Factors controlling the vegetation distribution and coal‐forming environments in a strike‐slip basin. The Pennsylvanian Peñarroya‐Belmez‐Espiel Basin,southern Spain          下载免费PDF全文

Felipe González  Carmen Moreno  Erica Lorenzo  Gonzalo Márquez 《地学学报》2016,28(3):171-180

Coal‐forming environments require humid to perhumid conditions. Tectonics governs the size, location and availability of coal seams developed in such environments. While large Pennsylvanian paralic basins generated thick and continuous coal seams, many other small coeval basins, which were tectonically active, developed a puzzling succession, with carbonaceous deposits that varied in size, thickness and the nature of the coal‐forming flora. This study, conducted in the Peñarroya‐Belmez‐Espiel coalfield, a Variscan strike‐slip basin in the south of Spain, provides insights into this subject. The coal seams analysed, generated in different depositional environments, have quantitatively different palynological assemblages. Lacustrine coals are dominated by lycopsids; distal alluvial plain/marginal lacustrine coals are dominated by sphenophytes and tree ferns, and middle alluvial fan coals are dominated by sphenophytes, tree ferns and lycopsids. This means that when conditions were favourable for peat accumulation, peat accumulated regardless of the nature of the available flora.  相似文献   

Short-term response of the slow growing seagrass Posidonia oceanica to simulated anchor impact     

Ceccherelli G  Campo D  Milazzo M 《Marine environmental research》2007,63(4):341-349

Experimental evaluations about the impact of anchors of small vessels have previously shown that each anchoring can on average damage up to six shoots of Posidonia oceanica, removing small amount of biomass and, at the same time, interrupting continuity among shoots. The aim of the paper was to investigate the response of P. oceanica to different damage intensity at two levels of substrata compactness. Three treatments were considered: control (no damage); low damage (simulated anchor damage by three strokes of a hoe); and high damage (six strokes). Disturbance was higher where the substratum was highly penetrable and after one year significant variation was observed among treatments for both the number of leaves per shoot and shoot density. Conversely, the number of leaves per shoot by the end of the study was similar among all treatment combinations, suggesting that this was the only phenological feature that recovered, and probably the only result that through clonal integration could be achieved. These data strongly highlighted the role that anchoring might have on the slow growing seagrass P. oceanica meadow.  相似文献   

The post-Newtonian mean anomaly advance as further post-Keplerian parameter in pulsar binary systems     

Lorenzo Iorio 《Astrophysics and Space Science》2007,312(3-4):331-335

The post-Newtonian gravitoelectric secular rate of the mean anomaly ℳ is worked out for a two-body system in the framework of the General Theory of Relativity. The possibility of using such an effect, which is different from the well known decrease of the orbital period due to gravitational wave emission, as a further post-Keplerian parameter in binary systems including at least one pulsar is examined. The resulting effect is almost three times larger than the periastron advance . E.g., for the recently discovered double pulsar system PSR J0737-3039 A+B it would amount to −47.79 deg yr⁻¹. This implies that it could be extracted from the linear part of a quadratic fit of the orbital phase because the uncertainties both in the linear drift due to the mean motion and in the quadratic shift due to the gravitational wave are smaller. The availability of such additional post-Keplerian parameter would be helpful in further constraining the General Theory of Relativity, especially for such systems in which some of the other post-Keplerian parameters can be measured with limited accuracy. Moreover, also certain pulsar-white dwarf binary systems, characterized by circular orbits like PSR B1855+09 and a limited number of measured post-Keplerian parameters, could be used for constraining competing theories of gravity.  相似文献   

The effect of the "Prestige" oil spill on the plankton of the N-NW Spanish coast     

Varela M  Bode A  Lorenzo J  Alvarez-Ossorio MT  Miranda A  Patrocinio T  Anadón R  Viesca L  Rodríguez N  Valdés L  Cabal J  Urrutia A  García-Soto C  Rodríguez M  Alvarez-Salgado XA  Groom S 《Marine pollution bulletin》2006,53(5-7):272-286

Chlorophyll, primary production, zooplankton biomass and the species composition of phytoplankton and zooplankton were studied in 2003, after the Prestige shipwreck. The information obtained was compared to previous data series available for the area affected by the spill. A large data series on plankton variables for the N-NW Spanish coast existed, and therefore a realistic evaluation of the effects by comparison with the range of natural variability could be carried out. We emphasized the evaluation of impact during the spring bloom, the first important biological event after the spill. Some minor changes were observed occasionally, but they did not show any clear pattern and were more related to the natural variability of the ecosystem than to effect of the spill. Plankton community structure did not undergo any changes. Only a few species were more abundant during spring 2003 than in previous years. No significant changes were detected in the planktonic community during productive periods, such as the spring bloom and the summer blooms related to intrusions of East North Atlantic Central Waters. The lack of evidence of the effects of the spill on planktonic communities is discussed in terms of the characteristics of the fuel, the high dynamics of the water masses, the biological mechanisms through which the fuel from the surface waters is transferred to the sea floor and, particularly, the influence of the natural variability by means of large and meso-scale hydrographic processes in the area under study. At the present time it is not possible to determine any minor effects the spill may have had on the plankton owing to the great variability of the planktonic cycles and the short-term impact of the oil from the Prestige on the pelagic system.  相似文献   

Uncertainty and risk in climate projections for the 21st century: comparing mitigation to non-intervention scenarios     

Lorenzo Tomassini  Reto Knutti  Gian-Kasper Plattner  Detlef P. van Vuuren  Thomas F. Stocker  Richard B. Howarth  Mark E. Borsuk 《Climatic change》2010,103(3-4):399-422

Probabilistic climate projections based on two SRES scenarios, an IMAGE reference scenario and five IMAGE mitigation scenarios (all of them multi-gas scenarios) using the Bern2.5D climate model are calculated. Probability distributions of climate model parameters that are constrained by observations are employed as input for the climate model. The sensitivity of the resulting distributions with respect to prior assumptions on climate sensitivity is then assessed. Due to system inertia, prior assumptions on climate sensitivity play a minor role in the case of temperature projections for the first half of the 21st century, but these assumptions have a considerable influence on the distributions of the projected temperature increase in the year 2100. Upper and lower probabilities for exceeding 2°C by the year 2100 are calculated for the different scenarios. Only the most stringent mitigation measures lead to low probabilities for exceeding the 2°C threshold. This finding is robust with respect to our prior assumptions on climate sensitivity. Further, probability distributions of total present-value damages over the period 2000–2100 for the different scenarios are calculated assuming a wide range of damage cost functions, and the sensitivity of these distributions with respect to the assumed discount rate is investigated. Absolute values of damage costs depend heavily on the chosen damage cost function and discount rate. Nevertheless, some robust conclusions are possible.  相似文献   

Coral Patch and Ormonde seamounts as a product of the Madeira hotspot,Eastern Atlantic Ocean     

Filippo D'Oriano  Lorenzo Angeletti  Lucilla Capotondi  Marinella A. Laurenzi  Matthias López Correa  Marco Taviani  Luigi Torelli  Teresa Trua  Luigi Vigliotti  Nevio Zitellini 《地学学报》2010,22(6):494-500

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The free oscillations of the Ligurian Sea computed by the H-N method     

Lorenzo Papa 《Ocean Dynamics》1977,30(3):81-90

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Applicazione della teoria di Chandrasekhar alle misure di polarizzazione atmosferica     

Dr. Lorenzo Casertano 《Pure and Applied Geophysics》1955,30(1):170-178

Riassunto E'stato calcolato il valore medio dello spessore ottico dell'atmosfera () in funzione degli elementi meteorologici al suolo, riconoscendo che esso può ritenersi praticamente indipendente da questi. Poichè i valori delle intensità delle radiazioni diffuse dall'atmosfera, ricavati dalla teoria delChandrasekhar, sono, per una data altezza del sole e per ogni direzione della visuale, funzioni soltanto di e dell'albedo, si deduce che queste intensità risultano indipendenti dalle condizioni meteorologiche. Il che porta a concludere che: 1^o) o effettivamente le intensità della luce diffusa dalle molecole d'aria non dipendono dai fattori meteorologici; 2^o) oppure la teoria delChandrasekhar, completa per quel che riguarda le diffusioni multiple, non risponde in pieno alle condizioni reali. — Il confronto delle curve teoriche della polarizzazione della luce-diffusa dalla volta celeste con quelle ottenute in base ad osservazioni eseguite all'Osservatorio Vesuviano, non dà un accordo accettabile. Pur non escludendo che il mancato accordo sia da attribuire, almeno in parte, alla diffusione non molecolare, si è portati verso la seconda alternativa.

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Summary The average optical atmospheric thickness () as a function of the meteorologic ground elements has been calculated, obtaining a result which shows its inependence from those elements. The intensity of the radiations scattered by the atmosphere, as deduced fromChandrasekhar's theory for a given hight of the suns and for every direction, being a function only of and of the albedo, it follows that these intensities are independent from the meteorologic conditions. Then it can be concluded that: 1st) either the intensity of the light scattered by the air molecules does not depend from the meteorologic factors, 2nd) orChandrasekhar's theory, adequate for the computation of the effect of multiple scattering, does not entirely represents the real phenomenon. — Comparing the theoretic patterns for the polarization of sky scattered light with the experimental data obtained in the Vesuvian Observatory, an acceptable agreement has not be found. Although taking into account the scattering of other than molecular origin, the second hypothesis seems more probable.

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Estimation of debris‐flow magnitude in the Eastern Italian Alps     

Lorenzo Marchi  Vincenzo D'Agostino 《地球表面变化过程与地形》2004,29(2):207-220

The estimation of debris‐?ow magnitude is an essential step in the assessment of debris‐?ow hazard. Although different methods have been developed for the assessment of debris‐?ow magnitude, this is still a dif?cult task because of the complexity of ?ow processes and the lack of data to test estimation procedures in many mountainous regions. Data on debris‐?ow magnitude from 127 basins in the Eastern Italian Alps have been collected from scienti?c and technical journals, technical reports, historical documents gathered from local archives, and ?eld surveys. These data were used to develop and test different predictive approaches, encompassing regression equations, geomorphological surveys and probabilistic analysis of time series. Regression techniques were used to correlate debris‐?ow magnitude to morphometric parameters and geological characteristics of the basins. Values of the channel debris yield rate (contribution per unit length of channel), proposed in the literature, were compared with data from the study area for identifying reference values for channel stretches of different morphological characteristics. Although limited to the few basins in which suf?cient data were available, the probabilistic analysis of time series of debris‐?ow magnitude provides indications about the relations between magnitude and frequency of debris ?ows. Some observations about the capability and drawbacks of considered methods are presented and the combined use of different approaches for the estimation of debris‐?ow magnitude is suggested. Copyright © 2004 John Wiley & Sons, Ltd.  相似文献   

Modelling the heat pulses generated on a fault plane during coseismic slip: Inferences from the pseudotachylites of the Copanello cliffs (Calabria, Italy)   总被引：1，自引：0，他引：1  

A. Caggianelli  S. de Lorenzo  G. Prosser 《Tectonophysics》2005,405(1-4):99-119

A pseudotachylite vein network crosscutting late Hercynian foliated tonalites can be observed along the Copanello cliffs (Calabria, Southern Italy). Pseudotachylites formed during the Oligocene–Miocene at intermediate crustal levels (ca. 10 km). They show variable thickness ranging from few mm up to 10 cm, as observed in injection veins branching from the fault plane. Microscopic observations indicate that pseudotachylite matrix mainly consists of plagioclase (An₄₆–An₅₈) and biotite microlites. Rounded clasts of quartz, plagioclase or of plagioclase–quartz lithic fragments are disseminated in the matrix. Intergranular, flow and spherulitic textures are commonly observed. Microstructural features are consistent with rapid crystallisation from melt. EDS analyses of rare and tiny glass veins indicated a trachyandesite or An₅₀ plagioclase melt composition.The conditions for pseudotachylite formation were reproduced by an analytical model taking into account the heat released by friction along a horizontal fault plane during a seismic event. The model is based on a three-stage rupture history that includes nucleation, propagation and stopping. In addition, by means of a numerical approach, the model reproduces cooling that follows the stopping stage.According to previous studies, the thermal perturbation induced by fault displacement is very intense. In fact, temperatures exceeding the tonalite and even An₅₀ plagioclase liquidus (1470 °C) are reproduced by small amount of slip (≤ 6 cm) in suprahydrostatic regime. On the other hand, the thermal perturbation is strongly localised and of short duration. Peak temperatures abruptly decrease at a short distance from the fault plane (typically in few millimetres). In these conditions a thin film of melt can be produced. Therefore, the presence of cm-scale pseudotachylite veins can be only explained assuming an efficient and fast melt migration towards dilatant sites, such as pull-apart structures and injections veins. Results of the model may be useful to predict the thermal disturbance produced by earthquakes of low intensity.  相似文献