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Inserting wavelengths values immediately before and after a discontinuity in the SWF, greatly reduces the errors caused by interpolating the weighted irradiance during integration of the effective spectral irradiance. This is specially true when data have a large wavelength step size.
insert_hinges(x, y, h)
numeric vector (sorted in increasing order)
numeric vector
a numeric vector giving the wavelengths at which the y values should be inserted by interpolation, no interpolation is indicated by an empty vector (numeric(0))
a data.frame with variables x
and y
. Unless the hinge
values were already present in y
, each inserted hinge, expands the
vectors returned in the data frame by one value.
Other low-level functions operating on numeric vectors.:
as_energy()
,
as_quantum_mol()
,
calc_multipliers()
,
div_spectra()
,
energy_irradiance()
,
energy_ratio()
,
integrate_xy()
,
interpolate_spectrum()
,
irradiance()
,
l_insert_hinges()
,
oper_spectra()
,
photon_irradiance()
,
photon_ratio()
,
photons_energy_ratio()
,
prod_spectra()
,
s_e_irrad2rgb()
,
split_energy_irradiance()
,
split_photon_irradiance()
,
subt_spectra()
,
sum_spectra()
,
trim_tails()
,
v_insert_hinges()
,
v_replace_hinges()
# NOT RUN {
with(sun.data,
insert_hinges(w.length, s.e.irrad,
c(399.99, 400.00, 699.99, 700.00)))
# }
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