Les depots d'enduits manganoferriferes en environnement marin littoral; l'exemple de grottes sous-marines en Mediterranee nord-occidentale

2001 ◽  
Vol 172 (6) ◽  
pp. 765-778 ◽  
Author(s):  
Jacques Allouc ◽  
Jean-Georges Harmelin

Abstract Black coating of hard substrates by Mn and Fe oxides has long been reported from shallow, dark, submarine caves. However, these littoral metallic deposits have never been studied in detail, despite expected analogies with deep-sea polymetallic crusts. Submarine caves are characterized by darkness and low rates of exchanges with the open sea. Lack of primary production and confinement of inner water bodies result in marked oligotrophy and extremely reduced biomass, i.e. conditions close to those prevailing in deep-sea habitats. Field evidences suggested that the formation of Mn-Fe coatings was closely tied to these particular environmental conditions. The goal of this study was to examine the detailed features of Mn-Fe coatings from dark caves with different local conditions, and to try to identify the processes responsible for their deposition. Study sites and methods: Three sublittoral, single-entrance, caves were sampled by scuba diving along the coasts of Provence (France, Mediterranean Sea). The first site is a large karstic cave (Tremies Cave, 16 m depth at entrance floor, 60 m long; Marseille-Cassis area) with an ascending profile which results in a buffered thermal regime and markedly oligotrophic conditions due to warm water trapping in its upper part. Wall fragments were sampled at 30 m (medium confinement: zone B) and 60 m (strong confinement: zone C) from the cave entrance. The second site is a large tubular cavity open in conglomerate formations (3PP Cave, 15 m depth at entrance floor, 120 m long; La Ciotat) with a descending profile which results in relative permanence of winter temperatures within the inner parts, complex water circulation and presumed greater input of sedimented particles than in the preceding cave. Wall samples were taken at 25 m, 70 m and 100 m from entrance. The third site is a small, horizontal, cave open in quartzite formations (Bagaud Cave, 7 m depth at entrance floor, about 10 m long; WNW of Port-Cros Island, bay of Hyeres). Sampling was performed on walls of a narrow corridor between an anterior room and a smaller inner room. A sporadic outflow of continental waters is located in the inner room. The samples were preserved in 50% ethylic alcohol or studied soon after their sampling. Before carbon coating and SEM examination, or microanalyses with SEM-associated spectrometers, they were treated in a 33% Chlorox solution and thereafter washed in demineralized water and dried. Micromorphology: At low-medium magnification (<20,000), the aspect of coatings varies between caves and, especially, between inner-cave locations. All the described structures are made up of Mn and Fe oxides. In Tremies Cave, coatings of walls from zone B are composed of irregular erected constructions (height: 10s to 100s mu m) formed by the aggregation of roughly ovoid primary concretions of about 10 mu m. The surface of those primary concretions displays numerous lacunose to reticulate films (pores, about 0.5 mu m in diameter, are often subrounded). Remnants of these films and organomorphic corpuscles occur also within the primary concretions. On younger substrates (broken wall exposed since 1970), primary concretions are poorly developed and no prominent construction is visible. In more confined conditions (zone C), the erected constructions of ancient coatings are smaller and less numerous than in zone B but are well individualized. In this zone C, besides some remnants of lacunose to reticulate films, there is an appearance of filaments and ovoid corpuscles (height/width: 10-30/5-15 mu m), which seem to be linked to filaments by a short stalk. In 3 PP Cave, at 25-70 m from entrance, wall coatings present porous heaps of primary concretions. The surface and the inside of the latter comprise remnants of lacunose to reticulate films that evoke those observed in Tremies Cave. On younger substrates (hard parts of sessile invertebrates), coatings are restricted to micrometric organomorphic corpuscles with some remnants of lacunose or fibrous films. At 100 m from the entrance, coatings are shaped by numerous erected constructions, more or less coalescing. Besides remnants of lacunose films, the primary concretions contain interlacing filaments (diameter: 0.2-0.3 mu m) forming cords or veils. In Bagaud Cave, the primary concretions are aggregated in irregular heaps. Lacunose films are particularly frequent and tend to form three-dimensional mamillated structures that were not observed in the other caves. In particular, there is an appearance of tubular structures and of numerous hemispheroidal structures (diameter: 4-5 mu m) with an upper orifice. At higher magnification (20,000), whatever the cave and inner-cave location, the aspect of oxide deposits is rather smooth or, especially, microgranular. Mineral composition: The composition of coatings is different between caves and according to their inner-cave location. In both large caves (Tremies and 3 PP), the Mn/Fe ratio increases with the distance from the cave entrance, i.e. when exchanges with the open sea diminish. This trend is particularly clear in Tremies Cave, where the confinement gradient is strongly marked.

2007 ◽  
Vol 36 (4) ◽  
Author(s):  
Małgorzata Robakiewicz

Seasonal variability of hydrodynamics in the Vistula Estuary in 1994The Vistula Estuary is a coastal water body boasting free connection with the open sea, where mixing processes of marine and fluvial waters are maintained by local conditions. Based on results from a hydrodynamic model, applied to represent conditions in the year 1994, and using salinity as a tracer, it was found that fluvial water has a tendency to spread westward from the river mouth. This is in contradiction with the dominant wind direction in the region. Model results confirmed field observations of specific hydrological and meteorological conditions required to transport fluvial water northward, towards the Hel Peninsula.


2015 ◽  
Vol 11 (S320) ◽  
pp. 397-402
Author(s):  
A. A. Vidotto ◽  
R. Fares ◽  
M. Jardine ◽  
C. Moutou ◽  
J.-F. Donati

AbstractThe proper characterisation of stellar winds is essential for the study of propagation of eruptive events (flares, coronal mass ejections) and the study of space weather events on exoplanets. Here, we quantitatively investigate the nature of the stellar winds surrounding the hot Jupiters HD46375b, HD73256b, HD102195b, HD130322b, HD179949b. We simulate the three-dimensional winds of their host stars, in which we directly incorporate their observed surface magnetic fields. With that, we derive the wind properties at the position of the hot-Jupiters’ orbits (temperature, velocity, magnetic field intensity and pressure). We show that the exoplanets studied here are immersed in a local stellar wind that is much denser than the local conditions encountered around the solar system planets (e.g., 5 orders of magnitude denser than the conditions experienced by the Earth). The environment surrounding these exoplanets also differs in terms of dynamics (slower stellar winds, but higher Keplerian velocities) and ambient magnetic fields (2 to 3 orders of magnitude larger than the interplanetary medium surrounding the Earth). The characterisation of the host star's wind is also crucial for the study of how the wind interacts with exoplanets. For example, we compute the exoplanetary radio emission that is released in the wind-exoplanet interaction. For the hot-Jupiters studied here, we find radio fluxes ranging from 0.02 to 0.13 mJy. These fluxes could become orders of magnitude higher when stellar eruptions impact exoplanets, increasing the potential of detecting exoplanetary radio emission.


2006 ◽  
Vol 33 (23) ◽  
Author(s):  
Peter G. Brewer ◽  
Baixin Chen ◽  
Robert Warzinki ◽  
Arthur Baggeroer ◽  
Edward T. Peltzer ◽  
...  

2015 ◽  
Vol 29 (2) ◽  
pp. 223-240 ◽  
Author(s):  
Wei-cai Quan ◽  
Zhu-ying Zhang ◽  
Ai-qun Zhang ◽  
Qi-feng Zhang ◽  
Yu Tian

2009 ◽  
Vol 75 (23) ◽  
pp. 7426-7435 ◽  
Author(s):  
Gabriela Hidalgo ◽  
Andrew Burns ◽  
Erik Herz ◽  
Anthony G. Hay ◽  
Paul L. Houston ◽  
...  

ABSTRACT Attached bacterial communities can generate three-dimensional (3D) physicochemical gradients that create microenvironments where local conditions are substantially different from those in the surrounding solution. Given their ubiquity in nature and their impacts on issues ranging from water quality to human health, better tools for understanding biofilms and the gradients they create are needed. Here we demonstrate the use of functional tomographic imaging via confocal fluorescence microscopy of ratiometric core-shell silica nanoparticle sensors (C dot sensors) to study the morphology and temporal evolution of pH microenvironments in axenic Escherichia coli PHL628 and mixed-culture wastewater biofilms. Testing of 70-, 30-, and 10-nm-diameter sensor particles reveals a critical size for homogeneous biofilm staining, with only the 10-nm-diameter particles capable of successfully generating high-resolution maps of biofilm pH and distinct local heterogeneities. Our measurements revealed pH values that ranged from 5 to >7, confirming the heterogeneity of the pH profiles within these biofilms. pH was also analyzed following glucose addition to both suspended and attached cultures. In both cases, the pH became more acidic, likely due to glucose metabolism causing the release of tricarboxylic acid cycle acids and CO2. These studies demonstrate that the combination of 3D functional fluorescence imaging with well-designed nanoparticle sensors provides a powerful tool for in situ characterization of chemical microenvironments in complex biofilms.


1982 ◽  
Vol 1 (18) ◽  
pp. 16
Author(s):  
G. De F Retief ◽  
G.K. Prestedge ◽  
F.P.J. Muller

The South African wave energy program has been underway for several years and has included an analysis of the temporal and spatial distribution of wave energy along the full coast-line, determination of energy attenuation perpendicular to the coast-line at a site on the south western coast, and the development of a wave energy converter which is most suited to local conditions and requirements. The resource analysis has shown that the inshore power levels occurring along the south western coast are as promising as any elsewhere in the world. A bottom mounted, V-shaped wave energy conversion device driving an air turbine has been found to be most suited to prevailing conditions. The conversion characteristics of the device are presented, based on 1:100 scale three dimensional and 1:50 scale two dimensional model studies. Preliminary design studies of the proposed conversion system have underlined its potential viability as a cost effective supplementary source of power.


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