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!!++ B01 ^oYM}
!! PATHS02.INR 3bts7<K=
!! Title: Typical PATHS Output % 6 ]\^
!! Category: Isolated Command MPvWCPB
!! Keywords: PATHS, Tracing, stray, ghost RpN <=
!! Description: Typical output from the PATHS 0yT Q{'Cc
!! command for all currently defined rays. This }vD;DSz:
!! output shows the default LONG form and listing ;*QN9T= 0
!! according to total flux. !!+Da>
!! Notes: C BlXC7_Mi
!! 1) Negative 'Hits' indicate incident rays that .,mM%w,^O
!! either got absorbed by the Current object (typical) \7
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!! or did not go through or interact with current 8IJ-]wHIb
!! object (such as with STEP -1). o<J5!
!! 2) The default LONG form provides for decimal places *w 21U!
!! under Current and Previous headings. This allows rIlBH*aT
!! for further breakout of paths according to specific CB ]l[hM$
!! facets for edge-based objects. T6=-hA^A
!! 3) Negative 'Split/Scatter' numbers indicate scatter %MuaW(I o
!! rays from that object number. Otherwise, they are hVZo"XUb
!! specular split rays. They are traced back to the source (}0S1)7t
!! from left to right (up to 10 levels possible). Refer to w \DspF
!! chart under PATHS command description for decimal number ,'_( DJX
!! meanings. K;C_Z/<%
!! Edit History (latest first) G>0)I
!! 10/10/2000 - cp - modified format; added description k<O y %+C
!! 01/01/1996 - bro - creation *(nJX.7
!!-- ^j iE9k)
[ R\=M'
--- PATHS pK"&QPv
OBJECTS 8KKz5\kn7
Path Rays SumTOTA Percent Hits Current Previous Split/Scatter ... LP?P=c
1 177 3.51E+01 98.23 -7 2.000 1.000 0.00 uk6g s)qxC
2 461 2.85E-01 0.80 -9 2.000 1.000 1.10 1.10 0.00 Y Z\@)D;
3 177 6.96E-02 0.19 -17 2.000 1.000 1.10 1.10 0.00 e>!E=J) j
4 216 1.19E-01 0.33 -11 2.000 1.000 1.10 1.10 0.00 H9E(\)@
5 215 1.06E-01 0.30 -13 2.000 1.000 1.10 1.10 0.00 ` sxN!Jj?
6 94 4.15E-02 0.12 -15 2.000 1.000 1.10 1.10 0.00 V4\56 0
7 8 4.71E-03 0.01 -10 2.000 1.000 1.10 1.10 0.00 j"6:A
8 8 5.24E-03 0.01 -8 2.000 1.000 1.10 1.10 0.00 ,-:a?#f>
-------------------- HTN$ >QTI
8 1356 3.57E+01 :iEA UM
',#
177 ray flags changed !l"tI#?6W%
3397 rays now selected
