P. Schmoldt, PhD - MTNet - DIAS
P. Schmoldt, PhD - MTNet - DIAS P. Schmoldt, PhD - MTNet - DIAS
11. Summary and conclusions 11.2.2. Suggestion for future work MT investigations are, like most geophysical studies, limited by availability and quality of the acquired data. Additional, target-oriented, recordings that could improve specific aspects are: • Broad-band recordings along the ‘Variscan Spain’ – ‘Alpine Spain’ boundary in the Tajo Basin region, inferred from seismic tomography, appraising seismic findings and confirming the proposed correlation between seismic velocity and electric resistivity interfaces. These measurements could proved the basis for revising the Iberian Massif outline beneath the Tajo Basin, which is currently based mainly on surface geology mapping. • An array of broad-band recordings in the Campo de Montiel region, to the west of stations pic017 – pic020, that further investigates properties and extent of the electrically conductive and seismically slow anomaly in the middle and lower crust. Particularly assessing the inferred contribution of a hydrous phase to the response of the proposed asthenospheric remnants and providing additional information about whether the hydrous phase originates from percolation or slab dehydration processes. • Long-period recordings in the centre of the Tajo Basin to enhance knowledge of the low electric resistivity – low seismic velocity anomaly in the lithospheric-mantle. Further, determining electrical properties of the inferred HIMU-like reservoir and its impact on the local geology. Future fieldwork campaigns should be scheduled for periods of increased solar activity and recording sites installed an adequate distance from DC railway lines in order to increase the signal-to-noise ratio, hence the quality of the impedance estimates. Since the study area is situated sufficiently far away from equatorial as well as the polar regions, recordings are considerably less affected by equatorial and polar electrojets that are amplified during high solar activity periods. Thus, presuming a continuation of the 11 year solar cycle, recordings during the years 2011–2016, 2022–2027, etc. are expected to yield high-quality results 1 . MT results should be supplemented by additional surface heat flow and seismic measurements, particularly in the Campo de Montiel region where the electrically conductive and seismically slow anomaly is determined. Moreover, advances in combining results of different geophysical methods and understanding of relations between corresponding parameters will significantly enhance understanding of the geological settings by ultimately yielding a petrophysical model of the subsurface. Approaches that seek to provide petrological models of the Earth’s mantle have been presented by Afonso et al. [2008] 1 It should be noted that the current solar cycle exhibits an elongated minimum, which may result in a shift 284 of subsequent maxima and minima.
11.2. PICASSO Phase I investigation and Fullea et al. [2009], but related codes are not yet able to cope with MT responses of complex mantle geometries; nor are they currently applicable to the much more complex crustal regions. Also suggested is a combination of MT responses from the PICASSO Phase I project and the MAGBET project in order to enhance data coverage in the Betic Cordillera region. With the combined dataset and through, potentially 3D, modelling of the subsurface it might be possible to enhance understanding of the highly complex tectonic orogeny. Again, information from complementary investigations, e.g. seismic tomography, heat flow and gravity measurements, should be used to construct a petrological model of the subsurface. Further, integrating results with projects that investigate the Alboran Sea subsurface (AMELIE, TopoMed), could facilitate detailed examination of the proposed subducting slab structure beneath Alboran Domain and Betic Cordillera. Such investigations may also allow for an evaluating of inferred dehydration processes in connection with the subducting slab and their influence on the regions above. 285
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- Page 361 and 362: Bibliography Abalos, B., J. Carrera
- Page 363 and 364: Bibliography Artemieva, I. M. (2006
- Page 365 and 366: Bibliography Berdichevsky, M., V. D
- Page 367 and 368: Bibliography Cebriá, J.-M., and J.
- Page 369 and 370: Bibliography de Vicente, G., J. Gin
11. Summary and conclusions<br />
11.2.2. Suggestion for future work<br />
MT investigations are, like most geophysical studies, limited by availability and quality<br />
of the acquired data. Additional, target-oriented, recordings that could improve specific<br />
aspects are:<br />
• Broad-band recordings along the ‘Variscan Spain’ – ‘Alpine Spain’ boundary in the<br />
Tajo Basin region, inferred from seismic tomography, appraising seismic findings<br />
and confirming the proposed correlation between seismic velocity and electric resistivity<br />
interfaces. These measurements could proved the basis for revising the<br />
Iberian Massif outline beneath the Tajo Basin, which is currently based mainly on<br />
surface geology mapping.<br />
• An array of broad-band recordings in the Campo de Montiel region, to the west<br />
of stations pic017 – pic020, that further investigates properties and extent of the<br />
electrically conductive and seismically slow anomaly in the middle and lower crust.<br />
Particularly assessing the inferred contribution of a hydrous phase to the response of<br />
the proposed asthenospheric remnants and providing additional information about<br />
whether the hydrous phase originates from percolation or slab dehydration processes.<br />
• Long-period recordings in the centre of the Tajo Basin to enhance knowledge of the<br />
low electric resistivity – low seismic velocity anomaly in the lithospheric-mantle.<br />
Further, determining electrical properties of the inferred HIMU-like reservoir and<br />
its impact on the local geology.<br />
Future fieldwork campaigns should be scheduled for periods of increased solar activity<br />
and recording sites installed an adequate distance from DC railway lines in order to increase<br />
the signal-to-noise ratio, hence the quality of the impedance estimates. Since the<br />
study area is situated sufficiently far away from equatorial as well as the polar regions,<br />
recordings are considerably less affected by equatorial and polar electrojets that are amplified<br />
during high solar activity periods. Thus, presuming a continuation of the 11 year<br />
solar cycle, recordings during the years 2011–2016, 2022–2027, etc. are expected to yield<br />
high-quality results 1 .<br />
MT results should be supplemented by additional surface heat flow and seismic measurements,<br />
particularly in the Campo de Montiel region where the electrically conductive<br />
and seismically slow anomaly is determined. Moreover, advances in combining results<br />
of different geophysical methods and understanding of relations between corresponding<br />
parameters will significantly enhance understanding of the geological settings by ultimately<br />
yielding a petrophysical model of the subsurface. Approaches that seek to provide<br />
petrological models of the Earth’s mantle have been presented by Afonso et al. [2008]<br />
1 It should be noted that the current solar cycle exhibits an elongated minimum, which may result in a shift<br />
284<br />
of subsequent maxima and minima.