This class makes use of the 1998 sky brightness model by Bradley Schaefer. More...
#include <Skybright.hpp>
This class makes use of the 1998 sky brightness model by Bradley Schaefer.
Compute the luminance of the sky according to some parameters like sun moon position or time or altitude etc...
Further reading: B. Schaefer: Sky&Telescope 4/1987 B. Schaefer: Astronomy and the Limits of Vision. Vistas in Astronomy 36, 311-361, 1993. B. Schaefer: To the Visual Limits. Sky&Telescope 5/1998 57-60. B. Schaefer: Archaeoastronomy XV, 2000. TASKS TO IMPROVE: Some components of the Schaefer model are strongly simplified. E.g.,
Definition at line 39 of file Skybright.hpp.
Constructor.()