[GRASS-user] running r.sun with ancillary layers.

Hi,

I need some suggestions to run r.sun and use the Albedo-Modis product as an input for the r.sun albedo parameter.
Albedo-Modis has two main products: White-sky and Black-sky

"White-sky is the bihemispherical reflectance under conditions of isotropic illumination, so it has the angular dependency removed. Black-sky is the directional hemispherical reflectance computed at local solar noon."

Which one of these is the most appropriate to use?

Moreover, “white-sky” and “black-sky” are computed at 10 wavelengths (0.47µm, 0.55µm, 0.67µm, 0.86µm, 1.24µm, 2.1µm, 0.3-0.7µm, 0.3-5.0µm, and 0.7-5.0µm).

Which one is the most appropriate to use?

The only info that i found for this is

i.albedo calculates the Albedo, that is the Shortwave surface reflectance in the range of 0.3-3 micro-meters. It takes input of individual bands of surface reflectance from Modis, AVHRR, Landsat or Aster and calculates the Albedo for those. This is an precursor to r.sun and any Energy-Balance processing.

so the 0.3-5.0µm should be the more suitable for this purpose. Correct?

My final aim is to use ancillary layers to “fill” all the different parameters of r.sun.

All the examples that i found use constant or default values.

May anyone point to me some source of information?

Thanks in Advance

Giuseppe Amatulli, Ph.D.

Center for Earth Observation
ESC Room 119A
Yale University
P.O. Box 208109
New Haven, CT, 06520-8109

Teaching: spatial-ecology.net
Work: http://sbsc.yale.edu/training-and-support