SM6.2 | Passive-source seismology for imaging sedimentary basins and energy transition targets
EDI
Passive-source seismology for imaging sedimentary basins and energy transition targets
Convener: Genevieve SavardECSECS | Co-conveners: Simone Pilia, Claudia FingerECSECS, Shubham AgrawalECSECS, Clément EstèveECSECS
Orals
| Fri, 19 Apr, 16:15–18:00 (CEST)
 
Room -2.33
Posters on site
| Attendance Thu, 18 Apr, 16:15–18:00 (CEST) | Display Thu, 18 Apr, 14:00–18:00
 
Hall X1
Orals |
Fri, 16:15
Thu, 16:15
Carbon capture and storage, hydrogen storage, geothermal energy and mining of critical minerals all have a key role in the energy transition in Europe and worldwide. Innovation in efficient low-cost exploration methods is critically needed to characterize and image sedimentary basins and other geological environments that present challenges due to, for example, deeper targets, remoteness, difficult terrain, high population density, or high lateral medium property contrasts.
In recent decades, passive-source methods have progressively emerged as powerful and versatile alternatives to conventional active-source methods, offering non-invasive and cost-effective insights into the geometry and properties of subsurface reservoirs and large-scale structures relevant to seismic hazard analysis. Numerous methodologies such as ambient noise tomography, seismic interferometry, horizontal-to-vertical spectral ratio and high-frequency receiver function analysis have been developed or adapted for exploration and monitoring applications. Meanwhile, the growth of large nodal networks and Distributed Acoustic Sensing (DAS) offers the potential to study the shallow upper crust in new ways.
In this session, we welcome contributions showing advancements in acquisition, methodology and modelling for imaging of the upper crust at different scales (from a few meters to a few kilometres) and case studies demonstrating the performance and benefit of passive seismic imaging and how it can be integrated into the industry exploration workflow. We invite contributions from all passive seismic disciplines, including ambient-noise and earthquake-based approaches. Contributions that take a multidisciplinary approach are particularly welcome.

Orals: Fri, 19 Apr | Room -2.33

Chairpersons: Genevieve Savard, Simone Pilia, Claudia Finger
16:15–16:20
16:20–16:30
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EGU24-3066
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solicited
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On-site presentation
Jordi Diaz, Sergi Ventosa, Martin Schimmel, Mario Ruiz, Albert Macau, Anna Gabàs, David Martí, Özgenç Akin, and Jaume Verges

The potential of different ambient noise methodologies to map the geometry of a small-scale sedimentary basin has been tested using data acquired in the Cerdanya Basin (eastern Pyrenees). We present results based on a 1-year long broad-band deployment covering a large part of the Eastern Pyrenees and a 2-month long high-density deployment covering the basin with interstation distances around 1.5 km. The explored techniques include autocorrelations, ambient noise Rayleigh wave tomography, horizontal-to-vertical spectral ratio, and band-pass filtered ambient noise amplitude mapping. The basement depth estimations retrieved from each of these approaches, based on independent datasets and different implicit assumptions, are consistent, showing that the deeper part of the basin is located in its central part, reaching depths of 600-700 m close to the Têt Fault trace bounding the Cerdanya Basin to the NE. The results show also that when high-density seismic data are available, HVSR and ambient noise amplitude analysis in a selected frequency band are useful tools to quickly map the basement of a sedimentary basin. On the other hand, surface wave tomography, more complex to obtain, provides detailed information on the 3D velocity structure. Besides this methodological aspect, our results help to improve the geological characterization of the Cerdanya Basin and will provide further constraints to refine the seismic risk maps of an area of relevant tourism and economic activity.

How to cite: Diaz, J., Ventosa, S., Schimmel, M., Ruiz, M., Macau, A., Gabàs, A., Martí, D., Akin, Ö., and Verges, J.: Testing multiple ambient noise methodologies to map the basement of small-scale sedimentary basins, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-3066, https://doi.org/10.5194/egusphere-egu24-3066, 2024.

16:30–16:40
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EGU24-8975
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On-site presentation
Zhihui Wang, Christopher Juhlin, Peter Hedin, Mikael Erlström, and Daniel Sopher

Carbon capture and storage (CCS) is a strategy that can be employed to reducing human impact on climate change In the 21st century. Geological storage has been currently considered the most promising strategy. It is reported that there is a large theoretical capacity to store CO2 in the Precambrian sedimentary succession of the Baltic Basin.

 

To aid in surveying and evaluating the potential storage reservoirs in the Baltic Sea, a seismic survey was performed over similar geology in the Sudret area of Gotland. Part of the survey consisted of 14-hours passive data, recorded along a 2.8 km profile with 10m receiver spacing and 1ms sample rate using 329 5Hz SmartSolo nodal units in the vicinity of two boreholes that had been drilled earlier.

 

We retrieved body wave and surface wave virtual shot gathers after applying signal separation and cross correlation calculations. For the body waves, conventional seismic data processing was conducted to obtain a stacked profile; for the surface waves, we could determine the dispersion curve in the frequency range 0.5 to 5.5 Hz and inverted these curves to obtain a velocity model from the ground surface down to c. 1500m depth.

 

Both the body waves and surface waves provide a high quality and high resolution image of the top of the Ordovician formation and have a good consistency with active seismic data in the same location. Moreover, they revealed some reliable deep geological information which active data cannot provide because of the limited source energy. Compared with active seismic exploration, passive seismic is friendly to the environment and cost effective. In some cases, it is an important complementary or alternative method to active seismic for CO2 storage and monitoring.

How to cite: Wang, Z., Juhlin, C., Hedin, P., Erlström, M., and Sopher, D.: Passive seismic imaging for CO2 geological storage in the Sudret area of Gotland, Sweden, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-8975, https://doi.org/10.5194/egusphere-egu24-8975, 2024.

16:40–16:50
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EGU24-18794
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ECS
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On-site presentation
Wen Zhou, Anna Stork, Jan van Elk, Ari David, Hanneke Paulssen, and Annemarie Muntendam-Bos

This study presents passive downhole Distributed Acoustic Sensing (DAS) measurements conducted in the Groningen gas field, Netherlands, for subsurface and induced seismicity monitoring. The optical fiber installation, completed in Sept 2015, was partially cemented behind the inner casing along a deviated well (~3800 m), extending into the sandstone reservoir at temperatures ranging from 100-110 degrees Celsius. In Nov 2022, we interrogated the optical fiber utilizing a 10 m gauge length and 1 m sampling spacing.

Within this setup, most DAS traces exhibit the lowest self-noise floor in the frequency range of 0.1 to 30 Hz. Noteworthy is the absence of visible differences between cemented and uncemented sections. Strong ambient seismic noise is observed in the near-surface unconsolidated sediment at approximately 800 m depth. Noise cross-correlation (CC) analysis is performed for DAS channels and DAS seismometer pairs. Surface wave signals in the 0.1 to 1 Hz range are identified in DAS-seismometer CCs, displaying amplitude and polarization changes with depth, following Surface wave theory.

Induced seismicity is also recorded, with wavefields of events exhibiting clear amplitude variations along the fiber, strongly correlating with sonic logging. Our findings suggest that downhole DAS has the potential to characterize the subsurface with high resolution.

How to cite: Zhou, W., Stork, A., van Elk, J., David, A., Paulssen, H., and Muntendam-Bos, A.: Subsurface characterization using downhole passive Distributed Acoustic Sensing data in the Groningen gas field, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-18794, https://doi.org/10.5194/egusphere-egu24-18794, 2024.

16:50–17:00
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EGU24-9327
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ECS
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On-site presentation
Clément Estève, Yang Lu, Götz Bokelmann, and Jeremy Gosselin

The Vienna Basin (VB) is currently the main target area for deep geothermal exploration in Austria. Knowledge of the subsurface heavily relies on active seismic reflection that are expensive and logistically demanding. Affordable geophysical prospecting methods are needed to reduce subsurface uncertainty. Over the recent years, seismic ambient noise tomography (ANT) has proven to be a cost-effective and environment-friendly exploration technique. Here, we present an ANT of the central Vienna Basin revealing the shear-wave velocity structure of the top 5 km beneath the surface. We deployed an array of ~100 seismic nodal instruments during 6 weeks over summer 2023. We measured fundamental-mode Rayleigh and Love-wave group velocity dispersion from seismic ambient noise and employed transdimensional Bayesian tomography to invert for isotropic group velocity maps at periods ranging from 0.8 to 5.5 s. We then extracted Rayleigh and Love group velocity dispersion curves from the group velocity maps at all locations and jointly inverted them for shear-wave velocity as a function of depth using a transdimensional Bayesian framework. We discuss features observed in our 3D shear-wave velocity model relevant to geothermal exploration.

How to cite: Estève, C., Lu, Y., Bokelmann, G., and Gosselin, J.: Ambient noise tomography for geothermal exploration: the central Vienna basin, Austria, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-9327, https://doi.org/10.5194/egusphere-egu24-9327, 2024.

17:00–17:10
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EGU24-4428
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ECS
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solicited
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Virtual presentation
HyeJeong Kim, Hitoshi Kawakatsu, Takeshi Akuhara, and Nozomu Takeuchi

Kim et al. (2023; JGRse) presents an approach to better characterize the P-wave and S-wave velocity structure of the seafloor sediment layer using ocean bottom seismometers. The presence of low-velocity seafloor sediment layers influences the observed seismic record at the seafloor over a broad frequency range, such that detailed knowledge of this sediment structure is essential to predict its effect on teleseismic records. We use the radial component of teleseismic P waves and autocorrelation functions of the radial, vertical, and pressure components of teleseismic P and S waves to obtain sediment layer models using the Markov chain Monte Carlo approach with parallel tempering. Synthetic tests show that the body waves constrain the P- and S-wave impedances and travel times and the P- to S-wave velocity ratio of the sediment layers. The proposed method resolves thin layers at a high resolution, including the uppermost thin (∼50 m to a few hundred meters) low S-wave velocity layer. Real data applications at sites across the Pacific Ocean that are coincident with previous in situ studies demonstrate the effectiveness of this method in characterizing the seafloor sediment unit. Furthermore, we widely apply the methodology to data from various OBS arrays in the Pacific to estimate in-situ sediment structures. The sediment models show multiple layers in some regions, including the top water-saturated layer with low S-wave velocity and high Vp/Vs values. The scaling relationship of Vp/Vs to Vp shows higher values than the previously discussed ones (e.g., Brocher, 2005; Hamilton, 1979). Furthermore, the sediment layer model constrained from the body waves exhibits agreement in predicted Rayleigh wave admittance with the sediment model from the Rayleigh wave admittance (Bell et al., 2015). The sediment models characterized by this new approach will allow us to more accurately predict and correct the effects of sediment layers in generating P- and S-wave reverberations. Additionally, in this presentation, we will discuss how the in-situ high-Vp/Vs multi-layer sediment model differs in predicting the reverberation effects on receiver function analysis for ocean bottom seismometers.

How to cite: Kim, H., Kawakatsu, H., Akuhara, T., and Takeuchi, N.: Characterizing the Seafloor Sediment Layer Using Teleseismic Body Waves Recorded by Ocean Bottom Seismometers, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-4428, https://doi.org/10.5194/egusphere-egu24-4428, 2024.

17:10–17:20
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EGU24-7809
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ECS
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On-site presentation
Ilaria Barone, Alessandro Brovelli, and Giorgio Cassiani

Seismic interferometry using ambient seismic noise is a powerful technique to constrain shear-wave velocities at different scales. Microseismic monitoring is essential to ensure the safety of industrial operations, including hydrocarbon extraction, gas storage and geothermal production. Microseismic monitoring involves recording seismic vibrations continuously, in order to identify and locate local earthquakes. However, most of the recorded seismic signals is ambient noise, that could be used to infer the shear-wave velocities in the area, thus allowing a more accurate location of the seismic events.

This study aims at applying seismic interferometry to ambient noise recorded by two small microsesimic monitoring networks in Switzerland, deployed around geothermal wells. The processing workflow for each station pair includes different steps as (1) cross-correlation of the raw seismic records, (2) analysis of the zero-crossings of the cross-spectra, (3) picking of the dispersion curve and (4) depth inversion. Due to the sparse nature of the seismic networks, surface wave tomography was not applied. Considerations on the topography effects, on the lateral variability of velocities and on the possible resonance effects due to the valley geometry will be done.

How to cite: Barone, I., Brovelli, A., and Cassiani, G.: Seismic interferometry applied to microseismic monitoring networks in mountain areas, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-7809, https://doi.org/10.5194/egusphere-egu24-7809, 2024.

17:20–17:30
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EGU24-13672
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On-site presentation
Martin Gal, Gerrit Oliver, Thomas Lecocq, and Grace Gunner

In the last decade, passive seismic techniques have found use in the mineral exploration sector. In particular, ambient noise tomography is a low cost viable option that can outperform competing geophysical methods when imaging down to a few kilometers depth. However, at present it does not belong to the core approaches (e.g. magnetic, gravity, etc.) mainly due to a lack of experience in the industry. Novel approaches often go through a period of testing where the industry is familiarized with the technique and expectations are "adjusted". In order to speed up this testing period, an extensive review of the technique and its capabilities for real geological settings is required.

In this work, we build geological models of well known mineral deposits and generate ambient noise cross correlation functions (ccfs) for synthetic deployments. The ccfs are then used in a state of the art fully probabilistic ambient noise tomography to assess the strengths and weaknesses of this technique. This work will allow the industry to better understand the methods capabilities and adjust their expectations for exploration purposes. 

How to cite: Gal, M., Oliver, G., Lecocq, T., and Gunner, G.: Assessing the Accuracy and Feasibility of Ambient Noise Tomography for Copper Exploration: Insights from Synthetic Data Generation with Realistic Geological Models, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-13672, https://doi.org/10.5194/egusphere-egu24-13672, 2024.

17:30–17:40
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EGU24-13498
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ECS
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On-site presentation
Tim Jones, Gerrit Olivier, Bronwyn Murphy, Martin Gal, Nick Smith, Brooke North, Darren Burrows, Lachlan Cole, Craig Went, and Steven Olsen

We use ambient noise tomography (ANT) to image the Hillside Iron-Ore-Copper-Gold (IOCG) deposit at prospect-scale, leveraging Fleet's direct-to-satellite technology for real-time data analysis. Our results capture aspects of the deposit's known geology, including depth of cover, structures linked to mineralisation, and the mineralised host rock, and identifies several new features, including the behavior of key structures down to 1 km depth and lithological variation that underlies the Hillside deposit. Results are compared to existing magnetic, gravity, induced-polarization and drilling data. An analysis of model convergence rates with respect to environmental noise conditions (signal-to-noise ratio) shows that real-time analysis can reduce data collection at the site to within 50% of traditional deployment times. We conclude by commenting on the efficacy of ANT for IOCG exploration more broadly.

How to cite: Jones, T., Olivier, G., Murphy, B., Gal, M., Smith, N., North, B., Burrows, D., Cole, L., Went, C., and Olsen, S.: Real-time Ambient Seismic Noise Tomography of the Hillside IOCG Deposit, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-13498, https://doi.org/10.5194/egusphere-egu24-13498, 2024.

17:40–17:50
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EGU24-16563
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ECS
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On-site presentation
Tobermory Mackay-Champion, Nicholas Harmon, Sekelo Mutelekesha, Mulenga Chanda, Thomas Hudson, John-Michael Kendall, and Michael C Daly

Improved passive seismic imaging of sedimentary basins plays a crucial role in improving our understanding of basin inversion tectonics and sedimentary-hosted mineral systems. The Central African Copperbelt of Zambia and the Democratic Republic of Congo is hosted in the Neoproterozoic Katangan sedimentary basin and accounted for 8.8% of global copper production in 2021 (World Economic Forum, 2024). Despite this, the tectonic evolution of the basin in Northern Zambia is currently unclear, significantly hampering our understanding of the Cu, Co and Ni mineralisation in that area. To investigate the geodynamics that shaped this region, and to assess the suitability of MEMS-accelerometers for passive seismic imaging of sedimentary basins, an array of nodal accelerometers was deployed around the Kansanshi Mine (NW Zambia), previously Africa’s largest Cu mine. Surface wave phase velocities in the mine and surrounding area were analysed using ambient noise tomography, with average Rayleigh wave phase velocities ranging from 3.05 +/- 0.2 km/s at 3 s period to 3.5 +/- 0.15 at 6 s period. The S-wave velocity at points of particular interest was examined using iterative non-linear inversions of surface wave dispersion curves constructed from the tomography results. These S-wave profiles provide new insight into the structural configuration of the Kansanshi copper mine and show that the mine overlies a large thickness of sediments from which the copper could be scavenged. This study illustrates the efficacy of performing ambient noise tomography on MEMS-accelerometer data to investigate the structures controlling the inversion of sedimentary basins and the formation of sedimentary-hosted metal deposits at a local to regional scale.

How to cite: Mackay-Champion, T., Harmon, N., Mutelekesha, S., Chanda, M., Hudson, T., Kendall, J.-M., and Daly, M. C.: Imaging of sediment-hosted Cu deposits using ambient noise tomography: a case study of the Kansanshi Cu-mine, Zambia., EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-16563, https://doi.org/10.5194/egusphere-egu24-16563, 2024.

17:50–18:00
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EGU24-6897
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ECS
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On-site presentation
Preliminary Results from Phase One of the WA Array Passive Seismic Project, Western Australia
(withdrawn)
Reza Ebrahimi, Ruth Murdie, Huaiyu Yuan, and John Paul O'Donnell

Posters on site: Thu, 18 Apr, 16:15–18:00 | Hall X1

Display time: Thu, 18 Apr, 14:00–Thu, 18 Apr, 18:00
Chairperson: Clément Estève
X1.140
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EGU24-3527
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ECS
Ali Riahi, Alexandre Kazantsev, Eleonore Stutzmann, Martin Schimmel, Jean-Paul Montagner, Mark Noble, and Jean-Philippe Metaxian

We estimated the Empirical Greens Functions (EGF) from ambient noise cross-correlations using a dense array of 3C broadband seismometers deployed above an anticline structure hosting an underground gas storage in France. In total, 580 recording locations are available. Several array configurations have been used, some of the seismometers being moved to new locations every day. The survey duration was of 16 days, with around 2 days of recording per location, and a typical interstation distance of 400 meters.

Our methodology uses polarization characteristics to separate body and surface waves. The approach uses the imaginary part of ZR+RZ cross-coherency (Z: vertical; R: radial) to enable the distinct reconstruction of diving P-waves. In order to enhance the signal-to-noise ratio of the retrieved P-wave, we employed common-offset bin-stacking over all virtual sources and receivers, with an offset bin of 50 meters. Subsequently, we assessed the stability of the extracted P-wave by computing a separate common-offset bin-stack for each recording day and each station couple azimuth interval. The consistent moveout of the extracted P-wave, regardless of various station couple azimuths and recording days, suggested that there was no significant source distribution bias in our EGFs.

In the next step, by using the P-wave window from the common-offset bin-stack as a template, we selected only the individual station pairs for which the correlation coefficient between the EGF and the template was above 0.8. This resulted in rejecting about 95% of the station couples. Around 7000 P- arrival times were picked from the selected EGFs in a semi-manual way. The accuracy of these arrival times was validated against the Eikonal solution for the first arrival within the “known” 3D velocity model of the site, based on active seismic and well logging data.

Finally, a 3D tomography based on the picked arrivals allowed us to invert for a P-velocity model up to a depth of around 700 meters. The consistency and the limits of the comparison between this inverted model and the known model are discussed.

How to cite: Riahi, A., Kazantsev, A., Stutzmann, E., Schimmel, M., Montagner, J.-P., Noble, M., and Metaxian, J.-P.: Body wave retrieval from seismic ambient noise: results validation workflow within a known velocity model, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-3527, https://doi.org/10.5194/egusphere-egu24-3527, 2024.

X1.141
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EGU24-4606
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ECS
Imaging the Crustal structure of Oman and the United Arab Emirates using  Seismic Noise Autocorrelation functions
(withdrawn after no-show)
Muhammad Yaqoob and Simone Pillia
X1.142
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EGU24-16191
The shallow subsurface characterization in relation to geothermal resources: Harnessing Passive Seismic Signals for Subsurface Imaging
(withdrawn)
Meysam Rezaeifar, Christopher J. Bean, and Duygu Kiyan and the DIG-team
X1.143
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EGU24-19600
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ECS
Michaïl Henry, Geneviève Savard, Francisco Muñoz, and Matteo Lupi

In recent years, seismic ambient noise interferometry has become a promising non-invasive time-lapse monitoring tool for near-surface studies. Indeed, researches have revealed that the coda of ambient noise cross-correlations can detect subsurface velocity changes (dv/v) as small as 0.01%. Seismic interferometry applications have been demonstrated for monitoring natural processes (groundwater cycle, volcano eruption dynamics) and human operations affecting the subsurface (e.g. geothermal, wastewater disposal). In such applications investigating human-induced effects, careful consideration must be given to site-specific natural background fluctuations to confidently determine if observed velocity changes can be attributed to human interventions. 

An upcoming Enhanced Geothermal System will be developed in the Swiss Jura mountains. Before seismic interferometry can be deployed to monitor geothermal operations, it is important to understand seasonal variations of the noise field. Hence, we are conducting a seismic interferometry study to investigate natural dv/v fluctuations in the area of the future geothermal plant. Using four years of continuous seismic data (August 1, 2017 to June 1, 2021) recorded by four triaxial high-gain broadband stations part of the Swiss national seismic network, we are applying both the moving window cross-spectral (MWCS) and stretching techniques across multiple cross-components. The objective is to quantify the range and magnitude of seasonal seismic velocity changes in the subsurface. Furthermore, our investigations involve exploring correlations between observed velocity changes and specific environmental factors, such as precipitation, groundwater level variations, and temperature fluctuations.

 

How to cite: Henry, M., Savard, G., Muñoz, F., and Lupi, M.: Seasonal variations in seismic velocities within the Swiss Jura using Ambient Noise Interferometry, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-19600, https://doi.org/10.5194/egusphere-egu24-19600, 2024.