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A temporary accelerometer network has been installed in Tarcento (Friuli, NE Italy), a small town heavily hit by the 1976–1977
Friuli earthquake sequence, as a part of an ongoing research project aimed at ground motion simulation and generation of shakemaps
in the near-field of an earthquake. The network operated from October 2008 to April 2010 and consisted of three K2 accelerographs
with internal Episensor, distributed over a linear array of about 1.5 km length. Tarcento town had been chosen, at the end
of the 1970s, as the ideal site for a pilot microzonation study, the first of this kind in Italy, in which a substantial number
of field (and laboratory) tests were carried out in order to assess the mechanical properties of local alluvium deposits and
their complex (3D) geometrical configuration. The data from the temporary network, illustrated herein, allow for proper verification
and review of some of the quantitative predictions formulated in the 1980 study. As argued in the discussion section, we also
believe that the data are apt to provide valuable information of more general interest on the complex seismic response of
alluvium-filled valleys, and we show therein how the observations can be interpreted in the light of presently available parametric
simulation studies and simplified criteria for handling basin amplification effects. 相似文献
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C. H. Mandrini P. Démoulin L. Van Driel-Gesztelyi B. Schmieder G. Cauzzi A. Hofmann 《Solar physics》1996,168(1):115-133
On May 1, 1993, a flaring X-ray bright point (XBP) was observed for about 16 hours in the old, disintegrating, bipolar active region (AR) NOAA 7493. During this period, a minor magnetic bipole (1020 Mx) emerged in the region. We have found observational evidence showing that the XBP brightenings were due to magnetic reconnection between the new bipole and pre-existing plage fields. The aim of the present work is to substantiate with magnetic modelling what has been shown by the observations. For this purpose we extrapolate the observed photospheric magnetic fields in the linear force-free approximation and follow its evolution during the lifetime of the XBP. From the computed coronal field lines we determine the location of regions of drastic change in field-line linkage, called quasi-separatrix layers or QSLs. QSLs are open layers that behave physically like separatrices: the break down of ideal magnetohydrodynamics and the release of free magnetic energy may occur at these locations when their thickness is small enough. The extrapolated field lines, with photospheric footpoints on both sides of QSLs, match the observed chromospheric and coronal structures (arch filament system, XBP and faint X-ray loops (FXL)). We study also the evolution of the width of the QSL located over the new negative polarity pore: the calculated QSL is very thin (typically less than 100 m) during the lifetime of the XBP, but becomes much thicker ( 104 m) after the XBP has faded. Furthermore we show that peaks in X-ray brightness propagate along the FXL with a velocity of 670 km s-1, starting from the XBP location, implying that the energy is released where the emerging bipole impacts against pre-existing coronal loops. We discuss the possible mechanism of energy transport and conclude that the energy is conducted to the remote footpoints of the FXL by a thermal front. These results strongly support the supposition that the XBP brightness and flaring are due to the interaction of different flux systems, through 3D magnetic reconnection, at QSLs.Member of the Carrera del Investigador Cientifíco, CONICET.Also at Konkoly Observatory, Budapest, Pf. 67, H-1525 Hungary. 相似文献
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Cauzzi Carlo Fäh Donat Wald David J. Clinton John Losey Stéphane Wiemer Stefan 《Natural Hazards》2018,92(2):1211-1235
Natural Hazards - In Switzerland, nearly all historical Mw?~?6 earthquakes have induced damaging landslides, rockslides and snow avalanches that, in some cases, also resulted in damage... 相似文献
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D. Bonaccini G. Cauzzi A. Falchi R. Falciani L. A. Smaldone 《Astrophysics and Space Science》1990,169(1-2):117-119
In this communication we briefly review the content of Cephei pulsating stars in young open clusters. The actual metallicity differences between clusters are suggested to be detectable as variations of the location of these stars in the photometric diagrams. We make a quantitative estimate of these differences and comment on the connections with the existence and possible determination of a metallicity gradient in the galactic plane.Paper presented at the 11th European Regional Astronomical Meetings of the IAU on New Windows to the Universe, held 3–8 July, 1989, Tenerife, Canary Islands, Spain. 相似文献
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Tobias Diehl John Clinton Nicolas Deichmann Carlo Cauzzi Philipp Kästli Toni Kraft Irene Molinari Maren Böse Clotaire Michel Manuel Hobiger Florian Haslinger Donat Fäh Stefan Wiemer 《Swiss Journal of Geoscience》2018,111(1-2):221-244
This report summarizes the seismicity in Switzerland and surrounding regions in the years 2015 and 2016. In 2015, the Swiss Seismological Service detected and located 735 earthquakes in the region under consideration. With a total of 20 earthquakes of magnitude ML ≥ 2.5, the seismic activity of potentially felt events in 2015 was close to the average of 23 earthquakes over the previous 40 years. Seismic activity was above average in 2016 with 872 located earthquakes of which 31 events had ML ≥ 2.5. The strongest event in the analyzed period was the ML 4.1 Salgesch earthquake, which occurred northeast of Sierre (VS) in October 2016. The event was felt in large parts of Switzerland and had a maximum intensity of V. Derived focal mechanisms and relative hypocenter relocations of aftershocks image a SSE dipping reverse fault, which likely also hosted an ML 3.9 earthquake in 2003. Another remarkable earthquake sequence in the Valais occurred close to Sion with four felt events (ML 2.7–3.2) in 2015/16. We associate this sequence with a system of WNW-ESE striking fault segments north of the Rhône valley. Similarities with a sequence in 2011, which was located about 10 km to the NE, suggest the existence of an en-echelon system of basement faults accommodating dextral slip along the Rhône-Simplon line in this area. Another exceptional earthquake sequence occurred close to Singen (Germany) in November 2016. Relocated hypocenters and focal mechanisms image a SW dipping transtensional fault segment, which is likely associated with a branch of the Hegau-Bodensee Graben. On the western boundary of this graben, micro-earthquakes close to Schlattingen (TG) in 2015/16 are possibly related to a NE dipping branch of the Neuhausen Fault. Other cases of earthquakes felt by the public during 2015/16 include earthquakes in the region of Biel, Vallorcine, Solothurn, and Savognin. 相似文献
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Roberto Paolucci Antonio Rovelli Ezio Faccioli Carlo Cauzzi Daniela Finazzi Manuela Vanini Carola Di Alessandro Giovanna Calderoni 《地震工程与结构动力学》2008,37(5):697-710
Using records from co‐located broadband and digital strong motion (SM) instruments, it is first shown that the displacement waveforms obtained by double integration of the accelerogram need not be free of unrealistic baseline drift to yield reliable spectral ordinates up to at least 10 s. Secondly, to provide objective criteria for selecting reliable digital SM records for ground motion predictions at long periods, a set of synthetic accelerograms contaminated by random long‐period noise has been used, and the difference between the original accelerograms and the spurious ones in terms of response spectra has been quantified, by introducing a noise index that can be easily calculated based on the velocity waveform of the record. The results of this study suggest that high‐pass filtering the digital acceleration record from a cutoff period selected to suppress baseline drifts on the displacement waveform appears to be in most cases too conservative and unduly depletes reliable information on long‐period spectral ordinates. Copyright © 2007 John Wiley & Sons, Ltd. 相似文献
9.
Broadband (0.05 to 20 s) prediction of displacement response spectra based on worldwide digital records 总被引：6，自引：0，他引：6
A new set of empirical equations for prediction of displacement response spectral ordinates from 20 Hz to T = 20 s is illustrated. The coefficients of the equations were obtained by regressing a dataset based on 1,155 tri-axial digital
and 9 analog accelerometer records from 60 earthquakes worldwide. Long period disturbances in the accelerograms were evaluated
and removed using a very recent method, aimed at preserving the long-period spectral content of the records. Analysis of variance
has disclosed only little evidence for regional dependence of ground motions, while a carefully conducted evaluation of site
effects resulted in clearly differentiated spectral amplification bands associated to the main ground types B, C, and D of
Eurocode 8. Spectral ordinates for vibration periods >5 s were found to scale with magnitude quite consistently with theoretical
scaling from Brune’s model. On the other hand, comparison of results with those yielded by recent prediction models in Europe
and the United States (NGA), indicated that the latter may not be uniformly reliable at long periods. The proposed empirical
equations are easily implemented in computer programs for seismic hazard assessment, being characterized by a simple functional
form and a restricted number of predictor variables.
Electronic supplementary material The online version of this article (doi:) contains supplementary material, which is available to authorized users. 相似文献