www.geologicacarpathica.sk
GEOLOGICA CARPATHICA, AUGUST 2009, 60, 4, 331—338 doi: 10.2478/v10096-009-0024-1
Microseismic identification of geological and tectonic
structures in the Komjatice Depression
(Western Carpathians)
ANNA V. KALININA
1
, SERGEY M. AMMOSOV
1
, VIKTOR A. VOLKOV
1
, NIKOLAY V. VOLKOV
1
,
JOZEF HÓK
2
, LADISLAV BRIMICH
3*
and MARTIN ŠUJAN
4
1
Institute of Physics of the Earth, Russian Academy of Sciences, B. Gruzinskaya 10, 123995 Moscow, Russia
2
Department Geology and Paleontology, Faculty of Natural Sciences, Comenius University, Mlynská dolina, 842 15 Bratislava,
Slovak Republic; hok@fns.uniba.sk
3
Geophysical Institute, Slovak Academy of Sciences, Dúbravská cesta, 845 28 Bratislava, Slovak Republic;
*
geofbrim@savba.sk
4
EQUIS Ltd., Račianska 57, 831 02 Bratislava, Slovak Republic
(Manuscript received July 24, 2008; accepted in revised form December 18, 2008)
Abstract: The microseismic survey method was applied to the study of the geological structures in the region around
the Mochovce nuclear power plant. The previous geological and geophysical investigations considered a contact be-
tween the Miocene volcanites and sediments as a neotectonic fault. The results of the microseismic investigations allow
us to interpret the zone of a supposed neotectonic fault as a transgressive contact of the sediments and the volcanic rocks
without a tectonic disruption.
Key words: Miocene, Western Carpathians, geological structure, microseismic survey, Rayleigh waves, microseisms.
Introduction
The Western Carpathians form a mountain range arc with
dominant nappe structures with a significant zonal arrange-
ment and orogen polarity processes migrating in time. It is
one of the essential reasons dividing the Western Car-
pathians into the Outer Western Carpathians (OWC) and the
Inner Western Carpathians (IWC). One of the typical mor-
photectonic features of the IWC are Neogene depressions
and volcanites. The investigated area belongs to the Ko-
mjatice Depression which is a north-eastern part of the
Danube Basin. Numerous studies focused on the geological
and tectonic structures of the Komjatice Depression in the
past (e.g. Gaža & Beihauerová 1976; Zbořil et al. 1987;
Harčár & Priechodská 1988; Priechodská & Harčár 1988;
Baráth & Kováč 1995; Nagy et al. 1998; Hók et al. 1999).
Detailed geological and tectonic studies were realized in the
vicinity of the Mochovce nuclear power plant (EMO) situat-
ed at the easternmost margin of the Komjatice Depression. In
the EMO vicinity a conspicuous contact was described be-
tween the Miocene volcanics and sediments. This contact is
situated on the eastern foothill of the Dobrica elevation
(Fig. 1). From the point of view of the conservative solution
approach the contact was interpreted as a neotectonic fault
with potential Quaternary activity (Hók et al. 2003). The
fault separates the Miocene volcanites from the Quaternary
and Miocene sediments. The application of the microseismic
survey method yielded new information, which helped to
specify the geological and tectonic structures, as well as a
supposed fault-like contact in the EMO vicinity, which is lo-
cated in the NE part of Komjatice Depression.
Geological setting
Miocene sediments of the Komjatice Depression overlay
an erosive divided pre-Tertiary substratum drilled in several
boreholes (Biela 1978) and rising up in the Tribeč Mts
(Fig. 1). The stratigraphic range of Neogene sediments is
Middle Badenian (Middle Miocene) to Pliocene. The sedi-
mentary fill of the Komjatice Depression during the Miocene
megacycle was characterized by a gradual decrease of salini-
ty of the depositional environment upward. There are three
lower-order shallowing upward cycles in sedimentary
record. The depositional environment changed from marine
to brackish, caspibrackish and lacustrine-swamp with coal
deposition. This succession is overlain by a Pliocene cycle,
composed of deltaic and fluvial deposits (Hók et al. 1999).
The occurrence of the Middle Badenian sediments (the Poz-
ba Formation) is restricted to the central part of the depres-
sion. The Sarmatian sediments (Vráble Formation) are
transgressively spread over the whole depression. The Vráble
Formation comprises calcareous clays, sands and conglomer-
ates with volcanic rocks at the bottom. The volcanic rocks
form subaquaceous lava flows, which belong to the distal
parts of the Štiavnica stratovolcano rock complexes (the Prie-
sil Formation sensu Konečný et al. 1998). The paleocurrents
of the lava flows were generally oriented in a NE—SW direc-
tion in the investigated area. Sediments of the Vráble Forma-
tion, biostratigraphically constrained to the Sarmatian
period, were found in the parametric borehole ŠVM-1 drilled
about 5 km SW from the investigated area (Sliva in Hók et
al. 2003). The Lower Sarmatian sediments of the Vráble For-
mation are situated directly above the volcanic lava flows.
332
KALININA, AMMOSOV, V.A. VOLKOV, N.V. VOLKOV, HÓK, BRIMICH and ŠUJAN
Fig. 1. Simplified geological map of the Komjatice Depression and the investigated area (according to Nagy in Hók et al. 2003).
333
MICROSEISMIC IDENTIFICATION OF GEOLOGICAL STRUCTURES (WESTERN CARPATHIANS)
The Pannonian sediments of the Ivánka Formation overlay
the Vráble Formation. The angular unconformity is present
between the Ivánka and the Vráble Formations. The Ivánka
Formation sediments are predominantly represented by cal-
careous clays and claystones with admixture of sands repre-
senting fluvial influence in sedimentary basin. The Beladice
Formation (Pontian) is the last member of the Miocene mega-
cycle sedimentation. It was deposited in a shallow lacustrine
to swamp environment. The variegated clays with coal inter-
calations are typical for the Beladice Formation. The Pliocene
sediments (the Volkovce and Kolárovo Formations) are prod-
ucts of the deltaic sedimentation. The most typical sediments
are coarse-grained gravels and sands with clay admixture.
The northeast trending faults are most remarkable in the
tectonic structures of the Komjatice Depression. The brittle
structures of the Mojmírovce and Šurany fault systems were
the most important of the faults activated during the devel-
opment of the Komjatice Depression (Hók et al. 1999). The
Mojmírovce fault system bounds the Miocene deposits with
the pre-Tertiary rocks of the Tribeč Mts. The Šurany fault
system is a comparative, partly antithetic fault system rela-
tive to the Mojmírovce fault system. It restrains the southeast
and east margin of the Komjatice Depression depositional
area and also the horst-like structure of the neovolcanic
rocks comprising the Kozmálovské vŕšky Hills. We assume
that the Mojmírovce and Šurany fault was active during the
initial rifting of the Komjatice Depression and the rifting was
connected with the Pozba Formation, deposition (cf. Hók et
al. 1999). The paleostress field with NW—SE oriented exten-
sion accompanying subsidence of the depression and deposi-
tion of the Vráble Formation, during the Sarmatian period.
The transgressive characteristic of deposits and modelling
suggest a moderate subsidence during this period (Lankreijer
et al. 1995). The next phase of a wide rifting manifests the
angular unconformity between the Sarmatian and Pannonian
sediments (the Vráble and Ivánka Formations). The Late
Miocene paleostress field, with a NE—SW to ENE—WSW
compression and perpendicularly oriented extension result-
ing in following subsidence of the depression. Deposition
during the Pannonian and Pontian suggests a rapid transition
of the synrift stage evolution to final thermal subsidence
(postrift stage) of the whole Danube Basin.
The Pliocene Volkovce Formation deposits, reaching up to
1000 m in thickness toward the Danube Basin centre (Baráth
& Kováč 1995) points to a rejuvenation of the tectonic activi-
ty. However, the end of the Pliocene and the beginning of the
Quaternary represents structural reworking of the Komjatice
Depression during the period of tectonic inversion. The cen-
tral part of the depression between the Tribeč Mts and the
Kozmálovské vŕšky Hills is characterized by uplift resulting in
erosion of older sediments (Priechodská & Harčár 1988).
The area southeast of the Kozmálovské vŕšky Hills has
been subsiding since the Mindelian. This is shown by the age
of the oldest preserved terrace of the Hron River (Halouzka
1968), as well as by the 40 m thick accumulations of Quater-
nary sediments (Tkáč et al. 1996). It was one of the reasons
why the sharp contact between the volcanics and the Mio-
cene sediments was interpreted as a fault structure with po-
tential activity during the Quaternary.
Methodology
Seismic background oscillations (microseisms) have been
studied for more than a hundred years. Recently many investi-
gations were devoted to developing methods using mi-
croseisms as sounding signals. Microseismic signals are
always present at every point on the Earth’s surface eliminat-
ing the necessity of artificial sources of registered signals. A
number of experiments demonstrate the relations between the
amplitude-frequency characteristic of the microseisms and the
elastic properties of the medium (Bard 1999).
The approaches utilizing microseisms for the study of the
geological environment could be approximately divided into
two groups. The first group studies the experimental disper-
sion dependencies between microseismic wave velocities
and corresponding frequencies. The main purpose of these
measurements consists of receiving the velocity section of
the investigated area after the inverse problem solution on
the basis of the experimental dispersion curves. This ap-
proach requires synchronous measurements with the help of
seismic arrays of different configurations (Shapiro & Ritz-
woller 2002). The second group studies the composition of
the correlation of stable statistical properties of the mi-
croseismic field and the structure of geological heterogene-
ities (Asten 1978; Nakamura 1989). In that case, the
measurements could be performed using a single seismic sta-
tion. But in practice a number of assumptions regarding the
nature of the microseisms sources, their spectral properties,
and the proportion of the content of different types of waves
are accepted based on previous experimental investigations,
both in the study area and in other regions. This group is
characterized by the simplicity of measurement procedures
and good consistency of microseismic investigation results
with other geological and geophysical methods despite the
set of initial assumptions.
The microseismic signal looks like interference by differ-
ent types of seismic waves, which propagate as separate
wave trains of limited duration, and which present the deter-
ministic signals within this duration. From the other side, the
microseismic signal is a random signal, because the propor-
tion of the content of waves of different type, initial phases,
amplitudes, and duration of wave trains are unknown. As an
illustration of the randomness of the process X(t), the follow-
ing example could be used:
X(t) = A cos (
ωt + ϕ),
where
Α and ω are constants, and ϕ is a random value with
defined probability distribution, so that for one realization
the random value
ϕ is equal for all values of t (for example
for the time interval of observation). In that case the random
variations take place only on the realization ensemble, but
not on time intervals.
The method of microseismic survey, where the spatial
properties of the spectral characteristics are used for the loca-
tion of the geological heterogeneities (Gorbatikov et al.
2004; Ammosov et al. 2007), was applied. This method
could be referred to as a statistical approach. The measure-
ments above the investigated structures were performed us-
334
KALININA, AMMOSOV, V.A. VOLKOV, N.V. VOLKOV, HÓK, BRIMICH and ŠUJAN
ing separate mobile station (one or several units). For proper
interpretation of the received data we shall ensure that the re-
sulting values are stationary and do not vary during the day,
month, and do not depend on changing climatic conditions,
etc. The estimation of the stationary interval of the signal
dispersion in the increasing temporal window takes into ac-
count the known dependence between the spectrum and the
dispersion of a random signal:
where
σ
x
2
and S
x
(f) are dispersion, and spectral density
correspondingly of the random microseismic process (Ben-
dat & Piersol 1966). The experimental investigations of the
stationarity of intervals of the microseisms for different lo-
calities and different conditions on the Earth’s surface
showed that the signal dispersion begins to stabilize after the
signal accumulation during 15—20 minutes for the frequency
range 10—12 Hz and during 40—60 minutes for the frequency
range 0.1—1.0 Hz (Gorbatikov & Stepanova 2008). It is nec-
essary to notice that the stationary interval is limited. More-
over the time is changing for different frequency ranges and
for different observation conditions. To separate the global
and local microseismic sources during the measurements, it
is necessary to install one seismic station (reference station)
for continuous recording of the microseismic signal in the
vicinity of the investigated area.
Physical background of the microseismic survey
method
The microseismic survey method is based on the analysis
of the spatial distribution of the vertical component of the
microseismic field for all frequencies of the spectra. The an-
alytical solutions proved that in the Rayleigh fundamental
mode the zone of maximum shear stresses is located at the
depth equal to half of their wave length. The zones of maxi-
mum amplitudes are situated close to the surface. The local
heterogeneities with different elastic modules lead to chang-
es of the oscillation character of the microseism and their
amplitudes. If seismic wave velocities in the heterogeneities
are higher than in the surrounding rocks the amplitude of the
microseismic waves above the heterogeneities decreases, and
vice versa (Gorbatikov et al. 2004; Kalinina et al. 2008).
The observations were performed at different points with
the step 100 m in the investigated area using mobile stations.
During processing the field data were corrected using the ref-
erence station data records. The results of the analysis are
maps of the distribution of microseismic amplitudes reflect-
ing the fields of the relative velocity changes for different
frequencies. The dependence of the Rayleigh wave ampli-
tudes on the depth of the half-space is given in (Levshin et
al. 1992). The maps of the distribution of microseismic am-
plitude for different frequencies give information about the
velocity properties of the medium at different depths.
It was necessary to check the following circumstances dur-
ing processing:
1. Type of waves dominated in registered signal;
2. Statistical stability of the registered parameters.
The main assumption of the microseismic survey method
is the prevalence of the Rayleigh-type waves in the vertical
component of the low frequency (lower than 1 Hz) mi-
croseismic field. However, our working frequency band also
lies in the high frequency area, which contains a high per-
centage of body waves. The wave composition using the po-
larized analysis of the particle movement was studied, and it
was necessary to preprocess the data to remove the high am-
plitude noises (mainly the noises caused by transportation).
The control of statistical stability was realized by the inves-
tigation of the behaviour of the signal dispersion in the in-
creasing temporal window for each observation point. During
processing the data were corrected using the reference station
records, and the ratio of accumulated (stationary) power spec-
tra was obtained. The pictorial representations of the resulting
matrix are the horizontal and vertical slices at any chosen site.
Processing and results
The investigated area represented a rectangle with the size
approximately 0.5 by 2.2 km (Fig. 2). The measurements
were realized along six profiles 100 m apart. The average
distance between points of registration along the profiles was
100 m. Close to the contact zone between volcanites and
sediments near the Dobrica Hill the registration points were
denser (25—50 m). For the continuous registration the refer-
ence station was installed in the center of the studied area.
The registration time interval for mobile stations at each
point was 45—50 min. The seismic station consisted of the
three-component velocimeter KMV and a registration block
UGRA (Marchenkov et al. 1997).
The main goal of the processing was the gathering and
analysis of the power spectra. In Fig. 3 the observed smooth-
ing power spectra of microseisms along profile 3 are shown.
The results of the microseismic survey are presented as verti-
cal profiles and horizontal layers (Figs. 4 and 5). The axes
are given in meters. The XY projection is UTM Zone 34
Northern Hemisphere (WGS 84). The zero depth on the ver-
tical axis corresponds to the level located at the absolute
mark equal to 200 m. The colour spectrum reflects the inten-
sity of the relative amplitude of the microseisms in decibels.
The microseismic survey method allows us to distinguish
rocks by velocity properties. It was meaningful to assume
that at least two types of lithological rocks – the Miocene
volcanites (intensity of the relative amplitude of the mi-
croseisms lg A < —2 dB ) and the Miocene and Pliocene sedi-
ments (lg A > 2 dB) – could appear in the resulting maps.
The vertical profiles and horizontal layers presented in
Figs. 4 and 5 exhibit the following characteristic features of
the investigated area:
1. The zones of low amplitudes lg A < —2 dB (blue colour)
interpreted as volcanic rocks are well distinguished down to
600—650 m. The sediments lg A > 2 dB (red colour) are lo-
cated between them.
2. The bottom stratum, —2 dB < lg A < 0 dB, (green co-
lour) has velocity properties, which are nearly average be-
335
MICROSEISMIC IDENTIFICATION OF GEOLOGICAL STRUCTURES (WESTERN CARPATHIANS)
Fig. 2. The map of study area with points of observations (the positions of observation points indicated as red triangles, the position of base
station – as a yellow star).
Fig. 3. The observed smoothing power spectra of microseisms along the profile 3.
336
KALININA, AMMOSOV, V.A. VOLKOV, N.V. VOLKOV, HÓK, BRIMICH and ŠUJAN
Fig. 4. The variations of spectral amplitudes of microseismic signals of investigated media volume; (a) the relief map with points of obser-
vations, the dashed lines show the positions of vertical sections presented on the maps (b—f).
tween volcanites and sediments; it looks homogeneous
enough and this hinders the identification of any fault fea-
tures there.
3. In the upper part of profiles 4 and 5 it is possible to dis-
tinguish the difference of sediment velocities, —2 dB < lg A
< 0 dB and by A > 0, (the green colour above the red one).
The more contrasting zones are displayed separately in Fig. 6
as isosurfaces bounding the difference values of microseismic
amplitudes. In Fig. 6a the isosurface bounds the high amplitudes
area (
Α > 9 dB), which corresponds to a low velocities area (the
sedimentary deposits). In Fig. 6b the volcanic rocks are present-
ed, their velocity properties increase (amplitudes of microseisms
decrease A < —2 dB). This figure allows us to investigate the
range of the softening and weathering of the volcanics.
The interpretation of the geophysical data shows two dif-
ferent horizons in the geological structure in the EMO vicini-
ty (Figs. 4, 5). The lower horizon could be interpreted as the
pre-Tertiary basement rocks (green colour). The upper hori-
zon represents the Miocene volcanites and sediments be-
tween them. The Miocene volcanic rocks (blue colour) are
337
MICROSEISMIC IDENTIFICATION OF GEOLOGICAL STRUCTURES (WESTERN CARPATHIANS)
Fig. 6. The isosurfaces bounding the different values of amplitudes; a – the isosurface bounding the high amplitudes area of microseisms
which correspond to the low velocities area (the sedimentary deposits); b – the isosurfaces bounding the different isovalues which corre-
spond to the high velocities area (volcanic deposits).
Fig. 5. The maps of spectral amplitude varia-
tions of microseismic signals for different cho-
sen depths.
338
KALININA, AMMOSOV, V.A. VOLKOV, N.V. VOLKOV, HÓK, BRIMICH and ŠUJAN
remnants of lava flows. The lava flows are situated directly
over the pre-Tertiary basement rocks. A similar situation is
described at borehole GK-6 drilled about 10 km NE from the
investigated area (Biela 1978). The Miocene and the
Pliocene sediments (red colour) are placed partly on the pre-
Tertiary basement rocks, partly on the volcanic lava flows.
This arrangement is in good agreement with the lithological
and sedimentological character of the Vráble Formation.
Between the Miocene volcanites and the sediments a nor-
mal fault (Fig. 2) was formerly supposed, separating the vol-
canites from the sediments at the east foothill of the Dobrica
elevation (Hók et al. 1999). The interpretation of the mi-
croseismic investigation results did not prove a fault contact
between the volcanites and the sediments. This result is also
supported by no existence of adequate offset along the sup-
posed fault in the pre-Tertiary basement (see Fig. 4).
Due to the above mentioned facts, it is possible to interpret
this structure as the transgressive contact of the sediments
overlaying the volcanic lava flows.
Conclusions
The interpretation of the geophysical investigation results
allows us to recognize two floors in the geological structure in
the EMO vicinity. The lower horizon contains the pre-Tertiary
rock sequence. The upper horizon belongs to the transgressive
formation of the Miocene volcano-sedimentary sequence. Ac-
cording to previous investigations (e.g. Priechodská & Harčár
1988; Hók et al. 1995) the upper horizon represents the
Vráble Formation. The uppermost part of this horizon most
probably belongs to the Volkovce Formation (e.g. Baráth &
Kováč 1995). The results of the geophysical investigation
show a transgressive contact without a tectonic disruption
(fault) between the volcanic rocks and the sediments at the
eastern foothill of the Dobrica elevation.
Acknowledgment: This work was supported by the Slovak
Research and Development Agency under the contract
No. APVV-0158-06, APVT-51-002804 and by VEGA Grant
Agency under Projects No. 2/0107/09, No. 1/0461/09.
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