4.3 Article

Ocean wave sources of seismic noise

期刊

出版社

AMER GEOPHYSICAL UNION
DOI: 10.1029/2011JC006952

关键词

-

资金

  1. ERC [240009 IOWAGA]
  2. U.S. National Ocean Partnership [N00014-10-1-0383]
  3. Consolider-Ingeno 2010 [CSD2006-00041]

向作者/读者索取更多资源

Noise with periods 3 to 10 s, ubiquitous in seismic records, is expected to be mostly generated by pairs of ocean wave trains of opposing propagation directions with half the seismic frequency. Here we present the first comprehensive numerical model of microseismic generation by random ocean waves, including ocean wave reflections. Synthetic and observed seismic spectra are well correlated (r > 0.85). On the basis of the model results, noise generation events can be clustered in three broad classes: wind waves with a broad directional spectrum (class I), sea states with a significant contribution of coastal reflections (class II), and the interaction of two independent wave systems (class III). At seismic stations close to western coasts, noise generated by class II sources generally dominates, but it is intermittently outshined by the intense class III sources, limiting the reliability of seismic data as a proxy for storm climates. The modeled seismic noise critically depends on the damping of seismic waves. At some mid-ocean island stations, low seismic damping is necessary to reproduce the observed high level and smoothness of noise time series that result from a spatial integration of sources over thousands of kilometers. In contrast, some coastal stations are only sensitive to noise within a few hundreds of kilometers. This revelation of noise source patterns worldwide provides a wealth of information for seismic studies, wave climate applications, and new constraints on the possible directional distribution of wave energy.

作者

我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。

评论

主要评分

4.3
评分不足

次要评分

新颖性
-
重要性
-
科学严谨性
-
评价这篇论文

推荐

Article Geochemistry & Geophysics

Empirical H/V spectral ratios at the InSight landing site and implications for the martian subsurface structure

Sebastian Carrasco, Brigitte Knapmeyer-Endrun, Ludovic Margerin, Cedric Schmelzbach, Keisuke Onodera, Lu Pan, Philippe Lognonne, Sabrina Menina, Domenico Giardini, Eleonore Stutzmann, John Clinton, Simon Stahler, Martin Schimmel, Matthew Golombek, Manuel Hobiger, Miroslav Hallo, Sharon Kedar, William Bruce Banerdt

Summary: The study investigates the local subsurface structure at the InSight landing site on Mars using the horizontal-to-vertical (H/V) spectral ratio inversion technique. Different H/V curves were obtained from ambient vibrations and seismic events. The recordings during high-wind periods were less favorable for traditional analysis, while the S-wave coda of marsquakes provided better results. The derived H/V curve showed a trough at 2.4 Hz and a peak at 8 Hz.

GEOPHYSICAL JOURNAL INTERNATIONAL (2023)

Article Fisheries

Developing an Observing Air-Sea Interactions Strategy (OASIS) for the global ocean

M. F. Cronin, S. Swart, C. A. Marandino, C. Anderson, P. Browne, S. Chen, W. R. Joubert, U. Schuster, R. Venkatesan, C. Addey, O. Alves, F. Ardhuin, S. Battle, M. A. Bourassa, Z. Chen, M. Chory, C. Clayson, R. B. de Souza, M. du Plessis, M. Edmondson, J. B. Edson, S. T. Gille, J. Hermes, V Hormann, S. A. Josey, M. Kurz, T. Lee, F. Maicu, E. H. Moustahfid, S-A Nicholson, E. S. Nyadjro, J. Palter, R. G. Patterson, S. G. Penny, L. P. Pezzi, N. Pinardi, J. E. J. Reeves Eyre, N. Rome, A. C. Subramanian, C. Stienbarger, T. Steinhoff, A. J. Sutton, H. Tomita, S. M. Wills, C. Wilson, L. Yu

Summary: The Observing Air-Sea Interactions Strategy (OASIS) is a program that aims to improve Earth system forecasts, CO2 uptake assessments, and provide ocean information for decision makers. It focuses on creating a global network of mobile air-sea observing platforms, a satellite network optimized for measuring air-sea fluxes, and improving the representation of air-sea coupling in Earth system models. The program consists of various activities such as network design, model improvement, partnership building, and best practices experiments.

ICES JOURNAL OF MARINE SCIENCE (2023)

Article Astronomy & Astrophysics

Crustal Structure Constraints From the Detection of the SsPp Phase on Mars

Jiaqi Li, Caroline Beghein, Paul Davis, Mark. A. Wieczorek, Scott M. M. McLennan, Doyeon Kim, Ved Lekic, Matthew Golombek, Martin Schimmel, Eleonore Stutzmann, Philippe Lognonne, William Bruce Banerdt

Summary: The shallowest layer beneath the Mars InSight Lander site has low seismic wave velocity due to high porosity and other lithological factors. The SsPp phase was detected on Mars for the first time, confirming the existence of an 8 km interface and a large wave speed contrast across it. The average P-wave speed in the top crustal layer was found to be between 2.5 and 3.2 km/s, providing a more precise estimate than previous studies.

EARTH AND SPACE SCIENCE (2023)

Article Geosciences, Multidisciplinary

Time of Emergence for Altimetry-Based Significant Wave Height Changes in the North Atlantic

Antoine Hochet, Guillaume Dodet, Florian Sevellec, Marie-Noelle Bouin, Anindita Patra, Fabrice Ardhuin

Summary: Satellite observations over the past 30 years indicate that changes in wave height are primarily driven by internal variability and not yet significantly affected by anthropogenic climate change. The dominant influence of climate change on wave height trends is expected to emerge after 2050.

GEOPHYSICAL RESEARCH LETTERS (2023)

Article Geosciences, Multidisciplinary

Investigation of Martian Regional Crustal Structure Near the Dichotomy Using S1222a Surface-Wave Group Velocities

Zongbo Xu, Adrien Broquet, Nobuaki Fuji, Taichi Kawamura, Philippe Lognonne, Jean-Paul Montagner, Lu Pan, Martin Schimmel, Eleonore Stutzmann, William Bruce Banerdt

Summary: Understanding the Martian crust and uppermost mantle is crucial for studying the planet's evolution, and NASA's InSight mission has provided seismic data to reveal the interior structure. While most studies have focused on the crustal structure beneath the InSight lander, the seismic structure of other regions remains poorly known. This study investigates the crustal structure along the Medusa Fossae Formation and the dichotomy using surface-wave data, and the findings suggest the presence of a high-velocity layer and a common intra-crustal structure in this region.

GEOPHYSICAL RESEARCH LETTERS (2023)

Article Geosciences, Multidisciplinary

Detection of Mars Normal Modes From S1222a Event and Seismic Hum

P. Lognonne, M. Schimmel, E. Stutzmann, P. Davis, M. Drilleau, G. Sainton, T. Kawamura, M. P. Panning, W. B. Banerdt

Summary: We have detected normal modes on Mars for the first time using vertical records from InSight's broad-band seismometer after a marsquake occurred on sol 1222. Our catalog includes 60 potential eigenfrequencies between 3 and 12 mHz, detected using the phasor walkout approach due to their low signal-to-noise ratio. The amplitudes of the normal modes are consistent with the upper limit of the S1222a magnitude and show high quality factors. Additionally, we have observed the first Martian hum before the quake at several frequencies. These proposed frequencies are within 1-sigma of those predicted by published models based on body wave travel time inversions. This detection of normal modes is significant as it is the first on a terrestrial planet other than Earth and can contribute to future interior models incorporating normal modes frequencies, surface waves velocities, and body wave travel times.

GEOPHYSICAL RESEARCH LETTERS (2023)

Article Oceanography

On Consistent Parameterizations for Both Dominant Wind-Waves and Spectral Tail Directionality

Matias Alday, Fabrice Ardhuin

Summary: Numerical wave models can reproduce wave evolution in all directions and wavelengths, though the understanding and representation of physical processes affecting wave energy distribution is limited. Models are typically adjusted to reproduce dominant wave characteristics, such as significant wave height, mean direction, and dominant wavelengths. Recent updates in wave dissipation parameterizations have shown realistic energy levels and directional distribution for shorter waves. This new formulation of wave energy sink can reproduce the variability of measured infrasound power and is sensitive to factors such as non-linear energy transfer and the influence of dominant and relatively long waves on the dissipation of shorter waves in other directions.

JOURNAL OF GEOPHYSICAL RESEARCH-OCEANS (2023)

Article Geosciences, Multidisciplinary

Constraints on the Cryohydrological Warming of Firn and Ice in Greenland From Rayleigh Wave Ellipticity Data

G. A. Jones, A. M. G. Ferreira, B. Kulessa, M. Schimmel, A. Berbellini, A. Morelli

Summary: Rayleigh wave ellipticity measurements from seismic ambient noise recorded on the Greenland Ice Sheet (GrIS) show complex and anomalous behavior at wave periods sensitive to ice (T < 3-4 s). To understand these complex observations, we compare them with synthetic ellipticity measurements obtained from synthetic ambient noise computed for various seismic velocity and attenuation models, including surface wave overtone effects. We find that in dry snow conditions within the interior of the GrIS, to first order the anomalous ellipticity observations can be explained by ice models associated with the accumulation and densification of snow into firn. We also show that the distribution of ellipticity measurements is strongly sensitive to seismic attenuation and the thermal structure of the ice. Our results suggest that Rayleigh wave ellipticity is well suited for monitoring changes in firn properties and thermal composition of the Greenland and Antarctic ice sheets in a changing climate.

GEOPHYSICAL RESEARCH LETTERS (2023)

Article Geosciences, Multidisciplinary

Constraints for the Martian Crustal Structure From Rayleigh Waves Ellipticity of Large Seismic Events

Sebastian Carrasco, Brigitte Knapmeyer-Endrun, Ludovic Margerin, Zongbo Xu, Rakshit Joshi, Martin Schimmel, Eleonore Stutzmann, Constantinos Charalambous, Philippe Lognonne, W. Bruce Banerdt

Summary: We measured the ellipticity of direct Rayleigh waves at intermediate periods (15-35 s) on Mars using recordings of three large seismic Martian events, including the largest event recorded by the InSight mission. These measurements, along with other seismic data, were used to determine the local crustal structure at the InSight landing site. The results suggest the presence of crustal discontinuities at depths around 10 km, 20 km, and a strong discontinuity at approximately 37 km, interpreted as the crust-mantle interface, as well as a shallow low-velocity layer of 2-3 km thickness.

GEOPHYSICAL RESEARCH LETTERS (2023)

Article Oceanography

Wave Groups and Small Scale Variability of Wave Heights Observed by Altimeters

Marine De Carlo, Fabrice Ardhuin, Annabelle Ollivier, Adrien Nigou

Summary: Recent satellite altimeter retracking and filtering methods have reduced noise in estimates of wave height, allowing for the study of processes with smaller scales. The contribution of wave groups to the uncertainty in wave height measurements is quantified using directional wave spectra measured by the China-France Ocean Satellite (CFOSAT). This study demonstrates that wave group effects account for a significant portion of the variance in wave height measurements, with the largest impact observed during storms and in the presence of long swells.

JOURNAL OF GEOPHYSICAL RESEARCH-OCEANS (2023)

Article Geochemistry & Geophysics

Broadband Empirical Green's Function Extraction With Data Adaptive Phase Correlations

Sergi Ventosa, Martin Schimmel

Summary: Seismic ambient noise has nonstationary time-frequency statistics, requiring better interstation correlation methods. The wavelet phase cross-correlation (WPCC) functions, incorporating ideas from the phase cross-correlation (PCC) method and wavelet cross-correlation, are introduced to analyze seismic ambient noise and extract clean broadband signals. WPCC has shown benefits in improving baseline corrections, signal extraction, and measurement accuracy compared to PCC. The use of GPU offsets the increase in computational cost, making WPCC an efficient approach for processing large data volumes in seismic interferometry studies.

IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING (2023)

Article Geochemistry & Geophysics

Mapping the basement of the Cerdanya Basin (eastern Pyrenees) using seismicambient noise

Jordi Diaz, Sergi Ventosa, Martin Schimmel, Mario Ruiz, Albert Macau, Anna Gabas, David Marti, Ozgenc Akin, Jaume Verges

Summary: In this study, ambient seismic noise acquired in the Cerdanya Basin was used to evaluate the capability of different methodologies to map the geometry of a small-scale sedimentary basin. The results from various techniques, including autocorrelations, ambient noise Rayleigh wave tomography, HVSR, and band-pass-filtered ambient noise amplitude mapping, consistently showed that the deeper part of the basin is located in its central part, reaching depths of 600-700 m close to the Tet fault trace. The overall consistency between the results provides solid constraints to the basement depth estimation and helps improve the geological characterization of the Cerdanya Basin.

SOLID EARTH (2023)

Article Geosciences, Multidisciplinary

Constraints for the Martian Crustal Structure From Rayleigh Waves Ellipticity of Large Seismic Events

Sebastian Carrasco, Brigitte Knapmeyer-Endrun, Ludovic Margerin, Zongbo Xu, Rakshit Joshi, Martin Schimmel, Eleonore Stutzmann, Constantinos Charalambous, Philippe Lognonne, W. Bruce Banerdt

Summary: In this study, we measured the ellipticity of direct Rayleigh waves at intermediate periods on Mars for the first time. These measurements, along with other seismic data, were used to infer the local crustal structure at the InSight landing site. Our results suggest the presence of intra-crustal discontinuities and a strong crust-mantle interface at around 37 km depth. We also found a shallow low-velocity layer of 2-3 km thickness. The lower seismic wave velocities in the crust compared to nearby regions indicate a higher porosity or alteration of the local crust.

GEOPHYSICAL RESEARCH LETTERS (2023)

暂无数据