Hydrated sulphuric acid in dense molecular clouds     

Flavio Scappini  Cesare Cecchi-Pestellini  Harvey Smith  William Klemperer  Alexander Dalgarno 《Monthly notices of the Royal Astronomical Society》2003,341(2):657-661

We consider sulphur depletion in dense molecular clouds, and suggest hydrated sulphuric acid, H₂SO₄ ·  n H₂O, as a component of interstellar dust in icy mantles. We discuss the formation of hydrated sulphuric acid in collapsing clouds and its instability in heated regions in terms of the existing hot core models and observations. We also show that some features of the infrared spectrum of hydrated sulphuric acid have correspondence in the observed spectra of young stellar objects.  相似文献   

A Block-Based Theoretical Model Suited to Gravitational Sliding     

Tinti  Stefano  Bortolucci  Elisabetta  Vannini  Cesare 《Natural Hazards》1997,16(1):1-28

An original theoretical model has been devised to simulate mass flow over hill slopes due to gravitational sliding. The sliding mass is discretized into a sequence of contiguous blocks which are subjected to gravitational forces, to bottom friction and to surface resistance stresses that are generally negligible for subaerial flows, but are relevant for submarine slides. The blocks interact with each other while sliding down the hill flanks because of internal forces that dissipate mechanical energy and produce a momentum exchange between the individual blocks, yet conserving the total momentum of the mass. Internal forces are expressed in terms of interaction coefficients depending on the instantaneous distance between the block centers of mass, which is a measure of the deformation experienced by the blocks: the functional dependence includes three parameters, namely the interaction intensity ¯, the deformability parameter and the shape parameter , by means of which a wide range of interaction types can be fully accounted for. The time integration is performed numerically by solving the equations for the block velocities and positions at any time ti by means of the block accelerations at the previous time t_i-1, and by subsequently updating the block accelerations, which allows to proceed iteratively to the following times. The model has been tested against laboratory results available from literature and by means of several numerical experiments involving a simplified geometry both for the sliding body and the basal surface, with the purpose of clarifying the influence of the model parameters on the slide dynamics. The model improves the performance of the existing kinematic models for slides, moreover preserving an equivalent numerical simplicity. Future applications and possible improvements of this model are suggested.  相似文献   

Response to the comment by V. Neck on “Hydrolysis of neptunium(V) at variable temperatures (10-85 °C)”, Geochimica et Cosmochimica Acta 68, 4821-4830     

Linfeng Rao  Thandankorai G. Srinivasan  PierLuigi Zanonato  Plinio Di Bernardo 《Geochimica et cosmochimica acta》2006,70(17):4556-4562

  相似文献   

Scales of predator detection behavior and escape in Fissurella limbata: A field and laboratory assessment          下载免费PDF全文

Tatiana Manzur  Avia Gonzalez‐Mendez  Bernardo R. Broitman 《Marine Ecology》2018,39(2)

The consumptive effects of predators are widely acknowledged, but predation can also impact prey populations through non‐consumptive effects (NCEs) such as costly antipredator behavioral responses. The magnitude of antipredator behavioral responses by prey is determined by an assessment of risk using sensory cues, which in turn is modulated by the environmental context. We studied the detection behavior and escape response of the keyhole limpet Fissurella limbata from the predatory sea star Heliaster helianthus. Through laboratory and field experimental trials, we quantified the distance and time of predator detection behavior by the prey, and measured their active escape responses when elicited. We found that predator detection by the limpet was chiefly mediated by distance, with experimental individuals capable of detecting predator presence effectively up to distances of at least 50 cm in the field and 70 cm under laboratory conditions. Our results indicate that this prey species is able to evaluate the proximity of its predator and use it as an indication of predation risk; therefore, predator–prey distance appears to be a primary predictor of the magnitude of the antipredator response. Given the tight relationship between predator distance and prey movement and the important role herbivores can play, particularly in this ecosystem, we expect that NCEs will cascade to the patterns of abundance and composition of rocky shore communities through changes in prey foraging behavior under risk.  相似文献   

Reconstructing fluvial bar surfaces from compound cross‐strata and the interpretation of bar accretion direction in large river deposits          下载免费PDF全文

Renato P. Almeida  Bernardo T. Freitas  Bruno B. Turra  Felipe T. Figueiredo  André Marconato  Liliane Janikian 《Sedimentology》2016,63(3):609-628

The interpretation of fluvial styles from the rock record is based for a significant part on the identification of different types of fluvial bars, characterized by the geometric relationship between structures indicative of palaeocurrent and surfaces interpreted as indicative of bar form and bar accretion direction. These surfaces of bar accretion are the boundaries of flood‐related bar increment elements, which are typically less abundant in outcrops than what would be desirable, particularly in large river deposits in which each flood mobilizes large volumes of sediment, causing flood‐increment boundary surfaces to be widely spaced. Cross‐strata set boundaries, on the other hand, are abundant and indirectly reflect the process of unit bar accretion, inclined due to the combined effect of the unit bar surface inclination and the individual bedform climbing angle, in turn controlled by changes in flow structure caused by local bar‐scale morphology. This work presents a new method to deduce the geometry of unit bar surfaces from measured pairs of cross‐strata and cross‐strata set boundaries. The method can be used in the absence of abundant flood‐increment bounding surfaces; the study of real cases shows that, for both downstream and laterally accreting bars, the reconstructed planes are very similar to measured bar increment surfaces.  相似文献   

Resilience and seismic risk perception at school: a geoethical experiment in Aiello Calabro,southern Italy     

De Pascale  Francesco  Bernardo  Marcello  Muto  Francesco  Di Matteo  Dante  Dattilo  Valeria 《Natural Hazards》2016,86(2):569-586

The last few years have seen the debate on the geoethics of environmental and climatic protection growing to include resilience as a central idea within this new discipline, which holds many similarities with geography. Resilience analysis often looks at the capacity to re-establish conditions of equilibrium within a system which has been hit by a serious shock, e.g. a natural or man-made disaster. Geoethics works, in tandem with geological analyses and the geography of risk, to inform a population and develop integrated risk management in such a way as to strengthen a community’s resilience. The aim of this work is to study some people’s capacity to overcome what was potentially a disastrous event and, through a process of reconstruction, turn it into an occasion for growth. The experiment, carried out in the primary and middle schools in Aiello Calabro (Calabria, southern Italy), was conducted on the basis of the belief that there is a close relationship between a population’s having a realistic understanding of the risk of such an event, e.g. an earthquake, and high levels of resilience. We also tried to gain an insight into the relationship that may exist between resilience in primary and secondary school children and methods of coping which give an appropriate management of seismic risk. To be more precise, we try to discover whether there is a link between good/appropriate resilience and good/appropriate risk management.

  相似文献   

The influence of physical and biological processes on the ichthyoplankton communities in the Gulf of Sirte (Southern Mediterranean Sea)          下载免费PDF全文

Angela Cuttitta  Sergio Bonomo  Salem Zgozi  Angelo Bonanno  Bernardo Patti  Enza Maria Quinci  Marco Torri  Mohamed Hamza  Abdul Fatah  Daw Haddoud  Akram El Turki  Abdul Bari Ramadan  Simona Genovese  Salvatore Mazzola 《Marine Ecology》2016,37(4):831-844

This paper reports on the first study on the ichthyoplankton community structure in the Gulf of Sirte and its spatial distribution in relation to environmental conditions and zooplankton abundance. The results make an important contribution to the future management of fisheries in this unexplored, but much exploited, area. Biological samples were collected in July 2008 using a Bongo40 net. In total, 1914 larvae were found and 1652 of these were identified. In particular, bathypelagic taxa were the most abundant, followed by demersal, mesopelagic, pelagic and epipelagic taxa. The ichthyoplankton community had a patchwork distribution influenced by oligotrophic conditions, the bottom depth and oceanographical features. The results suggest that environmental forcings were able to transport the ichthyoplankton to productive areas. Indeed, maximum fish egg densities were found in coastal stations in correspondence with the Atlantic Tunisian Current inflow, whereas larvae were mainly concentrated in the east side of the Gulf, probably as a result of advection by the anticyclonic circulation. Additionally, the distribution patterns of the total larvae density and the different assemblages were well matched with the abundance of the zooplankton, probably determining final larval survival, growth and recruitment.  相似文献   

Morphology and geological setting of Iseo Lake (Lombardy) through multibeam bathymetry and high-resolution seismic profiles     

Alfredo Bini  Daniele Corbari  Paolo Falletti  Mauro Fassina  Cesare R. Perotti  Andrea Piccin 《Swiss Journal of Geoscience》2007,100(1):23-40

  相似文献   

The Moon as a piece of Mercury     

Cesare Emiliani 《International Journal of Earth Sciences》1992,81(3):791-794

The giant impact on Earth proposed by some to generate the Moon could not have happened because the amount of carbonate rock and organic carbon present on Earth closely approximates the amount of CO₂ predicted for the Earth's early atmosphere by comparison with the present atmosphere of Venus. It is suggested that the Moon may have fissioned from Mercury more than 4.4 billion years ago and may have been captured by the Earth no later than 3.2 billion years ago.A model for the origin of the Earth-Moon system that has been gaining favor recently visualizes a Marssize body impacting Earth and excavating enough material from the Earth to form the Moon (Newsome &Taylor, 1989). This giant impact not only would have sterilized the planet (Maher &Stevenson, 1988), obliterating any form of life that might have existed at the time, but also would have blown off the Earth's atmosphere (Kaula, 1990). As the story goes, Venus suffered no giant impact and conserved its CO₂ atmosphere, whereas the loss of her CO₂ atmosphere cooled the Earth's surface allowing the oceans to rain out (Kaula, 1990). It is widely believed that the different histories in the early evolution of their atmospheres set markedly different courses for the subsequent evolution of the two planets. I agree with this conclusion but disagree with the cause for the difference.If the giant impact really happened, it must have taken place not only after the Earth's accumulation was practically completed but also after a substantial core had formed (to account for the lesser density of the Moon).Venus has approximately 89 kg/cm² of CO₂ for a total of 4.110²⁰kg. The Earth with a mass 1.226 greater than Venus, should have had 5.010²⁰ kg of CO₂. If entirely precipitated as carbonate, the Earth should now have 1.110²¹ kg of carbonate. A recent estimate (Hay, 1985) gives the total volume of carbonate rock on Earth as 276.110⁶ km³ which, for an average density of 2.83, corresponds to a mass of 7.810²⁰ kg. This figure and the ratio limestone/shale/sandstone of 15/74/11 (Garrels &Mackenzie, 1971) leads to the carbonate inventory shown in Table 1.  相似文献   

Gas-liquid phase transitions and critical point in hot white dwarf matter     

L. De Cesare  A. Forlani  G. Platania 《Astrophysics and Space Science》1973,21(2):461-474

We consider the gas-liquid first-order phase transitions and prove the existence of the critical point in white dwarf matter. The latent heat released in the liquefaction processes can be used in the interpretation of the spreading of the white dwarf sequence in H-R diagram. Some thermodynamic quantities, e.g., the saturation pressure, the latent heat, etc., are calculated along the gas-liquid coexistence curve, and their behaviour near critical point are studied.  相似文献