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: |
3.9.3 |
| 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) |
| Suggests: |
astrochron, ggplot2, tidyr, testthat, roxygen2, knitr, withr, curl, rmarkdown |
| Published: |
2024-04-24 |
| 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: |
yes |
| Citation: |
snvecR citation info |
| Materials: |
README NEWS |
| CRAN checks: |
snvecR results |