| infotek |
2022-01-24 09:30 |
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。 9
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成像示意图 ~0S_S +e 首先我们建立十字元件命名为Target 8T3j/D<r _0Mt*]L } 创建方法: 7#\\Ava$T K x7'm1 面1 : Aqi9@BH 面型:plane i+`N0!8lY 材料:Air K0681_bp 孔径:X=1.5, Y=6,Z=0.075,形状选择Box f@:.bp8VB8 B2}|b^'I
v.wHj@ 辅助数据: MiB"CcU 首先在第一行输入temperature :300K, "qb1jv#to emissivity:0.1; 3zV{cm0 -Re4G78% )ad-p.Hus 面2 : Gag=GHG 面型:plane .i^aYbB$X 材料:Air -kFPmM; 孔径:X=1.5, Y=6,Z=0.075,形状选择Box %hEhZW{: e
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z+G 位置坐标:绕Z轴旋转90度, s>i`=[qFc GqYE=Q
I-=H;6w7 辅助数据: *^]lFuX\&E .fZ*N/ 首先在第一行输入temperature :300K,emissivity: 0.1; 3B{B6w}t&
2aROY2 K'Gv+UC*6 Target 元件距离坐标原点-161mm; (5-4`:1ux 7hg)R
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.{pc5eUf 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 K6C@YY( \NIj&euF 5*Wo/%#q 探测器参数设定: H<hFA(M WH@CH4WM 在菜单栏中选择Create/Element Primitive /plane TB!z:n X>0$zE@0
?3X(`:KB !|SVRaS H)eecH$K =TTk5(m 元件半径为20mm*20,mm,距离坐标原点200mm。 38I .1p9 SHc<`M'+ 光源创建: Xup"gYTZQ F@+FXnz 光源类型选择为任意平面,光源半角设定为15度。 L)0j& f{m,?[1C, j,HUk,e^& 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。 >?pWbL C(RZ09,.S 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。 @raw8w\Zj+ x4r=ENO)q n!nXM 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。 !9w;2Z]uum mX4u#$xs: 创建分析面: fR:BF47 o$S/EZ k^x[(gw 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。 "kYzgi Q9Y$x{R&
;q8tOvQ 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。 M9_G X^2Txm d FRED在探测器上穿过多个像素点迭代来创建热图 R a> k#pQ H(MCY3t 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。 ucVWvXCr 将如下的代码放置在树形文件夹 Embedded Scripts, m'L7K K-Y) xK8n~.T('
1XwW4cZ>: 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。 & o2F4 F5*NK!U 绿色字体为说明文字, UG]]Vk1d] }I1A4=d '#Language "WWB-COM" Lq-Di|6q 'script for calculating thermal image map @[:JQ'R= 'edited rnp 4 november 2005 #/UlW
$O+e+Y 'declarations Ql%0%naq1 Dim op As T_OPERATION Vy+%sG
q" Dim trm As T_TRIMVOLUME Z#2AK63/T Dim irrad(32,32) As Double 'make consistent with sampling =nq9)4o Dim temp As Double Oq7R^t`b Dim emiss As Double n@hf{hA[a Dim fname As String, fullfilepath As String sSh=Idrx S%+$ 'Option Explicit r35'U#VMk? zW,Nv>Ac5 Sub Main 0+i\j`O& 'USER INPUTS BIFuQ?j3 nx = 31 3Zr'Mn ny = 31 ?r`UBR+[ numRays = 1000 :X?bWxOJ minWave = 7 'microns `I\)Kk@*b9 maxWave = 11 'microns *=6,}rX"I sigma = 5.67e-14 'watts/mm^2/deg k^4 Ab"mX0n fname = "teapotimage.dat" OG M9e! 1 z4s1Y Print "" |k
# ~ Print "THERMAL IMAGE CALCULATION" !Q`vOVSUD &$'=SL(Z detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 ~#doJ:^H3 #ny&bJj Print "found detector array at node " & detnode 6{XdLI SS4'yaQ srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 +npcU:(Kg r N"P
IH Print "found differential detector area at node " & srcnode Uf:G,%OYi SO}$96 GetTrimVolume detnode, trm ,P?R
3 detx = trm.xSemiApe F(-1m A&- dety = trm.ySemiApe Xv`c@n) area = 4 * detx * dety A?
=(q Print "detector array semiaperture dimensions are " & detx & " by " & dety ]^>#?yEA3 Print "sampling is " & nx & " by " & ny qep<7 QO [jOvy>2K] 'reset differential detector area dimensions to be consistent with sampling N|pyp*8Z pixelx = 2 * detx / nx |;L%hIR[
pixely = 2 * dety / ny -n C
5 SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False 64#6L.Q-c Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 WIe2j 4_#yl9+ 'reset the source power HuX{8nl a SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) Rwy<#9R[x Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" M5SAlj a"!D @a 'zero out irradiance array b&Dc DX For i = 0 To ny - 1 rKP;T"?; For j = 0 To nx - 1 F-=W7 D:[c irrad(i,j) = 0.0 [5v[Zqud Next j 5UFR^\e Next i I+) Acy; x*)@:W! 'main loop yM3]<~m EnableTextPrinting( False ) (I?CW~3# y=L9E? ypos = dety + pixely / 2 R+c
{Pl For i = 0 To ny - 1 ` "Gd/ xpos = -detx - pixelx / 2 'xO^2m+N; ypos = ypos - pixely =uZOpeviQ qR
WWG& EnableTextPrinting( True ) u>G#{$) Print i . Q#X'j EnableTextPrinting( False ) N6GvzmG#g |JpLMUG MTKd:.J6 For j = 0 To nx - 1 ; r SpM pg}9baW? xpos = xpos + pixelx x5Sc+5?* u&iMY3= 'shift source ,j4 ;:F LockOperationUpdates srcnode, True +^St"GWY GetOperation srcnode, 1, op ^-CQ9r* op.val1 = xpos 4= VAJ op.val2 = ypos J!Kk7!^| SetOperation srcnode, 1, op FW)G5^Tf LockOperationUpdates srcnode, False YN\!I 0]dL;~0y. raytrace `Gl@?9,i DeleteRays =] R_6# CreateSource srcnode a95QDz TraceExisting 'draw |%F[.9Dp &yKUf 'radiometry Ok-*xd For k = 0 To GetEntityCount()-1 u S$:J:Drx If IsSurface( k ) Then 0@R @L}m temp = AuxDataGetData( k, "temperature" ) {DPobyvwFk emiss = AuxDataGetData( k, "emissivity" ) \9T;-] If ( temp <> 0 And emiss <> 0 ) Then ^cYm.EHI ProjSolidAngleByPi = GetSurfIncidentPower( k ) :)GtPTD frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) yNk9KK ) irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi fP41B End If #ii,GN~N *@'\4OO End If +L4_] DrD68$,QN Next k hWGCYkuW <r*A(}Y Next j _rQM[{Bkg iJg3`1@j Next i D0?l$]aE EnableTextPrinting( True ) ^O
cM)Z6h 8$fiq}a 'write out file s=lkK/ [ fullfilepath = CurDir() & "\" & fname C7ZU)MEUd/ Open fullfilepath For Output As #1 9aw- n*< Print #1, "GRID " & nx & " " & ny '1{#I/P; Print #1, "1e+308" \JBJ$lBL Print #1, pixelx & " " & pixely /J8'mCuC. Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 ~eH+*U|\|M J4
yT| maxRow = nx - 1 ;J3az` maxCol = ny - 1 Ju$vuEO For rowNum = 0 To maxRow ' begin loop over rows (constant X) ;;E "+. row = "" Lh~Ym<CeN For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) UE4zmIq row = row & irrad(colNum,rowNum) & " " ' append column data to row string q9j9"M' Next colNum ' end loop over columns m/"\+Hv gt3;Xi Print #1, row RVmD& eATX8`W Next rowNum ' end loop over rows ,c:Fa)- Close #1 uy~KJn?Tu yQ>
*F Print "File written: " & fullfilepath T,h,)|:I^ Print "All done!!" $wa )e End Sub ?@
ei_<A{ *pN,@ZV$ 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: i)V-q9\ o6^^hc\ fL7ym,? 找到Tools工具,点击Open plot files in 3D chart并找到该文件 Hh=D:kE `F:PWG` }SHF 打开后,选择二维平面图: hS4Ljyeg }Y(yDg;"
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