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    [分享]十字元件热成像分析 [复制链接]

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    离线infotek
     
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    只看楼主 倒序阅读 楼主  发表于: 2020-11-18
    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。 SUhP e+  
    H/f= 2b  
    成像示意图
    6V/mR~F1r  
    首先我们建立十字元件命名为Target 5]+eLKXB  
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    创建方法: XW:(FzF  
    GssoT<Y)Z  
    面1 : t[~i})yS  
    面型:plane VZR6oia  
    材料:Air ~<LI p%5(  
    孔径:X=1.5, Y=6,Z=0.075,形状选择Box c2"OpI  
    OYy8u{@U:  
    rt z(Jt{<  
    辅助数据: IRB;Q(Z   
    首先在第一行输入temperature :300K, Gr?gHAT  
    emissivity:0.1; v<4zcMv  
    {S!~pn&^Y  
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    面2 : #D8)rs.9  
    面型:plane 0"Hf6xz  
    材料:Air  .~']gih#  
    孔径:X=1.5, Y=6,Z=0.075,形状选择Box _qfdk@@g  
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    位置坐标:绕Z轴旋转90度, ;$]R#1i44  
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    辅助数据: r@aFB@   
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    首先在第一行输入temperature :300K,emissivity: 0.1; O^GTPYW  
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    Target 元件距离坐标原点-161mm; +dRTHz  
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    单透镜参数设定:F=100, bend=0, 位置位于坐标原点 JaEyVe  
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    探测器参数设定: oc.x1<Nd  
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    在菜单栏中选择Create/Element Primitive /plane 0@KBQv"v  
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    元件半径为20mm*20,mm,距离坐标原点200mm。 =y ff.3mW\  
    &fWZ%C7|jC  
    光源创建: WA+v&* ]  
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    光源类型选择为任意平面,光源半角设定为15度。 );C !:?  
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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。 XyhdsH5%3!  
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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 [69aTl>/  
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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。 &p*N8S8  
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    创建分析面: /[mCK3_  
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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。 <[*s%9)'9  
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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。 f -#fi7  
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    FRED在探测器上穿过多个像素点迭代来创建热图 5D'8 l@7  
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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。 y8sI @y6  
    将如下的代码放置在树形文件夹 Embedded Scripts, n '&WIf3  
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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。 *`\>J.  
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    绿色字体为说明文字, 7oUYRqd  
    lA{Sr0f TP  
    '#Language "WWB-COM" o] = &  
    'script for calculating thermal image map H|Eu,eq-E  
    'edited rnp 4 november 2005 L3&NGcd  
    ^LZU><{';  
    'declarations <yeG0`}t  
    Dim op As T_OPERATION pNDL:vMWP  
    Dim trm As T_TRIMVOLUME t4nAy)I)P  
    Dim irrad(32,32) As Double 'make consistent with sampling #<)u%)`  
    Dim temp As Double q4VOK 'N  
    Dim emiss As Double b afYjF< 3  
    Dim fname As String, fullfilepath As String S\Q/ "Y  
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    'Option Explicit d6_ CsqV  
    "g0L n5&  
    Sub Main iNha<iS+  
        'USER INPUTS |d8/ZD  
        nx = 31 !Y5O3^I=u  
        ny = 31 ,]>Eg6B,u  
        numRays = 1000 G|.>p<q   
        minWave = 7    'microns &K}!R$[,:P  
        maxWave = 11   'microns s`&8tP  
        sigma = 5.67e-14 'watts/mm^2/deg k^4 #b:8-Lt:M  
        fname = "teapotimage.dat" fAJQ8nb{@]  
    a(bgPkPP  
        Print "" NoV2<m$  
        Print "THERMAL IMAGE CALCULATION" Wh"oL;O  
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        detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 iN_G|w[d  
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        Print "found detector array at node " & detnode " GgK,d}%  
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        srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 Ig]Gg/1G  
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        Print "found differential detector area at node " & srcnode Q[S""P.Z|  
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        GetTrimVolume detnode, trm :v=Yo  
        detx = trm.xSemiApe ) =sm{R%T  
        dety = trm.ySemiApe  |G{TA  
        area = 4 * detx * dety *l^h;RSx  
        Print "detector array semiaperture dimensions are " & detx & " by " & dety ?> }bg  
        Print "sampling is " & nx & " by " & ny C;M.dd  
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        'reset differential detector area dimensions to be consistent with sampling EG2NE,,r  
        pixelx = 2 * detx / nx n a_Y<R`  
        pixely = 2 * dety / ny pGh2 4E  
        SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False : >4{m)  
        Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 <T{PuS1<o  
    [<7Hy,xr_  
        'reset the source power 8v_HIx0xu  
        SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) {!@Pho)Q  
        Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" l}># p'$  
    pl%3RVpoc  
        'zero out irradiance array 1W;q(#q  
        For i = 0 To ny - 1 # KK>D?.:  
            For j = 0 To nx - 1 =.f]OWehu.  
                irrad(i,j) = 0.0 (pNA8i%=G  
            Next j 5Jlz$]f  
        Next i F`r=M%yh  
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        'main loop ~bhesWk8!  
        EnableTextPrinting( False ) d\+smED  
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        ypos =  dety + pixely / 2 ojni+}>_  
        For i = 0 To ny - 1 ?>LsIPa  
            xpos = -detx - pixelx / 2 \E5%.KR  
            ypos = ypos - pixely uAwT)km {  
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            EnableTextPrinting( True ) -=I*{dzly  
            Print i {=VauF  
            EnableTextPrinting( False ) <:fjWy  
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            For j = 0 To nx - 1 O|}97a^  
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                xpos = xpos + pixelx )<nr;n  
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                'shift source eYLeytF]Uy  
                LockOperationUpdates srcnode, True ?KDI'>"-v  
                GetOperation srcnode, 1, op ?kMG!stgp}  
                op.val1 = xpos <E[X-S%&  
                op.val2 = ypos ,IX:u1mO  
                SetOperation srcnode, 1, op fH-V!QYGF  
                LockOperationUpdates srcnode, False #8H  
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                'raytrace %{Ez0XwGCn  
                DeleteRays nSdta'6  
                CreateSource srcnode PBc.}TSGj  
                TraceExisting 'draw `VM@-;@w  
    rf?Q# KM\W  
                'radiometry Nz %{T  
                For k = 0 To GetEntityCount()-1 7vax[,a I  
                    If IsSurface( k ) Then Ju4={^#  
                        temp = AuxDataGetData( k, "temperature" ) L?T%;VdG'>  
                        emiss = AuxDataGetData( k, "emissivity" ) xj~5/)XX|X  
                        If ( temp <> 0 And emiss <> 0 ) Then *J&XM[t  
                            ProjSolidAngleByPi = GetSurfIncidentPower( k ) %Aq+t&-BCX  
                            frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) [x Xa3W  
                            irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi ?~s,O$o  
                        End If q'{LTg0kk  
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                    End If ~Q}JC3f>  
    +dIDFSd  
                Next k m08:EX P  
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            Next j UT!gAU  
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        Next i s=9gp$9m  
        EnableTextPrinting( True ) 9un* 1%  
    o\6A]T=R  
        'write out file ,*ZdM w!  
        fullfilepath = CurDir() & "\" & fname  JsAl;w  
        Open fullfilepath For Output As #1 huVw+vAA  
        Print #1, "GRID " & nx & " " & ny frV *+  
        Print #1, "1e+308" 6 B>1"h%Wf  
        Print #1, pixelx & " " & pixely S3EM6`q'  
        Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 H=b54.J8&  
    m!{Xuy  
        maxRow = nx - 1 Hg$t,\j  
        maxCol = ny - 1 /;>U0~K  
        For rowNum = 0 To maxRow                    ' begin loop over rows (constant X) l+g\xUP  
                row = "" gw[\7  
            For colNum = maxCol To 0 Step -1            ' begin loop over columns (constant Y) Uv|z c  
                row = row & irrad(colNum,rowNum) & " "     ' append column data to row string k=">2!O/  
            Next colNum                     ' end loop over columns 1|/P[!u  
    rS1mBrqD  
                Print #1, row Teq1VK3Hr  
    5MUM{(C  
        Next rowNum                         ' end loop over rows <Th) &  
        Close #1 d67Q@ ')00  
    k+Ew+j1_  
        Print "File written: " & fullfilepath !}%,rtI  
        Print "All done!!" mHcxK@qw  
    End Sub GiI|6z!  
    #lDf8G|ST~  
    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: 7u8HcHl  
    Hjl{M>z  
    uFxhr2 <z  
    找到Tools工具,点击Open plot files in 3D chart并找到该文件 zzmZ`Ya  
      
    ;:(kVdb  
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    打开后,选择二维平面图: oS3}xT" U  
    i$MYR @  
    QQ:2987619807
    " p]bsJG  
     
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