1 / 23

Overview of available data

Overview of available data. Swiss Sites. FLACH. X. FLACH. 4 Hz. WILA. X. WILA. 5 Hz. WILA. Relatively strong attenuation. BALST. X. BALST. 2.5 Hz. AIGLE. X. AIGLE. DAVOX. X. DAVOX. 1.5 Hz. Issues. INTR - N. “polluted” noise.

Télécharger la présentation

Overview of available data

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Overview of available data

  2. Swiss Sites

  3. FLACH X

  4. FLACH 4 Hz

  5. WILA X

  6. WILA 5 Hz

  7. WILA Relatively strong attenuation

  8. BALST X

  9. BALST 2.5 Hz

  10. AIGLE X

  11. AIGLE

  12. DAVOX X

  13. DAVOX 1.5 Hz

  14. Issues INTR - N “polluted” noise

  15. Topographic amplification studies based on earthquake resposne spectra (C. Cauzzi, SED) Combined used of numerical simulations (Sulmona, Irpinia) and recorded data; Relating topographic amplification with the local altitude, slope, and estimated natural frequencies of the relief; Focus on main topographic categories of the Eurocode 8 for station selection (data from CH, IT and JP); Measure kappa from response spectra to understand the role of attenuation on the observed amplification;

  16. Next steps • WCEE abstract submitted (though the deadline for the paper submission is approaching …) • Common processing tools for polarization analysis: • What should we compare? (frequencies, angles + uncertainties) • What should we do with earthquake data? • kappa (Carlo) • polarization – comparison with noise results • ??? • Shallow geophysics - Active Noise correlation with D arrays (Cecile?) • Work on DEM models (comparison with INGV Milan – V. Pessina)

  17. Modelling examples

  18. Modelling of unstable rockslopes (extreme case - Randa) 3Hz (Burjanek et al., GJI, 2010 Moore et al., BSSA, 2011)

  19. Modelling of unstable rockslopes (extreme case - Randa) • FE element modelling of eigen-modes • Effective elastic properties (Vs=900m/s) necessary to fit eigen-frequency of 3Hz (Burjanek et al., ESG, 2011)

  20. Modelling of unstable rockslopes (extreme case) • simulations of model wit cracks perfromed with UDEC (Moore et al., BSSA, 2011)

  21. Modelling of unstable rockslopes (extreme case - Randa) Modelled site-to-reference s. ratio Modelled crack displacement Observed crack displacement Observed site-to-reference s. ratio (Moore et al., BSSA, 2011)

  22. Modelling of unstable rockslopes (extreme case - Rawilhorn) • 1946 M6 Earthquake doublet (separated by 4 months) • Second event triggered the rockfall

  23. Modelling of unstable rockslopes (extreme case - Rawilhorn) After M6.1 earthquake (Moore et al., ISL, 2012)

More Related