I am dealing with r.sun. I am really confused and need your help. I have
couple of questions. First how can I use clear sky index raster map as an
input to r.sun? Regardless of the first question, I have measured cloudiness
data. How can I use this data in r.sun? Should I create coefbh and coefdh
from that data? If it is how?
I am dealing with r.sun. I am really confused and need your help. I have
couple of questions. First how can I use clear sky index raster map as an
input to r.sun? Regardless of the first question, I have measured
cloudiness
data. How can I use this data in r.sun? Should I create coefbh and coefdh
from that data? If it is how?
--
José A. Ruiz-Arias
Solar Radiation and Atmosphere Modelling Group http://matras.ujaen.es http://www.ujaen.es/investiga/tep220
Physics Department, University of Jaén
Campus Lagunillas, Building A3 066
23071 Jaén Spain
Tlf: +34 953 212 474
Fax: +34 953 212 838
Thank you... It really helped.
But now I have this kind of problem. I got clear sky index (K) data from
NASA SSE. Should I use that data coefbh or coefdh. If it's a global data how
can I separate it? In other words how can I derive coefbh and coefdh from
NASA SSE clear sky index(K) data?
I am dealing with r.sun. I am really confused and need your help. I have
couple of questions. First how can I use clear sky index raster map as an
input to r.sun? Regardless of the first question, I have measured
cloudiness
data. How can I use this data in r.sun? Should I create coefbh and coefdh
from that data? If it is how?
--
José A. Ruiz-Arias
Solar Radiation and Atmosphere Modelling Group http://matras.ujaen.es http://www.ujaen.es/investiga/tep220
Physics Department, University of Jaén
Campus Lagunillas, Building A3 066
23071 Jaén Spain
Tlf: +34 953 212 474
Fax: +34 953 212 838