Assessment of seismic hazard for the Sannio-Matese area of Southern Italy — A summary

The working group on Test Regions for Evaluation of Methods for Seismic Hazard Assessment in Europe (TERESA), consisted of 15 members from 10 different European countries. Methods and experience gathered in these countries have been compared and discussed for two test areas in Europe: the Sannio-Matese region, Southern Italy, with high seismic activity, and the border region between Belgium, The Netherlands, and Federal Republic of Germany, with low activity.This paper summarizes the results for one of the test areas, Sannio-Matese. Most of the participants used statistical procedures to assess earthquake hazard, receiving results in terms of probability of occurrence for intensity as the ground-motion parameter. It was found that careful preparation of input data and parameters is the major influencing factor, therefore most of the efforts of the working group was devoted to this task.The scatter of the obtained results of the group is considerable, mainly because of the uncertainties in the data and the subjectiveness involved in the procedures. For better control of both factors, more objective methods have to be developed.     

Seismic hazard computations for regions with low earthquake activity — A case study for the Belgium,The Netherlands and NW Germany area

The algorithms to evaluate seismic hazard, used and/or developed by five teams participating in the TERESA project, applied to the low seismicity area Belgium, The Netherlands and NW Germany are compared. The main differences in the results can be explained by the majority criterion of Egozcue et al. (1989), the differences in the upper bound and zonification and, in some cases, by a higher attenuation.     

Infrared estimates of aliphatic kerogen carbon in sedimentary rocks

An infrared routine has been developed to estimate the aliphatic portion of kerogen carbon in sedimentary rocks. The procedure does not require isolation of the organic matter and is based on a computer-assisted determination of global band areas in the region of the aliphatic carbon-hydrogen stretching vibrations around 2900cm⁻¹. From these integrated absorptions the amount of aliphatic carbon C_al (mg of aliphatic carbon per gram of solvent-extracted rock) is calculated by means of a calibration with model rocks. Carbonate overtones which interfere in the case of limestones are eliminated by comparison to a CaCO₃ standard.The method has been applied to rocks containing kerogens of different types and maturities at TOC levels of 0.5 to 12%. The aliphatic carbon concentrations range from 0.5 to 60mg·g⁻¹ and correlate reasonably well with the residual genetic potentials of the rocks as measured by S₂ values from Rock-Eval pyrolysis. The ratio S₂/C_al is found to decrease with burial depth reflecting a maturity enhanced conversion of aliphatic carbon to fixed aromatic carbon under Rock-Eval conditions.     

Seismotectonic scheme of Central and Eastern Europe

Summary The distribution of earthquake foci in the crust and the upper mantle indicates the position of mobile zones. Comparing epicentral maps of Central and Eastern Europe, known tectonic lines, results of deep seismic sounding and gravimetric survey enables a scheme of potential seismogenic zones, which correspond to active fault zones separating plates and blocks in the area, to be compiled. The level of earthquake activity varies along the investigated boundaries and can be considered as a measure of the intensity of the present geodynamic processes.Paper presented at the joint symposium AlO of the XVIIth General Assembly of the European Seismological Commission and of the 7th Annual Meeting of the European Geophysical Society, Budapest (Hungary), Aug. 21. – 29., 1980.     

Time pattern of large earthquake sequences in Europe in 1976–1979

Summary The time development of three large sequences, Friuli 1976, Thessaloniki 1978 and Monte Negro-Albania 1979, was investigated by analysing the characteristics of the time distribution of magnitudes of the events, M(t), of average magnitudes, (t), and of the number of events, n(t), as well as the strain release curves and the magnitude-frequency relations, N(M). The existence of time gaps and of an anomalous decay of the numbers of shocks before major events, as well as the oscillation of ( const b^–1) may be considered as precursory phenomena. The clustering of events has been tested by the Poisson and negative binomial laws.Communication presented at the XVIIth General Assembly of the European Seismological Commission in Budapest, 21–29 August, 1980 under the title Properties of Seismic Regime and Recent Earthquake Sequences in Europe.     

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Eine pleistozäne Rutschung bei Kitzbühel/Tirol

ZusammenfassungEine pleistozäne Rutschung bei Kitzbühel/Tirol Bei einem Grabenaushub wurden in Grundmoräne zwei fossile Rutschkörper festgestellt. Ein Beispiel wird anhand von alten Bewegungsstrukturen beschrieben, die durch Oxydationsstreifen abgebildet wurden. Nach dem Geländeschnitt rissen z. T. die alten Schwächestellen infolge geringer Abweichungen der Scherfestigkeit des Materials wieder auf.

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SummaryA Pleistocene Landslide near Kitzbühel/Tyrol During excavation of a ditch two fossil landslides have been ascertained. One example is described the structures of which are copied by oxide bands. After excavating the old joints have opened again.

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RésuméUn glissement pléistocène près de Kitzbühel/Tyrol Pendant l'excavation d'un fossé deux glissements fossiles étaient constatés dans la moraine. Un glissement est décrit dont les structures sont illustrées par bandes d'oxydes. Les observations ont demontré que les fissures vieilles se sont ouvertes après l'excavation.

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Mit 1 Abbildung     

Synchronous uplift of the lower crust of the Ivrea Zone and of Southern Calabria and its possible consequences for the Hercynian orogeny in Southern Europe

Along the border of the Adriatic microplate, pre-Alpine granulite-facies rocks from the deepest crust are outcropping at only two places: in the Ivrea Zone of the Southern Alps and in Southern Calabria. In these two areas the main features of the present crustal structures, i.e. overlapping of large continental crustal and upper mantle segments, are interpreted as resulting from their Hercynian geodynamic evolutions.The tilted, nearly complete crustal sections in both areas display very similar lithological sequences and experienced a common geological evolution, as deduced from petrological and radiometric dates. At the end of Hercynian time (～295 m.y.), the Ivrea body and the lower crustal rocks of Southern Calabria were contemporaneously sheared off from the upper mantle and uplifted into intermediate crustal levels, where they slowly cooled during Mesozoic time. The tectonic uplift was accompanied by granitoid plutonism and andesitic to rhyolitic volcanism, which continued after the Hercynian uplift.Considering the presently similar crustal structures and the Upper Carboniferous and Permian geological evolutions along the whole Adriatic plate boundary, the Ivrea Zone and Southern Calabria are used to resolve the pre-Alpine history of the boundary zone between the Adriatic and the Central European block: the uplift of the lower crustal/upper mantle flakes of the Adriatic block was due to flat overthrusting of these flakes on the continental crust of “Central Europe”. The material of the Central European crust underthrust (subducted) thereby melted during the re-equilibration of the geotherms which had been disturbed by the subduction process; this led to an extensive calc-alkaline plutonism and volcanism of crustal origin along the Adria boundary. In this boundary region, the overlying uppermost crustal levels (“Schiefergebirgsstockwerk”) were synchronously folded (“Asturian phase”) in response to the overlapping of the deeper crustal levels. Subsequently to the orogeny, the mountain chain was eroded and molasse basins developed on the overthrust Adriatic crustal segment during the Lower Permian.In this model, the granulite-facies flakes of the Ivrea Zone and of Southern Calabria are interpreted as pre-Hercynian lower crustal segments which were thrust into the middle crust during the Hercynian orogeny, thus giving rise to wave velocity inversions in the crust. Further, it is proposed that similar geodynamic processes have played a role in the genesis of the Conrad discontinuity which is present in many parts of the Hercynian fold belt. But only in the Ivrea Zone and in Southern Calabria the crustal discontinuities formed in Hercynian time were uplifted to the surface as a result of Alpine reactivation of the Adriatic boundary zone and due to their special positions in the bends of the Alpine-Apennine-Maghrebide mountain system.According to the present knowledge of the Carboniferous paleogeography and of the orogenic evolution on both sides of the Adria sufure zone, this fault zone was located within the European continent. Its role during the Hercynian orogeny is discussed envisaging two possibilities: an A-subduction zone or a subfluence zone (in the sense of Behr and Weber).     

Large impact features on middle-sized icy satellites

All of the large impact features of the middle-sized icy satellites of Saturn and Uranus that were clearly observed by the Voyager spacecraft are described. New image mosaics and stereo-and-photoclinometrically-derived digital elevation models are presented. Landforms related to large impact features, such as secondary craters and possible antipodal effects are examined and evaluated. Of the large impacts, Odysseus on Tethys appears to have had the most profound effect on its “target” satellite of any of the impact features we examined. Our modeling suggests that the Odysseus impact may have caused the prompt formation of Ithaca Chasma, a belt of tectonic troughs that roughly follow a great circle normal to the center of Odysseus, although other hypotheses remain viable. We identify probable secondary cratering from Tirawa on Rhea. We attribute a number of converging coalescing crater chains on Rhea to a putative, possibly relatively fresh, ∼350 km-diameter impact feature. We examine the antipodes of Odysseus, the putative ∼350 km-diameter Rhean impact feature, and Tirawa, and conclude that evidence from Voyager data for damage from seismic focusing is equivocal, although our modeling results indicate that such damage may have occurred. We propose a number of observations and tests for Cassini that offer the opportunity to differentiate among the various explanations and speculations reviewed and evaluated in this study.