with surrounding rocks. Locally thickened strata are present on the flanks of the central uplift. An increase of the bedrock velocity in the area surrounding the structure suggests localized dolomization of fractured bedrock, and a plug of fractured strata near the base of the brecciation appears to be uplifted. Based on the geometry of deformation seen in known impact structures, and the integration of this study with previous geological and geophysical work in the area, it is suggested that our results support the interpretation of the Versailles structure as an eroded astrobleme (Black, 1964b; Seeger, 1972).     

Annual variation of sporadic radar meteor rates

The activity of sporadic meteors has been measured from 2002 to 2005 with the Canadian Meteor Orbit Radar. Single-station data at 29.85 MHz have been used to find the positions of the five sporadic sources visible from the Northern hemisphere, and the activity measured for each source has been corrected for observing biases. Relative fluxes and the annual variation of each source are well determined. The variations in activity are of great interest in determining the history and origin of the sporadic meteoroid population.     

Spectral analysis of water vapour in cool stars

M-star spectra, at wavelengths beyond 1.35 μm, are dominated by water vapour, yet terrestrial water vapour makes it notoriously difficult to obtain accurate measurement from ground-based observations. We have used the short-wavelength spectrometer on the Infrared Space Observatory at four wavelength settings to cover the  2.5–3.0 μm  region for a range of M stars. The observations show a good match with previous ground-based observations and with synthetic spectra based on the Partridge & Schwenke line list, although not with the SCAN line list. We have used a least-squared minimization technique to systematically find best-fitting parameters for the sample of stars. The temperatures that we find indicate a relatively hot temperature scale for M dwarfs. We consider that this could be a consequence of problems with the Partridge & Schwenke line list which leads to synthetic spectra predicting water bands that are too strong for a given temperature. Such problems need to be solved in the next generation of water vapour line lists, which will extend the calculation of water vapour to higher energy levels with the good convergence necessary for reliable modelling of hot water vapour. Then water bands can assume their natural role as the primary tool for the spectroscopic analysis of M stars.     

Decision-support Systems: Do they have a Future in Estuarine Management?

Estuaries are highly complex ecosystems. Consequently they present daunting challenges to planners and regulators responsible for devising ‘ sustainable development ’ strategies or for taking rapid decisions with respect to ‘ crisis management ’. Over the lifetime of the Estuarine and Coastal Sciences Association, there have been significant developments in both the range and sophistication of the tools available to assist with these tasks. Indeed, managers are now faced with a confusing plethora of possibilities that may, or may not, help in achieving the optimum solution to a given problem.Typical problems confronting managers and the systems available to resolve the issues are considered. By way of illustration, we present some examples based on our experience over the last 25 years in the Mersey Estuary (which has seen dramatic improvements in water quality and a number of major proposed developments), from the Ribble Estuary and from along the north-west coast of the U.K.