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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。 ]%6XE) u85Uy
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成像示意图 ^1+=HdN, 首先我们建立十字元件命名为Target d+6-ten 4q`e<!MP)q 创建方法: >f~y2YAr k
3oR: 面1 : li)shp) 面型:plane Xa=oEG 材料:Air FJ
V!B& 孔径:X=1.5, Y=6,Z=0.075,形状选择Box uRRp8hht UV)!zgP
oAq<ag\qV 辅助数据: Pu0O6@Rg 首先在第一行输入temperature :300K, uKpWb1( emissivity:0.1; uU`Mq8)R )tR@\G >% mT#ebeBaf 面2 : e_t""h4D
面型:plane {$qLMx'; 材料:Air v^Pjvv = 孔径:X=1.5, Y=6,Z=0.075,形状选择Box +J(@. J*"G*x#u $n9Bp'< 位置坐标:绕Z轴旋转90度, S5xum_Dq ~g|z7o
A{KF<Omu 辅助数据: <lHVch"(^$ q5ja \ 首先在第一行输入temperature :300K,emissivity: 0.1; H6%%n
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ycSC'R Target 元件距离坐标原点-161mm; Y.v. EZ +G?nmXG[vj
@vkO(o 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 |qX[Dk VF] ~J=>i <aGfQg|554 探测器参数设定: -}Q^A_xK u8i!Fxu 在菜单栏中选择Create/Element Primitive /plane $"6O92G(hJ 2<8JY4]!]
u40<>A >]S-a-|Bp zDx*R3% I`FqZw 元件半径为20mm*20,mm,距离坐标原点200mm。 }
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XS( 光源创建: w{5v*SHl}` x72T5. 光源类型选择为任意平面,光源半角设定为15度。 tg'2v/ hNF. Yl0_?.1 z 我们将光源设定在探测器位置上,具体的原理解释请见本章第二部分。 b1ma(8{{{ eg
Zb)pP 我们在位置选项又设定一行的目的是通过脚本自动控制光源在探测器平面不同划分区域内不同位置处追迹光线。 5Cjh%rj(jl `hE@S |4 G[M{TS3&Ds 功率数值设定为:P=sin2(theta) theta为光源半角15度。我们为什么要这么设定,在第二部分会给出详细的公式推导。 ;f+bIYQz -"MB(` 创建分析面: nH7i)!cI~ hqVxvS" we;QrS(Hi 到这里元件参数设定完成,现在我们设定元件的光学属性,在前面我们分别对第一和第二面设定的温度和发射系数,散射属性我们设定为黑朗伯,4%的散射。并分别赋予到面一和面二。 <maYS2 6y+}=)J
:FqHMN 到此,所有的光学结构和属性设定完成,通过光线追迹我们可以查看光线是否可以穿过元件。 ym.:I@b?6 ( ,!G$~Sy FRED在探测器上穿过多个像素点迭代来创建热图 q7ubRak Y$&+2w,)H, FRED具有一个内置的可编译的Basic脚本语言。从Visual Basic脚本语言里,几乎所有用户图形界面(GUI)命令是可用这里的。FRED同样具有自动的客户端和服务器能力,它可以被调用和并调用其他可启动程序,如Excel。因此可以在探测器像素点上定义多个离轴光源,及在FRED Basic脚本语言里的For Next loops语句沿着探测器像素点向上和向下扫描来反向追迹光线,这样可以使用三维图表查看器(Tools/Open plot files in 3D chart)调用和查看数据。 yV/A%y-P 将如下的代码放置在树形文件夹 Embedded Scripts, 5x/LHsr=m 1&Ruz[F5
+ tza]r: 打开后清空里面的内容,此脚本为通用脚本适用于一切可热成像的应用。 g;G]Xi.B} C3>`e3v 绿色字体为说明文字, U+wfq%Fz T99\R% '#Language "WWB-COM" ;>Q.r{P 'script for calculating thermal image map %RX}sS 'edited rnp 4 november 2005 1NQstmd{ T5b*Ia 'declarations !au%D?w Dim op As T_OPERATION 7r,h[9~e Dim trm As T_TRIMVOLUME Qq*Ks
5 Dim irrad(32,32) As Double 'make consistent with sampling .T|1l$Jn Dim temp As Double QkU6eE<M* Dim emiss As Double +(l(|lQy$ Dim fname As String, fullfilepath As String uA~T.b\ wseb]=U 'Option Explicit C6ry]R@ eB,eu4+- Sub Main E\lel4ai 'USER INPUTS ?|,-Bft3 nx = 31 T i!<{> ny = 31 .R5(k'g? numRays = 1000 M:QM*?+) minWave = 7 'microns 8^>qzaf
8 maxWave = 11 'microns CP"
sigma = 5.67e-14 'watts/mm^2/deg k^4 oW\kJ>! fname = "teapotimage.dat" (>a8h~Na |];f?1 Print "" iz@LS Print "THERMAL IMAGE CALCULATION" yirQ .5K}R< detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 m(o^9R_=^9 ?4A$9H Print "found detector array at node " & detnode (dgBI}Za ~D1&CT#s srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 R7Z7o4jg ~us1Df0bp Print "found differential detector area at node " & srcnode QK0-jYG^ +fRABY5C GetTrimVolume detnode, trm 7x5wT ?2W detx = trm.xSemiApe S2,tv dety = trm.ySemiApe |(77ao3 area = 4 * detx * dety o`+$h:zm@ Print "detector array semiaperture dimensions are " & detx & " by " & dety
_(1Shm Print "sampling is " & nx & " by " & ny H2
Gj(Nc- &&$,BFY4 'reset differential detector area dimensions to be consistent with sampling 9_ru*j\ pixelx = 2 * detx / nx S<nf"oy_K pixely = 2 * dety / ny ` 5lW SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False o<Y[GW1pg Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 K2
b\9} R+b~m!58 'reset the source power x?rn<= SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) .mwB'Ll Print "resetting the source power to " & GetSourcePower( srcnode ) & " units"
_CImf1 =%Z5"]; 'zero out irradiance array S\"#E:A For i = 0 To ny - 1 QpI\\Zt6 For j = 0 To nx - 1 U *K6FWqiB irrad(i,j) = 0.0 A-*y[/ Next j 7I4<Dj Next i KMll8X %|AXVv7IN> 'main loop M,we9];N EnableTextPrinting( False ) up==g [
@ASAhV^+ ypos = dety + pixely / 2 V7(-<})8 For i = 0 To ny - 1 LTlbrB xpos = -detx - pixelx / 2 ;6AanwR6 ypos = ypos - pixely A!uO7".E )&vuT
q'7' EnableTextPrinting( True ) V ah&)&n Print i Mfinh@K, EnableTextPrinting( False ) [~{'"-3L0 ,+GS.]8< v9
*WM3 For j = 0 To nx - 1 =lZtI6tZ $eiW2@ xpos = xpos + pixelx Rv)*Wo!L 5hj
_YqQ7 'shift source Ou7nk:I@ LockOperationUpdates srcnode, True E]dc4US GetOperation srcnode, 1, op ?XllPnuKt% op.val1 = xpos U
uEm{ op.val2 = ypos S;iJQS SetOperation srcnode, 1, op ^@HWw@GA LockOperationUpdates srcnode, False *4OB
88$ VOGx 'raytrace iiLDl DeleteRays f<y-{.VnN$ CreateSource srcnode gN;
E}AQt TraceExisting 'draw (i;,D- :j&- Lc 'radiometry Nh[H[1"J For k = 0 To GetEntityCount()-1 ac%x\e$ If IsSurface( k ) Then Av>xgfX temp = AuxDataGetData( k, "temperature" ) rH$M6S emiss = AuxDataGetData( k, "emissivity" ) * -X`^R If ( temp <> 0 And emiss <> 0 ) Then Ejt?B')aB5 ProjSolidAngleByPi = GetSurfIncidentPower( k ) "h7Np/ m3 frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) {HbSty irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi wnjAiIE5 End If 66{Dyn7J~ Vy 7 )_D End If q+ 2v9K@ I(uM`g Next k N nq r{ub QB"+B]rV Next j vD76IG j m _[h!r;DsG Next i -,q
qQf EnableTextPrinting( True ) VQ;'SY:` M'nzoRk 'write out file ,wZq~;2 fullfilepath = CurDir() & "\" & fname 0@wXE\s Open fullfilepath For Output As #1 "Pl.G[Buc- Print #1, "GRID " & nx & " " & ny x}~Z[ bx Print #1, "1e+308"
PckAL Print #1, pixelx & " " & pixely 1EWskmp Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 zmFS]IOv$ M^{=& maxRow = nx - 1 Uc9hv? maxCol = ny - 1 /h 4rW>8D2 For rowNum = 0 To maxRow ' begin loop over rows (constant X) yp]z@SYA@ row = "" PkcvUJV For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) .UYhj8 row = row & irrad(colNum,rowNum) & " " ' append column data to row string l
p|`n Next colNum ' end loop over columns
{__NVv VV"w{#XKw Print #1, row f h:wmc' -`D<OSt7 Next rowNum ' end loop over rows 9B/iQCFtj$ Close #1 nd"$gi " ~q~)T1Z Print "File written: " & fullfilepath `SQobH Print "All done!!" ?Kg_bvoR End Sub N!./u(b QBd4ok:R 在输出报告中,我们会看到脚本对光源的孔径和功率做了修改,并最终经过31次迭代,将所有的热成像数据以dat的格式放置于: W9;9\k a5 pXn v]A %WPyc%I 找到Tools工具,点击Open plot files in 3D chart并找到该文件 Z+ _xX 0|ekwTx. %$N,6}n 打开后,选择二维平面图: "sT)<Wc O7m-_#/\
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