切换到宽版
  • 广告投放
  • 稿件投递
  • 繁體中文
    • 614阅读
    • 1回复

    [技术]十字元件热成像分析 [复制链接]

    上一主题 下一主题
    离线infotek
     
    发帖
    6243
    光币
    25360
    光券
    0
    只看楼主 倒序阅读 楼主  发表于: 2023-04-06
    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。 }.bhsy  
    R'M=`33M  
    成像示意图
    @K{1O|V  
    首先我们建立十字元件命名为Target NF9fPAF%;  
    [1Cs  
    创建方法: xLID @9Hbu  
    ,+LX.f&/8!  
    面1 : r57CyO  
    面型:plane Aun X[X9  
    材料:Air M.b1=Y  
    孔径:X=1.5, Y=6,Z=0.075,形状选择Box ;h|zNx0  
    >J4Tk1//b  
    -B+Pl*  
    辅助数据: \53(D7+  
    首先在第一行输入temperature :300K, QYl Pr&O9  
    emissivity:0.1; # !:u*1  
    OFcL h  
    _[J @w.l(  
    面2 : .x6c.Y.S  
    面型:plane =EE>QM  
    材料:Air _c[Bjip  
    孔径:X=1.5, Y=6,Z=0.075,形状选择Box g" c|%3  
    gzV&S5A{_  
    #Tm^$\*h\]  
    位置坐标:绕Z轴旋转90度, ,gag_o{*a  
    'MF|(`  
    {Y0Uln5u  
    辅助数据: BC*)@=7fx  
    . }#R  
    首先在第一行输入temperature :300K,emissivity: 0.1; -L zx3"  
    hrT!S  
    ~f:y^`+Q[  
    Target 元件距离坐标原点-161mm; K'/,VALp  
    ^a,Oi%  
    abs\Ku9  
    单透镜参数设定:F=100, bend=0, 位置位于坐标原点 & B CA  
    c%?31 t  
    E;I'b:U`  
    探测器参数设定: `1O<UJX  
    HV*D l$  
    在菜单栏中选择Create/Element Primitive /plane <in#_Of {E  
    ]x;*Z&  
    J #ukH`|-  
    1$+-?:i C  
    $ G\IzK  
    __B`0t  
    元件半径为20mm*20,mm,距离坐标原点200mm。 zc1y)s0G  
    !Eqp,"ts7  
    光源创建: htgtgW9 ^P  
    /=y _ #l  
    光源类型选择为任意平面,光源半角设定为15度。 u*W6fg/"  
    pgp@Zw)r)k  
    O6 :GE'S  
    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。 QGC%, F"+  
    NZ{)&ObBRt  
    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 d9qA\ [  
    Z30r|Ufh  
    7{"urs7 T  
    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。 &"_5?7_N  
    #0:N$'SZ  
    创建分析面: V"A*k^}  
    47/14rY 2  
    xE{PsN1 X;  
    到这里元件参数设定完成,现在我们设定元件的光学属性,在前面我们分别对第一和第二面设定的温度和发射系数,散射属性我们设定为黑朗伯,4%的散射。并分别赋予到面一和面二。 r2h{#2  
    Exu5|0AAE  
    YA?46[:  
    到此,所有的光学结构和属性设定完成,通过光线追迹我们可以查看光线是否可以穿过元件。 ],?$&  
    _NwB7@ e  
    FRED在探测器上穿过多个像素点迭代来创建热图 9/yE\p .  
    yJ0q)x sS  
    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。 ^8z~`he=_J  
    将如下的代码放置在树形文件夹 Embedded Scripts, "t ^yM`$5[  
    $2><4~T;|A  
    I1Jhvyd?$  
    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。 +N3f{-{"Yo  
    &"R`:`XF  
    绿色字体为说明文字, ntZl(]l  
    =sIkA)"!=  
    '#Language "WWB-COM" y\C_HCU H  
    'script for calculating thermal image map 8Ry%HV9VE  
    'edited rnp 4 november 2005 9w"kxAN  
    ]b+Nsr~  
    'declarations wf,B/[,d  
    Dim op As T_OPERATION o<\u Hr3  
    Dim trm As T_TRIMVOLUME V_Xq&!HN[  
    Dim irrad(32,32) As Double 'make consistent with sampling X+$IaLfCxD  
    Dim temp As Double y~r5KB6w  
    Dim emiss As Double wG-lR,glb  
    Dim fname As String, fullfilepath As String a3wk#mH  
    [S:{$4&  
    'Option Explicit @dHQ}Ni  
    >"/Sa_w  
    Sub Main vMHJgpd&j  
        'USER INPUTS IE0hC\C}  
        nx = 31 ; `Vbl_"L  
        ny = 31 {Y6;/".DM  
        numRays = 1000 T4e-QEH  
        minWave = 7    'microns R[bI4|t  
        maxWave = 11   'microns [+2iwfD  
        sigma = 5.67e-14 'watts/mm^2/deg k^4 D\LXjEm e.  
        fname = "teapotimage.dat" I$Ra*r  
    cxB{EH,2Um  
        Print "" `%<^$Ng;  
        Print "THERMAL IMAGE CALCULATION" H3Zs m)+:  
    6}"t;4@$x  
        detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 )r`F}_CEL  
    (DTXc2)c  
        Print "found detector array at node " & detnode wticA#mb  
    )d =8)9B  
        srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 3o.9}`/  
    k@=w? m  
        Print "found differential detector area at node " & srcnode t \;,$i  
    ?(2^lH~6h  
        GetTrimVolume detnode, trm 9J(jbJ7p  
        detx = trm.xSemiApe D6NgdE7b  
        dety = trm.ySemiApe 'g#EBy  
        area = 4 * detx * dety 6b7SA ,  
        Print "detector array semiaperture dimensions are " & detx & " by " & dety 2)4oe  
        Print "sampling is " & nx & " by " & ny 0w9[Z  
    |<Rf^"T  
        'reset differential detector area dimensions to be consistent with sampling ^,sKj-  
        pixelx = 2 * detx / nx V")u y&Ob  
        pixely = 2 * dety / ny `F,*NESv  
        SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False S @tpd'  
        Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 wxW\L!@  
    }\oy%]_mY  
        'reset the source power %]\IC(q  
        SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) ;cfmMt!QWJ  
        Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" Re]7G.y  
    qf?X:9Wt  
        'zero out irradiance array 3?Tk[m1b  
        For i = 0 To ny - 1 ?_BK(kL_  
            For j = 0 To nx - 1 Jd-u ?  
                irrad(i,j) = 0.0  X0&[cyP!  
            Next j P;DGs]PF  
        Next i $PbwC6>8  
    "qxu9Hg!  
        'main loop =1e>$E#  
        EnableTextPrinting( False ) 9yWQ}h  
    ? 1 ~C`I;  
        ypos =  dety + pixely / 2 E,$5 V^ 9  
        For i = 0 To ny - 1 d7i 0'R  
            xpos = -detx - pixelx / 2 6ntduXeNVh  
            ypos = ypos - pixely rhQv,F9  
    xu(N'l.7&  
            EnableTextPrinting( True ) s;!Tz)  
            Print i k*$[V17  
            EnableTextPrinting( False ) ,5J}Wo?Q}  
    am(jmf::  
    ffgb 3  
            For j = 0 To nx - 1 A.>L>uR  
    s:f%=4-7  
                xpos = xpos + pixelx ;lU]ilYv  
    :I/i"g7<  
                'shift source  bMDj+i  
                LockOperationUpdates srcnode, True :o=a@Rqx  
                GetOperation srcnode, 1, op kHx6]<  
                op.val1 = xpos )D>= \ Me  
                op.val2 = ypos &vHfuM`  
                SetOperation srcnode, 1, op jTE~^  
                LockOperationUpdates srcnode, False Kjfpq!NYE  
    [)KLmL%  
    'raytrace H=1Jq  
                DeleteRays y~-dQ7r  
                CreateSource srcnode % >}{SS  
                TraceExisting 'draw n7*.zI]%&  
    qEy]Rc%  
                'radiometry 3V)NM%Aw  
                For k = 0 To GetEntityCount()-1 MB:*WA&  
                    If IsSurface( k ) Then B kh1VAT  
                        temp = AuxDataGetData( k, "temperature" ) hsEQ6  
                        emiss = AuxDataGetData( k, "emissivity" ) d@#wK~I  
                        If ( temp <> 0 And emiss <> 0 ) Then N}5'Hk4+  
                            ProjSolidAngleByPi = GetSurfIncidentPower( k ) |xX>AMZc)D  
                            frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) dp~] Wx  
                            irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi Kh,zp{  
                        End If R^ &nBwp  
    p"ElO,\  
                    End If ,p7W4;?4  
    2Pz)vnV"  
                Next k 1C]mxV=%  
    Y}UVC|Ef  
            Next j R}J}Q b  
    ),;O3:n  
        Next i ccm(r~lhJ  
        EnableTextPrinting( True ) nLcOz3h  
    <V_P)b8$1  
        'write out file .M zAkZ=  
        fullfilepath = CurDir() & "\" & fname R[T94U  
        Open fullfilepath For Output As #1 l %M0^d6M  
        Print #1, "GRID " & nx & " " & ny Lj#K^c Ee  
        Print #1, "1e+308" s6+`cC4  
        Print #1, pixelx & " " & pixely RhQ[hI  
        Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 T=D|jt  
    #Rx|oSc}  
        maxRow = nx - 1 K]s*rPT/,  
        maxCol = ny - 1 ~4'AnoD1w  
        For rowNum = 0 To maxRow                    ' begin loop over rows (constant X) o b,%); m  
                row = "" ?X5Y8n]y\h  
            For colNum = maxCol To 0 Step -1            ' begin loop over columns (constant Y) !,z ==Qp|v  
                row = row & irrad(colNum,rowNum) & " "     ' append column data to row string \Uh$%#}.  
            Next colNum                     ' end loop over columns nlsif  
    6L4<c+v_  
                Print #1, row unZYFA}(  
    8{ooLdpX7  
        Next rowNum                         ' end loop over rows g*%z{w  
        Close #1 Z:3SI$tO  
    /CfgxPo  
        Print "File written: " & fullfilepath (m%A>e B  
        Print "All done!!" ~P;KO40K  
    End Sub &w7Ev21  
    m&!4*D  
    在输出报告中,我们会看到脚本对光源的孔径和功率做了修改,并最终经过31次迭代,将所有的热成像数据以dat的格式放置于: 4k4 d%  
    v"3($?au0  
    l Taw6;  
    找到Tools工具,点击Open plot files in 3D chart并找到该文件 C0v1x=(xiM  
      
    Ap)[;_9BD  
    4/:}K>S_  
    打开后,选择二维平面图: 5@&{%99  
    ^Pp2T   
     
    分享到
    离线谭健
    发帖
    6859
    光币
    24090
    光券
    0
    只看该作者 1楼 发表于: 2023-04-07
    感谢分享 b;k3B7<