Numerical Studies of Fluid Flow in Microgravity Conditions for Confined Crystal Growth     

Xavier Ruiz  Laureano Ramírez-Piscina  Jaume Casademunt 《Astrophysics and Space Science》2001,276(1):135-140

We study the convective flow induced by residual accelerations in microgravity conditions for different geometric arrangements which are relevant to crystal growth experiments. We consider both constantand oscillating acceleration and focus mostly on the transient relaxation dynamics. Results are relevant to estimate impact of more realistic residual accelerations in crystal growth experiments.  相似文献   

Near infrared spectroscopy of SL-9 impacts     

M. Ruiz  G. H. Rieke  M. J. Rieke  D. Means  P. Frawley 《Earth, Moon, and Planets》1994,66(1):91-97

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Topo-Iberia project: CGPS crustal velocity field in the Iberian Peninsula and Morocco     

J. Garate  J. Martin-Davila  G. Khazaradze  A. Echeverria  E. Asensio  A. J. Gil  M. C. de Lacy  J. A. Armenteros  A. M. Ruiz  J. Gallastegui  F. Alvarez-Lobato  C. Ayala  G. Rodríguez-Caderot  J. Galindo-Zaldívar  A. Rimi  M. Harnafi 《GPS Solutions》2015,19(2):287-295

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Dynamics of an isolated,viscoelastic, self-gravitating body     

C. Ragazzo  L. S. Ruiz 《Celestial Mechanics and Dynamical Astronomy》2015,122(4):303-332

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Onset of Convection,Heat Flow and Thickness of the Europa‘s ice Shell     

Ruiz  Javier 《Earth, Moon, and Planets》1997,77(2):99-104

The observational evidence given by Galileo spacecraft about Europa supports an icy rigid layer of several kilometers over another ductile layer of ice in convection, which floats over an internal ocean of liquid water. Before the onset of convection, heat is transmitted into the crust by conduction. The heat flow analysis in the potentially convective layer gives values higher than those obtained previously by tidal dissipation models, and suggests that the ice may be limited to a thin layer of ∼4 km total thickness. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

Bioremediation and toxicity determination of natural seawater polluted with weathered crude oil by salt-tolerant consortia in a SBR   总被引：1，自引：0，他引：1  

Ruiz M  Pasadakis N  Kalogerakis N 《Marine pollution bulletin》2006,52(11):1490-1493

The aim of this research was to compare the bioremediation treatment of seawater polluted with two different concentrations of weathered crude oil (0.2 for experiment (a) and 1.14% for experiment (b), v/v) by salt-tolerant consortia enriched from the sludge of a refinery wastewater treatment facility, in a SBR. The use of a commercial bioremediation stimulant (S200) was also evaluated as an alternative to the traditional nitrogen and phosphorus supplement.  相似文献   

Olive flowering phenology variation between different cultivars in Spain and Italy: modeling analysis     

H. Garcia-Mozo  F. Orlandi  C. Galan  M. Fornaciari  B. Romano  L. Ruiz  C. Diaz de la Guardia  M. M. Trigo  I. Chuine 《Theoretical and Applied Climatology》2009,95(3-4):385-395

Phenology data are sensitive data to identify how plants are adapted to local climate and how they respond to climatic changes. Modeling flowering phenology allows us to identify the meteorological variables determining the reproductive cycle. Phenology of temperate of woody plants is assumed to be locally adapted to climate. Nevertheless, recent research shows that local adaptation may not be an important constraint in predicting phenological responses. We analyzed variations in flowering dates of Olea europaea L. at different sites of Spain and Italy, testing for a genetic differentiation of flowering phenology among olive varieties to estimate whether local modeling is necessary for olive or not. We build models for the onset and peak dates flowering in different sites of Andalusia and Puglia. Process-based phenological models using temperature as input variable and photoperiod as the threshold date to start temperature accumulation were developed to predict both dates. Our results confirm and update previous results that indicated an advance in olive onset dates. The results indicate that both internal and external validity were higher in the models that used the photoperiod as an indicator to start to cumulate temperature. The use of the unified model for modeling the start and peak dates in the different localities provides standardized results for the comparative study. The use of regional models grouping localities by varieties and climate similarities indicate that local adaptation would not be an important factor in predicting olive phenological responses face to the global temperature increase.  相似文献   

A procedure for modelling asymptotic g‐mode pulsators: The case of γ Doradus stars     

A. Moya  J.C. Surez  S. Martín‐Ruiz  P.J. Amado  C. Rodríguez‐Lpez  A. Grigahcne  M.A. Dupret  E. Rodríguez  R. Garrido 《Astronomische Nachrichten》2008,329(5):541-544

Mode identification is one of the first and main problems we encounter in trying to develop the complete potential of asteroseismology. In the particular case of g‐mode pulsators, this is still an unsolved problem, from both the observational and theoretical points of view. Nevertheless, in recent years, some observational and theoretical efforts have been made to find a solution. In this work we use the latest theoretical and computational tools to understand asymptotic g‐mode pulsators: 1) the Frequency Ratio Method, and 2) Time Dependent Convection. With these tools, a self‐consistent procedure for mode identification and modelling of these g‐mode pulsators can be constructed. This procedure is illustrated using observational information available for the γ Doradus star 9Aurigae. (© 2008 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

The limits of validity of the Frequency Ratio Method: The particular case of γ Doradus stars     

J.C. Surez  S. Martín‐Ruiz  A. Moya  P.J. Amado  C. Rodríguez‐Lpez  E. Rodríguez  R. Garrido 《Astronomische Nachrichten》2008,329(5):545-548

This work provides a general vision of the limits of validity of the Frequency Ratio Method applied to the g‐mode pulsators in asymptotic regime, the γ Doradus stars. In particular, the work is mainly focused on the role of rotation which is found one of the most important source of uncertainty of the method. The particular case of the moderately rotating γ Doradus star HD48501 is discussed. (© 2008 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

Subsidence and thermal history of an inverted Late Jurassic‐Early Cretaceous extensional basin (Cameros,North‐central Spain) affected by very low‐ to low‐grade metamorphism          下载免费PDF全文

Silvia Omodeo‐Salé  Ramon Salas  Joan Guimerà  Robert Ondrak  Ramon Mas  José Arribas  Isabel Suárez‐Ruiz  Luis Martinez 《Basin Research》2017,29(Z1):156-174

The Cameros Basin (North Spain) is a Late Jurassic‐Early Cretaceous extensional basin, which was inverted during the Cenozoic. It underwent a remarkable thermal evolution, as indicated by the record of anomalous high temperatures in its deposits. In this study, the subsidence and thermal history of the basin is reconstructed, using subsidence analysis and 2D thermal modelling. Tectonic subsidence curves provide evidence of the occurrence of two rapid subsidence phases during the syn‐extensional stage. In the first phase (Tithonian‐Early Berriasian), the largest accommodation space was formed in the central sector of the basin, whereas in the second (Early Barremian‐Early Albian), it was formed in the northern sector. These rapid subsidence phases could correspond to relevant tectonic events affecting the Iberian Plate at that time. By distinguishing between the initial and thermal subsidence and defining their relative magnitudes, Royden's (1986) method was used to estimate the heat flow at the end of the extensional stage. A maximum heat flow of 60–65 mW/m² is estimated, implying only a minor thermal disturbance associated with extension. In contrast with these data, very high vitrinite reflectance, anomalously distributed in some case with respect to the typical depth‐vitrinite reflectance relation, was measured in the central‐northern sector of the basin. Burial and thermal data are used to construct a 2D thermal basin model, to elucidate the role of the processes involved in sediment heating. Calibration of the thermal model with the vitrinite reflectance (%Ro) and fluid inclusion (FI) data indicates that in the central and northern sectors of the basin, an extra heat source, other than a typical rift, is required to explain the observed thermal anomalies. The distribution of the %Ro and FI values in these sectors suggests that the high temperatures and their distribution are related to the circulation of hot fluids. Hot fluids were attributed to the hydrothermal metamorphic events affecting the area during the early post‐extensional and inversion stages of the basin.  相似文献