ptimization of any kind. If I were to add a space voxelization algorithm to it I could probably do away with 90% of the force vectors in a large particle cloud.
http://www.youtube.com/watch?v=RmsbzTf79bc
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David Rutten
david@mcneel.com
Poprad, Slovakia…
Added by David Rutten at 5:35am on December 16, 2009
ide into 80 branches, and 80 outputs of explode and 80 dispatches - its my nightmare. Is there any way to do this with parametric Number of brunches? …
rom two surface offsets. I did a merge list to create a pattern from an wavy surface. I obtained several surfaces made of two toggle boolean.
Capture%20d%E2%80%99e%CC%81cran%202016-05-18%20a%CC%80%2016.26.16.png
How can i simplify those surfaces (made of two surfaces)?
Capture%20d%E2%80%99e%CC%81cran%202016-05-18%20a%CC%80%2016.26.38.png
Also, how can i link the two offset surfaces in a closed volume?
Thank you guys!
Best,
Rémy…
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.…