Nothing
#' Calculate density function and integrate between limits
#'
#' #' \code{liksrss} calculates density function for a normal distribution and
#' integrates between limits of SRSS times (dawn/dusk)
#'
#' @param obs input light observation. See \code{\link{calc.srss}}
#' @param srss is raster of possible SR or SS times within study area
#' @param srsd is raster of SD of SRSS times in study area calculated with \code{raster::focal}
#'
#' @return an array of SRSS-based likelihoods
liksrss <- function(obs, srss, srsd){
if(is.na(obs)){
srssout = srss
raster::values(srssout) = 0
} else{
# midT = (maxT + minT) / 2
# Tsd = (maxT - minT) / 4
#d = obs-srss
# widx = w >= minT & w <= maxT & !is.na(w)
sdf = data.frame(sr = as.vector(srss), srsd = as.vector(srsd))
sdf$srsd[is.na(sdf$srsd)] = 0
# wint = apply(wdf, 1, function(x) pracma::integral(dnorm, minT, maxT, mean = x[1], sd = x[2]))
# wint = apply(wdf, 1, function(x) integrate(dnorm, x[1]-x[2], x[1]+x[2], mean = midT, sd = Tsd * 2)$value)
res = stats::dnorm(obs, sdf$sr, sdf$srsd)
srssout = srss
raster::values(srssout) = res
# w = w * 0
# w[widx] = wint
# w
}
srssout
}
Any scripts or data that you put into this service are public.
Add the following code to your website.
For more information on customizing the embed code, read Embedding Snippets.