The hardware and bandwidth for this mirror is donated by METANET, the Webhosting and Full Service-Cloud Provider.
If you wish to report a bug, or if you are interested in having us mirror your free-software or open-source project, please feel free to contact us at mirror[@]metanet.ch.
NNS
offers several novel sampling methods from any
distribution, as well as simulating variables while maintaining their
dependence.
Cumulative distribution functions (CDFs) represent the probability a variable \(X\) will take a value less than or equal to \(x\). \[F(x) = P(X \leq x)\]
The empirical CDF is a simple construct, provided in the base package
of R. We can generate an empirical CDF with the ecdf
function and create a function (P)
to return the CDF of a
given value of \(X\).
## Empirical CDF
## Call: ecdf(x)
## x[1:100] = -2.3092, -1.9666, -1.6867, ..., 2.169, 2.1873
## [1] 0.48
## [1] 0.83
LPM.ratio
) The empirical CDF and Lower Partial Moment CDF
(LPM.ratio
) are identical when the degree
term of the LPM.ratio
is set to zero.
Degree 0 LPM: \[LPM(0,t,X)=\frac{1}{N}\sum_{n=1}^{N}[max(t-X_n),0]^0\]
LPM.ratio
is equivalent to the following form for any
target \((t)\) and variable \(X\): \[LPM(0,t,X)=\frac{LPM(0,t,X)}{LPM(0,t,X)+UPM(0,t,X)}\]
Using the same targets from our ecdf
example above (0,1)
we can compare LPM.ratio
s.
## [1] 0.48
## [1] 0.83
Calculating the probability for every target
value in
\(X\), we can plot both methods
visualizing their identical results. ecdf
function in black
and LPM.ratio
in red.
LPM.ratio
degree > 0By simply increasing the degree
parameter to any
positive real number, we can generate different CDFs of our initial
distribution \(x\).
LPM.VaR
)We can now generate distributions using the same insights and
degree
manipulation in the corresponding
LPM.VaR
function, a la value-at-risk,
providing inverse CDF estimates.
The general form in the following plots is:
LPM.VaR(percentile = seq(0, 1, length.out = 100), degree = 0, x = x)
Any length percentile
can be used to sample from the
underlying distribution \(x\).
Viewing the first 10 samples from each of the degree
s
compared to our original \(X\).
degree.0.samples = LPM.VaR(percentile = seq(0, 1, length.out = 100), degree = 0, x = x)
degree.0.25.samples = LPM.VaR(percentile = seq(0, 1, length.out = 100), degree = 0.25, x = x)
degree.0.5.samples = LPM.VaR(percentile = seq(0, 1, length.out = 100), degree = 0.5, x = x)
degree.1.samples = LPM.VaR(percentile = seq(0, 1, length.out = 100), degree = 1, x = x)
degree.2.samples = LPM.VaR(percentile = seq(0, 1, length.out = 100), degree = 2, x = x)
head(data.table::data.table(cbind("original x" = sort(x), degree.0.samples,
degree.0.25.samples,
degree.0.5.samples,
degree.1.samples,
degree.2.samples)), 10)
original x degree.0.samples degree.0.25.samples degree.0.5.samples
1: -2.309169 -2.309169 -2.309097 -2.3090915
2: -1.966617 -1.966617 -1.941190 -1.6935509
3: -1.686693 -1.686693 -1.599486 -1.4541494
4: -1.548753 -1.548753 -1.382553 -1.2462731
5: -1.265396 -1.265396 -1.250823 -1.1453748
6: -1.265061 -1.265061 -1.176436 -1.0745440
7: -1.220718 -1.220718 -1.119655 -1.0252742
8: -1.138137 -1.138137 -1.067793 -0.9868693
9: -1.123109 -1.123109 -1.026429 -0.9322105
10: -1.071791 -1.071791 -1.014276 -0.8710942
degree.1.samples degree.2.samples
1: -2.3091021 -2.3091170
2: -1.4744653 -1.1614908
3: -1.2159961 -0.9709972
4: -1.0823023 -0.8610192
5: -0.9968028 -0.7810300
6: -0.9290505 -0.7169770
7: -0.8666886 -0.6631888
8: -0.8090433 -0.6170691
9: -0.7556644 -0.5765608
10: -0.7069835 -0.5403318
NNS.meboot
)NNS.meboot
is based on the maximum
entropy bootstrap, available in the R-package meboot
. This
procedure is specifically designed for time-series and avoids the IID
assumption in traditional methods.
The ability to sample from specified correlations ensures the full spectrum of future paths is sampled from. Typical Monte Carlo samples are restricted to [-0.3, 0.3] correlations to the original data.
We will generate 1 replicate of \(X\) for each value of a sequence of \(\rho\) values, and then plot the results
compared to our original \(X\) (black
line). NNS.MC
is a streamlined wrapper
function for this functionality of
NNS.meboot
.
boots = NNS.MC(x, reps = 1, lower_rho = -1, upper_rho = 1, by = .5)$replicates
reps = do.call(cbind, boots)
plot(x, type = "l", lwd = 3, ylim = c(min(reps), max(reps)))
matplot(reps, type = "l", col = rainbow(length(boots)), add = TRUE)
Checking our replicate correlations:
sapply(boots, function(r) cor(r, x, method = "spearman"))
rho = 1 rho = 0.5 rho = -0.5 rho = -1
1.0000000 0.4988059 -0.4995740 -0.9982358
More replicates and ensembles thereof can be generated for any number
of \(\rho\) values. Please see the full
NNS.meboot
and
NNS.MC
argument documentation.
Analogous to an empirical copula transformation, we can generate
new data
from the dependence structure of our
original data
via the following steps:
This is accomplished using
LPM.ratio(1, x, x)
for continuous
variables, and LPM.ratio(0, x, x)
for
discrete variables, which are the empirical CDFs of the marginal
variables.
new data
:new data
does not have to be of the same distribution or
dimension as the original data
, nor does each dimension of
new data
have to share a distribution type.
new data
:We then utilize LPM.VaR
to ascertain
new data
values corresponding to original data
position mappings, and return a matrix of these transformed values with
the same dimensions as new.data
.
set.seed(123)
x <- rnorm(1000); y <- rnorm(1000); z <- rnorm(1000)
# Add variable x to original data to avoid total independence (example only)
original.data <- cbind(x, y, z, x)
# Determine dependence structure
dep.structure <- apply(original.data, 2, function(x) LPM.ratio(degree = 1, target = x, variable = x))
# Generate new data with different mean, sd and length (or distribution type)
new.data <- sapply(1:ncol(original.data), function(x) rnorm(nrow(original.data)*2, mean = 10, sd = 20))
# Apply dependence structure to new data
new.dep.data <- sapply(1:ncol(original.data), function(x) LPM.VaR(percentile = dep.structure[,x], degree = 1, x = new.data[,x]))
Similar dependence with radically different values, since we used \(N(10, 20)\) in place of our original \(N(0,1)\) observations.
head(original.data)
head(new.dep.data)
x y z x
[1,] -0.56047565 -0.99579872 -0.5116037 -0.56047565
[2,] -0.23017749 -1.03995504 0.2369379 -0.23017749
[3,] 1.55870831 -0.01798024 -0.5415892 1.55870831
[4,] 0.07050839 -0.13217513 1.2192276 0.07050839
[5,] 0.12928774 -2.54934277 0.1741359 0.12928774
[6,] 1.71506499 1.04057346 -0.6152683 1.71506499
[,1] [,2] [,3] [,4]
[1,] -2.028109 -10.498044 -0.2090467 -1.682949
[2,] 4.608303 -11.390485 15.6213689 4.852534
[3,] 39.478741 8.836581 -0.8508203 40.585505
[4,] 10.683731 6.609255 36.0328589 10.877677
[5,] 11.866922 -47.955235 14.3111350 12.064633
[6,] 42.665726 29.639640 -2.4141874 43.797025
NNS.meboot
Alternatively, if we wish to keep the simulated values close to the
original data, we can apply the NNS.meboot
procedure to each of the variables.
We will generate 1 replicate (for brevity) of \(\rho = 0.95\) to our
original.data
, use their ensemble
and note the
multivariate dependence among our new.boot.dep.data
.
# Apply bootstrap to each variable
new.boot.dep.data = apply(original.data, 2, function(r) NNS.meboot(r, reps = 1, rho = .95))
# Reformat into vectors
boot.ensemble.vectors = lapply(new.boot.dep.data, function(z) unlist(z["ensemble",]))
# Create matrix from vectors
new.boot.dep.matrix = do.call(cbind, boot.ensemble.vectors)
Checking ensemble
correlations with
original.data
:
for(i in 1:4) print(cor(new.boot.dep.matrix[,i], original.data[,i], method = "spearman"))
[1] 0.9453275
[1] 0.9523726
[1] 0.9498499
[1] 0.9524516
Similar dependence with similar values.
head(original.data)
head(new.boot.dep.matrix)
x y z x
[1,] -0.56047565 -0.99579872 -0.5116037 -0.56047565
[2,] -0.23017749 -1.03995504 0.2369379 -0.23017749
[3,] 1.55870831 -0.01798024 -0.5415892 1.55870831
[4,] 0.07050839 -0.13217513 1.2192276 0.07050839
[5,] 0.12928774 -2.54934277 0.1741359 0.12928774
[6,] 1.71506499 1.04057346 -0.6152683 1.71506499
x y z x
ensemble1 -0.4667731 -0.8418413 -0.6139059 -0.4708890
ensemble2 -0.2333747 -1.0908710 0.3748315 -0.2711240
ensemble3 1.4799734 0.2893831 -0.3851513 1.3645317
ensemble4 0.1751654 0.2995113 1.1342461 0.1486429
ensemble5 0.4128802 -2.9789634 -0.1141124 0.3846150
ensemble6 1.5592660 1.1800553 -0.5285532 1.5041917
If the user is so motivated, detailed arguments and proofs are provided within the following:
These binaries (installable software) and packages are in development.
They may not be fully stable and should be used with caution. We make no claims about them.