Tools to detect structures in dynamical systems using Jet Transport     

Daniel Pérez-Palau  Josep J. Masdemont  Gerard Gómez 《Celestial Mechanics and Dynamical Astronomy》2015,123(3):239-262

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The role of massive AGB stars in the early solar system composition     

Josep M. TRIGO‐RODRÍGUEZ  Domingo Aníbal GARCÍA‐HERNÁNDEZ  Maria LUGARO  Amanda I. KARAKAS  M. van RAAI  Pedro García LARIO  Arturo MANCHADO 《Meteoritics & planetary science》2009,44(5):627-639

Abstract— We demonstrate that a massive asymptotic giant branch (AGB) star is a good candidate as the main source of short‐lived radionuclides in the early solar system. Recent identification of massive (4–8 M⊙) AGB stars in the galaxy, which are both lithium‐ and rubidium‐rich, demonstrates that these stars experience proton captures at the base of the convective envelope (hot bottom burning), together with high‐neutron density nucleosynthesis with ²²Ne as a neutron source in the He shell and efficient dredge‐up of the processed material. A model of a 6.5 M⊙ star of solar metallicity can simultaneously match the abundances of ²⁶Al, ⁴¹Ca, ⁶⁰Fe, and ¹⁰⁷Pd inferred to have been present in the solar nebula by using a dilution factor of 1 part of AGB material per 300 parts of original solar nebula material, and taking into account a time interval between injection of the short‐lived nuclides and consolidation of the first meteorites equal to 0.53 Myr. Such a polluting source does not overproduce ⁵³Mn, as supernova models do, and only marginally affects isotopic ratios of stable elements. It is usually argued that it is unlikely that the short‐lived radionuclides in the early solar system came from an AGB star because these stars are rarely found in star forming regions, however, we think that further interdisciplinary studies are needed to address the fundamental problem of the birth of our solar system.  相似文献   

Influence of pore morphology on the durability of sedimentary building stones from Aragon (Spain) subjected to standard salt decay tests     

Oscar Buj  Josep Gisbert 《Environmental Earth Sciences》2010,61(7):1327-1336

The aim of the present article is to identify the influence of the pore morphology on the physical behaviour and durability of natural stone. Fifteen sedimentary rocks commonly used in the cultural and architectural heritage of Aragon (Spain) were characterized. The petrography, porous structure, fluid transport properties and durability of these rocks were analysed. They were classified into two different groups according to the results of the different tests. For each of these groups the physical behaviour was established. A principal components analysis was used in order to examine the correlation between pore structure, hydric properties and durability. The results show that the percentage of pore throats <0.1 μm control the fluid transport properties, have an important influence on stone durability, and can be used to predict resistance to salt decay while the average pore size does not. Stones with a high percentage of pore throats <0.1 μm are less susceptible to salt decay than stones with higher pore size if their pore network is characterized by high tortuosity and low connectivity.  相似文献   

The Canary Eddy Corridor: A major pathway for long-lived eddies in the subtropical North Atlantic     

Pablo Sangrà  Ananda Pascual  Ángel Rodríguez-Santana  Francisco Machín  Evan Mason  James C. McWilliams  Josep L. Pelegrí  Changming Dong  Anna Rubio  Javier Arístegui  Ángeles Marrero-Díaz  Alonso Hernández-Guerra  Antonio Martínez-Marrero  Maricel Auladell 《Deep Sea Research Part I: Oceanographic Research Papers》2009,56(12):2100-2114

We report, from remote sensing and in situ observations, a new type of permanent structure in the eastern subtropical Atlantic Ocean, that we call the “Canary Eddy Corridor”. The phenomenon, is a zonal long-lived (>3 months) mesoscale eddy corridor, whose source is the flow perturbation of the Canary Current and the Trade Winds at the Canary Islands. The latitudinal range of the corridor spans 22°N–29°N and extends from the Canaries to at least 32ºW, near the mid-Atlantic. This is the main region of long-lived westward-propagating eddies in the subtropical northeast Atlantic. From a age-distribution study we observe that at least 10% of mesoscale eddies in this region are long-lived, with a dominance of anticyclones over cyclones. Another four westward-propagating eddy corridors were also detected: two small corridors north and south of the Azores Front; a small zonal corridor located near 31ºN, south of the island of Madeira; and a small corridor located near the Cape Blanc giant filament. The existence of these corridors may change, at least for the northeastern subtropical Atlantic, the general idea that mesoscale eddies are disorganized, ubiquitous structures in the ocean. The Canary Eddy Corridor constitutes a direct zonal pathway that conveys water mass- and biogeochemical properties offshore from the Canary Island/Northwest Africa upwelling system, and may be seen as a recurrent offshore pump of organic matter and carbon to the oligotrophic ocean interior. Estimates of volume and mass transport indicate that Canary Eddy Corridor westward transport is more than one-fourth of the southward transport of the Canary Current. The westward transport of kinetic energy by the eddies of the Canary Corridor is as important as the southward transport by the Canary Current. The total primary production related to the Corridor may be as high as the total primary production of the northwest Africa upwelling system for the same latitude range.  相似文献   

On the frequency contents of local events: source or path effect?     

Antoni M. Correig  Josep Vila 《Geophysical Journal International》1993,115(3):863-877

Local events which occurred in the Timanfaya volcanic field are analysed and their spectral contents are interpreted as being due to the effect of a finely layered medium with large impedance contrast, the presence of which is well known from well-logging data. By considering the layered medium as a filter, its spectral response (amplitude and phase) is computed from different randomly generated values of its parameters (total thickness, mean thickness of the individual layers and impedance contrast), showing that this stratigraphic filter acts as a low-pass filter. This effect can be correctly modelled by means of an exponential correlation function. However, in some cases resonant peaks appear in the spectrum superimposed on the low-pass filter effect, which can only be attributed to resonant scattering. An analysis of the phase and group delay associated with the amplitudes is made and strongly suggests that it is necessary to incorporate the theory of resonant scattering for the retrieval of medium properties. From the point of view of the amplitudes, the superposition of both effects, low-pass filter and resonant peaks, allows us to reproduce the gross features that are usually attributed to source effects. The need for a careful analysis of the local site response previous to any interpretation of the spectral features in terms of source characteristics is thus emphasized.  相似文献   

Systematics in uranium-ionium dating of sediments     

Michel Bernat  Claude J. Allegre 《Earth and Planetary Science Letters》1974,21(3):310-314

The mineral separates of a core have been systematically dated by the Io/Th chronology method. The results show that authigenic minerals, though not always completely authigenic, are suitable for dating.We give some evidence against the hypothesis of Io/²³²Th isotopic equilibrium in marine conditions and suggest that the minerals are mixtures of two components.  相似文献   

Variations of element distribution in ferromanganese nodules and its bearing on growth rates     

M. Bernat  C. Causse  E. A. Perseil  G. Féraud 《Mineralium Deposita》1989,24(4):258-269

Mineralogical, chemical, and radiochemical analyses of nodules sampled at various distances from the East Pacific Rise indicate that the mineralogical composition is not clearly linked to distance, but chemical composition seems to be. The pelagic nodules accrete at a lower rate and are, on the whole, richer in manganese, uranium, and thorium and poorer in lead and silicon than nodules from the ridge. The deep-seated nodules display a marked decrease in thorium concentration toward their centers, which can be explained in several ways. One hypothesis involves a decrease in the growth rate as the plate moves away from the ridge and manganese flux diminishes. As suggested in previous studies, some dissolution of the bottom of the nodules may occur and contribute to abnormal element distributions.  相似文献   

A high-temperature hydrothermal deposit on the East Pacific Rise near 7°N     

J. Boulegue  E.A. Perseil  M. Bernat  B. Dupr  P. Stouff  J. Francheteau 《Earth and Planetary Science Letters》1984,70(2):249-259

A SEABEAM survey of the East Pacific Rise (EPR) led to the selection of several sites having structural characteristics favorable for hydrothermal activity. Dredging of such an area located at 7°N on the EPR resulted in the recovery of sulfides, oxides and fresh basalt. Chemical analyses and isotopic compositions showed that the recovered pyrites were probably precipitated directly from hot vent hydrothermal waters. Chemical analyses and isotopic composition of manganese-iron oxides indicated that they too were of hydrothermal origin. ²¹⁰Pb/Pb measurements yielded ages of 90 ± 10years for the deposits. This site may still be undergoing hydrothermal activity.  相似文献   

Study of the transfer between libration point orbits and lunar orbits in Earth–Moon system     

Yu Cheng  Gerard Gómez  Josep J. Masdemont  Jianping Yuan 《Celestial Mechanics and Dynamical Astronomy》2017,128(4):409-433

This paper is devoted to the study of the transfer problem from a libration point orbit of the Earth–Moon system to an orbit around the Moon. The transfer procedure analysed has two legs: the first one is an orbit of the unstable manifold of the libration orbit and the second one is a transfer orbit between a certain point on the manifold and the final lunar orbit. There are only two manoeuvres involved in the method and they are applied at the beginning and at the end of the second leg. Although the numerical results given in this paper correspond to transfers between halo orbits around the \(L_1\) point (of several amplitudes) and lunar polar orbits with altitudes varying between 100 and 500 km, the procedure we develop can be applied to any kind of lunar orbits, libration orbits around the \(L_1\) or \(L_2\) points of the Earth–Moon system, or to other similar cases with different values of the mass ratio.  相似文献   

Spatial collinear restricted four-body problem with repulsive Manev potential     

Esther Barrabés  Josep M. Cors  Claudio Vidal 《Celestial Mechanics and Dynamical Astronomy》2017,129(1-2):153-176

We outline some aspects of the dynamics of an infinitesimal mass under the Newtonian attraction of three point masses in a symmetric collinear relative equilibria configuration when a repulsive Manev potential (\(-1/r +e/r^{2}\)), \(e>0\), is applied to the central mass. We investigate the relative equilibria of the infinitesimal mass and their linear stability as a function of the mass parameter \(\beta \), the ratio of mass of the central body to the mass of one of two remaining bodies, and e. We also prove the nonexistence of binary collisions between the central body and the infinitesimal mass.  相似文献