切换到宽版
  • 广告投放
  • 稿件投递
  • 繁體中文
    • 1267阅读
    • 0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
    6374
    光币
    26015
    光券
    0
    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。 !'f3>W\   
    /U$8TT8+-  
    成像示意图
    =1oNZKBP  
    首先我们建立十字元件命名为Target f7hXQ|$  
    u=&Bmn_  
    创建方法: O%f8I'u$  
    &48_2Q"{  
    面1 : d"U(`E=H9  
    面型:plane 6] z}#"  
    材料:Air  UkfB^hA  
    孔径:X=1.5, Y=6,Z=0.075,形状选择Box 3I|3wQ&#(  
    XTeb9h)3  
    Vh<A2u3&  
    辅助数据: R 4wr  
    首先在第一行输入temperature :300K, *zWWmxcJa  
    emissivity:0.1; ;$BdP7i:  
    3_`szl-  
    }E}8_ 8T6  
    面2 : -Z^4L  
    面型:plane S)A'Y]2X  
    材料:Air M]HgIL@9#  
    孔径:X=1.5, Y=6,Z=0.075,形状选择Box *]x*B@RF  
    >?YNW   
    3,);0@I  
    位置坐标:绕Z轴旋转90度, Ze!92g  
    BwJuYH7QJ$  
    y_}SK6{  
    辅助数据: A%vsno!  
    'FzN[% K"  
    首先在第一行输入temperature :300K,emissivity: 0.1; R: aYL~  
    #vf_D?^  
    i_F$&?)  
    Target 元件距离坐标原点-161mm; l9/:FiJ_  
    *C,N'M<u  
    z]Acs  
    单透镜参数设定:F=100, bend=0, 位置位于坐标原点 DI&MC9j(   
    m]IysyFFK  
    {6xPdUhw  
    探测器参数设定: ~ H[%vdR  
    RP(/x+V  
    在菜单栏中选择Create/Element Primitive /plane hN(L@0)  
    aEx(rLd+  
    3SARr>HRyI  
    ?Ay3u^X  
    }`9`JmNM  
    sIm#_+Y  
    元件半径为20mm*20,mm,距离坐标原点200mm。 vv 7+ >%  
    LW39YMw<  
    光源创建: &-GuKH(Y<  
    FBsn;,3<W  
    光源类型选择为任意平面,光源半角设定为15度。 !%mi&ak(Rn  
    rF'R >/H  
    G^Xd-7 GQ  
    我们将光源设定在探测器位置上,具体的原理解释请见本章第二部分。 @+^c"=d1S  
    5a(<%Q <"  
    我们在位置选项又设定一行的目的是通过脚本自动控制光源在探测器平面不同划分区域内不同位置处追迹光线 #@Ujx_F  
    eO{@@?/y  
    KtTza5aF  
    功率数值设定为:P=sin2(theta) theta为光源半角15度。我们为什么要这么设定,在第二部分会给出详细的公式推导。 64D%_8#m  
    F@hYA  
    创建分析面: IM ad$AKc  
    fQQ |gwVki  
    ):bu;3E  
    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。 WF/l7u#4i  
    ';/84j-3F  
    lIuXo3  
    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。 { (\(m/!Z  
    KtMbze  
    FRED在探测器上穿过多个像素点迭代来创建热图 r]t )x*  
    U1Yo7nVf  
    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。 3c u9[~K  
    将如下的代码放置在树形文件夹 Embedded Scripts, )!C7bTv 4  
    93I'cWN  
    G\1J _al  
    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。 9Q@*0-  
    nC~fvyd<P  
    绿色字体为说明文字, 8^w/HCC8O  
    `{G?>z Fp  
    '#Language "WWB-COM" S+FQa7k  
    'script for calculating thermal image map )C}KR`"  
    'edited rnp 4 november 2005 T _~KxQ  
    k_Tswf3  
    'declarations b5Q8pWZg,  
    Dim op As T_OPERATION UE)fUTS  
    Dim trm As T_TRIMVOLUME J v<$*TVS0  
    Dim irrad(32,32) As Double 'make consistent with sampling d~<QAh#rG  
    Dim temp As Double IIax gfhZ  
    Dim emiss As Double M@O2 WB1ws  
    Dim fname As String, fullfilepath As String 6F`\YSn+  
    kV 1vb  
    'Option Explicit B+Q+0tw*i  
    NQ!<f\m4n  
    Sub Main ,xj3w#`zaf  
        'USER INPUTS OMd# ^z  
        nx = 31 hrT%XJl  
        ny = 31 M;qb7Mu  
        numRays = 1000 \[T{M!s  
        minWave = 7    'microns f N0bIE Y  
        maxWave = 11   'microns \ 522,n`  
        sigma = 5.67e-14 'watts/mm^2/deg k^4 -,/3"}<^78  
        fname = "teapotimage.dat" qsvpW%?aE  
    e;;):\p4  
        Print "" \c68n  
        Print "THERMAL IMAGE CALCULATION" M*H< n*  
    _vIO !*h0  
        detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 3"vRK5Bf  
    kdBV1E+:C  
        Print "found detector array at node " & detnode Wo2 v5-  
    }Eb]9c\  
        srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 V{FE[v_  
    ixzTJ]yu  
        Print "found differential detector area at node " & srcnode |>@ -grs  
    !Y|8z\ Q  
        GetTrimVolume detnode, trm d|3o/@k  
        detx = trm.xSemiApe ;24'f-Eri  
        dety = trm.ySemiApe $vqU|]J`  
        area = 4 * detx * dety >3+FZ@.iT  
        Print "detector array semiaperture dimensions are " & detx & " by " & dety QxA0I+i  
        Print "sampling is " & nx & " by " & ny '&)D>@g  
    H1C%o0CPY  
        'reset differential detector area dimensions to be consistent with sampling Pn J*Zea  
        pixelx = 2 * detx / nx HNFhH0+^  
        pixely = 2 * dety / ny _^b@>C>O  
        SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False +:!ScG*  
        Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 s~)L_ p  
    -HN%B?}. x  
        'reset the source power %GS\1 Q%  
        SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) ~ z>BfL  
        Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" v}&#f&q!  
    [5!'ykZ  
        'zero out irradiance array v#-E~;C cC  
        For i = 0 To ny - 1 $mD>r x  
            For j = 0 To nx - 1 2pjW,I!`  
                irrad(i,j) = 0.0 m'SmN{(t  
            Next j QS5H >5M)  
        Next i \.kTe<.:_  
    )X~#n  
        'main loop -$OD}5ku#  
        EnableTextPrinting( False ) ^A- sS~w  
    ^IYJEqK  
        ypos =  dety + pixely / 2 s><IykIi  
        For i = 0 To ny - 1 hc6.#~i  
            xpos = -detx - pixelx / 2 5pB^Y MP  
            ypos = ypos - pixely N:OD0m%`)  
    Et)9 20  
            EnableTextPrinting( True ) T6,V  
            Print i rv`2*B  
            EnableTextPrinting( False ) -!i;7[N  
    6EZ1YG}  
    z;U LQ  
            For j = 0 To nx - 1 -`Da`ml  
    xkF$D:s P  
                xpos = xpos + pixelx HRj7n<>L=  
    yB=C5-\F  
                'shift source jT{f<P0  
                LockOperationUpdates srcnode, True c1PViko,>  
                GetOperation srcnode, 1, op 0Y[*lM-  
                op.val1 = xpos Y:rJK|m  
                op.val2 = ypos hTDV!B-_(  
                SetOperation srcnode, 1, op bd} r#^'K  
                LockOperationUpdates srcnode, False BSOjyy1f  
    @l)\?IEF@f  
    raytrace Td5bDO  
                DeleteRays +O&RBEa[  
                CreateSource srcnode @X K>  
                TraceExisting 'draw FPvuzBJ  
    tF<^9stM  
                'radiometry %A8Pkr<&E  
                For k = 0 To GetEntityCount()-1 W)|c[Q\  
                    If IsSurface( k ) Then /SbSID_a  
                        temp = AuxDataGetData( k, "temperature" ) S^|$23}  
                        emiss = AuxDataGetData( k, "emissivity" ) nt drXg  
                        If ( temp <> 0 And emiss <> 0 ) Then /3OC7!~;fM  
                            ProjSolidAngleByPi = GetSurfIncidentPower( k ) yI3Q|731)  
                            frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) GSC{F#:z  
                            irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi WC3W+v G7  
                        End If -)4uYK*  
    U)u\1AV5  
                    End If -,FK{[h]ka  
    79 TPg  
                Next k }Q!h ov  
    >g>f;\mD7$  
            Next j mYiSR   
    g8LT7  
        Next i &/sGh0  
        EnableTextPrinting( True ) i/5y^  
    rny@n^F  
        'write out file (m<R0  
        fullfilepath = CurDir() & "\" & fname XyvZ&d6(d  
        Open fullfilepath For Output As #1 m5X3{[a :  
        Print #1, "GRID " & nx & " " & ny NQDLI 1o  
        Print #1, "1e+308" w 9G_>+?E  
        Print #1, pixelx & " " & pixely 5dg-d\ 6S  
        Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 /!^L69um  
    +R2^* *<  
        maxRow = nx - 1 h9w@oRp`~  
        maxCol = ny - 1 G /NT e  
        For rowNum = 0 To maxRow                    ' begin loop over rows (constant X) 's$A+8;L  
                row = "" jN31\)/i  
            For colNum = maxCol To 0 Step -1            ' begin loop over columns (constant Y) c_@XQ&DC`  
                row = row & irrad(colNum,rowNum) & " "     ' append column data to row string ~!8%_J_  
            Next colNum                     ' end loop over columns T g3:VD  
    8]sTX9  
                Print #1, row I++W0wa.n  
    U(rr vNt:t  
        Next rowNum                         ' end loop over rows 6.7`0v?,n  
        Close #1 \Pw8wayr%  
    tn"Y9 k|  
        Print "File written: " & fullfilepath H @_eFlT t  
        Print "All done!!" A Oby*c  
    End Sub ybD{4&ZE  
    IW5*9)N?  
    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: `V]egdO  
    i!CKA}",  
    >v^2^$^u  
    找到Tools工具,点击Open plot files in 3D chart并找到该文件 .'l.7t  
      
    9 eSN+q  
    4(` 2#  
    打开后,选择二维平面图: w^ixMn~nLF  
    ]NaMZ  
     
    分享到