Reproduction of thermal pressurization and fluidization of clay-rich fault gouges by high-velocity friction experiments and implications for seismic slip in natural faults

2011 ◽  
Vol 359 (1) ◽  
pp. 267-285 ◽  
Author(s):  
Kohtaro Ujiie ◽  
Akito Tsutsumi ◽  
Jun Kameda
2019 ◽  
Vol 124 (10) ◽  
pp. 10197-10209 ◽  
Author(s):  
Matteo Demurtas ◽  
Steven A. F. Smith ◽  
David J. Prior ◽  
Frank E. Brenker ◽  
Giulio Di Toro
Keyword(s):  

Terra Nova ◽  
2010 ◽  
Vol 22 (5) ◽  
pp. 347-353 ◽  
Author(s):  
Fabio Ferri ◽  
Giulio Di Toro ◽  
Takehiro Hirose ◽  
Toshihiko Shimamoto

Geology ◽  
2007 ◽  
Vol 35 (12) ◽  
pp. 1131 ◽  
Author(s):  
Raehee Han ◽  
Toshihiko Shimamoto ◽  
Jun-ichi Ando ◽  
Jin-Han Ree

2006 ◽  
Vol 424 (1-2) ◽  
pp. 109-118 ◽  
Author(s):  
Kieran O'Hara ◽  
Kazuo Mizoguchi ◽  
Toshihiko Shimamoto ◽  
James C. Hower

2014 ◽  
Vol 27 (5) ◽  
pp. 469-497 ◽  
Author(s):  
Shengli Ma ◽  
Toshihiko Shimamoto ◽  
Lu Yao ◽  
Tetsuhiro Togo ◽  
Hiroko Kitajima

1966 ◽  
Vol 25 ◽  
pp. 93-97
Author(s):  
Richard Woolley

It is now possible to determine proper motions of high-velocity objects in such a way as to obtain with some accuracy the velocity vector relevant to the Sun. If a potential field of the Galaxy is assumed, one can compute an actual orbit. A determination of the velocity of the globular clusterωCentauri has recently been completed at Greenwich, and it is found that the orbit is strongly retrograde in the Galaxy. Similar calculations may be made, though with less certainty, in the case of RR Lyrae variable stars.


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