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1.
G. Cevolani G. Bortolotti L. Foschini C. Franceschi G. Grassi G. Trivellone A. Hajduk V. Porubčan 《Earth, Moon, and Planets》1995,68(1-3):247-255
Continuous radio-wave monitoring of the Geminid activity in December 1992 and 1993 by using a forward scatter (FS) bistatic radar over the Bologna-Lecce baseline (700 km) in Italy, reveals peculiar structural aspects of the stream in terms of signal amplitude-rate and duration-rate dependence. The observational results of the Geminid display obtained in the two consecutive years with differentiated peak levels of transmitted power, exhibit different time distributions of underdense meteors against the signal received power. Both sets of the data relative to the peak activity in December 12–14, show reflection properties of Geminids which are atypical if compared with echoes from cometary-type showers, with really high echo counts at mid-upper levels of the peak received power. An assymmetric curve of activity of the Geminids complex is evidenced, with the peak flux of smaller particles occurring earlier than that of larger ones. 相似文献
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Dauphiné twinning and texture memory in polycrystalline quartz. Part 3: texture memory during phase transformation 总被引：1，自引：0，他引：1
Hans-Rudolf?WenkEmail author N.?Barton M.?Bortolotti S.?C.?Vogel M.?Voltolini G.?E.?Lloyd G.?B.?Gonzalez 《Physics and Chemistry of Minerals》2009,36(10):567-583
Samples of quartz-bearing rocks were heated above the α (trigonal)–β (hexagonal) phase transformation of quartz (625–950°C)
to explore changes in preferred orientation patterns. Textures were measured both in situ and ex situ with neutron, synchrotron
X-ray and electron backscatter diffraction. The trigonal–hexagonal phase transformation does not change the orientation of
c- and a-axes, but positive and negative rhombs become equal in the hexagonal β-phase. In naturally deformed quartzites measured by
neutron diffraction a perfect texture memory was observed, i.e. crystals returned to the same trigonal orientation they started
from, with no evidence of twin boundaries. Samples measured by electron back-scattered diffraction on surfaces show considerable
twinning and memory loss after the phase transformation. In experimentally deformed quartz rocks, where twinning was induced
mechanically before heating, the orientation memory is lost. A mechanical model can explain the memory loss but so far it
does not account for the persistence of the memory in quartzites. Stresses imposed by neighboring grains remain a likely cause
of texture memory in this mineral with a very high elastic anisotropy. If stresses are imposed experimentally the internal
stresses are released during the phase transformation and the material returns to its original state prior to deformation.
Similarly, on surfaces there are no tractions and thus texture memory is partially lost. 相似文献
4.
A sequence of graded ophiolitic sandstones, 120 m thick (Sanguigna Formation), outcrops within the Messinian Evaporite Group in a limited area near Gabbro, Fine Basin, western Tuscany.The formation lies between fine-grained sediments laid down under a thin water-cover. The graded beds show, on the other hand, many features typical of proximal turbidites, such as amalgamated layers, scour-and-fill structures, clay flakes and lumps, top-truncated Bouma sequences. Grain-size analyses suggest that they were deposited from high-density turbidity flows.The petrographic composition and the grain fabric indicate that the feeding was from the northeast across the Fine Basin. From the inferred dimensions and depth of the basin, the mean slope should have been less than 1°. The turbidity currents probably originated at a river mouth during flood stages.The Sanguigna graded beds are compared with occurrences of shallow-water turbidites. 相似文献
5.
Abstract In this paper, a summary of the tectonic history of the Mirdita ophiolitic nappe, northern Albania, is proposed by geological and structural data. The Mirdita ophiolitic nappe includes a subophiolite mélange, the Rubik complex, overlain by two ophiolite units, referred to as the Western and Eastern units. Its history started in the Early Triassic with a rifting stage followed by a Middle to Late Triassic oceanic opening between the Adria and Eurasia continental margins. Subsequently, in Early Jurassic time, the oceanic basin was affected by convergence with the development of a subduction zone. The existence of this subduction zone is provided by the occurrence of the supra‐subduction‐zone‐related magmatic sequences found in both the Western and Eastern units of the Mirdita ophiolitic nappe. During the Middle Jurassic, continuous convergence resulted in the obduction of the oceanic lithosphere, in two different stages – the intraoceanic and marginal stages. The intraoceanic stage is characterized by the westward thrusting of a young and still hot section of oceanic lithosphere leading to the development of a metamorphic sole. In the Late Jurassic, the marginal stage developed by the emplacement of the ophiolitic nappe onto the continental margin. During this second stage, the emplacement of the ophiolites resulted in the development of the Rubik complex. In the Early Cretaceous, the final emplacement of the ophiolites was followed by the unconformable sedimentation of the Barremian–Senonian platform carbonate. From the Late Cretaceous to the Middle Miocene, the Mirdita ophiolitic nappe was translated westward during the progressive migration of the deformation front toward the Adria Plate. In the Middle to Late Miocene, a thinning of the whole nappe pile was achieved by extensional tectonics, while the compression was still active in the westernmost areas of the Adria Plate. On the whole, the Miocene deformations resulted in the uplift and exposition of the Mirdita ophiolites as observed today. 相似文献
6.
H.-R. Wenk M. Bortolotti N. Barton E. Oliver D. Brown 《Physics and Chemistry of Minerals》2007,34(9):599-607
Mechanical twinning in polycrystalline quartz was investigated in situ with time-of-flight neutron diffraction and a strain
diffractometer. Dauphiné twinning is highly temperature sensitive. It initiates at a macroscopic differential stress of 50–100 MPa
and, at 500°C, saturates at 400 MPa. From normalized diffraction intensities the patterns of preferred orientation (or texture)
can be inferred. They indicate a partial reversal of twinning during unloading. The remaining twins impose residual stresses
corresponding to elastic strains of 300–400 microstrain. Progressive twinning on loading and reversal during unloading, as
well as the temperature dependence, can be reproduced with finite element model simulations. 相似文献
7.
Geodynamic evolution of ophiolites from Albania and Greece (Dinaric-Hellenic belt): one, two, or more oceanic basins? 总被引：1，自引：0，他引：1
Valerio Bortolotti Marco Chiari Michele Marroni Luca Pandolfi Gianfranco Principi Emilio Saccani 《International Journal of Earth Sciences》2013,102(3):783-811
All the geological constraints for an exhaustive reconstruction of the Triassic to Tertiary tectonic history of the southern Dinaric-Hellenic belt can be found in Albania and Greece. This article aims to schematically reconstruct this long tectonic evolution primarily based on a detailed analysis of the tectonic setting, the stratigraphy, the geochemistry, and the age of the ophiolites. In contrast to what was previously reported in the literature, we propose a new subdivision on a regional scale of the ophiolite complexes cropping out in Albania and Greece. This new subdivision includes six types of ophiolite occurrences, each corresponding to different tectonic units derived from a single obducted sheet. These units are represented by: (1) sub-ophiolite mélange, (2) Triassic ocean-floor ophiolites, (3) metamorphic soles, (4) Jurassic fore-arc ophiolites, (5) Jurassic intra-oceanic-arc ophiolites, and (6) Jurassic back-arc basin ophiolites. The overall features of these ophiolites are coherent with the existence of a single, though composite, oceanic basin located east of the Adria/Pelagonian continental margin. This oceanic basin was originated during the Middle Triassic and was subsequently (Early Jurassic) affected by an east-dipping intra-oceanic subduction. This subduction was responsible for the birth of intra-oceanic-arc and back-arc oceanic basins separated by a continental volcanic arc during the Early to Middle Jurassic. From the uppermost Middle Jurassic to the Early Cretaceous, an obduction developed, during which the ophiolites were thrust westwards firstly onto the neighboring oceanic lithosphere and then onto the Adria margin. 相似文献
8.
Roberto Ambrosini Pietro Bolli Claudio Bortolotti Francesco Gaudiomonte Filippo Messina Mauro Roma 《Experimental Astronomy》2010,27(3):121-130
Apart from externally generated Radio Frequency Interference (RFI), the occurrence of self-interference is a major concern
at any modern radio telescope site. Antenna servo motor controllers, data acquisition processors, and fast computing capabilities
operate very close to extremely sensitive and wideband radio astronomical receivers. In this paper, we present a set of measurements
of the RFI level generated by a cluster of computers that will be installed at the site of the Sardinia Radio Telescope (SRT).
The measured levels are compared to Recommendation ITU-R RA.769-2, which gives the threshold levels for interference detrimental
to radio astronomy observations. Our analysis shows that, with proper shielding of the noisiest devices, it will be possible
to preserve the present excellent RFI conditions of the SRT site. 相似文献
9.
The core of the Troodos Massif consists of a major tectonitic harzburgite—dunite unit (Mt. Olympus Unit) overlain by three tectonic units which, in descending order, consist of dunites, wherlites and gabbros, respectively. Furthermore, the Mt. Olympus Unit is underlain by three other tectonic units with the same lithology as the upper ones. The thrusts show a north-to-south emplacement, probably of latest Cretaceous age.It is suggested that Troodos, Southern Turkey, Hatay and Oman ophiolites could belong to the same oceanic domain; they underwent different displacement toward the Arabian—African plate. 相似文献
10.
M. Di Martino S. Montebugnoli S. Ostro S. Righini S. Poppi A. Orlati C. Bortolotti Y. Gavrik 《Planetary and Space Science》2004,52(4):325-330
We describe the first intercontinental planetary radar initiative undertaken in Italy.We present the results of the observations of Near-Earth Asteroid (NEA) 33342 (1998 WT24), performed in December 2001 using the bistatic configurations Goldstone-Medicina and Evpatoria-Medicina, with the 32-m Medicina dish used to receive echoes in both cases.The experiment goal was to characterise the system for radar follow-up observations of NEA and artificial orbiting debris, in the framework of a feasibility study which aims at using the Sardinia Radio Telescope, at present under construction, also as a planetary radar facility. 相似文献