Minnaert function
The Minnaert function is a photometric function used to interpret astronomical observations [1][2] and remote sensing data for the Earth.[3] This function expresses the radiance factor (RADF) as a function the phase angle () and the photometric latitude (
) and the photometric longitude (
).
where is the Minnaert albedo,
is an empirical parameter,
is the scattered radiance in the direction
,
is the incident radiance, and
The phase angle is the angle between the light source and the observer with the object as the center.
The assumptions made are:
- the surface is illuminated by a distant point source.
- the surface is isotropic and flat.
Minnaert's contribution is the introduction of the parameter , having a value between 0 and 1,[4] originally for a better interpretation of observations of the Moon. In remote sensing the use of this function is referred to as Minnaert topographic correction, a necessity when interpreting images of rough terrain.
References
- ↑ http://dx.doi.org/10.1016/S0019-1035(03)00075-7
- ↑ http://dx.doi.org/10.1016/j.icarus.2006.05.006
- ↑ http://dx.doi.org/10.1080/01431160500104194
- ↑ http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1941ApJ....93..403M&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf