| infotek |
2023-04-06 08:38 |
十字元件热成像分析
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。 q) _r3 9s
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成像示意图 v>I<| 首先我们建立十字元件命名为Target GVObz?Z]SB 8t``NZ[ 创建方法: \!PV*%P @&:VKpu\ 面1 : zz3 r<?#5 面型:plane TzY!D*%z 材料:Air u9}!Gq 孔径:X=1.5, Y=6,Z=0.075,形状选择Box
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`@\^m_!} 辅助数据: 2?1}ZXr 首先在第一行输入temperature :300K, '^1o/C emissivity:0.1; OX)BP.h# ((9YG 51/sTx<Z} 面2 : J{H?xc
o 面型:plane *. dKR 材料:Air i@{*O@m 孔径:X=1.5, Y=6,Z=0.075,形状选择Box 8_awMVAy YAMfP8S 2lJZw@ 位置坐标:绕Z轴旋转90度, &fHc"-U} FG _,
=BW9/fG 辅助数据: 7<4xtK`+b M\jB)@) 首先在第一行输入temperature :300K,emissivity: 0.1; $P_x v LH.%\TMN$ pg5&= Target 元件距离坐标原点-161mm; JP_kQ KE#$+,?
a'^0.1 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 g`.{K"N>! m|`VJ0 U_}hfLILi 探测器参数设定: "_oLe;?$c 5])8qb/F 在菜单栏中选择Create/Element Primitive /plane vhNohCt r?]%d!
U>1b9G"_ 6*V8k%H ( w5f(4 -Fa98nV.WB 元件半径为20mm*20,mm,距离坐标原点200mm。 5d(qtFH1 8LeKwb 光源创建: x36NL^ iU,/!IQ 光源类型选择为任意平面,光源半角设定为15度。 @%%bRY `+Xe'ey LAos0bc)w\ 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。 5C*?1&
! +yiU@K).0 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。 CY5w$E $oc9
|Q 7 M!-q}5' ; 功率数值设定为:P=sin2(theta) theta为光源半角15度。我们为什么要这么设定,在第二部分会给出详细的公式推导。 .2/,XwIr !2wETs? 创建分析面: |C|:i@c
H =}"R5 mUiOD$rO 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。 2>ys2:z HmFNE$k
q'by;g*m 到此,所有的光学结构和属性设定完成,通过光线追迹我们可以查看光线是否可以穿过元件。 OoE9W F],TG&>5 FRED在探测器上穿过多个像素点迭代来创建热图 s5nB(L*Pjp {GAsFnZk FRED具有一个内置的可编译的Basic脚本语言。从Visual Basic脚本语言里,几乎所有用户图形界面(GUI)命令是可用这里的。FRED同样具有自动的客户端和服务器能力,它可以被调用和并调用其他可启动程序,如Excel。因此可以在探测器像素点上定义多个离轴光源,及在FRED Basic脚本语言里的For Next loops语句沿着探测器像素点向上和向下扫描来反向追迹光线,这样可以使用三维图表查看器(Tools/Open plot files in 3D chart)调用和查看数据。 H a90 将如下的代码放置在树形文件夹 Embedded Scripts, 4YBf ~Pp ZHb7+
'}@e5^oL 打开后清空里面的内容,此脚本为通用脚本适用于一切可热成像的应用。 jm4)gmC ^z38<L=z" 绿色字体为说明文字, /%-o.hT ;r%<2( '#Language "WWB-COM" x
Ridc^ 'script for calculating thermal image map }Z^FEd"y 'edited rnp 4 november 2005 _ \_3s :l4^iSf 'declarations gZ1N&/9; Dim op As T_OPERATION #&}%70R) Dim trm As T_TRIMVOLUME gYRqqV Dim irrad(32,32) As Double 'make consistent with sampling =z+-l5Gu" Dim temp As Double )_X;9%L7 Dim emiss As Double
4$..r4@ Dim fname As String, fullfilepath As String #j\*Lc"Ur: 8rla0d@ 'Option Explicit ]~$c~*0g md.* Sub Main eB)UXOu1 'USER INPUTS sV]i/B nx = 31 :O5Tr03z ny = 31 [5x+aW%ql numRays = 1000 aeLBaS minWave = 7 'microns (MZ A maxWave = 11 'microns t)YFTO"Jj sigma = 5.67e-14 'watts/mm^2/deg k^4 22l|!B%o fname = "teapotimage.dat" E=$7ieW IiG4ib>)W Print "" ]}jgB2x7 Print "THERMAL IMAGE CALCULATION" 6(\q< fx c& 9+/JYMo detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 "(9=h@@Y" ]|H]9mys98 Print "found detector array at node " & detnode -HO6K)ur \Sz4Gr0g3Z srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 KteZK.+#: F!
|TW6)gv Print "found differential detector area at node " & srcnode U@1#!ZZ6 @SX%?
mk8G GetTrimVolume detnode, trm JrY"J]/ detx = trm.xSemiApe de3yP, dety = trm.ySemiApe 8Sd?b5|G~ area = 4 * detx * dety gEcnn.(S Print "detector array semiaperture dimensions are " & detx & " by " & dety ;mCGh~?G Print "sampling is " & nx & " by " & ny iKP\/LR<n @h ,h=X 'reset differential detector area dimensions to be consistent with sampling (:tTx>V# pixelx = 2 * detx / nx yt]Oj*nn0K pixely = 2 * dety / ny F]dmc,Q SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False (ouRf;\6$8 Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 a!s.850@ dVY(V&p 'reset the source power X3&SL~&>g SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) hlABu)B'1 Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" Z&?+&q
r^ f(@"[-[ 'zero out irradiance array ~ wJ3AqNC? For i = 0 To ny - 1 p*(U*8Q For j = 0 To nx - 1 D}k-2RM2k irrad(i,j) = 0.0 1{;[q3a Next j x
mrugNRg Next i X#f+m) S
/)eNx 'main loop %_%f#S EnableTextPrinting( False ) Q]2sj: wfU&{7yt ypos = dety + pixely / 2 q9g[+*9]$ For i = 0 To ny - 1 RGx]DP$5G xpos = -detx - pixelx / 2 O>tC]sm% ypos = ypos - pixely B6Wq/fl/ [F BCz> EnableTextPrinting( True ) E)rOlh7 Print i i+qLc6|S=2 EnableTextPrinting( False ) S4aHce5PXA =2vMw] 3<~2"@J For j = 0 To nx - 1 ,_5YaX:<4 jx5[bUp4u xpos = xpos + pixelx {8*d;[X50 5pKvNLy.t 'shift source {{4p{ LockOperationUpdates srcnode, True y. ivz GetOperation srcnode, 1, op iA^+/Lt op.val1 = xpos t^bdi}[ op.val2 = ypos u]>>B>KOJ7 SetOperation srcnode, 1, op 'o#J>a~!9L LockOperationUpdates srcnode, False GP7)m Ma*dIwEp 'raytrace [Q.4]K2 DeleteRays #$vhC u<I CreateSource srcnode HIWmh4o/. TraceExisting 'draw YKX>@)Dxv SceCucT 'radiometry 9qu24zz$P For k = 0 To GetEntityCount()-1 j~,LoGuPh If IsSurface( k ) Then 8y4D9_{ temp = AuxDataGetData( k, "temperature" ) :+%h emiss = AuxDataGetData( k, "emissivity" ) ~y-vKCp| If ( temp <> 0 And emiss <> 0 ) Then yV+ E; ProjSolidAngleByPi = GetSurfIncidentPower( k ) ,GXfy9x7U frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) /qz "I-a irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi 5{d9,$%8& End If L@k;L eV{FcJha End If h,WY2Hr rJc)<OZjT Next k %Dr4~7=7a ,wb|?>Y Next j Oih2UrF yzM+28}L<I Next i ?od}~G4s# EnableTextPrinting( True ) 1f pS"_} cLyuCaH>c 'write out file !qw=I( fullfilepath = CurDir() & "\" & fname ?m_R U Open fullfilepath For Output As #1 :!iPn% Print #1, "GRID " & nx & " " & ny ?lwQne8/ Print #1, "1e+308" Uh|__DUkh Print #1, pixelx & " " & pixely kFIB lPV Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 :rs\ydDUF .dKRIFo maxRow = nx - 1 )D@n?qbG maxCol = ny - 1 6 XOu~+7 For rowNum = 0 To maxRow ' begin loop over rows (constant X) noUZ9M|hz row = "" K%TKQ<R| For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) [ls ?IFg row = row & irrad(colNum,rowNum) & " " ' append column data to row string @<TfA>*VJ Next colNum ' end loop over columns 4wj| (8-lDoW Print #1, row =@jMx^A" ~~:8Yv[( Next rowNum ' end loop over rows ;Y|~!%2~ Close #1 |Q)w3\S$ PSQ:' Print "File written: " & fullfilepath >wS:3$Q Print "All done!!" =Wy`X0h End Sub S.F=$z.% jme5'FR 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: PD
T\Q\J^X C94UF7al eZod}~J8 找到Tools工具,点击Open plot files in 3D chart并找到该文件 dbUZGn~ &P{p\ v2Y 4d._Hd=' 打开后,选择二维平面图: 6L> "m0 vwH7/+
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