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dctimestep - compute annual simulation time-step via matrix multiplication |
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.SH SYNOPSIS |
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.B dctimestep |
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.B DCspec |
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[ |
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.B skyvec |
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] |
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.br |
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.B dctimestep |
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.B Vspec |
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.B Tbsdf.xml |
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.B Dmat.dat |
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[ |
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.B tregvec |
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.B skyvec |
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] |
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.SH DESCRIPTION |
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.I Dctimestep |
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has two invocation forms. |
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In the first form, |
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.I dctimestep |
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is given a daylight coefficient specification and an optional sky |
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vector, which may be read from the standard input if unspecified. |
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The daylight coefficients are multiplied against this vector and the results |
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are written to the standard output. |
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This may be a list of color values or a combined Radiance image, |
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as explained below. |
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.PP |
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In the second form, |
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.I dctimestep |
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takes four input files, forming a matrix expression. |
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The first argument is the View matrix file that specifies how window output |
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directions are related to some set of measured values, such as an array of |
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as there are rows in the View matrix, or a combined |
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.I Radiance |
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picture. |
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Which output is produced depends on the |
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.I Vspec |
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argument. |
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Which output is produced depends on the first argument. |
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A regular file name will be loaded and interpreted as a matrix to |
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generate a color results vector. |
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A file specification containing a '%d' format string will be |
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component pictures, which will be summed according to the computed |
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vector. |
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.SH EXAMPLES |
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To compute workplane illuminances at 3:30pm on Feb 10th: |
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.IP "" .2i |
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gensky 2 10 15:30 | genskyvec | dctimestep workplaneDC.dmx > Ill_02-10-1530.dat |
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.PP |
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To compute an image at 10am on the equinox from a set of component images: |
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.IP "" .2i |
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gensky 3 21 10 | genskyvec | dctimestep viewc%03d.hdr > view_03-21-10.hdr |
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.PP |
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To compute a set of illuminance contributions for Window 1 on |
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the Winter solstice at 2pm: |
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.IP "" .2i |
