Decadal Climatic Anomalies in the Northern Adriatic Sea Inferred from a New Oceanographic Data Set   总被引：1，自引：0，他引：1  

Aniello Russo  Sandro Rabitti  Mauro Bastianini 《Marine Ecology》2002,23(S1):340-351

Abstract. In 1997, Artegiani et al. depicted for the first time the seasonal climatology of the Adriatic Sea; they used the ATOS data set, formed by 5540 oceanographic stations sampled over this continental basin from 1911 to 1980. Lately, two Italian institutes working on the Adriatic Sea for long time, IBM and IRPEM, merged their recent data sets for the northernmost part of the basin. This yielded 3600 new oceanographic stations, concentrated in an area where 809 ATOS stations were located. The new data were quality checked, and then a seasonal climatology was drawn up as a first analysis step. The new climatology differed significantly from the ATOS results; this could be explained, at least partially, by the climatic changes that have occurred on this area. For example, air temperature increased significantly over northern Italy starting from 1988. Variations of the observed air temperature and Po River runoff qualitatively agree with sea surface temperature and salinity variations. A preliminary computation of heat fluxes based on ECMWF reanalysis confirms an increased heat flux to the Northern Adriatic Sea starting from 1988.  相似文献   

Macrofauna Associated With Sponge Species of Different Morphology     

A. Koukouras  A. Russo  E. Voultsiadou-Koukoura  C. Arvanitidis  D. Stefanidou 《Marine Ecology》1996,17(4):569-582

Abstract. The macrofaunas associated with the three morphologically different North Aegean Sea sponge species Agelas oroides, Aplysina aerophoba , and Axinella cannabina were compared. The faunal abundance was not related to sponge surface area for any of the three species. Each sponge species supported a significantly different number of individuals per unit canal volume; A. aerophoba supported the most, A. oroides the least. A. aerophoba supported the highest species richness, A. cannabina the lowest. Canal volume was a good predictor of associated faunal abundance and species richness for two of the three sponge species. Faunal abundance was also directly related to sponge mean canal diameter. The species composition of associated fauna was similar on A. aerophoba and A. oroides and significantly different on A. cannabina .  相似文献   

Midlittoral Soft Substratum Macrofaunal Assemblages in the North Aegean Sea   总被引：1，自引：0，他引：1  

Athanasios  Koukouras Anthony  Russo 《Marine Ecology》1991,12(4):293-316

Abstract. The soft substratum macrobenthic assemblages of the midlittoral zone, along the atidal shores of the upper Thermaikos (polluted) and Strymonikos (unpolluted) Gulfs in the North Aegean Sea, arc qualitatively and quantitatively described. The composition of each of the seven assemblages found (four in Thermaikos and three in Strymonikos Gulf) is statistically tested and discussed in relation to abiotic factors. One of the four Thermaikos Gulf assemblages is located on a silt to fine sand substrate in brackish waters and is characterized by the dominance of the polychactc Hedisie diversicolor and the amphipod Corophium orientate. The other three assemblages arc located on coarse substrates and characterized by the very high dominance of the bivalve Donacillu corneu and the polychactc Ophelia bicornis (both of which are exclusive inhabitants of the midlittoral zone); the First is additionally characterized by the very high dominance of the polychactc Nerine cirratulus , both the second and the third by the dominance of turbellarians due to the pollution of the Gulf (stations located near sewage discharge, high organic carbon, low oxygen). In Strymonikos Gulf, one of the three assemblages is dominated by H. diversicolor and C. orientate; it is similar to the corresponding assemblage found in Thermaikos Gulf, although located on a relatively coarSér sediment. The second is dominated by D. cornea and O. bicornis and is also similar to that of Thermaikos Gulf. The third assemblage does not have a corresponding one in Thermaikos Gulf, is located on a substrate consisting of granules to pebbles, arid is characterized by the high dominance of the amphipods Allorchestes aquilinus and Echinogammarus olivii and the isopod Sphaeroma Sérratum. The corresponding assemblages of the two gulfs are compared. The results of the data analysis are discussed and compared with the literature.  相似文献   

UU CNC and VZ PSC,contact systems before the common envelope phase?     

F. Barone  L. Milano  G. Russo  M. J. Sarna 《Astrophysics and Space Science》1989,159(1):67-83

We have analyzed the existing photoelectric light curves of twoK-type binary systems: UU Cnc, with a period of about 100 days, and VZ Psc, with a period of about 6 hours. Both show a large overcontact (38% for UU Cnc, 56% for VZ Psc) and a large temperature difference between components (T1500 K and 1100 K, respectively). In the case of VZ Psc, the variability is due only to the non-spherical shape, i.e., no eclipse occurs, but the determination of the photometric solution is made possible by the existence of a spectroscopic mass ratio. We find that UU Cnc is now probably undergoing Case C mass transfer in a dynamical time-scale, with the mass ratio reversal having already occurred; the system is in contact, and is likely to evolve to a 100% filling factor, that is the so-called pre-common envelope phase, a unique case never observed before. The situation for VZ Psc is more uncertain, but a similar, although not identical, possibility exists.Associated with the Istituto Nazionale Fisica Nucleare, Italy.On leave from N. Copernicus Astronomical Center, Polish Academy of Sciences, Warsaw, Poland.  相似文献   

An XMM-Newton proton response matrix     

Teresa Mineo  Simone Lotti  Silvano Molendi  Simona Ghizzardi 《Experimental Astronomy》2017,44(3):287-296

Soft protons constitute an important source of background in focusing X-ray telescopes, as Chandra and XMM-Newton experience has shown. The optics in fact transmit them to the focal plane with efficiency similar to the X-ray photon one. This effect is a good opportunity to study the environment of the Earth magnetosphere crossed by the X-ray satellite orbits, provided that we can link the spectra detected by the instruments with the ones impacting on the optics. For X-ray photons this link has the form of the so-called response matrix that includes the optics effective area and the energy redistribution in the detectors. Here we present a first attempt to produce a proton response matrix exploiting ray-tracing and GEANT4 simulations with the final aim to be able to analyse XMM-Newton soft proton data and link them to the external environment. If the procedure is found to be reliable, it can be applied to any future X-ray missions to predict the soft particles spectra impacting on the focal plane instruments.  相似文献   

Subsidence due to crack closure and depressurization of hydrothermal systems: a case study from Mt Epomeo (Ischia Island,Italy)     

Vincenzo Sepe  Simone Atzori  Guido Ventura 《地学学报》2007,19(2):127-132

Levelling surveys carried out between 1990 and 2003 on the Mt Epomeo resurgent block (Ischia Island) record negative dislocations on its northern and southern flanks with a maximum subsidence rate of 1.27 cm yr⁻¹. This deformation is not associated with the cooling, crystallization or lateral drainage of magma and cannot be explained by a pressure point or prolate ellipsoid source. Results from dislocation models and the available structural and geochemical information indicate that the subsidence is due to crack closure processes along two main ENE–WSW and E–W preexisting faults, which represent the preferred pathway of CO₂ degassing from the hydrothermal system located beneath Mt Epomeo. The monitoring of the dislocations and CO₂ flux along these faults could give useful information on the dynamics of the hydrothermal system.  相似文献   

Near-infrared light curve of Comet 9P/Tempel 1 during Deep Impact     

Y.R. Fernández  C.M. Lisse  N. Dello Russo  C.E. Woodward 《Icarus》2007,187(1):220-227

On UT 2005 July 4 we observed Comet 9P/Tempel 1 during its encounter with the Deep Impact flyby spacecraft and impactor. Using the SpeX near-infrared spectrograph mounted on NASA's Infrared Telescope Facility, we obtained 0.8-to-2.5 μm flux-calibrated spectral light curves of the comet for 12 min before and 14 min after impact. Our cadence was just 1.1 s. The light curve shows constant flux before the impact and an overall brightening trend after the impact, but not at a constant rate. Within a 0.8-arcsec-radius circular aperture, the comet rapidly-brightened by 0.63 mag at 1.2 μm in the first minute. Thereafter, brightening was more modest, averaging about 0.091 mag/min at 1.2 μm, although apparently not quite constant. In addition we see a bluing in the spectrum over the post-impact period of about 0.07 mag in J-H and 0.35 mag in J-K. The majority of this bluing happened in the first minute, and the dust only marginally blued after that, in stark contrast to the continued brightening. The photometric behavior in the light curve is due to a combination of crater formation effects, expansion of the ejecta cloud, and evolution of liberated dust grains. The bluing is likely due to an icy component on those grains, and the icy grains would have had to have a devolatilization timescale longer than 14 min (unless they were shielded by the optical depth of the cloud). The bluing could also have been caused by the decrease in the “typical” size of the dust grains after impact. Ejecta dominated by submicron grains, as inferred from other observations, would have stronger scattering at shorter wavelengths than the much larger grains observed before impact.  相似文献   

Hydrogeological and thermal characterization of shallow aquifers in the plain sector of Piemonte region (NW Italy): implications for groundwater heat pumps diffusion     

Stefano Lo Russo  Massimo Vincenzo Civita 《Environmental Earth Sciences》2010,60(4):703-713

The low annual and seasonal variability of the shallow groundwater temperature in the alluvial plain aquifers of the Piemonte region (NW Italy) confirmed the potentiality of the low-enthalpy open-loop groundwater heat pumps (GWHP) diffusion to contribute to the reduction of regional greenhouse gas emissions. The distribution of mean groundwater temperatures ranged from a minimum of 10.3°C to a maximum of 17.9°C with a mean of 14.0°C. Differences among diverse areas were slight according with the modest variations in the general climatic condition. Like the air, temperature distribution of the shallow groundwater temperatures is generally similar to topographic elevations in reverse manner. Higher temperature values recorded were typical of summer months (June, July). On the opposite lower values were measured in January and February. No significant difference phase (time) difference between air and groundwater temperature appeared in the data analysis. Besides air-temperature influence (seasonal variability) seemed strictly connected to the depth to groundwater in the measure point and it was negligible when the value was over 9.5 m. For the application of the open-loop systems, extensive examinations of the hydrogeological local conditions should be conducted at site scale and groundwater heat transport modelling should be developed.  相似文献   

Diagenesis of the Khuff Formation (Permian–Triassic), northern United Arab Emirates     

Simone Fontana  Fadi H. Nader  Sadoon Morad  Andrea Ceriani  Ihsan S. Al-Aasm 《Arabian Journal of Geosciences》2010,3(4):351-368

This diagenetic study (including fieldwork, petrographic, fluid inclusion, and stable isotope investigations) deals with the outcrop of Upper Permian–Lower Triassic carbonate rocks, which are equivalent to the Khuff Formation. The studied succession, which outcrops in the Ras Al Khaimah region, northern United Arab Emirates, comprises three formations, including the Bih, the Hagil, and the Ghail formations. The study focuses on unraveling the conditions and fluid compositions encountered during diagenesis of the succession. Emphasize is also made on linking diagenesis to major stratigraphic surfaces and to highlight reservoir property evolution and heterogeneity of the studied rocks. The evolution of fluids and related diagenetic products can be summarized as follows: (1) formation of near-surface to shallow burial, fine-crystalline dolomite (dolomite matrix) through pervasive dolomitization of carbonate sediments by modified marine pore waters; (2) formation of coarse-crystalline dolomite cement by highly evolved marine pore waters (13–23 wt.% NaCl eq.) at elevated temperatures (120–208°C), and (3) calcite cementation by highly saline fluid (20–23 wt.% NaCl eq.) at high temperature (170–212°C). A final calcite cement generation has been formed by the percolation of meteoric fluids during uplift. Fracture- and vug-filling diagenetic minerals are mainly restricted to the mid-Bih breccia marker level, suggesting preferential focused fluid flow through specific stratigraphic surfaces as well as along tectonic-related structures. Reservoir properties have been evolved as result of the interplay of the original sedimentary texture and the diagenetic evolution. Porosity is higher in the Bih Formation, which is dominated by dolomitized packstones and grainstones, than in the Hagil and Ghail formations, consisting mainly of dolomitized mudstones and wackestones. Image analyses were used to quantify the visual porosity in thin sections. The highest porosity values were measured in the Bih Formation, which is characterized by significant amounts of vug- and fracture-filling cements. This feature is attributed to the increase of porosity owing to substantial dissolution of abundant intergranular and vug-filling cements. In contrast, the Hagil and Ghail formations, which consist of finer-grained rock than the Bih Formation, were less cemented, and thus, the porosity enhancement by cement dissolution was insignificant.  相似文献   

An integrated evaluation of thirteen modelling solutions for the generation of hourly values of air relative humidity     

Simone Bregaglio  Marcello Donatelli  Roberto Confalonieri  Marco Acutis  Simone Orlandini 《Theoretical and Applied Climatology》2010,102(3-4):429-438

The availability of hourly air relative humidity (HARH) data is a key requirement for the estimation of epidemic dynamics of plant fungal pathogens, in particular for the simulation of both the germination of the spores and the infection process. Most of the existing epidemic forecasting models require these data as input directly or indirectly, in the latter case for the estimation of leaf wetness duration. In many cases, HARH must be generated because it is not available in historical series and when there is the need to simulate epidemics either on a wide scale or with different climate scenarios. Thirteen modelling solutions (MS) for the generation of this variable were evaluated, with different input requirements and alternative approaches, on a large dataset including several sites and years. A composite indicator was developed using fuzzy logic to compare and to evaluate the performances of the models. The indicator consists of four modules: Accuracy, Correlation, Pattern and Robustness. Results showed that when available, daily maximum and minimum air relative humidity data substantially improved the estimation of HARH. When such data are not available, the choice of the MS is crucial, given the difference in predicting skills obtained during the analysis, which allowed a clear detection of the best performing MS. This study represents the first step of the creation of a robust modelling chain coupling the MS for the generation of HARH and disease forecasting models, including the systematic validation of each step of the simulation.  相似文献