Preliminary results of optical searches of IPN3 localizations

We present preliminary results from deep optical searches of small (5 arcmin²) GRB error boxes determined using the Third Interplanetary Network (IPN³). Two of these fields also have been found to have historical OT events located within the IPN³ error boxes. We compare the preliminary results of these searches to those reported for the larger IPN¹ error boxes. The small size of the IPN³ error boxes should allow a test of the hypothesis suggested by the IPN¹ study that there are excess QSOs associated with the GRB fields.     

High resolution fabry-perot and multi-pupil spectral observations of the genuine blue compact dwarf galaxy IZW18

We present the observations of the BCDG IZW18 performed with a Fabry-Perot interferometer at the CFH 3.6 m telescope and with a multi-pupil spectrograph at the SAO (Russia) 6 m telescope. The morphological structure of the galaxy in emission lines and in continuum, the velocity field of the ionized gas, and [OIII]/H ratio distribution along the NW component have been investigated. Besides the NW and SE HII components, we find a population of small HII regions. Continuum maps show that the peaks of the stellar light distribution are displaced with respect to the emission lines maxima. the velocity field shows peculiar motions superposed on an approximately regular background implying solid body rotation. Emission line profiles exhibit an asymmetric structure, except for the NW compact component. The [OIII]/H ratio decreases from the center of the NW component to its edge with the gradient of 1.86 kpc^–1.Published in Astrofizika, Vol. 38, No. 4, pp. 602–615, October–December, 1995.     

French-Armenian scientific cooperation on study of some HII-regions with cigale

The results of the scientific cooperation between astronomers of the Byurakan and Marseille observatories on the study of diffuse matter in the Galaxy are presented.H -emission is discovered in the direction of h and x Per. Fabry-Perot observations of three HII-regions, Sh2-152, 153, and 106, show the expansion of the diffuse matter relative to the exciting stars. In the Sh2-106 region a probable jet is found. It is shown that in star forming regions the diffuse matter takes part in expansion motions together with stars.Published in Astrofizika, Vol. 38, No. 4, pp. 559–564, October–December, 1995.     

Vinciennite and Cu-excess tennantite from the Layo (Cu,Sn, As,Au) epithermal deposit (Southern Peru)

Summary The Layo epithermal deposit, cutting Miocene-Pliocene calc-alkaline volcanites of the Tacaza group, includes a well-developed eastern zone (Vetas 7 and 8) in which brecciated and banded textures are associated with a large, intensely argillized zone containing diaspore and alunite. The vetas contain a typical Cu-As mineralogy of the acid-sulfate type (pyrite, enargite, Cu-excess tennantite, chalcopyrite, covellite) with an associated original stanniferous paragenesis including vinciennite and mawsonite. The vinciennite is close to the ideal end-member (Cu₁₀Fe₄SnAsS₁₆) and the Cu-excess tennantite (Cu₁₁FeAs₄S₁₃) shows a total absence of Zn and Ag; its very specific chemical composition suggests that all the iron is Fe³⁺, equilibrated by Cu⁺ and probably minor Cu²⁺.This particular mineralogical association implies deposition at relatively low temperature (300°C) and high aS₂ (10^–6.5 decreasing to 10^–8.5), from a Cu-S-rich and Fe-Zn-poor fluid. The acid-sulfate epithermal mineralization of the eastern vetas of Layo appears to have preceded an adularia-sericite epithermal mineralization expressed in the western vetas of Layo and also in the nearby large epithermal veins at Orcopampa and Shila. It also supports the genetic relationship that is commonly evoked between porphyry copper and epithermal deposits.

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Le minéralogie originale à vinciente et tennantite riche du gisement épithermal (Cu, Sn, As, Au) de Layo (Sud Péru)

Résumé Le gîte épithermal de Layo est encaissé dans les volcanites calco-alcalines Miocène-Pliocène du groupe de Tacaza. Sa zone orientale renferme des corps minéralisés (Vetas 7 et 8) bien développés, à textures bréchiques et rubanées associées à une large zone intensément argilisée contenant diaspore et alunite.Les vetas présentent une association minéralogique à As-Cu typique des gisements acide-sulfate (pyrite, énargite, tennantite riche en cuivre, chalcopyrite, covellite) et une paragenèse stannifère originale renfermant vinciennite et mawsonite. La vinciennite est proche du pôle théorique (Cu₁₀Fe₄SnAsS₁₆) et la tennantite riche en Cu (Cu₁₁FeAs₄S₁₃) est dépourvue de Zn et de Ag; sa composition chimique suggère que tout le fer se présente sous la forme Fe³⁺, en équilibre avec Cu⁺, avec probablement une participation mineure de Cu²⁺.Cette association minéralogique particulière implique une mise en place sous forte fugacité en soufre (aS₂ = 10^–6.5 décroissant jusqu'à 10^–8.5) à une température relativement basse de l'ordre de 300°C à partir d'un fluide riche en Cu et S et pauvre en Fe et Zn. La minéralisation de type acide-sulfate des vetas orientales de Layo précéderait celles de type adulaire-sericite des vetas occidentales de Layo et des gisements voisins de Orcopampa et Shila. Elle contribue à renforcer le lien fréquemment évoqué entre les porphyres cuprifères et les gisements épithermaux.

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With 10 Figures     

On the quality of resonant absorption as a coronal loop heating mechanism

The qualityQ of a resonance is defined as the ratio of the total energy contained in the system to the dissipation per driving cycle. Hence, a good quality resonance is one with little losses, i.e., little dissipation per driving cycle. However, for heating coronal plasmas by means of resonant absorption of waves, bad quality resonances are required. Here, the quality of the MHD resonances that occur when an inhomogeneous coronal loop is excited by incident waves is investigated for typical coronal loop parameter values in the frame work of linear, resistive MHD. It is shown that the resonances in coronal loops have bad quality and, hence, yield a lot of Ohmic heating per driving cycle compared to the total energy stored in the loop. As a consequence, the time scales of the heating process are relatively short and resonant absorption turns out to be a viable candidate for the heating of the magnetic loops observed in the solar corona.     

Numerical Modeling of Wave-Enhanced Turbulence in the Oceanic Upper Layer

A coupled model of air-wave-sea interaction is modified based on a new roughness formulation and the latest data. The model parameters for aerodynamic roughness from below (ARB) and wave-dependent roughness from above (ARA, z _0a ) are assumed equal. The combined roughness is assumed to be a function of friction velocity, gravity, air and seawater densities, and wave age (c _w ). The model is used in a study of wave-enhanced turbulence under breaking waves to predict turbulent dissipation (), ARA, and drag coefficient (C _d ). Both waves and shear production are considered as sources of ocean turbulent energy. The atmospheric part of the model is used only to specify a correct condition at the interface. Numerical experiments are performed to study the -distribution, z _0a and C _d , and to compare with data. The major achievement is model verification using all available data. The first full application of this model is in conjunction with an ocean circulation model in a coupled circulation-wave system. Simulations show that the -distribution is strongly dependent on local wind-forced wave heights. For each wind and wave state there is a particular wave-dependent depth that is verified by data. The comparison shows that the model predicted agrees well with the observed of the z ^–4 law distribution of Gargett (1989). Simulations also show that waves have an important role in causing to differ from the classical wall-layer theory and z _0a , with a value of 0.30 for the empirical constant a _a . The model-predicted , z _0a , C _d and C _gd agree well with data.     

Submarine hydrothermal brine seeps off Milos, Greece. Observations and geochemistry

A shallow hydrothermal brine seep located off the Greek island of Milos in the Aegean Sea was studied. The brine fluid outcropped as a pool of water in a seabed depression and was detected in the surrounding pore-waters of sediments colonised by the sulphur bacterium Achromatium volutans. The seep fluid was highly saline and sulphidic, depleted in Mg²⁺ and SO₄²⁻, but enriched over seawater in Na⁺, Ca²⁺, K⁺, Cl⁻, SiO₂, reduced species and dissolved gases. The high concentrations of Na⁺, Ca²⁺ and K⁺ were consistent with the Milos tectonic setting. Na-K and Na-K-Ca geothermometers predicted a reservoir temperature of 300–325 °C for the most concentrated seep samples. The deep geothermal reservoir within the metamorphic basement of Milos island has already been located and studied and may represent the source of the seep fluid. Faunal diversity was lowest in seep-influenced sediments, but a sulphide-intolerant species was found in areas of the bacterial mat where salinity and temperature were much lower. Pressure-induced variations in the vertical depth of the brine interface may be occurring in the sediment.     

Horizontal Pressure Gradient Errors of the Monterey Bay Sigma Coordinate Ocean Model with Various Grids

A coastal ocean -coordinate model of Monterey Bay (MOB) with realistic bottom topography and coastlines is developed using the Princeton Ocean Model (POM) and grid generation technique (GGT) to study the horizontal pressure gradient errors associated with the MOB steep topography. The submarine canyon in MOB features some of the steepest topography encountered anywhere in the world oceans. The MOB grids are designed using the EAGEAL View and GENIE⁺⁺ grid generation systems. A grid package developed by Ly and Luong (1993) is used in this study to couple grids to the model. The MOB model is tested with both orthogonal and curvilinear nearly-orthogonal (CNO) grids. The CNO grid has horizontal resolution which varies from 300 m to 2 km, while the resolution of the orthogonal grid is uniform with x = 1.25 km and y = 1.38 km. These grids cover a domain of 180 × 160 km with the same number of grid points of 131 × 131. Vertical resolutions of 25, 35 and 45 vertical sigma levels are tested. The error in the MOB are evaluated in terms of mean kinetic energy and velocity against various grids, vertical, horizontal resolution and distributions, and bottom topography smoothing. Simulations with various grids show that GGT can be used as another tool in reducing -coordinate errors in coastal ocean modeling besides increasing resolution and smoothing bottom topography. Topographical smoothing not only reduces topographic slope, but changes realistic topography. A CNO grid with a high grid density packed along steep slopes and Monterey Submarine Canyon reduces the errors by 40% compared to a rectangular grid with the same number of grid points. The CNO grid is more efficient than the rectangular grid, since it has most of its grids over water. The simulations show that the presented MOB -coordinate model can be used with a confidence regarding horizontal pressure gradient error.     

Marine and Brackish Ecosystems of South Brittany (Lorient and Vilaine Bays) with Particular Reference to the Effect of the Turbidity Maxima

The south Brittany coast of France offers considerable opportunities to study the transition between estuaries and the sea. The sea coast is semi-enclosed, due to the local geomorphology, with sheltered conditions. The infaunal macrobenthic communities have been identified and characterized by species richness (S), abundance (A) and biomass (B), related to environmental factors. The spatial succession of infauna along the estuarine gradient shows the presence of an area with a much reduced fauna, and an oligobiotic area with low values of S, A and B. In these strongly stratified estuaries, concentration of organic matter and sediment can result in oxygen depletion, which is not favourable for survival of the infauna. The oligobiotic area seems to be related to the presence of the turbidity maximum, the location and importance of which are functions of river discharge and hydrodynamic mixing. The turbidity maximum which causes these conditions is shown to be at a higher salinity than has previously been described for this phenomenon, and is shown to break the spatial gradient of marine to brackish communities which has been described in larger estuaries.     

Austauschuntersuchungen mittels luftelektrischer Messungen

Zusammenfassung Die bekannten Parallelen im tagesperiodischen Verhalten von Dampfdruck und Potentialgefälle in verschiedenen Höhen sind als Auswirkungen der gleichen Grunderscheinung des atmosphärischen Massenaustausches zu werten. Es liegt nahe, beide Elemente gemeinsam zu Austauschuntersuchungen heranzuziehen. Die Möglichkeiten, luftelektrische Untersuchungen in verschiedenen Höhenniveaus für solche Zwecke zu benutzen, werden im einzelnen diskutiert.

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Summary The well known parallels between vapour-pressure and potentialgradient with regard to their diurnal variation in different heights results from the same basic element, the atmospheric mass exchange. It is obvious to use a combination of both elements for an investigation of the exchange. In this paper the possibilities for a utilisation of measurements of the atmospheric electricity in different heights for such purposes are discussed in detail.

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Résumé Le parallélisme bien connu entre la variation diurne de la pression de vapeur d'eau et du gradient de potentiel électrique à différents niveaux peut être regardé comme l'effet du même phénomène de l'échange turbulent de l'atmosphère. Il est donc légitime d'employer ces deux éléments pour l'étude de l'échange turbulent. On discute ici en détail les possibilités d'étudier à cet effet les mesures de l'électricité atmosphérique faites à différentes altitudes.

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Mit 3 Textabbildungen.