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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。 g{^(EZ, LhQidvCNJ 成像示意图 AN4(]_] 首先我们建立十字元件命名为Target e\WG-zi/
3y]rhB 创建方法: 0w ;#4X:m ^s6C']q *O 面1 : vlx\hJ<I 面型:plane N7}yU~j^ 材料:Air g <5G# 孔径:X=1.5, Y=6,Z=0.075,形状选择Box MVZ9x% HRW}Yl 4KZ)`KPE 辅助数据: SS"Z>talw 首先在第一行输入temperature :300K, Ufv0Xj emissivity:0.1; D}L4uz? ;7bY>zc(w n_1,-(t 面2 : &1M#;rE;D# 面型:plane Jec<1|
材料:Air A]AM|2 D 孔径:X=1.5, Y=6,Z=0.075,形状选择Box Aj "SSX!L CQ^I;[=d ~PiCA 位置坐标:绕Z轴旋转90度, '^~38=FA Xr$hQbl5D zR_yxs' 辅助数据: vC _O!2E cvO;xR 首先在第一行输入temperature :300K,emissivity: 0.1; e3x;(@j =*Y=u6? eW zyydl Target 元件距离坐标原点-161mm;
z+F:_ VO+3@d: kq=tL@W`0} 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 iYl$25k/1 eVB.g@%T _~_6qTv-d 探测器参数设定: ?%RR+(2m <]kifiN# 在菜单栏中选择Create/Element Primitive /plane }*3#*y " <nE |Y@S 7T@"2WYat AAld2"r ,Z p9,nf ffE&=eh) 元件半径为20mm*20,mm,距离坐标原点200mm。 "Go)t+- @AAkEWo)_ 光源创建: *'hvYl/?> ?ne!LDlE| 光源类型选择为任意平面,光源半角设定为15度。 et0yS%7+?@ N~@VZbS(6 'ktWKW$
D 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。 }c-tvK1g 4E.K6=k|=a 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。 B^sHFc""V
txW<r8 qvhol 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[JPr 8/* 6&#- 创建分析面: 5Pu
F]5 2gb MUdpp Pw_[{ LL 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。 Je~d/,^WU 2e @zd\ %xWscA%^u 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。 %*wOJx zO07X*Bw FRED在探测器上穿过多个像素点迭代来创建热图 IRW%*W# W9ewj:4\0 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。 niIjatT 将如下的代码放置在树形文件夹 Embedded Scripts, B[rxV :g[G&Ds8 $6]7>:8mz 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。 OY/sCx+c _Ak?i\ 绿色字体为说明文字, ET7(n0*P}] c(<,qWH '#Language "WWB-COM" $@blP<I 'script for calculating thermal image map (iZE}qf7g 'edited rnp 4 november 2005 ^v].mV/ 4SqZV 'declarations (~>L \]! Dim op As T_OPERATION ceu}Lp^%/ Dim trm As T_TRIMVOLUME &G>EBKn\2` Dim irrad(32,32) As Double 'make consistent with sampling JyX7I,0 Dim temp As Double kGZ_/"iuO Dim emiss As Double a+CHrnU\; Dim fname As String, fullfilepath As String Ur]~>-Z uUczD 8y 'Option Explicit $LF 2S\~ Sub Main 7gV"pa 'USER INPUTS NgnHo\) nx = 31 ( |1 $zF+ ny = 31 \
l+RX* numRays = 1000 _r}oYs%1 minWave = 7 'microns /WVnyz0 maxWave = 11 'microns M_2[Wypw sigma = 5.67e-14 'watts/mm^2/deg k^4 rwlV\BU fname = "teapotimage.dat" X]Emz" :fr 2K Print "" `1NxS35u Print "THERMAL IMAGE CALCULATION" OT9\K_ *My? l75 detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 OKp(A r'p;Nj. Print "found detector array at node " & detnode WRJ+l_81 *a@pZI0' srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 TIV1?S v?yH j- Print "found differential detector area at node " & srcnode .6[xX?i^T HlB'yOHv! GetTrimVolume detnode, trm $;_'5`xs detx = trm.xSemiApe ^ZFbp@#U dety = trm.ySemiApe z+1#p.F$@ area = 4 * detx * dety QY2!.a^q Print "detector array semiaperture dimensions are " & detx & " by " & dety KLXv?4! Print "sampling is " & nx & " by " & ny hltH{4 |
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FQ 'reset differential detector area dimensions to be consistent with sampling )Xa`LG=| pixelx = 2 * detx / nx !UD62yw~ pixely = 2 * dety / ny Fz16m7. SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False DFs
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$ Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 r6Z&i^cMe | zj$p~ 'reset the source power Y$EqBN SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) 0gVylQ Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" &{* [7Ad .b vB8VOrW 'zero out irradiance array T IPb ] For i = 0 To ny - 1 :>'^l?b'WX For j = 0 To nx - 1 K,' ]G&K irrad(i,j) = 0.0 b^PYA_k-Xn Next j #
3uXgZi Next i 7I`e5\ u /yIkHb^c 'main loop q:-8W[_ EnableTextPrinting( False ) sRo%=7Z ~,Q+E8 ypos = dety + pixely / 2 C$)#s{* For i = 0 To ny - 1 PBr-<J xpos = -detx - pixelx / 2 FgRlxz ypos = ypos - pixely J']1^"_' oj@B'j EnableTextPrinting( True ) hH{&k> Print i ZSYXUFz EnableTextPrinting( False ) }MrRsvN /bVU^vo S8<O$^L^ For j = 0 To nx - 1 -U"(CGb5 ?`,UW; Br6 xpos = xpos + pixelx I2%{6g@ j$zw(EkN 'shift source s9qr;}U.` LockOperationUpdates srcnode, True rayC1#f GetOperation srcnode, 1, op !3 $Ph op.val1 = xpos zXvAW7 op.val2 = ypos I9ubV cV8 SetOperation srcnode, 1, op J`uV $l: LockOperationUpdates srcnode, False ar=uDb; [1dlV/ 'raytrace F^&_O*" DeleteRays d~O\zLQ; CreateSource srcnode Z|uUE TraceExisting 'draw {?l#*XH; +Ld4e] 'radiometry ed2QGTgR For k = 0 To GetEntityCount()-1 }!(cm;XA" If IsSurface( k ) Then [$]vi`c2 temp = AuxDataGetData( k, "temperature" ) br>"96A1l emiss = AuxDataGetData( k, "emissivity" ) CG@ LYN If ( temp <> 0 And emiss <> 0 ) Then OYgD9T.8^ ProjSolidAngleByPi = GetSurfIncidentPower( k ) &voyEvX/S frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) lycY1 lK irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi zm9>"(H End If U=QV^I Qm 9EK5#_L[= End If 'F?T4 %rzC+=*; Next k W7S`+Pq <E|i3\[p Next j VW I{ wC bwqla43gX Next i bB->\ EnableTextPrinting( True ) &o=
#P2Qd ]P<u^ `{* 'write out file V?t^ J7{' fullfilepath = CurDir() & "\" & fname tVvRT*>Wb Open fullfilepath For Output As #1 1xar
L)) Print #1, "GRID " & nx & " " & ny fl!8 \4 Print #1, "1e+308" H@qA X Print #1, pixelx & " " & pixely >pbO\=j]X Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 ^0R.'XL z^T/kK3I maxRow = nx - 1 /G9wW+1 maxCol = ny - 1 /w^}(IJ4 For rowNum = 0 To maxRow ' begin loop over rows (constant X) 6x^#|;e>lI row = "" kKr7c4q For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) E;*#fD~@ row = row & irrad(colNum,rowNum) & " " ' append column data to row string `6)GjZh^ Next colNum ' end loop over columns 5(^&0c>P UIi;&[ Print #1, row C,P>7 )/1AF^ E Next rowNum ' end loop over rows Ya<S/9c Close #1 R7r` (c! 4%LG Ph Print "File written: " & fullfilepath 7;jwKA;k Print "All done!!" "9jt2@< End Sub <kN4@bd; -hiG8%l5 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: 3vfm$sx@ __fa,kK {? "-88bF~ 找到Tools工具,点击Open plot files in 3D chart并找到该文件 0/S|h"-L
V##=-KZ pwtB{6)VH{ 打开后,选择二维平面图: 7xTgG!>v 0?8O9i
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