切换到宽版
  • 广告投放
  • 稿件投递
  • 繁體中文
    • 1584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
    6429
    光币
    26290
    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。 Pe<VPf9+  
    A5nggg4  
    成像示意图
    j_<qnBeQ  
    首先我们建立十字元件命名为Target UarLxPQ  
    |Y3w6!$  
    创建方法: *w0!C:mL&  
    orjtwF>^  
    面1 : ]0UYxv%]  
    面型:plane JSL&` `  
    材料:Air '{ <RX  
    孔径:X=1.5, Y=6,Z=0.075,形状选择Box $Cz2b/O  
    hF'VqJS  
    !)bZ.1o  
    辅助数据: ?UsCSJ1V  
    首先在第一行输入temperature :300K, )LGVR 3#  
    emissivity:0.1; 5]&sXs  
    "rB B&l  
    coXg]bUKo  
    面2 : JwI99I'  
    面型:plane |dR}S!fmG  
    材料:Air \,13mB6  
    孔径:X=1.5, Y=6,Z=0.075,形状选择Box (OiV IH  
    wUaWF$~y  
    f&<+45JI  
    位置坐标:绕Z轴旋转90度, TtkHMPlm_  
    "^&H9.z,v  
    {Z2nc)|7C  
    辅助数据: t oGiG|L  
    iq' PeVo  
    首先在第一行输入temperature :300K,emissivity: 0.1; +jhzE%  
    n.g-%4\q  
    %`i*SF(gV  
    Target 元件距离坐标原点-161mm; ]N 9N][n  
    "qgwuWbM  
    |%|03}Q  
    单透镜参数设定:F=100, bend=0, 位置位于坐标原点 k2 Ju*W&  
    $b`nV4p  
    t+v %%N_  
    探测器参数设定: ==Egy:<:Q  
    G2|jS@L#  
    在菜单栏中选择Create/Element Primitive /plane xt}.0dC!/%  
    %SC Jmn2  
    SZH`-xb!+5  
    3CD#OCz7&  
    '8]p]#l  
    CHGa_  
    元件半径为20mm*20,mm,距离坐标原点200mm。 z)M#9oAM  
    t`B@01;8A  
    光源创建: *v%y;^{k[/  
    ~61b^L}$  
    光源类型选择为任意平面,光源半角设定为15度。 X,G<D}  
    4x6n,:;  
    t*hy"e{*a  
    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。 !=eNr<:V.  
    4'z)J1M  
    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 u\Cf@}5(  
    Xf4~e(O  
    jJIP $  
    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。 D% jGK  
    L2>e@p\>  
    创建分析面: !JXiTI!  
    (tYZq86`  
    1 tOslP@  
    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。 Q0(6n8i  
    m\qeYI6,Z  
    B>nj{W<o  
    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。 6FzB-],  
    [2-n*a(q  
    FRED在探测器上穿过多个像素点迭代来创建热图 KRL.TLgq)  
    ?Kgb-bXB  
    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。 lWYp  
    将如下的代码放置在树形文件夹 Embedded Scripts, :|n[zjK/S  
    'S3<' X  
    X.>=&~[  
    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。 *b>RUESF  
    c*rH^Nz  
    绿色字体为说明文字, :&wb+tV  
    6C VH)=%  
    '#Language "WWB-COM" ?JZ$M  
    'script for calculating thermal image map ;j%I1k%A  
    'edited rnp 4 november 2005 2]vTedSOl  
    9:p-F+  
    'declarations P7F"#R0QB  
    Dim op As T_OPERATION 5TJd9:\Af  
    Dim trm As T_TRIMVOLUME estiS  
    Dim irrad(32,32) As Double 'make consistent with sampling by<@\n2B:U  
    Dim temp As Double ?=9'?K/~a  
    Dim emiss As Double |OJWQU![by  
    Dim fname As String, fullfilepath As String v82wnP-~7  
    X8ulaa  
    'Option Explicit ZGZNZ}~#  
    8</wQ6&|  
    Sub Main -Fd&rq:GB(  
        'USER INPUTS :V.@:x>id  
        nx = 31 |^l_F1+w  
        ny = 31 mcQL>7ts  
        numRays = 1000 l(NQk> w  
        minWave = 7    'microns }O*`I(  
        maxWave = 11   'microns qS\#MMsTd  
        sigma = 5.67e-14 'watts/mm^2/deg k^4 '$OUe {j<  
        fname = "teapotimage.dat" 3'.@aMA@  
    J- S.m(  
        Print "" }T4|Kyu?  
        Print "THERMAL IMAGE CALCULATION" N#l2wT  
    67iI wY*8'  
        detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 .yy-jf/  
    ~Fuq{e9`  
        Print "found detector array at node " & detnode D#LV&4e>.E  
    l$/pp  
        srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 2yK">xYY@  
    Y]SF0:v!n  
        Print "found differential detector area at node " & srcnode  ;v.[aq  
    wNHn.  
        GetTrimVolume detnode, trm tQ{/9bN?P  
        detx = trm.xSemiApe bvtpqI QZ  
        dety = trm.ySemiApe o=YOn&@%  
        area = 4 * detx * dety {[2o  
        Print "detector array semiaperture dimensions are " & detx & " by " & dety ]QaKXg)3q  
        Print "sampling is " & nx & " by " & ny >S I'Q7k  
    gNEcE9y 2  
        'reset differential detector area dimensions to be consistent with sampling :rL%,o"  
        pixelx = 2 * detx / nx #`u}#(  
        pixely = 2 * dety / ny _4N.]jr5  
        SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False bKpy?5&>  
        Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 ~`AB-0t.u  
    /Q3>w-h  
        'reset the source power <}J !_$A  
        SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) {T-\BTh&Q  
        Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" _uO$=4Sd  
    6axxyh%  
        'zero out irradiance array :dt[ #  
        For i = 0 To ny - 1 Y]([K.I=  
            For j = 0 To nx - 1 -LiGO#U  
                irrad(i,j) = 0.0 jUm-!SK}q  
            Next j Hi09?AX  
        Next i  57q=  
    Q|)>9m!tt  
        'main loop !}!KT(% %  
        EnableTextPrinting( False ) 'o IE:#b  
    DDr\Kv)k(  
        ypos =  dety + pixely / 2 )5b_>Uy  
        For i = 0 To ny - 1 X_2N9$},  
            xpos = -detx - pixelx / 2 fv7VDo8vb  
            ypos = ypos - pixely 4fKvB@O@.  
    9}6_B|  
            EnableTextPrinting( True ) NIQ}A-b  
            Print i @SD XJJ h  
            EnableTextPrinting( False ) Rmw=~NP5  
    A1p~K*[[  
    nG'Yo8I^5  
            For j = 0 To nx - 1 5$ =[x!x  
    Ixn|BCi60A  
                xpos = xpos + pixelx i?/Q7D<P  
    9&* 7+!  
                'shift source Sl8+A+  
                LockOperationUpdates srcnode, True  ]ltCJq  
                GetOperation srcnode, 1, op :Vxt2@p{  
                op.val1 = xpos sa+ JN^[X  
                op.val2 = ypos 1;/SXJ s  
                SetOperation srcnode, 1, op ^(TCUY~f&  
                LockOperationUpdates srcnode, False lW c[Q1  
    )(]rUJ~+~A  
    raytrace pl>b 6 |  
                DeleteRays Gt*<Awn8  
                CreateSource srcnode 'b.jKkW7  
                TraceExisting 'draw Xgx/ubca0  
    q(qm3OxYo  
                'radiometry W_wC"?A%  
                For k = 0 To GetEntityCount()-1 iOZ9A~Ywy  
                    If IsSurface( k ) Then Kk}, PU=  
                        temp = AuxDataGetData( k, "temperature" ) K.yc[z)un  
                        emiss = AuxDataGetData( k, "emissivity" ) W$jRS  
                        If ( temp <> 0 And emiss <> 0 ) Then ]izHn;+  
                            ProjSolidAngleByPi = GetSurfIncidentPower( k ) D]E=0+  
                            frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) bR7tmJ[)Z  
                            irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi _qE9]mU  
                        End If d[?RL&hJO  
    O + aK#eF  
                    End If Tp-W/YC  
    N[Xm5J  
                Next k ,u|>%@h  
    |$/#,Dv7  
            Next j #v(As) 4^  
    -Cvd3%Jje  
        Next i 93n%:?l"<W  
        EnableTextPrinting( True ) sFZdj0tQ4  
    C5(XZscq  
        'write out file #Tc`W_-  
        fullfilepath = CurDir() & "\" & fname Y"t|0dO%b  
        Open fullfilepath For Output As #1 2(!W 9#]  
        Print #1, "GRID " & nx & " " & ny =EVB?k ,  
        Print #1, "1e+308" (tA[]ne2  
        Print #1, pixelx & " " & pixely EJ {vJZO  
        Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 C)m@/w  
    N=u( 3So  
        maxRow = nx - 1 jy~hLEt7  
        maxCol = ny - 1 cWnEp';.  
        For rowNum = 0 To maxRow                    ' begin loop over rows (constant X) }'vQUG u8z  
                row = "" 9=}#.W3.  
            For colNum = maxCol To 0 Step -1            ' begin loop over columns (constant Y) 1;m?:|6K{  
                row = row & irrad(colNum,rowNum) & " "     ' append column data to row string JVg}XwR  
            Next colNum                     ' end loop over columns kDJYEI9j>  
    =,*/Ph&  
                Print #1, row .K^gh$z!  
    9+(6 /<  
        Next rowNum                         ' end loop over rows B0RVtbK  
        Close #1 :JBt qpo2  
    YP!}Bf  
        Print "File written: " & fullfilepath GF@` ~im  
        Print "All done!!" ,MHK|8!  
    End Sub Eva&FHRTY  
    [GCaRk>b,  
    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: 6-$95.Y2  
    R,.qQF\*  
    : HU|BJ>  
    找到Tools工具,点击Open plot files in 3D chart并找到该文件 "uZ^zV`"  
      
    0XljFQ  
    <b~~X`Z  
    打开后,选择二维平面图: X r o5~G  
    &9gI?b8  
     
    分享到