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This function returns the red:far-red photon ratio of a light source spectrum.
R_FR(spct, std = "Smith10", use.cached.mult = FALSE, use.hinges = TRUE)
a single numeric dimensionless value giving the R:FR photon ratio, with name attribute set to the name of the wavebands, with "(q:q)" appended.
an object of class "source.spct".
select which definition of red and far-red should be used, defaults to "Smith".
logical indicating whether multiplier values should be cached between calls.
logical indicating whether to use hinges to reduce interpolation errors.
Red, Far_red and q_ratio.
Red
Far_red
q_ratio
R_FR(sun.spct)
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