get_solution | R Documentation |
Download supported astronomical solutions from the web and store it in the
user's cache directory. The next use of the function will load the data from
the cache rather than downloading it again. This also provides a wrapper for
astrochron::getLaskar()
if one of their supported solutions is specified,
but converts the output to a tibble. Note that we
do not cache these solutions locally, however.
get_solution(
astronomical_solution = "full-ZB18a",
quiet = FALSE,
force = FALSE
)
astronomical_solution |
Character vector with the name of the desired
solution. Defaults to |
quiet |
Be quiet?
|
force |
Force re-downloading the results, even if the solution is saved to the cache. |
A tibble with the astronomical solution (and some preprocessed new columns).
Zeebe, R. E., & Lourens, L. J. (2019). Solar System chaos and the Paleocene–Eocene boundary age constrained by geology and astronomy. Science, 365(6456), 926–929. \Sexpr[results=rd]{tools:::Rd_expr_doi("10.1126/science.aax0612")}.
Zeebe, R. E. and Lourens, L. J. (2022). A deep-time dating tool for paleo-applications utilizing obliquity and precession cycles: The role of dynamical ellipticity and tidal dissipation. Paleoceanography and Paleoclimatology. \Sexpr[results=rd]{tools:::Rd_expr_doi("10.1029/2021PA004349")}
full_ZB18a, ZB17, ZB18a_100, ZB18a_300 ZB20, PT_ZB18a, ZB23
get_solution("full-ZB18a") # input for snvec
get_solution("ZB18a-300") # eccentricity
get_solution("ZB20a")
get_solution("La11")
get_solution("PT-ZB18a(1,1)") # pre-computed precession-tilt
get_solution("ZB23.R01") # one of the 3.6 Gyr solutions
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