Crustal structures of Southmost Mariana Trench revealed by wide-angle seismic profile TS01

被引:0
|
作者
Li ZiZheng [1 ,2 ,3 ,4 ,5 ]
Qiu XueLin [1 ,2 ,3 ,4 ]
He EnYuan [1 ,2 ,3 ]
Zhang HaoYu [1 ,4 ,5 ]
Wang Qiang [6 ,7 ]
机构
[1] Chinese Acad Sci, South China Sea Inst Oceanol, Key Lab Ocean & Marginal Sea Geol, Guangzhou 510301, Peoples R China
[2] Southern Marine Sci & Engn Guangdong Lab Guangzho, Guangzhou 511458, Peoples R China
[3] Chinese Acad Sci, Innovat Acad South China Sea Ecol & Environm Engn, Guangzhou 510301, Peoples R China
[4] Univ Chinese Acad Sci, Beijing 100049, Peoples R China
[5] SINOPEC Geophys Res Inst Co Ltd, Nanjing 211103, Peoples R China
[6] Fujian Xiamen Inst Geol Engn, Inst Marine Geol Survey, Xiamen 361008, Fujian, Peoples R China
[7] Fujian Geol Engn Survey Inst, Key Lab Geohazard Prevent Hilly Mt, Minist Nat Resources China, Fuzhou 350002, Peoples R China
来源
关键词
South Mariana Trench; Ocean Bottom Seismometer (OBS); Wide-angle seismic survey; Crustal structure; Gravity modeling; SUBDUCTION ZONE; OCEANIC PLATEAU; CAROLINE RIDGE; YAP SUBDUCTION; UPPER-MANTLE; FORE-ARC; CHINA; INVERSION; GRAVITY; MODEL;
D O I
10.6038/cjg2022P0923
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Mariana Trench of Western Pacific Subduction System possesses complicated tectonic settings and vigorous subduction dynamics. Wide-angle seismic profile TS01 traverses the Caroline Plateau, Southmost Mariana Trench and Forearc. We obtained a velocity structure of TS01 via forward modeling based on reflection and refraction phases recorded by 9 OBSs. Furthermore, Bouguer gravity anomaly was calculated based on satellite gravity and multi-beam bathymetric data, and is used to analyze the variations of crustal thickness. Gravity modeling was further conducted to constrain the crustal and uppermost mantle structure. Our velocity model shows a wedge-shaped forearc crust, and relatively low velocities at inner trench slope, which may have arisen from subduction erosion. The velocities of subducting crust range from 4. 0 to 7. 2 km . s(-1). The crustal thickness of the subducting plate is approximately 12 similar to 13 km, thicker than typical oceanic crust but thinner than many oceanic plateaus. Three interfaces (interfaces between upper and lower plates, mid-crustal interface and Moho of subducting slab) are constrained by reflection phases of OBSs. Gravity modeling shows a low-density area beneath the trench, indicating serpentinization in the uppermost mantle of the downgoing plate. Our results lay a solid foundation for revealing the subduction dynamics near an oceanic plateau.
引用
收藏
页码:4691 / 4704
页数:14
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