EMRP2.16
Electromagnetic induction in Geophysics: Methodology, Data, Modelling and Inversion

EMRP2.16

Electromagnetic induction in Geophysics: Methodology, Data, Modelling and Inversion
Convener: Ute Weckmann | Co-conveners: Duygu Kiyan, Graham Hill, Shunguo Wang
Presentations
| Tue, 24 May, 13:20–14:50 (CEST)
 
Room -2.31

Presentations: Tue, 24 May | Room -2.31

Chairpersons: Shunguo Wang, Duygu Kiyan, Maik Neukirch
13:20–13:22
13:22–13:32
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EGU22-2196
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solicited
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Highlight
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On-site presentation
Rita Streich, Gurban Orujov, and Andrei Swidinsky

Controlled-Source Electromagnetic (CSEM) methods have the potential to be powerful geophysical tools for imaging and monitoring the distribution of electrically resistive fluids, such as freshwater aquifers, CO2 injected into the subsurface or hydrocarbons during oil and gas production.  However, the presence of metallic infrastructure (steel well casings, pipelines etc.) presents an enormous challenge, because the highly conductive metal masks the electromagnetic response of subsurface geology and distorts any associated time-lapse changes. Therefore, numerical techniques to predict and mitigate the contamination caused by pipelines and casings on CSEM surveys are critical for real world imaging and 4D applications near any such metal objects.

In a collaborative project between the Colorado School of Mines and Shell, we have developed CSEM modeling and inversion tools that can handle realistic scenarios with multiple vertical as well as deviated casings and complex pipeline networks, as will be encountered in mature oil field environments. First, we implemented a forward modeling code based on the Method of Moments technique, which effectively turns the casings into extra sources, such that we do not need to discretize them into excessive numbers of very small model cells. We used this modeling tool to demonstrate quantitatively how steel casings impact synthetic and real time-lapse EM data. The forward modeling code was then combined with a newly developed Gauss-Newton inversion engine, which by itself has been demonstrated to provide images of superior resolution, depth penetration and data fit with less dependency on initial conditions compared to previous quasi-Newton inversion engines.

In this contribution, we first demonstrate on synthetic data that the combination of these two algorithms provides high-quality electrical resistivity images in the immediate vicinity of well casings. Then, we show encouraging results of applying the new tools to field trial data acquired over known casings under semi-controlled conditions. The images obtained are nearly free of casing imprint and subsurface geology could be recovered. These results suggest that this technology may enable us to explain severely distorted field data that were previously uninterpretable.

How to cite: Streich, R., Orujov, G., and Swidinsky, A.: Advances in electromagnetic imaging in the presence of well casings: algorithms and field experiments, EGU General Assembly 2022, Vienna, Austria, 23–27 May 2022, EGU22-2196, https://doi.org/10.5194/egusphere-egu22-2196, 2022.

13:32–13:39
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EGU22-13529
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ECS
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Highlight
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On-site presentation
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Artur Benevides, Naser Meqbel, Sergio Fontes, Williams Lima, Gary Egbert, Paulo Werdt, and Emanuele La Terra

This work presents results from a controlled source electromagnetic (CSEM) set of inversion runs of real data in the Campos basin, Southeast Brazil. The Campos basin is in the Brazilian east margin, with origin in the Neocomian stage of the Cretaceous period 145–130 million years ago during the breakup of the supercontinent Gondwana (South America and Africa split). The clastic reservoirs in this basin have been the largest oil producer in Brazil for the past three decades. The present challenge in exploring clastic reservoirs has moved to deeper waters, enforced by the complex geology posed by the tectonics associated with giant salt domes. Electromagnetic (EM) methods are sensitive to subsurface resistive variations and have been frequently used in exploration programs for fresh water, mining and for hydrocarbon (HC), mainly in joint approaches with seismic to minimize ambiguity in the interpretations. Reservoirs filled with HC are generally more resistive than the host rocks which is an advantage for the EM method. Combining resistive models with seismic results considerably improves the resolution of the subsurface structures and the geometry of the HC reservoirs. A set of 40 Controlled Source EM (CSEM) receivers were deployed at the seafloor (water thickness is around 1.7 km) in a grid-shape array with varying spacing between 5 km to 10 km. The electric field components have been recorded from an active electromagnetic source towed 50 m above the seafloor. The processed data consist of inline components of the horizontal electric field (Ex and Ey) for four main frequencies (0.125 Hz, 0.25 Hz, 0.5 Hz and 1.25Hz). The CSEM 3D inversion models have been obtained using the modified version of Modular System for EM inversion (ModEM code) which is under development within a research project at Observatório Nacional – Brazil. Preliminary 3D CSEM inversion results yielded a good agreement with resistivity values observed in the well logs. In the second step of this work, information from seismic and well logs are being introduced as a priori information to improve resolution of the CSEM inversion in different scenarios involving hydrocarbon accumulations in thin post-salt reservoirs in Campos basin. 

How to cite: Benevides, A., Meqbel, N., Fontes, S., Lima, W., Egbert, G., Werdt, P., and La Terra, E.: Marine controlled source electromagnetic inversion data from a field at Campos basin SE-Brazil, post-salt reservoirs constrained by seismic and well log, EGU General Assembly 2022, Vienna, Austria, 23–27 May 2022, EGU22-13529, https://doi.org/10.5194/egusphere-egu22-13529, 2022.

13:39–13:46
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EGU22-3498
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Highlight
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Virtual presentation
Svetlana Byrdina, Jean-Luc Got, Laurent Metral, Philip Hering, Marion Baques, Louis De Barros, Stephane Garambois, Philippe Gueguen, and Volker Rath

The Ubaye Region is a seismically active region in the Western Alps (France), regularly struck by seismic swarms characterized by a high number of small to moderate earthquakes, such as in 2003–2004 or 2012–2015. While some earthquakes could be associated with known faults, the character of the observations (high seismicity – low deformation rate) requires complex driving processes beyond local or regional tectonics. Most conceptual models involve fluids present down to depths of several km, and/or long-range transport.

Magnetotellurics (MT) is known to be an efficient imaging method sensitive to crustal fluids. During 2020/21, a data set of 30 MT sites was acquired, covering a signal period ranging between 10-4 to 104 s, with generally all 5 components measured. Data quality was generally satisfactory up to 3 s and sometimes up to 100 s. Major problems were related to topography (including logistics), and to the presence of electromagnetic noise, only to be mitigated by advanced processing methods (FFMT). For the 3-D inversion required by the data (phase tensors, WAL, topography), we have chosen a joint inversion of induction vectors, phase tensors and off-diagonal impedances (previously corrected for static shift with help of phase tensor inversion). This allowed us to obtain the best 3-D model using the ModEM inversion code, explaining all three data types reasonably well.

The main findings from this investigation include (a) a prominent conductor (down to 20 Ωm) located along the axis of the swarm zone, though generally above it; (b) a regional dominance of the Penninic Front in the East and the overridden Mesozoic (Dauphinoise) sediments in the West, both not fully covered by the current survey; (c) strike directions that agree well with most of the mapped faults and focal mechanisms of the strongest seismic events.

Uncertainties associated with the insufficient data coverage in some of the most interesting zones were studied by analysing the sensitivities provided by the inversion and direct forward modelling of significant model features. In general, this led to the conclusion that our sensitivity does reach the border of the seismic swarm activity, but does not cover its depth extent. Due to the gap in data in the central area of interest, the geometry and connectivity of the main conductor remains a hypothesis. Thus, a truly quantitative characterization of prominent identified structures is not currently possible and should be better assessed with additional measurement sites. The different conceptual models proposed for the origin of the seismic swarm activity will be discussed in the light of the MT imaging, and the associated uncertainties.

How to cite: Byrdina, S., Got, J.-L., Metral, L., Hering, P., Baques, M., De Barros, L., Garambois, S., Gueguen, P., and Rath, V.: Magnetotelluric investigations in the Ubaye seismic swarm region, Western Alps: a connection between electrical conductivity, fluids, and earthquakes?, EGU General Assembly 2022, Vienna, Austria, 23–27 May 2022, EGU22-3498, https://doi.org/10.5194/egusphere-egu22-3498, 2022.

13:46–13:53
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EGU22-916
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Virtual presentation
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Maria Constanza Manassero, Juan Carlos Afonso, Alison Kirkby, Alan Jones, Ilya Fomin, and Karol Czarnota

In the context of whole-lithosphere structure, the joint inversion of magnetotelluric (MT) with seismic data is particularly interesting as they provide complementary information on the thermal structure, fluid pathways and water content. Both data sets can put tight constrains on the first-order thermal structure and mineralogical structure of the lithosphere, but only MT is strongly sensitive to anomalous features such as hydrogen content, minor conductive phases and/or small volumes of fluid or melt. This makes joint inversions of MT with other observables a powerful means to detect fluid pathways in the lithosphere including the locus of partial melting, ore deposits and hydrated (or metasomatized) lithologies. This unique potential of joint inversions of MT with other datasets has given impetus to the acquisition of collocated MT and seismic data over large regions. Concrete examples are the US Array, Sinoprobe in China, and the AusLAMP/AusArray in Australia. These multi-disciplinary programs are providing high-quality seismic and MT data with unprecedented resolution and coverage, allowing the pursuit of large-scale 3D joint inversions to image the structure, dynamics and evolution of the whole lithosphere and upper mantle.

 

Within probabilistic approaches the solution to the inverse problem is given by the so-called posterior probability density function which provides complete information about the unknown parameters and their uncertainties conditioned on the data and modelling assumptions. Joint probabilistic inversions of MT and seismic data have been successfully implemented in the context of 1D MT data only. For the cases of 2D and 3D MT data, however, the large computational cost of the MT forward problem has been the main impediment for pursuing probabilistic inversions, as the number of forward solutions required are typically on the order of 105 – 107. To overcome this limitation, we have recently presented a novel strategy [2,3], called RB+MCMC, that computes 3D MT surrogate models and uses complementary parameterizations to couple different data sets. This strategy reduces the computational cost of the 3D MT forward solver and allow us to perform full joint probabilistic inversions of MT and other datasets for the 3D imaging of deep thermochemical anomalies.

 

In this contribution, we first illustrate the benefits and general capabilities of our method for 3D joint probabilistic inversions of MT with other datasets using whole-lithosphere synthetic models. Last, as part of the Exploring for the Future program, we present results of the first joint probabilistic inversion of 3D MT in southeast Australia using the AusLAMP data and a seismic velocity model derived from teleseismic tomography [4]. These results demonstrate the capabilities of our conceptual and numerical framework for 3D joint probabilistic inversions of MT with other geophysical data sets and open up exciting opportunities for elucidating the Earth’s interior in other regions.

 

 

 

References

[1] Afonso, J.C. et al., (2016), Journal of Geophysical Reseach, 121, doi:10.1002/2016JB013049

[2] Manassero, M. C., et al., (2020), Geophysical Journal International, 223(3), doi: 10.1093/gji/ggaa415

[3] Manassero, M. C., et al., (2021), doi: 10.1029/2021JB021962

[4] Rawlinson, N., et al., (2016), Tectonophysics, doi: 10.1016/j.tecto.2015.11.034

How to cite: Manassero, M. C., Afonso, J. C., Kirkby, A., Jones, A., Fomin, I., and Czarnota, K.: Joint Probabilistic Inversion of 3D Magnetotelluric and Seismic Data in Southeast Australia, EGU General Assembly 2022, Vienna, Austria, 23–27 May 2022, EGU22-916, https://doi.org/10.5194/egusphere-egu22-916, 2022.

13:53–14:00
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EGU22-5056
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ECS
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On-site presentation
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Monica Aquino, Guy Marquis, and Jerome Vergne

We use a correspondence map approach to jointly invert surface-wave dispersion curves and magnetotelluric data for subsurface shear velocity and resistivity but also for a possible relationship between them. Our first experiments consist of inversions of synthetic data computed from models linked by linear and second-order polynomial relationships. Our methodology produces joint inversion model-pairs (resistivity-shear velocity) from where 80% fit the 'observed' parameter relationship within a 5% error vs only 1%  of the separate inversion model-pairs for the linear relationship experiment. For the non-linear relationship synthetic test, 85% of the joint inversion model-pairs fit the 'observed' relationship within a 5% error while just 40% of the separate inversion model-pairs. This reduces the number of acceptable models without compromising the data fit ('reduction of non uniqueness'). Using the non-linear synthetic data we show how to select an appropriate polynomial degree for joint inversion. Having validated the approach with synthetic cases, we applied our methodology to field data from the ECOGI and EstOF surveys in North Alsace, France. We compare separate and joint inversions and we find that the 1D subsurface models obtained from joint inversions are more similar to previous models documented in the area than the separate inversion models. We are currently extending this work to higher dimensions. At the spatial scale of our problem, sensitivity analysis suggests that shear velocity models can benefit from the lateral sensitivity of the magnetotelluric data.

How to cite: Aquino, M., Marquis, G., and Vergne, J.: Joint inversion of Magnetotelluric Data and Surface-Wave Dispersion Curves using Correspondence Maps, EGU General Assembly 2022, Vienna, Austria, 23–27 May 2022, EGU22-5056, https://doi.org/10.5194/egusphere-egu22-5056, 2022.

14:00–14:07
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EGU22-1034
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On-site presentation
Maik Neukirch, Alexander Minakov, Maxim Smirnov, Carmen Gaina, Ionelia Panea, Anca Isac, Marine Collignon, Alexandru Zlibut, Cosmin Coverca, Bogdan Sebastian Paralescu, and Ana-Maria Henriuc Morosan

Geothermal energy extracted from hydrothermal systems can play a key role in mitigating the effects of climate change, while meeting the world’s increasing energy demand. Moreover, not only does it represent a highly economic and adaptive source of renewable energy, but it is genetically related with the formation of ore deposits which are necessary to fuel our energy transition.

The presented study is part of a larger multidisciplinary and international project that aims at investigating the geothermal potential of the Baia Mare region, in northern Romania and for which geological, geochemical, hydrogeological and geophysical data have been. In this framework, the magnetotelluric (MT) method is used to study the hydrothermal system and more specifically to locate heat sources, highlight the presence of fluids and identify the system’s structure.

The largest cluster of measurements with anomalously high heat flow values in Romania (100-160 mW/m2) is situated in the greater Baia Mare region, revealing this area as a prime interest for geothermal exploration. The study area is located within the Neogene Inner Carpathians volcanic arc. Crustal hydraulic properties and associated hydrothermal systems are possibly controlled by the regional Dragos-Voda strike-slip fault zone, which could also provide a pathway for late Miocene magmatic intrusions and lava flows. The associated magmatic plumbing system crosscuts the Neogene sedimentary deposits of the Pannonian Basin. The region is known for surface hot springs, salt and metal mining, which all suggest the presence of a hydrothermal system that could be exploited for geothermal energy.

Broadband magnetotelluric transfer functions have been obtained at 24 sites in the Baia Mare region ranging from 300 Hz up to around 1000s using two MTU instruments from Luleå University of Technology. In addition, we collected continuous telluric broadband recordings at the Surlari National Geomagnetic Observatory to be used as remote reference data together with data from other INTERMAGNET observatories. We applied non-stationary, robust remote processing, which allowed to improve poorly constrained estimates of the impedance tensor in the MT dead band (1 to 10s). Phase tensor and impedance maps provide data overview and a first glimpse of subsurface structures. The preliminary 3D inversion results are presented.

How to cite: Neukirch, M., Minakov, A., Smirnov, M., Gaina, C., Panea, I., Isac, A., Collignon, M., Zlibut, A., Coverca, C., Paralescu, B. S., and Henriuc Morosan, A.-M.: Geothermal Exploration of the Baia Mare Region (Romania) with Magnetotellurics – Responses, Analysis and 1D Models, EGU General Assembly 2022, Vienna, Austria, 23–27 May 2022, EGU22-1034, https://doi.org/10.5194/egusphere-egu22-1034, 2022.

14:07–14:14
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EGU22-4884
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ECS
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Virtual presentation
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Basel Aleid, Ute Weckmann, Anna Platz, and Johannes Mair

The Bohemian Massif is part of the geodynamically active European Cenozoic Rift System and represents its easternmost termination. The study area is situated at the junction of three different Variscan tectonic units and hosts beside the Eger Rift a series of different fault systems. The entire region is characterized by ongoing magmatic processes in the intra-continental lithospheric mantle expressed by, e.g., the occurrence of repeated earthquake swarms, the presence of Quaternary volcanoes, and massive degassing of mantle-derived CO2 in mineral springs, mofettes as well as. Several geoscientific studies suggest that fluid circulation along the deep-reaching faults seems to play an important role in explaining the underlying geodynamic processes. As part of an ICDP drilling programme, we applied the Magnetotelluric (MT) method with the goal to contribute to the understanding of the physical and chemical processes and interaction that led to the magma and fluid transport by mapping potential fluid pathways from the crust-mantle boundary up to the surface. Here, we present 3D inversion models of two different overlapping regional and one local MT experiments located in the Cheb basin close to the Hartoušov mofette field. The most prominent large-scale conductivity features of the regional models are several channels from the lower crust to the surface, possibly representing pathways for fluids into the earthquake swarm region, mofette fields, and known spas. However, such a conductive channel is absent in the local model beneath the surface expression of the mofettes. We will test two different hypotheses, namely a vertical ascending channel versus lateral fluid migration. Results from synthetic modelling studies and available geoscientific constraints hint that such a channel might exist directly beneath the mofette field, but due to the given data quality, station distribution, and the subsurface conductivity structure within a conductive sediment basin, it might be challenging to resolve.

How to cite: Aleid, B., Weckmann, U., Platz, A., and Mair, J.: Magnetotellurics in the Eger Rift: Regional and local three-dimensional subsurface imaging and modelling of fluid pathways from the crust-mantle boundary to the surface, EGU General Assembly 2022, Vienna, Austria, 23–27 May 2022, EGU22-4884, https://doi.org/10.5194/egusphere-egu22-4884, 2022.

14:14–14:21
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EGU22-6586
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ECS
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On-site presentation
Sergio Luiz Fontes, Artur Benevides, Liliane Panetto, Ved Prakash Maurya, Emanuele Francesco La Terra, and Antonio Padilha

Long period magnetotelluric (LMT) stations were deployed on an array format covering much of the Parnaíba basin and western edge of the Borborema Province in NE Brazil. A grid with 56 LMT stations (from 10 s to over 104 s) with 70 km spacing were acquired during periods of acquisition varying from 2-3 weeks up to 6 months through two field campaigns between November 2018 and July 2019. This study is the first of this kind undertaken in Brazil, much in line with the American EarthScope, the Chinese SiinoProbe and AUSLAMP - Australia array initiatives suggesting the way forward for a comprehensive understanding of large 3D electrical structures of the continental crust and the lithospheric mantle in the entire country.  The results already published show that the resolution of the models obtained is comparable to the inversions of seismic tomography, the sensitivity of the MT method being superior in sensing the melting fraction, temperature and water content in the mantle. As an example, the 70 km spacing between EarthScope stations proved adequate to delineate the main structural features of the middle crust to the upper mantle of the United States. The Parnaíba Basin is a cratonic basin that has been formed by sedimentary mega sequences deposited along the Phanerozoic, after the formation of the Gondwana Supercontinent, with sedimentation expanding over the Borborema Province. The basin's evolution was conditioned by subsidence processes along unstable crustal areas at the end of the Brazilian cycle and demarcated by grabens, fault zones and magmatism. The shallow sediments of the basin (around 2.5 to 3.4 km maximum) however widely spread 60,000 km2 cover prominent crustal features including the location of the trans-Brazilian lineament, limits of the Borborema Province, Amazon craton and other important shear and suture zones that may be important to better understand the evolutionary geodynamics of the supercontinents. The time series of electric and magnetic fields recorded in the field have been passed through extensive quality control analysis and then were robustly processed in the frequency domain generating good quality impedance tensor and tipper transfer functions. Currently we are concentrating our efforts on testing several parameters (e.g. mesh design, starting resistivity, damping and covariance analysis) involved in the 3D inversion nonlinear conjugate gradient ModEM code. Following the best practical procedures suggested by previous MT studies to avoid bad impact on the inversion results, misfits have been achieved nRMS ~ 2.2 in joint inversion of impedance tensor and tipper and nRMS < 2 for separate inversion of these transfer functions. Notwithstanding, preliminary resistivity models present good agreement with previous geophysical studies in the area and portray remarkable large-scale middle crust and deep conductive structures inside the covered area. Since there are several geodynamic processes associated with this area and electrical signatures may still exist the MT data set can be an important key to understand the evolution of the pan-African cycle and unravel new findings related to the formation of the Parnaiba basin.

How to cite: Fontes, S. L., Benevides, A., Panetto, L., Maurya, V. P., La Terra, E. F., and Padilha, A.: Deep images of electrical conductivity in Parnaiba basin - NE Brazil, EGU General Assembly 2022, Vienna, Austria, 23–27 May 2022, EGU22-6586, https://doi.org/10.5194/egusphere-egu22-6586, 2022.

14:21–14:28
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EGU22-2268
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ECS
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On-site presentation
Shunguo Wang, Steven Constable, Arnold Orange, and Ståle Emil Johansen

The marine controlled-source electromagnetic (CSEM) method has been used for offshore natural resource exploration for a few decades, and it has the potential to be used for offshore CO2 storage monitoring. Airwaves, previously treated as distortions, often dominate marine CSEM data when the offshore seawater is shallower than a couple of kilometers. Therefore, different methods have been proposed to distinguish and then correct the airwaves in marine CSEM data. In this study, we analyzed the airwave features by different model parameter perturbations with two-dimensional (2D) modeling. After a thorough study of differentiated EM fields and Poynting vectors for each single model component, we summarize the airwave propagation features and sensitivities regarding different modeling parameters. Particularly, the scenario with and without an oil reservoir or CO2 storage is carefully studied. It turns out that the airwave can provide useful information at certain transmitter and receiver offsets. Nevertheless, we propose to model the airwave as what it is in the marine CSEM data rather than correct it before feeding the offshore CSEM data to inversion. This idea is demonstrated with a field example from offshore of Svalbard, Norway.

How to cite: Wang, S., Constable, S., Orange, A., and Johansen, S. E.: New insights of airwave in controlled-source electromagnetic offshore data, EGU General Assembly 2022, Vienna, Austria, 23–27 May 2022, EGU22-2268, https://doi.org/10.5194/egusphere-egu22-2268, 2022.

14:28–14:35
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EGU22-7541
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ECS
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On-site presentation
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Aaron Hornschild, Jan Saynisch-Wagner, Julien Baerenzung, Christopher Irrgang, and Maik Thomas

The movement of conductive seawater through Earth's magnetic field leads to electromagnetic induction processes in the oceans. The resulting radial magnetic fields have been successfully modeled and, in the case of tidal-induced magnetic fields, also identified in satellite magnetometer data. However, the magnetic signals caused by ocean circulation have still remained unobserved.
We introduce a new method to detect these signals using an observing system simulation experiment. Our approach relies on a Kalman filter-based assimilation of satellite magnetometer data. A key aspect of identifying ocean-induced signals is separating them from other magnetic contributions. For this separation, we used both estimations of the temporal behavior and spatial constraints as prior information. The observing system simulation experiment allows us to evaluate the proposed method.  
We present the results of this evaluation and report on the detectability of magnetic fields induced by ocean circulation.

How to cite: Hornschild, A., Saynisch-Wagner, J., Baerenzung, J., Irrgang, C., and Thomas, M.: The detection of the magnetic fields induced by ocean circulation - An observing system simulation experiment, EGU General Assembly 2022, Vienna, Austria, 23–27 May 2022, EGU22-7541, https://doi.org/10.5194/egusphere-egu22-7541, 2022.

14:35–14:42
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EGU22-8692
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Presentation form not yet defined
Peculiarities of geomagnetic field measurements at Lampedusa island in relation with geomagnetic activity, seasons and tidal modes: possible link with the sea level rise and current flows in the Mediterranean
(withdrawn)
Mauro Regi, Antonio Guarnieri, Stefania Lepidi, and Domenico Di Mauro
14:42–14:49
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EGU22-12240
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ECS
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Virtual presentation
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Shu Kaneko, Toru Mogi, Chie Yoshino, and Katsumi Hattori

The Boso Peninsula is one of the most tectonically active regions in Japan due to its location on a plate boundary. Focal zones of the past enormous earthquakes (1703 Genroku Kanto Earthquake (M8.2), the 1923 Taisho Kanto Earthquake (M7.9)) and slow slip events (SSE) region are located southwest and southeast of the peninsula, respectively. Therefore, it is important to survey the subsurface resistivity structure of these regions from a geophysical point of view. The magnetotelluric (MT) survey was conducted to clarify the resistivity structure from 2014 to 2016. However, observed MT data was contaminated by artificial noise sources (e.g., leak current from DC-driven trains and power lines). Conventional noise reduction methods using remote reference (Gamble et al., 1979) and robust statistics such as BIRRP (Chave and Thomson. 2004) are inadequate to deal with the noise. The reason is that the noise included in Boso MT data is originated from a near field source and is coherent between the magnetic field and the electric field.

Therefore, we propose a NEW method using MSSA(Multi-channel Singular Spectrum Analysis) to reduce the influence of the noise. MSSA can decompose multiple time series to several principal components (PCs). In our new method, choosing PCs based on the correlation between each component, they are discriminated into trend components, quasi-periodic components (=interested MT signal), and noise components. We applied MSSA to 7ch (5ch for observation site data (horizontal magnetic field, vertical magnetic field, and horizontal electric field) and 2ch for reference site data (horizontal magnetic field)) to extract 'clean' MT data from noisy Boso MT data. In this presentation, the results of time series and MT analysis applying this method will be presented.

How to cite: Kaneko, S., Mogi, T., Yoshino, C., and Hattori, K.: Development of noise reduction method based on MSSA (Multi-channel Singular Spectrum Analysis)     -Application to near field noise observed in Boso Peninsula, Japan-, EGU General Assembly 2022, Vienna, Austria, 23–27 May 2022, EGU22-12240, https://doi.org/10.5194/egusphere-egu22-12240, 2022.

14:49–14:50