scholarly journals Late Permian palaeomagnetism of Northern Eurasia: data evaluation and a single-plate test of the geocentric axial dipole model

2010 ◽  
Vol 180 (1) ◽  
pp. 136-146 ◽  
Author(s):  
Mikhail L. Bazhenov ◽  
Andrey V. Shatsillo
1996 ◽  
Vol 144 (3-4) ◽  
pp. 337-346 ◽  
Author(s):  
Gary D. Acton ◽  
Katerina E. Petronotis ◽  
Cheryl D. Cape ◽  
Sue Rotto Ilg ◽  
Richard G. Gordon ◽  
...  

2022 ◽  
Author(s):  
James W. Sears

ABSTRACT A robust, geology-based Proterozoic continental assembly places the northern and eastern margins of the Siberian craton against the southwestern margins of Laurentia in a tight, spoon-in-spoon conjugate fit. The proposed assembly began to break apart in late Neoproterozoic and early Paleozoic time. Siberia then drifted clockwise along the Laurussian margin on coast-parallel transforms until suturing with Europe in late Permian time. The proposed drift path is permitted by a geocentric axial dipole (GAD) magnetic field from Silurian to Permian time. However, the Proterozoic reconstruction itself is not permitted by GAD. Rather, site-mean paleomagnetic data plot ted on the reconstruction suggest a multipolar Proterozoic dynamo dominated by a quadrupole. The field may have resembled that of present-day Neptune, where, in the absence of a large solid inner core, a quadrupolar magnetic field may be generated within a thin spherical shell near the core-mantle boundary. The quadrupole may have dominated Earth’s geomagnetic field until early Paleozoic time, when the field became erratic and transitioned to a dipole, which overwhelmed the weaker quadrupole. The dipole then established a strong magnetosphere, effectively shielding Earth from ultraviolet-B (UV-B) radiation and making the planet habitable for Cambrian fauna.


2015 ◽  
Vol 112 (49) ◽  
pp. 15036-15041 ◽  
Author(s):  
Huapei Wang ◽  
Dennis V. Kent ◽  
Pierre Rochette

The geomagnetic field is predominantly dipolar today, and high-fidelity paleomagnetic mean directions from all over the globe strongly support the geocentric axial dipole (GAD) hypothesis for the past few million years. However, the bulk of paleointensity data fails to coincide with the axial dipole prediction of a factor-of-2 equator-to-pole increase in mean field strength, leaving the core dynamo process an enigma. Here, we obtain a multidomain-corrected Pliocene–Pleistocene average paleointensity of 21.6 ± 11.0 µT recorded by 27 lava flows from the Galapagos Archipelago near the Equator. Our new result in conjunction with a published comprehensive study of single-domain–behaved paleointensities from Antarctica (33.4 ± 13.9 µT) that also correspond to GAD directions suggests that the overall average paleomagnetic field over the past few million years has indeed been dominantly dipolar in intensity yet only ∼60% of the present-day field strength, with a long-term average virtual axial dipole magnetic moment of the Earth of only 4.9 ± 2.4 × 1022 A⋅m2.


2017 ◽  
Vol 265 ◽  
pp. 54-61 ◽  
Author(s):  
Toni Veikkolainen ◽  
Moritz Heimpel ◽  
Michael E. Evans ◽  
Lauri J. Pesonen ◽  
Kimmo Korhonen

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