This function returns the energy to mole of photons ratio for each waveband and a light source spectrum.
eq_ratio(spct, w.band, wb.trim, use.cached.mult, use.hinges, ...)# S3 method for default
eq_ratio(spct, w.band, wb.trim, use.cached.mult, use.hinges,
...)
# S3 method for source_spct
eq_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
eq_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 numeric value giving number of Joule per mol of photons 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 "e:q" prepended..
default
: Default for generic function
source_spct
: Method for source_spct
objects
source_mspct
: Calculates energy:photon from a source_mspct
object.
Other photon and energy ratio functions: e_ratio
,
energy_ratio
, photon_ratio
,
photons_energy_ratio
,
q_ratio
, qe_ratio
# NOT RUN {
eq_ratio(sun.spct, new_waveband(400,700))
# }
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