Incompatible Ediacaran paleomagnetic directions suggest an equatorial geomagnetic dipole hypothesis

被引:95
作者
Abrajevitch, Alexandra [1 ]
Van der Voo, Rob [2 ]
机构
[1] Kochi Univ, Ctr Adv Marine Core Res, Kochi 7838502, Japan
[2] Univ Michigan, Ann Arbor, MI 48109 USA
关键词
paleomagnetism; Ediacaran; Laurentia; Baltica; paleogeography; equatorial dipole; TRUE POLAR WANDER; LAYERED MAFIC INTRUSION; INERTIAL INTERCHANGE; SEPT-ILES; FIELD; REVERSALS; PALEOGEOGRAPHY; LAURENTIA; AGE; MA;
D O I
10.1016/j.epsl.2010.02.038
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
Paleomagnetic results obtained from rocks of Ediacaran age in several localities in Laurentia and Baltica persistently display co-existence of two magnetization components, one shallowly and the other steeply inclined. Both components pass criteria for a primary magnetization while geological considerations and radiometric age dating indicate that these magnetizations are surprisingly close in age. The conventional interpretation of these results, translating the inclination into paleolatitudes using the geocentric axial dipole hypothesis, would imply that rocks acquired magnetizations in positions switching back and forth between equatorial and near-polar latitudes. In a geographic reference frame, such large-scale and fast (>45 cm/yr) migrations of a continent have been rejected as dynamically implausible: neither plate tectonics nor True Polar Wander are thought to be able to attain the required velocities. A highly irregular behavior of the geomagnetic field during the Ediacaran, possibly an alternation of the geomagnetic dipole axis between a coaxial and an equatorial alignment, remains the only viable explanation for the paleomagnetic data. Such a behavior entails specific outer core conditions, which in turn impose strong constraints on the possible models for the thermal evolution of the Earth's interior. (C) 2010 Elsevier B.V. All rights reserved.
引用
收藏
页码:164 / 170
页数:7
相关论文
共 61 条
[1]   HOTSPOTS, POLAR WANDER, MESOZOIC CONVECTION AND THE GEOID [J].
ANDERSON, DL .
NATURE, 1982, 297 (5865) :391-393
[2]  
[Anonymous], EARTH PLANET SCI LET
[3]   Axial vs. equatorial dipolar dynamo models with implications for planetary magnetic fields [J].
Aubert, J ;
Wicht, J .
EARTH AND PLANETARY SCIENCE LETTERS, 2004, 221 (1-4) :409-419
[4]   BREAKUP OF A SUPERCONTINENT BETWEEN 625 MA AND 555 MA - NEW EVIDENCE AND IMPLICATIONS FOR CONTINENTAL HISTORIES [J].
BOND, GC ;
NICKESON, PA ;
KOMINZ, MA .
EARTH AND PLANETARY SCIENCE LETTERS, 1984, 70 (02) :325-345
[5]   MORPHOLOGICAL DISPARITY IN THE CAMBRIAN [J].
BRIGGS, DEG ;
FORTEY, RA ;
WILLS, MA .
SCIENCE, 1992, 256 (5064) :1670-1673
[6]   Exploring the influence of the non-dipole field on magnetic records for field reversals and excursions [J].
Brown, Maxwell C. ;
Holme, Richard ;
Bargery, Alistair .
GEOPHYSICAL JOURNAL INTERNATIONAL, 2007, 168 (02) :541-550
[7]   The thermal state of Earth's core [J].
Buffett, BA .
SCIENCE, 2003, 299 (5613) :1675-1677
[8]   Dependence of the duration of geomagnetic polarity reversals on site latitude [J].
Clement, BM .
NATURE, 2004, 428 (6983) :637-640
[9]   GEOGRAPHICAL-DISTRIBUTION OF TRANSITIONAL VGPS - EVIDENCE FOR NON-ZONAL EQUATORIAL SYMMETRY DURING THE MATUYAMA-BRUNHES GEOMAGNETIC REVERSAL [J].
CLEMENT, BM .
EARTH AND PLANETARY SCIENCE LETTERS, 1991, 104 (01) :48-58
[10]   An examination of simulated geomagnetic reversals from a palaeomagnetic perspective [J].
Coe, RS ;
Hongre, L ;
Glatzmaier, GA .
PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES, 2000, 358 (1768) :1141-1170