Easily calculate precession and obliquity from an orbital solution (defaults to ZB18a from Zeebe and Lourens (2019) <doi:10.1126/science.aax0612>) and assumed or reconstructed values for tidal dissipation (Td) and dynamical ellipticity (Ed). This is a translation and adaptation of the 'C'-code in the supplementary material to Zeebe and Lourens (2022) <doi:10.1029/2021PA004349>, with further details on the methodology described in Zeebe (2022) <doi:10.3847/1538-3881/ac80f8>. The name of the 'C'-routine is 'snvec', which refers to the key units of computation: spin vector s and orbit normal vector n.
Version: 3.10.1 Depends: R (≥ 3.6.0) Imports: deSolve, cli (≥ 3.4.0), stats, dplyr, tibble, purrr, readr, tidyselect, rlang (≥ 0.4.11), glue, tools, backports (≥ 1.1.6), stringr Suggests: astrochron, ggplot2, tidyr, testthat, roxygen2, knitr, withr, curl, rmarkdown Published: 2025-03-06 DOI: 10.32614/CRAN.package.snvecR Author: Ilja Kocken [aut, cre, trl, cph], Richard Zeebe [aut] Maintainer: Ilja Kocken <ikocken at hawaii.edu> BugReports: https://github.com/japhir/snvecR/issues License: GPL (≥ 3) URL: https://japhir.github.io/snvecR/, https://github.com/japhir/snvecR NeedsCompilation: no Citation: snvecR citation info Materials: README NEWS CRAN checks: snvecR results Documentation: Downloads: Linking:Please use the canonical form https://CRAN.R-project.org/package=snvecR to link to this page.
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