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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。 )L_@l5l }"/>, 成像示意图 e YiqT Wn: 首先我们建立十字元件命名为Target ~{{7y]3M- (SA^>r 创建方法: c;n\HYk H}8kku>7 面1 : %P C[-(Q
面型:plane Pv*]AF;9pQ 材料:Air /7ykmW 孔径:X=1.5, Y=6,Z=0.075,形状选择Box fOP3`G^\ y3P4]sq B f.- 5 辅助数据: {CX06BP 首先在第一行输入temperature :300K, \J-D@b; emissivity:0.1; _Y)Wi[ bH%d* g?@fHFct 面2 : 74c5\UxA 面型:plane [88PCA: 材料:Air xgvwH?< 孔径:X=1.5, Y=6,Z=0.075,形状选择Box [&lH[:Y# "}S6a?]V &&zsUAkS 位置坐标:绕Z轴旋转90度, j&q%@%Gm \]3[Xw-$ E+$D$a 辅助数据: ~CHVU3 0u
+_D8G 首先在第一行输入temperature :300K,emissivity: 0.1; m@",Zr`f= {9cjitl lx> ."rW Target 元件距离坐标原点-161mm; 8KsPAK_ a/[)A _- $KS!vS7 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 fGWXUJ a&7uRR26 nW
oh(a 探测器参数设定: }q,d JE StiWa<"c 在菜单栏中选择Create/Element Primitive /plane eAjsMED !%N@>[ hV
fANbs mrig5{ dq0!.gBT2 $KP;9 元件半径为20mm*20,mm,距离坐标原点200mm。 )^
P Wr^ HumL(S'm 光源创建: d)d0,fi?- h-DHIk3/ 光源类型选择为任意平面,光源半角设定为15度。 ,E"n 7*6mr *JZlG%z 3^-\=taN<m 我们将光源设定在探测器位置上,具体的原理解释请见本章第二部分。 ClNuO o4agaA3k 我们在位置选项又设定一行的目的是通过脚本自动控制光源在探测器平面不同划分区域内不同位置处追迹光线。 I__a}|T% &q#.
> MSB/O. 功率数值设定为:P=sin2(theta) theta为光源半角15度。我们为什么要这么设定,在第二部分会给出详细的公式推导。 m ^w{:\p ,;f5OUl?[ 创建分析面: ,wngS= AHHV\r #5iy^?N"w 到这里元件参数设定完成,现在我们设定元件的光学属性,在前面我们分别对第一和第二面设定的温度和发射系数,散射属性我们设定为黑朗伯,4%的散射。并分别赋予到面一和面二。 Kq(JHB+ B&<P >AZ DcE4r>8B 到此,所有的光学结构和属性设定完成,通过光线追迹我们可以查看光线是否可以穿过元件。 !'B=']. R@U4Ae{+ FRED在探测器上穿过多个像素点迭代来创建热图 |/n IR8yE`(h FRED具有一个内置的可编译的Basic脚本语言。从Visual Basic脚本语言里,几乎所有用户图形界面(GUI)命令是可用这里的。FRED同样具有自动的客户端和服务器能力,它可以被调用和并调用其他可启动程序,如Excel。因此可以在探测器像素点上定义多个离轴光源,及在FRED Basic脚本语言里的For Next loops语句沿着探测器像素点向上和向下扫描来反向追迹光线,这样可以使用三维图表查看器(Tools/Open plot files in 3D chart)调用和查看数据。 45OAJ?N 将如下的代码放置在树形文件夹 Embedded Scripts, ? 51i0~O= 6h0}ZM R`B} T<* 打开后清空里面的内容,此脚本为通用脚本适用于一切可热成像的应用。 <kWkc|zBY 8s
%YudW 绿色字体为说明文字, vin3
i&k 0%)T]SDS '#Language "WWB-COM" e0j4t-lL 'script for calculating thermal image map dnh~An 9 'edited rnp 4 november 2005 9SJSUv:@ }_('3C,Ba 'declarations {qOqtkj Dim op As T_OPERATION }(,{^".[} Dim trm As T_TRIMVOLUME Z*-a=u%gl' Dim irrad(32,32) As Double 'make consistent with sampling 9'@G7*Yn Dim temp As Double u4bVp+ Dim emiss As Double z;_vl Dim fname As String, fullfilepath As String S#<y_w% J~50#vHY 'Option Explicit t0Jqr)9}6 >8b%*f8R Sub Main mI]gDL1 'USER INPUTS 'sE["eC nx = 31 mkrVeBp ny = 31 lD-2 5~YV numRays = 1000 .Lu3LVS minWave = 7 'microns N
Hn#c3o maxWave = 11 'microns {s@ 0<! sigma = 5.67e-14 'watts/mm^2/deg k^4 SpYmgL?wJ fname = "teapotimage.dat" lxr;AJ( cBv"d ~ Print "" 2e03m62* Print "THERMAL IMAGE CALCULATION" B2|0.G|[j ).A9>^6?{ detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 M|zTs\1I L&~' SC Print "found detector array at node " & detnode D@:'*Z( o\; hF3 srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 29m$S7[
g/i%XTX> Print "found differential detector area at node " & srcnode f1;@a>X
"_&c[VptWi GetTrimVolume detnode, trm @#$(Cs*{] detx = trm.xSemiApe e8#83|h dety = trm.ySemiApe M{)&SNI*C area = 4 * detx * dety s|`wi}"x Print "detector array semiaperture dimensions are " & detx & " by " & dety 7upWM~H^ Print "sampling is " & nx & " by " & ny W/}_ y8q +\)Y,@cw 'reset differential detector area dimensions to be consistent with sampling gNc;P[ pixelx = 2 * detx / nx Nh}u]<B pixely = 2 * dety / ny #dD0vYT&od SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False $G5:/,Q Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 1[$zdv{A Px9 K 'reset the source power #TC}paIpj SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) ST0TWE' Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" Pai8r%Zfu i]L=M
5^C 'zero out irradiance array ]!~?j3-k Q For i = 0 To ny - 1 >/lB%<$/ For j = 0 To nx - 1 ]f&f_"D irrad(i,j) = 0.0 4>a(!ht Next j }`%ks Next i C'R6mz% Q? 1uCF9P
ai 'main loop 3HW&\:q5'M EnableTextPrinting( False ) D.|r
[c #NYHwO<0- ypos = dety + pixely / 2 }L&LtW{X For i = 0 To ny - 1 }/,Rp/+7] xpos = -detx - pixelx / 2 *Ms"{+C ypos = ypos - pixely g_N^Y Li"+` EnableTextPrinting( True ) P=6d<no&< Print i :K"~PrHm EnableTextPrinting( False ) c))?9H
,e) mfS}+_ C &[_@f# For j = 0 To nx - 1 OP" _I!t W$()W) xpos = xpos + pixelx ?6{g7S% ?6hd(^ 'shift source YD;d*E%t LockOperationUpdates srcnode, True 0a^bAEP GetOperation srcnode, 1, op u@`a~ op.val1 = xpos h]+;"v6 / op.val2 = ypos &5${k' SetOperation srcnode, 1, op hayJgkZ' LockOperationUpdates srcnode, False VB#&`]rdo 4Orq;8!BW raytrace \AH5zdK DeleteRays peT91b CreateSource srcnode #D|%r-:" TraceExisting 'draw o3GkTn O 19c_=$mV 'radiometry _aF8Us For k = 0 To GetEntityCount()-1 ir>h3Zk If IsSurface( k ) Then UcOP 0_/ temp = AuxDataGetData( k, "temperature" ) ~cfXEjE6 emiss = AuxDataGetData( k, "emissivity" ) l>`66~+s,` If ( temp <> 0 And emiss <> 0 ) Then $u'"C|>8 ProjSolidAngleByPi = GetSurfIncidentPower( k ) jZPGUoRLg frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) jC>#`gD irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi a0gg<Ml End If ~:o$}`mW D}lqd Ja End If D4|Ajeo;1 I`rN+c: Next k (dD7"zQ PnInsf%; Next j Mj6,VD9L -]Su+/3(, Next i JGTsVa2 EnableTextPrinting( True ) {wj%WSQj/y }2"W0ZdWD 'write out file SZ9DT fullfilepath = CurDir() & "\" & fname _ahp7-O Open fullfilepath For Output As #1 AWx@Z7\z"g Print #1, "GRID " & nx & " " & ny W02z}"# Print #1, "1e+308" /j}Tv.'d Print #1, pixelx & " " & pixely K sE$^` Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 v;9(FLtL ;-@: }/ maxRow = nx - 1 o:W*#dt maxCol = ny - 1 L6Brs"9B For rowNum = 0 To maxRow ' begin loop over rows (constant X) G'#u!<(^h row = "" !/u For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) W&R67ff| row = row & irrad(colNum,rowNum) & " " ' append column data to row string Ky,upU Next colNum ' end loop over columns AG9DJ{T 5[jS(1a`c Print #1, row buN@O7\ 0m4M@94 Next rowNum ' end loop over rows { +w.Z,D" Close #1 4:NMZ `~ l5Ko9CG Print "File written: " & fullfilepath 9?hZf$z Print "All done!!" H1B%}G*Ir- End Sub 7x>^ip"7 3~Fag1Hp 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: 5$'[R;r b~:)d>s8wY qve'Gm) 找到Tools工具,点击Open plot files in 3D chart并找到该文件 .24z+|j ;hO6 p
BlU&=;#r5> 打开后,选择二维平面图: !E?+1WDS0 ."^\1N(.n
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