World Library  
Flag as Inappropriate
Email this Article

Supershear earthquake

Article Id: WHEBN0017909377
Reproduction Date:

Title: Supershear earthquake  
Author: World Heritage Encyclopedia
Language: English
Subject: Ares J. Rosakis, Coordinating Committee for Earthquake Prediction, Body wave magnitude, Earthquake duration magnitude, Earthquake engineering
Collection:
Publisher: World Heritage Encyclopedia
Publication
Date:
 

Supershear earthquake

A supershear earthquake is an earthquake in which the propagation of the rupture along the fault surface occurs at speeds in excess of the seismic shear wave (S-wave) velocity. This causes an effect analogous to a sonic boom.[1]

Rupture propagation velocity

During seismic events along a fault surface the displacement initiates at the focus and then propagates outwards. Typically the focus lies towards one end of the slip surface and much of the propagation is unidirectional (e.g. the 2008 Sichuan and 2004 Indian Ocean earthquakes). Theoretical studies have in the past suggested that the upper bound for propagation velocity is that of Rayleigh waves, approximately 0.92 of the shear wave velocity.[2] However, evidence of propagation at velocities between S-wave and compressional wave (P-wave) values have been reported for several earthquakes[3][4] in agreement with theoretical and laboratory studies that support the possibility of rupture propagation in this velocity range.[5][6]

Occurrence

Mode-I, Mode-II, and Mode-III cracks.

Evidence of rupture propagation at velocities greater than S-wave velocities expected for the surrounding crust have been observed for several large earthquakes associated with strike-slip faults. During strike-slip, the main component of rupture propagation will be horizontal, in the direction of displacement, as a Mode II (in-plane) shear crack. This contrasts with a dip-slip rupture where the main direction of rupture propagation will be perpendicular to the displacement, like a Mode III (anti-plane) shear crack. Theoretical studies have shown that Mode III cracks are limited to the shear wave velocity but that Mode II cracks can propagate between the S and P-wave velocities [7] and this may explain why supershear earthquakes have not been observed on dip-slip faults.

Examples

Directly observed

Inferred

See also

References

  1. ^ A century after the 1906 earthquake, geophysicists revisit 'The Big One' and come up with a new model, Press release, Stanford University
  2. ^ Broberg,K.B. 1996. How fast can a crack go?. Materials Science, 32, 80-86
  3. ^ a b Archuleta,R.J. 1984. A faulting model for the 1979 Imperial Valley earthquake, J. Geophys. Res., 89, 4559–4585.
  4. ^ Ellsworth,W.L. & Celebi,M. 1999. Near Field Displacement Time Histories of the M 7.4 Kocaeli (Izimit), Turkey, Earthquake of August 17, 1999, Am. Geophys. Union, Fall Meeting Suppl. 80, F648.
  5. ^ Okubo, P. G. (1989). Dynamic rupture modeling with laboratory-derived constitutive relations, J. Geophys. Res. 94, 12321-12335
  6. ^ Rosakis,A.J., Samudrala,O. & Coker,D. 1999. Cracks Faster than the Shear Wave Speed. Science, 284. no. 5418, pp. 1337 - 1340
  7. ^
  8. ^ a b [1] Bouchon, M., M.-P. Bouin, H. Karabulut, M. N. Toksöz, M. Dietrich, and A. J. Rosakis (2001), How Fast is Rupture During an Earthquake ? New Insights from the 1999 Turkey Earthquakes, Geophys. Res. Lett., 28(14), 2723–2726.]
  9. ^ Bouchon,M. & Vallee,M. 2003.Observation of Long Supershear Rupture During the Magnitude 8.1 Kunlunshan Earthquake, Science, 301, 824-826.
  10. ^ a b
  11. ^ Dunham,E.M. & Archuleta,R.J. 2004.Evidence for a Supershear Transient during the 2002 Denali Fault Earthquake, Bulletin of the Seismological Society of America, 92, S256-S268
  12. ^
  13. ^
  14. ^
  15. ^ Song,S. Beroza,G.C. & Segall,P. 2005. Evidence for supershear rupture during the 1906 San Francisco earthquake. Eos.Trans.AGU, 86(52), Fall Meet.Suppl., Abstract S12A-05
  16. ^

External links

  • Eric Dunham's webpage on Supershear Dynamics
  • New Scientist article on Supershear earthquakes
This article was sourced from Creative Commons Attribution-ShareAlike License; additional terms may apply. World Heritage Encyclopedia content is assembled from numerous content providers, Open Access Publishing, and in compliance with The Fair Access to Science and Technology Research Act (FASTR), Wikimedia Foundation, Inc., Public Library of Science, The Encyclopedia of Life, Open Book Publishers (OBP), PubMed, U.S. National Library of Medicine, National Center for Biotechnology Information, U.S. National Library of Medicine, National Institutes of Health (NIH), U.S. Department of Health & Human Services, and USA.gov, which sources content from all federal, state, local, tribal, and territorial government publication portals (.gov, .mil, .edu). Funding for USA.gov and content contributors is made possible from the U.S. Congress, E-Government Act of 2002.
 
Crowd sourced content that is contributed to World Heritage Encyclopedia is peer reviewed and edited by our editorial staff to ensure quality scholarly research articles.
 
By using this site, you agree to the Terms of Use and Privacy Policy. World Heritage Encyclopedia™ is a registered trademark of the World Public Library Association, a non-profit organization.
 


Copyright © World Library Foundation. All rights reserved. eBooks from Project Gutenberg are sponsored by the World Library Foundation,
a 501c(4) Member's Support Non-Profit Organization, and is NOT affiliated with any governmental agency or department.