Please use this identifier to cite or link to this item:
http://hdl.handle.net/2122/15803
Authors: | Morasca, Paola* Bindi, Dino* Mayeda, Kevin* Roman-Nieves, Jorge* Barno, Justin* Walter, William R* Spallarossa, Daniele* |
Title: | Source scaling comparison and validation in Central Italy: data intensive direct S waves versus the sparse data coda envelope methodology | Journal: | Geophysical Journal International | Series/Report no.: | /231 (2022) | Publisher: | Oxford University Press - The Royal Astronomical Society | Issue Date: | 23-Jul-2022 | DOI: | 10.1093/gji/ggac268 | Keywords: | source parameters, coda waves, radiated energy, moment magnitude, corner frequency | Subject Classification: | 04.06. Seismology | Abstract: | Robustness of source parameter estimates is a fundamental issue in understanding the relationships between small and large events; however, it is difficult to assess how much of the variability of the source parameters can be attributed to the physical source characteristics or to the uncertainties of the methods and data used to estimate the values. In this study, we apply the coda method by Mayeda et al. using the coda calibration tool (CCT), a freely available Java-based code (https://github.com/LLNL/coda-calibration-tool) to obtain a regional calibration for Central Italy for estimating stable source parameters. We demonstrate the power of the coda technique in this region and show that it provides the same robustness in source parameter estimation as a data-driven methodology [generalized inversion technique (GIT)], but with much fewer calibration events and stations. The Central Italy region is ideal for both GIT and coda approaches as it is characterized by high-quality data, including recent well-recorded seismic sequences such as L'Aquila (2009) and Amatrice–Norcia–Visso (2016–2017). This allows us to apply data-driven methods such as GIT and coda-based methods that require few, but high-quality data. The data set for GIT analysis includes ∼5000 earthquakes and more than 600 stations, while for coda analysis we used a small subset of 39 events spanning 3.5 < Mw < 6.33 and 14 well-distributed broad-band stations. For the common calibration events, as well as an additional 247 events (∼1.7 < Mw < ∼5.0) not used in either calibration, we find excellent agreement between GIT-derived and CCT-derived source spectra. This confirms the ability of the coda approach to obtain stable source parameters even with few calibration events and stations. Even reducing the coda calibration data set by 75 per cent, we found no appreciable degradation in performance. This validation of the coda calibration approach over a broad range of event size demonstrates that this procedure, once extended to other regions, represents a powerful tool for future routine applications to homogeneously evaluate robust source parameters on a national scale. Furthermore, the coda calibration procedure can homogenize the Mw estimates for small and large events without the necessity of introducing any conversion scale between narrow-band measures such as local magnitude (ML) and Mw, which has been shown to introduce significant bias.</jats:p> | Description: | This article has been accepted for publication in Geophysical Journal International ©:The Author(s) 2022. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.Uploaded in accordance with the publisher's self-archiving policy. |
Appears in Collections: | Article published / in press |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
Morasca_et_al_2022_CCT_Central_Italy.pdf | source parameters in Central Italy: comparison of different techniques (Coda calibration and GIT) | 14.56 MB | Adobe PDF | View/Open |
Page view(s)
68
checked on Apr 27, 2024
Download(s)
26
checked on Apr 27, 2024