Geophysical Journal International

SummaryThis study investigates the longitudinal (T1) to transverse (T2) relaxation time ratios in unconsolidated geological materials to determine how they vary across different geological units. Assessing the T1/T2 ratio can inform about the validity of the presumed relationship between T1 and T2 relaxation times in steady-state surface NMR modeling (i.e. T1/T2 ratio is assumed to be constant and equal to one). The T1/T2 ratio investigation is conducted by two-dimensional T1-T2 correlation data using laboratory and borehole NMR measurements at a Larmor frequency of 2 MHz and 430 kHz, respectively. Laboratory NMR measurements were performed on 73 sediment samples from 9 sites in Denmark and Germany, and borehole NMR measurements were conducted at 59 selected depth intervals in unconsolidated geological units across 8 sites in the same countries. Volumetric magnetic susceptibility of the laboratory samples was measured to evaluate the effects of magnetic susceptibility on the T1/T2 ratio. Our results indicate that the T1/T2 ratios in mineral soils and sediments are pretty similar for borehole NMR and lab NMR datasets, regardless of the geological unit. In these geological materials, the mean value of the T1/T2 ratios is 1.64 in lab-NMR and 1.82 in borehole NMR datasets. In contrast, in our in-situ borehole NMR measurements in organic peat soils, the mean value of the T1/T2 ratios was higher (i.e. 2.77), exhibiting a broader distribution ranging from 1 to 4.8. Moreover, we observed that magnetic susceptibility did not have a significant effect on the T1/T2 ratio in the investigated samples. More importantly, the findings in this study can be adopted in the modeling of steady-state surface NMR modeling routines where a constant ratio of 1 for T1/T2 is assumed when solving the Bloch equations. It is expected that updating the T1/T2 ratio can improve the accuracy of water content and relaxation time estimations derived from steady-state surface NMR measurements.

SummaryIn this study, the microseismicity and damage-zone characteristics of a locked fault are investigated on a major left-lateral strike slip fault segment north of the Dead Sea Lake, the Jericho Fault (JF). The JF was observed as seismically silent for ${M}_w > 2$ earthquakes during recent decades, although it has generated significant earthquakes in the past. We extend seismological observations towards the microseismic range by deploying nine strong motion accelerometers directly on the inferred surface trace. From one year of continuous recordings (06/22–06/23) we found 61 seismic events in the range of 0.9 < ${M}_w$< 2.4, that are below the detection threshold of the permanent regional network. Most of these events are located west of the fault zone and represent activity on other smaller faults, with only three events located along the JF zone itself. We also found that the JF is more seismically quiescent than an analogous segment of the San Jacinto Fault (California)—the Anza gap, indicating that the JF is a particularly quiet fault segment even for microseismic activity and therefore, may be accumulating significant elastic strain energy along the locked-creeping boundary. The JF segment shows a characteristic earthquake distribution behaviour that could reasonably cause an earthquake of ${{\rm{M}}}_{\rm{w}}$ ∼ 7–7.4 if all strain energy, accumulated since the last major earthquake in 1033 AD, is released seismically in a single event. We also provide a new observational-based approach to characterise fault zone properties from trapped waves’ delay-times. Here we emphasise the damage zone velocity as the endmember on a continuum of discrete velocity values that progressively decrease towards the fault. This approach can be applied to other fault zones assisting in characterising rupture zone properties of fault segments. We report the first trapped waves observations at the Dead Sea Transform, caused by waves propagating along a damaged segment of the JF fault zone. We introduce a new trapped-waves inversion scheme, solely data driven, that does not make use of synthetic seismograms and model-based pre-assumptions. The JF coherently trends northwards from the Dead Sea Lake, showing a fault zone trapped-wave velocity estimation of 0.95 -1.15 ${\rm{km\ }}{{\rm{s}}}^{{\rm{ - 1}}}$ with $\~$35 per cent reduction from the surrounding host rock to the fault's damaged rock. A significant velocity drop is observed at the Jericho Escarpment reflecting a geological transfer from hard rock to soft sedimentary layers, towards the Jericho Fault. The trapped-waves inversion indicates ∼16 km of coherently damaged rock trending northwards from the Dead Sea Lake; this serves as a minimum estimate of the JF length, and appears to coincide with the silent section of the JF, rather than extending coherently further north.

SummaryThis study presents the results of an interlaboratory test designed to evaluate the accuracy of Spectral Induced Polarization (SIP) measurements using controlled electrical test networks. The study, conducted in Germany since 2006, involved 12 research institutes, six different impedance measurement devices, and four types of electrical test networks specifically designed to evaluate phase shift errors in SIP measurements. The test networks, with impedances ranging from 100 kΩ to 150 kΩ, represent high-impedance samples with different phase characteristics, and pose the measurement challenges typical of such samples, including high contact impedances and parasitic capacitances. Four key findings emerged from the study: (1) Impedance measurements across all devices showed deviations within 1% over a wide frequency range (0.001 Hz - 1000 Hz); (2) phase errors remained below 1 mrad up to 100 Hz for most devices, but increased at higher frequencies due to parasitic capacitances and electromagnetic coupling effects; (3) lab-specific instruments have lower phase errors than field instruments when used in a laboratory environment, primarily due to the effects of long cables and too low input impedances of the field instruments; and (4) short cables and driven shielding technology effectively minimized parasitic capacitance and improved measurement accuracy. The study highlights the usefulness of test networks in assessing the accuracy of SIP measurements and raises awareness of the various factors influencing the quality of SIP data.

SummaryGas-bearing sediments in shallow-water environments have recently attracted attention from the perspectives of energy resources, potential geohazards, and climate change. Our laboratory measurements demonstrate the potential for gas-bubble manipulation in gas-bearing sands via radiating repeated pulse signals. By monitoring the temporal changes in the waveform of repeated ultrasonic pulse irradiation with a dominant frequency of 100 kHz transmitted through gas-bearing sand, we observe energy amplification and a frequency shift toward the dominant frequency in the recorded waveforms over 880 h. These results imply that gas bubbles may deform or move autonomously to propagate irradiated ultrasonic waves most efficiently and thereby minimize the energy loss of the transmitted waves. Gas bubbles larger than sand grains detected using three-dimensional X-ray computed tomography cannot explain the phenomena of energy amplification and frequency shifts, indicating the need for a higher spatial resolution to capture the behavior of smaller gas bubbles.

SummaryAirborne magnetotelluric (AirMT) systems generate transfer function data from magnetic fields measured in the air and either electric or magnetic fields measured at a base station. AirMT anomalies are fundamentally controlled by the anomalous magnetic fields within the survey region. While AirMT data acquired using a magnetic field base station are not directly sensitive to the conductivity at the base station, AirMT data acquired using an electric field base station are scaled by the inverse square root of the conductivity at the base station. The transfer function data collected by various AirMT systems have different sensitivity functions. Consequently, the inversion of AirMT data for different acquisition systems may not recover the same conductivity model for the same set of inversion parameters. In this paper, we aim to characterize the fundamental similarities and differences between AirMT inversion for data collected using a magnetic field base station, and for data collected using an electric field base station. We adopt an unconstrained, smoothest model inversion approach to characterize the structures that are naturally recovered by inverting AirMT data when the base station is far away and located on the surface of a homogeneous quarter-space. Our work shows that when a-priori knowledge of the host conductivity within the survey region is available, AirMT inversion effectively recovers conductive and resistive structures within the survey region, regardless of whether the data are collected using an electric or magnetic base station. We show that a single ground magnetotelluric station might provide enough information about the host conductivity to construct a suitable starting model for AirMT inversion, and we discuss the impact of jointly inverting AirMT data and ground magnetotelluric data for a single station.

SummaryThe global oceans are a noisy environment with characteristic acoustic and seismic soundscapes. The enclosed, sea ice-covered Arctic Ocean constitutes a particular noise environment that is rapidly changing. Here, we present a first, comprehensive description of the seismic soundscape of the Arctic Ocean recorded by ocean bottom seismometers especially equipped for the operation in sea ice. They were deployed at 4 km water depth in the Laptev Sea near the sea ice edge in September 2018 and recovered one year later. Analysis of the spectral power between 20 s and 60 Hz demonstrates that ambient noise levels are generally very low compared to other ocean bottom seismic records. Distinct noise bands at high frequencies (>6 Hz) characterize the winter time and are likely caused by the deformation of sea ice emitting seismic signals recordable at the ocean bottom over tens of kilometers. Sea ice noise decays suddenly in May while sea ice concentration is still 100 per cent, but freezing stops and compressional stresses decrease. It only gradually develops in autumn as sea ice becomes thicker, brittle and internally stressed. Microseisms with frequencies of 0.2-2 Hz appear with open water on the Laptev Shelf. Swell events in autumn cause large microseisms and high-frequency noise although ice-noise is not yet present in this season. Ice concentration decreases following the swell events, showing the impact of swell on the sea ice. Ocean bottom seismic records thus represent a powerful tool to monitor the interplay between wave action in the emerging Arctic Ocean and the physical state of its sea ice cover.

SummaryGeologically, Europe consists of a combination of Phanerozoic and Precambrian terranes. Our research focuses on understanding the collision and suture zones between these terranes by imaging the lithosphere-asthenosphere boundary (LAB) and the mid-lithospheric discontinuity (MLD) using seismic S-to-P converted waves. The amount of available data from permanent broadband stations and temporary deployments has significantly increased in recent years. This development allows us to resolve new details regarding continental collisions in Europe.We interpret the new data to show that the Scandinavian MLD extends southward beneath the Caledonides and Variscides, reaching as far as the Bohemian Massif. We have also identified a west-dipping seismic phase extending from the East European Platform (EEP) to the centre of the Pannonian Basin. This phase could represent the MLD of the EEP, akin to the collision between Scandinavia and Phanerozoic Europe in the north. To support these novel findings, geodynamic modelling is required to explain the processes leading to such a structure, which is beyond the scope of this paper. Below the Alps, we confirm earlier observations of the European plate subducting below the Adriatic lithosphere.

SummaryFault Zone Head Waves (FZHW) are a key diagnostic tool to identify bimaterial interfaces along fault zones. We detect and analyze FZHW recorded in the waveforms from the local MONGAN (MONitoring of the GANos Fault) seismic network along the Ganos section of the North Anatolian Fault Zone, northwestern Türkiye, between October 2017 and July 2019. MONGAN covers the Ganos fault with different inter-station distances ranging from 25 m to ∼4 km. To detect FZHW, an automatic detector is used as a preliminary analysis method followed by manual revision and particle-motion analyses to distinguish between FZHW and direct P waves. FZHWs are predominantly detected at the southern side of the fault. The observed FZHWs have a moveout (∆t) with respect to the direct P arrivals, increasing with distance traveled along the fault and indicating a deep bimaterial interface down to the bottom of the seismogenic crust. The average velocity contrast is estimated to be 5.9% across the fault. Near fault-recordings indicate that the Ganos Fault is offset by ∼250 m with respect to the surface trace obtained from literature. To a lesser extent, FZHW are also observed in the northern stations from the fault, indicating a shallow wedge-shaped low-velocity portion constituted by highly fractured material to either side along the southwestern section of the Ganos Fault between the fast Eocene block to the north and the slow Miocene block to the south. The seismic velocity contrast and geological complexity have important implications for the rupture evolution during future earthquakes on the Ganos fault in that they would progress predominantly westward, away from Istanbul and Tekirdağ. Furthermore, an asymmetric aftershock distribution skewed to the northern block can be expected, with subsequent implications for site-dependent risk there. Our results allow to revise focal mechanism solutions by separating FZHW from direct-P wave for previous Sea of Marmara earthquakes.

SummaryBorehole breakout (BO) has increasingly been utilised to estimate in-situ stress magnitudes given the importance of the stress field in subsurface activities and the limitations of conventional stress measurement techniques. In this study, a new backpropagation neural network model is developed to estimate both maximum and minimum horizontal stress magnitudes from multi-scale BO data. A total of 150 experimental data points from pre-stressed true-triaxial laboratory tests and 44 field data from a mine site in Australia and the literature are collected and employed for model development and validation. Compared to previous studies, the collected dataset is significantly enhanced in both quantity and quality. To address discrepancies in stress magnitudes between experimental and field data, the three principal stresses are normalised by borehole wall strength (BWS). Overall, the model achieves mean absolute percentage errors of below 8% for the maximum horizontal stress and below 20% for the minimum horizontal stress, significantly outperforming the previous model developed for this purpose. Furthermore, these error rates fall within the typical error range (10-20%) of conventional stress measurement techniques, indicating the model's sufficient accuracy for practical applications. Moreover, the effectiveness and generalisability of the model are verified using 166 additional BOs from two mine sites, which are independent of those used in model development. Continuous and detailed stress profiles are established based on these BOs, covering greater depth intervals than the stress measurements from the overcoring method. The results of this study demonstrate that the proposed model can provide reliable and accurate stress estimation, utilising input parameters that can be readily obtained from borehole geophysical logs.

SummaryThe behavior of uniaxial single domain magnetite particles in rock and paleomagnetic experiments was first described in the 1940s by Néel and Stoner and Wohlfarth. Since this time, micromagnetism has allowed us to gain a better understanding of magnetic particles in the single vortex or multi-domain states. By contrast, when describing the behavior of assemblages of single domain particles, simplifying assumptions made in the 1940s are still used today. In particular, most rock and paleomagnetic simulations involve magnetite with a uniaxial anisotropy. These assumptions are not necessary in the modern day, as data on other magnetic minerals has been collected, and modern computers are powerful enough to easily calculate the behavior of multiaxial particles. We present a new software package called the Single Domain Comprehensive Calculator (SDCC). This package can simulate a large number of thermally activated rock and paleomagnetic experiments with distributions of single domain particles. These include acquisition of viscous remanence, thermal demagnetization experiments, hysteresis loops, and paleointensity protocols. The package provides a simple Python scripting interface for users to define custom experiments and run models on a laptop computer. Preliminary simulations run with the SDCC demonstrate that magnetocrystalline anisotropy can have a significant effect on the thermoviscous behavior of single domain particles, despite normally being ignored in models. This highlights a need for further investigation into the behavior of single domain particles.

SummaryIn this study, a modified two-dimensional gravimetric inversion algorithm is presented that is based on the reversible-jump Markov chain Monte Carlo (RJMCMC) method with the Talwani equation. To ensure the validity of the Talwani equation and accurate gravity anomaly calculations, the Shamos-Hoey algorithm is incorporated as an additional acceptance condition to prevent intersections in the model polygon. This improves upon the method proposed by Luo by iteratively refining a polygon model based on gravity anomalies while maintaining physical validity. Additionally, we suggest a revision of the prior density function to better test the proposal models. This method estimates the shape and location of subsurface intrusions, providing valuable insights into subsurface geological structures. This positions the algorithm as a valuable tool for geophysical research.

SummaryNear-field large-amplitude seismograms are essential for the rapid inversion of earthquake source parameters using waveform inversion methods such as the Cut And Paste (CAP) method for disaster assessment. High-rate Global Navigation Satellite System (GNSS) relative positioning (RP) provides precise, rapid, and real-time measurement of near-field large-amplitude displacements. However, RP records motion with respect to a reference station, and the reference station's movements become part of the relative displacement waveforms. Therefore, seismic source parameter estimates may be inaccurate if the reference station's motion is not taken into consideration, and doing so affects some basic assumptions made in the CAP method. To overcome this problem, we develop an expanded differential CAP inversion approach specifically for high-rate GNSS RP (CAP-RP) that accounts for the motion of the reference station. Two methods are proposed to implement CAP-RP: an expanded differential CAP (D-CAP) and an iterative post-processing CAP (P-CAP). We assess the performance of CAP-RP with different datasets, using the July 2019 Mw 6.4 earthquake in California as a case study. Both CAP-RP techniques produce accurate source parameters in synthetic data inversion tests, indicating the feasibility of the strategy. However, P-CAP is more time-efficient than D-CAP, making it the better option. Generally, results from high-rate GNSS RP, broadband seismographs, and their inverted combinations exhibit consistency in observational data inversion testing. Our results also demonstrate that more accurate source parameters can be obtained by combining sensitive far-field broadband seismograph data with large amplitude near-field GNSS RP waveforms.

SummarySpectral induced polarization (SIP) has been suggested as a non-invasive and cost-effective tool to detect and monitor aromatic rich organic matter such as biochar. In our study, we show that SIP can track biochar concentration up to 10% (wt.) in a soil with a clay content of 20%. Assessment of changes in the concentration of biochar was conducted according to double Pelton parameters and the maximal phase determined at 11.7 Hz, a frequency at which a polarization peak is observed in the presence of biochar. All SIP-derived parameters were correlated with the biochar content, with the exception of the relaxation time of the polarization peak occurring at 11.7 Hz, which was related to soil water saturation in previous investigations. Among studied parameters, the phase value that we measured at 11.7 Hz may therefore consist in a simple and reliable methodology to evaluate the biochar content on SIP in our experiment. Several steps are still necessary before a widespread field application notably by considering how modifications in the chemistry of biochar with time can interact with biochar concentration and water saturation to modify polarization processes shaping SIP curves. Beyond the scope of tracking changes in the content of highly aromatic OM – such as biochar - in soils, this study suggests that the degree of aromaticity of OM can play a key role in the SIP response paving the way for wider use of SIP in soil science.

SummaryLong-period seismic events (LPs) are observed within active volcanoes, hydrothermal systems, and hydraulic fracturing. The prevailing model for LP seismic events suggests that they result from pressure disturbances in fluid-filled cracks that generate slow, dispersive waves known as Krauklis waves. These waves oscillate within the crack, causing it to act as a seismic resonator whose far-field radiations are known as LP events. Since these events are generated from fluid-filled cracks, they have been used to analyze fluid transport and fracturing in geological settings. Additionally, they are deemed precursors to volcanic eruptions. However, other mechanisms have been proposed to explain LP seismicity. Thus, a robust interpretation of these events requires understanding all parameters contributing to LP seismicity. To achieve this, for the first time, we have developed a physical model to investigate LP seismicity under controlled-source conditions. The physical model consists of a 30 cm × 15 cm × 0.2 cm crack embedded within a concrete slab with dimensions of 3 m × 3 m × 0.24 m. Using this apparatus, we investigate fundamental factors affecting long-period seismic signals, including crack stiffness, fluid density and viscosity, radiation patterns, and triggering location. Our findings are consistent with the theoretical model for Krauklis waves within a fluid-filled crack.In this study, we examine the interplay between fluid properties and characteristics of waves within and radiated from the crack model. Records from a pressure transducer within the crack model have the same frequency characteristics as the surface sensors, indicating that the surface sensors are recording the crack waves. Because the crack stiffness parameters for all the fluids are relatively high, fluid density variations have a larger effect on the crack wave frequency, with higher density fluids yielding lower resonance frequencies. Similarly, the quality factor (Q) decreases with increasing fluid density. We also find that an increase in fluid viscosity along with the increased fluid density results in a decrease in resonance frequency and Q. Trigger locations at the middle of the crack length and width most effectively resonated the first and second transverse modes. Thus, this physical model can offer new horizons in understanding LP seismicity and bridge the gap between theoretical models and observed LP signals.

SummaryMany geophysical studies require knowledge on the present-day temperature distribution in Earth’s mantle. One example are geodynamic inverse models, which utilize data assimilation techniques to reconstruct mantle flow back in time. The thermal state of the mantle can be estimated from seismic velocity perturbations imaged by tomography with the help of thermodynamic models of mantle mineralogy. Unique interpretations of the tomographically imaged seismic heterogeneity can either be obtained by incorporating additional data sets or requires assumptions on the chemical composition of the mantle. However, even in the case of (assumed) known chemical composition, both the seismic and the mineralogical information are significantly affected by inherent limitations and different sources of uncertainty. Here, we investigate the theoretical ability to estimate the thermal state of the mantle from tomographic models in a synthetic closed-loop experiment. The ‘true’ temperature distribution of the mantle is taken from a 3-D mantle circulation model with Earth-like convective vigour. We aim to recover this reference model after: 1) mineralogical mapping from the ‘true’ temperatures to seismic velocities, 2) application of a tomographic filter to mimic the effect of limited seismic resolution, and 3) mapping of the ‘imaged’ seismic velocities back to temperatures. We test and quantify the interplay of tomographically damped and blurred seismic heterogeneity in combination with different approximations for the mineralogical ‘inverse’ conversion from seismic velocities to temperature. Owing to imperfect knowledge of the parameters governing mineral anelasticity, we additionally investigate the effects of over- or underestimating the corresponding correction to the underlying mineralogical model. Our results highlight that, given the current limitations of seismic tomography and the incomplete knowledge of mantle mineralogy, magnitudes and spatial scales of a temperature field obtained from global seismic models deviate significantly from the true state, even in the idealized case of known bulk chemical composition. The average deviations from the reference model are on the order of 50–100 K in the upper mantle and – depending on the resolving capabilities of the respective tomography – can increase with depth throughout the lower mantle to values of up to 200 K close to the core-mantle boundary. Furthermore, large systematic errors exist in the vicinity of phase transitions due to the associated mineralogical complexities. When used to constrain buoyancy forces in time-dependent geodynamic simulations, errors in the temperature field might grow non-linearly due to the chaotic nature of mantle flow. This could be particularly problematic in combination with advanced implementations of compressibility, in which densities are extracted from thermodynamic mineralogical models with temperature-dependent phase assemblages. Erroneous temperatures in this case might activate ‘wrong’ phase transitions and potentially flip the sign of the associated Clapeyron slopes, thereby considerably altering the model evolution. Additional testing is required to evaluate the behaviour of different compressibility formulations in geodynamic inverse problems. Overall, the strategy to estimate the present-day thermodynamic state of the mantle must be selected carefully to minimize the influence of the collective set of uncertainties.

SummaryGeomagnetic observations at Eskdalemuir observatory in Southern Scotland reveal reduced amplitudes in the vertical component variations compared with the horizontal components for periods of less than an hour. A subsurface high conductivity feature has previously been suggested to account for this anomaly. However, past studies have overlooked the effect of seasonal source changes and impact of solar activity on external geomagnetic field variations. The vertical magnetic transfer function - referred to as the tipper - relates temporal variation in the vertical magnetic field to those in the horizontal magnetic field and is sensitive to lateral electrical conductivity contrasts in the subsurface. Quantifying the seasonal variations in the tipper helps to identify times when external field variations minimally bias tipper estimates, thereby providing a more accurate representation of subsurface conductivity. Ionospheric current systems, particularly during geomagnetic storms, may violate the plane wave assumption underlying tipper estimation at mid-latitudes. This may allude to a more complex source geometry responsible for magnetic field variations. Our study quantifies and proposes a correction for space weather-driven external field contributions to observations for periods shorter than one hour. Using high-quality digital magnetic field data with a one-minute sampling rate from 2001 to 2019, we estimate the tipper at Eskdalemuir, revealing seasonal differences that increase with periods between 1000 s and 10000 s. After finding that tipper estimates during the 2016 time series are least affected by seasonal effects, we used one-second time series and a simple empirical model to quantify the daily variability of the tipper. The model consists of annual and semi-annual terms plus a term proportional to either the F10.7 cm solar flux or geomagnetic Ap index. Neither model fits the data to within the expected error, but the model that uses Ap has better fit. Tipper estimates from temporary site deployments are affected by these seasonal external variations, and we correct those obtained at sites near Eskdalemuir during a recent field experiment using this model.

SummaryControlled-source marine seismic experiments are key in advancing our understanding of the Earth’s subsurface structure to study tectonic, magmatic, sedimentary and fluid flow processes. Joint acquisition of Wide-Angle Seismic (WAS) and Multi-Channel Seismic (MCS) streamer data stands as the most robust approach for marine exploration, however effectively mapping subsurface structure remains challenging. The lack of identifiable refractions as first arrivals at short offsets in WAS data creates shallow subsurface illumination gaps up to 6-8 km offsets around Ocean Bottom Seismometers or Hydrophones (OBS/OBH). This inadequate ray coverage, more pronounced in areas with deeper water column and lower seabed velocities, limits the performance of Travel Time Tomography (TTT) techniques. Velocity determination in the sedimentary layer and reflector location are affected, and errors propagate to deeper layers. This study integrates Downward Continuation (DC) to WAS data. Similarly to our former study where DC is applied to MCS data, redatuming WAS data involves solving the acoustic wave equation backward in time. This process virtually repositions the sources to the seafloor, revealing previously masked near-seafloor refractions as first arrivals. This transformation significantly enhances ray coverage in the shallow subsurface, leading to more accurate determinations of both seismic velocity and reflector geometry. By bridging theoretical concepts with a real data application, this study demonstrates the optimization of field seismic data for improved TTT results. This methodology is particularly beneficial for deep water exploration where spatially coincident WAS and MCS are jointly inverted. In such scenarios, DC-processed WAS data provides the refracted phases key for velocity determinations, and that are typically not present in MCS data due to insufficient streamer length relative to the water column depth. Additionally, we contribute to the community by releasing our open-source, High-Performance Computing (HPC) software for WAS data redatuming.

SummaryMexico City is one of the largest cities in North America, facing high seismic hazards and water supply problems. This paper presents an ambient seismic noise tomography of the city's south area in Xochimilco, where large amplifications have already been registered during subduction earthquakes. Eighty-four seismic stations have been installed, and their records processed. The tomography method combines the inversion of the Horizontal-to-Vertical Spectral Ratios (HVSR) and multimodal dispersion curves. The importance of considering a multimodal approach is justified in light of the complex geological setting. The dispersion curves analysis shows that the surface wave energy is divided over the fundamental and the higher modes, particularly between 50 and 300 m/s, and in the whole frequency range analyzed. We observe a spatially continuous decrease of the dominant peak frequency of the HVSRs toward the lake interior but a heterogeneous amplification. By analyzing the velocity profiles associated with the highest amplifications, we discovered that these latter result from the superposition of several resonance peaks. Their coincidence in frequency is due to the overall constant linear gradient velocity in the sedimentary basin crossed by several low-velocity anomalies due to high water content or high-velocity anomalies due to lavas. Although most of the shallow water is trapped in clay sediment, the velocity model also allows for identifying deeper water reserves. All these analyses are of fundamental importance for the correct seismic mitigation in Mexico City but might also be extended to other cities built on top of sedimentary basins.

SummaryIn geodetic slip inversions, resolution decreases rapidly with depth because deformation data are measured at the ground surface. Traditionally, this decrease in resolution has been attributed to the weak deformation signals caused by slips at greater depths. However, this study demonstrated that the primary cause is the stronger smoothing applied to deeper slips compared to shallower ones. This work proposes a method that scales the Green's functions to equalize smoothing effects across depths. The method's effectiveness was validated through both synthetic tests and real earthquake applications. In synthetic tests, it improved recovery of deep slips in both location and amplitude. When applied to the 2008 MW7.9 Wenchuan earthquake, the method produced smaller slips near the ground surface and larger slips at depth. For the land-based deformation inversion of the 2011 MW9.0 Tohoku earthquake, the method resulted in larger shallow slips near the trench and greater sea-floor uplift compared to the conventional inversion, which is valuable for accurate prediction of tsunami wave height. Additionally, this method may also be applicable to other inversions where smoothing is used and observation amplitudes vary with distance.

SummaryLocating earthquakes plays an important role in the study of seismic activity and geological structures. Traditional methods for locating earthquakes mainly rely on waveform matching and travel time fitting. With the development of artificial intelligence technology, machine learning methods have often been applied to locate earthquakes. However, current machine learning approaches may face challenges related to physical constraints. In this study, we build a 3D U-Net network with station distribution constraints to locate earthquakes. To improve the generalizability of the network model, we apply data augmentation techniques, including data shifting, selection, rotation, and fusion. The location results are evaluated using a testing dataset from Oklahoma, showing an average location error of about 5 km. The origin time can be determined based on the earthquake's location and the waveforms recorded by stations through waveform shifting and stacking. This method does not require the complex processing steps of traditional seismic approaches, allowing for rapid earthquake location. Additionally, we apply the network model to data recorded in Southern California through transfer learning for further application. The results show that this new method is stable and generalized, making it applicable to earthquake location problems associated with arbitrary station networks. Furthermore, we discuss the effects of data augmentation, network architecture, and the Gaussian radius of labels on the outcomes. These insights help us better understand machine learning algorithms and improve the application of deep learning in earthquake location.