English
 
Privacy Policy Disclaimer
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT

Released

Journal Article

Near-source magnitude scaling of spectral accelerations: analysis and update of Kotha et al.(2020) model

Authors

Kotha,  Sreeram Reddy
External Organizations;

/persons/resource/gweather

Weatherill,  Graeme
2.6 Seismic Hazard and Risk Dynamics, 2.0 Geophysics, Departments, GFZ Publication Database, Deutsches GeoForschungsZentrum;

/persons/resource/bindi

Bindi,  Dino
2.6 Seismic Hazard and Risk Dynamics, 2.0 Geophysics, Departments, GFZ Publication Database, Deutsches GeoForschungsZentrum;

/persons/resource/fcotton

Cotton,  Fabrice
2.6 Seismic Hazard and Risk Dynamics, 2.0 Geophysics, Departments, GFZ Publication Database, Deutsches GeoForschungsZentrum;

External Ressource
No external resources are shared
Fulltext (public)
There are no public fulltexts stored in GFZpublic
Supplementary Material (public)
There is no public supplementary material available
Citation

Kotha, S. R., Weatherill, G., Bindi, D., Cotton, F. (2022): Near-source magnitude scaling of spectral accelerations: analysis and update of Kotha et al.(2020) model. - Bulletin of Earthquake Engineering, 20, 1343-1370.
https://doi.org/10.1007/s10518-021-01308-5


Cite as: https://gfzpublic.gfz-potsdam.de/pubman/item/item_5011360
Abstract
Ground-motion models (GMMs) are often used to predict the random distribution of Spectral accelerations ( SAs ) at a site due to a nearby earthquake. In probabilistic seismic hazard and risk assessment, large earthquakes occurring close to a site are considered as critical scenarios. GMMs are expected to predict realistic SAs with low within-model uncertainty ( σμ ) for such rare scenarios. However, the datasets used to regress GMMs are usually deficient of data from critical scenarios. The (Kotha et al., A Regionally Adaptable Ground- Motion Model for Shallow Crustal Earthquakes in Europe Bulletin of Earthquake Engineering 18:4091–4125, 2020) GMM developed from the Engineering strong motion (ESM) dataset was found to predict decreasing short-period SAs with increasing M W ≥ Mh = 6.2 , and with large σμ at near-source distances ≤ 30km . In this study, we updated the parametrisation of the GMM based on analyses of ESM and the Near source strong motion (NESS) datasets. With Mh = 5.7 , we could rectify the M W scaling issue, while also reducing σμ at M W ≥ Mh . We then evaluated the GMM against NESS data, and found that the SAs from a few large, thrust-faulting events in California, New Zealand, Japan, and Mexico are significantly higher than GMM median predictions. However, recordings from these events were mostly made on soft-soil geology, and contain anisotropic pulse-like effects. A more thorough non-ergodic treatment of NESS was not possible because most sites sampled unique events in very diverse tectonic environments. We provide an updated set of GMM coefficients, σμ , and heteroscedastic variance models; while also cautioning against its application for M W ≤ 4 in low-moderate seismicity regions without evaluating the homogeneity of M W estimates between pan-European ESM and regional datasets.