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Tectonophysics 410
Soft-sediment deformation structures in Late Miocene–Pleistocene
sediments on the pediment of the Matra Hills (Visonta, Atkar,
Verseg): Cryoturbation, load structures or seismites?
Zoltan Horvath a,*, Erika Micheli b,1, Andrea Mindszenty a,2, Judit Berenyi-Uveges c,3
a Department of Applied and Environmental Geology, Eotvos Lorand University, H-1117 Budapest, Pazmany Peter s. 1/C, room: 710, Hungaryb Department of Soil Science and Agricultural Chemistry, Szent Istvan University, H-2103 GodollI, Pater Karoly u. 1, Hungary
c Central Service for Plant Protection and Soil Conservation, H-1118 Budapest, Budaorsi ut 141–145, Hungary
Received 18 June 2003; accepted 18 August 2005
Available online 20 October 2005
Abstract
The studied area, built up by silty clayey and partly sandy sediments and paleosols, lies on the tectonically active Northern
margins of the Pannonian Basin. Wavy, sagging load casts can be observed in the upper part of the Late Miocene alluvial complex
and larger scale sagging load casts, flame structures, drops and pillows detected in its Quaternary cover were studied in detail, in
order to understand the origins of soft sediment deformation which characterized this young sedimentary suite. Sedimentological,
paleopedological and mineralogical observations suggest that:
1. One of the reasons for the soft-sediment deformation might have been the relatively low cohesive strength of the predominantly
smectitic sediment covering a gentle slope similar to the actual landscape.
2. On such a surface, the down-slope gravitational component of the mud-blanket might easily have been sufficient to overcome its
cohesive strength.
3. Frost action traceable in the studied formations might also have contributed to the observed deformation, particularly along the
eroded top of the Late Miocene sediments.
Combined evidence from field observations and laboratory analyses support the idea that liquefaction–fluidization was of
prime importance in bringing about the observed structures. In conclusion two alternative Quaternary/Holocene scenarios are
proposed, which might have resulted in the unusual behaviour of the sediments/paleosols. One is a seismic event, the other is
the combined effect of freeze–thaw cycles and of the sloping foothill position, which might have resulted in episodic downslope
transport and the associated deformation of the eroded soil material when its water content surpassed a certain threshold. We
accept that the anomalous abundance of soft-sediment deformation in this marginal position may be causally related to paleo-
earthquakes, but the obvious complexity of the phenomenon requires caution. In case the proposed scenarios would not have
0040-1951/$ - s
doi:10.1016/j.tec
* Correspondi
E-mail addr
BerenyiUveges.1 Tel.: +36 282 Tel.: +36 1 33 Tel.: +36 1 3
(2005) 81–95
ee front matter D 2005 Elsevier B.V. All rights reserved.
to.2005.08.012
ng author. Tel.: +36 1 381 2129 or +36 1 209 0555/1782; fax: +36 1 381 2130.
esses: [email protected] (Z. Horvath), [email protected] (E. Micheli), [email protected] (A. Mindszenty),
[email protected] (J. Berenyi-Uveges).
410 200/1812 or 1809.
81 2129 or +36 1 209 0555/1789; fax: +36 1 381 2130.
09 1047; fax: +36 1 246 2962.
Z. Horvath et al. / Tectonophysics 410 (2005) 81–9582
been alternatives but acted simultaneously, the analysed phenomena were to be interpreted as the joint results of tectonics and
climate change.
D 2005 Elsevier B.V. All rights reserved.
Keywords: Soft-sediment deformation; Pannonian basin; Late Miocene; Quaternary; Environmental change; Frost; Seismites; Calcrete
1. Introduction
There is a general consensus about the study and
interpretation of soft-sediment deformation structures
being helpful in paleoenvironmental reconstructions.
The target of the present paper is the description and
tentative interpretation of a set of unusual structures
observed in Late Miocene (Upper Pannonian)—partly
lignitiferous—alluvial sediments and their Quaternary
cover which is a pedo-sedimentary complex. The struc-
tures suggest that the soil-complex may have been
subject to soft-sediment deformation triggered either
by seismic shock-related sudden pore-pressure increase
or by frost-and-thaw induced instability on a gentle
slope. In order to decide which one of the possible
mechanisms was predominant, field and laboratory
data were collected, evaluated and combined with the
available general geological and paleoclimatological
evidence.
1.1. Soft-sediment deformation structures
Soft-sediment deformation is a general term for
altering the fabric and layering of a bed of unconsoli-
dated sediments (Ricci-Lucci and Amorosi, 2003). It
affects most commonly multilayer deposits, especially
sand-clay alternations, and can be diffused through the
whole packet or concentrated along bedding planes or
individual beds. Terms for soft-sediment deformations
in modern and ancient sediments were reviewed by
Ricci-Lucci and Amorosi (2003).
Generally it is accepted that soft-sediment deforma-
tion structures may form when the sediment has low or
zero shear resistance. This natural condition may result
in liquefaction–fluidization either in cohesionless sedi-
ments (Lowe, 1975, Allen, 1982, Owen, 1987, Alfaro
et al., 1997), or in cohesive fine sediments as a conse-
quence of smectitic clays reacting in water systems
(thixotropy, viscosity, plasticity, shrinkage). They are
determined by the individual structural features and the
type of the interlayer cation of smectites (Grim and
Guven, 1978). The driving mechanism for formation
of soft-sediment deformations is primarily pore–water
pressure in combination with liquefaction of sand-rich
sediment (Obermeier, 1996).
Pore–water pressure may increase as a result of
melting ice in the soil (Van Vliet-Lanoe, 1985, 1998).
Involutions are surficial manifestations of frost-related
stirring (cryoturbations) and are generally characterized
by distortion and mixing of the uppermost meters of the
ground (Obermeier, 1996). Load casting during melt-
ing, pressure-development in water trapped between
freezing fronts and pressures and heaving during freez-
ing could be correlated to the genesis of involutions
(Vandenberghe, 1988).
Seismic shock is another important liquefaction pro-
cess (e.g. Munson et al., 1995; Van Vliet-Lanoe et al.,
1997).
Obermeier (1996) called attention to features of
nonseismic or unknown origin (artesian flow, stream-
banks landslides, ground disturbance by trees, load
structures in muds, water escape structures in granular
sediments, etc.).
Swelling and shrinking in Vertisol type paleosols
(rich in smectitic clays) may generate wavy formations
which are usually called bmukkaraQ or bgilgaiQ (Paton,1974). Soft-sediment deformation (converging forms)
may be significantly enlarged due to differential swell-
ing and shrinking of clayey soils (Knight, 1980).
1.2. Tectonic framework
Subsidence and sedimentation in the greater part of
the Pannonian Basin were interrupted in the early Qua-
ternary; extensional basin formation had come to an end
and compressional inversion had started (Horvath and
Cloetingh, 1996). From that time on the Pannonian
lithosphere has been bent. As a result of increasing
intraplate stress, the peripheral areas of the basin expe-
rienced uplift, while subsidence of some of the internal
sectors accelerated (Fig. 1) (Bada et al., 1999).
According to earlier geomorphological analyses
(Franyo, 1982; Pecsi, 1992) and our latest observations
(Horvath et al., 2001) the Matra Hills could have been
uplifted at least 100–200 m from the beginnings of the
Quaternary. However taking into consideration the re-
cent vertical movement (average 1–2 mm/year uplift in
the hills and a subsidence of similar magnitude in the
basins after Joo, 1992) and the proven 1–1.5 km
Middle–Late Miocene and Pliocene paleoburial of the
Fig. 1. The studied Matra Foreland is situated on the Northern margins of the subsiding Great Hungarian Plains, in front of the uplifting Matra Hills
(modified after Horvath and Cloetingh, 1996).
Z. Horvath et al. / Tectonophysics 410 (2005) 81–95 83
adjacent tectonic Unit called Bukkium (Dunkl et al.,
1994; Dunkl and Frisch, 2002) permits to suppose that
the uplift of the Matra Hills during the Quaternary
might have been some hundred meters. In addition
the studied area is close to the Mid-Hungarian linea-
ment system (comprising the Vatta-Maklar line next to
the Matra Foreland), which has shown compressional
reactivations during Quaternary times (Csontos and
Nagymarosy, 1998). This geodynamic position has ob-
viously resulted in numerous earthquakes during the
Quaternary. In historical times more than 20,000 earth-
quakes were registered from 456 AD up to our days
which sometimes caused even substantial damage (Toth
et al., 2002).
1.3. Quaternary climatic change in the Carpathian
Basin
In the beginning of the Quaternary, cooling is trace-
able by the spread of the so called bArctotercierQ spe-cies and the gradual impoverishment of the flora. All
tropical genera almost fully disappeared from Europe
(Andreanszky, 1941; Jarai-Komlodi and Vida, 1983).
The rate of cooling, the duration of glacial periods and
the extension of ice-cover showed occasional and areal
diversity. In the Pleistocene, the Carpathian Basin was a
periglacial area without continuous ice-cover. Depen-
ding on the presence of the available moisture, ground-
water permafrost formed in patches. During the last
glaciation (about 20,000–18,000 year B.P.) the central
part of the Carpathian Basin (including Hungary) was
part of the area of discontinuous and sporadic perma-
frost (Frenzel et al., 1992).
Due to frost-action the slopes of mountainous areas
of Hungary are covered by periglacial sediments of
varying grain-size. According to Pinczes (1982) and
others, these sediments have evolved during Pleisto-
cene times. Cryoplanational processes resulted in a
number of characteristic degradational and depositional
forms: frost-riven cliffs and block fields (Csorba, 1982).
On the forelands of the Matra Hills latest research
has detected frost features on the eroded, uppermost
Z. Horvath et al. / Tectonophysics 410 (2005) 81–9584
part of the Late Miocene sediments (Horvath, 1999;
Horvath et al., 2002; Berenyi Uveges et al., 2003).
1.4. Geological history, geomorphology and soils
The studied area is situated at the Southern foothills
of the eroded remnants of the Miocene volcanic mas-
sif of the Matra Hills. It is part of the Neovolcanic
chain, along the northern boundary of the Great Plains
sector of the Neogene Pannonian Basin. Geomorpho-
logically, it forms a part of an ancient pediment con-
necting the surface of the uplifted mass of the Matra
Hills with the adjoining lowlands of the still partly
subsiding Great Hungarian Plains (Fig. 2). Volcanics
on this margin are covered by shallow marine to
terrestrial sediments (including lignite) deposited in
an alluvial depositional environment landward from
a prograding delta. This contributed to the filling up
of the basin in Late Miocene times (Csilling et al.,
1985).
Due to the growing relief and frequent changes in
climate the rate of sediment transport and erosion has
increased. A complex system of colluvial and alluvial
fans built up by gravels, sand, clay, red-clayey paleosol
and other paleosols were formed in the foreland of the
Matra Hills (Franyo, 1982; Kretzoi et al., 1982). Some
of the red paleosols were formed on the eroded and
reworked sediments originating in the Matra Hills
(Berenyi Uveges et al., 2002). Loess and bloess-likeQsediments of the Weichselian age also occur in this area
as vestiges of a once continuous loess-blanket (Fukoh,
Fig. 2. Simplified geological profile across the M
1999; Krolopp, 2002). The surface soils are Luvic
Chernozems (Micheli et al., 1999).
As a result of the intricate intergrowth of pristine
and pedogenically modified sediments with the paleo-
sols, the collective term bpedo-sedimentary complexQwas proposed for the entire Post Pannonian part of
the section (Horvath, 1999; Berenyi Uveges et al.,
2003).
1.5. The problems of the stratigraphy
The stratigraphy of the studied area is best known at
the Visonta site. However, the stratigraphy of the whole
Matra-Foreland is yet far from being understood, main-
ly because of the efficient coverage of the terrain by the
terrestrial alluvial fan systems.
Important key formations in the stratigraphy are
the red silty clays. Litho-, bio- and magnetostrati-
graphic data show that they formed in different per-
iods. The oldest one the bpurplish-red soilQ is of
Early Pleistocene age (Lower Villanyium). The
other one was formed probably in the Gilbert or in
the previous epoch (4.0–5.5 My) under warm-semi-
arid climatic conditions (Kretzoi et al., 1982; Pecsi,
1992; Schweitzer and SzoIr, 1997). Based on sedi-
mentological and pedological observations and on the
traces of frost features on the eroded surface of the
Late Miocene alluvial formations just below the red
silty clays, it was proposed that at least a part of the
red silty clays is resedimented at Visonta (Horvath,
1999; Horvath et al., 2002).
atra Foreland (modified after Varga, 1985).
Plate I. 1. Photo: Overview of the Matra pediment and the Visonta
lignite quarry. All the reported profiles are on the margin of a paleoval
ley indicated by arrow. 2. Photo: Secondary CaCO3 (powdery calcrete
forms flames, drops or isolated patches in the yellowish brown silty
clay. The red clay occurs as droplets. Biogalleries are abundant. The
white coloured spade-stem is about 50 cm. 3. Photo: Irregular flames
are seen on the top of the Late Miocene alluvial formation. Note the
asymmetry of the flames dipping to the north and also partly to the
south. They may be convergent and divergent flames as well.
Z. Horvath et al. / Tectonophysics 410 (2005) 81–95 85
2. Methods
Sedimentological and pedological characters of the
studied formations were recorded in the field. Colours
were established by using Munsell Soil Colour Charts
(1990). The morphological terms used to described the
observed soft-sediment deformations were those by
Alfaro et al. (1997). The observed soils and sediments
were grouped into units based on the presence or
absence of the red clay, and other sedimentary and
pedological characters.
Micromorphological investigations were carried out
on 30 thick thin-sections under the standard petro-
graphic microscope. Broken surfaces were studied
with AMRAY-Scanning electron microscope (the lat-
ter equipped with an EDAX PV 9800 ED X-ray
spectrometer).
2.1. Descriptions of sites
At these margins of the Matra Hills (1014 m) im-
mediately on the northern edge of the Great Hungarian
Plains (Fig. 1), the present elevation of the studied area
is between 120 and 140 m. The soft sediment deforma-
tions are listed in a separate chapter.
2.2. Visonta site
This is an open-pit lignite mine (South Quarry of the
Matra Power Station) near Visonta village (Fig. 2, Plate
I. 1. Photo). Sitting on the top of the ancient pediment of
the Matra Hills, this site offers the best opportunity to
study sediments, soils and related paleolandforms. Here
the studied section is 1.5 km long, and about 30 m high.
The quarry exposes the Late Miocene lignite bearing
alluvial complex, divided by an erosional unconformity
from the overlying Plio-Pleistocene paleosol-bearing
colluvial and alluvial formations. The thickness of the
Post Miocene, mostly Quaternary pedo-sedimentary
complex, varies between a few meters to 60 m. Both
formations are penetrated by different types of second-
ary CaCO3 precipitations (nodules, lenses, various
infillings in cracks) (Fig. 3a–d).
Three main pedo-lithostratigraphical units distin-
guished at the Visonta site are as follows:
Unit 1 Unit 1 comprises the Late Miocene (Upper
Pannonian) formations which are characterised
by alternating cross-stratified sand, clay, silty
clay and coal bearing clay as part of the Late
Miocene alluvial fan covering the coal beds in
the Matra Foreland. The thickness of these
-
)
sediments in the Matra Foreland varies between
200 and 300 m (Csilling et al., 1985). The
exposed thickness of Unit 1 varies normally
between 1 and 100 m. On the top of Unit 1
platy soil-structure is obvious in the studied
profiles. Soft-sediment deformations are pre-
sent in the uppermost part of this unit.
Unit 2 This unit (the bpaleosolQ) consists of a red silty
clay soil-sedimentary complex that varies be-
Z. Horvath et al. / Tectonophysics 410 (2005) 81–9586
tween 1 and 15 m in thickness. Large and small
biogalleries, and the soil structure indicate that
in situ pedogenesis contributed to the formation
of this clay complex. Faecal pellets of insects
found at depths far below their normal habitat in
soils show that pedogenesis was repeatedly
Z. Horvath et al. / Tectonophysics 410 (2005) 81–95 87
interrupted by sedimentation (Horvath, 1999).
The source of this red silty clay can be Matra
Hills that still bear occasional remnants of a
former red soil blanket. Mineralogical compar-
ison of the two red clays reinforces this idea
(Berenyi Uveges et al., 2002).
The following forms of carbonates were ob-
served in Unit 1: nodular calcretes in the
lower part, powdery calcrete in the upper part
and rhizoconcretions in some places of the up-
permost part. We have observed conspicuous
soft-sediment deformations in Unit 2.
Unit 3 Unit 3 contains the recent soil which is a cher-
nozem brown forest soil (Luvic Chernozem, soil
horizons: A, B, BC). The average thickness of
the recent soil horizon is about 1–1.5 m. The
colour of this unit varies from the very dark
greyish brown to yellowish brown. The texture
is silty clay. The soil structure is platy in the top
part of the sediments and it is granular and
prismatic in the sediments situated lower in
this unit. No soft-sediment deformations were
observed in this unit.
2.3. Verseg site
Verseg is situated in the south-western part of the
Matra Foreland. The present elevation of the studied
profile is about 138 m. The section is exposed close to
the top of a gentle hillock. From the bottom to the top
the section is built up by:
Unit 1 Pale yellowish brown silty clay penetrated by
abundant crotovine. By its particle size and
colour it is interpreted as loess-like sediment.
The thickness observed is about 1 m, but in
some places in the quarry the thickness exceeds
3 m. The upper part of this unit is strongly
cemented by calcium-carbonate. The calcrete
is powdery. The matrix is calcareous.
Unit 2 Reddish brown silty clay, is about 100 cm thick.
Its horizon consists of flames of secondary
CaCO3 precipitates (powdery calcrete). The ma-
trix is calcareous.
Fig. 3. (a)–(d) Location of the studied profiles in the Visonta South Quarry o
represent pedo-lithostratigraphic Units (1,2,3). Boxes in the profile consist
paleo-valley, flames, pillows and drops of CaCO3 rich material are visible on
irregular flames dipping to the south and also to the north on the top of the La
as well. (c) Cracked, brecciated structure visible just below the wavy erosi
formation and the Post Miocene red clay. In the upper part of the profile crac
Greenish grey, black clay on top of the Late Miocene alluvial formation form
traceable for tens of meters.
Unit 3 150 cm thick, dark brown silty clay. Calcareous.
Recent soil (Luvic, Chernozem).
2.4. Atkar site
The present elevation of the studied profile is about
132 m. The geology of Atkar is similar to that of
Visonta. As described by Micheli and Mindszenty
(2002) the following stratigraphic units could be distin-
guished:
Unit 1 The Late Miocene alluvial sequence is about
50 cm thick here with no particular soil struc-
ture except on the top of this unit, where
platy, lenticular structure was detected. This
unit is penetrated by abundant powdery cal-
crete, but the matrix of the clayey sediment is
non-calcareous.
Unit 2 Above Unit 1 the mixed zone of white, finely
divided CaCO3, red silty clay, yellow clay loam
and some gray clay can be found. The red silty
clay material appears within the matrix as tubu-
lar fillings (5–15 cm in diameter) and as elon-
gated drops or as streaks. In some areas, thin
layers of contrasting white (calcrete), red and
grey, form cm to dm sized wavy bands, pillows
and drops. They appear compressed and bend
from the horizontal up into flames. Powdery
calcrete shows more deformations than red
silty clay. The whole horizon is impregnated
with calcium-carbonate including numerous
hard and powdery concretions ranging in size
from 1 mm to 10 cm.
Unit 3 The top soil horizon is a chernozem brown forest
soil (Luvic, Chernozem). It is a very dark greyish
brown (10YR 3/2) silty clay with granular soil
structure. The top soil is truncated due to mining
activities. Unit 3 is non-calcareous.
2.5. Particle size distribution and mineralogy of the
above described Units at Visonta and at Atkar
Data on particle size distribution are presented in
Table 1. At the Visonta and Atkar profiles the sand
f the Matra Power Station. Boxes on the left hand side of the profiles
of the soft-sediment deformations. (a) On the Western margin of the
the top of the Late Miocene formations. (b) Secondary CaCO3 forms
te Miocene formations. They may be convergent and divergent flames
onal unconformity surface between the Late Miocene lignite bearing
ks are filled by powdery calcrete and they are dipping slopewards. (d)
s asymmetric waves with 5 cm amplitude and 10 cm wave-length. It is
Table 1
Analysis data of the Visonta site (colour, CaCO3 content, particle size distribution)
Visonta units Horizons Munsell color
code
CaCO3
content (%)
Clay %
b0.002 mm
Total silt %
0.002–0.2 mm
Sand %
N0.2 mm
Texture
Unit 1 Recent soil A horizon 10YR 3/2 0.5 44.3 51.8 3.9 Silty clay
Recent soil B horizon 10YR 6/3 1 52.6 43.4 4.0 Silty clay
Recent soil BC
(carbonate accumulation)
10 YR 4/6 14 43.0 53.7 3.3 Silty clay
Unit 2 Red paleosol part I 10YR 4/6 11 49.9 47.8 2.4 Silty clay
Red paleosol part II 10 YR 5/8 15 42.1 56.0 3.2 Silty clay
Unit 3 Grey clay 5Y 5/3 0-1 62.0 37.7 0.3 Clay
Z. Horvath et al. / Tectonophysics 410 (2005) 81–9588
content in Units 2 and 3 is less than 5%. The clay
content is between 41% and 62%. The grey clay layers
(Unit 1), differ from the sediments in other units. The
sand content is less then 0.3% and the clay content is
slightly higher (N55%). Based on XRD and DTA inves-
tigations, quartz, feldspars, calcite and clay minerals
occur throughout the red clay profile and the predom-
inant clay mineral is smectite. Kaolinite, illite, vermic-
ulite, chlorite, illite/smectite and chlorite/vermiculite
can also be identified in minor amounts in most of
the samples. Smectites in the red paleosol have a pri-
marily high layer charge. According to the origin of the
layer charge both montmorillonitic and beidellitic char-
acter is present. FTIR data also support the presence of
beidellite and the iron-rich nature of smectite. The same
features were observed in several present day Vertisols
(Righi et al., 1995, 1998; Wilding et al., 1983). The red
silty clay was subject to pedogenesis and, by mineral-
ogy and clay content in its present state, according to
the WRB soil classification system (FAO/ISRIC/ISSS,
1998), it is closest to a Vertisol (Nemeth et al., 1999;
Berenyi-Uveges, 2000).
2.6. Soft sediment structures
2.6.1. Visonta site
2.6.1.1. Soft sediment deformation structures
A) In Unit 2, powdery calcrete forms dm to m scaled
flames (c.f. with Cooper, 1943) and 2 to 4 dm
diameter drops, pillows or isolated patches (irreg-
ular pseudo-nodules) within the overlying yel-
Table 2
Analysis data of the Verseg site (colour, CaCO3 content, particle size distri
Verseg units Horizons Munsell colour
code
C
c
Unit 1 Recent soil 7.5RY 4/3 2
Unit 2 Reddish brown paleosol (deformed) 7.5YR 4/6 2
Unit 3 CaCO3 impregnated loess 10YR 6/4 4
lowish brown silty clay, Unit 1 (Fig. 3a, Plate I.
2. Photo). Crotovine are abundant. They criss-
cross even the underlying Late Miocene sedi-
ments (Unit 1). Their shape is rounded to sub-
rounded. Sometimes they form drop like
channels. They are filled by red or greyish
brown clay according to the kind of paleosol
immediately overlying the bioturbated layer.
B) Irregular dm to m scale flames are also seen on
the top of Unit 1. The material of the flames is
powdery calcrete surrounded by a rusty brown
silty clay matrix. The flames are asymmetric,
dipping to north and also partly to the south.
They may be convergent and divergent (Fig. 3b.
Plate I. 3. Photo).
C) Deformed greenish grey to black clay on top of
Unit 1. It forms asymmetric waves with 5 cm
amplitude and 10 cm wave-length. It is traceable
for tens of meters (Fig. 3d, Plate II. 4. Photo).
2.6.1.2. Brittle-deformation structures
A) Immediately under the red clay paleosol (Unit 2)
the Late Miocene greyish green clay (Unit 1) is
fragmented into a fitted-breccia. The matrix of this
clay-clast breccia is rich in calcium-carbonate. The
amount and size of the conspicuously flat (platy)
greenish gray clay clasts (5Y 5/6) decrease gradu-
ally towards the boundary with the overlying
sandy-silty layer. Platy-lenticular structure is relat-
ed to this brecciated structure (Fig. 3d, Plate II. 5.
Photo). Field evidence shows that soft-sediment
deformation of this layer was parallel to the (slo-
bution)
aCO3
ontent
Clay %
b0.002 mm
Total silt %
0.002–0.2 mm
Sand %
N0.2 mm
Texture
2 43 41 16 Silty clay
9 45 46 9 Silty clay
9 37 27 36 Clay loam
Z. Horvath et al. / Tectonophysics 410 (2005) 81–95 89
ping) ground surface. Platy, lenticular structure
shows deformation and suggesting creep along
the slope of the paleovalley. (Plate II. 6. Photo).
B) The platy, lenticular, fitted breccia structure (at the
bottom) is connected to involutions and flames.
The laminae of this structure follow the curve of
involutions. Accepting that the platy, lenticular
structure could be a good evidence for frost-action
(Van Vliet-Lanoe, 1985; Becze-Deak, 1997), this
observation suggests that frost played a role in the
formation of the involutions (Plate II. 7. Photo).
2.6.2. Verseg site
The visible extent of the deformed unit is 20 m in
length and 1.5 m in height (Plate III. 8. Photo). Platy-
blady structure is related to the elongate flames (Table 2).
2.6.2.1. Soft sediment deformation structures. 0.5–1
m long, 5–20 cm thick parallel flames of powdery
calcrete (the top of Unit 1) are tilted NE parallel to
the slope direction. The boundary of the flames is
sharp. 1–10 mm thick, zig-zag shaped cracks are visible
in flames of powdery calcrete. The cracks are parallel to
each other and the boundaries of the flames (platy
structure).
2.6.3. Atkar site
The exposed extent of the deformation horizon is
about 30 m in length and 1.5 m in height (Plate III. 9.
Photo; Table 3).
A) Sagging load casts (sensu Allen, 1982) are very
common, mainly in the upper and middle part of
the deformed horizon. These are 0.1 to 0.5 m
sized bands in which former stratification and
pedogenic horizons are discernible. The material
of sagging load casts is red clay and lime pre-
cipitations. These bands are more or less contin-
uous and have a downward convex shape.
B) Drops which are dm scaled, rounded, ellipsoidal
bodies built up by red clay and yellowish interme-
diate silty clay. They occur in the upper and middle
part of the deformed horizon but occasionally are
traceable also at the lower levels. We observed
several examples of drop-like structures which
Plate II. 4. Photo: Greenish grey to black clay forms small, asymmet
ric waves on top of the Late Miocene alluvial formation. 5. Photo
Late Miocene greyish green clay (Unit 1) is cracked into a fitted
breccia immediately under the red clay paleosol (Unit 2). The matrix
of this clay-clast breccia is rich in calcium-carbonate. 6. Photo: In the
Late Miocene formation the platy, lenticular structure shows defor
mation and it is creeping along the slope of the paleovalley. 7. Photo
Platy, lenticular, fitted breccia structure (at the bottom) is connected to
involutions, flames. The laminas of this structure follow the curve o
involutions.
-
:
-
-
:
f
Z. Horvath et al. / Tectonophysics 410 (2005) 81–9590
originally had been obviously crotovinee, or pat-
ches and nodules of secondary CaCO3 and were
later on slightly modified by ductile deformation.
C) Irregular load casts do not have regular morpho-
logy. They are cm to dm sized, variegated, later-
ally or vertically thinning or thickening bodies
made up by red clay, yellowish silty clay and
powdery calcrete.
D) Pillows were observed in the upper part of the
deformed horizon. They are of 0.1 to 0.3 m size
made up by red, yellow silty clay. In normal
density gradient systems (Alfaro et al., 1997)
during the liquefaction process, a sandy layer
(here silty and consisting of powdery calcrete),
tries to break the upper clay bed, forming a water
escape structure. We suggest that here the rede-
posited, aggregated soil material of probably
greater specific density could have formed pil-
low-like structures as a consequence of sinking
into the powdery calcrete.
E) Water escape structures (flames) were observed
as dm to meter scale, steeply upward directed
structures, made up of powdery secondary
CaCO3 and red clay. They appear on the top of
the deformed horizon. The average distance be-
tween the larger (z50 cm) flames is about 1 m. In
some cases they reach the present surface. Some-
times barely visible fissures are connected to this
type of soft-sediment deformation. Unit 2 is char-
acterized by platy, lenticular structure.
3. Micromorphological observations of the top part
of Unit 1,Visonta site
The sample derived from just below the undulating
erosional unconformity surface between the red clay
paleosol (above) and the Late Miocene alluvial forma-
tion (below).
3.1. Observation
Compact aggregates of micritic carbonate and clay
organized into horizontal, subhorizontal layers and
occurring in association with the platy breccia structure.
On the margins of these aggregates forming the platy,
lenticular structure, Fe-oxide hypo-coatings are clearly
discernible (Plate III. 10. Photo).
Plate III. 8. Photo: Picture at Verseg site. The flames of powdery
calcrete (the top of Unit 1) are tilted to the slope direction (NE).
9. Photo: The view of the Atkar site. 1 m scale flames, waves, load
casts, and drops are visible in this profile. 10. Photo: Micritic aggre-
gates with Fe-oxide hypo-coatings connected to platy structure in the
upper part of the Late Miocene alluvial complex (Unit 1) (�1.5
magnitude, +N). 11. Photo: Powdery calcrete from Visonta is built
up by silt size calcite crystals (SEM image). This size of rhombohedral
calcite were found in all samples from Visonta and Atkar sites as well.
Table 3
Analysis data of the Atkar site (colour, CaCO3 content, particle size distribution)
Atkar units Horizons Munsell color
code
CaCO3
content
Clay %
b0.002 mm
Total silt %
0.002–0.2 mm
Sand %
N0.2 mm
Texture
Unit 1 Recent soil 10YR 3/2 0,3% 45.7 49.2 5.1 Silty clay
Unit 2 Red clay fillings 10YR 4/6 15% 50.0 46.8 3.2 Silty clay
Yellow clay 2.5Y 6/4 11% 45.1 52.2 2.7 Silty clay
Unit 3 Grey clay 5Y 5/3 1% 44.8 55.1 0.1 Silty clay
Z. Horvath et al. / Tectonophysics 410 (2005) 81–95 91
3.1.1. Interpretation
This platy, lenticular structure could be correlated
with segregated ice of ice lenses growing parallel to the
thermal gradient in the sediment, usually roughly para-
llel to the soil surface. Due to the suction of capillary
water induced by thermal gradient-related desiccation
of the underlying sediment, shrinkage cracks were
formed.
During freezing salt becomes concentrated in the
solution and due to suction gypsum or calcite can
precipitate (Van Vliet-Lanoe, 1985). By the orientation
of micritic aggregates associated with the platy, lentic-
ular structure, we suggest that the precipitation of
CaCO3 could be the result of dessication (oversatura-
tion) during frost as described above.
Aggregates created by ice lenses are generally
very stable (Van Vliet-Lanoe, 1985). This structure
is very similar to that described by also Becze-Deak
(1997) as clear evidence of frost action in soils.
Therefore we suggest, the platy fitted-breccia should
be considered as an indication of frost effect on the
profile.
Iron oxide- and oxihydroxide precipitations on the
margins of the aggregates may be the result of ultra-
drying associated with freezing (Krivan, 1958) or of
bacterial activity (Ellis, 1983). However, the latter
would have happened at the time of thawing rather
than freezing.
3.2. Characteristics of calcretes based on SEM
investigations
3.2.1. Morphology
Calcretes from the deformed layers (Unit 1
Visonta site, Unit 2 Atkar site) are entirely built up
by 30–50 Am sized aggregates of well developed
rhombohedral calcite crystals (Plate III. 11. Photo).
Traces of biocrystallization as described by Freytet
and Verrecchia (1998) were not identified. According
to the Udden–Wentworth grain-size scale (Lewis,
1984) the 30–50 Am sized loose aggregation of cal-
cite crystals can be considered as a well sorted
medium to coarse silt.
4. Discussion
4.1. Temporal relationship between sediment deforma-
tions and the growing of calcretes
According to the classification of Netterberg (1967,
1980) and Goudie (1983) several types of calcretes
were identified in the Units of the three sites: (i) hard
nodular calcretes, (iii) hard nodules made of powdery
calcium-carbonates and (iii) laminar and irregular
shaped calcretes made of powdery calcium-carbonates
(Horvath, 1999; Micheli and Horvath, 2004). Mainly
powdery calcretes and hard nodules made from now
autocemented powdery calcium-carbonate bear rela-
tionship to soft-sediment deformations.
The huge amount and different forms of calcretes
may simultaneously have had groundwater (Horvath,
1999; Szinger et al., 2004) and/or loess origin (Micheli
et al., 1999).
Calcretes and their formation in soils have been
studied by several authors including Wieder and Yaalon
(1974), Gile et al. (1966) and Wright and Tucker
(1991). They agree that a gradual enrichment and pre-
cipitation of authigenic carbonates take place during
nodule formation. Brewer (1964) suggested that the
carbonate nodules are formed in situ by processes of
diffusion and/or crystallization in small voids due to
local variations in chemical conditions. Tandon and
Friend (1989), Hay and Reeder (1978) and Szinger et
al. (2004) concluded that the precipitation of carbonate
can replace the original material without significant
disturbance of the sediments around.
Our opinion is that the replacement mechanism (in-
cluding extruding-structures, crystal growing) could
only cause negligible shift of the surrounding material.
According to Pustonvoitov (2003) the average growth
rate of calcium-carbonate crust could reach 2 mm/year,
depending on the circumstances of soil formation. The
calcium-carbonate probably precipitated rather slowly
(20 cm sized nodule at least 50–100 years). The possible
partial dissolution as a consequence of the interaction
between sediment/soil and groundwater could change
this rate. It appears, that it could not have been a strong
Z. Horvath et al. / Tectonophysics 410 (2005) 81–9592
enough triggering agent to cause the observed involu-
tions. However, the fact that powdery calcrete is built up
entirely by silt size calcite crystals (SEM image) indi-
cates that the porosity within the calcretes, is different
from the surrounding material (silty clays, clays). This
can make the calcrete easily subject to ductile deforma-
tion under water saturated conditions, because it has
much higher liquefaction potential than clay or silty clay.
Calcium-carbonates (calcretes) are related to most of
the observed deformations. This observation could help
in evaluating the stratigraphic importance of soft-sedi-
ment and brittle deformations (platy structure, cracked,
brecciated formations). Considering the preliminary age
dating on nodular calcretes (Leel-Hssy and Suranyi,
2002) in the red clay (Unit 2) at the Visonta site, we
may infer that the observed frost structure on the major
erosional surface just below the red clay (on the top of
Unit 1) developed earlier than 300,000 years ago.
Powdery calcretes connected to soft-sediment defor-
mations on the upper part of Unit 2 suggest that these
calcretes and the related deformation is younger than
oxygen isotope stage 10 (340–360 ka BP after Schack-
leton et al., 1991).
4.2. Formation of the studied soft sediment deformation
structures
The soft sediment structures of Unit 2 at all the 3
sites are the result of complex processes. The morphol-
ogy of involutions formed due to frost action, could be
very similar to the ones formed due to seismic shock. In
most cases deformation is limited to Unit 2 (Visonta,
Atkar, Verseg) that is the Post Miocene, mainly Qua-
ternary complex overlying the Late Miocene forma-
tions. Exceptions are small asymmetric waves in Unit
1 at Visonta site which were encountered on the very
top of the Late Miocene strata.
4.2.1. Unit 2 at Visonta site
The flames in Unit 2 are built up by powdery
calcrete and are interpreted as water escape structures.
The silt size powdery calcrete with higher liquefaction
potential under water saturated conditions broke the
silty clay material above and created symmetrical and
assymmetrical flames. The formation of water escape
structures was accompanied by the development of
drops, pillows or isolated patches (irregular pseudo-
nodules) and involutions.
The general presence of the platy, lenticular structure
indicating frost action on the uppermost part of the Late
Miocene sediments (Unit 1) suggest that the involutions
in the Post Miocene soil-sedimentary complex were
formed as a result of cryoturbation. Climatic conditions
favourable for this type of frost-action occurred during
the Pleistocene in the Carpathian Basin. The exact
timing of frost action is impossible at present because
in the lack of available data it cannot be correlated with
any one of the Pleistocene isotope stages.
4.2.2. Unit 2 at Atkar site
Soft sediment deformations observed at this site are
similar but more strongly expressed than the ones at
Visonta site. Traces of ice segregation on the top of the
eroded Late Miocene alluvial formations (Unit 1) just
below the mixed Unit 2, suggest that frost action played
a significant role in the formation of these involutions.
Other observations of cryogenic features in the area
(Stefanovits, 1973; Szekely, 1983; Micheli and Mind-
szenty, 2002) and the comparison of other cryogenic
features presented by Van Vliet-Lanoe et al. (1997,
1998) support the cryogenic origin.
4.2.3. Unit 2 at Verseg site
The possible frost feature (platy structure) closely
related to the flames suggests that the process of soli-
fluction must have been the major deformation mecha-
nism here. Platy-blady structure appears during frost
action due to thin ice lenses in the soil/sediment. The
formation is solidified during frost action, however dur-
ing melting, the grains of soil or sediment start to roll
downslope and the laminae of the platy structure provide
a favourable sliding surfaces for the movement.
The small asymmetric waves (Unit 1 Visonta site)
are not associated either with platy structure or with
slickensides along wedge-shaped aggregates, therefore
their deformation cannot be due to either the shrinking-
swelling of clays or to frost action. We suggest that this
structure may be the result of seismic shock.
Due to the presence of evidence indicating seismic
shock in Unit 1 the role of seismic activity cannot be
excluded as a triggering agent from the formation of the
involutions observed in Unit 2 at all the sites.
If the study sites lie in a relatively flat position, pure
seismically induced deformation (like the above pre-
sented involutions) would require that the triggering
earthquakes must have been at least 4.5=Magnitude
(calculation based on Marco and Agnon, 1995). Be-
cause the sites are found on very gentle slopes (1–28)earthquake events of lower magnitude could have gen-
erated the involutions. In other words, seismic shock
could have been responsible for the formation of the
described structures. This seismic activity might have
occurred several times from the Plio-Pleistocene times
on. Fig. 4 shows the schematic positions of the three
Fig. 4. Schematic position of the studied three sites on the margin of the Great Hungarian Plains. 1: Verseg, 2: Atkat, 3: Visonta. The map shows
how the areal distribution of the observed deformation structures fit the spatial distribution of the total seismic energy release in the Pannonian
Region (after Toth et al., 2002). Heavy lines show tectonic lineaments as defined by F. Horvath and G. Bada, (Toth et al., 2002).
Z. Horvath et al. / Tectonophysics 410 (2005) 81–95 93
studied sites (1: Verseg, 2: Atkar, 3: Visonta) and the
relationship to the spatial distribution of the total seis-
mic energy release in the Pannonian Region in histo-
rical times (after Toth et al., 2002).
5. Summary and conclusions
Soft sediment deformation structures and brittle de-
formation structures were observed in Late Miocene and
Quaternary sediments at 3 sites (Visonta, Verseg, Atkar)
on the northern margins of the Pannonian Basin (south-
ern part of the Matra Foreland). The sequences were
grouped into pedo-lithostratigraphical units.
The common factor in the formation of the soft
sediment structures is that all the original sediments
went through liquefaction–fluidization, but the trigger-
ing mechanism may be different. Evidences of both
frost action and of seismic activity can be found in
the formations. Evidence that involutions are the results
of cryoturbation was supported by the presence of platy
structure in the underlying sediment bearing the involu-
tions (Unit 2 Visonta and Atkar site). However, it could
not be excluded, that at least some of the frost features
were formed independently. In such cases the deforma-
tion structures may be interpreted as the results of
seismic shock.
The units containing the involutions do not show
evidence of shrinking-swelling phenomena due to wet-
ting and drying (wedge-shaped aggregates, slicken-
sides). Therefore this mechanism can be excluded
from triggering agents of the studied soft sediment
deformations even in the clayey parts of Unit 1 at
Visonta and Atkar site, where the clay content and
the smectitic mineralogy would support a high shrink-
swell potential.
The involutions are associated with powdery cal-
cretes (both soft and hardened) that have much higher
liquefaction potential than the surrounding clay or silty
clay in the sequence. This indicates that the presence of
this type of calcium-carbonate had an important role in
the development of the involutions.
Acknowledgements
Thanks are due to the Matra Power Station Co.
for the permission to visit their coal-mines, and for
the logistical support in field-work. Kissne Mezei
Agnes, Kovats Andras, Stefanovits Pal, Jambor
Aron, Roger Langohr, Brigitte Van Vliet-Lanoe, Hor-
vath Erzsebet, Magyari Arpad and William F. McFee
helped us with useful discussions. SCANNING lab-
oratory works were done with Solymos Kamilla and
Ghidan Zsuzsanna. Lantos Zoltan helped technically.
Hilary Putman and Kris Vanhuesden are thanked for
having groomed the English version of the text. We
thank Bada Gabor, Kris Vanneste and the Anonym
reviewer for helpful suggestions. Kovacs Edit and the
technical crew of the Department of Applied and
Environmental Geology (ELTE University) and the
Department of Soil Science and Agricultural Chem-
istry (SzIE University) are also thanked for their
manyfold support.
Z. Horvath et al. / Tectonophysics 410 (2005) 81–9594
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