| 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。 zZDr=6|r_ gHm^@
成像示意图 Jw86P= 首先我们建立十字元件命名为Target Ak1f*HGl| xXyzzr1[ 创建方法: 7g=Ze~aq D}_\oE/n 面1 : `HHbQXB 面型:plane hup]Jk 材料:Air +C+3DwN 孔径:X=1.5, Y=6,Z=0.075,形状选择Box htkyywv {)Gh~~57_W
_o`'b80; 辅助数据: )\s:.<?EQ 首先在第一行输入temperature :300K, ]{;K|rCR- emissivity:0.1; {^N=hI sGzd c ,@2O_O`: 面2 : 9aXm} 面型:plane LxG :?=O. 材料:Air b9:E0/6
孔径:X=1.5, Y=6,Z=0.075,形状选择Box ebQYk$@ kiXa2Yn*(d [OMKk#vW 位置坐标:绕Z轴旋转90度, A]>0lB bbnAF*7s8
&18} u~M 辅助数据: 3<Cd>o. 8T1`TGSFC 首先在第一行输入temperature :300K,emissivity: 0.1; rb9x|| /.}&yRR fXL$CgXG\x Target 元件距离坐标原点-161mm; `!rHH !.F`8OD`u
v1;`.PWD 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 8rw;Yo<k Q PGssQR6 BV7GzJ2([{ 探测器参数设定: ,g/ UPK8K= $3FFb#r 在菜单栏中选择Create/Element Primitive /plane cU*7E39 }G-qOt
ZL-@2ZU{1 YwKY3kL f9#B(4Tgi ww[STg 元件半径为20mm*20,mm,距离坐标原点200mm。 `33+OW [=XsI]B\ 光源创建: 3"q%-M|+Q ZfMJU 光源类型选择为任意平面,光源半角设定为15度。 `<[Zs]Fe4 d<#Xqc RJ@d_~%U 我们将光源设定在探测器位置上,具体的原理解释请见本章第二部分。 U4Qc$&j> X8Gw8^t 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。 0Wk}d(f =#uXO< RN!oflb 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。 ^2Op?J CM7j^t 创建分析面: !a?o9<V I_N"mnn@Nr QK//bV) 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。 $(C71M|CT "i9$w\lm
ynDa4HB 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。 8a"aJYj (}bP`[@rX! FRED在探测器上穿过多个像素点迭代来创建热图 Rqu;;VI[ Cm>8r5LG 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。 [f^~Z'TIN/ 将如下的代码放置在树形文件夹 Embedded Scripts, ~)WE Jw9|I)H
[L9e.n1 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。 5P+3D{ ]xV7)/b5G 绿色字体为说明文字, 2<U5d` {8b6A~/ '#Language "WWB-COM" 6rdm=8WFA 'script for calculating thermal image map %vyjn&13 'edited rnp 4 november 2005 R1A!ob Dh J<\_; 'declarations RM QlciG Dim op As T_OPERATION H6*F?a`)I Dim trm As T_TRIMVOLUME ~9 K4]5K- Dim irrad(32,32) As Double 'make consistent with sampling jG8ihi Dim temp As Double @;Yb6&I; Dim emiss As Double 2I6 c7H s Dim fname As String, fullfilepath As String 7?/ Fr(\ Ge|caiH1I 'Option Explicit =3""D{l GT2;o Sub Main c~z{/L 'USER INPUTS JF!!)6!2# nx = 31 N',]WZ} ny = 31 Rnun() plJ numRays = 1000 SyX>zN! minWave = 7 'microns oP_'0h0X maxWave = 11 'microns Uu8Z2M sigma = 5.67e-14 'watts/mm^2/deg k^4 ;k!bv|>n fname = "teapotimage.dat" "'dt"x) h dPKeqg7 Print "" "7iHTV Print "THERMAL IMAGE CALCULATION" Z}$.Tm CKrh14ul detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 I6h{S}2 ym8\q:N(R Print "found detector array at node " & detnode q<.^DO~$L Y!CZ?c)@ srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 |L<oKMZY ) Q]kUG#` Print "found differential detector area at node " & srcnode bWG}>{fj }JAg<qy} GetTrimVolume detnode, trm !9OAMHa*9 detx = trm.xSemiApe
//f[%j*> dety = trm.ySemiApe d),@&MSN area = 4 * detx * dety x-(?^g Print "detector array semiaperture dimensions are " & detx & " by " & dety ?cowey\m
. Print "sampling is " & nx & " by " & ny \d%&_rp =`Nnd@3v 'reset differential detector area dimensions to be consistent with sampling -9vAY+s. pixelx = 2 * detx / nx {Km|SG[-q pixely = 2 * dety / ny `L7 cS SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False XOVZ'V Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 a{el1_DIGK rh/3N8[6 'reset the source power $l-j(=Md SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) &I <R|a Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" 4- N># 5{[3I|m{ 'zero out irradiance array h$4V5V For i = 0 To ny - 1 (a@cK, For j = 0 To nx - 1 zxTm`Dh;[ irrad(i,j) = 0.0 6D_4o&N Next j bP(V#6IJ8 Next i oI/@w `Nc3I\tCM 'main loop 31<hn+pE& EnableTextPrinting( False ) R qOEQ*k yV=hi?f-[V ypos = dety + pixely / 2 !fyE
Hk For i = 0 To ny - 1 "?}QwtUW xpos = -detx - pixelx / 2 A\.k['! ypos = ypos - pixely /$]dVvhX% ir3iW*5k EnableTextPrinting( True ) C[_{ $j(J Print i VOp8 ,! EnableTextPrinting( False ) ~ m,z| DTAEfs!ZW Xj?j1R>GB For j = 0 To nx - 1 6EP5n daY^{u3 xpos = xpos + pixelx nLJ]tpw^DH 6aXsRhQ~ 'shift source z2wR]G5! LockOperationUpdates srcnode, True nYTI\f/8v GetOperation srcnode, 1, op |o|0qG@g op.val1 = xpos ~|R"GloUw op.val2 = ypos S'B7C>i`#N SetOperation srcnode, 1, op ,`S"nq LockOperationUpdates srcnode, False m 9.QGX\] V?0|#=_mE raytrace %fK"g2: DeleteRays 'hg, W] CreateSource srcnode /vwGSuk._ TraceExisting 'draw ^L*:0P~ JY_+p9KfyQ 'radiometry ].7)^ For k = 0 To GetEntityCount()-1 `b# w3 2 If IsSurface( k ) Then z^ KrR temp = AuxDataGetData( k, "temperature" ) 6(<M.U_ft emiss = AuxDataGetData( k, "emissivity" ) *.ZV.( If ( temp <> 0 And emiss <> 0 ) Then &z&Jl#t-) ProjSolidAngleByPi = GetSurfIncidentPower( k ) #eR*|W7o frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) GriL< =?t irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi V)_mo/D!D End If : ,LX3, L`yS' End If *"q ~z $ [M8G Next k !NZFo S~ Go+f0aig Next j \62|w HX L#m1!+J Next i Q~ te` EnableTextPrinting( True ) NcB^qv &AoXv`l4 'write out file zG+oZ fullfilepath = CurDir() & "\" & fname Mpb|qGi! Open fullfilepath For Output As #1 A
ElNf: Print #1, "GRID " & nx & " " & ny ^W3xw[{ Print #1, "1e+308" s)8g4Yc* Print #1, pixelx & " " & pixely _u]Wr%D@ Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 {CYFM[V u=p([
5] maxRow = nx - 1 sj0Hv d9 maxCol = ny - 1 OiJ1&Fz( For rowNum = 0 To maxRow ' begin loop over rows (constant X) ]@C&Q,~q row = ""
s@K|zOx For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) '<4/Md[ row = row & irrad(colNum,rowNum) & " " ' append column data to row string ) zz"DH Next colNum ' end loop over columns Kw"7M~ `>g:
: Print #1, row <vhlT#p
G#
.z((Rj Next rowNum ' end loop over rows xCiY
jl$ Close #1 v`*!Bhc- 6rq:jvlx$ Print "File written: " & fullfilepath #L`@[" Print "All done!!" yAW%y End Sub 3K_J"B*7 m!tB;:6 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: }3V Q*'X>i ys u"+J CM!bD\5 找到Tools工具,点击Open plot files in 3D chart并找到该文件 roVGS{4T\ .?@$Rd2@W ,_F1g<^@u 打开后,选择二维平面图: ri.;& k-*H=km
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