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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。 xq.,7#3 X'WbS 成像示意图 rRL:]%POT 首先我们建立十字元件命名为Target &B7X LO[ cyG3le& +G 创建方法: ,`MUd0 n TgVvp0F; 面1 : Fmk,
"qs 面型:plane 9#.nNv*z3 材料:Air PSNrY e 孔径:X=1.5, Y=6,Z=0.075,形状选择Box _bn*B$ {(AYs*5 u-At k-2M 辅助数据: Y_)!U`>N? 首先在第一行输入temperature :300K, k 0z2)3L emissivity:0.1; !,PG!Gnl O!kBp(?] Qhsh{muw( 面2 : ?x"<0k1g 面型:plane @%fNB,H` 材料:Air diGPTV-?$ 孔径:X=1.5, Y=6,Z=0.075,形状选择Box 6fQNF22E 4WZ:zr N cWP34;NNM 位置坐标:绕Z轴旋转90度, NB;8 e>8 kb]PWOz <l(LQmM; 辅助数据: lh&Q{t(+8 &%}6&PWi 首先在第一行输入temperature :300K,emissivity: 0.1; >Q#_<IcI r'uD|T H znzh$9tH Target 元件距离坐标原点-161mm; b'4{l[3~nl %%}U
-*b m@R!o 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 {A2(a7vV &aqF||v%) 7/w)^&8 探测器参数设定: 9"KEHf! r'#5ncB 在菜单栏中选择Create/Element Primitive /plane Q}2aBU.f Wqy|Y*$qT &xo,49`! !v;N@C3C nxkbI:+t K2<"O qp_W 元件半径为20mm*20,mm,距离坐标原点200mm。 1~Zmc1] }eetx68\ 光源创建: qI"Xh"
c? Q\z6/1:9Z 光源类型选择为任意平面,光源半角设定为15度。 /qa{*"2Qo Tz[ck'k EaaQC]/OX5 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{`In8G>y w5w,jD[ 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。 D]\of#%T V6P2W0m eW,{E)x: 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。 SKt&]H iqm]sC` 创建分析面: w{l}(:xPp 7v3'JG1r- >M=_:52.+ 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。 3DRJl,v `>-fU<Q1 ce@1#}* 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。 $5N %! mQdF+b1o FRED在探测器上穿过多个像素点迭代来创建热图 S-l<+O1fy ^)oBa=jL4 FRED具有一个内置的可编译的Basic脚本语言。从Visual Basic脚本语言里,几乎所有用户图形界面(GUI)命令是可用这里的。FRED同样具有自动的客户端和服务器能力,它可以被调用和并调用其他可启动程序,如Excel。因此可以在探测器像素点上定义多个离轴光源,及在FRED Basic脚本语言里的For Next loops语句沿着探测器像素点向上和向下扫描来反向追迹光线,这样可以使用三维图表查看器(Tools/Open plot files in 3D chart)调用和查看数据。 f]%:.N~1w 将如下的代码放置在树形文件夹 Embedded Scripts, 9.u}<m *:S_v.Y3" uF,F<%d 打开后清空里面的内容,此脚本为通用脚本适用于一切可热成像的应用。
|Hx#Uk# *?bOH5$@Nw 绿色字体为说明文字, Od_xH .aS`l~6 '#Language "WWB-COM" ;Z^\$v9? 'script for calculating thermal image map \PReQ|[ah 'edited rnp 4 november 2005 'D_a2xo0 prtNfwJz1j 'declarations yp}J+/PX} Dim op As T_OPERATION NULew]:5 Dim trm As T_TRIMVOLUME J5dwd,FQ Dim irrad(32,32) As Double 'make consistent with sampling >TI/W~M Dim temp As Double #gW"k;7P Dim emiss As Double XhEZTg; Dim fname As String, fullfilepath As String eX)'C>4W kU:ge 'Option Explicit tb$I8T Sc b' Sub Main u@&e{w~0 'USER INPUTS ;wGoEN nx = 31 0'wchy> ny = 31 mIW8K
): numRays = 1000 5@QJ+@j| minWave = 7 'microns (\8IgQ{ maxWave = 11 'microns gq%U5J"x;J sigma = 5.67e-14 'watts/mm^2/deg k^4 ;|qbz]t2( fname = "teapotimage.dat" -g n!8G1 74_':,u;]~ Print "" qa-%j + Print "THERMAL IMAGE CALCULATION" jk(tw-B |P_voht detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 >]{{5oOQ> \/XU v( Print "found detector array at node " & detnode ":v^Y
9 B*Z}=$1j srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 uNKf!\Y *@;bWUJ Print "found differential detector area at node " & srcnode oU l0w~Xn g)dKXsy(F GetTrimVolume detnode, trm g"{`g6(+ detx = trm.xSemiApe 8|JPQDS7 dety = trm.ySemiApe (N"9C+S} area = 4 * detx * dety xe"A;6H Print "detector array semiaperture dimensions are " & detx & " by " & dety i/{dD"HwM Print "sampling is " & nx & " by " & ny |@W|nbAfX U8S<wf& 'reset differential detector area dimensions to be consistent with sampling q}PUwN6 pixelx = 2 * detx / nx 4 :phq pixely = 2 * dety / ny :3N6Ej SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False _<Ip0?N Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 n +v(t ajCe&+ 'reset the source power /'4]"%i%3 SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) GvzaLEo Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" we0haK q#6|/R* 'zero out irradiance array b{BiC&3 For i = 0 To ny - 1 ?%cZO" For j = 0 To nx - 1 lb{X 6_. irrad(i,j) = 0.0 aH7@:=B Next j w-];!;% Next i -G[TlH06 QVF561Yz 'main loop qXprD.; } EnableTextPrinting( False ) yxtfyf|9 ' xsIfR3Ze9 ypos = dety + pixely / 2 5d;(D i5z For i = 0 To ny - 1 WN $KS"b6} xpos = -detx - pixelx / 2 Z*R~dHr ypos = ypos - pixely !a4`SjOgu _WGWU7h EnableTextPrinting( True ) !q~f;&rg Print i c8N pk< EnableTextPrinting( False ) 2Akh/pb ]n!oa \#v(f2jPF For j = 0 To nx - 1 $a|>>?8 ]k$:sX xpos = xpos + pixelx ,V9r2QY aI>F8R? 'shift source _VB;fH$ LockOperationUpdates srcnode, True |['SiO$) GetOperation srcnode, 1, op G%junS'zt
op.val1 = xpos KBoW(OP4' op.val2 = ypos D;h JK-Y SetOperation srcnode, 1, op _H@8qR LockOperationUpdates srcnode, False SBaTbY0 RA!8AS? raytrace WOeG3jMz? DeleteRays F=?GV\Tw CreateSource srcnode BI<(]`FP;s TraceExisting 'draw k$.l^H u 4}Y? :R 'radiometry RWB]uHzE For k = 0 To GetEntityCount()-1 Zbr1e5? If IsSurface( k ) Then tiy#b8 temp = AuxDataGetData( k, "temperature" ) J|@O4g emiss = AuxDataGetData( k, "emissivity" ) E<p<"UjcCJ If ( temp <> 0 And emiss <> 0 ) Then ,g 1~4,hqQ ProjSolidAngleByPi = GetSurfIncidentPower( k ) ?k=)T]-} frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) E Uq6)
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irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi _7R6%^ End If y#P_ }Kfo "AlR%:]24~ End If [U$`nnp F ~e}=Nb Next k a
*bc#!e /GO((v+J Next j -^*8D(j* p`S~UBcL. Next i Gx|/
Jq EnableTextPrinting( True ) 29W`L2L -j^G4J 'write out file w[uwhd fullfilepath = CurDir() & "\" & fname Pk8(2fAYk Open fullfilepath For Output As #1 6|Crc$4l Print #1, "GRID " & nx & " " & ny rc}=`D` Print #1, "1e+308" ()fYhk|W Print #1, pixelx & " " & pixely oMxpdG3y- Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 9? |m ^ F3nPQw{; maxRow = nx - 1 0
d2to5 ( maxCol = ny - 1 5(DnE?}vo For rowNum = 0 To maxRow ' begin loop over rows (constant X) /b{Ufo3v row = "" gT|&tTS1@ For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) j[w5#]&% row = row & irrad(colNum,rowNum) & " " ' append column data to row string ^56#{~%^? Next colNum ' end loop over columns )IuwI #pm ab5i7@Ed Print #1, row kCKCJ}N fM<g++X Next rowNum ' end loop over rows ,*wj~NE Close #1 aVn+@g<. qjR p5 Print "File written: " & fullfilepath af/;D r@ Print "All done!!" H"rIOoxf End Sub z.:IUm{z AH
]L C6- 在输出报告中,我们会看到脚本对光源的孔径和功率做了修改,并最终经过31次迭代,将所有的热成像数据以dat的格式放置于: !Mk]% =l$qwcfbo (PnrY~9 找到Tools工具,点击Open plot files in 3D chart并找到该文件 HTP~5J j2:A@a6 \fC}l
Ll 打开后,选择二维平面图: q%FXox~b g@S?5S.Av
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