切换到宽版
  • 广告投放
  • 稿件投递
  • 繁體中文
    • 1005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
    5979
    光币
    24048
    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。 .+h pxZ  
    WEAXqDjM  
    成像示意图
    S]O Hv6  
    首先我们建立十字元件命名为Target %tQ{Hf~  
    ^?[<!VBI  
    创建方法: N)WG~=Gi  
    4[0?F!%  
    面1 : 1Z8oN3  
    面型:plane aZ`ags ofk  
    材料:Air >Fk `h=Wd  
    孔径:X=1.5, Y=6,Z=0.075,形状选择Box Wb4{*~  
    gi@ji-10  
    wJ*-K-  
    辅助数据: #2ASzCe  
    首先在第一行输入temperature :300K, <W') ~o}  
    emissivity:0.1; z}&C(m:al  
    u@u.N2H.%  
    l{m~d!w`a  
    面2 : E9 q;>)}  
    面型:plane Am0C|(#Xm  
    材料:Air Ab<Ok\e5  
    孔径:X=1.5, Y=6,Z=0.075,形状选择Box Ltd?#HP  
    l5]oS? >y  
    bMOM`At>z  
    位置坐标:绕Z轴旋转90度, C-^%g [#  
    'oQP:*Btl3  
    f<altz_\q  
    辅助数据: 15o *r  
    mX.3R+t  
    首先在第一行输入temperature :300K,emissivity: 0.1; Mq lo:7 ^F  
    M2P@ &  
    yZ)aKwj%U  
    Target 元件距离坐标原点-161mm; VN-#R=D  
    7r[ %| :  
    GKujDx+h  
    单透镜参数设定:F=100, bend=0, 位置位于坐标原点 /uXRZ  
    <*Kh=v  
    Fxth> O`$  
    探测器参数设定: Y!1^@;)^  
    VIYksv   
    在菜单栏中选择Create/Element Primitive /plane G1;'nwf}  
    UQ.D!q  
    H@2"ove-uC  
    @f5@0A\0  
    ~d7Wjn$@  
    <+-Yh_D  
    元件半径为20mm*20,mm,距离坐标原点200mm。 %6IlE.*,  
    S|q!? /jqj  
    光源创建: ')u5l  
    _95}ifSVm  
    光源类型选择为任意平面,光源半角设定为15度。 ZkB6bji  
    {~p7*j^0  
    y LgKS8b  
    我们将光源设定在探测器位置上,具体的原理解释请见本章第二部分。 ',H$zA?i  
    )}Rfa}MD  
    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 $D/bU lFx  
    s@ 2 0#D  
    WE.$at{*h  
    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。 lsB9;I^+x  
    /K,|k EE'n  
    创建分析面: K(Q]&&<  
    O@r.>  
    kBy rhK5U  
    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。 hEv=T'*,K)  
    k'@7ZH  
    !]rETP_  
    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。 ]|,q|c,  
    r:c@17  
    FRED在探测器上穿过多个像素点迭代来创建热图 5@+4  
    . 0 s[{x  
    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。 hgweNRTh!  
    将如下的代码放置在树形文件夹 Embedded Scripts, kqKj7L  
    G`]v_`>  
    '?"t<$b  
    打开后清空里面的内容,此脚本为通用脚本适用于一切可热成像的应用。 UCn*UX  
    M5GY>3P$c  
    绿色字体为说明文字, Mw"xm9(Q  
    -?< Ww{  
    '#Language "WWB-COM" 1B)Y;hg6&  
    'script for calculating thermal image map w]>"'o{{  
    'edited rnp 4 november 2005 &W=V%t>Z  
    -{X<*P4p  
    'declarations [3O^0-:6E  
    Dim op As T_OPERATION r]A" Og_U  
    Dim trm As T_TRIMVOLUME 1~}m.ER  
    Dim irrad(32,32) As Double 'make consistent with sampling .:}.b"%m  
    Dim temp As Double <y@,3DD3A9  
    Dim emiss As Double M{`/f@z(  
    Dim fname As String, fullfilepath As String -O|&c9W.O  
    /> ^@ O  
    'Option Explicit -1qZqU$h  
    d"#gO,H0  
    Sub Main wYZT D*A2h  
        'USER INPUTS Z?m -&%  
        nx = 31 x|]\1sb"  
        ny = 31 \Sg<='/{L;  
        numRays = 1000 >qR7'QwP  
        minWave = 7    'microns 81~Kpx  
        maxWave = 11   'microns  t?gJNOV  
        sigma = 5.67e-14 'watts/mm^2/deg k^4 }$o*  
        fname = "teapotimage.dat" L2KG0i`+  
    Aj [?aL  
        Print "" x&'o ]Y  
        Print "THERMAL IMAGE CALCULATION" rkkU"l$v  
    <lUOJV{&\  
        detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 K&*iw`  
    YRPm^kW  
        Print "found detector array at node " & detnode g%ubvu2t]  
    `>s7M.|X  
        srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 Mtm/}I  
    d')-7C  
        Print "found differential detector area at node " & srcnode ][,4,?T7  
    0o;O`/x  
        GetTrimVolume detnode, trm >&OUGu|  
        detx = trm.xSemiApe zrs<#8!Y_!  
        dety = trm.ySemiApe -T7%dLHY  
        area = 4 * detx * dety } ^i b  
        Print "detector array semiaperture dimensions are " & detx & " by " & dety Y2C9(Zk U  
        Print "sampling is " & nx & " by " & ny Ur^j$B}  
    Wqra8u#  
        'reset differential detector area dimensions to be consistent with sampling D==Mb~  
        pixelx = 2 * detx / nx $J.T$0pFa  
        pixely = 2 * dety / ny ,_D" ?o  
        SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False 1G;8MPU  
        Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 V >Hf9sZ  
    l?/Y  
        'reset the source power RW_q~bA9  
        SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) 4,G w#@  
        Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" ][d,l\gu+s  
    |9Yi7.  
        'zero out irradiance array n,j$D62[  
        For i = 0 To ny - 1 &.Q8Mi aT  
            For j = 0 To nx - 1 ;;Ds  
                irrad(i,j) = 0.0 :m'+tGs  
            Next j NOt@M  
        Next i ~9=aT1S|  
    @*MC/fe  
        'main loop #z!^ <,  
        EnableTextPrinting( False ) Jq ]:<TQ  
    V-!"%fO.s  
        ypos =  dety + pixely / 2 DNkWOY#{  
        For i = 0 To ny - 1 ;n6b%,s  
            xpos = -detx - pixelx / 2 93O;+Z5J  
            ypos = ypos - pixely 8FkFM^\1L  
    -n5 B)uw=  
            EnableTextPrinting( True ) ' GG=Ebt  
            Print i l4y{m#/  
            EnableTextPrinting( False ) {/<6v. v  
    QHt4",Ij  
    _qXa=|}V.  
            For j = 0 To nx - 1 bEV<iZDq%  
    !xIm2+:(  
                xpos = xpos + pixelx ]i*](UQ  
    " =] -%B  
                'shift source sJ z@7.  
                LockOperationUpdates srcnode, True h*B|fy4K9U  
                GetOperation srcnode, 1, op o>/O++7Ra  
                op.val1 = xpos ,m=4@ofX  
                op.val2 = ypos  j2l55@  
                SetOperation srcnode, 1, op A"5z6A4WB  
                LockOperationUpdates srcnode, False Mg,:UC:  
    k n[Y   
    raytrace NS)}6OI3~"  
                DeleteRays I zbU)ud  
                CreateSource srcnode 6 15s5ZA  
                TraceExisting 'draw 6]zd.W  
    P|tNL}2`;  
                'radiometry iJ' xh n  
                For k = 0 To GetEntityCount()-1 >gwz,{  
                    If IsSurface( k ) Then u]+~VT1C,3  
                        temp = AuxDataGetData( k, "temperature" ) Cv ejb+  
                        emiss = AuxDataGetData( k, "emissivity" ) C;QAT  
                        If ( temp <> 0 And emiss <> 0 ) Then -x8nQ%X  
                            ProjSolidAngleByPi = GetSurfIncidentPower( k ) {j5e9pg1L|  
                            frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) Z+j\a5d?,  
                            irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi h_1T,f (  
                        End If km^^T_ M/  
    Z[\ O=1E,  
                    End If I1oje0$  
    Uw,2}yR  
                Next k G7--v,R1x  
    wn_b[tdxq  
            Next j >9RD_QG7  
    p~noM/*2r  
        Next i t#%R q  
        EnableTextPrinting( True ) %sHF-n5P  
    k+I}PuG  
        'write out file H$G0`LP0/a  
        fullfilepath = CurDir() & "\" & fname (b'B%rFO  
        Open fullfilepath For Output As #1 *(PL _/:  
        Print #1, "GRID " & nx & " " & ny xss`Y,5?  
        Print #1, "1e+308" ,g%&|FAP  
        Print #1, pixelx & " " & pixely K\XH4kic  
        Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 `tjH<  
    p-1 3H0Kt  
        maxRow = nx - 1 \(t@1]&jw  
        maxCol = ny - 1 DJgTA]$&  
        For rowNum = 0 To maxRow                    ' begin loop over rows (constant X) )(y) A[  
                row = "" /-bO!RTwf  
            For colNum = maxCol To 0 Step -1            ' begin loop over columns (constant Y) rvr-XGK36\  
                row = row & irrad(colNum,rowNum) & " "     ' append column data to row string G7N| :YK  
            Next colNum                     ' end loop over columns =gcM%=*'  
    hWH:wB  
                Print #1, row +la2n(CAK  
    .BFYY13H  
        Next rowNum                         ' end loop over rows e["2QIOe  
        Close #1 F<!)4>2@  
    -?(E_^ng  
        Print "File written: " & fullfilepath bQ~j=\[r  
        Print "All done!!" ;vt8R=T  
    End Sub @:KJYm[  
    _x!7}O#k  
    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: xhRngHU\z<  
    )c8j}  
    :>+s0~  
    找到Tools工具,点击Open plot files in 3D chart并找到该文件 <n(*Xak{a  
      
    {#)0EzV6  
    ;pnD0bH  
    打开后,选择二维平面图: W^s ;Bi+Nw  
    ^$ t7+g  
     
    分享到