2013
DOI: 10.1016/j.tecto.2013.09.017
|View full text |Cite
|
Sign up to set email alerts
|

Presence of a layered lithosphere beneath the Zagros collision zone

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1

Citation Types

2
17
1

Year Published

2015
2015
2022
2022

Publication Types

Select...
6
1
1

Relationship

0
8

Authors

Journals

citations
Cited by 27 publications
(20 citation statements)
references
References 66 publications
2
17
1
Order By: Relevance
“…Pn velocities(Al--Lazki et al, 2003 Amini et al, 2012) and P-and S-wave tomography(Alinaghi et al, 2007; Kaviani et al, 2007;Paul et al, 2010) -that found low velocities in the uppermost mantle of Central Iran. But, our findings do not support the idea of a breakoff of the oceanic Neo-Tethyan slab beneath Central Iran as suggested byMohammadi et al (2013a) andShomali et al (2011). A sketch representing a new model for the deep structures beneath Iranian Plateau based on our results is presented inFig.…”
contrasting
confidence: 80%
“…Pn velocities(Al--Lazki et al, 2003 Amini et al, 2012) and P-and S-wave tomography(Alinaghi et al, 2007; Kaviani et al, 2007;Paul et al, 2010) -that found low velocities in the uppermost mantle of Central Iran. But, our findings do not support the idea of a breakoff of the oceanic Neo-Tethyan slab beneath Central Iran as suggested byMohammadi et al (2013a) andShomali et al (2011). A sketch representing a new model for the deep structures beneath Iranian Plateau based on our results is presented inFig.…”
contrasting
confidence: 80%
“…Following previous studies (e.g., Kaviani et al, ; Mahmoodabadi et al, ; Motaghi et al, ; Priestley et al, ), we attribute this high‐V anomaly to be the Arabian lithosphere. Previous seismological studies show that there is a thick lithosphere beneath the Zagros with a thickness of ~170–225 km (Mohammadi et al, ; Motaghi et al, ; Priestley et al, ). Our results are generally consistent with the previous results and suggest that the Arabian lithosphere has subducted beneath the Zagros orogen.…”
Section: Discussionmentioning
confidence: 98%
“…The variations of Q 0 and n versus lapse time for two datasets is depicted in Figure 7 and Figure 8. As it can be seen in Figure 7-a, the Q 0 values of Zagros and SSZ become larger than those of WA and NWCI at lapse time about 20 s. The average depth at this lapse time is about 75 km, and it approximately coincides with a low velocity zone beneath WA and NWCI and with a high velocity (Arabian lithosphere) zone beneath Zagros and SSZ [Sodoudi et al, 2009;Mohammadi et al, 2013;Motaghi et al, 2017;Rastgoo et al, 2018].…”
mentioning
confidence: 77%