2020
DOI: 10.1007/s00531-020-01880-2
|View full text |Cite
|
Sign up to set email alerts
|

Cenozoic tectonic rotations in different parts of the NE Pamir: implications for the evolution of the arcuate orogen

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1
1
1

Citation Types

0
3
0

Year Published

2021
2021
2024
2024

Publication Types

Select...
7
2

Relationship

0
9

Authors

Journals

citations
Cited by 11 publications
(7 citation statements)
references
References 105 publications
0
3
0
Order By: Relevance
“…The Western arcuate Variscan belt has been compared to the Pamir West Himalayan syntax (Matte, 1986, 1991). Since oroclinal bending appears to occur in a very different way as the Indian Craton indenter have no equivalent in the weak late‐Variscan domain squeezed between the Laurussia and Gondwana cratonic land‐masses (Figure 13), these two belts are indeed characterized by (i) development of crustal‐scale strike‐slip shear zones on the two branches of a nascent syntax (e.g., Martínez Catalán, 2011; Zhang & Sun, 2020), (ii) strain partitioning processes leading to the exhumation of the deep crustal rock within extensional gneiss domes and syn‐convergence lateral and transverse escape of the weak mid‐lower crust (Gapais et al., 1992, 2015; Martínez Catalán et al., 2014; Rutte et al., 2017; Stephenson et al., 2001), and (iii) accommodation of deformation over large distances (i.e., more than 600‐km wide orogenic belts) in a hot and weak orogenic lithosphere bounded by strong and colder cratonic lithospheres (Figure 13).…”
Section: Discussionmentioning
confidence: 99%
“…The Western arcuate Variscan belt has been compared to the Pamir West Himalayan syntax (Matte, 1986, 1991). Since oroclinal bending appears to occur in a very different way as the Indian Craton indenter have no equivalent in the weak late‐Variscan domain squeezed between the Laurussia and Gondwana cratonic land‐masses (Figure 13), these two belts are indeed characterized by (i) development of crustal‐scale strike‐slip shear zones on the two branches of a nascent syntax (e.g., Martínez Catalán, 2011; Zhang & Sun, 2020), (ii) strain partitioning processes leading to the exhumation of the deep crustal rock within extensional gneiss domes and syn‐convergence lateral and transverse escape of the weak mid‐lower crust (Gapais et al., 1992, 2015; Martínez Catalán et al., 2014; Rutte et al., 2017; Stephenson et al., 2001), and (iii) accommodation of deformation over large distances (i.e., more than 600‐km wide orogenic belts) in a hot and weak orogenic lithosphere bounded by strong and colder cratonic lithospheres (Figure 13).…”
Section: Discussionmentioning
confidence: 99%
“…KYTS: Kashgar-Yecheng transfer system, MPT: Main Pamir Thrust, QFTS: Qimugen fold-thrust system, TKT: Tam Karaul fault, WKFT: West Kunlun frontal thrust, and WKFR: West Kunlun frontal blind ramp. Tectonics 10.1029/2023TC008233 rotations, such as limited rotations during the Cenozoic (Chen et al, 1992;Gilder et al, 1996;Li et al, 2013;Rumelhart et al, 1999) or systematic regional clockwise rotations (∼15-20°) during the Oligocene (Bosboom et al, 2014;Zhang & Sun, 2020) or after ∼15 Ma (Blayney et al, 2019) (Figure 1a). These inconsistent rotations were mostly related to the northward indentation of the Pamir salient during the Cenozoic.…”
Section: 1029/2023tc008233mentioning
confidence: 99%
“…Paleomagnetism is also essential for providing independent constraints and can be used to quantify and date the VARs of the upper crust along the FTBs (Figure 1a) (Bazhenov et al., 1994; Bosboom et al., 2014; Chen et al., 1991; Li et al., 2018; Rumelhart et al., 1999; Tong et al., 2020; Xu et al., 2024; Zhang et al., 2019). Many paleomagnetic studies have been conducted along the West Kunlun Mountains, most of them were distributed in the northwestern or eastern part of the Pamir salient, with large discrepancies in both the pattern and magnitude of rotations, such as limited rotations during the Cenozoic (Chen et al., 1992; Gilder et al., 1996; Li et al., 2013; Rumelhart et al., 1999) or systematic regional clockwise rotations (∼15–20°) during the Oligocene (Bosboom et al., 2014; Zhang & Sun, 2020) or after ∼15 Ma (Blayney et al., 2019) (Figure 1a). These inconsistent rotations were mostly related to the northward indentation of the Pamir salient during the Cenozoic.…”
Section: Introductionmentioning
confidence: 99%
“…0°) (Bazhenov et al, 1994; Pozzi & Feinberg, 1991; Thomas et al, 1994). The timing of the rotation, however, remains controversial due to poor age constraints in the basin (Bosboom et al, 2014; Thomas et al, 1994; Zhang & Sun, 2020).…”
Section: Geological Backgroundmentioning
confidence: 99%