Seismic Characterization of the Chelyabinsk Meteor's Terminal Explosion
2013; Seismological Society of America; Volume: 84; Issue: 6 Linguagem: Inglês
10.1785/0220130042
ISSN1938-2057
AutoresSebastian Heimann, Álvaro González, R. Wang, Simone Cesca, Torsten Dahm,
Tópico(s)Earthquake Detection and Analysis
ResumoResearch Article| November 01, 2013 Seismic Characterization of the Chelyabinsk Meteor’s Terminal Explosion Sebastian Heimann; Sebastian Heimann aGFZ German Research Centre for Geosciences, Section on Earthquake Risk and Early Warning, Helmholtzstr. 7, 14467 Potsdam, Germanysebastian.heimann@gfz-potsdam.de Search for other works by this author on: GSW Google Scholar Álvaro González; Álvaro González aGFZ German Research Centre for Geosciences, Section on Earthquake Risk and Early Warning, Helmholtzstr. 7, 14467 Potsdam, Germanysebastian.heimann@gfz-potsdam.de Search for other works by this author on: GSW Google Scholar Rongjiang Wang; Rongjiang Wang aGFZ German Research Centre for Geosciences, Section on Earthquake Risk and Early Warning, Helmholtzstr. 7, 14467 Potsdam, Germanysebastian.heimann@gfz-potsdam.de Search for other works by this author on: GSW Google Scholar Simone Cesca; Simone Cesca bUniversity of Potsdam, Institute of Earth and Environmental Science, Karl‐Liebknecht‐Str. 24‐25, 14476 Potsdam, Germany Search for other works by this author on: GSW Google Scholar Torsten Dahm Torsten Dahm aGFZ German Research Centre for Geosciences, Section on Earthquake Risk and Early Warning, Helmholtzstr. 7, 14467 Potsdam, Germanysebastian.heimann@gfz-potsdam.de Search for other works by this author on: GSW Google Scholar Author and Article Information Sebastian Heimann aGFZ German Research Centre for Geosciences, Section on Earthquake Risk and Early Warning, Helmholtzstr. 7, 14467 Potsdam, Germanysebastian.heimann@gfz-potsdam.de Álvaro González aGFZ German Research Centre for Geosciences, Section on Earthquake Risk and Early Warning, Helmholtzstr. 7, 14467 Potsdam, Germanysebastian.heimann@gfz-potsdam.de Rongjiang Wang aGFZ German Research Centre for Geosciences, Section on Earthquake Risk and Early Warning, Helmholtzstr. 7, 14467 Potsdam, Germanysebastian.heimann@gfz-potsdam.de Simone Cesca bUniversity of Potsdam, Institute of Earth and Environmental Science, Karl‐Liebknecht‐Str. 24‐25, 14476 Potsdam, Germany Torsten Dahm aGFZ German Research Centre for Geosciences, Section on Earthquake Risk and Early Warning, Helmholtzstr. 7, 14467 Potsdam, Germanysebastian.heimann@gfz-potsdam.de Publisher: Seismological Society of America First Online: 14 Jul 2017 Online ISSN: 1938-2057 Print ISSN: 0895-0695 © 2013 by the Seismological Society of America Seismological Research Letters (2013) 84 (6): 1021–1025. https://doi.org/10.1785/0220130042 Article history First Online: 14 Jul 2017 Cite View This Citation Add to Citation Manager Share Icon Share Facebook Twitter LinkedIn MailTo Tools Icon Tools Get Permissions Search Site Citation Sebastian Heimann, Álvaro González, Rongjiang Wang, Simone Cesca, Torsten Dahm; Seismic Characterization of the Chelyabinsk Meteor’s Terminal Explosion. Seismological Research Letters 2013;; 84 (6): 1021–1025. doi: https://doi.org/10.1785/0220130042 Download citation file: Ris (Zotero) Refmanager EasyBib Bookends Mendeley Papers EndNote RefWorks BibTex toolbar search Search Dropdown Menu toolbar search search input Search input auto suggest filter your search All ContentBy SocietySeismological Research Letters Search Advanced Search Impacts with our planet cause seismic shaking by a variety of mechanisms. Catastrophic ground motion, even at antipodal distances, can be generated by the extremely infrequent, hypersonic collisions with large asteroids or comets (Meschede et al., 2011). Fortunately, the atmosphere effectively shields the smaller (and far more common) meteoroids, greatly reducing their initial kinetic energy at high altitude, causing them to slow down, break up, and even vaporize, producing a meteor (Ceplecha and Revelle, 2005). In most instances, the ground shaking is triggered by the atmospheric shock wave of a meteor, not by the impact... You do not have access to this content, please speak to your institutional administrator if you feel you should have access.
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