Joint inversion of local, regional and teleseismic data for crustal thickness in the Eurasia-Africa plate boundary region

被引:67
作者
Marone, F [1 ]
van der Meijde, M [1 ]
van der Lee, S [1 ]
Giardini, D [1 ]
机构
[1] ETH Honggerberg, HPP, Inst Geophys, CH-8093 Zurich, Switzerland
关键词
broad-band; isostasy; Mediterranean; Moho discontinuity; Rayleigh waves; waveform analysis;
D O I
10.1046/j.1365-246X.2003.01973.x
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
A new map for the Moho discontinuity (EAM02) in the Eurasia-Africa plate boundary region is presented. Reliable results have also been obtained for the southern and eastern Mediterranean Basin, the northern African coasts and the eastern Atlantic Ocean, regions only occasionally considered in studies on the Mediterranean region. The Moho topography model is derived from two independent sets of constraints. Information contained in the fundamental and higher-mode Rayleigh waves obtained from waveform modelling is used to constrain the Moho depth between estimates of crustal thickness taken from published reflection and refraction surveys, gravity studies and receiver function analysis. Strong lateral variations in the Moho topography have been observed in the Mediterranean Sea, confirming the complex evolution of this plate boundary region. In the west, the Moho discontinuity has been found at 15-20 km depth, suggesting extended and, at least in some locations, oceanic crust, while in the east the crust is on average 25-30 km thick. There it is interpreted either as Mesozoic oceanic or thinned Precambrian continental crust covered by thick sedimentary deposits. Standard continental crust (30-35 km) is observed along the eastern part of the northern African coast, while to the west a rapid change from a relatively deep Moho (down to 42 km) below the Atlas Mountain Range to the thin crust of the southwestern Mediterranean Sea has been found. The crust beneath the eastern North Atlantic Ocean can be up to 5 km thicker compared with standard oceanic crust (6 km). The crust has been interpreted to be heterogeneous as a consequence of irregular magma supply at the Mid-Atlantic ridge. In addition, serpentinization of the sub-Moho mantle could contribute to the imaging of apparently anomalous thick oceanic crust. In Europe, the presence of crustal roots (>45 km) beneath the major mountain belts has been confirmed, while thin crust (<25 km) has been found beneath extensional basins. Comparing the obtained Moho topography and Moho depth computed assuming isostatic compensation at 60 km depth shows that most of the Mediterranean and eastern Atlantic region appears to be in isostatic equilibrium. The large positive residuals observed for the eastern Mediterranean are likely to be due to overestimating crustal thickness, owing to the thick sediment deposits present.
引用
收藏
页码:499 / 514
页数:16
相关论文
共 113 条
[1]  
AHUSER F, 2001, STARKBEBEN GEOWISSEN, P1
[2]  
[Anonymous], 1989, ALPINE TECTONICS
[3]   DEEP-STRUCTURE OF THE LITHOSPHERE BENEATH THE TERRITORY OF BULGARIA [J].
BABUSKA, V ;
PLOMEROVA, J ;
SPASOV, E .
STUDIA GEOPHYSICA ET GEODAETICA, 1987, 31 (03) :266-283
[4]   FEATURES OF CRUSTAL STRUCTURE UNDER THE CANARY ISLANDS [J].
BANDA, E ;
DANOBEITIA, JJ ;
SURINACH, E ;
ANSORGE, J .
EARTH AND PLANETARY SCIENCE LETTERS, 1981, 55 (01) :11-24
[5]   CRUST AND UPPER MANTLE STRUCTURE OF THE CENTRAL IBERIAN MESETA (SPAIN) [J].
BANDA, E ;
SURINACH, E ;
APARICIO, A ;
SIERRA, J ;
DELAPARTE, ER .
GEOPHYSICAL JOURNAL OF THE ROYAL ASTRONOMICAL SOCIETY, 1981, 67 (03) :779-789
[6]  
Bassin C, 2000, EOS T AGU, V81, pF897, DOI DOI 10.1002/EOST.V81.10
[7]   Crustal structure of the Levant Basin, eastern Mediterranean [J].
Ben-Avraham, Z ;
Ginzburg, A ;
Makris, J ;
Eppelbaum, L .
TECTONOPHYSICS, 2002, 346 (1-2) :23-43
[8]   Lithospheric structure of the southern French Alps inferred from broadband analysis [J].
Bertrand, E ;
Deschamps, A .
PHYSICS OF THE EARTH AND PLANETARY INTERIORS, 2000, 122 (1-2) :79-102
[9]  
BEST JA, 1990, GEOLOGY, V18, P1235, DOI 10.1130/0091-7613(1990)018<1235:BGTACS>2.3.CO
[10]  
2