This function returns the photon to energy ratio for each waveband of a light source spectrum.
qe_ratio(spct, w.band, wb.trim, use.cached.mult, use.hinges, ...)# S3 method for default
qe_ratio(spct, w.band, wb.trim, use.cached.mult, use.hinges,
...)
# S3 method for source_spct
qe_ratio(spct, w.band = NULL,
wb.trim = getOption("photobiology.waveband.trim", default = TRUE),
use.cached.mult = FALSE,
use.hinges = getOption("photobiology.use.hinges"), ...)
# S3 method for source_mspct
qe_ratio(spct, w.band = NULL,
wb.trim = getOption("photobiology.waveband.trim", default = TRUE),
use.cached.mult = FALSE,
use.hinges = getOption("photobiology.use.hinges"), ...,
idx = !is.null(names(spct)))
source_spct
waveband or list of waveband objects
logical if TRUE wavebands crossing spectral data boundaries are trimmed, if FALSE, they are discarded
logical Flag telling whether multiplier values should be cached between calls
logical Flag telling whether to use hinges to reduce interpolation errors
other arguments (possibly ignored)
logical whether to add a column with the names of the elements of spct
A vector of numeric
values giving number of moles of photons
per Joule for each waveband, with name attribute set to the name of each
waveband unless a named list of wavebands is supplied in which case the
names of the list elements are used, with "q:e" prepended..
default
: Default for generic function
source_spct
: Method for source_spct
objects
source_mspct
: Calculates photon:energy ratio from a
source_mspct
object.
Other photon and energy ratio functions: e_ratio
,
energy_ratio
, eq_ratio
,
photon_ratio
,
photons_energy_ratio
, q_ratio
# NOT RUN {
qe_ratio(sun.spct, new_waveband(400,700))
# }
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