genwwn.thpower {hwwntest} | R Documentation |
Compute (approximation) to the theoretical power of the
genwwn.test
test for
ARMA processes (including, of course, white noise itself).
Description
Compute (approximation) to the theoretical power of the
genwwn.test
test. Note: this
function does no simulation, it merely computes an approximation
to the likely statistical power (or size) of the
genwwn.test
function. It can be useful to establish
the reverse question: what sample size do I require to
achieve a certain power for a given ARMA process?
Usage
genwwn.thpower(N = 128, ar = NULL, ma = NULL, plot.it = FALSE,
sigsq = 1, alpha = 0.05, away.from = "standard",
filter.number = 10, family = "DaubExPhase", verbose = FALSE)
Arguments
N |
The length of the series you want to get a theoretical power result for. |
ar |
Autoregressive parameters. A vector with p entries for AR(p) with the first entry being the value for lag-one term (alpha_1), the second entry being the value for the lag-two term (alpha_2) etc. If this argument is NULL then there are no AR terms. |
ma |
Similar to the |
plot.it |
If |
sigsq |
The theoretical innovation variance (also the variance
of white noise if |
alpha |
The nominal size of the test for this theoretical power calculation. |
away.from |
Describes how many fine scales to exclude, the
same as in |
filter.number |
The number of vanishing moments in the Daubechies series of wavelets. |
family |
The wavelet family. |
verbose |
If TRUE then informative messages are printed during the progress of the function. |
Details
Function calculates the value of the power function at the specified arguments. It does this by: (i) specifying the functional spectrum of the ARMA process (which can be flat, ie white noise); (ii) calculating the variance of the ARMA process by numerical integration of the spectrum; (iii) calculating the spectrum values at the Fourier frequencies; (iv) calculating the wavelet coefficients at the exact spectrum values; (v) computing the exact variance of the wavelet coefficients of the squared normalized spectrum; (vi) computing the approximate power of the whole lot.
Value
A list containing the following components.
C.alpha.c |
The critical value for the test, which is the nominal size critical value after correction for multiple hypothesis tests (correction using Bonferroni). |
th.power |
The computed theoretical power |
norspecwd |
The wavelet coefficients of the true spectrum |
norspecvarwd |
The squared wavelet transform of the squared normalized spectrum |
all.hwc |
All of the wavelet coefficients from the normalized true specturm as a single vector |
all.sdwc |
The ‘true’ standard deviations of the wavelet coefficients |
Author(s)
Delyan Savchev and Guy Nason
References
Nason, G.P. and Savchev, D. (2014) White noise testing using wavelets. Stat, 3, 351-362. doi:10.1002/sta4.69
See Also
Examples
#
# Calculate what the theoretical actual size is likely to be for the
# genwwn.test for a white noise sequence of T=64, nominal size=0.05
#
genwwn.thpower(N=64)$th.power
#[1] 0.04894124
#
# This is pretty close to the nominal size of 5%. Good.
#
# What is the power of detection for the AR(1) process with alpha=0.3?
# Let's say with sample size of T=32
#
genwwn.thpower(N=32, ar=0.3)$th.power
#[1] 0.2294128
#
# That's pretty poor, we'll only detect about 23% of cases. Can we achieve
# a power of 90%? Actually, it turns out that by repeating these above
# functions with N=128 gives a power of 61%, and for N=256 we get a power of
# 90%.