Palaeosecular variation in central Mexico over the last 30000 years: The record from lavas

被引:57
作者
Gonzalez, S
Sherwood, G
Bohnel, H
Schnepp, E
机构
[1] Univ Nacl Autonoma Mexico, INST GEOFIS, MEXICO CITY 04510, DF, MEXICO
[2] UNIV MUNSTER, INST GEOPHYS, D-48149 MUNSTER, GERMANY
关键词
magnetic mineralogy; Mexico; palaeointensity; palaeomagnetism; Quaternary; secular variation;
D O I
10.1111/j.1365-246X.1997.tb00999.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
13 lava flows of known age (ages from C-14 dating), which have been erupted in the last 30000 years, have been studied to determine the palaeosecular variation of the geomagnetic field in Central Mexico. Samples were taken from two different monogenetic volcanic fields: the Michoacan-Guanajuato Volcanic field (six sites) and the Chichinautzin Formation (seven sites), both part of the Transmexican Volcanic Belt. The lavas were studied in detail using rock magnetic methods (magnetic susceptibility at room temperature, low-temperature susceptibility behaviour, hysteresis loops, Curie temperatures), combined with reflected light microscopy, in order to deduce their magnetic mineralogy and the domain states of the magnetic minerals. The magnetic carriers are titanomagnetites, which show differing degrees of high-temperature deuteric oxidation, and seem to be predominantly pseudo-single domain (PSD), though in many cases are probably a mixture of domain states. Mean palaeomagnetic directions and palaeointensity values using Shaw and Thellier techniques were obtained using several specimens from each flow. Our data seem to indicate a sharp easterly swing in declination about 5000 years ago, which is also observed in lake sediments from Central Mexico. The calculated values of the virtual dipole moment (VDM) range from 3.1 to 14.9 x 10(22) A m(2). Our data indicate that the virtual dipole moment seems to have increased gradually in magnitude over the last 30 kyr, with a peak at about 9000 years BP. These are features that have been observed in other parts of the globe and are probably caused by variations in the dipole part of the geomagnetic field.
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收藏
页码:201 / 219
页数:19
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