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11.
Anthropogenic subsidence in the Mexicali Valley,Baja California,Mexico, and slip on the Saltillo fault 总被引:2,自引:1,他引:1
Ewa Glowacka Olga Sarychikhina Francisco Suárez F. Alejandro Nava Robert Mellors 《Environmental Earth Sciences》2010,59(7):1515-1524
Deep fluid extraction in the Cerro Prieto geothermal field (CPGF) has caused subsidence and induced slip on tectonic faults
in the Mexicali Valley (Baja California, Mexico). The Mexicali Valley is located in the southern part of the Salton Trough,
at the boundary between the Pacific and North American plates. The Valley is characterized by being a zone of continuous tectonic
deformation, geothermal activity, and seismicity. Within the Cerro Prieto pull-apart basin, seismicity is concentrated mainly
in swarms, while strong earthquakes have occurred in the Imperial and Cerro Prieto transform faults, that are the eastern
and western bound of the basin. Since 1973, fluid extraction at the CPGF has influenced deformation in the area, accelerating
the subsidence and causing rupture (frequently as vertical slip or creep) on the surface traces of tectonic faults. Both subsidence
and fault slip are causing damage to infrastructure like roads, railroad tracks, irrigation channels, and agricultural fields.
Currently, accelerated extraction in the eastern part of CPGF has shifted eastwards the area of most pronounced subsidence
rate; this accelerated subsidence can be observed at the Saltillo fault, a southern branch of the Imperial fault in the Mexicali
Valley. Published leveling data, together with field data from geological surveys, geotechnical instruments, and new InSAR
images were used to model the observed deformation in the area in terms of fluid extraction. Since the electricity production
in the CPGF is an indispensable part of Baja California economy, extraction is sure to continue and may probably increase,
so that the problem of damages caused by subsidence will likely increase in the future. 相似文献
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Natural Hazards - The study of flood risk perception factors can be considered by using different paradigms. In an attempt to understand risk perception, two basic paradigms can be distinguished:... 相似文献
14.
Pham Quoc Bao Ali Sk Ajim Bielecka Elzbieta Calka Beata Orych Agata Parvin Farhana Łupikasza Ewa 《Natural Hazards》2022,113(2):1043-1081
Natural Hazards - Advances in the availability of multi-sensor, remote sensing-derived datasets, and machine learning algorithms can now provide an unprecedented possibility to predict flood events... 相似文献
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Ewa Bednorz 《Theoretical and Applied Climatology》2009,97(3-4):279-286
Circulation patterns favourable for rapid snowmelt in the Polish-German lowlands are described in the study. Composite maps of the SLP and 500 hPa geopotential heights means and composite anomaly maps, constructed for the days with the decrease in snow cover depth of ≥5 cm/day, show deeper than usual low-pressure systems over the northern Atlantic and slightly higher than usual pressure over the Mediterranean. Such pressure patterns corresponds to the positive NAO phase with large pressure gradients, which intensify west and south-west air flows over Central Europe. Warm and humid air masses from the west and south-west contribute to substantial daily temperature increases and, frequently, to higher-than-usual precipitation, which speeds up ablation. 相似文献
17.
Jarosaw Klimentowski Ewa L. okas Stelios Kazantzidis Lucio Mayer Gary A. Mamon 《Monthly notices of the Royal Astronomical Society》2009,397(4):2015-2029
We conduct high-resolution collisionless N -body simulations to investigate the tidal evolution of dwarf galaxies on an eccentric orbit in the Milky Way (MW) potential. The dwarfs originally consist of a low surface brightness stellar disc embedded in a cosmologically motivated dark matter halo. During 10 Gyr of dynamical evolution and after five pericentre passages, the dwarfs suffer substantial mass loss and their stellar component undergoes a major morphological transformation from a disc to a bar and finally to a spheroid. The bar is preserved for most of the time as the angular momentum is transferred outside the galaxy. A dwarf spheroidal (dSph) galaxy is formed via gradual shortening of the bar. This work thus provides a comprehensive quantitative explanation of a potentially crucial morphological transformation mechanism for dwarf galaxies that operates in groups as well as in clusters. We compare three cases with different initial inclinations of the disc and find that the evolution is fastest when the disc is coplanar with the orbit. Despite the strong tidal perturbations and mass loss, the dwarfs remain dark matter dominated. For most of the time, the one-dimensional stellar velocity dispersion, σ, follows the maximum circular velocity, V max , and they are both good tracers of the bound mass. Specifically, we find that M bound ∝ V 3.5 max and in agreement with earlier studies based on pure dark matter simulations. The latter relation is based on directly measuring the stellar kinematics of the simulated dwarf, and may thus be reliably used to map the observed stellar velocity dispersions of dSphs to halo circular velocities when addressing the missing satellites problem. 相似文献
18.
Arkadiusz?M.?TomczykEmail author Piotr?Piotrowski Ewa?Bednorz 《Theoretical and Applied Climatology》2017,128(3-4):623-634
This study describes warm spells in Northern Europe and determines the synoptic situations that cause their occurrence. In this article, a relatively warm day was defined as a day when the maximum temperature exceeded the 95th annual percentile, and a warm spell (WS) was considered to be a sequence of at least five relatively warm days. In the analysed multiannual period and within the investigated area, 24 (Kallax) to 53 (Oslo) WSs were observed. The occurrence of WSs was mainly connected with positive anomalies of sea level pressure and a 500-hPa isobaric surface, displaying the presence of high-pressure systems. This occurrence was also accompanied by positive T850 anomalies. 相似文献
19.
Olga Sarychikhina Ewa Glowacka Braulio Robles F. Alejandro Nava Miguel Guzmán 《Pure and Applied Geophysics》2015,172(11):3139-3162
20.