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简介:本文是以十字元件为背景光源,经过一个透镜元件成像在探测器上,并显示其热成像图。 BJM_kKH >lo,0oG 成像示意图 *o/Q# 首先我们建立十字元件命名为Target )1>fQ9 *}t,:N;i 创建方法: :\+;5Se+l }NQ{S3JW 面1 : *E Z'S+wR 面型:plane .{-&3++WZ 材料:Air l%aiG+z%6} 孔径:X=1.5, Y=6,Z=0.075,形状选择Box ^_5Nh^ .@Z-<P" a!1\,. 辅助数据: (W7cQ> 首先在第一行输入temperature :300K, (W<n<sl:- emissivity:0.1; IT3xX=|b PD$gW`V 6$}hb|j 面2 : `YDe<@6' 面型:plane o;+J3\ 材料:Air k+au42:r 孔径:X=1.5, Y=6,Z=0.075,形状选择Box 6#/Riu% Ip/_uDi+!Z a'LM6A8~x 位置坐标:绕Z轴旋转90度, ,FvBZ.4c3= YQzs0t , 0L
"+, 辅助数据: z@lUaMm:F &></l| hY 首先在第一行输入temperature :300K,emissivity: 0.1; 1D42+cy /7$3RV( FbMX?T"yH Target 元件距离坐标原点-161mm; GW_@hYIqD HWFI6N L{K:XiPn 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 OY'490 IK%fX/tDyc :%M[|Fj 探测器参数设定: J?\z{ ;qa D8otUDB{ 在菜单栏中选择Create/Element Primitive /plane l@ +]XyLj DwXzmp[qWH w<?v78sT #]ZOi`; gDP\u<2! S!0ocS!t 元件半径为20mm*20,mm,距离坐标原点200mm。 wl1JKiodg k<xiP@b{y 光源创建: Mf0XQ3n`H fqaysy 光源类型选择为任意平面,光源半角设定为15度。 y*,3P0*z %m:T?![XO sK~d{)+T 我们将光源设定在探测器位置上,具体的原理解释请见本章第二部分。 b?#k fL9R{=I% 我们在位置选项又设定一行的目的是通过脚本自动控制光源在探测器平面不同划分区域内不同位置处追迹光线。 _ri1RK, XG
fLi $`:/OA<. 功率数值设定为:P=sin2(theta) theta为光源半角15度。我们为什么要这么设定,在第二部分会给出详细的公式推导。 mOj6
4}_`" 8U8l
5r 创建分析面: VXforI }(AgXvRq +kF$I7LN 到这里元件参数设定完成,现在我们设定元件的光学属性,在前面我们分别对第一和第二面设定的温度和发射系数,散射属性我们设定为黑朗伯,4%的散射。并分别赋予到面一和面二。 bP%0T++vo #4. S2m4 zmf`}j[ 到此,所有的光学结构和属性设定完成,通过光线追迹我们可以查看光线是否可以穿过元件。 wv>uT{g# krkRP%jy FRED在探测器上穿过多个像素点迭代来创建热图 3%Jg' Tr+ 5b9v`6Kq FRED具有一个内置的可编译的Basic脚本语言。从Visual Basic脚本语言里,几乎所有用户图形界面(GUI)命令是可用这里的。FRED同样具有自动的客户端和服务器能力,它可以被调用和并调用其他可启动程序,如Excel。因此可以在探测器像素点上定义多个离轴光源,及在FRED Basic脚本语言里的For Next loops语句沿着探测器像素点向上和向下扫描来反向追迹光线,这样可以使用三维图表查看器(Tools/Open plot files in 3D chart)调用和查看数据。 i]{M G'tg 将如下的代码放置在树形文件夹 Embedded Scripts, jHPJk8@y
V\8vJ3.YV ,bRvj8"M 打开后清空里面的内容,此脚本为通用脚本适用于一切可热成像的应用。 7dl]f#uZU @`<v d@ 绿色字体为说明文字, e-;$Iv 8fzmCRFH '#Language "WWB-COM" j[!'l,I 'script for calculating thermal image map ,5" vzGLJ 'edited rnp 4 november 2005 #87:Or1 OHeVm-VC 'declarations K9co_n_L Dim op As T_OPERATION M9{?gM9 Dim trm As T_TRIMVOLUME [xT2c.2__J Dim irrad(32,32) As Double 'make consistent with sampling ($^XF: #5 Dim temp As Double ;\=W=wL( Dim emiss As Double a%>p"4WL Dim fname As String, fullfilepath As String o0Qy?14T- Pb$ep|`u 'Option Explicit -R
4t EJ P##eGx Sub Main 1bb~u/jU 'USER INPUTS }PGl8F ! nx = 31 L 0kK' n? ny = 31 6y&d\_?Y numRays = 1000 0}]k>ndT minWave = 7 'microns gCAWRNp maxWave = 11 'microns ]Lq9Ompf(t sigma = 5.67e-14 'watts/mm^2/deg k^4
V2kNJwwk fname = "teapotimage.dat" _|.q?;C]$ (v*$ExF Print "" c #+JG Print "THERMAL IMAGE CALCULATION" E!J;bX5 O.S(H1z<G detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 IbAGnl { v|~ yIywf Print "found detector array at node " & detnode T'2(sHk X_XeI!,b srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 v/6QE;BY&Q /)?]vKMiI Print "found differential detector area at node " & srcnode TfK$tTkM {'8a'9\ GetTrimVolume detnode, trm a?%X9 +1A detx = trm.xSemiApe A<.`HCv2 dety = trm.ySemiApe jvn:W{'Q area = 4 * detx * dety }~$zdgMT Print "detector array semiaperture dimensions are " & detx & " by " & dety <N^2|*3 Print "sampling is " & nx & " by " & ny w~sr2;rp< lTsl= 'reset differential detector area dimensions to be consistent with sampling `V[{(&?,n pixelx = 2 * detx / nx niY9`8 pixely = 2 * dety / ny ;cIs$ SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False rz0~W6 U Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 rwr>43S5<3 'VCF{0{H~ 'reset the source power XPE{]4 g SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) '~A~gK0 Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" ,dK<2XP \M1- 'zero out irradiance array D]resk For i = 0 To ny - 1 qazM@ For j = 0 To nx - 1 1QXv}36#3n irrad(i,j) = 0.0 Yd:8iJA Next j u$d
T^c Next i I?@9;0R =xFw4D9 'main loop "
cx\P,< EnableTextPrinting( False ) CGvU{n," MHJH@$|] ypos = dety + pixely / 2 lw0l86^Y For i = 0 To ny - 1 *?%DdVrO@ xpos = -detx - pixelx / 2 LDHuf<` ypos = ypos - pixely wN8-Me 2ku\R7 EnableTextPrinting( True ) -L(F:
Print i ZFh2v]|! EnableTextPrinting( False ) dX-Xzg }7E2,A9_" 9/TF# For j = 0 To nx - 1 <7cm[ Ds c{- <v xpos = xpos + pixelx 8W
Mhe=[ |]sh*<:?, 'shift source b&X- &F LockOperationUpdates srcnode, True RSXYz8{ GetOperation srcnode, 1, op jHq.W95+P op.val1 = xpos
ju`x op.val2 = ypos _oxhS!.* SetOperation srcnode, 1, op iE>E*!aBg LockOperationUpdates srcnode, False V9qA.NV2 k2o98bK&; raytrace <eKF DeleteRays 8.bIP
ju%v CreateSource srcnode &=y)C/u TraceExisting 'draw 8V@ /h6-e, :hB/|H*= 'radiometry <5
G+(vP For k = 0 To GetEntityCount()-1 )J#7:s]eo If IsSurface( k ) Then :786Z,') temp = AuxDataGetData( k, "temperature" ) Kf#9-.}? emiss = AuxDataGetData( k, "emissivity" ) +m kub}<a If ( temp <> 0 And emiss <> 0 ) Then +]P??`,R; ProjSolidAngleByPi = GetSurfIncidentPower( k ) Z}6 frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) CEjMHP$= irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi OI</o0Ca End If C;#vW FE [=imF^=3Vb End If qB
PUB( ,,vl+Z<& Next k f]N2(eM
o_hk!s^4m Next j -@f5d d[ (KgX9 Next i 9`eu&n@Z EnableTextPrinting( True ) v1wMXOR 57*`y'CW 'write out file 'B0=
"7 fullfilepath = CurDir() & "\" & fname Lq.aM.&;# Open fullfilepath For Output As #1 %7WGodlXW Print #1, "GRID " & nx & " " & ny M:i;;)cq Print #1, "1e+308" udYk
6 Print #1, pixelx & " " & pixely |9cJO@ Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 ]pC/6' X;/~d>@ maxRow = nx - 1 dHjJLs_ maxCol = ny - 1 7kJ =C For rowNum = 0 To maxRow ' begin loop over rows (constant X) J+tpBPmb row = "" Ao>] ~r0 For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) :s|" ZR row = row & irrad(colNum,rowNum) & " " ' append column data to row string qBL>C\V + Next colNum ' end loop over columns 2Ur9*#~kGp _s{on/u Print #1, row J_) .Hd H]2cw{2 Next rowNum ' end loop over rows 5{?J5 Close #1 ;G !JKg O3H dPQ Print "File written: " & fullfilepath YmXh_bk Print "All done!!" HX\^ecZ#E End Sub @}sxA9a ^]_[dqd 在输出报告中,我们会看到脚本对光源的孔径和功率做了修改,并最终经过31次迭代,将所有的热成像数据以dat的格式放置于: e%_2n=p~)% wJ
0KI[p(S #qqIOjS^w 找到Tools工具,点击Open plot files in 3D chart并找到该文件 z2:^Qg >p"ytRu^ Kxs_R#k 打开后,选择二维平面图: K]5@bm 'a8{YT4
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