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author | Joe Hunkeler <jhunkeler@gmail.com> | 2015-08-11 16:51:37 -0400 |
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committer | Joe Hunkeler <jhunkeler@gmail.com> | 2015-08-11 16:51:37 -0400 |
commit | 40e5a5811c6ffce9b0974e93cdd927cbcf60c157 (patch) | |
tree | 4464880c571602d54f6ae114729bf62a89518057 /sys/plio/plucircle.x | |
download | iraf-osx-40e5a5811c6ffce9b0974e93cdd927cbcf60c157.tar.gz |
Repatch (from linux) of OSX IRAF
Diffstat (limited to 'sys/plio/plucircle.x')
-rw-r--r-- | sys/plio/plucircle.x | 54 |
1 files changed, 54 insertions, 0 deletions
diff --git a/sys/plio/plucircle.x b/sys/plio/plucircle.x new file mode 100644 index 00000000..5a23d20a --- /dev/null +++ b/sys/plio/plucircle.x @@ -0,0 +1,54 @@ +# Copyright(c) 1986 Association of Universities for Research in Astronomy Inc. + +include <plset.h> +include <plio.h> +include "plcircle.h" + + +# PL_UCIRCLE -- Regionrop ufcn for a circle (circular region), clipped at +# the borders of the mask. + +bool procedure pl_ucircle (ufd, y, rl_reg, xs, npix) + +pointer ufd #I user function descriptor +int y #I mask line number +int rl_reg[3,ARB] #O output range list for line Y +int xs #O first pixel to be edited +int npix #O number of pixels affected + +pointer pl +real radius, dx, dy +int rn, axlen, x1, x1_clipped, x2, x2_clipped + +begin + pl = C_PL(ufd) + rn = RL_FIRST + axlen = PL_AXLEN(pl,1) + radius = C_RADIUS(ufd) + + dy = abs (C_YCEN(ufd) - y) + if (dy <= radius) { + dx = sqrt (radius**2 - dy**2) + x1 = C_XCEN(ufd) - int(dx) + x2 = C_XCEN(ufd) + int(dx) + x1_clipped = max(1, min(axlen, x1)) + x2_clipped = max(1, min(axlen, x2)) + + xs = x1_clipped + npix = x2_clipped - x1_clipped + 1 + + RL_X(rl_reg,rn) = 1 + RL_N(rl_reg,rn) = npix + RL_V(rl_reg,rn) = C_PV(ufd) + rn = rn + 1 + + } else { + npix = 0 + xs = 1 + } + + RL_LEN(rl_reg) = rn - 1 + RL_AXLEN(rl_reg) = npix + + return (true) +end |