Paleomagnetic data from the Trans-Mexican Volcanic Belt:: implications for tectonics and volcanic stratigraphy

被引:20
作者
Alva-Valdivìa, LM
Goguitchaichvili, A
Ferrari, L
Rosas-Elguera, J
Urrutia-Fucugauchi, J
Zamorano-Orozco, JJ
机构
[1] Univ Nacl Autonoma Mexico, Inst Geofis, Lab Paleomagnetismo & Geofis Nucl, Mexico City 04510, DF, Mexico
[2] Univ Nacl Autonoma Mexico, Inst Geol, Mexico City 04510, DF, Mexico
[3] Univ Guadalajara, Ctr Ciencias Tierra, Guadalajara 44840, Jalisco, Mexico
[4] Univ Nacl Autonoma Mexico, Inst Geog, Mexico City 04510, DF, Mexico
来源
EARTH PLANETS AND SPACE | 2000年 / 52卷 / 07期
关键词
D O I
10.1186/BF03351651
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
We report a paleomagnetic and rock-magnetic study of Miocene volcanic rocks from the Trans-Mexican Volcanic Belt, A total of 32 sites (238 oriented samples) were collected from three localities: Queretaro, Guadalajara and Los Altos dr Jalisco basaltic plateaux, which span from Il to 7.5 Ma. Several rock-magnetic experiments were carried out in order to identify the magnetic carriers and to obtain information about their paleomagnetic stability. Microscopic observation of polished sections shows that the main magnetic mineral is Ti-poor titanomagnetite associated with exsolved ilmenite. Continuous susceptibility measurements with temperature yield in most cases reasonably reversible curves with Curie points close to that of magnetite. Judging from the ratios of hysteresis parameters, it seems that all samples fall in the pseudo-single domain (PSD) grain size region, probably indicating a mixture of multidomain (MD) and a significant amount of single domain (SD) grains. Based on our paleomagnetic and available radiometric data, it seems that the volcanic units have been emplaced during a relatively short time span of 1 to 2 My at each locality. The mean paleomagnetic directions obtained from each locality differ significantly from that expected for the Middle Miocene. The mean paleomagnetic direction calculated from 28 sites discarding those of intermediate polarity is I = 32.46 degrees, D = 341.2 degrees, k = 7.2 and alpha(95) = 11.6 degrees. Comparison with the expected direction indicates some 20 degrees anticlockwise tectonic rotations for the studied area, in accordance with the proposed left-lateral transtensional tectonic regime already proposed for this period.
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页码:467 / 478
页数:12
相关论文
共 49 条
[1]  
[Anonymous], 1985, GEOFISC INT
[2]  
[Anonymous], ESTUDIO PETROGENETIC
[3]   REVISED AND SYNTHETIC APPARENT POLAR WANDER PATHS OF THE AFRICAN, EURASIAN, NORTH-AMERICAN AND INDIAN PLATES, AND TRUE POLAR WANDER SINCE 200 MA [J].
BESSE, J ;
COURTILLOT, V .
JOURNAL OF GEOPHYSICAL RESEARCH-SOLID EARTH AND PLANETS, 1991, 96 (B3) :4029-4050
[4]   A statistical model of the fluctuations in the geomagnetic field from paleosecular variation to reversal [J].
Camps, P ;
Prevot, M .
SCIENCE, 1996, 273 (5276) :776-779
[5]   REVISED CALIBRATION OF THE GEOMAGNETIC POLARITY TIMESCALE FOR THE LATE CRETACEOUS AND CENOZOIC [J].
CANDE, SC ;
KENT, DV .
JOURNAL OF GEOPHYSICAL RESEARCH-SOLID EARTH, 1995, 100 (B4) :6093-6095
[6]  
CASTILLOHERNAND.D, 1991, 0291 COM FED EL GER
[7]  
CERCAMARTINEZ LM, 1998, THESIS BAJA CALIFORN
[8]  
Damon P.E., 1979, ASOCIACION INGENIERO, V13, P156
[9]  
Dunlop J., 1997, ROCK MAGNETISM FUNDA, V1st, DOI DOI 10.1017/CBO9780511612794
[10]   Late Miocene volcanism and intra-arc tectonics during the early development of the Trans-Mexican Volcanic Belt [J].
Ferrari, L ;
Conticelli, S ;
Vaggelli, G ;
Petrone, CM ;
Manetti, P .
TECTONOPHYSICS, 2000, 318 (1-4) :161-185