Paleomagnetism applied to tectonics;
Block rotation;
Rock magnetism;
Main Ethiopia rift;
Oblique rifting;
CONTINENTAL BREAK-UP;
EXTENSION DIRECTION;
REMAGNETIZATION CIRCLES;
EVOLUTION;
CONSTRAINTS;
SEGMENTATION;
INSIGHTS;
GENESIS;
INTRUSION;
LINEAMENT;
D O I:
10.1016/j.jafrearsci.2024.105326
中图分类号:
P [天文学、地球科学];
学科分类号:
07 ;
摘要:
A total of 208 paleomagnetic core samples were collected from twenty-seven sites within the Butajira volcano chains of the central Main Ethiopian rift (MER), providing insights into tectonic rotation. Core samples were taken from ignimbrite (similar to 1.7-2.54Ma), basalt, and trachyte rock units (<1.6Ma) along the western margin of the central MER. Each core sample underwent analysis using twin specimens subjected to stepwise alternate field (AF) and thermal (Th) demagnetization techniques. Furthermore, a single specimen from every site was employed for rock-magnetic experiments. Detailed rock magnetic experiments identified titano-magnetite, magnetite, and hematite as the remanence carrier magnetic minerals. The natural remanent magnetization (NRM) directional analysis revealed two components:1) a low-stability (LS) component removed by low-temperature (<300 degrees C) and low-field (<20 mT) and 2) a high-stability (HS) with heating >300 degrees C or 20 mT increments showed vectors pointing to the plot's origin, indicative of the characteristic remanent magnetization (ChRM). All sites, except one, displayed reverse polarity NRM. The tilt-corrected mean direction calculated from 19 sites, yielded D-o = 355.7 degrees, I-o = 9.9 degrees (N = 19, K = 22.9, alpha(95) = 7.3 degrees), indicates a 6.2 degrees +/- 6.2 degrees counterclockwise (CCW) tectonic rotation relative to the reference dipole geomagnetic field direction of 2Ma D-x = 1.9 degrees, I-x = 15.5 degrees (N = 32, K = 105.6, alpha(95) = 2.5 degrees) for stable Africa (Besse and Courtillot, 2003). The oblique rifting and pure-dip slip kinematics that characterize the border faults in the study area could have caused this minor counterclockwise rotation and agrees with analogue model prediction of Corti et al.,2013.
机构:
Univ Warsaw, IGMiP Fac Geol, PL-02089 Warsaw, PolandUniv Warsaw, IGMiP Fac Geol, PL-02089 Warsaw, Poland
Macdonald, Ray
Baginski, Boguslaw
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Univ Warsaw, IGMiP Fac Geol, PL-02089 Warsaw, PolandUniv Warsaw, IGMiP Fac Geol, PL-02089 Warsaw, Poland
Baginski, Boguslaw
Ronga, Fiorenzo
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机构:
Univ Naples Federico II, Dipartimento Sci Terra, I-80134 Naples, ItalyUniv Warsaw, IGMiP Fac Geol, PL-02089 Warsaw, Poland
Ronga, Fiorenzo
Dzierzanowski, Piotr
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Univ Warsaw, IGMiP Fac Geol, PL-02089 Warsaw, PolandUniv Warsaw, IGMiP Fac Geol, PL-02089 Warsaw, Poland
Dzierzanowski, Piotr
Lustrino, Michele
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Univ Roma La Sapienza, Dipartimento Sci Terra, CNR Ist Geol Ambientale Geoingn IGAG, I-00185 Rome, ItalyUniv Warsaw, IGMiP Fac Geol, PL-02089 Warsaw, Poland
Lustrino, Michele
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机构:
Marzoli, Andrea
Melluso, Leone
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Univ Naples Federico II, Dipartimento Sci Terra, I-80134 Naples, ItalyUniv Warsaw, IGMiP Fac Geol, PL-02089 Warsaw, Poland