rface(test_brep, test_surface, 0.1, curves_list, points_list)
and I get back:
1. Error (BC30311): Value of type 'System.Collections.Generic.List(Of Rhino.Geometry.Curve)' cannot be converted to '1-dimensional array of Rhino.Geometry.Curve'. (line 97)
2. Error (BC30311): Value of type 'System.Collections.Generic.List(Of Rhino.Geometry.Point3d)' cannot be converted to '1-dimensional array of Rhino.Geometry.Point3d'. (line 97)
Could anyone tell me what I'm doing wrong?
Thanks!…
on for curves, if you make an algorithm that dynamically defines the possition of the controlpoints for NURBS curves as a function of the parameteres in F(t, a1,...,b1,...,c1,...)= x(t, a1, a2...)+y(t, b1, b2...)+ z(t, c1, c2...) or F(x, a, b ,c...)?
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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.…
tting masks but haven't found what I'm looking for, ideally I'd like to do it that way rather than plug in more bits as it's getting clunky.
Thanks in advance!
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