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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。 XHU$&t`7>g  
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    成像示意图
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    首先我们建立十字元件命名为Target XSC=qg$  
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    创建方法: f(pq`v^-n  
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    面1 : bVUIeX'  
    面型:plane ;(?tlFc  
    材料:Air }PJsPIa3j  
    孔径:X=1.5, Y=6,Z=0.075,形状选择Box os{ iY  
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    辅助数据: 14 & KE3`  
    首先在第一行输入temperature :300K, gbuh04#~  
    emissivity:0.1; c9nR&m8(+  
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    面2 : sm-[=d%@L  
    面型:plane JVu j u$k  
    材料:Air &MSU<S?1  
    孔径:X=1.5, Y=6,Z=0.075,形状选择Box hiS|&5#  
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    位置坐标:绕Z轴旋转90度, Z8 v8@Y  
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    辅助数据: |@AXW   
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    首先在第一行输入temperature :300K,emissivity: 0.1; JjS+'A$A5  
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    Target 元件距离坐标原点-161mm; 4SI~y;c)  
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    单透镜参数设定:F=100, bend=0, 位置位于坐标原点 vntJe^IaFd  
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    探测器参数设定: +fk*c[FG  
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    在菜单栏中选择Create/Element Primitive /plane .rK0C)  
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    元件半径为20mm*20,mm,距离坐标原点200mm。 VwI  
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    光源创建: )P(S:x'b0  
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    光源类型选择为任意平面,光源半角设定为15度。 9;L4\  
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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。 Leb Kzqe  
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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 dCoP qKy  
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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。 :i!fPNn  
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    创建分析面: 6!]@ S|vDX  
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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。 aA4RC0'  
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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。 ~Fb@E0 }!  
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    FRED在探测器上穿过多个像素点迭代来创建热图 O H>.N"IG  
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    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。 tCrEcjT-  
    将如下的代码放置在树形文件夹 Embedded Scripts, wK2$hsque  
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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。 eA1g}ipm  
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    绿色字体为说明文字, eI ( S)q  
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    '#Language "WWB-COM" H}r]j\  
    'script for calculating thermal image map c $1u  
    'edited rnp 4 november 2005 Q qF<HCO  
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    'declarations IrZjlnht  
    Dim op As T_OPERATION =-oP,$k  
    Dim trm As T_TRIMVOLUME Y!j/,FU  
    Dim irrad(32,32) As Double 'make consistent with sampling _t-6m2A  
    Dim temp As Double <9&GOaJ  
    Dim emiss As Double 6H0kY/quL|  
    Dim fname As String, fullfilepath As String F2zo !a8  
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    'Option Explicit ,IhQ%)l  
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    Sub Main N_ ODr]L  
        'USER INPUTS Vl$RMW@Ds  
        nx = 31 0 @#Jz#?  
        ny = 31 K_+M?ap_  
        numRays = 1000 N|mggz  
        minWave = 7    'microns OF*E1B M  
        maxWave = 11   'microns jkl dr@t  
        sigma = 5.67e-14 'watts/mm^2/deg k^4 pImq< Z  
        fname = "teapotimage.dat" r4u ,I<ZbH  
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        Print "" Bj{J&{  
        Print "THERMAL IMAGE CALCULATION" (;g/wb:  
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        detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 kR1 12J9P  
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        Print "found detector array at node " & detnode x(>XM:|  
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        srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 5q4wREh  
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        Print "found differential detector area at node " & srcnode <>KQ8:  
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        GetTrimVolume detnode, trm R[j'<gd.  
        detx = trm.xSemiApe W/RB|TMT  
        dety = trm.ySemiApe nEUH;z  
        area = 4 * detx * dety 0Bgj.?l  
        Print "detector array semiaperture dimensions are " & detx & " by " & dety 6 [bQ'Ir^8  
        Print "sampling is " & nx & " by " & ny |9i[*]  
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        'reset differential detector area dimensions to be consistent with sampling 6a9:P@tY  
        pixelx = 2 * detx / nx `!X8Cn  
        pixely = 2 * dety / ny @ebY_*  
        SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False @=g{4(zR ^  
        Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 yz3=#  
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        'reset the source power V,zFHXO  
        SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) , MqoX-+  
        Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" bfb9A+]3'  
    @}^VA9ULK  
        'zero out irradiance array 9Pvv6WyKy  
        For i = 0 To ny - 1 L   
            For j = 0 To nx - 1 \1?'JdN  
                irrad(i,j) = 0.0 pQZ`dS\  
            Next j >`WQxkpy  
        Next i _TdH6[9  
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        'main loop 4<<eqxI$|  
        EnableTextPrinting( False ) qz)KCEs  
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        ypos =  dety + pixely / 2 Y x66Xy  
        For i = 0 To ny - 1 kg(}%Ih  
            xpos = -detx - pixelx / 2 ;fQIaE&H  
            ypos = ypos - pixely *k&V;?x|wt  
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            EnableTextPrinting( True ) #$ka.Pj  
            Print i jc32s}/H  
            EnableTextPrinting( False ) iig4JP'h  
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            For j = 0 To nx - 1 lwG)&qyVd  
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                xpos = xpos + pixelx b5~p:f-&4B  
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                'shift source DgRn^gL{Q  
                LockOperationUpdates srcnode, True u!HbS*jqq  
                GetOperation srcnode, 1, op [@pumH>  
                op.val1 = xpos $Ups9pQ  
                op.val2 = ypos qs8^qn0A  
                SetOperation srcnode, 1, op vEE\{1  
                LockOperationUpdates srcnode, False mWP&N#vwh  
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    raytrace P=P']\`p+  
                DeleteRays .f[z_% ar  
                CreateSource srcnode `.~*pT*u  
                TraceExisting 'draw @5 ??`n  
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                'radiometry !u:;Ew  
                For k = 0 To GetEntityCount()-1 klc$n07  
                    If IsSurface( k ) Then %LqT>HXJ  
                        temp = AuxDataGetData( k, "temperature" ) sA+K?_  
                        emiss = AuxDataGetData( k, "emissivity" ) 44k8IYC*o  
                        If ( temp <> 0 And emiss <> 0 ) Then lN"@5(5%  
                            ProjSolidAngleByPi = GetSurfIncidentPower( k ) 2H] 7=j  
                            frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) ,l,q;]C%  
                            irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi EKuLt*a/  
                        End If ym` 4v5w  
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                    End If SpIiMu(  
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                Next k g^#,!e  
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            Next j McbbEs=)  
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        Next i lQRtsmZ0  
        EnableTextPrinting( True ) %n,_^voE  
    )RWY("SUy1  
        'write out file y34<B)Wy  
        fullfilepath = CurDir() & "\" & fname w%oa={x  
        Open fullfilepath For Output As #1 " w /Odd  
        Print #1, "GRID " & nx & " " & ny yYTOp^  
        Print #1, "1e+308" 3<1x>e2nT  
        Print #1, pixelx & " " & pixely eT2Tg5Etc  
        Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 &:}WfY!hX  
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        maxRow = nx - 1 Osy_C<O  
        maxCol = ny - 1 s? Gv/&  
        For rowNum = 0 To maxRow                    ' begin loop over rows (constant X) F{ C2% s#  
                row = "" xNRMI!yv   
            For colNum = maxCol To 0 Step -1            ' begin loop over columns (constant Y) #B!M,TWf9s  
                row = row & irrad(colNum,rowNum) & " "     ' append column data to row string B <G,{k  
            Next colNum                     ' end loop over columns p%#'`*<a_  
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                Print #1, row xbCQ^W2YU|  
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        Next rowNum                         ' end loop over rows rodqa  
        Close #1 /z}b1m+  
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        Print "File written: " & fullfilepath wIWO?w2  
        Print "All done!!" d+ [2Sm(7  
    End Sub I;UT; /E2  
    }Q6o#oZ  
    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: XBcbLF  
    ,.|/B^jV  
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    找到Tools工具,点击Open plot files in 3D chart并找到该文件 Uaj_,qb(  
      
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    打开后,选择二维平面图: -I;\9r+  
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