Ground-motion scenarios on Mt. Etna inferred from empirical relations and synthetic simulations     

Horst Langer  Giuseppina Tusa  Luciano Scarfì  Raffaele Azzaro 《Bulletin of Earthquake Engineering》2016,14(7):1917-1943

Ground motion scenarios for Mt. Etna are created using synthetic simulations with the program EXSIM. A large data set of weak motion records is exploited to identify important input parameters which govern the modeling of wave propagation effects, such as Q-values, high frequency cut-off and geometrical spreading. These parameters are used in the simulation of ground motion for earthquakes causing severe damage in the area. Two seismotectonic regimes are distinguished. Volcano-tectonic events, though being of limited magnitude (M_max ca. 5), cause strong ground shaking for their shallow foci. Being rather frequent, these events represent a considerable threat to cities and villages on the flanks of the volcano. A second regime is related to earthquakes with foci in the crust, at depths of 10–30 km, and magnitudes ranging from 6 to 7. In our synthetic scenarios, we chose two examples of volcano-tectonic events, i.e. the October 29, 2002, Bongiardo event (I = VIII) and the May 8, 1914, Linera earthquake (I = IX–X). A further scenario regards the February 20, 1818 event, considered representative for stronger earthquakes with foci in the crust. We were able to reproduce the essential features of the macroseismic field, in particular accounting for the possibility of strong site effects. We learned that stress drop estimated for weak motion events is probably too low to explain the intensity of ground motion during stronger earthquakes. This corresponds to findings reported in the literature claiming an increase of stress drop with earthquake size.  相似文献   

Interaction of bentonite colloids with Cs, Eu, Th and U in presence of humic acid: A flow field-flow fractionation study   总被引：2，自引：0，他引：2  

Muriel Bouby  Horst Geckeis  Silvia Mihai  Thorsten Schäfer 《Geochimica et cosmochimica acta》2011,75(13):3866-3880

The interaction of Cs(I), Eu(III), Th(IV) and U(VI) with montmorillonite colloids was investigated in natural Grimsel Test Site groundwater over a 3 years period. The asymmetric flow field-flow fractionation combined with various detectors was applied to study size variations of colloids and to monitor colloid association of trace metals. The colloids suspended directly in the low ionic strength (I), slightly alkaline granitic groundwater (I = 10⁻³ mol/L, pH 9.6) showed a gradual agglomeration with a size distribution shift from initially 10-200 nm to 50-400 nm within over 3 years. The Ca²⁺ concentration of 2.1 × 10⁻⁴ mol/L in the ground water is believed to be responsible for the slow agglomeration due to Ca²⁺ ion exchange against Li⁺ and Na⁺ at the permanently charged basal clay planes. Furthermore, the Ca²⁺ concentration lies close to the critical coagulation concentration (CCC) of 10⁻³ mol L⁻¹ for clay colloids. Slow destabilization may delimit clay colloid migration in this specific groundwater over long time scales. Eu(III) and Th(IV) are found predominantly bound to clay colloids, while U(VI) prevails as the UO₂(OH)₃⁻ complex and Cs(I) remains mainly as aquo ion under our experimental conditions. Speciation calculations qualitatively represent the experimental data. A focus was set on the reversibility of metal ion-colloid binding. Addition of humic acid as a competing ligand induces rapid metal ion dissociation from clay colloids in the case of Eu(III) even after previous aging for about 3 years. Interestingly only partial dissociation occurs in the case of Th(IV). Experiments and calculations prove that the humate complexes dominate the speciation of all metal ions under given conditions. The partial irreversibility of clay bound Th(IV) is presently not understood but might play an important role for the colloid-mediated transport of polyvalent actinides over wide distances in natural groundwater.  相似文献   

Increasing levels and biomagnification of persistent organic pollutants (POPs) in Antarctic biota   总被引：3，自引：0，他引：3  

Goerke H  Weber K  Bornemann H  Ramdohr S  Plötz J 《Marine pollution bulletin》2004,48(3-4):295-302

Representatives of the Antarctic food web (krill, cephalopod, fish, penguin, seal) of the area around Elephant Island and from the Weddell Sea were analysed for the most recalcitrant organochlorine compounds. Due to sorption of the compounds to sinking particles and accumulation in sediments, two benthic fish species (Gobionotothen gibberifrons, Chaenocephalus aceratus) feeding on benthos invertebrates and fish reflected significantly increasing concentrations within a decade (1987-1996), while a benthopelagic species (Champsocephalus gunnari) feeding on krill did not. In the pelagic food chain, lipid normalised concentrations of all compounds increased from Antarctic krill to fish proving that biomagnification of highly lipophilic pollutants (log octanol-water partition coefficient>5) occurs in water-breathing animals. As top predators Weddell and southern elephant seals (Leptonychotes weddellii, Mirounga leonina) biomagnified the persistent organic pollutants relative to krill 30-160 fold with the exception of hexachlorobenzene, the levels of which were lower than in fish indicating its intense specific elimination.  相似文献   

Quiet-time periods observed by EPHIN/SOHO during the minimum of the 22nd solar cycle     

Gómez-Herrero  Raúl  RodrÍguez-FrÍas  M. Dolores  del Peral  Luis  Sequeiros  Juan  Müller-Mellin  Reinhold  Kunow  Horst  Sierks  Holger 《Solar physics》2000,194(2):405-413

An analysis of the hydrogen and helium isotopic composition from EPHIN data, during the quiet-time period from January 1 to June 1, 1996, is presented. An isotopic discrimination and background rejection have been applied and relationships between the abundances of ²H/¹H, ³He/⁴He, and ⁴He/¹H have been calculated. The energy spectra in the 4–50 MeV nucl^–1 range have been obtained and the contribution of the different spectral components have been analysed in this energy range. We conclude that the main contribution to the ⁴He spectrum is of anomalous origin, while the proton and ³He spectra have contributions mainly from particles of solar origin at low energies and from the galactic cosmic radiation modulated by the heliosphere at high energies. The deuterium spectrum is mainly of galactic origin.  相似文献   

The development and structure of nocturnal slope winds in a simple valley     

J. C. Doran  T. W. Horst  C. D. Whiteman 《Boundary-Layer Meteorology》1990,52(1-2):41-68

The results of an observational and modeling study of the nocturnal slope winds in a simple valley are presented. The valley was approximately 225 m deep in the region of the measurements, and featured a uniform slope angle of approximately 23 ° on one of its sidewalls. The wind and temperature structure of the katabatic flows on the valley sidewalls were measured with tower-mounted instruments, and a Doppler sodar and instruments on a tethered balloon and a 61-m tower were used to determine the atmospheric conditions near the center of the valley. The temperature structure of the slope flows was summarized by characteristic scale parameters h and T for the inversion depth and strength, respectively. On the sidewalls 50 m above the valley floor, the inversion depths were generally smaller and the inversion strengths were weaker than they were on the sidewalls 100 m higher. These results differ significantly from those obtained over a simple slope of an isolated mountain or ridge. The down-valley winds are shown to be important in limiting the strength of the sidewall inversions. The formation of an inversion in the valley also has a pronounced effect on the structure of the slope flows. Numerical simulations suggest that the presence of adiabatic layers in the valley atmosphere is associated with decreases in the slope-flow inversion depth with increasing downslope distance. The simulations also indicate that the length scales that characterize the momentum and inversion depths behave similarly in flows down simple slopes but not in flows down the sidewalls of a valley.Work supported by the U.S. Army Research Office under Contract DA-AG29-K-0231 and the U.S. Department of Energy under Contract DE-AC06-76RLO 1830.  相似文献   

Chemical and tectonic controls on the formation of sparry magnesite deposits — the deposits of the northern Greywacke Zone (Austria)     

Giulio Morteani  Horst Neugebauer 《International Journal of Earth Sciences》1990,79(2):337-344

The sparry magnesite deposits of the northern Greywacke Zone are situated at the base of thrust sheets. Model calculations and natural examples suggest that an inverse temperature gradient can only be established at the base of a thrust sheet if thrusting is so rapid as to be geologically unrealistic. Independently of this thrusting induces a fluid flow from the lower units to the front of the moving thrust sheet. Stability data of magnesite and dolomite in contact with fluids with different Ca/(Ca+Mg) ratios suggest that this tectonically induced fluid flow produce magnesite from preexisting dolomite by metasomatism.

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Zusammenfassung Die Spatmagnesitvorkommen der Nördlichen Grauwackenzone liegen innerhalb von Deckengrenzen. Modellberechnungen zeigen, daß ein inverser Temperaturgradient sich nur dann an der Basis von Decken einstellen kann, wenn die Überschiebungsgeschwindigkeit so groß wird, daß sie geologisch unglaubwürdig ist. Deckenüberschiebungen erzeugen aber in jedem Fall in der überschobenen Einheit einen zur Deckenfront hin gerichteten Fluidstrom. Eine Betrachtung der Stabilitätsdaten für Magnesit und Dolomit im Gleichgewicht mit einer fluiden Phase mit unterschiedlichen Ca/(Ca+Mg)-Verhältnissen zeigt, daß durch einen solchen Fluidstrom metasomatisch Magnesit aus Dolomit gebildet werden kann.

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Résumé Les dépôts de magnésite spathique de la Grauwacken Zone septentrionale sont situés à la base d'unités charriées. Un calcul de modélisation et des exemples naturels montrent qu'un gradient inverse de température ne peut s'établir à la base d'une unité charriée qu'à la condition d'admettre une vitesse de charriage tellement élevée qu'elle est irréaliste. D'autre part, le phénomene de charriage induit un déplacement de fluide depuis les unités inférieures vers le front de la nappe. Les données relatives aux conditions de stabilité de la magnésite et de la dolomite en présence de fluides de divers rapports Ca/Ca+Mg permettent de déduire que le flux ainsi engendré par la tectonique peut engendrer la magnésite par métasomatose à partir de dolomite préexistante.

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. , , , , . . , Ca/(Ca+Mg) , , , , , , - .

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Evaluation of the recharge processes and impacts of irrigation on groundwater using CFCs and radiogenic isotopes in the Silao-Romita basin, Mexico     

Axel Horst  Jürgen Mahlknecht  Broder J. Merkel  Ramon Aravena  Yann R. Ramos-Arroyo 《Hydrogeology Journal》2008,16(8):1601-1614

The recharge processes in the overexploited aquifer of the Silao Romita basin, central Mexico, were investigated by means of gaseous tracers (chlorofluorocarbons, CFCs) and radioactive isotopes (C-14, tritium). CFC concentrations varied between 0.06 and 12 pmol/l (CFC-11), 0.03 and 1.7 pmol/l (CFC-12), and <0.01 and 0.23 pmol/l (CFC-113). CFC concentrations are controlled by irrigation return flow which became apparent by the comparison with tritium. Tritium activities ranged from 0 to 3.5 TU. The calculated mean residence times of 70 to more than 300 years are considerably lower than the ages estimated based on the CFCs data. These data showed that CFCs were not appropriate for groundwater dating in this particular area but the CFCs were suitable as a qualitative measure of the magnitude of irrigation return flow which proved to be a significant source of recharge in the irrigated areas. Radiocarbon activities were in the range of 6–109 pmC. Carbon-13 values varied between –11.9 and –7.2‰ VPDB. Modelling of carbon isotopes with NETPATH along a plausible flow path reveals considerable influences of exchange with soil CO₂ and carbonate dissolution. Radiocarbon data indicate, at least in one case, the existence of groundwaters with residence times of more than 10,000 years.  相似文献   

Methane emission measurements in urban areas in Eastern Germany     

Joanne H. Shorter  J. Barry Mcmanus  Charles E. Kolb  Eugene J. Allwine  Brian K. Lamb  Byard W. Mosher  Robert C. Harriss  Uwe Partchatka  Horst Fischer  Geoffrey W. Harris  Paul J. Crutzen  Hans-Josef Karbach 《Journal of Atmospheric Chemistry》1996,24(2):121-140

We have investigated methane emissions from urban sources in the former East Germany using innovative measurement techniques including a mobile real-time methane instrument and tracer release experiments. Anthropogenic and biogenic sources were studied with the emphasis on methane emissions from gas system sources, including urban distribution facilities and a production plant. Methane fluxes from pressure regulating stations ranged from 0.006 to 24. l/min. Emissions from diffuse sources in urban areas were also measured with concentration maps and whole city flux experiments. The area fluxes of the two towns studied were 0.37 and 1.9 g/m²/s. The emissions from individual gas system stations and total town emissions of this study are comparable to results of similar sites examined in the United States.  相似文献   

On the collisional energy transfer between the constituents of the coronal plasma     

Horst Fichtner  Norbert Vormbrock  S. Ranga Sreenivasan 《Solar physics》1995,160(1):105-120

It has been suggested that the distribution functions characterizing the constituents of the solar coronal plasma are non-Maxwellian. If so, an accurate treatment of the collisional momentum and energy exchange between the plasma constituents within the framework of hydrodynamic models requires a re-evaluation of the general transfer integrals in multi-component plasmas. We have evaluated these integrals numerically for both Maxwellian and non-Maxwellian distribution functions of the plasma species avoiding the standard approximation for the collision cross sections frequently employed in the literature. Significant differences are shown to exist in the energy exchange rates for different distributions. We also demonstrate the inadequacy of the assumption of thermodynamic equilibrium in the innermost solar wind and reveal the importance of an accurate evaluation of the transfer integrals for the solar coronal plasma based on more realistic velocity distributions.Presented at the CESRA-Workshop on Coronal Magnetic Energy Release at Caputh near Potsdam in May 1994.  相似文献   

Geomagnetische Induktionspfeile in der ČSSR,Hervorgerufen durch Grossräumige Elektrische Leitfähigkeitsstrukturen     

Horst Wiese 《Studia Geophysica et Geodaetica》1965,9(4):415-419

Резюме Значительные раэности электропроводности в горизонтальном направлении заставляют индуцируемые ионосферными временными вариациями электрические токи в подстиляющих слоях протекать по преимущественным направлениям. В статье представляются вызванные этим вариации вертикальной и горизонтальной составляющих для периодов 19–40 мун в 20 пунктах в ЧССР, где регистрировались магнитные вариации при помощи полевых регистрирующих станций.

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Mitteilung Nr. 194 des Geomagnetischen Instituts Potsdam.  相似文献