scholarly journals High‐Velocity Friction Experiments Indicate Magnetic Enhancement and Softening of Fault Gouges During Seismic Slip

2019 ◽  
Vol 124 (1) ◽  
pp. 26-43 ◽  
Author(s):  
Tao Yang ◽  
Jianye Chen ◽  
Huiru Xu ◽  
Mark J. Dekkers
Keyword(s):  
High Velocity ◽  
Seismic Slip ◽  
Magnetic Enhancement ◽  
Fault Gouges

scholarly journals Grain Size Sensitive Creep During Simulated Seismic Slip in Nanogranular Fault Gouges: Constraints From Transmission Kikuchi Diffraction (TKD)

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):  
Grain Size ◽  
Seismic Slip ◽  
Fault Gouges

Seismic slip record in carbonate-bearing fault zones: An insight from high-velocity friction experiments on siderite gouge

Geology ◽  
2007 ◽  
Vol 35 (12) ◽  
pp. 1131 ◽  
Author(s):  
Raehee Han ◽  
Toshihiko Shimamoto ◽  
Jun-ichi Ando ◽  
Jin-Han Ree
Keyword(s):  
High Velocity ◽  
Fault Zones ◽  
Bearing Fault ◽  
Seismic Slip

scholarly journals A rotary-shear low to high-velocity friction apparatus in Beijing to study rock friction at plate to seismic slip rates

2014 ◽  
Vol 27 (5) ◽  
pp. 469-497 ◽  
Author(s):  
Shengli Ma ◽  
Toshihiko Shimamoto ◽  
Lu Yao ◽  
Tetsuhiro Togo ◽  
Hiroko Kitajima
Keyword(s):  
High Velocity ◽  
Slip Rates ◽  
Rock Friction ◽  
Seismic Slip ◽  
Rotary Shear

Galactic orbits of stars

1966 ◽  
Vol 25 ◽  
pp. 93-97
Author(s):  
Richard Woolley
Keyword(s):  
Globular Cluster ◽  
Potential Field ◽  
High Velocity ◽  
Velocity Vector ◽  
Variable Stars ◽  
The Sun ◽  
Proper Motions ◽  
Rr Lyrae ◽  
The Galaxy

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.

Supernovae and interstellar gas dynamics

1967 ◽  
Vol 31 ◽  
pp. 117-119
Author(s):  
F. D. Kahn ◽  
L. Woltjer
Keyword(s):  
Lower Limit ◽  
High Velocity ◽  
Gas Dynamics ◽  
Interstellar Cloud ◽  
Interstellar Gas ◽  
Random Motions ◽  
Relativistic Particles

The efficiency of the transfer of energy from supernovae into interstellar cloud motions is investigated. A lower limit of about 0·002 is obtained, but values near 0·01 are more likely. Taking all uncertainties in the theory and observations into account, the energy per supernova, in the form of relativistic particles or high-velocity matter, needed to maintain the random motions in the interstellar gas is estimated as 1051·4±1ergs.

Super-high Velocity Cartridges and Three-barrel Guns

1914 ◽  
Vol 111 (5) ◽  
pp. 82-82
Author(s):  
Frank C. Perkins
Keyword(s):  
High Velocity

ATOMIZATION CHARACTERISTICS OF LIQUID JETS INJECTED INTO A HIGH-VELOCITY FLOW FIELD

1994 ◽  
Vol 4 (4) ◽  
pp. 451-471 ◽  
Author(s):  
Nobuyuki Yatsuyanagi ◽  
Hiroshi Sakamoto ◽  
Kazuo Sato
Keyword(s):  
Flow Field ◽  
High Velocity ◽  
Liquid Jets ◽  
High Velocity Flow ◽  
Velocity Flow ◽  
Atomization Characteristics
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