Directional change during a M iocene R ‐ N geomagnetic polarity reversal recorded by mafic lava flows, S heep C reek R ange, north central N evada, USA
Author:
Affiliation:
1. Department of GeologyOccidental CollegeLos Angeles California USA
2. U.S. Geological Survey, MS 989Menlo Park California USA
3. Scripps Institution of Oceanography, University of California San DiegoLa Jolla California USA
Funder
National Science Foundation
Publisher
American Geophysical Union (AGU)
Subject
Geochemistry and Petrology,Geophysics
Link
https://onlinelibrary.wiley.com/doi/pdf/10.1002/2017GC007049
Reference46 articles.
1. Can downwelling at the top of the Earth’s core be detected in the geomagnetic secular variation?
2. Stationary, oscillating or drifting mantle-driven geomagnetic flux patches?
3. Polarity Reversals from Paleomagnetic Observations and Numerical Dynamo Simulations
4. The time-dependence of intense archeomagnetic flux patches
5. The magnetic structure of convection-driven numerical dynamos
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