D. D. Billett, R. A. Rohel, C. J. Martin, K. A. McWilliams, K. M. Laundal
{"title":"The Fast Borealis Ionosphere: High Time-Resolution Mapping of Polar Ionospheric Flows With SuperDARN","authors":"D. D. Billett, R. A. Rohel, C. J. Martin, K. A. McWilliams, K. M. Laundal","doi":"10.1029/2024EA003876","DOIUrl":"https://doi.org/10.1029/2024EA003876","url":null,"abstract":"<p>Recent improvements to hardware for the Super Dual Auroral Radar Network systems have allowed for a much greater control of radar transmit and receive functionalities than previously possible. One of these functionalities is the application of a new operational mode, known as wide-beam, which vastly improves the temporal resolution of the radars without compromising their spatial coverage. Wide-beam allows for the retrieval of line-of-sight ionospheric drift velocities at a temporal resolution of 3.7 s, a sixteen-fold improvement from the one-minute resolution offered by traditional operational modes. In this paper, we use wide-beam data from the Borealis SuperDARN systems, located in Canada, to derive local horizontal ionospheric plasma velocity fields above Northern Canada, Greenland, and the polar cap, at a 3.7 s temporal resolution. For this local fitting of ionospheric velocity data, we use the Local Mapping of Ionospheric Electrodynamics (Lompe) spherical elementary current systems technique. This new data product, which we call the Fast Borealis Ionosphere, is compared to both the global SuperDARN spherical harmonic convection pattern data product (the Map Potential technique), as well as Lompe convection patterns derived using the traditional SuperDARN narrow-beam scanning mode. We show that Lompe systematically produces a better representation of the underlying radar velocity data than Map Potential, that the 3.7 s wide-beam data contains a significant amount more ionospheric variability than narrow-beam, and that the high time-resolution convection patterns can resolve dynamic ionospheric events lasting on the order of tens of seconds.</p>","PeriodicalId":54286,"journal":{"name":"Earth and Space Science","volume":"12 6","pages":""},"PeriodicalIF":2.9,"publicationDate":"2025-06-06","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1029/2024EA003876","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"144220167","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Asiye Aziz Zanjani, Heather R. DeShon, Vamshi Karanam, Alexandros Savvaidis
{"title":"Insights Into Spatiotemporal Evolution of Induced Earthquakes in the Southern Delaware Basin Using Calibrated Relocations From the TexNet Catalog (2017–2022)","authors":"Asiye Aziz Zanjani, Heather R. DeShon, Vamshi Karanam, Alexandros Savvaidis","doi":"10.1029/2024EA004027","DOIUrl":"https://doi.org/10.1029/2024EA004027","url":null,"abstract":"<p>This study presents a comprehensive analysis of induced seismicity (2017–2022) and InSAR-derived surface deformation in the southern Delaware basin. The relocated catalog features improved 3-D locations for 5,453 events from the Texas Seismological Network through nested inversions, rigorous data calibration, and additional S-P phase-time differences for seismic stations within 10 km distance. Time and space variations in absolute and relative earthquake location errors reflect the complicated history of station coverage in the region and the importance of having close-in stations to resolve shallow-depth earthquakes. The mean seismogenic depth of the new catalog is 1.5 km below mean-sea-level, consistent with reactivation of shallow normal faults within the Delaware Mountain Group (DMG) and the Bone Spring Formation driven by shallow saltwater disposal. Linearly segmented, short-wavelength subsidence patterns align with seismically active lineaments interpreted as shallow normal faults, while long-wavelength production-related subsidence signals are radially symmetric and aseismic where they do not coincide with injection hotspots and faults. The revised M2+ catalog maps a reduction in the number of events in the northern and central parts as well as an increase in the number of events in the southeast since 2020, and this signal precedes measurable surface deformation. We posit that this relationship reflects efficient pressure diffusion along permeable northwest-southeast faults and/or the thickening of porous sandstone in the DMG prone to seismic slip. The spatial and temporal patterns of seismicity, uplift-subsidence, and basin-wide fluid extraction and disposal indicate inhomogeneous and time-variant seismic and aseismic deformation under an anthropogenically modulated stress regime.</p>","PeriodicalId":54286,"journal":{"name":"Earth and Space Science","volume":"12 6","pages":""},"PeriodicalIF":2.9,"publicationDate":"2025-06-05","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1029/2024EA004027","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"144214176","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Chia-Lun Tsai, Kwonil Kim, Heechul Park, Hongmok Park, Wonbae Bang, GyuWon Lee
{"title":"Association Between Upstream Conditions and the Intensity of Orographic Precipitation in the Main Mountain Ranges of South Korea","authors":"Chia-Lun Tsai, Kwonil Kim, Heechul Park, Hongmok Park, Wonbae Bang, GyuWon Lee","doi":"10.1029/2024EA003989","DOIUrl":"https://doi.org/10.1029/2024EA003989","url":null,"abstract":"<p>This study uses high temporospatial surface precipitation rate obtained from radar observations (hybrid surface rainfall, HSR), 3D winds retrieved from the Wind Synthesis System using Doppler Measurements (WISSDOM), and 3D thermodynamic fields to investigate the association between orographic precipitation and upstream conditions for the main mountain ranges of South Korea during the 2018–2020. The main objective was to determine the dominate meteorological factors affecting the rain intensity over this terrain. Three rainfall cases were analyzed covering western, and eastern slopes of the Taebaek mountain range (TMR), Mt. Jiri, and Busan City. Correlation coefficients (<span></span><math>\u0000 <semantics>\u0000 <mrow>\u0000 <mi>R</mi>\u0000 </mrow>\u0000 <annotation> $R$</annotation>\u0000 </semantics></math>) were used to evaluate the strength of the relationship between rain intensity and meteorological factors in these regions, including the wind directions, wind speed, Froude number, saturated Froude number, water vapor, moist flux, stability, vertical velocity, and convergence. The results revealed that the wind direction determined the location of precipitation in the mountains, with the wind speed and moist flux identified as the most influential factors for rain intensity, with high correlation coefficients of 0.55–0.85. The upstream Froude number appeared to modulate the orographic enhancement on rain intensity over Mt. Jiri and the western slopes of the TMR. Low-level convergence was another critical factor affecting the rain intensity along the northeastern coast of South Korea (i.e., the eastern slopes of the TMR) and Busan (<span></span><math>\u0000 <semantics>\u0000 <mrow>\u0000 <mi>R</mi>\u0000 </mrow>\u0000 <annotation> $R$</annotation>\u0000 </semantics></math> of ∼0.6–0.7). Statistical analysis of all orographic precipitation cases (52 cases over the 3 years) revealed that the upstream wind speed, and moist flux in the mid-layers had a higher correlation with rain intensity over the western slopes of the TMR and Mt. Jiri. The relationship between rain intensity and both water vapor and low-level convergence was also stronger along the northeastern coast of South Korea.</p>","PeriodicalId":54286,"journal":{"name":"Earth and Space Science","volume":"12 6","pages":""},"PeriodicalIF":2.9,"publicationDate":"2025-06-05","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1029/2024EA003989","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"144213751","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Evaluation of Vegetation Bias in InSAR Time Series for Agricultural Areas Within the San Joaquin Valley, CA","authors":"Kelly R. Devlin, Rowena B. Lohman","doi":"10.1029/2024EA004062","DOIUrl":"https://doi.org/10.1029/2024EA004062","url":null,"abstract":"<p>Agricultural regions present a particularly difficult set of challenges during interferometric synthetic aperture radar (InSAR) displacement time series analyses due to the existence of abrupt transitions in land use over short spatial scales and rapid temporal changes associated with different stages of the agricultural cycle. Plant growth and soil moisture changes can introduce phase biases within interferograms that could be misinterpreted as displacement. We analyze a full-resolution, multi-year SAR time series over California's San Joaquin Valley, an intensively cultivated region producing a wide variety of crops. Using independent information about land cover and crop type, we isolate the effects of individual crops on backscatter amplitude, interferometric phase change, and interferometric coherence over space and time. We determine the temporal behavior of the phase changes associated with several key crop types by isolating the difference between the phase of pixels averaged over each agricultural field and the phase values of pixels in nearby roads and developed areas. We find that some fields are associated with a bias of ∼2–4 cm/yr of apparent subsidence, with strong seasonal variability in the degree of bias. When InSAR imagery is spatially averaged or filtered, these biases also impact the inferred phase in nearby roads and other land cover types. We show that even a simple approach, where pixels associated with agricultural fields are removed or masked out before further processing, can mitigate the crop-related biases that we observe in the study area.</p>","PeriodicalId":54286,"journal":{"name":"Earth and Space Science","volume":"12 6","pages":""},"PeriodicalIF":2.9,"publicationDate":"2025-06-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1029/2024EA004062","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"144206445","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Mechanism of Multiple Anomalies Prior to Japan Earthquakes From 2021 to 2023: Lithosphere-Coversphere-Atmosphere-Ionosphere Coupling Driven by Pressure-Stimulated Rock Current","authors":"Busheng Xie, Lixin Wu, Licheng Sun, Youyou Xu, Akimasa Yoshikawa, Wenfei Mao","doi":"10.1029/2025EA004320","DOIUrl":"https://doi.org/10.1029/2025EA004320","url":null,"abstract":"<p>This study investigated the underlying mechanism of multiple anomalies preceding the earthquakes occurred in Japan from 2021 to 2023. Key parameters, including induced magnetic field (IMF), atmospheric electric field (AEF), and total electron content (TEC), were analyzed to explore their spatiotemporal relationships with seismic activity. The IMF, AEF, and TEC anomalies were found to consistently appear a few days or hours preceding the earthquakes, following a clear temporal sequence. By integrating multi-source data and excluding external factors such as weather conditions and solar activity, this study identified strong correlations between the anomalies and seismic events. Spatially, these anomalies were concentrated near the seismogenic zones. Additionally, a linear relationship was observed between the electric parameters derived from IMF and AEF anomalies. The lithosphere-coversphere-atmosphere-ionosphere (LCAI) coupling driven by pressure-stimulated rock current (PSRC) is supposed essentially possible. The LCAI coupling explains how tectonic stress triggers the migration of positive hole (p-hole) charges from the lithosphere to ground surface, thereby influencing both the atmosphere and ionosphere. The geological conditions of the study area, which is rich in igneous rocks such as granite and andesite embodied with massive peroxy bonds, lead to the generation of PSRC. By comparing the timing differences between the anomalies, a deeper understanding of how pre-seismic electric and magnetic signals evolve and interact across different geospheres was proposed, which could be referenced for earthquake prediction especially in this particular region.</p>","PeriodicalId":54286,"journal":{"name":"Earth and Space Science","volume":"12 6","pages":""},"PeriodicalIF":2.9,"publicationDate":"2025-06-03","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1029/2025EA004320","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"144206492","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Multitaper Magnitude-Squared Coherence for Time Series With Missing Data: Understanding Oscillatory Processes Traced by Multiple Observables","authors":"Sarah E. Dodson-Robinson, Charlotte Haley","doi":"10.1029/2025EA004256","DOIUrl":"https://doi.org/10.1029/2025EA004256","url":null,"abstract":"<p>To explore the hypothesis of a common source of variability in two time series, observers may estimate the magnitude-squared coherence (MSC), which is a frequency-domain view of the cross correlation. For time series that do not have uniform observing cadence, MSC can be estimated using Welch's overlapping segment averaging. However, multitaper has superior statistical properties to Welch's method in terms of the tradeoff between bias, variance, and bandwidth. The classical multitaper technique has recently been extended to accommodate time series with underlying uniform observing cadence from which some observations are missing. This situation is common for solar and geomagnetic data sets, which may have gaps due to breaks in satellite coverage, instrument downtime, or poor observing conditions. We demonstrate the scientific use of missing-data multitaper magnitude-squared coherence by detecting known solar mid-term oscillations in simultaneous, missing-data time series of solar Lyman <span></span><math>\u0000 <semantics>\u0000 <mrow>\u0000 <mi>α</mi>\u0000 </mrow>\u0000 <annotation> $alpha $</annotation>\u0000 </semantics></math> flux and geomagnetic Disturbance Storm Time index. Due to their superior statistical properties, we recommend that multitaper methods be used for all heliospheric time series with underlying uniform observing cadence.</p>","PeriodicalId":54286,"journal":{"name":"Earth and Space Science","volume":"12 6","pages":""},"PeriodicalIF":2.9,"publicationDate":"2025-06-03","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1029/2025EA004256","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"144206490","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Method to Improve the Equatorial Components of Effective Angular Momentum Forecasts Based on Real Environments","authors":"Wei Miao, Xueqing Xu, Yonghong Zhou, Cancan Xu","doi":"10.1029/2024EA004174","DOIUrl":"https://doi.org/10.1029/2024EA004174","url":null,"abstract":"<p>The findings from the Second Earth Orientation Parameters Prediction Comparison Campaign (2nd EOP PCC) suggest that integrating effective angular momentum (EAM) is vital for enhancing the accuracy of polar motion (PM) predictions. Building on Dill et al. (2021), https://doi.org/10.1029/2021ea002070, who identified systematic errors in the motion terms of atmospheric angular momentum (AAM), we discovered additional systematic errors in mass and motion terms of forecasts for the AAM, oceanic angular momentum (OAM) and hydrologic angular momentum (HAM), and promptly implemented corrections following their updates. During the hindcast experiment period from 20/5/2021 to 31/12/2023, and in the first three days in the <i>X</i> and <i>Y</i> directions, the proposed method showed advantages over the Helmholtz-Centre Potsdam—German Research Centre for Geosciences (GFZ) and Eidgenössische Technische Hochschule Zürich (ETH Zürich). Then, the corrected EAM forecasts and reference values were used in the PM forecasting experiments, which showed no improvement, likely due to the existing PM forecasting system and overcompensation. However, when employing the perfect analysis of GEAM (the difference between geodesic angular momentum (GAM) and EAM), the proposed method herein achieves a maximum improvement of 30.0% and 55.5% in the <i>X</i> direction and 8.4% and 48.4% in the <i>Y</i> direction, compared to the official EAM forecasts of GFZ and ETH Zürich. This fully demonstrates that improvements in both EAM and GEAM are essential for enhancing PM predictions, and the EAM forecasts corrected by the proposed method are more competitive than those of GFZ and ETH Zürich.</p>","PeriodicalId":54286,"journal":{"name":"Earth and Space Science","volume":"12 6","pages":""},"PeriodicalIF":2.9,"publicationDate":"2025-05-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1029/2024EA004174","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"144179364","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Huan Guo, Levi G. Silvers, David Paynter, Wenhao Dong, Songmiao Fan, Xianwen Jing, Ryan Kramer, Kristopher Rand, Kentaroh Suzuki, Yuying Zhang, Ming Zhao
{"title":"Assessing Clouds in GFDL's AM4.0 With Different Microphysical Parameterizations Using the Satellite Simulator Package COSP","authors":"Huan Guo, Levi G. Silvers, David Paynter, Wenhao Dong, Songmiao Fan, Xianwen Jing, Ryan Kramer, Kristopher Rand, Kentaroh Suzuki, Yuying Zhang, Ming Zhao","doi":"10.1029/2024EA004053","DOIUrl":"https://doi.org/10.1029/2024EA004053","url":null,"abstract":"<p>We evaluate cloud simulations using satellite simulators against multiple observational data sets. These simulators have been run within the Geophysical Fluid Dynamics Laboratory's Atmosphere Model version 4.0 (AM4.0), as well as an alternative configuration where a fully two-moment Morrison-Gettelman cloud microphysical parameterization with prognostic precipitation (MG2) is applied, denoted as AM4-MG2. The modeled cloud spatial distributions, vertical profiles, phase partitioning, cloud-to-precipitation transitions, and radiative effects compare reasonably well with satellite observations. Model biases include the under-prediction of total and low-level clouds, especially optically thin/intermediate clouds with cloud optical depth of less than 23, but the over-prediction of thick clouds, indicating “too few, too bright” biases. These biases counteract each other, and give rise to reasonable estimates of cloud radiative effects. The underestimate of low-level clouds is associated with too early and too frequent drizzle/precipitation formation. The precipitation bias is improved in AM4-MG2, where the autoconversion scheme initiates the precipitation more realistically. There also exist discrepancies between models and observations for midlevel and high-level clouds. Additional biases include the underestimate of liquid cloud fraction and the overestimate of ice cloud fraction.</p>","PeriodicalId":54286,"journal":{"name":"Earth and Space Science","volume":"12 6","pages":""},"PeriodicalIF":2.9,"publicationDate":"2025-05-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1029/2024EA004053","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"144171983","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Analyzing the Inversion Performance of a Permanent Urban Column GHG Network: An OSSE Perspective","authors":"Jun Zhang, Jia Chen, Kai Wu, Haoyue Tang","doi":"10.1029/2024EA004175","DOIUrl":"https://doi.org/10.1029/2024EA004175","url":null,"abstract":"<p>Observations of atmospheric columns offer an effective approach to monitoring greenhouse gas (GHG) emissions, as they are less sensitive to the dynamics of atmospheric transport in comparison to in situ measurements. MUCCnet, the world's first permanent urban ground-based column network, has been utilized as an innovative method for measuring column GHGs. We present here an observing system simulation experiment framework to characterize the behavior of this unique network in estimating urban CO<sub>2</sub> emissions. An assumed in situ tower-based network (AISTnet) is performed to improve our understanding of MUCCnet's observing performance. We conduct a set of Bayesian atmospheric inversions to validate the current network deployment strategy and analyze its sensitivity to large point sources (LPSs). From our base inversions, we found overall good consistency between MUCCnet and AISTnet inversions, with nearly all grid cells showing corrections in the same direction during the inversions. While the sensitivities of in situ CO<sub>2</sub> synthetic observations are approximately an order of magnitude higher than those of column measurements, the column measurements have the advantage of broader coverage. This leads to larger uncertainty reduction around the site locations in the AISTnet inversions, while the MUCCnet inversions present larger values over the area away from the network. The inaccurate information of the LPSs provided in the prior estimate can adversely impact the estimated emissions. Our results suggest that MUCCnet is less sensitive to LPSs errors compared to AISTnet. The findings of this work can contribute valuable insights for advancing future observing strategies in an urban environment.</p>","PeriodicalId":54286,"journal":{"name":"Earth and Space Science","volume":"12 5","pages":""},"PeriodicalIF":2.9,"publicationDate":"2025-05-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1029/2024EA004175","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"144140377","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
K. Stephan, K. Rammelkamp, M. Baqué, S. Schröder, A. Pisello, K. Gwinner, G. Ortenzi, P. Irmisch, F. Sohl, V. Unnithan
{"title":"Multi-Spectral Field Study of Planetary Analog Material in Extreme Environments—Alteration Products of Volcanic Deposits of Vulcano/Italy","authors":"K. Stephan, K. Rammelkamp, M. Baqué, S. Schröder, A. Pisello, K. Gwinner, G. Ortenzi, P. Irmisch, F. Sohl, V. Unnithan","doi":"10.1029/2024EA004036","DOIUrl":"https://doi.org/10.1029/2024EA004036","url":null,"abstract":"<p>The potential of multi-spectral investigations for planetary exploration strongly depends on the specific geologic environment and related science questions. In this work, we used a visible-near infrared spectrometer, a laser-induced breakdown spectroscopy (LIBS) instrument, and a Raman spectrometer for studying acid alteration of volcanic deposits in the field as an analog for what can be potentially observed on Mars. These deposits were studied on Vulcano, one of the Aeolian Islands/Italy, where volcanic deposits are affected by active hydrothermal alteration processes and fumarolic activity. The results show that VIS-NIR spectroscopy is sufficient to identify the major minerals formed through the alteration process. This is the only technique that can identify and characterize hydrated silica, the major alteration residue, whose spectral properties vary depending on environmental conditions and the formation process. However, only LIBS spectra allow a detailed insight into the geochemistry of the pristine volcanic deposits, which is needed to define the starting point of the alteration process. LIBS also indicated the existence of chemical elements for which no corresponding mineral could be identified in the VIS-NIR data, presumably since their spectral signature is masked by strongly absorbing species. These minerals, however, could be confirmed in the Raman spectra—nicely completing the achieved results and highlighting the high potential of the sensor suite for our study.</p>","PeriodicalId":54286,"journal":{"name":"Earth and Space Science","volume":"12 5","pages":""},"PeriodicalIF":2.9,"publicationDate":"2025-05-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1029/2024EA004036","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"144140378","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}