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greg |
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.\" RCSid $Id: gendaymtx.1,v 1.5 2013/09/05 17:53:22 greg Exp $
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greg |
1.1 |
.TH GENDAYMTX 1 01/19/13 RADIANCE
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.SH NAME
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gendaymtx - generate an annual Perez sky matrix from a weather tape
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.SH SYNOPSIS
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.B gendaymtx
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[
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.B "\-v"
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][
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1.6 |
.B "\-h"
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][
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1.1 |
.B "\-d|\-s"
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][
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1.2 |
.B "\-r deg"
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][
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1.1 |
.B "\-m N"
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][
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.B "\-g r g b"
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][
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.B "\-c r g b"
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][
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.B "-o{f|d}"
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1.4 |
][
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.B "-O{0|1}"
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1.1 |
]
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[
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.B "tape.wea"
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]
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.SH DESCRIPTION
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.I Gendaymtx
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takes a weather tape as input and produces a matrix of sky patch
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values using the Perez all-weather model.
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The weather tape is assumed to be in the simple ASCII format understood
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by DAYSIM, which contains a short header with the site parameters followed
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by the month, day, standard time, direct normal and diffuse horizontal
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irradiance values, one time step per line.
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Each time step line is used to compute a column in the output matrix,
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where rows correspond to sky patch positions, starting with 0 for
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the ground and continuing to 145 for the zenith using the default
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.I "\-m 1"
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parameter setting.
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.PP
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Increasing the
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.I \-m
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parameter, typically by factors of two, yields a higher resolution
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sky using the Reinhart patch subdivision.
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For example, setting
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.I "\-m 4"
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yields a sky with 2305 patches plus one patch for the ground.
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Each matrix entry is in fact three values, corresponding to
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red green and blue radiance channels (watts/sr/meter^2).
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Thus, an hourly weather tape for an entire year would
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yield 8760x3 (26280) values per output line (row).
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.PP
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The
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.I \-c
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option may be used to specify a color for the sky.
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The gray value should equal 1 for proper energy balance
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The default sky color is
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.I "\-c 0.960 1.004 1.118".
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Similarly, the
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.I \-g
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option may be used to specify a ground color.
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The default value is
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.I "\-g 0.2 0.2 0.2"
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corresponding to a 20% gray.
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.PP
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The
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.I \-d
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option may be used to produce a sun-only matrix, with no sky contributions.
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Alternatively, the
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.I \-s
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option may be used to exclude any direct solar component from the output.
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.PP
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1.3 |
By default,
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.I gendaymtx
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assumes the positive Y-axis points north such that the first sky patch
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is in the Y-axis direction on the horizon, the second patch is just
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west of that, and so on spiraling around to the final patch near the zenith.
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greg |
1.1 |
The
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greg |
1.2 |
.I \-r
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(or
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.I \-rz)
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option rotates the sky the specified number of degrees counter-clockwise
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1.3 |
about the zenith, i.e., west of north.
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1.2 |
This is in keeping with the effect of passing the output of
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.I gensky(1)
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or
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.I gendaylit(1)
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through
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.I xform(1)
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using a similar transform.
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.PP
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The
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1.1 |
.I \-of
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or
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.I \-od
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option may be used to specify binary float or double output, respectively.
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This is much faster to write and to read, and is therefore preferred on
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systems that support it.
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(MS Windows is not one of them.)\0
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greg |
1.4 |
The
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.I \-O1
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option specifies that output should be total solar radiance rather
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than visible radiance.
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greg |
1.6 |
The
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.I \-h
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option prevents the output of the usual header information.
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greg |
1.1 |
Finally, the
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.I \-v
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option will enable verbose reporting, which is mostly useful for
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finding out how many time steps are actually in the weather tape.
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.SH EXAMPLES
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Produce an uncolored Tregenza sky matrix without solar direct:
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.IP "" .2i
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gendaymtx -m 1 -c 1 1 1 -s Detroit.wea > Detroit.mtx
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.PP
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Produce an hourly, annual Reinhart sky matrix
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with 2306 patches including solar contributions
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and send float output to
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.I dctimestep(1)
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to compute a sensor value matrix:
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.IP "" .2i
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gendaymtx -m 4 -of VancouverBC.wea | dctimestep -if -n 8760 DCoef.mtx > res.dat
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.SH AUTHORS
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Ian Ashdown wrote most of the code,
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based on Jean-Jacques Delaunay's original gendaylit(1) implementation.
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Greg Ward wrote the final parameter parsing and weather tape conversion.
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.SH "SEE ALSO"
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greg |
1.5 |
dctimestep(1), genBSDF(1), gendaylit(1), gensky(1), genskyvec(1),
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rcollate(1), rcontrib(1), xform(1)
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