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Comparing ray/doc/man/man1/rfluxmtx.1 (file contents):
Revision 1.9 by greg, Wed Sep 23 22:36:28 2015 UTC vs.
Revision 1.15 by greg, Thu Mar 27 01:26:55 2025 UTC

# Line 111 | Line 111 | If it is not given,
111   defaults to 1, which is just the Tregenza sky.
112   (Use "h=-rN" for left-handed coordinates.)
113   .TP
114 + .BI h =cie
115 + Divide the hemisphere into CIE sky scanner directions, which is
116 + similar to Tregenza but with different starting azimuths and
117 + reversing row direction at each new altitude.
118 + (Use "h=-cie" for left-handed coordinates.)
119 + .TP
120   .BI h =scN
121   Subdivide the hemisphere using the Shirley-Chiu square-to-disk mapping with an
122   .I NxN
# Line 121 | Line 127 | grid over the square.
127   Orient the "up" direction for the hemisphere using the indicated axis or direction
128   vector.
129   .TP
130 < .BI o =output.mtx
131 < Send the matrix data for this receiver to the indicated output file.
130 > .BI o =output_spec
131 > Send the matrix data for this receiver to the indicated file or command.
132 > Single or double quotes may be used to contain strings with spaces, and
133 > commands must begin with an exclamation mark ('!').
134   The file format will be determined by the command-line
135   .I \-fio
136   option and will include an information header unless the
# Line 169 | Line 177 | rfluxmtx int_aperture.rad ext_aperture.rad lpipe.rad >
177   .SH AUTHOR
178   Greg Ward
179   .SH "SEE ALSO"
180 < genBSDF(1), getinfo(1), rcalc(1), rcollate(1), rcontrib(1), rmtxop(1),
181 < vwrays(1), wrapBSDF(1)
180 > genBSDF(1), getinfo(1), pvsum(1), rcalc(1), rcollate(1), rcomb(1), rcontrib(1),
181 > rcrop(1), rmtxop(1), vwrays(1), wrapBSDF(1)

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