Abstract

We propose a new distribution for analyzing paleomagnetic directional data, that is, a novel transformation of the von Mises–Fisher distribution. The new distribution has ellipse-like symmetry, as does the Kent distribution; however, unlike the Kent distribution the normalizing constant in the new density is easy to compute and estimation of the shape parameters is straightforward. To accommodate outliers, the model also incorporates an additional shape parameter, which controls the tail-weight of the distribution. We also develop a general regression model framework that allows both the mean direction and the shape parameters of the error distribution to depend on covariates. The proposed regression procedure is shown to be equivariant with respect to the choice of coordinate system for the directional response. To illustrate, we analyses paleomagnetic directional data from the GEOMAGIA50.v3 database. We predict the mean direction at various geological time points and show that there is significant heteroscedasticity present. It is envisaged that the regression structures and error distribution proposed here will also prove useful when covariate information is available with (i) other types of directional response data; and (ii) square-root transformed compositional data of general dimension. Supplementary materials for this article are available online. Code submitted with this article was checked by an Associate Editor for Reproducibility and is available as an online supplement.

Highlights

  • 1.1 Background: paleomagnetic directional dataSpherical data are frequently encountered in the earth and environmental sciences (e.g. Schuenemeyer and Drew, 2011; Borradaile, 2003)

  • We mention that Rivest et al (2016) suggest some interesting ideas for regression modelling on the circle; some of these ideas may prove useful for regression modelling on the sphere

  • The model is a Q-symmetric model as defined by Rivest (1984) and Rivest showed that the information matrix in such models is block diagonal

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Summary

Background: paleomagnetic directional data

Spherical data are frequently encountered in the earth and environmental sciences (e.g. Schuenemeyer and Drew, 2011; Borradaile, 2003). In other cases, depending on the data available, it is of interest to explore the relationships between the directions versus geological time and/or space to understand how the Earth’s magnetic field has evolved In this case, to account for the highly non-linear relationships between the geomagnetic field directions and the covariates, in the geophysics literature, the geomagnetic field is usually expressed in terms of spherical harmonics, and the temporal evolution of the process is modelled using cubic B-splines. In the conversion we use the following reference frame: y1 = sin I, y2 = cos I cos D and y3 = cos I sin D, where I represents inclination defined on [−90◦, 90◦] and D represents declination defined on [0◦, 360◦] Both the Kent distribution and von Mises-Fisher have been used to a limited extent to summarise paleomagnetic data samples They based inference for the moments on a nonparametric bootstrap method, but this has the disadvantage of being computationally intensive and is cumbersome to apply

Main contributions of the paper
Relevant literature
Structure of the paper
Construction of a Kent-like distribution
Moment and M-estimators of location parameters
Maximum likelihood estimation of all parameters
Regression case
Link functions
Estimation
Equivariance
Analysis of paleomagnetic directional data
Simulation
Conclusion
A Proofs
Proof of Proposition 1
Proof of Proposition 2
Proof of Proposition 3
Proof of Proposition 4
Full Text
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