P. Schmoldt, PhD - MTNet - DIAS
P. Schmoldt, PhD - MTNet - DIAS P. Schmoldt, PhD - MTNet - DIAS
10. Data inversion Depth off LAB (km) 70 80 90 100 110 120 130 140 150 160 170 RMS misfit 1.25 1.5 1.75 2 2.25 2.5 2.75 3 3.25 3.5 053081 053081+ea 053081+ca LAB LAB+ea LAB+ca Sidelobe Sidelobe+ea Sidelobe+ca Fig. 10.31.: RMS misfit for different Tajo Basin subsurface models used to investigate the electric resistivity of the lithospheric-mantle and depth of the lithosphere–asthenosphere boundary (LAB). Models are created using crustal values of the minimum misfit model from the second 3D inversion sequence (RMS misfit = 1.50, indicate by the dotted grey line) and an exponential decrease of electric resistivity in the lithospheric-mantle with a variable LAB depth; see text for details about model construction and Figure 10.30 for a sketch of the resistivity – depth profile of the models. Symbols indicate the LAB depth of the model; the original model ‘053081’ has no pre-defined LAB depth, thus is indicated by a dashed line. Models with the suffix ‘ca’ comprise an entirely electrically conductive (20 Ωm) asthenosphere, whereas models with the suffix ‘ea’ comprise a thin, electrically conductive asthenospheric layer in form of two rows of 20 Ωm immediately below the lithosphere; in the case of model ‘053081’ the asthenospheric anomaly is introduced below a depth of 110 km. crust (e.g. thermal conductance, radiogenic heat production) significantly affect surface heat flow values, rendering respective findings less conclusive. The hypothesis of partial melt as the cause of the low velocity – high conductivity region is supported by the previously suggested extensive HIMU-like 7 reservoir beneath central and western Europe [e.g. Cebriá and Wilson, 1995; Hoernle et al., 1995; Goes et al., 1999]. Respective low velocity structures have been observed for a range of regions along the Trans-Morocean, western-Mediterranean, European fault zone (Fig. 7.17) and related to volcanic provinces in, among others, the Massif Central in France and the Eifel region in Germany [e.g. Spakman et al., 1993; Zielhuis and Nolet, 1994; Granet et al., 1995; Bijwaard et al., 1998; Goes et al., 2000; Piromallo et al., 2001; Ritter et al., 2001; Wilson and Downes, 2006; Koulakov et al., 2009; Tesauro et al., 2009b]. A lower mantle source for the European volcanism has been proposed by different authors, however, as discussed by Goes et al. [1999] with the current resolution of seismic tomography it is not possible to verify this hypothesis. For the southern Tajo Basin region, partial melting may further be promoted by dehydration processes in relation with the subducting slab beneath Alboran Domain and Betic Cordillera (cf. Sec. 7.2). Hydrous phases can significantly lower the solidus of mantle materials, thereby facilitating melting at lower temperatures which results in a respectively lower surface temperature expression [e.g. Gaillard, 2004; Nover, 2005]. In addition, the presence of a hydrous phase by itself can yield a reduction of seismic veloc- 7 HIMU: “high µ” with µ = 238 U/ 204 Pb 270
Period (s) Period (s) Period (s) r a XY 0.01 0.1 1 10 100 1000 10000 0.01 0.1 1 10 100 1000 10000 0.01 0.1 1 10 100 1000 10000 Minimum misfit model LM77 model Minimum misfit model +ea LM110 model ‘sidelobes’ model LM160 model pic020 pic019 pic017 pic015 pic013 pic011 pic009 pic007 pic005 pic004 pic003 pic002 pic001 pic020 pic019 pic017 pic015 pic013 pic011 pic009 pic007 pic005 pic004 pic003 pic002 pic001 10.2. Inversion for mantle structures 0.01 0.1 1 10 100 1000 10000 0.01 0.1 1 10 100 1000 10000 0.01 0.1 1 10 100 1000 10000 Period (s) Period (s) Period (s) norm_misf 2.7 Fig. 10.32.: Misfit distribution for XY apparent resistivity data (ρXY a ) of the PICASSO Phase I stations and periods for a selection of Tajo Basin subsurface models; therein, the x-axis is positive towards North and y-axis positive towards East. Station responses are derived through forward modelling with the wsinv3d [Siripunvaraporn et al., 2005a] and the normalised misfit is calculated via ρ O a −ρ misfit = log10 C a Err(ρO ; with ρ a ) O a and ρC a observed and calculated apparent resistivity, respectively. The particularly low misfit for longer periods of stations pic013 – pic017 originates from rejection of data due to their low signal-to-noise ratio (cf. Sec. 9). The variation in misfit between models is most significant for longer period data (>10 s) of stations in the centre of the profile (pic007 – pic011) related to the lithospheric-mantle beneath the central region of the Tajo Basin. ity and an increase of electric conductivity (cf. Secs. 5.1 and 5.2.2), and may be the cause of the lithospheric-mantle anomaly beneath the Tajo Basin. Answering the question regarding the origin of the low velocity – high conductivity anomaly in the Tajo Basin mantle is impeded by limitations of MT and seismic tomography approaches: whereas MT investigation is challenging due to the limited penetration of EM waves for regions of increased conductivity and the resulting lower sensitivity to deeper regions (cf. Sec. 3.3) as well as the increased uncertainty levels of long periods in the PICASSO Phase I dataset; seismic tomography suffers from, particularly vertically, smearing of features [e.g. Nolet, 2008, Section 15.3]. Thus, the extent of subsurface features is not particularly well defined. In addition, the resolution of MT and seismic models is limited by the, downward increasing, cell height of the underlying meshes, resulting in a vertical extent of approximately 20 km and 13 km for cells at a depth of 100 km in the MT and seismic tomography mesh, respectively. In case of the MT model, increasing cell size is required to yield a model with a manageable number of cells that can be handled by the 3D inversion algorithm (cf. Sec. 6.3). A model with a non-linear variation of cell size, which would facilitate smaller cells in an area of interest, is not feasible as it introduces inversion artefacts to the model owing to insufficient resolution at this depth range. In addition to information about the Tajo Basin mantle, the 3D inversion model pro- 2.4 2.1 1.8 1.5 1.2 0.9 0.6 0.3 0.0 271
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Period (s)<br />
Period (s)<br />
Period (s)<br />
r a XY<br />
0.01<br />
0.1<br />
1<br />
10<br />
100<br />
1000<br />
10000<br />
0.01<br />
0.1<br />
1<br />
10<br />
100<br />
1000<br />
10000<br />
0.01<br />
0.1<br />
1<br />
10<br />
100<br />
1000<br />
10000<br />
Minimum misfit model<br />
LM77 model<br />
Minimum misfit model +ea LM110 model<br />
‘sidelobes’ model LM160 model<br />
pic020<br />
pic019<br />
pic017<br />
pic015<br />
pic013<br />
pic011<br />
pic009<br />
pic007<br />
pic005<br />
pic004<br />
pic003<br />
pic002<br />
pic001<br />
pic020<br />
pic019<br />
pic017<br />
pic015<br />
pic013<br />
pic011<br />
pic009<br />
pic007<br />
pic005<br />
pic004<br />
pic003<br />
pic002<br />
pic001<br />
10.2. Inversion for mantle structures<br />
0.01<br />
0.1<br />
1<br />
10<br />
100<br />
1000<br />
10000<br />
0.01<br />
0.1<br />
1<br />
10<br />
100<br />
1000<br />
10000<br />
0.01<br />
0.1<br />
1<br />
10<br />
100<br />
1000<br />
10000<br />
Period (s)<br />
Period (s)<br />
Period (s)<br />
norm_misf<br />
2.7<br />
Fig. 10.32.: Misfit distribution for XY apparent resistivity data (ρXY a ) of the PICASSO Phase I stations and periods for a selection<br />
of Tajo Basin subsurface models; therein, the x-axis is positive towards North and y-axis positive towards East. Station responses<br />
are derived through<br />
forward modelling with the wsinv3d [Siripunvaraporn et al., 2005a] and the normalised misfit is calculated via<br />
ρ O<br />
a −ρ<br />
misfit = log10 C <br />
<br />
a <br />
Err(ρO <br />
; with ρ<br />
a )<br />
O a and ρC a observed and calculated apparent resistivity, respectively. The particularly low misfit for<br />
longer periods of stations pic013 – pic017 originates from rejection of data due to their low signal-to-noise ratio (cf. Sec. 9). The<br />
variation in misfit between models is most significant for longer period data (>10 s) of stations in the centre of the profile (pic007 –<br />
pic011) related to the lithospheric-mantle beneath the central region of the Tajo Basin.<br />
ity and an increase of electric conductivity (cf. Secs. 5.1 and 5.2.2), and may be the cause<br />
of the lithospheric-mantle anomaly beneath the Tajo Basin.<br />
Answering the question regarding the origin of the low velocity – high conductivity<br />
anomaly in the Tajo Basin mantle is impeded by limitations of MT and seismic tomography<br />
approaches: whereas MT investigation is challenging due to the limited penetration<br />
of EM waves for regions of increased conductivity and the resulting lower sensitivity to<br />
deeper regions (cf. Sec. 3.3) as well as the increased uncertainty levels of long periods<br />
in the PICASSO Phase I dataset; seismic tomography suffers from, particularly vertically,<br />
smearing of features [e.g. Nolet, 2008, Section 15.3]. Thus, the extent of subsurface features<br />
is not particularly well defined. In addition, the resolution of MT and seismic models<br />
is limited by the, downward increasing, cell height of the underlying meshes, resulting in<br />
a vertical extent of approximately 20 km and 13 km for cells at a depth of 100 km in the<br />
MT and seismic tomography mesh, respectively. In case of the MT model, increasing cell<br />
size is required to yield a model with a manageable number of cells that can be handled by<br />
the 3D inversion algorithm (cf. Sec. 6.3). A model with a non-linear variation of cell size,<br />
which would facilitate smaller cells in an area of interest, is not feasible as it introduces<br />
inversion artefacts to the model owing to insufficient resolution at this depth range.<br />
In addition to information about the Tajo Basin mantle, the 3D inversion model pro-<br />
2.4<br />
2.1<br />
1.8<br />
1.5<br />
1.2<br />
0.9<br />
0.6<br />
0.3<br />
0.0<br />
271