scholarly journals Earthquake slip vectors in the Himalayan thrust Zone and their tectonic implications

MAUSAM ◽  
2021 ◽  
Vol 44 (1) ◽  
pp. 61-68
Author(s):  
R.S. DATTATRAYAM ◽  
TETSOZO SENO

Slip vectors of thirty-nine thrust events occurring along the Himalayan collision zone have been compared with the velocity vectors between the Indian-Eurasian plates derived from the RM 2 and NUVEL 1 models, The observed deviations of the slip vector from the velocity vector have been interpreted in terms of a simple kinematic model according to which the eastern and western blocks of south Tibet are separating from each other, From the model it is estimated that the western and eastern blocks of Tibet are moving at the rate of 3.6 cm/year westwards at 76°Eand 2.6 cm/year eastwards at 94°E with respect to Eurasia respectively, resulting in an east-west extension, projected to the trend at 85°E, at the rate of 5, 5 cm/year. This would correspond to a strain rate of about 6.9 x 10-8year in central Tibetan region.

Author(s):  
S. M. L. Sastry

Ti3Al is an ordered intermetallic compound having the DO19-type superlattice structure. The compound exhibits very limited ductility in tension below 700°C because of a pronounced planarity of slip and the absence of a sufficient number of independent slip systems. Significant differences in slip behavior in the compound as a result of differences in strain rate and mode of deformation are reported here.Figure 1 is a comparison of dislocation substructures in polycrystalline Ti3Al specimens deformed in tension, creep, and fatigue. Slip activity on both the basal and prism planes is observed for each mode of deformation. The dominant slip vector in unidirectional deformation is the a-type (b) = <1120>) (Fig. la). The dislocations are straight, occur for the most part in a screw orientation, and are arranged in planar bands. In contrast, the dislocation distribution in specimens crept at 700°C (Fig. lb) is characterized by a much reduced planarity of slip, a tangled dislocation arrangement instead of planar bands, and an increased incidence of nonbasal slip vectors.


2011 ◽  
Vol 44 (5) ◽  
pp. 979-983 ◽  
Author(s):  
Stéphane Avril ◽  
Fabien Schneider ◽  
Christian Boissier ◽  
Zhi-Yong Li

2017 ◽  
Vol 602 ◽  
pp. L11 ◽  
Author(s):  
◽  
P.-O. Petrucci ◽  
I. Waisberg ◽  
J.-B. Le Bouquin ◽  
J. Dexter ◽  
...  

We present the first optical observation of the microquasar SS 433 at sub-milliarcsecond (mas) scale obtained with the GRAVITY instrument on the Very Large Telescope interferometer (VLTI). The 3.5-h exposure reveals a rich K-band spectrum dominated by hydrogen Brγand He i lines, as well as (red-shifted)emission lines coming from the jets. The K-band-continuum-emitting region is dominated by a marginally resolved point source (<1 mas) embedded inside a diffuse background accounting for 10% of the total flux. The jet line positions agree well with the ones expected from the jet kinematic model, an interpretation also supported by the consistent sign (i.e., negative/positive for the receding/approaching jet component) of the phase shifts observed in the lines. The significant visibility drop across the jet lines, together with the small and nearly identical phases for all baselines, point toward a jet that is offset by less than 0.5 mas from the continuum source and resolved in the direction of propagation, with a typical size of 2 mas. The jet position angle of ~80° is consistent with the expected one at the observation date. Jet emission so close to the central binary system would suggest that line locking, if relevant to explain the amplitude and stability of the 0.26c jet velocity, operates on elements heavier than hydrogen. The Brγprofile is broad and double peaked. It is better resolved than the continuum and the change of the phase signal sign across the line on all baselines suggests an East-West-oriented geometry similar to the jet direction and supporting a (polar) disk wind origin.


Lithos ◽  
2017 ◽  
Vol 268-271 ◽  
pp. 260-273 ◽  
Author(s):  
Chao Wang ◽  
Lin Ding ◽  
Zhi-Chao Liu ◽  
Li-Yun Zhang ◽  
Ya-Hui Yue

2011 ◽  
Vol 52 (5) ◽  
pp. 389-405 ◽  
Author(s):  
Xin Dong ◽  
Zeming Zhang ◽  
M. Santosh ◽  
Wei Wang ◽  
Fei Yu ◽  
...  

2006 ◽  
Vol 49 (2) ◽  
pp. 432-440 ◽  
Author(s):  
Jian-Zhong LI ◽  
Cheng-Shan WANG ◽  
Zhong-Xi PAN ◽  
Xin-Tao FENG ◽  
Zhong-Hai ZHUANG ◽  
...  

Sign in / Sign up

Export Citation Format

Share Document