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    [技术]十字元件热成像分析 [复制链接]

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    只看楼主 倒序阅读 楼主  发表于: 2022-01-24
    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探测器上,并显示其热成像图。 ^hC'\09=c  
    cqNK`3:.j  
    成像示意图
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    首先我们建立十字元件命名为Target w6% Q"%rp  
    ;hX(/T  
    创建方法: H,!xTy"Wh  
    7z{wYCw  
    面1 : <=q} Nd\  
    面型:plane B )r-,M  
    材料:Air }~XWtWbd-  
    孔径:X=1.5, Y=6,Z=0.075,形状选择Box `Z?wj@H1`  
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    辅助数据: jmM|on!  
    首先在第一行输入temperature :300K, []>'Dw_r  
    emissivity:0.1; '-;[8:y.  
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    面2 : 9Eyx Ob  
    面型:plane k"(]V  
    材料:Air $<^t][{  
    孔径:X=1.5, Y=6,Z=0.075,形状选择Box 9)q3cjP{<  
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    位置坐标:绕Z轴旋转90度, 'pdTV:]zA  
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    辅助数据: /U~|B.z@6  
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    首先在第一行输入temperature :300K,emissivity: 0.1; ~&?bU]F  
    *v>ZE6CL  
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    Target 元件距离坐标原点-161mm; J-F".6i5  
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    单透镜参数设定:F=100, bend=0, 位置位于坐标原点 ggr  
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    探测器参数设定: 6o 3 bq|  
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    在菜单栏中选择Create/Element Primitive /plane ~GaGDS\V  
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    元件半径为20mm*20,mm,距离坐标原点200mm。 {f!/:bM  
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    光源创建: xvr5$x|h  
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    光源类型选择为任意平面,光源半角设定为15度。 dhl[=Y ` Q  
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    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。 W .7rHa  
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    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 E h%61/  
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    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。 ]$ew 5%  
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    创建分析面: 29R-Up!SVN  
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    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。  6 K $mW  
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    到此,所有的光学结构和属性设定完成,通过光线追迹我们可以查看光线是否可以穿过元件。 E*_^+ %  
    DT1gy:?L  
    FRED在探测器上穿过多个像素点迭代来创建热图 PJnC  
    ?0tg}0|  
    FRED具有一个内置的可编译的Basic脚本语言。从Visual Basic脚本语言里,几乎所有用户图形界面(GUI)命令是可用这里的。FRED同样具有自动的客户端和服务器能力,它可以被调用和并调用其他可启动程序,如Excel。因此可以在探测器像素点上定义多个离轴光源,及在FRED Basic脚本语言里的For Next loops语句沿着探测器像素点向上和向下扫描来反向追迹光线,这样可以使用三维图表查看器(Tools/Open plot files in 3D chart)调用和查看数据。 .p`4>XA  
    将如下的代码放置在树形文件夹 Embedded Scripts, %B3~t>  
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    打开后清空里面的内容,此脚本为通用脚本适用于一切可热成像的应用。 |Lq8cA)|y  
    W+nu=iQ!  
    绿色字体为说明文字, l{3B }_,  
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    '#Language "WWB-COM" wN 2+3LY{  
    'script for calculating thermal image map +Qs]8*^?;  
    'edited rnp 4 november 2005 N!A20Bv  
    'nJF:+30ZH  
    'declarations )n/%P4l  
    Dim op As T_OPERATION ;?6vKpj;  
    Dim trm As T_TRIMVOLUME WKf<% E$  
    Dim irrad(32,32) As Double 'make consistent with sampling #F*|@  
    Dim temp As Double K,f:X g!:  
    Dim emiss As Double mgxIxusR  
    Dim fname As String, fullfilepath As String w7nt $L5  
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    'Option Explicit B( [x8A]  
    N,ht<l\  
    Sub Main I8F+Z  
        'USER INPUTS NGra/s,9 |  
        nx = 31 TyxIlI4"  
        ny = 31 gmTBT#{6yH  
        numRays = 1000 }ze+ tf  
        minWave = 7    'microns U%{GLO   
        maxWave = 11   'microns 1I Yip\:lS  
        sigma = 5.67e-14 'watts/mm^2/deg k^4 #GsOE#*>T  
        fname = "teapotimage.dat" l,wlxh$}(  
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        Print "" (5a73%>@  
        Print "THERMAL IMAGE CALCULATION" Q&m85'r5X  
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        detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 vr!J3H f  
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        Print "found detector array at node " & detnode PN}+LOD<t  
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        srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 D6SUzI1+H  
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        Print "found differential detector area at node " & srcnode ycGY5t@K@  
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        GetTrimVolume detnode, trm zVhyAf  
        detx = trm.xSemiApe >T$0*7wF  
        dety = trm.ySemiApe ,"qCz[aDN1  
        area = 4 * detx * dety wcHk]mLM  
        Print "detector array semiaperture dimensions are " & detx & " by " & dety *k$[/{S1-  
        Print "sampling is " & nx & " by " & ny #J5BHY~  
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        'reset differential detector area dimensions to be consistent with sampling \u=d`}E  
        pixelx = 2 * detx / nx {sTf4S\S  
        pixely = 2 * dety / ny ,CE/o7.FG  
        SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False %wD#[<BGn>  
        Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 D(cD8fn,J  
    ,n|si#  
        'reset the source power 68%aDs  
        SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) IrwQ~z3I  
        Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" c '|*{%<e2  
    egmUUuO  
        'zero out irradiance array W5j wD  
        For i = 0 To ny - 1 YMGy-]!o  
            For j = 0 To nx - 1 Q+CJd>B  
                irrad(i,j) = 0.0 /SvhOi  
            Next j |T#cq!  
        Next i Fwm$0=BXL  
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        'main loop 9#E *o~1  
        EnableTextPrinting( False ) x/QqG1q  
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        ypos =  dety + pixely / 2 #%,X),%-  
        For i = 0 To ny - 1 uJ`N'`Z  
            xpos = -detx - pixelx / 2 cS&KD@.  
            ypos = ypos - pixely o Rfb4+H&  
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            EnableTextPrinting( True ) Zy0M\-Mn  
            Print i 2:LUB)&i  
            EnableTextPrinting( False )  D2e-b  
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            For j = 0 To nx - 1 +h) "m/mE  
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                xpos = xpos + pixelx ~z^l~Vyg?  
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                'shift source KFM[caKeJO  
                LockOperationUpdates srcnode, True N'1I6e"  
                GetOperation srcnode, 1, op 2 BY|Cp4R  
                op.val1 = xpos s/1r{;q  
                op.val2 = ypos 3}L3n*Ft#.  
                SetOperation srcnode, 1, op ];.5 *a%*  
                LockOperationUpdates srcnode, False 3mgvWR  
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    raytrace %<i sdvF  
                DeleteRays U$:^^Zt`B  
                CreateSource srcnode %Z;RY5  
                TraceExisting 'draw 1N/4W6  
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                'radiometry %Tp9G Gt  
                For k = 0 To GetEntityCount()-1 v]JET9hY  
                    If IsSurface( k ) Then >WHajYO"  
                        temp = AuxDataGetData( k, "temperature" ) 0+&WIs  
                        emiss = AuxDataGetData( k, "emissivity" ) aru2H6  
                        If ( temp <> 0 And emiss <> 0 ) Then _ep&`K  
                            ProjSolidAngleByPi = GetSurfIncidentPower( k ) [gzaOP`f  
                            frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) Gm+D1l i  
                            irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi ^C gg1e1  
                        End If .+7n@Sc  
    4DIU7#GG  
                    End If t!D'ZLw  
    Q}#4Qz~n  
                Next k /X8a3Eqp9  
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            Next j !&%KJS6p4  
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        Next i j)i c7 b  
        EnableTextPrinting( True ) Vy& X1lG:  
    f:j:L79}  
        'write out file P IG,a~  
        fullfilepath = CurDir() & "\" & fname (JU8F-/9  
        Open fullfilepath For Output As #1 \:'GAByy  
        Print #1, "GRID " & nx & " " & ny j ,rc9  
        Print #1, "1e+308" ~HY)$Yp;  
        Print #1, pixelx & " " & pixely Zl_sbIY  
        Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 5|0}bv O  
    l@4pZkdq  
        maxRow = nx - 1 DzC`yWstP  
        maxCol = ny - 1 jS,Pu%fR  
        For rowNum = 0 To maxRow                    ' begin loop over rows (constant X) U& GPede  
                row = "" 8hV]t'/;  
            For colNum = maxCol To 0 Step -1            ' begin loop over columns (constant Y) U/c+j{=~  
                row = row & irrad(colNum,rowNum) & " "     ' append column data to row string |@d(2f8  
            Next colNum                     ' end loop over columns X&Oo[Z  
    %>&~?zrq  
                Print #1, row J5b3r1~D"[  
    eg~ Dm>Es  
        Next rowNum                         ' end loop over rows ' !huU   
        Close #1 "'B DVxp'w  
    R14&V1 tZ  
        Print "File written: " & fullfilepath j1Ys8k%$l  
        Print "All done!!" :] Wn26z)  
    End Sub )t~ad]oM  
    +@$VJM%^7b  
    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:  7]@M  
    ~vP_c(8f  
    C,;?`3bH@  
    找到Tools工具,点击Open plot files in 3D chart并找到该文件 D~inR3(}  
      
    52^3N>X4X  
    ^uX"04>;  
    打开后,选择二维平面图: K*^'t ltJ  
    A@M2(?w4  
     
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