Abstract
Summary. Rotational remanent magnetization, RRM, is the magnetization acquired when a sample is rotated during alternating field demagnetization. Although the existence of RRM has been well documented in different laboratories, until now no physical mechanism explaining its origin has been given. We propose that the RRM originates from thermal fluctuations biased by a precessional torque associated with the alternating field. Our theory is consistent with the observation that no directional preference exists in the experimental situation until the sample is rotated relative to the alternating field. Moreover, our theory predicts that the combined sample rotation and precession will produce a RRM that switches direction when the frequency of sample rotation increases from any value below the frequency of the alternating field to any value above that frequency as observed in experiments. Although no precise theory is given for the intensity of RRM, the model presented here can qualitatively explain previous intensity observations. Copyright © 1980, Wiley Blackwell. All rights reserved
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CITATION STYLE
Smith, G., & Merrill, R. T. (1980). The origin of rotational remanent magnetization. Geophysical Journal of the Royal Astronomical Society, 61(2), 329–336. https://doi.org/10.1111/j.1365-246X.1980.tb04320.x
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