Early cretaceous absolute geomagnetic paleointensities from Cordoba Province (Argentina)

被引:14
|
作者
Ruiz, Ruben Cejudo
Goguitchaichvili, Avto
Geuna, Silvana E.
Alva-Valdivia, Luis M.
Sole, Jesus
Morales, Juan
机构
[1] Univ Nacl Autonoma Mexico, Inst Geofis, Lab Paleomagnetismo, Mexico City 04510, DF, Mexico
[2] Univ Nacl Autonoma Mexico, Inst Geofis, Lab Interinst Magnetismo Nat, Coeneo, Michoacan, Mexico
[3] Univ Buenos Aires, Fac Ciencias Exactas & Nat, Dept Ciencias Geol, Lab Daniel Valencio, RA-1428 Buenos Aires, DF, Argentina
[4] Univ Nacl Autonoma Mexico, Inst Geol, Mexico City 04510, DF, Mexico
来源
EARTH PLANETS AND SPACE | 2006年 / 58卷 / 10期
关键词
paleointensity; rock-magnetism; Early Cretaceous; South America;
D O I
10.1186/BF03352629
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
We present here new paleointensity and geochronology results from Early Cretaceous volcanic rocks of Sierra Chica de Cordoba (Argentina). The new K-Ar isotopic ages of 5 samples range from 136 to 122 Ma. Twenty five samples from 7 individual flows yielded acceptable paleointensity estimates. The mean paleointensity values per flow are ranging from 53.0 +/- 1.9 to 25.4 +/- 2.6 mu T and the corresponding Virtual Dipole Moments (VDMs) are ranging, from 9.3 +/- 1.3 to 4.6 +/- 0.5 (10(22) Am-2). This corresponds to the mean value of 7.3 +/- 1.7 x 10(22) Am-2, which is compatible to the present geomagnetic axial dipole. Currently available selected paleointensity data from 80 to 130 Ma suggest that geomagnetic field strength frequently fluctuated before and during the Cretaceous Normal Superchron while the magnetic polarity maintained stable. The mean paleointensities derived from Cordoba lavas agree remarkably well with those obtained from the Parana Magmatic Province (133-132 Ma). This reinforces the hypothesis about the unreliability of 'Mesozoic Dipole Low'.
引用
收藏
页码:1333 / 1339
页数:7
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