Turbulent generation of magnetic fields in astrophysical jets

We consider evolution of the regular magnetic field in turbulent astrophysical jets. The observed lateral expansion of a jet is approximately described by a linear in coordinates regular velocity field (the Hubble flow). It is shown that in expanding turbulent jets with non-vanishing mean helicity of the turbulence temporal amplification and effective realignment of the regular magnetic field occurs with the field changing orientation from the transverse to the longitudinal one along the jet axis. The distance at which the realiggment occurs depends on parameters of the jet, in particular, on the power of the central source. Estimates for the jet in a weak source 3C 31 favourably agree with observations.     

Photoelectric photometry of the eclipsing binary V1425 Cygni

Photoelectric differentialB andV magnitudes of the eclipsing binary V1425 Cygni are presented yielding the complete photoelectric light curve of this relatively bright system. The improved light elements are calculated using the least-squares method.     

Long slit spectroscopy of the nuclear zone of NGC 253

We have undertaken a study of the physical conditions of the lonized gas within the starburst region of the galaxy NGC 253, using long slit spectroscopy at high spatial and spectral resolution. Our aim was to identify the appropriate parameters describing the dynamics of the gas and the excitation conditions, in relation with the starburst process. Non-gaussian line profiles and line spliting are clearly observed, indicating a complicated dynamical structure; furthermore, the zones presenting non-circular motions and localized outflow of gas have been spatially sampled at the seeing limit.Paper presented at the 11th European Regional Astronomical Meetings of the IAU on New Windows to the Universe, held 3–8 July, 1989, Tenerife, Canary Islands, Spain.     

太阳辐射和地面气象要素的日环食效应

本文通过对1987年9月23日日环食期间太阳辐射和地面气象要素等实测资料的分析,指出了在日环食过程中太阳辐射和地面气象要素等的变化,也叙述了日食期间地面臭氧含量的变化;第一次在国内测得了由日食引起的大气重力波,进而讨论了大气重力波的若干特性.     

A conceptual hydrogeological model of ophiolite hard-rock aquifers in Oman based on a multiscale and a multidisciplinary approach

Ophiolites are found all over the world: from the Alps to the Himalayas, in Cuba, Papua-New Guinea, New Caledonia, Newfoundland, etc. They are composed of hard rocks—basalt, dolerite, gabbro and peridotite, which are formed at the mid-oceanic ridges, with specific ridge-related tectonic fracturing and intense hydrothermal alteration. Their geological and thus their hydrogeological properties differ from those of both granite or classical gabbro and classical basaltic lava. A conceptual hydrogeological model of these hard-rock aquifers was developed based on the convergent results of a multidisciplinary approach at several spatial scales, from rock-sample (centimetre) to catchment (kilometre), on well-preserved ophiolite rocks in Oman. In ophiolite rocks, groundwater circulation takes place mostly in the fissured near-surface horizon (50 m thick), and, to a lesser degree, in the tectonic fractures. Hydrograph analysis (Water Resour Res 34:233–240, 1977), interpretation of numerous pumping tests using both classical Theis and dual porosity models [Water Resour Res 32:2733–2745, 1996; Comput Geosci J (in press)], and mercury porosity and hydraulic conductivity lab-measurements support the aquifer parameter estimates. The hydraulic conductivity K of the fissured horizon is estimated at 10^–5 to 10^–6 m/s for gabbro and dolerite, and 10^–7 m/s for peridotite. The storage coefficient S of the peridotite aquifer is estimated at 10^–3 and appears to be controlled mainly by microcracks (20 to 100 m wide). Tectonic fractures in the ophiolite have similar hydrodynamic properties regardless of lithology (10^–1<T<10^–4 m²/s and 10^–1<S<10^–3) though the probability of obtaining productive wells is two to three times greater in gabbro and dolerite than in peridotite. Some of the tectonic fractures produce small hydrothermal, hyperalkaline springs in the peridotite. The water budget and hydrochemistry of the Oman ophiolite are characterized and support the conceptual hydrogeological model. Despite low annual rainfall, a relatively low hydraulic conductivity and a significant storage coefficient explain why most of the streams in peridotite are perennial.

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Résumé Les ophiolites se trouvent partout dans le monde : des Alpes à lHymalaya, à Cuba, Papouasie Nouvelle-Guinée, Nouvelle Calédonie, etc. Les ophiolites sont composées de roches dures basaltiques, de dolérites, gabbros et péridotites, qui sont formées aux rides mi-océaniques, avec, en relation avec les rides, une fracturation tectonique et une altération hydrothermale intense. Leurs propriétés géologiques et hydrogéologiques diffèrent de celles des granites ou des gabbros classiques ou des laves basaltiques classiques. Un modèle hydrogéologique conceptuel des aquifères de hard-rock a été développé sur les résultats convergents dune approche multidisciplinaire à différentes échelles spatiales, de léchantillon de roche de quelques centimètres à la taille du bassin versant en kilomètres, des ophiolites bien conservées dOman. Dans les roches ophiolitiques, la circulation des eaux souterraines est surtout localisée dans les fissures dun horizon de surface de plus dune cinquantaine de mètres et à un degré moindre dans les fractures tectoniques. Lanalyse des hydrographes (Water Resour Res 34:233–240, 1977), linterprétation des nombreux essais de pompage utilisant des modèles classiques de Theis et des modèles à double porosité (Water Resour Res 32:2733–2745, 1996; Comput Geosci J (Soumis), la porosité au mercure et la conductivité hydraulique calculée en laboratoire supportent lestimation des paramètres de laquifère. La conductivité hydraulique K de lhorizon fissuré est estimée entre 10^–5 et 10^–6 m/s pour les gabbros et les dolérites, et 10^–7 m/s pour les péridotites. Le coefficient demmagasinement S de laquifère de péridotite est estimé à 10^–3 et semble être contrôlé par les micro-fractures (20 à 100 m de largeur). Les fractures tectoniques dans les ophiolites possèdent des propriétés hydrodynamiques en regard de la lithologie (10-1<T<10-4 m²/s et 10-1/S/10-3) bien que la probabilité dobtenir des puits productifs est trois plus grand dans le grabbro et la dolérite que la péridétite. Quelques unes des fractures tectoniques produisent de petites sources hydrothermales hyperalcalines dans la péridotite. Le bilan hydrologique et hydrochimique de lophiolite dOman caractérise le modèle hydrogéologique conceptuel. Malgré des faibles précipitations annuelles, une relativement basse conductivité hydraulique et un coefficient demmagasinement significatif expliquent pourquoi la plus part des cours deau sur les péridotites ne sont jamais taris.

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Resumen Las rocas ofiolitas se encuentran en muchas partes del mundo desde los Alpes a los Himilaya, Newfoundland, Nueva Caledonia etc. Son rocas duras compuestas de basalto, dolerita, gabro y peridotita que son formadas por los cordones medio-oceánicos y por fracturación relacionada con los cordones tectónicos específicos y alteración hidrotermal intensa. La geología y los propiedades hidrogeológicas varian entre las de granito y gabro clásico y lava de basalto clásico. Se desarrolló un modelo conceptual de los acuíferos de las rocas duras Basado en los resultados convergentes de un enfoce multidisciplinario a varias escalas a partir de muestras de roca (centímetro) a cuenca kilómetro) enfocado en las rocas ofilíticas bien preservados en Oman. En las rocas ofiolíticas la circulación de agua ocurre principalmente en el horizonte de fisuras cercanas a la superficie (>50 m de espesor) y en un grado menos importante en fracturas tectónicas. Los estimados de los parámetros de estos acuíferos se basan en análisis de hidrógrafos (Water Resour Res 34:233–240, 1977), en la interpretación de pruebas de bombeo usando los modelos clásicos de Theis y de porosidad doble (Hamm y Bidaux 1996; Lods y Gouze, [en prensa]), y porosidad de mecurio y conductividad hidraúlica medida en el laboratorio. La conductividad hidraúlica K del horizonte fisurado se estima en 10E-5 a 10E-6 m-s para gabro y dolerita y 10E-7 para peridotita. El coeficiente de abastecimiento S del acuífero peridotita se estima en 10–3 y parece ser controlado principalmente por microfracturas (20 to 100 m de ancho). Las fracturas tectónicas en la ofiolita tienen propiedades hidrodinámicas similares independientes de la litología (10–1<T<10–4 m²/s and 10–1<S<10–3) pero la probabilidad de obtener pozos productivos es dos o tres veces mayor en gabro que en dolerita o peridotita. Algunas de las fracturas tectónicas producen pequeñas descargas de agua hidrotermal hiperalcalina en la peridotita. El presupuesto e hidroquímica de las ofilitas de Omán se caracteriza y apoya en el modelo conceptual hidrogeológico. La baja lluvia anual, una conductividad hidraúlica relativamente baja y un coeficiente de abastecimiento importante explican porqué la mejoría de los drenajes en peridotita es peremne.

     

Nature and timing of magma interactions before,during, and after the caldera-forming eruption of Volcán Ceboruco,Mexico

Volcán Ceboruco, Mexico, erupted ~1,000 years ago, producing the Jala pumice and forming a ~4-km-wide caldera. During that eruption, 2.8 to 3.5 km³ of rhyodacite (~70 wt% SiO₂) magma and 0.2 to 0.5 km³ of mixed dacite (~67 wt% SiO₂) magma were tapped and deposited as the Jala pumice. Subsequently, the caldera was partially filled by extrusion of the Dos Equis dome, a low-silica (~64 wt% SiO₂) dacite dome with a volume of ~1.3 km³. Petrographic evidence indicates that the Jala dacite and Dos Equis dacite originated largely through the mixing of three end-member magmas: (1) rhyodacite magma, (2) dacite magma, and (3) mafic magma. Linear least-squares modeling and detailed modal analysis indicate that the Jala dacite is predominantly a bimodal mixture of rhyodacite and dacite with a small additional mafic component, whereas the Dos Equis dacite is composed of mostly dacite mixed with subordinate amounts of rhyodacite and mafic magma. According to Fe–Ti oxide geothermometry, before the caldera-forming eruption the rhyodacite last equilibrated at ~865 °C, whereas the dacite was originally at ~890 °C but was heated to ~960 °C by intrusion of mafic magma as hot as ~1,030 °C. Zoning profiles in plagioclase and/or magnetite phenocrysts indicate that mixing between mafic and dacite magma occurred ~34–47 days prior to eruption, whereas subsequent mixing between rhyodacite and dacite magmas occurred only 1–4 days prior to eruption. Following the caldera-forming eruption, continued inputs of mafic magma led to effusion of the Dos Equis dome dacite. In this case, timing between mixing and eruption is estimated at ~93–185 days based on the thickness of plagioclase overgrowth rims.Editorial responsibility: T.L. Grove     

Rôle des héritages latéritiques et du niveau des nappes dans l'évolution des modelés et des sols en zone intertropicale forestière humide

Analysis of landscapes and soil covers from the outer to the inner part of a $75\text{km}\times 60\text{km}$ watershed in the South-Cameroon rainforest zone, characterized by important remnants of inherited ferricretes and stable hydrostatic base levels, indicates that the development of present landforms has not involved significant erosion by slope retreat because of the relative preservation of downslope residual ferricrete and that soil covers have vertically decayed under in situ geochemical process. To cite this article: D. Bitom et al., C. R. Geoscience 336 (2004).