Rf. Sachsenhofer et al., SUBSIDENCE ANALYSIS AND QUANTITATIVE BASIN MODELING IN THE STYRIAN BASIN (PANNONIAN BASIN SYSTEM, AUSTRIA), Tectonophysics, 272(2-4), 1997, pp. 175-196
We present the results of subsidence analysis and of quantitative basi
n modelling using isostatical and flexural models for basin evolution
along four cross-sections in the Styrian Basin, the westernmost subbas
in of the Pannonian Basin System. Subsidence analysis reveals a first
Ottnangian-Karpatian synrift phase. Our local isostatic models predict
crustal stretching values up to 1.3 and subcrustal stretching values
of 1.6 for this event. Stretching factors of a minor Sarmatian extensi
on phase are below 1.04. The termination of subsidence during the Pann
onian and a rapid Quaternary uplift phase can be explained by major ch
anges in the regional stress field. A W-E cross-section through the no
rthern Furstenfeld Subbasin provides a key for the understanding of th
e dynamics of basin formation. It crosses a narrow Karpatian rift basi
n, the metamorphic core complex of the Penninic Eisenberg Window and s
hows an eastward tilting of the easternmost part of the basin during P
annonian times. Uplift of the Penninic window can only be modelled wit
h an extremely weak lithosphere (equivalent elastic thickness (EET) <
2 km), whereas a best fit between observed and modelled tilting is obt
ained with an EET value of 5 km. These results suggest that the lithos
phere was extremely weak during the onset of basin evolution in Ottnan
gian-Karpatian times, probably caused by high extension rates and high
heat flows associated with Karpatian to early Badenian magmatic activ
ity. Subsequent cooling led to a pronounced increase in flexural rigid
ity. An EET of 5 km fits well with estimations in other parts of the P
annonian realm. Depth-dependent rheology models based on palaeo-heat f
low estimates indicate a similar increase in lithospheric strength wit
h time. The impact of Plio-Pleistocene volcanism on rheology appears t
o be relatively modest, which can be explained by a deep position of t
he magma chamber for this event.