DCTIMESTEP

NAME
SYNOPSIS
DESCRIPTION
EXAMPLES
AUTHOR
SEE ALSO

NAME

dctimestep - compute annual simulation time-step via matrix multiplication

SYNOPSIS

dctimestep DCspec [ skyvec ]
dctimestep Vspec Tbsdf.xml Dmat.dat
[ skyvec ]

DESCRIPTION

Dctimestep has two invocation forms. In the first form, dctimestep is given a daylight coefficient specification and an optional sky vector, which may be read from the standard input if unspecified. The daylight coefficients are multiplied against this vector and the results are written to the standard output. This may be a list of color values or a combined Radiance image, as explained below.

In the second form, dctimestep takes four input files, forming a matrix expression. The first argument is the View matrix file that specifies how window output directions are related to some set of measured values, such as an array of illuminance points or images. This matrix is usually computed by rtcontrib(1) for a particular set of windows or skylight openings. The second argument is the window transmission matrix, or BSDF, given as a standard XML description. The third argument is the Daylight matrix file that defines how sky patches relate to input directions on the same opening. This is usually computed using genklemsamp(1) with rtcontrib in a separate run for each window or skylight orientation. The final input is the sky contribution vector, usually computed by genskyvec(1), which may be passed on the standard input. This data must be in ASCII format, whereas the View and Daylight matrices are more efficiently represented as binary float data if machine byte-order is not an issue.

Sent to the standard output of dctimestep is either an ASCII color vector with as many RGB triplets as there are rows in the View matrix, or a combined Radiance picture. Which output is produced depends on the first argument. A regular file name will be loaded and interpreted as a matrix to generate a color results vector. A file specification containing a ’%d’ format string will be interpreted as a list of Radiance component pictures, which will be summed according to the computed vector.

EXAMPLES

To compute workplane illuminances at 3:30pm on Feb 10th:

gensky 2 10 15:30 | genskyvec | dctimestep workplaneDC.dmx > Ill_02-10-1530.dat

To compute an image at 10am on the equinox from a set of component images:

gensky 3 21 10 | genskyvec | dctimestep viewc%03d.hdr > view_03-21-10.hdr

To compute a set of illuminance contributions for Window 1 on the Winter solstice at 2pm:

gensky 12 21 14 | genskyvec | dctimestep IllPts.vmx Blinds20.xml Window1.dmx > Ill_12-21-14.dat

To compute Window2’s contribution to an interior view at 12 noon on the Summer solstice:

gensky 6 21 12 | genskyvec | dctimestep view%03d.hdr Blinds30.xml Window2.dmx > view_6-21-12.hdr

AUTHOR

Greg Ward

SEE ALSO

genklemsamp(1), genskyvec(1), mkillum(1), rtcontrib(1), rtrace(1), vwrays(1)