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The Vogtland, located at the border region between the Czech Republic and Germany, is known for Holocene volcanism, gas and fluid emissions as well as for reoccurring earthquake swarms, pointing towards a high geodynamic activity. During the earthquake swarm in 2008/2009, a temporary array was installed close to Rohrbach (Germany), at an epicentral distance of about 10 km from the Nový Kostel focal zone (aperture ~0.75 km).
22 events of the recorded swarm were selected to set up a source array. Source arrays are spatially clustered earthquakes, which can be used in a similar manner as receiver array recordings of single events (Green’s functions reciprocity). The application of array seismology techniques like beam forming requires similar waveforms and precisely known origin times and locations. The resemblance of waveforms was assured by visual selection of events and quantified with the calculation of cross-correlation coefficients. We observed that the different events recorded at a single station generally show greater resemblances than the recordings of one event at all stations of the receiver array. This indicates a heterogeneous subsurface beneath the receiver array and a comparably homogeneous source array volume with respect to the frequency-dependent resolution of both arrays.
Beam forming was applied on the Z, N and E component recordings of the source array events at 11 stations, and the results were analysed with respect to converted or reflected crustal phases. While the theoretical back azimuth of the direct phases match the beam forming results in case of the source array analysis, in case of receiver array beam forming derivations of 15°-25° are observed.
PS phases, closely following the direct P phase and presumably SP phases, arriving shortly before the direct S phase can be observed on several stations. Based on the time differences to the direct P and S phases we inferred a conversion depth of about 0.6-0.9 km. A second deeper source array was set up in order to interpret a structural phase arriving 0.85 s after the direct P phase on records of deeper events only.
Additionally to the source array beam forming method an analytical method with a fixed medium velocity and a grid search method, both for determining conversion/ reflection locations of phases traveling off the direct line between source and receiver array, were developed and applied to other observed phases.
In conclusion, we think that the distinct beam forming results along with the striking waveform resemblance reveal the opportunities of using source arrays consisting of small swarm events for the analysis of crustal structures.
Assuming that liquid iron alloy from the outer core interacts with the solid silicate-rich lower mantle the influence on the core-mantle reflected phase PcP is studied. If the core-mantle boundary is not a sharp discontinuity, this becomes apparent in the waveform and amplitude of PcP. Iron-silicate mixing would lead to regions of partial melting with higher density which in turn reduces the velocity of seismic waves. On the basis of the calculation and interpretation of short-period synthetic seismograms, using the reflectivity and Gauss Beam method, a model space is evaluated for these ultra-low velocity zones (ULVZs). The aim of this thesis is to analyse the behaviour of PcP between 10° and 40° source distance for such models using different velocity and density configurations. Furthermore, the resolution limits of seismic data are discussed. The influence of the assumed layer thickness, dominant source frequency and ULVZ topography are analysed. The Gräfenberg and NORSAR arrays are then used to investigate PcP from deep earthquakes and nuclear explosions. The seismic resolution of an ULVZ is limited both for velocity and density contrasts and layer thicknesses. Even a very thin global core-mantle transition zone (CMTZ), rather than a discrete boundary and also with strong impedance contrasts, seems possible: If no precursor is observable but the PcP_model /PcP_smooth amplitude reduction amounts to more than 10%, a very thin ULVZ of 5 km with a first-order discontinuity may exist. Otherwise, if amplitude reductions of less than 10% are obtained, this could indicate either a moderate, thin ULVZ or a gradient mantle-side CMTZ. Synthetic computations reveal notable amplitude variations as function of the distance and the impedance contrasts. Thereby a primary density effect in the very steep-angle range and a pronounced velocity dependency in the wide-angle region can be predicted. In view of the modelled findings, there is evidence for a 10 to 13.5 km thick ULVZ 600 km south-eastern of Moscow with a NW-SE extension of about 450 km. Here a single specific assumption about the velocity and density anomaly is not possible. This is in agreement with the synthetic results in which several models create similar amplitude-waveform characteristics. For example, a ULVZ model with contrasts of -5% VP , -15% VS and +5% density explain the measured PcP amplitudes. Moreover, below SW Finland and NNW of the Caspian Sea a CMB topography can be assumed. The amplitude measurements indicate a wavelength of 200 km and a height of 1 km topography, previously also shown in the study by Kampfmann and Müller (1989). Better constraints might be provided by a joined analysis of seismological data, mineralogical experiments and geodynamic modelling.