3D structure of the Thuringian Basin, Germany

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Presentation transcript:

3D structure of the Thuringian Basin, Germany Interpretation of gravity and magnetic data with geological constraints for 3D structure of the Thuringian Basin, Germany I. Prutkin, F. Bleibinhaus, T. Jahr (Jena University, Germany) v

Outline of the talk Gravitational effect of the TLUG geological model and its subtraction. Separation of fields into long, intermediate and short wavelengths Modeling for intermediate wavelengths: three granitic intrusions and 3D topography of the density interface below them Short wavelengths: two types of anomalies, correlation with magnetic data and known faults Study of salt tectonics for local areas (Tannrodaer anticline, Ettersberg, Fahner Hoehe)

Our approach to 3D interpretation of gravity/magnetic data Preliminary separation of sources - in depth based on subsequent upward and downward continuation - in the lateral direction using approximation with the field of several 3D line segments - according to density and magnetization contrast by calculation of pseudo-gravity Original algorithms for 3D gravity and magnetic data inversion - for restricted objects of arbitrary shape - for 3D topography of contact surfaces

Initial data set (GGD Leipzig) Initial data. Left: gravity (Bouguer anomalies, grid distance 500m). Right: magnetic (total magnetic intensity anomalies, grid distance 250 m)

Gravitational effect of TLUG model Top left: gravity signal from TLUG model Right: initial gravity data (top) and residual field after subtraction the effect of TLUG model (bottom)

Long wavelengths Low-frequency component of the TLUG model effect (top left), the same for initial data (top right) and for residuals (bottom right), which we attribute to an uplift of Moho

Comparison with magnetic data Long wavelengths for gravity (left) and magnetic data (right) Their comparison reveals that gravitational and magnetic anomalies are caused partly by different objects. The low-frequency component of gravity is caused by the uplift of Moho and the long-wave effect of the basin structure, meanwhile the same component of the magnetic field is generated by the Mid-German Crystalline High

Intermediate wavelengths ρ = 2.75g/cm3 Gravity (intermediate wavelengths) (top left) and its inversion after subtracting negative anomalies Top right: depths to the contact surface, bottom: 3D model of topography ρ = 2.85g/cm3 z≈10km

Approximation of a local anomaly Top: zoomed anomaly (left), regional field model (right). Bottom: residuals (left) and their approximation with 3D line segments (right). RMS=0.41mGal

3D model for intermediate wavelengths We transform line segments to 3D restricted bodies with the same field and put them back. The obtained model for the the main intermediate sources includes three low-density bodies that we interpret as granitic intrusions, and a density interface with topography below them (~10 km depth)

Short wavelengths High frequencies: a signal from the TLUG model (top left), initial data (top right) and residuals (bottom right). Known anomalies have smaller amplitude, two different types of anomalies are better visible

Comparison of gravity anomalies and known faults

Interpretation of the arc-shaped anomaly Top: magnetics. Bottom: pseudo-gravity and measured gravity

3D inversion for an uplift of the crystalline basement 3D model of the topography Kyffhäuser represents not an isolated hill surrounded by a flat surface (TLUG model), but a top of a prolonged mountain chain. Magnetic anomaly continues farther to Sachsen-Anhalt Geomagnetische Karte von Sachsen-Anhalt als Pseudoreliefdarstellung © 2014 LAGB Kyffhäuser Depths to the contact surface

3D inversion for SW-NE anomaly Top: gravity (left) and magnetics (right). Bottom: depths to the contact surface found by our inversion algorithm. Both anomalies are caused allegedly by the same uplift of the crystalline basement

Areas of detailed IGMAS modeling . Fahner Hoehe Ettersberg Tannrodaer Sattel

Tannrodaer Sattel: comparison of gravity and magnetic data Top: gravity (left) and magnetics (right). The positive anomaly is attributed to an uplift of Permian rocks (TLUG), the negative one – to a salt deposit 17

Gravity for the area of Ettersberg After subtracting the effect of the uplift of crystalline, we obtain two negative anomalies separated by a positive one. The shape of the positive anomaly is similar to an outcrop of Muschelkalk. Both negative anomalies are assumed to be caused by salt deposits 18

Ettersberg: IGMAS modeling

Fahner Hoehe: residual gravity 3D inversion for a salt deposit geometry. Red – upper boundary of the Zechstein layer (according to the TLUG geological model), blue – shape of the salt pillow found based on our inversion algorithm Gravity data. A star – location of the Neudietendorf borehole, dashed line - a south-north profile, the section along it is shown in the next slide

Fahner Hoehe: IGMAS modeling According to IGMAS modeling, for the area of the Fahner anticline, process of folding affects also the upper boundary of the crystalline layer

Conclusions Subtracting effect of TLUG geological model and separating into long, intermediate and short wavelengths provide opportunity to investigate deep structure of the Thuringian Basin: uplift of Moho, tree granitic intrusions and a density interface below them Our methodology for separation of sources and 3D inversion can be applied to both gravity and magnetic data for a big area. For a local area, we subtract the model of the regional field (2D harmonic function), approximate the residuals with 3D line segments and transform a chosen set of line segments into a restricted object or a contact surface For short wavelengths, we observe two types of positive anomalies. Anomalies of the first type are not presented in magnetic data. They are correlated with known faults. Anomalies of the second type are correlated with magnetic ones. We transform them to pseudo-gravity and compare with measured gravity. These anomalies have been explained by an uplift of the crystalline basement After subtracting these anomalies, we investigate salt tectonics for local areas (Tannrodaer anticline, Ettersberg, Fahner Hoehe). With some preliminary assumptions it is possible, to isolate the effect of a salt deposit and to find its unknown geometry