Minnaert function explained
The Minnaert function is a photometric function used to interpret astronomical observations[1] [2] and remote sensing data for the Earth.[3] It was named after the astronomer Marcel Minnaert. This function expresses the radiance factor (RADF) as a function the phase angle (
), 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
\mu0=\cos\varphi~\cos(\alpha-λ)~;~~\mu=\cos\varphi~\cosλ~.
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
- 10.1016/S0019-1035(03)00075-7 . 2003Icar..163..150C . 163 . Probing Titan's lower atmosphere with acousto-optic tuning . Icarus . 2003 . 150–163. Chanover . N.J. . Anderson . C.M. . McKay . C.P. . Rannou . P. . Glenar . D.A. . Hillman . J.J. . Blass . W.E. . 1 .
- 10.1016/j.icarus.2006.05.006 . 2006Icar..184..401S . 184 . Martian phase function: Modeling the visible to near-infrared surface photometric function using HST-WFPC2 data . Icarus . 2006 . 401–423. Soderblom . J. . Belliii . J. . Hubbard . M. . Wolff . M. . 2 .
- 10.1080/01431160500104194 . 26 . The use of the Minnaert correction for land-cover classification in mountainous terrain . International Journal of Remote Sensing . 2005 . 3831–3851. Blesius . L. . Weirich . F. . 17 . 2005IJRS...26.3831B . 129750287 .
- The reciprocity principle in lunar photometry. 1941ApJ....93..403M. Minnaert. M.. The Astrophysical Journal. 1941. 93. 403. 10.1086/144279.