scholarly journals Thickness of the oceanic crust, the lithosphere, and the mantle transition zone in the vicinity of the Tristan da Cunha hot spot estimated from ocean-bottom and ocean-island seismometer receiver functions

2017 ◽  
Vol 716 ◽  
pp. 33-51 ◽  
Author(s):  
Wolfram H. Geissler ◽  
Wilfried Jokat ◽  
Marion Jegen ◽  
Kiyoshi Baba
2018 ◽  
Vol 230 ◽  
pp. 155-189 ◽  
Author(s):  
Jakub Ciazela ◽  
Juergen Koepke ◽  
Henry J.B. Dick ◽  
Roman Botcharnikov ◽  
Andrzej Muszynski ◽  
...  

2016 ◽  
Vol 675 ◽  
pp. 159-167 ◽  
Author(s):  
Ruiqing Zhang ◽  
Zhanyong Gao ◽  
Qingju Wu ◽  
Zhenxing Xie ◽  
Guangcheng Zhang

2017 ◽  
Vol 474 ◽  
pp. 226-236 ◽  
Author(s):  
Matthew R. Agius ◽  
Catherine A. Rychert ◽  
Nicholas Harmon ◽  
Gabi Laske

2009 ◽  
Vol 278 (3-4) ◽  
pp. 163-174 ◽  
Author(s):  
Denis Lombardi ◽  
Jochen Braunmiller ◽  
Edi Kissling ◽  
Domenico Giardini

2017 ◽  
Vol 702 ◽  
pp. 61-69 ◽  
Author(s):  
Yaohui Duan ◽  
Xiaobo Tian ◽  
Xiaofeng Liang ◽  
Wei Li ◽  
Chenglong Wu ◽  
...  

Solid Earth ◽  
2014 ◽  
Vol 5 (1) ◽  
pp. 327-337 ◽  
Author(s):  
C. Haldar ◽  
P. Kumar ◽  
M. Ravi Kumar

Abstract. Deciphering the seismic character of the young lithosphere near mid-oceanic ridges (MORs) is a challenging endeavor. In this study, we determine the seismic structure of the oceanic plate near the MORs using the P-to-S conversions isolated from quality data recorded at five broadband seismological stations situated on ocean islands in their vicinity. Estimates of the crustal and lithospheric thickness values from waveform inversion of the P-receiver function stacks at individual stations reveal that the Moho depth varies between ~ 10 ± 1 km and ~ 20 ± 1 km with the depths of the lithosphere–asthenosphere boundary (LAB) varying between ~ 40 ± 4 and ~ 65 ± 7 km. We found evidence for an additional low-velocity layer below the expected LAB depths at stations on Ascension, São Jorge and Easter islands. The layer probably relates to the presence of a hot spot corresponding to a magma chamber. Further, thinning of the upper mantle transition zone suggests a hotter mantle transition zone due to the possible presence of plumes in the mantle beneath the stations.


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