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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。 CM"s9E8y 'h k @>" 成像示意图 ;=#qHo9k1% 首先我们建立十字元件命名为Target v3Eo@,- I'P!,Y/> 创建方法: |NXFla m8p4U-*j 面1 : >|(WS.n 3C 面型:plane )|Jr|8 材料:Air 95VqaR, 孔径:X=1.5, Y=6,Z=0.075,形状选择Box 2AmR(vVa" RBPYGu'6B u"eZa!# 辅助数据: xR _DY'z 首先在第一行输入temperature :300K, E|\3f(aF emissivity:0.1; JW2W>6Dgv[ :K?iNZqWN6 H_v/}DEG 面2 : omr:C8T> 面型:plane jjNxatAN 材料:Air :LG}yq^ 孔径:X=1.5, Y=6,Z=0.075,形状选择Box *%;6P5n% |I4D(#w. /\Jc:v#Q 位置坐标:绕Z轴旋转90度, YstXNN4 UX03"gX
4D0(Fl 辅助数据: iFY]0@yt MI?]8+l 首先在第一行输入temperature :300K,emissivity: 0.1; 9[B<rz Ti /;|lP@ k:@a[qnY Target 元件距离坐标原点-161mm; V>DXV-%&C PsacXZNs\N "bLP3 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 lrM.RM96 bwv/{3G,Ys hn*}5!^ 探测器参数设定: 3ZLr"O1l ) d91I 在菜单栏中选择Create/Element Primitive /plane /2=_B4E2 qFB9,cUqh aU,0gvI(} }mkA Hmu4 Nu>sp,|A $@XPL~4 元件半径为20mm*20,mm,距离坐标原点200mm。 y=y/d>=w 7]R6 光源创建: :5q^\xmmq ;))[P_$zB 光源类型选择为任意平面,光源半角设定为15度。 wR`w@5,d AycA:< ~7F EY0 / 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。 5M/%%Ox '` BjRg57] 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。 e)fJd*P {m1t~ S /1s 9;'I 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。 $_%2D3-;D eP-R""uPw 创建分析面: |:J*>"sq *RUd!]bh Fj4l %= 到这里元件参数设定完成,现在我们设定元件的光学属性,在前面我们分别对第一和第二面设定的温度和发射系数,散射属性我们设定为黑朗伯,4%的散射。并分别赋予到面一和面二。 ][T9IAn uaZ"x&oZ# y&KoL\ 到此,所有的光学结构和属性设定完成,通过光线追迹我们可以查看光线是否可以穿过元件。 k}+MvGq KBUAdpU8 FRED在探测器上穿过多个像素点迭代来创建热图 giA~+m~fN Rz])wBv e FRED具有一个内置的可编译的Basic脚本语言。从Visual Basic脚本语言里,几乎所有用户图形界面(GUI)命令是可用这里的。FRED同样具有自动的客户端和服务器能力,它可以被调用和并调用其他可启动程序,如Excel。因此可以在探测器像素点上定义多个离轴光源,及在FRED Basic脚本语言里的For Next loops语句沿着探测器像素点向上和向下扫描来反向追迹光线,这样可以使用三维图表查看器(Tools/Open plot files in 3D chart)调用和查看数据。 g(z#h$@S 将如下的代码放置在树形文件夹 Embedded Scripts, Cz$Hk;3\6 [5}cU{M ~0Q\Lp); 打开后清空里面的内容,此脚本为通用脚本适用于一切可热成像的应用。 Xm0&U?dZB NUxAv= xl 绿色字体为说明文字, Y_aP:+ iPtm@f,bI '#Language "WWB-COM" !Ed<xG/ 'script for calculating thermal image map iYmzk?U 'edited rnp 4 november 2005 {U+9,6.` ?()E5 4y 'declarations "=v J} Dim op As T_OPERATION :*w:eKk Dim trm As T_TRIMVOLUME (pRy1DH~ Dim irrad(32,32) As Double 'make consistent with sampling 7kWZMi Dim temp As Double Cx1Sh#9 Dim emiss As Double M7cI$=G Dim fname As String, fullfilepath As String ?L~=Z\H x"h)"Y[c5 'Option Explicit *6\`A!C (0+ GLI8 Sub Main {) '"
k6w 'USER INPUTS 5G42vTDzS4 nx = 31 G+\~rl ny = 31 '8kL1 numRays = 1000 Br.$L minWave = 7 'microns 'piF_5(@ maxWave = 11 'microns 2=UTH%1D sigma = 5.67e-14 'watts/mm^2/deg k^4 ;MdK3c fname = "teapotimage.dat" zxynEdO %(wsGNd Print "" w!GU~0~3[ Print "THERMAL IMAGE CALCULATION" }1^tK(Am 7+2aG detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 bQ:3G; #dn%KMo2r Print "found detector array at node " & detnode kdueQ(\ lG^mW\O srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 5GWM
)vrZg F" #3s= Print "found differential detector area at node " & srcnode uvK%d\d 0 S`b;f GetTrimVolume detnode, trm 9Av- ;!] detx = trm.xSemiApe +Muia5G dety = trm.ySemiApe h}VYA\+<B area = 4 * detx * dety
M$-(4 0 Print "detector array semiaperture dimensions are " & detx & " by " & dety iJp!ROI Print "sampling is " & nx & " by " & ny JcALFKLB m#}{"d&J 'reset differential detector area dimensions to be consistent with sampling J Wyoh| pixelx = 2 * detx / nx %+OPas8C pixely = 2 * dety / ny pa> 2JF* SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False 4>ce,*B1 Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 !E.lyz fB ,!|u 'reset the source power ~>-;(YU"t SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) AZ Lt'9UD Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" fm2M i~}0 pUEok + 'zero out irradiance array ST[1'T+L For i = 0 To ny - 1 $4~}_phi For j = 0 To nx - 1 M&\ ?)yG irrad(i,j) = 0.0 j!8+|eAkk Next j s$y#Ufz Next i 2n+XML "l;8
O2;g 'main loop kp>Z /kt EnableTextPrinting( False ) oX]1>#5UMg
7~9f rW<K ypos = dety + pixely / 2 S/:QVs For i = 0 To ny - 1 2]3Jb{8FI> xpos = -detx - pixelx / 2 \iE9&3Ie ypos = ypos - pixely ~E|V{z% YaZ"&i EnableTextPrinting( True ) 9PfU'm|h Print i o 0
#]EMr EnableTextPrinting( False ) .t%Vx $U.'K!B X|B;>q For j = 0 To nx - 1 I\6<)2j/L tNf" X! xpos = xpos + pixelx : )*Ge3 ]M"'qC3g 'shift source r{jD,x2 LockOperationUpdates srcnode, True EuA<{%i GetOperation srcnode, 1, op !OVEA^6 op.val1 = xpos /g7?,/vnZ op.val2 = ypos o[ W3/ SetOperation srcnode, 1, op +\$|L+@Z LockOperationUpdates srcnode, False l%5%oN`4 ]@}BdMlHp raytrace v23Uh2[@Yy DeleteRays /%w[q:..h CreateSource srcnode R'HA>?D TraceExisting 'draw 0BD((oNg ;<R_j%* 'radiometry ga9:*G!b{) For k = 0 To GetEntityCount()-1 0lh6b3tdP If IsSurface( k ) Then >^HTghgRD temp = AuxDataGetData( k, "temperature" ) y%l#lz=6 emiss = AuxDataGetData( k, "emissivity" ) cyeDZ) If ( temp <> 0 And emiss <> 0 ) Then r:rJv ProjSolidAngleByPi = GetSurfIncidentPower( k ) ,T[
+omo frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) %Z0S"B 3 irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi <5vB{)Tq End If ]7
mSM 7f,WzvV End If qyfxT Q5 *%BI*p Next k R*C+Yk)Tkt "
CoR?[,x Next j z5'nS&x P;/wb/ Next i WN1-J(x6 EnableTextPrinting( True ) !jnIXvT1qy fG5} '8 'write out file ID+k`nP fullfilepath = CurDir() & "\" & fname IomJo Open fullfilepath For Output As #1 Q
kpmPQK Print #1, "GRID " & nx & " " & ny 8{t&8Ql n Print #1, "1e+308" 74Wg@!P Print #1, pixelx & " " & pixely [ i#Gqx>'w Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 E1g$WhXIS E NjD~ S maxRow = nx - 1 =upP3rw maxCol = ny - 1 =(\!,S' For rowNum = 0 To maxRow ' begin loop over rows (constant X) @1Lc`;Wd row = "" ^k##a-t<_> For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) ZfikNQU9r row = row & irrad(colNum,rowNum) & " " ' append column data to row string /MtacR Next colNum ' end loop over columns giJyMd}x nJg2O@mRJ Print #1, row Xy}S}9 5Vqvb| Next rowNum ' end loop over rows <2d@\"AoHE Close #1 z(eAwmuli !{;RtUPz* Print "File written: " & fullfilepath s'4p+eJ Print "All done!!" czRh.kz, End Sub o#6}?g. cf!R 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: 4*W7{MPY &nProzC SiT &p 找到Tools工具,点击Open plot files in 3D chart并找到该文件 .5xg;Qg\Y UkV] F] T7'$A!c 打开后,选择二维平面图: ^+<uHd> q(W@=-uDK
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