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91.
Alireza Hassanzadegan Guido Blöcher Harald Milsch Luca Urpi Günter Zimmermann 《Rock Mechanics and Rock Engineering》2014,47(2):421-434
A porosity change influences the transport properties and the elastic moduli of rock while circulating water in a geothermal reservoir. The static and dynamic elastic moduli can be derived from the slope of stress–strain curves and velocity measurements, respectively. Consequently, the acoustic velocities were measured while performing hydrostatic drained tests. The effect of temperature on static and dynamic elastic moduli and porosity variations of Flechtinger sandstone was investigated in a wide range of confining pressure from 2 to 55 MPa. The experiments were carried out in a conventional triaxial system whereas the pore pressure remained constant, confining pressure was cycled, and temperature was increased step wise (25, 60, 90, 120, and 140 °C). The porosity variation was calculated by employing two different theories: poroelasticity and crack closure. The porosity variation and crack porosity were determined by the first derivative of stress–strain curves and the integral of the second derivative of stress–strain curves, respectively. The crack porosity analysis confirms the creation of new cracks at high temperatures. The porosity variation was increasing with an increase in temperature at low effective pressures and was decreasing with a rise in temperature at high effective pressures. Both compressional and shear wave velocities were increasing with increasing pressure due to progressive crack closure. Furthermore, the thermomechanical behavior of Flechtinger sandstone was characterized by an inversion effect where the sign of the temperature derivative of the drained bulk modulus changes. 相似文献
92.
In north-eastern Greece the mid-greenschist facies Makri Unit and the anchizonal Melia Formation belong to the eastern Circum-Rhodope Belt that forms the uppermost tectonostratigraphic unit of the Rhodope metamorphic nappe pile. The two metasedimentary successions had different source areas, although they now lie in close proximity in the Rhodope Massif. The U-Pb isotopic ages of detrital zircons from a metasandstone of the Makri Unit analysed using LA-SF-ICP-MS and SHRIMP-II gave age clusters at ca. 310-290 Ma and at ca. 240 Ma for magmatic zircons, which may have been derived from Carboniferous-Permian basement rocks of the Thracia Terrane (Lower Tectonic Unit of the Rhodope Massif) that subsequently underwent Triassic rifting. The youngest detrital zircon grains found so far indicate that the metasedimentary succession of the Makri Unit, or at least parts of it, cannot be older than Late Triassic. By contrast, clastic sedimentary rocks of the Melia Formation contain the primary detrital mineral assemblage of epidote, zoisite, garnet, and phengitic mica, which is absent in the Makri Unit, and clearly points to metamorphic rocks being the major source for these sediments. U-Pb analyses of detrital zircons gave a prominent age cluster at ca. 315-285 Ma for magmatic zircons. Inherited cores indicate the involvement of Pan-African and Late Ordovician-Early Silurian crustal sources during Late Carboniferous-Early Permian igneous event(s). Moreover, U-Pb detrital zircon geochronology indicates that the Melia Formation cannot be older than latest Middle Jurassic. We suggest that the Melia Formation was deposited in front of a metamorphic nappe pile with Rhodopean affinities in Tithonian or Cretaceous times. Both the Makri Unit and the Melia Formation have been tectonically juxtaposed from different sources to their present location during Balkan and Alpine orogenic processes. 相似文献
93.
Full-scale Modelling of Falling Rock Protection Barriers 总被引:1,自引:0,他引:1
Full-scale impact tests, carried out to evaluate the behaviour of flexible falling rock protection barriers, are described
and relevant results presented and discussed. Falling rock protection barriers, which may be numbered among passive measures
against rockfall, are designed to intercept and stop falling rocks by dissipation of impact energies through the elasto-plastic
deformation of a system made up of metallic nets and supporting and connecting components. The testing programme involved
models of barriers subjected to the impact of free-falling blocks of kinetic energy ranging from 500 to 5,000 kJ. The experimental
test site, set-up in Fonzaso (Italy), and the experimental procedure were developed according to the new European testing
standards (ETAG 027) on falling rock protection kits. The paper is aimed at presenting an extensive and high quality database,
which can be extremely useful for a better understanding of the actual response of such structures and for any subsequent
analytical and numerical modelling. 相似文献
94.
Theodor Kostiuk Tilak Hewagama Kelly E. Fast John Annen Guido Sonnabend Juan D. Delgado Richard Achterberg 《Planetary and Space Science》2010,58(13):1715-1723
The Cassini Huygens mission provides a unique opportunity to combine ground-based and spacecraft investigations to increase our understanding of chemical and dynamical processes in Titan’s atmosphere. Spectroscopic measurements from both vantage points enable retrieving global wind structure, temperature structure, and atmospheric composition. An updated analysis of Titan data obtained with the NASA Goddard Space Flight Center’s Infrared Heterodyne Spectrometer (IRHS) and Heterodyne Instrument for Planetary Wind and Composition (HIPWAC) prior to and during the Cassini Huygens mission is compared to retrievals from measurements with the Cassini Composite Infrared Spectrometer (CIRS). IRHS/HIPWAC results include the first direct stratospheric wind measurements on Titan, constraints on stratospheric temperature, and the study of atmospheric molecular composition. These results are compared to CIRS retrievals of wind and temperature profile from thermal mapping data and ethane abundance at 10-15° South latitude, near the equatorial region. IRHS/HIPWAC wind results are combined with other direct techniques, stellar occultation measurements, and CIRS results to explore seasonal variability over nearly one Titan year and to provide an empirical altitude profile of stratospheric winds, varying from ∼50 to 210 m/s prograde. The advantage of fully resolved line spectra in species abundance measurements is illustrated by comparing the possible effect on retrieved ethane abundance by blended spectral features of other molecular constituents, e.g., acetylene (C2H2), ethylene (C2H4), allene (C3H4), and propane (C3H8), which overlap the ν9 band of ethane, and are not resolved at lower spectral resolution. IR heterodyne spectral resolution can discriminate weak spectral features that overlap the ν9 band of ethane, enabling ethane lines alone to be used to retrieve abundance. Titan’s stratospheric mean ethane mole fraction (8.6±3 ppmv) retrieved from IRHS/HIPWAC emission line profiles (resolving power λ?Δλ∼106) is compared to past values obtained from lower resolution spectra and from CIRS measurements (resolving power λ?Δλ∼2×103) and more compatible recent analysis. Results illustrate how high spectral resolution ground-based studies complement the spectral and spatial coverage and resolution of moderate spectral resolution space-borne spectrometers. 相似文献
95.
A simple numerical procedure for timely prediction of precipitation-induced landslides in unsaturated pyroclastic soils 总被引:4,自引:4,他引:0
In the last 20 years, several catastrophic precipitation-induced landslides have hit villages, towns and roads in Campania
(southern Italy), causing extensive damage and many fatalities. Although such phenomena have occurred since time immemorial,
recent urbanisation and infrastructural development have produced a major increase in landslide risk. Due to climatic changes
and further unavoidable increases in exposure, in the near future, the risk will become even greater. It is therefore high
time to develop reliable criteria for landslide prediction. The paper discusses the main factors which affect the triggering
of precipitation-induced landslides, highlighting the key role played by antecedent rainfalls which cannot be precisely accounted
for using empirical criteria. We propose a simple 1D numerical approach able to predict the evolution of the key factors governing
slope stability as a tool to predict the onset of slope failure, with potential benefits for early warning systems. The approach
is calibrated through a well-documented case history. 相似文献
96.
Guido Agapito Carmelo Arcidiacono F. Quirós-Pacheco Simone Esposito 《Experimental Astronomy》2014,37(3):503-523
The First Light Adaptive Optics (FLAO) system has been successfully commissioned at the Large Binocular Telescope. It delivers extreme adaptive optics performance using bright natural guide stars reaching 90 % Strehl Ratios in H-band. Observations with current adaptive optics systems are limited to the near infrared wavelengths, in these bands the diffraction limited resolution of the largest ground-based telescopes (8–10 meter class) is comparable to the one of the much smaller Hubble Space Telescope that observes in the visible bands. This study aims to demonstrate the feasibility of an adaptive optics system designed to achieve very high order correction at visible wavelengths (0.5 to 0.8 μ m) with significant sky coverage. Upgrading the FLAO design with a low noise CCD relaxes the reference magnitude limit needed to achieve greater performance. In particular, we demonstrate that a gain of 1–2 magnitudes is possible by upgrading the wavefront sensor with a very low read out noise CCD. For future AO systems, in addition to low noise CCDs, deformable (secondary) mirrors with a higher actuator density will be able to move the high order correction capability from the near infrared to the visible wavelengths (Strehl Ratio of 80 % in R (0.7 μ m), 60 % in V (0.5 μ m)). We investigate, by means of numerical simulation, the gain in imaging performance obtained at Near Infrared, Visible, and UV wavelengths. The results of these simulations have been used to derive the empirical relation between Strehl Ratio and magnitude of the reference star and we then use this relationship to perform a detailed sky coverage analysis based on astronomical catalog data. The detailed simulations of the Point Spread Functions allow us to compute Ensquared Energy and Strehl Ratio for the magnitude working range of such an Adaptive Optics system. We present the results of the instrumental isoplanatic angle determination. We then used these values to compute the relationship between correction level and the off-axis angle from the reference star. The Strehl Ratio relationship with the reference magnitude and the angular distance provides the information needed to perform the sky-coverage analysis, which demonstrates that the designed system is able to provide V and R bands correction on a not negligible few percent of the sky. 相似文献
97.
3D-electrical resistivity tomography monitoring of salt transport in homogeneous and layered soil samples 总被引:1,自引:1,他引:0
Cesare Comina Renato Maria Cosentini Gabriele Della Vecchia Sebastiano Foti Guido Musso 《Acta Geotechnica》2011,6(4):195-203
Monitoring transport of dissolved substances in soil deposits is particularly relevant where safety is concerned, as in the
case of geo-environmental barriers. Geophysical methods are very appealing, since they cover a wide domain, localising possible
preferential flow paths and providing reliable links between geophysical quantities and hydrological variables. This paper
describes a 3D laboratory application of electrical resistivity tomography (ERT) used to monitor solute transport processes.
Dissolution and transport tests on both homogeneous and heterogeneous samples were conducted in an instrumented oedometer
cell. ERT was used to create maps of electrical conductivity of the monitored domain at different time intervals and to estimate
concentration variations within the interstitial fluid. Comparisons with finite element simulations of the transport processes
were performed to check the consistency of the results. Tests confirmed that the technique can monitor salt transport, infer
the hydro-chemical behaviour of heterogeneous geomaterials and evaluate the performances of clay barriers. 相似文献
98.
99.
Ray A. F. Cas Heather M. N. Wright Christopher B. Folkes Chiara Lesti Massimiliano Porreca Guido Giordano Jose G. Viramonte 《Bulletin of Volcanology》2011,73(10):1583-1609
The 2.08-Ma Cerro Galán Ignimbrite (CGI) represents a >630-km3 dense rock equivalent (VEI 8) eruption from the long-lived Cerro Galán magma system (∼6 Ma). It is a crystal-rich (35–60%),
pumice (<10% generally) and lithic-poor (<5% generally) rhyodacitic ignimbrite, lacking a preceding plinian fallout deposit.
The CGI is preserved up to 80 km from the structural margins of the caldera, but almost certainly was deposited up to 100 km
from the caldera in some places. Only one emplacement unit is preserved in proximal to medial settings and in most distal
settings, suggesting constant flow conditions, but where the pyroclastic flow moved into a palaeotopography of substantial
valleys and ridges, it interacted with valley walls, resulting in flow instabilities that generated multiple depositional
units, often separated by pyroclastic surge deposits. The CGI preserves a widespread sub-horizontal fabric, defined by aligned
elongate pumice and lithic clasts, and minerals (e.g. biotite). A sub-horizontal anisotropy of magnetic susceptibility fabric
is defined by minute magnetic minerals in all localities where it has been analysed. The CGI is poor in both vent-derived
(‘accessory’) lithics and locally derived lithics from the ground surface (‘accidental’) lithics. Locally derived lithics
are small (<20 cm) and were not transported far from source points. All data suggest that the pyroclastic flow system producing
the CGI was characterised throughout by high sedimentation rates, resulting from high particle concentration and suppressed
turbulence at the depositional boundary layer, despite being a low aspect ratio ignimbrite. Based on these features, we question
whether high velocity and momentum are necessary to account for extensive flow mobility. It is proposed that the CGI was deposited
by a pyroclastic flow system that developed a substantial, high particle concentration granular under-flow, which flowed with
suppressed turbulence. High particle concentration and fine-ash content hindered gas loss and maintained flow mobility. In
order to explain the contemporaneous maintenance of high particle concentration, high sedimentation rate at the depositional
boundary layer and a high level of mobility, it is also proposed that the flow(s) was continuously supplied at a high mass
feeding rate. It is also proposed that internal gas pressure within the flow, directed downwards onto the substrate over which
the flow was passing, reduced the friction between the flow and the substrate and also enhanced its mobility. The pervasive
sub-horizontal fabric of aligned pumice, lithic and even biotite crystals indicates a consistent horizontal shear force existed
during transport and deposition in the basal granular flow, consistent with the existence of a laminar, shearing, granular
flow regime during the final stages of transport and deposition. 相似文献
100.
We present a synopsis of detrital zircon U–Pb ages of sandstones from North Africa and neighboring Israel and Jordan, which allows us to identify zones with characteristic sediment provenance along the northern Gondwana margin (in present-day coordinates) in Cambrian–Ordovician times, and helps us to unravel the peri-Gondwana jigsaw puzzle. A special feature of the early Paleozoic cover sequence of North Africa is the eastward increase of 1.1–0.95 Ga detrital zircons, which become ubiquitous in the early Paleozoic sandstones of the Saharan Metacraton. Detrital zircons aged about 2.7–2.5, 2.15–1.75 and 0.75–0.53 Ga are also present. Early Paleozoic sandstones with similar provenance are known from peri-Gondwana terranes in the Eastern and Western Mediterranean and from NW Iberia. These terranes need not be transported from western Gondwana (Amazonia) as suggested previously. They were likely located to the north of the Saharan Metacraton during the early Paleozoic before they rifted off from Gondwana. Furthermore, we recognize an increase, as stratigraphic ages get younger, of ca. 1.0 Ga detrital zircons at some point between the Late Cambrian and late Middle Ordovician. We speculate that this might be linked to far-field tectonics and regional uplift in central Gondwana related to plate-tectonic reorganization along the Gondwana margin, leading to erosion of ca. 1.0 Ga basement and country rocks of the Transgondwanan supermountain and fluvial dispersal of detritus toward the Gondwana margin. 相似文献