High gene flow promotes the genetic homogeneity of the fish goby Pomatoschistus marmoratus (Risso, 1810) from Mar Menor coastal lagoon and adjacent marine waters (Spain)     

Carlos Vergara‐Chen  Mercedes González‐Wangüemert  Concepción Marcos  Ángel Pérez‐Ruzafa 《Marine Ecology》2010,31(2):270-275

The extreme environmental variability of coastal lagoons suggests that physical and ecological factors could contribute to the genetic divergence among populations occurring in lagoon and open‐coast environments. In this study we analysed the genetic variability of lagoon and marine samples of the sand goby, Pomatoschistus marmoratus (Risso, 1810) (Pisces: Gobiidae), on the SW Spain coast. A fragment of mitochondrial DNA control region (570 bp) was sequenced for 196 individuals collected in five localities: Lo Pagan, Los Urrutias and Playa Honda (Mar Menor coastal lagoon), and Veneziola and Mazarrón (Mediterranean Sea). The total haplotype diversity was h = 0.9424 ± 0.0229, and the total nucleotide diversity was π = 0.0108 ± 0.0058. Among‐sample genetic differentiation was not significant and small‐scale patterns in the distribution of haplotypes were not apparent. Gene flow and dispersal‐related life history traits may account for low genetic structure at a small spatial scale. The high genetic diversity found in P. marmoratus increases its potential to adapt to changing conditions of the Mar Menor coastal lagoon.  相似文献   

Predicting significant wave height with artificial neural networks in the South Atlantic Ocean: a hybrid approach     

Marangoni Gazineu Marinho Pinto  Paula  Martins Campos  Ricardo  Gallo  Marcos Nicolas  Parente Ribeiro  Carlos Eduardo 《Ocean Dynamics》2023,73(6):303-315

Ocean Dynamics - Accurate simulations of significant wave height (Hs) are extremely important for the safety of navigation, port operations, and oil and gas exploration. Thus, accurate forecasts of...  相似文献   

Sediment characteristics and internal architecture of offshore sand ridges on a tideless continental shelf (western Mediterranean)     

Ruth Durán  Jorge Guillén  Marta Ribó  Gonzalo Simarro  Araceli Muñoz  Albert Palanques  Pere Puig 《地球表面变化过程与地形》2020,45(14):3592-3606

An integrated approach combining swath bathymetry, an extensive dataset of vibrocores and high-resolution seismic reflection data was used to assess the origin and evolution of offshore sand ridges on a tideless continental shelf (Gulf of Valencia, western Mediterranean). The sand ridges are located in the mid-outer shelf at 55–85 m water depth, obliquely oriented to the shoreline. They are 1.5 to 7 m high, with a wavelength between 600 and 1,100 m and a mean height-to-wavelength ratio of 0.004. The sand ridges are composed of well-sorted medium sand and are partially covered by a mud layer, evidencing a moribund stage. They overlie an erosion surface that locally crops out at the seafloor and is interpreted as the Holocene wave-ravinement surface. In the sediment cores, this surface corresponds to an erosional lag composed of coarse sand and gravel with pebbles. Small topographic irregularities on this surface are interpreted as shoreline-associated features that may act as the precursor for ridge development. Their preservation within the sand ridges could be related to the hardness of these features. Internally, the sand ridges display high-angle dipping reflections, indicating ridge migration towards the southeast in the direction of the present-day sediment transport direction. The presence of interbedded mud layers, associated with these reflections, indicates intermittent episodes of mud deposition when active. The internal architecture of some small ridges also provides new insights into their transition from an active to moribund state, as evidenced by a change in the geometry of the internal units from progradational to aggradational, finally being overlain by onlapping finer deposits over the flanks and in the troughs. The Gulf of Valencia sand ridge field constitutes a valuable potential sand resource of 22 million m³ of well-sorted medium and coarse sand with limited mud content, which must be preserved as a strategic sand reservoir. © 2020 John Wiley & Sons, Ltd.  相似文献   

Assessing rheological properties of fluid mud samples through tuning fork data     

Fonseca  Diego Luiz  Marroig  Patrícia Cunha  Carneiro  Juliane Castro  Gallo  Marcos Nicolás  Vinzón  Susana Beatriz 《Ocean Dynamics》2019,69(1):51-57

Ocean Dynamics - At the nautical bottom approach, part of the fluid mud layers can be included in the available depth if they present favorable rheology. As it is difficult to perform in situ...  相似文献   

Long-term Regional Dynamic Sea Level Changes from CMIP6 Projections     

Bruno FERRERO  Marcos TONELLI  Fernanda MARCELLO  Ilana WAINER 《大气科学进展》2021,38(2):157-167

Anthropogenic climate forcing will cause the global mean sea level to rise over the 21st century.However,regional sea level is expected to vary across ocean basins,superimposed by the influence of natural internal climate variability.Here,we address the detection of dynamic sea level(DSL)changes by combining the perspectives of a single and a multimodel ensemble approach(the 50-member CanESM5 and a 27-model ensemble,respectively,all retrieved from the CMIP6 archive),under three CMIP6 projected scenarios:SSP1-2.6,SSP3-7.0 and SSP5-8.5.The ensemble analysis takes into account four key metrics:signal(S),noise(N),S/N ratio,and time of emergence(ToE).The results from both sets of ensembles agree in the fact that regions with higher S/N(associated with smaller uncertainties)also reflect earlier ToEs.The DSL signal is projected to emerge in the Southern Ocean,Southeast Pacific,Northwest Atlantic,and the Arctic.Results common for both sets of ensemble simulations show that while S progressively increases with increased projected emissions,N,in turn,does not vary substantially among the SSPs,suggesting that uncertainty arising from internal climate variability has little dependence on changes in the magnitude of external forcing.Projected changes are greater and quite similar for the scenarios SSP3-7.0 and SSP5-8.5 and considerably smaller for the SSP1-2.6,highlighting the importance of public policies towards lower emission scenarios and of keeping emissions below a certain threshold.  相似文献   

Determination of stress directions from plagioclase fabrics in high grade deformed rocks (Além Paraíba shear zone, Ribeira fold belt, southeastern Brazil)     

Marcos Egydio-Silva  David Mainprice 《Journal of Structural Geology》1999,21(12):1023

A new method to determine stress directions using the preferential orientation of plagioclase mechanical twins has been applied to high-temperature mylonitic rocks from the Além Paraíba shear zone, Ribeira fold belt, southeastern Brazil. We have measured the lattice-preferred orientation of plagioclase grains and calculated the orientation of the stress axes possible for the observed twin orientations. The maximum compressive stress direction (σ₁), determined for all studied samples, is a function of the mechanical twin orientations of a number of distinct plagioclase populations. The σ₁ direction is generally subperpendicular to the (010) plane. The statistical treatment for most of the plagioclase grains examined for each sample shows that σ₁ is almost perpendicular to the foliation plane, suggesting a significant coaxial component in the deformation process of these rocks.  相似文献   

Some Results from the Hailpad Network in León (Spain): Noteworthy Correlations among Hailfall Parameters     

R. Fraile  J. L. Sánchez  J. L. de la Madrid  A. Castro  J. L. Marcos 《Theoretical and Applied Climatology》1999,64(1-2):105-117

Summary  Since 1990 the Laboratory for Atmospheric Physics at the University of León has made use of a network of 250 hailpads spread over an area of 1000 km² in the province of León (north-western Spain). By the end of 1995, the network had detected 25 hailfalls of more than 15 km² in area, registered on 13 different days during the summer months. The 25 hailfalls were precipitated over more than 300 separate hailpads, leaving nearly 40 000 measurable prints. The size of each hailstone, whose mass and kinetic energy were taken simply as a function of the diameter of the stone was calculated using the hailpad network. In this way, an estimate has been made of the total quantity of ice which fell in each hailfall (circa 19 000 metric tons on average, although a figure ten times this was calculated for one particular hailstorm). The spatial evolution of the physical variables of the hail, determined from each pad, has also been graphically represented. In addition, the distribution of hailstone sizes has been analysed, and the characteristic distribution parameters calculated. Although exponential distribution is often used, the Kolmogorov-Smirnov test of goodness-of-fit shows a better fit for gamma distribution. The information provided by these parameters has been analysed for both distributions, in relation to some specific variables associated with hail. There is a good correlation between total energy and mass precipitated, but the quantity of hail per unit area correlates with the total energy or mass of the precipitation only through the area affected. The size distribution parameters only show good correlations with the maximum hailstone size recorded. Received October 1, 1998 Revised March 8, 1999  相似文献   

Reconstructing the ancestral (Plio-Pleistocene) Rio Grande in its active tectonic setting, southern Rio Grande rift, New Mexico, USA     

Marta Perez-Arlucea  Greg Mack  & Mike Leeder 《Sedimentology》2000,47(3):701-720

Deposits of the ancestral Rio Grande (aRG) belonging to the Camp Rice Formation are preserved and exposed in the uplifted southern portion of the Robledo Mountains horst of the southern Rio Grande rift. The sediments are dated palaeomagnetically to the Gauss chron (upper Pliocene). The lower part of the succession lies in a newly discovered palaeocanyon cut into underlying Eocene rocks whose margins are progressively onlapped by the upper part. Detailed sedimentological studies reveal the presence of numerous river channel and floodplain lithofacies, indicative of varied deposition in channel bar complexes of low‐sinuosity, pebbly sandbed channels that traversed generally dryland floodplains and shifted in and out of the study area five times over the 1 Myr or so recorded by the succession. Notable discoveries in the deposits are: (1) complexes of initial avulsion breakout channels at the base of major sandstone storeys; (2) common low‐angle bedsets ascribed to deposition over low‐angle dunes in active channels; (3) palaeocanyon floodplain environments with evidence of fluctuating near‐surface water tables. Sand‐body architecture is generally multistorey, with palaeocurrents indicative of funnelling of initial avulsive and main fluvial discharge from the neighbouring Mesilla basin through a narrow topographic gap into the palaeocanyon and out over the study area. An avulsion node was evidently located at the stationary southern tip to the East Robledo fault during Gauss times, with aRG channels to the north flowing close to the fault and preventing fan progradation. Subsequent Matuyama growth of the fault caused (1) deposition to cease as the whole succession was uplifted in its footwall, (2) development of a thick petrocalcic horizon, and (3) fan progradation into the Mesilla basin. Parameters for the whole aRG fluvial system are estimated as: active single channels 2 m deep and 25 m wide; valley slope 0·24–0·065°; maximum mean aggradation rate 0·05 mm year^–1; major channel belt avulsion interval 200 ky; individual channel recurrence interval 100 ky; minimum bankfull mean flow velocity 1·54 m s^–1, minimum single‐channel discharge 77 m³ s^–1, bed shear stress 22·3 N m^–2; and stream power 34·3 W m^–2.  相似文献   

The heating of the temperature minimum region in solar flares — A reassessment     

A. Gordon Emslie  Marcos E. Machado 《Solar physics》1979,64(1):129-134

As a sequel to the work by Machado et al. (1978), we discuss and evaluate the suggestions made by these authors on how to possibly reconcile the observed temperature enhancements at temperature-minimum levels in solar flares with some form of theoretical heating mechanism. After establishing the H^– LTE assumption used by Machado et al., we then consider EUV irradiation, and joule heating by steady currents, as heating mechanisms. We find that, unless there are strong inhomogeneities associated with either mechanism, neither can reasonably be reconciled with observations. It is concluded that detailed, high resolution (both spatial and temporal) measurements are necessary to further our understanding of the flare process at temperature-minimum levels.On leave from: Department of Astronomy, The University, Glasgow G12 8QQ, Scotland, U. K.  相似文献   

Macroscopic motions in prominences     

Hugo Grossi Gallegos  Marcos E. Machado 《Solar physics》1973,31(2):427-436

We have studied three pairs of prominences, two of them clearly showing the effect of interaction by a dynamical plasma bridge. The other one was a superimposed optical pair which also showed, after being spectroscopically studied, the possible effect of interaction. We have calculated the atom density in the prominence and bridges, and applied the Goldberg-Unno method for the determination of Doppler-widths of the calcium H and K lines.  相似文献