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11.
Filippo Santucci de Magistris Anna d’Onofrio Augusto Penna Rodolfo Puglia Francesco Silvestri 《Natural Hazards》2014,74(3):2005-2035
The prediction of the variability of the seismic ground motion in a given built-up area is considered an effective tool to plan appropriate urban development, to undertake actions on seismic risk mitigation and to understand the damage pattern caused by a strong-motion event. The procedures for studying the seismic response and the seismic microzonation of an urban area are well established; nevertheless, some controversial points still exists and are discussed here. In this paper, the selection of a reference input motion, the construction of a subsoil model and the seismic response analysis procedures are discussed in detail, based on the authors’ experience in two Italian case histories: the seismic microzonation of the city of Benevento, which was a predictive study, and the simulation of seismic response and damage distribution in the village of San Giuliano di Puglia, which was a retrospective analysis. 相似文献
12.
Pedro Augusto Peter N. Wilkinson Ian W.A. Browne 《Astrophysics and Space Science》1998,261(1-4):261-264
In this paper we present a subsample of 55 flat-spectrum radio sources dominated by (∼ 100 mas) kpc-scale structure, selected
from a parent sample of 1665 VLA sources. Most are core-jets and 23 are CSO/MSO candidates. Properties of the subsample are
discussed.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
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Photographs of Comet Bennett 1969i taken in the dust-scattered continuum reveal that the dust particles, leading to the formation of the type II tail, leave the vicinity of the nucleus only within a certain cone with the aperture in the direction to the Sun. Three parabolic envelopes embracing the nucleus are formed by the dust (vertex always about on the radius vector) reaching distances from the nucleus of 30 000, 60 000 and 100 000 km.There exists no relation between the production and motion of this dust and the production and motion of the neutral coma gases. The cone of expulsion of the dust is identical with the cone of expulsion for the ions leading to the formation of the type I tail. Dust- and ion envelopes have, however, different kinematical properties. The cone of expulsion is identical with Bessel's Ausströmungskegel of visible matter observed by him in Comet Halley 1835.Comet Bennett is compared with Comet Halley 1910; they are related in many respects although Comet Halley had a lower dust production than the Comet Bennett.We ascribe to the dust particles of the tail II from the beginning of the expulsion an electrical charge. 相似文献
20.
E. Wiedner D. Scholz A. Mangini D. Polag C. Mühlinghaus M. Segl 《Quaternary International》2008,187(1):15
Many speleothems show evidence for calcite precipitation under disequilibrium conditions. To improve the understanding of these kinetic processes, several laboratory experiments were performed to study the fractionation of stable oxygen and carbon isotopes during the precipitation of calcite. Carbonate was precipitated under controlled conditions from both a body of standing water (beaker experiments) and a solution flowing along a channel (channel experiments) at a relative humidity of 100%. Slow degassing of CO2, simulated by the beaker experiments, results in δ18O values in equilibrium with the solution. In contrast, the δ13C values show a significant enrichment, inversely proportional to the height of the solution in the beakers. Fast degassing of CO2, simulated by the channel experiments, showed an enrichment of both δ13C and δ18O and a slope of Δδ13C/Δδ18O of 1.4±0.6. These results represent experimental evidence for the Hendy effect, which is manifested in (i) a progressive increase in δ18O and δ13C away from the growth axis and (ii) a positive correlation between δ18O and δ13C along a single growth layer of a stalagmite. 相似文献