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#' Integrate ranges under curve.
#'
#' \code{stat_wb_column} computes means under a curve. It first integrates the
#' area under a spectral curve and also the mean expressed per nanaometre of
#' wavelength for each waveband in the input. Sets suitable default aesthetics
#' for "rect" geom.
#'
#' @param mapping The aesthetic mapping, usually constructed with
#' \code{\link[ggplot2]{aes}} or \code{\link[ggplot2]{aes_}}. Only needs
#' to be set at the layer level if you are overriding the plot defaults.
#' @param data A layer specific dataset - only needed if you want to override
#' the plot defaults.
#' @param geom The geometric object to use display the data
#' @param position The position adjustment to use for overlapping points on this
#' layer
#' @param show.legend logical. Should this layer be included in the legends?
#' \code{NA}, the default, includes if any aesthetics are mapped. \code{FALSE}
#' never includes, and \code{TRUE} always includes.
#' @param inherit.aes If \code{FALSE}, overrides the default aesthetics, rather
#' than combining with them. This is most useful for helper functions that
#' define both data and aesthetics and shouldn't inherit behaviour from the
#' default plot specification, e.g. \code{\link[ggplot2]{borders}}.
#' @param ... other arguments passed on to \code{\link[ggplot2]{layer}}. This
#' can include aesthetics whose values you want to set, not map. See
#' \code{\link[ggplot2]{layer}} for more details.
#' @param na.rm a logical value indicating whether NA values should be stripped
#' before the computation proceeds.
#' @param w.band a waveband object or a list of waveband objects or numeric
#' vector of at least length two.
#' @param integral.fun function on $x$ and $y$.
#' @param chroma.type character one of "CMF" (color matching function) or "CC"
#' (color coordinates) or a \code{\link[photobiology]{chroma_spct}} object.
#'
#' @return A data frame with one row for each waveband object in the argument
#' to \code{w.band}. Wavebeand outside the range of the spectral data are
#' trimmed or discarded.
#'
#' @section Computed variables:
#' What it is named integral below is the result of appying \code{integral.fun},
#' with default \code{integrate_xy}.
#' \describe{
#' \item{x}{w.band-midpoint}
#' \item{wb.xmin}{w.band minimum}
#' \item{wb.xmax}{w.band maximum}
#' \item{wb.ymin}{data$y minimum}
#' \item{wb.ymax}{data$y maximum}
#' \item{wb.ymean}{yint divided by wl_expanse(w.band)}
#' \item{y}{wb.ymeam}
#' \item{wb.color}{color of the w.band}
#' \item{wb.name}{label of w.band}
#' \item{BW.color}{\code{black_or_white(wb.color)}}
#' }
#'
#' @section Default aesthetics:
#' Set by the statistic and available to geoms.
#' \describe{
#' \item{xmin}{..wb.xmin..}
#' \item{xmax}{..wb.xmax..}
#' \item{ymin}{0}
#' \item{ymax}{..wb.ymean..}
#' \item{fill}{..wb.color..}
#' }
#'
#' @section Required aesthetics:
#' Required by the statistic and need to be set with \code{aes()}.
#' \describe{
#' \item{x}{numeric, wavelength in nanometres}
#' \item{y}{numeric, a spectral quantity}
#' }
#'
#' @examples
#'
#' library(photobiologyWavebands)
#' # ggplot() methods for spectral objects set a default mapping for x and y.
#' ggplot(sun.spct) +
#' stat_wb_column(w.band = VIS_bands()) +
#' geom_line() +
#' scale_fill_identity()
#'
#' ggplot(sun.spct) +
#' stat_wb_column(w.band = VIS_bands(), alpha = 0.5) +
#' geom_line() +
#' scale_fill_identity()
#'
#' @note If the argument passed to \code{w.band} is a BSWF it is silently
#' converted to a wavelength range and the average of spectral values without
#' weighting is returned as default value for \code{ymax} while the default
#' value for \code{ymin} is zero.
#'
#' @export
#'
#' @family stats functions
#'
stat_wb_column <- function(mapping = NULL,
data = NULL,
geom = "rect",
w.band = NULL,
integral.fun = integrate_xy,
chroma.type = "CMF",
position = "identity",
na.rm = FALSE,
show.legend = NA,
inherit.aes = TRUE,
...) {
ggplot2::layer(
stat = StatWbColumn, data = data, mapping = mapping, geom = geom,
position = position, show.legend = show.legend, inherit.aes = inherit.aes,
params = list(w.band = w.band,
integral.fun = integral.fun,
chroma.type = chroma.type,
na.rm = na.rm,
...)
)
}
# Defined here to make sure R check does not skip it.
#' @rdname gg2spectra-ggproto
#'
#' @format NULL
#' @usage NULL
#'
wb_col_compute_group <-
function(data,
scales,
w.band,
integral.fun,
chroma.type){
if (length(w.band) == 0) {
w.band <- waveband(data[["x"]])
}
if (is.any_spct(w.band) ||
(is.numeric(w.band) && length(stats::na.omit(w.band)) >= 2)) {
w.band <- waveband(range(w.band, na.rm = TRUE))
}
if (!is.list(w.band) || is.waveband(w.band)) {
w.band <- list(w.band)
}
stopifnot(is.function(integral.fun))
w.band <- trim_wl(w.band, data[["x"]])
integ.df <- data.frame()
for (wb in w.band) {
if (is.numeric(wb)) { # user supplied a list of numeric vectors
wb <- waveband(wb)
}
range <- range(wb)
mydata <- trim_tails(data[["x"]], data[["y"]], use.hinges = TRUE,
low.limit = range[1],
high.limit = range[2])
yint.tmp <- integral.fun(mydata[["x"]], mydata[["y"]])
ymean.tmp <- yint.tmp / wl_expanse(wb)
wb.color <- photobiology::fast_color_of_wb(wb, chroma.type = chroma.type)
integ.df <- rbind(integ.df,
data.frame(x = midpoint(mydata[["x"]]),
wb.xmin = min(wb),
wb.xmax = max(wb),
y = ymean.tmp,
yzero = 0,
wb.ymin = min(data[["y"]]),
wb.ymax = max(data[["y"]]),
wb.ymean = ymean.tmp,
wb.color = wb.color,
wb.name = labels(wb)[["label"]],
BW.color = black_or_white(wb.color))
)
}
integ.df
}
#' @rdname gg2spectra-ggproto
#' @format NULL
#' @usage NULL
#' @export
StatWbColumn <-
ggplot2::ggproto("StatWbColumn", ggplot2::Stat,
compute_group = wb_col_compute_group,
default_aes = ggplot2::aes(xmin = after_stat(wb.xmin),
xmax = after_stat(wb.xmax),
ymax = after_stat(wb.ymean),
ymin = after_stat(yzero), # a numeric constant is ignored!!
fill = after_stat(wb.color)),
required_aes = c("x", "y")
)
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