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1.
R. Albrecht R. Albrecht P. Benvenuti P. Benvenuti F. Pierfederici 《Astrophysics and Space Science》2004,290(3-4):431-438
Given the high cost of modern astronomical observing facilities it is evident that efforts must be made to optimally exploit the data in order to maximize the return on investment. This concept was first implemented on a large scale for the Hubble Space Telescope, and has since been taken over for other space borne and large ground-based facilities. The European HST Science Data Archive is located at the European Southern Observatory (ESO). It has been extended to include data from ESO telescopes and instruments, especially the Very Large Telescope (VLT) and Wide Field Imager (WFI). It was thus natural to design the archive such that queries could be extended across its full content, regardless of the origin of the data. This constituted a first step toward a virtual observatory. The Astrovirtel program, first established in 1999–2000 with funding provided by the European Commission, makes it possible for scientists to use this facility for their investigations. At the same time it allowed us to establish science requirements for archive cross queries, and to define capabilities required for VO's. Recently the European Commission decided to provide the funding for the implementation of the Astrophysical Virtual Observatory (AVO). This will include several European observatories and scientific organizations. It is being developed in close coordination with the US National Virtual Observatory. 相似文献
2.
Mine waste dumps and heavy metal pollution in abandoned mining district of Boccheggiano (Southern Tuscany, Italy) 总被引：12，自引：1，他引：11
M. Benvenuti I. Mascaro F. Corsini P. Lattanzi P. Parrini G. Tanelli 《Environmental Geology》1997,30(3-4):238-243
Mining activity in the Boccheggiano-Fontalcinaldo area (Southern Tuscany) dates back at least to the 16th century AD and
lasted up to very recent times. Copper-rich hydrothermal veins, massive pyrite deposits, and their gossans were exploited.
Two mine waste dumps (Fontalcinaldo, Fontebona), one flotation tailings impoundment (Gabellino), and one roasting/smelting
waste dump (Merse-Ribudelli) in the study area were selected to ascertain the environmental effects of such protracted mining
activity. Primary waste mineralogy is mainly characterized by pyrite, gypsum, quartz, carbonates, chlorites, and micas. Secondary
oxidation mineralogy includes Fe and Cu sulfates and hydroxy sulfates, Cu carbonates, Fe and Al oxyhydroxides, and other phases
[neogenic cassiterite at Fontalcinaldo; probable calkinsite, (Ce,La)2(CO3)3· 4H2O, at Fontebona]. Mine waste samples show extremely variable contents of toxic elements (Cu, Pb, Zn, Bi, Cd, As), with average
values in the order of hundreds to thousands of parts per million (except for Bi and Cd). In some samples, the abundance of
proper minerals of these metals cannot account for the entire metal load. Conceivably, either solid solution substitutions
or adsorption processes contribute to the intake of released metals into newly formed minerals. Release and transport of pollutants
was affected to variable degrees by acid-neutralization processes. The highest metal and acid concentrations occur close to
the investigated wastes and rapidly decrease moving downstream some hundreds of meters or less, with the partial exception
for Mn and Fe. Other than dilution effects, this phenomenon may be ascribed to metal adsorption and precipitation of solid
phases.
Received: 16 April 1995 · Accepted: 14 December 1995 相似文献
3.
Marco Benvenuti Marco Bonini Giovanna Moratti Marianna Ricci Chiara Tanini 《Geomorphology》2008,100(3-4):269-284
Integration of geomorphology, stratigraphy, sedimentology and morphotectonics in the analysis of the lower Cecina River reach, coastal Tuscany, reveals an undocumented historical channel avulsion. Geomorphological evidence and radiocarbon dating support that, from the Last Glacial Maximum until the end of the 16th century, the Cecina River flowed north of the present course and formed a well-developed cuspate delta. Two concurrent factors, active tectonics as a preparing factor and discharge regime as an activation factor, are thus inferred to have favored the avulsion of Cecina River. Fragmentary archaeological and historical records indicate that the late Holocene Cecina River plain was virtually unpopulated until the latest 16th century. This seems the main reason why high-magnitude hydrological events and prominent river channel avulsions were not reported in historical chronicles. From this perspective, geomorphological data may provide important knowledge and understanding of recent dynamics of environmental change when historical record is lacking or missing. 相似文献
4.
Pilario Costagliola Marco Benvenuti Laura Chiarantini Sara Bianchi Francesco Di Benedetto Mario Paolieri Luca Rossato 《Applied Geochemistry》2008
A significant As anomaly has been reported in the literature for stream sediments and unlithified Quaternary deposits of the Pecora River valley in Southern Tuscany, extending from the “Colline Metallifere” pyrite-base metals district to the Tyrrhenian Sea. The As anomaly spreads over several square kilometers around a core that exceeds 500 ppm. Several source contributions (from natural to anthropogenic) have been invoked to explain the observed As distribution in the Pecora Valley, including the metal-working industry which was active in this area, particularly in Etrusco-Roman times and in the Middle Ages. In order to evaluate the contribution of ancient mining and metallurgical activities in the Pecora Valley to elevated As concentrations in the environment, a detailed mineralogical and geochemical survey of metallurgical slags and smelted ore minerals was undertaken from six different sites through the Pecora Valley: Poggio Butelli (Etrusco-Roman iron slags); Sata Creek, Arialla, Marsiliana, Forra and Cascata sites (all Medieval base metals slags). The As content of Etrusco-Roman slags is relatively low (few tens of ppm), whereas Medieval slags show variable, but higher amounts of base metals (±Ag) (ranging from tens to tens of thousands ppm) and As (up to 267 ppm, with average contents of about 40 ppm). Arsenic is mostly partitioned in sulfides disseminated through the glassy groundmass rather than in solid solution with the glassy matrix. Remnants of the ore used for base metal and Ag smelting during the Middle Ages had the highest As contents (up to about 1000 ppm). 相似文献
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Moratti G. Benvenuti M. Santo A. P. Laurenzi M. A. Braschi E. Tommasini S. 《International Journal of Earth Sciences》2018,107(7):2491-2515
International Journal of Earth Sciences - This study is based upon a stratigraphic and structural revision of a Middle Jurassic–Upper Cretaceous mostly continental succession exposed between... 相似文献
8.
Summary The barite-pyrite-(Pb-Zn-Ag) deposit of Pollone is located in the southernmost tip of the Apuane Alps metamorphic core complex, and is hosted by a siliciclastic formation of pre-Norian age. The southern sector of the deposit mainly consists of stratiform, supposedly syngenetic, barite-pyrite orebodies, whereas the northern area is characterized by a barite-pyrite-(Pb-Zn-Ag) vein system. Vein geometry in the northern area is controlled by a shear zone, developed during the greenschist facies metamorphism which affected the Apuane Alps core complex between 27 and 8 Ma, that was responsible for fluid focusing and vein emplacement. At Pollone, arsenopyrite and chlorite geothermometers show broadly comparable results, and suggest local metamorphic peak temperatures between 320 and 350°C. Phengite geobarometry indicates minimum pressures of about 3.5 kbar. Fluid inclusion data and mineral equilibria suggest that the mineralizing fluids were initially hotter than the country rocks (about 450°C at 3.5–4.0 kbar). Rocks in direct contact with the orebodies are depleted in Rb and enriched in Sr in comparison to similar rocks elsewhere in the area. This is attributed to the presence of Rb-poor muscovite and Sr-rich barite. Rb-depleted muscovites suggest mineral-fluid interaction in a rock reservoir characterized by a different (modal) mineralogical composition than the Pollone host rocks. The progressive decrease of Sr in barite with increasing distance from the orebodies may be explained with a temperature decrease along the infiltration paths of mineralizing fluids (i.e., from the vein into the wall rocks). The similar O-isotope composition of quartz from veins and host rocks is explained with the overall homogeneous O-isotope composition of the Alpi Apuane basement rocks. This indicates a limited interaction between mineralizing fluids and the rocks exposed at Pollone. Remobilization of syngenetic orebodies was conceivably of minor importance in the production of metamorphogenec veins. Fluid cooling along a major tectonic lineament is thought to be responsible for barite deposition.
Die metamorphogenen Baryt-Pyrit (Pb-Zn-Ag) Gänge von Pollone, Apuanische Alpen, Toskana: Geometrie der Gänge, Geothermobarometrie, Flüssigkeitseinschlüsse und Geochemie
Zusammenfassung Die Baryt-Pyrit (Pb-Zn-Ag) Lagerstätte von Pollone liegt im südlichsten Ende des metamorphen Kern-Komplexes der Apuanischen Alpen, und sitzt in einer siliziklastischen Formation prä-Norischen Alters auf. Der südliche Sektor der Lagerstätte besteht hauptsächlich aus stratiformen, wahrscheinlich syngenetischen Baryt-Pyrit-Erzkörpern, während der nördliche Teil des Gebietes durch ein Baryt-Pyrit (Pb-Zn-Ag) Gangsystem charakterisiert wird. Die Geometrie der Gänge im Nordteil wird durch eine Scherzone kontrolliert, die während einer grünschieferfaziellen Metamorphose entstanden ist, die den Kernkomplex der Apuanischen Alpen zwischen 27 und 8 Ma betroffen hat. Diese Scherzone war auch für die Zufuhr der Fluide und die Platznahme der Gänge verantwortlich. In Pollone zeigen Arsenopyrit- und Chlorit-Geothermometrie weithin vergleichbare Ergebnisse und weisen auf lokale Maximaltemperaturen der Metamorphose zwischen 320 und 350°C hin. Phengit-Geobarometrie läßt Minimal-Drucke von ungefähr 3,5 kbar erkennen. Fluidflüssigkeitseinschluß-Daten und Mineral-Gleichgewichte zeigen, daß die erzbringenden Fluide ursprünglich heißer als die Wirtsgesteine waren (ca. 450 °C für P von 3,5 bis 4 kbar). Gesteine, die im direkten Kontakt mit den Erzkörpern sind, zeigen eine Anreicherung an Rb und eine Anreicherung an Sr, im Vergleich mit ähnlichen Gesteinen, die im Gebiet anzutreffen sind. Dies wird auf das Vorkommen von Rb-armen Muscovit und Sr-reichen Baryt zurückgeführt. An Rbabgereicherte Muscovite legen Mineral-Fluid-Reaktionen nahe, die in einem Gesteinsreservoir abliefen, das durch eine andere mineralogische Zusammensetzung als die Wirtsgesteine von Pollone charakterisiert war. Der zunehmende Verlust von Sr im Baryt mit zunehmender Entfernung von den Erzkörpern, kann durch einen Temperaturabfall entlang der Infitrations-Pfade der erzführenden Lösungen erklärt werden (d.h. von Gang in die Nebengeseine). Die ähnliche Sauerstoff-Isotopen-Zusammensetzung für Quarz aus den Gängen und den Nebengesteinen läßt sich auf die allgemein homogene Sauerstoffisotopen-Signatur des Basements der Apuanischen Alpen zurückführen. Dies weist auf beschränkte Wechselwirkung zwischen erzführenden Lösungen und den in Pollone anstehenden Gesteinen hin. Die Remobilisation von syngenetischen Erzkörpern in Pollone war nur von geringer Bedeutung für die Entstehung der metamorphogenen Gänge. Abkühlung der Fluide an einem wichtigen tektonischen Lineament gilt als Ursache für den Absatz von Baryt.相似文献
9.
This article reports a stratigraphic and structural analysis of the Neogene‐Quaternary Valdelsa Basin (Central Italy), filled with up to 1000 m of uppermost Miocene to lower Pleistocene strata. The succession is subdivided into seven unconformity‐bounded stratigraphic units (synthems, or large‐scale depositional sequences) that include fluvio‐deltaic and shallow‐marine deposits. Structures related to basin shoulders and internal boundaries controlled the Neogene location and geometry of different depocentres. During the Tortonian‐Messinian, a buried NE‐trending high related to regional, basin‐transverse lineaments separated two adjacent sub‐basins. During the lower Pliocene, compressional displacement along NW‐trending, thrust‐related highs controlled the distribution of depocentres and dispersal of sediment. Extensional tectonics, although previously considered the dominant deformation style affecting the rear of the Northern Apennines since the late Miocene, is no longer considered a dominant control on tectono‐sedimentary development of the Valdelsa basin. Instead, the Valdelsa Basin shares features with continental hinterland basins of orogenic belts where compression, extension, and transcurrent stress fields determine a complex spatial and temporal record of accommodation and sediment supply. In the Valdelsa Basin tectonics and eustatic sea‐level fluctuations were dominant in forcing the deposition of sedimentary cycles at several scales. Zanclean and Gelasian large‐scale depositional sequences were mainly controlled by crustal shortening, whereas a eustatic signal was preferentially recorded during the Piacenzian. Smaller scale depositional sequences, common to most synthems, were controlled by orbitally forced glacio‐eustatic cycles. 相似文献
10.
Sericitic alteration at the La Crocetta deposit (Elba Island,Italy): interplay between magmatism,tectonics and hydrothermal activity 总被引：2，自引：0，他引：2
Cinzia?MaineriEmail author Marco?Benvenuti Pilar?Costagliola Andrea?Dini Pierfranco?Lattanzi Giovanni?Ruggieri Igor?M.?Villa 《Mineralium Deposita》2003,38(1):67-86
The La Crocetta mine near Porto Azzurro (Elba Island, Tuscany, Italy) is an important producer of raw material for the ceramic industry. Exploitation focuses on a pervasively sericitized porphyritic aplite of the Tuscan Magmatic Province, locally known as "eurite", which underwent significant potassium enrichment during sericitic alteration. Eurites are located along the hanging wall of the Elba Centrale Fault, a low-angle extensional lineament of regional significance. A later carbonatization stage, apparently associated with high-angle extensional tectonics, locally overprinted the sericitized facies. It is expressed by carbonate ± pyrite ± quartz veins, with adverse effects on ore quality. Sericitization was accompanied by addition of potassium, and loss of Na (± Ca, Fe). Rubidium was not enriched along with potassium during sericitization, contrary to what would be expected for interaction with late-magmatic fluids. New 40Ar–39Ar data from eurites provide an isochron age of about 6.7 Ma for the sericitization, whereas the age of the unaltered protolith is ca. 8.8 Ma. Field evidence indicates the Elba Centrale Fault to be the main channel for the hydrothermal fluids. On the other hand, the involvement of heat and/or fluids contributed by the Porto Azzurro pluton, which crops out in the La Crocetta area, is ruled out by field, geochemical and geochronological data (40Ar–39Ar age of Porto Azzurro =5.9 Ma, i.e. significantly younger than the sericitization event). Fluid inclusion studies suggest that sericitization was associated with a low-temperature (<250 °C) hydrothermal system. Fluids were locally boiling, of variable salinity (4–17 wt% NaCl equiv.), and contained some CO2 (XCO2≤0.027). Their ultimate source is not unequivocally constrained; meteoric and/or magmatic contributions may be possible. Low-salinity (≤2.6 wt% NaCl equiv.), low-temperature (<250 °C) fluids are associated with the late carbonate veining. They are considered to be of dominantly meteoric nature because of their low salinity. In summary, sericitization at La Crocetta is regarded as the product of a detachment fault-related, low temperature hydrothermal system, resulting from the structurally controlled focusing of meteoric and possibly magmatic fluids. Hence, potential targets for exploration for similar resources are represented by aplitic bodies located in the hanging wall of Elba Centrale Fault. Electronic supplementary material to this paper can be obtained by using the Springer LINK server located at http://dx.doi.org/10.1007/s00126-002-0279-2. 相似文献