Estimates the Secchi disk visibility depth using the Tyler (1968) approximation \(z_S \approx 1.7 / K_d\). When a spectral irradiance is supplied the function first computes an irradiance-weighted mean Kd across the visible range before applying the approximation.
References
Tyler JE (1968) Limnol. Oceanogr. 13:1-6. Preisendorfer RW (1986) Limnol. Oceanogr. 31:909-926.
Examples
secchi_depth(jerlov_Kd("IA", lambda = 490))
#> [1] 78.7037