2016
DOI: 10.1002/2016jb013194
|View full text |Cite
|
Sign up to set email alerts
|

Crustal structure of the Kermadec arc from MANGO seismic refraction profiles

Abstract: Three active‐source seismic refraction profiles are integrated with morphological and potential field data to place the first regional constraints on the structure of the Kermadec subduction zone. These observations are used to test contrasting tectonic models for an along‐strike transition in margin structure previously known as the 32°S boundary. We use residual bathymetry to constrain the geometry of this boundary and propose the name Central Kermadec Discontinuity (CKD). North of the CKD, the buried Tonga … Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1
1
1

Citation Types

1
35
0

Year Published

2018
2018
2024
2024

Publication Types

Select...
9
1

Relationship

1
9

Authors

Journals

citations
Cited by 38 publications
(37 citation statements)
references
References 116 publications
(354 reference statements)
1
35
0
Order By: Relevance
“…Strong correlations ( R 2 > 0.85) between the elevation and Moho depth in modern subduction and collision zones confirm the effectiveness of Equations – (Figure 1). The differences in equations for subduction zones and equations for collision zones are interpreted to be caused by the variations in crust and upper mantle density (Figure 1; Bassett et al, 2016; Lee et al, 2015). Previous studies that calculating paleo‐elevation based on Airy isostasy and paleocrustal thickness (e.g., Chapman et al, 2020; Zhu et al, 2017) implicitly assume that the crust and upper mantle density have not changed, which may not be valid for ancient orogens.…”
Section: Resultsmentioning
confidence: 99%
“…Strong correlations ( R 2 > 0.85) between the elevation and Moho depth in modern subduction and collision zones confirm the effectiveness of Equations – (Figure 1). The differences in equations for subduction zones and equations for collision zones are interpreted to be caused by the variations in crust and upper mantle density (Figure 1; Bassett et al, 2016; Lee et al, 2015). Previous studies that calculating paleo‐elevation based on Airy isostasy and paleocrustal thickness (e.g., Chapman et al, 2020; Zhu et al, 2017) implicitly assume that the crust and upper mantle density have not changed, which may not be valid for ancient orogens.…”
Section: Resultsmentioning
confidence: 99%
“…The tsunami waveforms can be well reproduced with a RMSE of 0.0612 ( Figure S8c) by a CLVD source model at depth of 1.5 km with a total length of 7 km, thickness of 1 km, and a nonuniform distribution of vertical expansion and horizontal compression amounts ( Figure S8a). If we assume a rigidity at this depth of 10 GPa ( Figure S9), based on the velocity model of Bassett et al (2016), then the total seismic moment of the shallow CLVD source model from the tsunami waveform analysis is 1.5 times that of GCMT solution. Kanamori et al (1993) suspected that this kind of tsunami earthquake was a result of hydrofracturing by heated water in a sediment layer above a shallow magma chamber.…”
Section: The Dual-depth Source Model 521 Deep Clvd and Shallow CLVmentioning
confidence: 99%
“…Alternatively, magmatism may play a considerable role in the thickening of the Jurassic oceanic arc within the BNO. Studies on modern oceanic arcs, such as the Izu-Bonin-Marina [70][71][72][73], the Lesser Antilles [74][75][76], the Tonga-Kermadec [77][78][79], and the Aleutian [80][81][82] arcs show a variation of crustal thickness (9-35 km) within a single arc or between different arcs. In addition, an important finding of these studies is that the thick part of an arc is always related to high magmatic flux.…”
Section: Mechanism For the Crustal Thickening Of The Jurassic Oceanicmentioning
confidence: 99%