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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。 STRyW Ml p[gAZ9 成像示意图 R\
e#$"a5 首先我们建立十字元件命名为Target v1K4 $&{F u2om5e: 创建方法: w6v1 q:20 3H <`Z4;
面1 : /0!$p[cjm 面型:plane |nfH-JytV 材料:Air c0hdLl;5 孔径:X=1.5, Y=6,Z=0.075,形状选择Box i59k"pNm ]o!&2:'N` J ZNyC!u 辅助数据: 4Xr"d@2( 首先在第一行输入temperature :300K, $"(3M nR emissivity:0.1; o"f%\N0_8 EK.c+Or, '[xut1{ 面2 : h!~|6nj 面型:plane fl!1AKSn@N 材料:Air "$4hv6 s 孔径:X=1.5, Y=6,Z=0.075,形状选择Box Z%A<#% $q.p$JQ: 7TR'zW2W 位置坐标:绕Z轴旋转90度, k0=|10bi eb(m8vLR )/
n29] 辅助数据: 739l%u }< P@-R5GK 首先在第一行输入temperature :300K,emissivity: 0.1; >02i8:Tp5K [lrmuf
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zW^ Target 元件距离坐标原点-161mm; &<#/&Pq/i Ho:}Bn
g E^'C" 6 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 ` 3vN R" *%z<P~} (#CBq 探测器参数设定: cRjL3 )moo?Q 在菜单栏中选择Create/Element Primitive /plane 0 %C!`7 ~4}*Dhsh B/:>{2cm 01UqDdoj gE-lM/w \>w@=bq26 元件半径为20mm*20,mm,距离坐标原点200mm。 (4E.Li<O s=3EBh 光源创建: B6^w{eXN \E>%W 光源类型选择为任意平面,光源半角设定为15度。 q^Q|.&_k / 4Q&Xb < cob9hj#&7 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。 Z5{*? 2 fbi H 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。 ?Aj\1y4L1 O1l4gduN|i *S,v$ VX 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。 =<Zwv\U DtI%-I. 创建分析面: k4]R]=Fh. @#G6z`, w}]3jc84 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。 weTK#O0@v "E4i >g hqwz~Ky} 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。 p
P_wBX sPZV>Q:zY FRED在探测器上穿过多个像素点迭代来创建热图 =[v2 !nZI? z ; 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。 ,.1&Ff)S 将如下的代码放置在树形文件夹 Embedded Scripts, 38zR\@'j]4 6x`\
J2x Bh.6:9{ 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。 >@q2FSMf kM6
EZ`mj 绿色字体为说明文字, vQ9xG)) +c~O0U1 '#Language "WWB-COM" 1+.y,}F6b 'script for calculating thermal image map {VrAh*#h
'edited rnp 4 november 2005 Wb*T _KT]l./ 'declarations uv_P{%TK Dim op As T_OPERATION W! 5Blo Dim trm As T_TRIMVOLUME K!$\REs Dim irrad(32,32) As Double 'make consistent with sampling O(:u( U7e Dim temp As Double f%(e,KgW= Dim emiss As Double kW7&~tX Dim fname As String, fullfilepath As String x1 R! 2={K-s20 'Option Explicit v/4X[6( B 7x"ef Sub Main #o}{cXX# 'USER INPUTS Z7k1fv:S^ nx = 31 cfO^CC ny = 31 ,vHX>)M| numRays = 1000 A~%g" minWave = 7 'microns "O"^\f maxWave = 11 'microns ;Wp`th!F sigma = 5.67e-14 'watts/mm^2/deg k^4 hVQ+
J!qD fname = "teapotimage.dat" ?>< AS/\IHZ\ Print "" LRLhS<9 Print "THERMAL IMAGE CALCULATION" 7\|NYT4 tpy:o(H detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 "KQ\F0/ NnSI)*%' Print "found detector array at node " & detnode o<eWg PPIG?fK) srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 SE7 (+r V~%WKQ Print "found differential detector area at node " & srcnode #,|_d>p: XxrO:$ GetTrimVolume detnode, trm D%";!7u detx = trm.xSemiApe c]/O^/ dety = trm.ySemiApe ?X5glDZ$ area = 4 * detx * dety c# 4ZDjvm6 Print "detector array semiaperture dimensions are " & detx & " by " & dety 9zM4D Print "sampling is " & nx & " by " & ny V'BZ=.= @"#gO:|[i0 'reset differential detector area dimensions to be consistent with sampling 4OESsN$O pixelx = 2 * detx / nx .L5T4) pixely = 2 * dety / ny p<^/T,&I SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False @#O| Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 d .lu OM&\Mo 'reset the source power e]y=]}A3{ SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) ]ge^J3az$u Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" 1k70>RQ&69
Dg2#Gv0B 'zero out irradiance array AFF>r#e For i = 0 To ny - 1 }A&Xxh!Fwo For j = 0 To nx - 1 CSg5i&A= irrad(i,j) = 0.0 =dw*B Next j ,-NLUS
"w Next i 07WIa@Q $hY]EB 'main loop -*{(#k$ EnableTextPrinting( False ) CIs1*:Q9 SoON@h/ ypos = dety + pixely / 2 n<(5B|~y For i = 0 To ny - 1 LW8{a& xpos = -detx - pixelx / 2 Y_iF$m/R ypos = ypos - pixely 1:l&&/Wy ]Pl6:FB8%@ EnableTextPrinting( True ) :^.8 7>V7 Print i $S-;M0G
x EnableTextPrinting( False ) 9g,L1 W*
!z6/.>QJ~ l\l]9Z6% For j = 0 To nx - 1 $;j6*,H VDI S`E xpos = xpos + pixelx .Y Frb+6 a\j\eMC 'shift source JdNPfkOF LockOperationUpdates srcnode, True ` vmk GetOperation srcnode, 1, op ve/6-J!5Y. op.val1 = xpos -tdON op.val2 = ypos ra#)*fG,~ SetOperation srcnode, 1, op +OuG!3+w LockOperationUpdates srcnode, False lNnbd?D8 u2Z^iY raytrace */h9 "B DeleteRays ENF@6] CreateSource srcnode 9%'HB\A TraceExisting 'draw f$*9J k |aOUW 'radiometry 4!RI2?4V For k = 0 To GetEntityCount()-1 x/q$RcDOm If IsSurface( k ) Then -(,6w? temp = AuxDataGetData( k, "temperature" ) YY>Uf1}*9 emiss = AuxDataGetData( k, "emissivity" ) 42[:s: If ( temp <> 0 And emiss <> 0 ) Then @<{#v.T ProjSolidAngleByPi = GetSurfIncidentPower( k ) TVh7h`Eg frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) @V
CQ4X7T irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi /
{bK*A! End If D`@U[ `Sw SPm5tU End If hl~F1"q) YU"\Wd[ Next k |(8h:g "TNUw&ih Next j ':>*=& >~8Df61o` Next i y:Ab5/bHy EnableTextPrinting( True ) vF\zZ<R/ :iC\#i]6 'write out file Nm.>C4 fullfilepath = CurDir() & "\" & fname $7
Uk;xV Open fullfilepath For Output As #1 -L<Pm(v& Print #1, "GRID " & nx & " " & ny ]xeyXw84k Print #1, "1e+308" L2A#OZZu Print #1, pixelx & " " & pixely O
lIH0 Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 $
T_EsnN DLM9o3/*J maxRow = nx - 1 Qz$Dv@*y\ maxCol = ny - 1 < tq9 For rowNum = 0 To maxRow ' begin loop over rows (constant X) _cs9R% row = "" D6:J*F&? For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) ]>i0;RME row = row & irrad(colNum,rowNum) & " " ' append column data to row string /Day5\Q# Next colNum ' end loop over columns U2?gODh' muq|^Hfb Print #1, row NUtyUv *\vc_NP] Next rowNum ' end loop over rows ',%&DA2 Close #1 <LZvh8 *0zH5c Print "File written: " & fullfilepath e)(| Print "All done!!" D/`E!6Fk= End Sub '$^ F.2 :*nBo 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: H)+kN'J )5OU!c Z9^$jw] 找到Tools工具,点击Open plot files in 3D chart并找到该文件 [SvwJIJJ !r
<|F @S92D6 打开后,选择二维平面图: Oei2,3l,? nd1*e
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