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This function gives the result of integrating spectral irradiance over wavelengths.
integrate_xy(x, y)
numeric vector.
a single numeric value with no change in scale factor: e.g. [W m-2 nm-1] -> [W m-2]
Other low-level functions operating on numeric vectors.: as_energy(), as_quantum_mol(), calc_multipliers(), div_spectra(), energy_irradiance(), energy_ratio(), insert_hinges(), 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()
as_energy()
as_quantum_mol()
calc_multipliers()
div_spectra()
energy_irradiance()
energy_ratio()
insert_hinges()
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, integrate_xy(w.length, s.e.irrad)) # }
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