TY - JOUR
T1 - An Automatic Model Selection-Based Machine Learning Framework to Estimate FORC Distributions
AU - Heslop, D.
AU - Roberts, A. P.
AU - Oda, H.
AU - Zhao, X.
AU - Harrison, R. J.
AU - Muxworthy, A. R.
AU - Hu, P. X.
AU - Sato, T.
N1 - Funding Information:
We are grateful to the associate editor, Ramon Egli, and an anonymous reviewer for their constructive comments that have improved the paper. We acknowledge the insight by Ramon Egli in his review that third‐order polynomial surfaces are incompatible with Stoner‐Wohlfarth particles. We thank Ayako Katayama for her invaluable assistance in this work. This work was supported financially by the National Institute of Advanced Industrial Science and Technology, Ministry of Economy, Trade and Industry, Japan (A. P. R., H. O., D. H., X. Z., R. J. H., A. R. M., P. X. H., and T. S.), the Australian Research Council through grants DP160100805 and DP200100765 (A. P. R., D. H., R. J. H., A. R. M., X. Z., and P. X. H.), and the European Research Council under the European Union's Seventh Framework Programme (FP/2007–2013)/ERC grant agreement number 320750 (R. J. H.).
Publisher Copyright:
©2020. American Geophysical Union. All Rights Reserved.
PY - 2020/10/1
Y1 - 2020/10/1
N2 - First-order reversal curve (FORC) distributions are a powerful diagnostic tool for characterizing and quantifying magnetization processes in fine magnetic particle systems. Estimation of FORC distributions requires the computation of the second-order mixed derivative of noisy magnetic hysteresis data. This operation amplifies measurement noise, and for weakly magnetic systems, it can compromise estimation of a FORC distribution. Previous processing schemes, which are based typically on local polynomial regression, have been developed to smooth FORC data to suppress detrimental noise. Importantly, the smoothed FORC distribution needs to be consistent with the measurement data from which it was estimated. This can be a challenging task even for expert users, who must adjust subjectively parameters that define the form and extent of smoothing until a “satisfactory” FORC distribution is obtained. For nonexpert users, estimation of FORC distributions using inappropriate smoothing parameters can produce distorted results corrupted by processing artifacts, which can lead to spurious inferences concerning the magnetic system under investigation. We have developed a statistical machine learning framework based on a probabilistic model comparison to guide the estimation of FORC distributions. An intuitive approach is presented that reveals regions of a FORC distribution that may have been smoothed inappropriately. An associated metric can also be used to compare data preparation and local regression schemes to assess their suitability for processing a given FORC data set. Ultimately, our approach selects FORC smoothing parameters in a probabilistic fashion, which automates the derivative estimation process regardless of user expertise.
AB - First-order reversal curve (FORC) distributions are a powerful diagnostic tool for characterizing and quantifying magnetization processes in fine magnetic particle systems. Estimation of FORC distributions requires the computation of the second-order mixed derivative of noisy magnetic hysteresis data. This operation amplifies measurement noise, and for weakly magnetic systems, it can compromise estimation of a FORC distribution. Previous processing schemes, which are based typically on local polynomial regression, have been developed to smooth FORC data to suppress detrimental noise. Importantly, the smoothed FORC distribution needs to be consistent with the measurement data from which it was estimated. This can be a challenging task even for expert users, who must adjust subjectively parameters that define the form and extent of smoothing until a “satisfactory” FORC distribution is obtained. For nonexpert users, estimation of FORC distributions using inappropriate smoothing parameters can produce distorted results corrupted by processing artifacts, which can lead to spurious inferences concerning the magnetic system under investigation. We have developed a statistical machine learning framework based on a probabilistic model comparison to guide the estimation of FORC distributions. An intuitive approach is presented that reveals regions of a FORC distribution that may have been smoothed inappropriately. An associated metric can also be used to compare data preparation and local regression schemes to assess their suitability for processing a given FORC data set. Ultimately, our approach selects FORC smoothing parameters in a probabilistic fashion, which automates the derivative estimation process regardless of user expertise.
KW - First-order reversal curves
KW - Machine learning
KW - Rock magnetism
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U2 - 10.1029/2020JB020418
DO - 10.1029/2020JB020418
M3 - Article
AN - SCOPUS:85094157789
SN - 2169-9313
VL - 125
JO - Journal of Geophysical Research: Space Physics
JF - Journal of Geophysical Research: Space Physics
IS - 10
M1 - e2020JB020418
ER -