# \donttest{
#Extract the 405 kyr eccentricity cycle from the the magnetic susceptibility \cr
#record of the Sullivan core and use the Gabor uncertainty principle to define \cr
#the mathematical uncertainty of the analysis and use a factor of that standard \cr
#deviation to define boundaries.
#Perform the CWT
mag_wt <- analyze_wavelet(data = mag,
dj = 1/100,
lowerPeriod = 0.1,
upperPeriod = 254,
verbose = FALSE,
omega_nr = 10)
#Track the 405 kyr eccentricity cycle in a wavelet spectra
#mag_track <- track_period_wavelet(astro_cycle = 405,
# wavelet=mag_wt,
# n.levels = 100,
# periodlab = "Period (metres)",
# x_lab = "depth (metres)")
#Instead of tracking, the tracked solution data set \code{\link{mag_track_solution}} is used \cr
mag_track <- mag_track_solution
mag_track_complete <- completed_series(
wavelet = mag_wt,
tracked_curve = mag_track,
period_up = 1.2,
period_down = 0.8,
extrapolate = TRUE,
genplot = FALSE
)
# smooth the tracking of the 405 kyr eccentricity cycle
mag_track_complete <- loess_auto(time_series = mag_track_complete,
genplot = FALSE, print_span = FALSE)
# extract the 405 kyr eccentricity cycle from the wavelet spectrum and use the \cr
# tracked cycle curve and set factors of the extracted cycle as boundaries
mag_405_ecc <- extract_signal(
tracked_cycle_curve = mag_track_complete,
wavelet = mag_wt,
period_up = 1.2,
period_down = 0.8,
add_mean = TRUE,
tracked_cycle_period = 405,
extract_cycle = 405,
tune = FALSE,
plot_residual = FALSE
)
# }
Run the code above in your browser using DataLab