2017
DOI: 10.1002/2016jb013848
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Seismic crustal structure of the North China Craton and surrounding area: Synthesis and analysis

Abstract: We present a new digital model (NCcrust) of the seismic crustal structure of the Neoarchean North China Craton (NCC) and its surrounding Paleozoic‐Mesozoic orogenic belts (30°–45°N, 100°–130°E). All available seismic profiles, complemented by receiver function interpretations of crustal thickness, are used to constrain a new comprehensive crustal model NCcrust. The model, presented on a 0.25° × 0.25°grid, includes the Moho depth and the internal structure (thickness and velocity) of the crust specified for fou… Show more

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Cited by 38 publications
(38 citation statements)
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References 81 publications
(142 reference statements)
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“…Calculation of RMGA requires knowledge on the gravitational effect of the crust, which can be calculated from the crustal density model NCcrust (Xia et al, 2017). However, the next step, calculation of mantle density anomalies, requires additional information on the thickness of the layer to which the density anomalies are confined.…”
Section: Lm Thicknessmentioning
confidence: 99%
See 1 more Smart Citation
“…Calculation of RMGA requires knowledge on the gravitational effect of the crust, which can be calculated from the crustal density model NCcrust (Xia et al, 2017). However, the next step, calculation of mantle density anomalies, requires additional information on the thickness of the layer to which the density anomalies are confined.…”
Section: Lm Thicknessmentioning
confidence: 99%
“…Journal of Geophysical Research: Solid Earth nearly uniform average crustal velocity and density (Xia et al, 2017), so that the difference between the Bouguer plate approximation and the full 3-D solution is also small (Shulgin & Artemieva, 2019). Due to the small density contrast across the LAB and its large depth, the 3-D gravitational effects from the LAB are insignificant.…”
Section: 1029/2020jb020296mentioning
confidence: 99%
“…Kaban et al, 2003Kaban et al, , 2016Mooney & Kaban, 2010;Yegorova & Starostenko, 2002), and the other includes mantle density calculation from lithosphere buoyancy in regions that are close to isostatic equilibrium (Artemieva, 2003;Artemieva & Vinnik, 2016;Cherepanova & Artemieva, 2015;Mooney & Vidale, 2003). In both cases the results are critically dependent on the quality and resolution of the crustal model (Herceg et al, 2016;Kaban & Schwintzer, 2001), which necessitates the development of highquality regional seismic models for the crust Cherepanova et al, 2013;Grad et al, 2009;Kennett et al, 2011;Tesauro et al, 2014;Xia et al, 2017). For example, a global gravity modeling demonstrated the presence of strong low-density anomalies (−0.10-0.05 g/cm 3 ) in the subcontinental lithospheric mantle (SCLM) of the cratons (Kaban et al, 2003), but the resolution is insufficient to resolve reliably intracratonic density variations due to limitations of a global model of the crustal structure used in calculations.…”
Section: Introductionmentioning
confidence: 99%
“…Instead, a highvelocity anomaly appears (Figures 9e and 9f). Previous studies such as the thermal structure of the lithosphere across the YSFZ (Lai et al, 2007;Zu et al, 1996), the Moho discontinuities topography using receiver function methods (Chen et al, 2006), and wide-angle seismic profiles (Jia et al, 2014;Li et al, 2011;Xia et al, 2017) indicate that the YSFZ has the features of mantle uplift and crustal thinning. One is that the HVZ corresponds to juvenile lower crust resulting from the basalt underplating at the bottom of the Moho.…”
Section: Geochemistry Geophysics Geosystemsmentioning
confidence: 96%