切换到宽版
  • 广告投放
  • 稿件投递
  • 繁體中文
    • 1873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
    在线infotek
     
    发帖
    6593
    光币
    27114
    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。 TxJoN]Z.  
    7eNLs  
    成像示意图
    8F>u6Y[P  
    首先我们建立十字元件命名为Target 2[!3!@.  
    gB _/(  
    创建方法: < `$svM  
    q ~%'V  
    面1 : 2[Ofa(mkkp  
    面型:plane y^!>'cdV  
    材料:Air (@DqKB  
    孔径:X=1.5, Y=6,Z=0.075,形状选择Box =Bg $OX  
    2LfiaHO  
    U g:  
    辅助数据: Bd'X~Vj<  
    首先在第一行输入temperature :300K, @V?T'@W7D  
    emissivity:0.1; L@5sY0 M  
    &Fiesi!tET  
    V` T l$EF  
    面2 : c,2OICj  
    面型:plane H(hE;|q/  
    材料:Air ^4b;rLfk@  
    孔径:X=1.5, Y=6,Z=0.075,形状选择Box 6i+<0b}!/  
    Y#,&Tu  
    lRk_<A  
    位置坐标:绕Z轴旋转90度, b(IZ:ekZ5  
    |}7!'f\M  
    XF&_**0n  
    辅助数据: YpOcLxFL  
    4wMZNa<Sx  
    首先在第一行输入temperature :300K,emissivity: 0.1;  )[S#:PP  
    tk)J E^'  
    o%b6"_~%3  
    Target 元件距离坐标原点-161mm; lfAiW;giJ  
    k vpkWD;  
    E^iShe  
    单透镜参数设定:F=100, bend=0, 位置位于坐标原点 wBWqibY|  
    o;9 G{Xj3@  
    %G|Rb MP  
    探测器参数设定: ?8w5tfN6t  
    <{+U- ^rzR  
    在菜单栏中选择Create/Element Primitive /plane UX2@eyejQ7  
    Z0/$XS9|h;  
    &cWC&Ws"  
    1{ H=The  
     >akC  
    { 2%'=v  
    元件半径为20mm*20,mm,距离坐标原点200mm。 Pn,>eD*g  
    )Q 5 x%  
    光源创建: g~ii^[W  
    J-|&[-Z  
    光源类型选择为任意平面,光源半角设定为15度。 3(Ns1/;?,  
    DfU]+;AE  
    ?I8r2M]  
    我们将光源设定在探测器位置上,具体的原理解释请见本章第二部分。 _dY5qW1p  
    74 W Ky  
    我们在位置选项又设定一行的目的是通过脚本自动控制光源在探测器平面不同划分区域内不同位置处追迹光线 eslvg#Q  
    Pl. y9g~  
    04WxV(fo'  
    功率数值设定为:P=sin2(theta) theta为光源半角15度。我们为什么要这么设定,在第二部分会给出详细的公式推导。 f}~=C2R1<!  
    (rc 7Cp3  
    创建分析面: l^XOW- ;u  
    cyLl,OA  
    m68>`  
    到这里元件参数设定完成,现在我们设定元件的光学属性,在前面我们分别对第一和第二面设定的温度和发射系数,散射属性我们设定为黑朗伯,4%的散射。并分别赋予到面一和面二。 d[{!^,%x"  
    M&jlUr&l  
    Kx?.g#>U;  
    到此,所有的光学结构和属性设定完成,通过光线追迹我们可以查看光线是否可以穿过元件。 Y_}_)nE@m  
     @M OaXe  
    FRED在探测器上穿过多个像素点迭代来创建热图 7|o!v);uR  
    UlWm). b;v  
    FRED具有一个内置的可编译的Basic脚本语言。从Visual Basic脚本语言里,几乎所有用户图形界面(GUI)命令是可用这里的。FRED同样具有自动的客户端和服务器能力,它可以被调用和并调用其他可启动程序,如Excel。因此可以在探测器像素点上定义多个离轴光源,及在FRED Basic脚本语言里的For Next loops语句沿着探测器像素点向上和向下扫描来反向追迹光线,这样可以使用三维图表查看器(Tools/Open plot files in 3D chart)调用和查看数据。 gAh#H ?MM  
    将如下的代码放置在树形文件夹 Embedded Scripts, &"?99E>  
    yM}3u4FG  
    ?yxQs=&-q~  
    打开后清空里面的内容,此脚本为通用脚本适用于一切可热成像的应用。 hH9~.4+*`g  
    {+ Ibi{  
    绿色字体为说明文字, em95ccs'-  
    blWtC/!Aq;  
    '#Language "WWB-COM" c|d,:u#  
    'script for calculating thermal image map 3~Lsa"/  
    'edited rnp 4 november 2005 >S-JAPuO  
    }VRl L>HAC  
    'declarations aM xd"cTzx  
    Dim op As T_OPERATION H0!$aO  
    Dim trm As T_TRIMVOLUME gkX7,J-0  
    Dim irrad(32,32) As Double 'make consistent with sampling tUuARo7#  
    Dim temp As Double f`KO#Wc  
    Dim emiss As Double (t\U5-w  
    Dim fname As String, fullfilepath As String 7x=4P|(\}  
    QFnpp\K  
    'Option Explicit S8B?uU  
    Fc8 0HK5R  
    Sub Main gTgoS:M"_O  
        'USER INPUTS >&Oql9_  
        nx = 31 a'`?kBK7`U  
        ny = 31 MRw4?HqB  
        numRays = 1000 ;X a N  
        minWave = 7    'microns SSxz1y  
        maxWave = 11   'microns $.t>* Bq  
        sigma = 5.67e-14 'watts/mm^2/deg k^4 Q-!gO  
        fname = "teapotimage.dat" +zd/<  
    qp)Wt6 k?  
        Print "" o$Ylqb#  
        Print "THERMAL IMAGE CALCULATION" c_CVZR?  
    xkw=os  
        detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 r{t6Vv2J  
    zd)QCq  
        Print "found detector array at node " & detnode $qr6LIKGw  
    !zm;C@}ln  
        srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 Y8^ WuN$  
    A^p{Cq@E  
        Print "found differential detector area at node " & srcnode %LzARTX  
    !V(r p80  
        GetTrimVolume detnode, trm >d=pl}-kOQ  
        detx = trm.xSemiApe mhX66R  
        dety = trm.ySemiApe 5 2 Qr  
        area = 4 * detx * dety "/RMIS K[;  
        Print "detector array semiaperture dimensions are " & detx & " by " & dety AD^I1 ]2f  
        Print "sampling is " & nx & " by " & ny c|`$ h  
    Zhv%mUj~  
        'reset differential detector area dimensions to be consistent with sampling kxd*B P  
        pixelx = 2 * detx / nx hdi0YL  
        pixely = 2 * dety / ny i\l}M]Z#  
        SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False $Hj;i/zD  
        Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 A6 .wXv,  
    ,Pcg+^A  
        'reset the source power .4U*.Rf  
        SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) *!JB^5(H  
        Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" `Fo/RZOW  
    JKfJ%yy |  
        'zero out irradiance array \lm]G7h  
        For i = 0 To ny - 1 fqY'Uq$=  
            For j = 0 To nx - 1 })P!7t  
                irrad(i,j) = 0.0 KK #E qJ  
            Next j X[r0$yuE  
        Next i 23i2yT  
    qbeUc5`1  
        'main loop }mK,Bi?bj  
        EnableTextPrinting( False ) "O0xh_Nr  
    'sH_^{V2  
        ypos =  dety + pixely / 2 {QylNC9  
        For i = 0 To ny - 1 OqDP{X:  
            xpos = -detx - pixelx / 2 M2|h.+[Q  
            ypos = ypos - pixely tE {M  
    +)WU:aKI  
            EnableTextPrinting( True ) \.O&-oi  
            Print i jq*`| m;Q  
            EnableTextPrinting( False ) =#[oi3k  
    dd<l;4(  
    Y 0Fq -H  
            For j = 0 To nx - 1 b^C27s  
    @-L]mLY  
                xpos = xpos + pixelx eh<mJL%T  
    ^}p##7t [  
                'shift source -5 PVWL\  
                LockOperationUpdates srcnode, True 'UWkJ2:!  
                GetOperation srcnode, 1, op 4F G0'J&hw  
                op.val1 = xpos vVw@^7U  
                op.val2 = ypos RPgz"-  
                SetOperation srcnode, 1, op tx>7?e8E  
                LockOperationUpdates srcnode, False K&`1{,  
    ;J TY#)Bh  
    raytrace |r Aot2  
                DeleteRays o}114X4q;  
                CreateSource srcnode p? o[+L<  
                TraceExisting 'draw `3i>e<m~  
    F c5t,P  
                'radiometry 0>7Ij7\[8  
                For k = 0 To GetEntityCount()-1 }URdoTOvb  
                    If IsSurface( k ) Then gAdqZJR%]  
                        temp = AuxDataGetData( k, "temperature" ) "W%YsN0  
                        emiss = AuxDataGetData( k, "emissivity" ) r4X}U|s!0  
                        If ( temp <> 0 And emiss <> 0 ) Then =FhP$r*  
                            ProjSolidAngleByPi = GetSurfIncidentPower( k ) aMhVO(+FW  
                            frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) 0t^FM<7G  
                            irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi 5kTs7zJ^  
                        End If v { >3)$1  
    mLZ1u\ 7W  
                    End If h Fv{?v  
    }rfikm  
                Next k N=<`|I  
    6d6cZGS[:  
            Next j oC>J{z  
    O;<wD h)Yt  
        Next i !P=Cv=  
        EnableTextPrinting( True ) KoNu{TJ  
    s{'Sl{-Eu  
        'write out file { sC Ni  
        fullfilepath = CurDir() & "\" & fname G5/A {1sz&  
        Open fullfilepath For Output As #1 /ki-Tha  
        Print #1, "GRID " & nx & " " & ny MmjZq  
        Print #1, "1e+308" ^BA%]pe$I  
        Print #1, pixelx & " " & pixely FefroaJ:u  
        Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 )&j`5sSXcr  
    fF0i^E<  
        maxRow = nx - 1 [A84R04_%  
        maxCol = ny - 1 _P qq*  
        For rowNum = 0 To maxRow                    ' begin loop over rows (constant X) OLb s~ >VA  
                row = "" ~?ezd0  
            For colNum = maxCol To 0 Step -1            ' begin loop over columns (constant Y) 6(`N!]e*L  
                row = row & irrad(colNum,rowNum) & " "     ' append column data to row string 8eS(gKD  
            Next colNum                     ' end loop over columns ZgxB7zl//  
    >[;@ [4}  
                Print #1, row xjo`u:BH  
    HD=F2p  
        Next rowNum                         ' end loop over rows (O0Ry2u k  
        Close #1 '37 {$VHw  
    Mc@9ivwL#  
        Print "File written: " & fullfilepath ZDFq=)0C  
        Print "All done!!" O0qG 6a  
    End Sub =){ G  
    gA(npsUHI  
    在输出报告中,我们会看到脚本对光源的孔径和功率做了修改,并最终经过31次迭代,将所有的热成像数据以dat的格式放置于: }Kgi!$<aQx  
    jDY B*Y^F  
    U~: H>  
    找到Tools工具,点击Open plot files in 3D chart并找到该文件 1PwtzH .w  
      
    dw<i)P^   
    s0?'mC+p  
    打开后,选择二维平面图: rS BI'op  
    .pUB.l$)  
     
    分享到