
Geomagnetic fluctuations during a polarity transition
Author(s) -
Audunsson Haraldur,
Levi Shaul
Publication year - 1997
Publication title -
journal of geophysical research: solid earth
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/96jb02534
Subject(s) - earth's magnetic field , declination , paleomagnetism , geology , secular variation , geomagnetic secular variation , polarity (international relations) , magnetic dip , geodesy , outcrop , magnetostratigraphy , geomagnetic pole , amplitude , geophysics , magnetic declination , geomagnetic reversal , physics , paleontology , magnetic field , astrophysics , geomagnetic storm , optics , chemistry , quantum mechanics , cell , biochemistry
The extensive Roza Member of the Columbia River Basalt Group (Washington State) has intermediate paleomagnetic directions, bracketed by underlying normal and overlying reverse polarity flows. A consistent paleomagnetic direction was measured at 11 widely distributed outcrops; the average direction has a declination of 189° and an inclination of −5°, with greater variation in the inclination [ Rietman , 1966]. In this study the Roza Member was sampled in two Pasco Basin drillcores, where it is a single cooling unit and its thickness exceeds 50 m. Excellent core recovery allowed uniform and dense sampling of the drillcores. During its protracted cooling, the Roza flow in the drillcores recorded part of a 15.5 Ma geomagnetic polarity transition. The inclination has symmetric, quasicyclic intraflow variation, while the declination is nearly constant, consistent with the results from the outcrops. Thermal models of the cooling flow provide the timing for remanence acquisition. The inclination is inferred to have progressed from 0° to −15° and back to −3°over a period of 15 to 60 years, at rates of 1.6° to 0.5°/yr. Because the geomagnetic intensity was probably weak during the transition, these apparently high rates of change are not significantly different from present‐day secular variation. These results agree with the hypothesis that normal secular variation persists through geomagnetic transitions. The Iow‐amplitude quasicyclical fluctuations of the field over tens of years, recorded by Roza, suggest that the geomagnetic field reverses in discrete steps, and that more than 15–60 years were required to complete this reversal.