Target periodogram from an astronomical time series (e.g. La2004 ETP)
Source:R/coco_target_from_series.R
coco_target_from_series.RdPeriodogram of an astronomical series, or of an ETP series built from eccentricity, obliquity and precession as in gentarget.m.
Usage
coco_target_from_series(
time_kyr,
value = NULL,
ecc = NULL,
obl = NULL,
prec = NULL,
ne = 1,
nt = 0.6,
np = 0.5,
f1 = 0,
f2 = 0.06,
pad = 10000
)Arguments
- time_kyr
Time axis of the astronomical series, in kyr (numeric vector, evenly spaced; the series is sorted by it and its first step is used as the sampling interval). Required, no default.
- value
Astronomical series to use as target (numeric vector, same length as
time_kyr), e.g. an ETP series;NULLbuilds an ETP series fromecc,oblandprec.Default=NULL.- ecc
Eccentricity series (numeric vector, same length and order as
time_kyr), used withoblandprecinstead ofvalue: the ETP series isne * z(ecc) + nt * z(obl) - np * z(prec), withzthe standardisation to zero mean and unit standard deviation (as in Acycle gentarget.m).Default=NULL.- obl
Obliquity series (numeric vector, same length and order as
time_kyr), used to build the ETP series whenvalueisNULL.Default=NULL.- prec
Precession (index) series (numeric vector, same length and order as
time_kyr), used with a negative sign to build the ETP series whenvalueisNULL.Default=NULL.- ne
Weight of the standardised eccentricity in the ETP series (numeric).
Default=1.- nt
Weight of the standardised obliquity in the ETP series (numeric).
Default=0.6.- np
Weight of the standardised precession in the ETP series (numeric).
Default=0.5.- f1
Lowest frequency of the target that is returned, in cycles/kyr (numeric, >= 0).
Default=0.- f2
Highest frequency of the target that is returned, in cycles/kyr (numeric, >
f1).Default=0.06.- pad
Length (number of points) to which the series is zero-padded for the periodogram (integer; at least the series length is used); a larger value gives a finer frequency grid.
Default=10000.