Turbulence Over Urban-type Roughness: Deductions from Wind-tunnel Measurements     

Ian P. Castro  Hong Cheng  Ryan Reynolds 《Boundary-Layer Meteorology》2006,118(1):109-131

Turbulence data from experiments conducted over a staggered cube array, modelling a neutrally stable atmospheric boundary layer in an urban environment, are presented. The results support the contention that organised eddy structures in the near-wall region differ significantly from those in regular smooth-wall flows or in rough-wall boundary layers with much smaller h/δ ratios (where δ and h are the boundary-layer thickness and the height of the roughness elements, respectively). Attention is concentrated on spatial correlations, spectra (and thus the dominant length and time scales), maps of anisotropy invariants and quadrant analyses of the stress tensor. Results are obtained within both the roughness sublayer (i.e. the region above the roughness but within which the flow is spatially inhomogeneous) and the canopy region (i.e. below the height of the roughness elements) and discussion includes consideration of the turbulence kinetic energy balance at various heights.  相似文献   

The Central Extremadura batholith: Geotectonic implications (European Hercynian Belt)—an outline     

Antonio Castro 《Tectonophysics》1985,120(1-2)

Study of the Central Extremadura batholith and shear zone, described for the first time herein, provides new insights into the tectonomagmatic evolution of the Ibero-Armorican arc.The main plutonic event may be closely related to intracontinental shear-zone development. The Central Extremadura shear zone may provide a model for the interpretation of collision structures related to the origin of the Ibero-Armorican arc.  相似文献   

Emplacement fractures in granite plutons (Central Extremadura batholith,Spain)     

Antonio Castro 《International Journal of Earth Sciences》1984,73(3):869-880

Some plutons of the Central-Extremadura batholith show lateral widening at the final stage of their emplacement. Consequently, various fracture systems have developed, generally filled by aplites that appear both in the plutonic mass and in the metamorphic host rocks.The spatial arrangement of fractures may be interpreted in a simple model in which an important role is played by fluid pressure, as it determines the value of the acting effective stress and, naturally, the different failure mechanisms reflected in different dike systems.

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Zusammenfassung In einigen Granit-Plutonen des Zentralextremadura-Batholithen konnte eine laterale Ausdehnung in den Endetappen ihrer Platznahme festgestellt werden. Dabei wurden verschiedene Bruchsysteme entwickelt, die im allgemeinen mit Aplit gefüllt sind und sowohl im Inneren der plutonischen Masse als auch im metamorphen Nebengestein auftreten.Die spezielle Anordnung der Bruchsysteme konnte anhand eines einfachen Modells interpretiert werden. Dabei spielt der Durchströmungsdruck eine wichtige Rolle, da er den Wert der effektiven Spannung bestimmt und verschiedene Bruchmechanismen, die sich in verschiedenen Gangsystemen widerspiegeln.

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Résumé Quelques plutons du batholite de l'Estremadure centrale ont donné lieu à une expansion latérale au stade final de leur mise en place. Plusieurs systèmes de fractures se sont ainsi développées; elles sont généralement occupées par des aplites et apparaissent aussi bien à l'intérieur de la masse plutonique que dans l'encaissant métamorphique.La distribution spatiale de ces fractures a pu être interprétée par un modèle simple dans lequel la pression des fluides joue un rôle important: cette pression détermine la valeur de la contrainte effective et conditionne les divers mécanismes de facturation, qui se traduisent dans différents systèmes de filons.

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Assessment of regional seasonal rainfall predictability using the CPTEC/COLA atmospheric GCM     

J. A. Marengo  I. F. A. Cavalcanti  P. Satyamurty  I. Trosnikov  C. A. Nobre  J. P. Bonatti  H. Camargo  G. Sampaio  M. B. Sanches  A. O. Manzi  C. A. C. Castro  C. D'Almeida  L. P. Pezzi  L. Candido 《Climate Dynamics》2003,21(5-6):459-475

This is a study of the annual and interannual variability of regional rainfall produced by the Center for Weather Forecasts and Climate Studies/Center for Ocean, Land and Atmospheric Studies (CPTEC/COLA) atmospheric global climate model. An evaluation is made of a 9-member ensemble run of the model forced by observed global sea surface temperature (SST) anomalies for the 10-year period 1982–1991. The Brier skill score and, Relative Operating Characteristics (ROC) are used to assess the predictability of rainfall and to validate rainfall simulations, in several regions world wide. In general, the annual cycle of precipitation is well simulated by the model for several continental and oceanic regions in the tropics and mid latitudes. Interannual variability of rainfall during the peak rainy season is realistically simulated in Northeast Brazil, Amazonia, central Chile, and southern Argentina–Uruguay, Eastern Africa, and tropical Pacific regions, where the model shows good skill. Some regions, such as northwest Peru–Ecuador, and southern Brazil exhibit a realistic simulation of rainfall anomalies associated with extreme El Niño warming conditions, while in years with neutral or La Niña conditions, the agreement between observed and simulated rainfall anomalies is not always present. In the monsoon regions of the world and in southern Africa, even though the model reproduces the annual cycle of rainfall, the skill of the model is low for the simulation of the interannual variability. This is indicative of mechanisms other than the external SST forcing, such as the effect of land–surface moisture and snow feedbacks or the representation of sub-grid scale processes, indicating the important role of factors other than external boundary forcing. The model captures the well-known signatures of rainfall anomalies of El Niño in 1982–83 and 1986–87, indicating its sensitivity to strong external forcing. In normal years, internal climate variability can affect the predictability of climate in some regions, especially in monsoon areas of the world.  相似文献   

Photoionization of cool MHD disk winds     

A.I. Gómez de Castro  C. Ferro-Fontán 《Astrophysics and Space Science》2003,287(1-4):31-34

Recent ultraviolet observations point out that there is hot, dense plasma associated with the optical jet in some T Tauri stars. In this contribution, cool MHD disk wind physics is reviewed by means of a self-similar analytical model to analyze whether hot (Te ? 80,000 K) and dense (n_e ? 10⁹ cm^-3) plasma can be produced in disk winds. It is shown that these high densities can only be achieved at the base of the wind where the stellar X-rays radiation field is strong. The propagation of the X-rays radiation through the disk wind is analyzed: a cocoon of photoionized gas is generated around the star. However, it is difficult to foresee how temperatures as high as ～ 5 × 10⁴ can be reached unless a significant fraction of the X-rays radiation is produced by magnetic reconnection at the boundary between the stellar magnetosphere and the accretion disk.  相似文献   

On the individual calibration of hailpads     

Covadonga Palencia  Claude Berthet  Marta Massot  Amaya Castro  Jean Dessens  Roberto Fraile   《Atmospheric Research》2007,83(2-4):493-504

This paper is a comparative study between the two most common hailpad calibration systems: one annual calibration of a whole consignment of material, and the individual calibration of each plate after a hailfall. Individual calibration attempts to minimize errors due to differences in sensitivity to the impact of hailstones between plates from the same consignment, or due to differences in the inking process before the actual measurement.The comparison was carried out using calibration data from the past few years in the hailpad network in south-western France, and data from an individual calibration process on material provided by the hailpad network in Lleida (Spain). The same type of material was used in the two cases.The results confirm that the error in measuring hailstone sizes is smaller in the case of an individual calibration of hailpads than when one single calibration process was carried out for a whole consignment. The former is approximately 80% of the latter. However, this error could have been higher if it had not been the same person carrying out the single calibration process and the measuring of the dents: it has been found that differences in the inking process may account for up to 20% of the error in the case of small hailstones. Calibration errors affecting other variables, e.g. energy or parameter λ of the exponential size distribution are generally higher (5% and 18%, respectively) than errors due to the spatial variability of the hailstones. However, the calibration method does not influence the maximum size, since the relative error attributed to the spatial variability is about 8 times the calibration error.In conclusion, if errors in determining energy or parameter λ are to be reduced to a minimum, it is highly advisable to be consistent in applying the measuring procedure (if possible with the same person carrying out the measurements all the time), and even to use individual calibration on each plate, always bearing in mind that technicians have to be trained appropriately in order to achieve the highest possible degree of uniformity.  相似文献   

The use of a climate-type classification for assessing climate change effects in Europe from an ensemble of nine regional climate models     

M. de Castro  C. Gallardo  K. Jylha  H. Tuomenvirta 《Climatic change》2007,81(1):329-341

Making use of the Köppen–Trewartha (K–T) climate classification, we have found that a set of nine high-resolution regional climate models (RCM) are fairly capable of reproducing the current climate in Europe. The percentage of grid-point to grid-point coincidences between climate subtypes based on the control simulations and those of the Climate Research Unit (CRU) climatology varied between 73 and 82%. The best agreement with the CRU climatology corresponds to the RCM “ensemble mean”. The K–T classification was then used to elucidate scenarios of climate change for 2071–2100 under the SRES A2 emission scenario. The percentage of land grid-points with unchanged K–T subtypes ranged from 41 to 49%, while those with a shift from the current climate subtypes towards warmer or drier ones ranged from 51 to 59%. As a first approximation, one may assume that in regions with a shift of two or more climate subtypes, ecosystems might be at risk. Excluding northern Scandinavia, such regions were projected to cover about 12% of the European land area.  相似文献   

Diffuse Component Spectra of Solar Active Regions at Submillimeter Wavelengths     

Adriana?V.?R.?SilvaEmail author  Tatiana?F.?Laganá  C.?Guillermo?Gimenez?De?Castro  Pierre?Kaufmann  Joaquim?E.?R.?Costa  Hugo?Levato  Marta?Rovira 《Solar physics》2005,227(2):265-281

Solar maps at 212 and 405 GHz obtained by the Solar Submillimetric Telescope (SST) show regions of enhanced brightness temperature, which coincide with the location of active regions. A statistical study of the radio emission from these active regions was performed for the first time at such high frequencies during 23 days on June and July 2002, when the atmospheric opacity was low. The brightest regions on the maps were chosen for this study, where the brightness excess observed varies from 3 to 20% above quiet Sun levels (i.e., 200–1000 K) at both wavelengths. Sizes of the regions of enhanced emission calculated at half the maximum value were estimated to be between 2′ and 7′. These sizes agree with observed sizes of active regions at other wavelengths such as Hα and ultraviolet. An important result is that the flux density spectra of all sources increase toward submillimeter frequencies, yielding flux density spectral index with an average value of 2.0. The flux density of the active region sources were complemented with that from maps at 17 and 34 GHz from the Nobeyama Radio Heliograph. The resulting spectra at all four frequencies were fit considering the flux density to be due to thermal bremsstrahlung from the active region. In the calculations, the source radius was assumed to be the mean of the measured values at 212 and 405 K. The effective temperatures of the radio emitting source, assumed homogeneous, obtained from this fit were 0.6–2.9 × 10⁴ K, for source diameters of 2′–7′.  相似文献   

Biochemical indices for instantaneous growth estimation in young cephalopod Sepia officinalis L.   总被引：1，自引：0，他引：1  

Koueta  N.; Castro  B. G.; Boucaud-Camou  E. 《ICES Journal of Marine Science》2000,57(1):1-7

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XMM‐Newton detection of relativistic Fe emission in the X‐ray spectrum of SAX J1711.6–3808     

C. Snchez‐Fernndez  M. Santos‐Lle  J. J. M. In' t Zand  R. Gonzlez‐Riestra  B. Altieri  R. Saxton  A. J. Castro‐Tirado 《Astronomische Nachrichten》2006,327(10):1004-1007

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