timeOptTemplateSim {astrochron} R Documentation

## Simulations for timeOptTemplate

### Description

Simulations for timeOptTemplate

### Usage

timeOptTemplateSim(dat,template=NULL,corVal=NULL,numsim=2000,rho=NULL,sedmin=0.5,sedmax=5,
difmin=NULL,difmax=NULL,fac=NULL,numsed=50,linLog=1,limit=T,fit=1,fitModPwr=T,
iopt=3,flow=NULL,fhigh=NULL,roll=NULL,targetE=NULL,targetP=NULL,
cormethod=1,detrend=T,detrendTemplate=F,flipTemplate=F,ncores=1,output=0,
genplot=T,check=T,verbose=T)


### Arguments

 dat Stratigraphic series for modulation assessment. First column should be depth or height (in meters), second column should be data value. template Instantaneous sedimentation rate template to fit. This represents a unitless proportional sedimentation rate history. Default template is a copy of dat, which will be scaled for instantaneous accumulation optimization. corVal r2opt value for data. By default this will be calculated. numsim Number of Monte Carlo AR1 simulations. rho AR1 coefficient to use in simulations. By default this will be estimated from the stratigraphic series. sedmin Minimum AVERAGE sedimentation rate for investigation (cm/ka). sedmax Maximum AVERAGE sedimentation rate for investigation (cm/ka). difmin Minimum instantaneous sedimentation rate to investigate (cm/ka). difmax Maximum instantaneous sedimentation rate to investigate (cm/ka). By default, this is ignored, and fac is used. fac Maximum instantaneous accumulation factor. Maximum rate is scaled to each investigated sedrate as fac*sedrate. Default value of 5 is based on experimentation. If larger than this, risk getting into local minimum during fit. numsed Number of sedimentation rates to investigate in optimization grid. linLog Use linear or logarithmic scaling for sedimentation rate grid spacing? (0=linear, 1=log) limit Limit evaluated sedimentation rates to region in which full target signal can be recovered? (T or F) fit Test for (1) precession amplitude modulations or (2) short eccentricity amplitude modulations? fit= 2 is not yet functional. fitModPwr Include the modulation periods in the spectral fit? (T or F) iopt Optimize on (1) modulations, (2) power, (3) mod*power flow Low frequency cut-off for Taner bandpass (half power point; in cycles/ka) fhigh High frequency cut-off for Taner bandpass (half power point; in cycles/ka) roll Taner filter roll-off rate, in dB/octave. Default value is 10^3. targetE A vector of eccentricity periods to evaluate (in ka). These must be in order of decreasing period, with first value of 405 ka. targetP A vector of precession periods to evaluate (in ka). These must be in order of decreasing period. cormethod Method used for calculation of correlation coefficient (1=Pearson, 2=Spearman) detrend Remove linear trend from data series? (T or F) detrendTemplate Remove linear trend from sedimentation rate template? (T or F) flipTemplate Flip direction of sedimentation rate template? (T or F) ncores Number of cores to use for parallel processing output Which results you like to return to console? (0) no output; (1) return sedimentation rate grid, p, r, r*p; (2) return optimal time series, bandpassed series, Hilbert and fitted periods genplot Generate summary plots? (T or F) check Conduct compliance checks before processing? (T or F) In general this should be activated; the option is included for Monte Carlo simulation. verbose Verbose output? (T or F)

### Details

TimeOpt employs a probabilistic linear regression model framework to investigate amplitude modulation and frequency ratios (bundling) in stratigraphic data, while simultaneously determining the optimal time scale. This function further develops the method to optimize upon complex sedimentation templates. The approach is demonstrated below with a series of examples.

The statistical significance of the r^2_opt is determined via Monte Carlo simulation (see timeOptSim). See timeOpt for more information on the basic methodology.

### Value

QUESTION: is this correct?

if output = 1, a data frame containing the following will be returned: Sedimentation rate (cm/ka), r-squared value for instantaneous amplitude vs. fitted periods, r-squared value for fit to specified periods, r-squared*r-squared.

if output = 2, a data frame containing the following will be returned: Time (ka), tuned time series, bandpassed series, instantaneous amplitude, fitted periods.

### References

S.R. Meyers, 2015, The evaluation of eccentricity-related amplitude modulations and bundling in paleoclimate data: An inverse approach for astrochronologic testing and time scale optimization: Paleoceanography.

S.R. Meyers, 2019, Cyclostratigraphy and the problem of astrochronologic testing: Earth-Science Reviews.

### Examples

## Not run:

# EXAMPLE (1): Differential accumulation across bedding couplets
ex=etp(tmin=0,tmax=1000,dt=5,pWt=1,oWt=0,eWt=1,esinw=TRUE)
ex2=diffAccum(ex,0.01,.05)
ex2=linterp(ex2)
# first with the nominal timeOpt approach
timeOpt(ex2,sedmin=1,sedmax=4,numsed=100)
timeOptSim(ex2,sedmin=1,sedmax=4,numsed=100,numsim=2000)
# then with the timeOptTemplate approach
timeOptTemplate(ex2,sedmin=1,sedmax=4,difmin=.5,difmax=6,numsed=100,ncores=2)
timeOptTemplateSim(ex2,sedmin=1,sedmax=4,difmin=.5,difmax=6,numsed=100,numsim=1000,
ncores=2)

# EXAMPLE (2): Linear sedimentation rate increase
ex=etp(tmin=0,tmax=1000,dt=5,pWt=1,oWt=0,eWt=1,esinw=TRUE)
ex2=sedRamp(ex,srstart=0.01,srend=0.05)
ex2=linterp(ex2)
# first with the nominal timeOpt approach
timeOpt(ex2,sedmin=1,sedmax=4,numsed=100)
# then with the timeOptTemplate approach
# create linear model for input. the magnitude does not matter, it will be rescaled.
# (it just needs to be a line)
template=ex2; template[2]=ex2[1]
timeOptTemplate(ex2,template=template,sedmin=1,sedmax=4,numsed=100,ncores=2)
# view optimization procedure
timeOptTemplate(ex2,template=template,sedmin=2.75,sedmax=3.25,numsed=20,ncores=1,genplot=2)

# EXAMPLE (3): Step increase in sedimentation rate, from 1 cm/kyr to 2 cm/kyr at 7 meters depth
ex=etp(tmin=0,tmax=1000,dt=5,pWt=1,oWt=0,eWt=1,esinw=TRUE)
ex2=ex
ex2[1]=ex[1]*.01
ex2[141:201,1]=ex2[141:201,1]*2-7
ex2=linterp(ex2)
# first with the nominal timeOpt approach
timeOpt(ex2,sedmin=1,sedmax=4,numsed=100)
# then with the timeOptTemplate approach
# create step model for input. the magnitude does not matter, it will be rescaled.
template=ex2; template[1:140,2]=1; template[141:261,2]=2
timeOptTemplate(ex2,template=template,sedmin=1,sedmax=4,numsed=100,ncores=2)
# view optimization procedure
timeOptTemplate(ex2,template=template,sedmin=1,sedmax=2,numsed=20,ncores=1,genplot=2)

# EXAMPLE (4): A record with a 100 kyr hiatus at 10 meters depth
ex=etp(tmin=0,tmax=1000,dt=5,pWt=1,oWt=0,eWt=1,esinw=TRUE)
ex2=delPts(ex,del=101:121)
# use a background sedimentation rate of 2 cm/kyr
ex2[1]=0:179*5*0.02
# first evaluate the distorted record with the nominal timeOpt approach
timeOpt(ex2,sedmin=1,sedmax=4,numsed=100)
# then with the timeOptTemplate approach
# create a constant sedimentation rate model with possible hiatus of unknown
#  duration at 10 m
template=ex2; template[2]=10; template[101,2]=1
timeOptTemplate(ex2,template=template,sedmin=1,sedmax=3,difmax=3,numsed=100,ncores=2)
# now perform a finer grid search near the maximum, using power only
#  notice the oscillatory nature of the power fit.
res=timeOptTemplate(ex2,template=template,sedmin=1.5,sedmax=2,difmax=3,numsed=100,ncores=2,
iopt=2,output=2)
# compare true eccentricity to TimeOpt-derived eccentricity
pl(2)
plot(ex,type="l",main="True Eccentricity Series",xlab="True Time (kyr)",ylab="")
plot(res[,1],res[,4],type="l",main="Black=TimeOpt precession AM;  Red=TimeOpt eccentricity model",
xlab="TimeOpt derived time (kyr)",ylab="")
lines(res[,1],res[,5],col="red",lwd=2)

## End(Not run)


[Package astrochron version 1.1 Index]