Journal
JOURNAL OF GEOPHYSICAL RESEARCH-SOLID EARTH
Volume 128, Issue 8, Pages -Publisher
AMER GEOPHYSICAL UNION
DOI: 10.1029/2023JB026983
Keywords
paleomagnetism; nonparametric bootstrap; directional data
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Paleomagnetic statistical inference is often hindered by distributional assumptions of parametric null hypothesis tests. To address this, the bootstrap method has been proposed as a nonparametric alternative. However, the current bootstrap test for a common mean direction in paleomagnetic analysis lacks consideration of a null hypothesis. In this study, we integrate recent advances to incorporate bootstrap tests into a null hypothesis significance testing framework, improving interpretability and unifying paleomagnetic statistical tests.
Paleomagnetic statistical inference is underpinned by a family of parametric null hypothesis tests. In many cases, however, paleomagnetic data do not meet the distributional assumptions of these tests, which can lead to spurious inferences. Earlier studies have proposed the bootstrap as a nonparametric alternative for paleomagnetic analysis, which can be applied even when the distributional form of the data is unknown. Key among these approaches is the bootstrap test for a common mean direction, which relies on assessment of the overlap of estimated confidence regions. In its current form, the bootstrap test for a common mean paleomagnetic direction does not consider a null hypothesis and can yield outcomes that cannot be interpreted in terms of a statistical significance level. To resolve these issues, we use recent advances to place such bootstrap tests within a null hypothesis significance testing framework, and unify them with the existing family of paleomagnetic statistical tests. Furthermore, using numerical experiments we demonstrate the applicability of such a nonparametric approach to moderately sized paleomagnetic data sets typical of modern and legacy studies. Finally, we demonstrate how a confidence region can be estimated for the common mean of two sets of directions and how known directions, such as the expected field produced by a geocentric axial dipole, can be compared to that mean.
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