ole refresh part so that it will try one combination at a time. I dont have a full understanding of how to do this given that everything in GH is runtime.
Outputs: A,B,C,D
A0: Cat
B0: Cat
C0: Cat
D0: Cat
A1: Cat
A2: Cat
A3: Cat
A4: Dog
etc, per refresh.....…
,2,n)
c (0,1,2,n)
And i Would like to have:
d (0(a0+b0+c0),1(a1+b1+c1),n(an+bn+cn) , d being a list of polylines ( triangles in this particular case because an, bn and cn are three sides of a same triangle.)
Thank you…
0.533000void brightfunc skyfunc2 skybright perezlum.cal010 1.382e+00 3.201e-01 1.066879 -0.754821 0.015485 -0.048998 -0.089403 0.066341 -0.860010 0.505947
The values in bold are then evaluated using the equations in the file perezlum.cal inside the RAYPATH directory in Radiance..
{ All-weather Angular Sky Luminance Distribution . Additional arguments required for calculation of skybright: A1 - diffus normalization A2 - ground brightness A3,A4,A5,A6,A7 - coefficients for the Perez model A8,A9,A10 - sun direction}skybright = wmean((Dz+1.01)^10, intersky, (Dz+1.01)^-10, A2 );wmean(a, x, b, y) = (a*x+b*y)/(a+b);intersky = if( (Dz-0.01), A1 * (1 + A3*Exp(A4/Dz) ) * ( 1 + A5*Exp(A6*gamma) + A7*cos(gamma)*cos(gamma) ), A1 * (1 + A3*Exp(A4/0.01) ) * ( 1 + A5*Exp(A6*gamma) + A7*cos(gamma)*cos(gamma) ) );
This data is then mapped to the "glow" material that represents the celestial hemisphere...You can edit the climate based sky produced by Honeybee and enter your own values. The other option would be to just use gendaylit from DOS Prompt.…
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