切换到宽版
  • 广告投放
  • 稿件投递
  • 繁體中文
    • 1910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
    6613
    光币
    27214
    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。 0Nk!.gY  
    UpQda`rb  
    成像示意图
    ?vik2RW  
    首先我们建立十字元件命名为Target ,k@i Nid  
    t!FC)iY  
    创建方法: #'i,'h+F  
    &`]T# ">  
    面1 : :UKc:JVNM  
    面型:plane }U}ppq0Eo  
    材料:Air @L607[!?  
    孔径:X=1.5, Y=6,Z=0.075,形状选择Box '['x'G50  
    ]_!NmB_3  
    =yJV8%pa  
    辅助数据: d,'gh4C  
    首先在第一行输入temperature :300K, 2>CR]  
    emissivity:0.1; SFEDR?s   
    ]R09-s 0$7  
    5VVU%STP  
    面2 : uXA}" f2  
    面型:plane ~e]l  
    材料:Air Oq}7q!H  
    孔径:X=1.5, Y=6,Z=0.075,形状选择Box -" r4  
    AOqL&z  
    FId,/la  
    位置坐标:绕Z轴旋转90度, x'Nc}  
    egWfKL&iy  
    3^)c5kcI  
    辅助数据: uE%2kB*]  
    |@'K]$vZ*  
    首先在第一行输入temperature :300K,emissivity: 0.1; NUtKT~V  
    Z#kB+.U  
    %w!x \UV  
    Target 元件距离坐标原点-161mm; ( p CU:'"  
    e!k4Ij-]  
    [*H h6  
    单透镜参数设定:F=100, bend=0, 位置位于坐标原点 ^%U`|GBZp  
    Cs vwc%  
    =|c7#GaiF  
    探测器参数设定: pQ ul0]  
    f$?`50D"1  
    在菜单栏中选择Create/Element Primitive /plane &!+1GI9z  
    gEgd/Le  
    eQfXUpk3@I  
    u&f|z9  
    je%y9*V  
    aOUTKyR ~  
    元件半径为20mm*20,mm,距离坐标原点200mm。 Uw)B(;Hy?  
    SK@lr  
    光源创建: z4]z3U<}3]  
    I;{Ua *  
    光源类型选择为任意平面,光源半角设定为15度。 + =U9<8  
    |b!Bb<5  
    xHkxrXqeI  
    我们将光源设定在探测器位置上,具体的原理解释请见本章第二部分。 ?'tFTh  
    g/i.b&  
    我们在位置选项又设定一行的目的是通过脚本自动控制光源在探测器平面不同划分区域内不同位置处追迹光线 ,nUovWN07  
    zRR^v&.9K  
    =,s5>2  
    功率数值设定为:P=sin2(theta) theta为光源半角15度。我们为什么要这么设定,在第二部分会给出详细的公式推导。 u3jLe=Y'\  
    K@"B^f0mU  
    创建分析面: c'bh`H4  
    O? 7hT!{  
    BGstf4v>A<  
    到这里元件参数设定完成,现在我们设定元件的光学属性,在前面我们分别对第一和第二面设定的温度和发射系数,散射属性我们设定为黑朗伯,4%的散射。并分别赋予到面一和面二。 R@IwmJxX  
    zUWWXC%R  
    [a#*%H{OC  
    到此,所有的光学结构和属性设定完成,通过光线追迹我们可以查看光线是否可以穿过元件。 |A=~aQot  
    ^*,?x  
    FRED在探测器上穿过多个像素点迭代来创建热图 >5t]Zlb`  
    MJn=  
    FRED具有一个内置的可编译的Basic脚本语言。从Visual Basic脚本语言里,几乎所有用户图形界面(GUI)命令是可用这里的。FRED同样具有自动的客户端和服务器能力,它可以被调用和并调用其他可启动程序,如Excel。因此可以在探测器像素点上定义多个离轴光源,及在FRED Basic脚本语言里的For Next loops语句沿着探测器像素点向上和向下扫描来反向追迹光线,这样可以使用三维图表查看器(Tools/Open plot files in 3D chart)调用和查看数据。 h~=~csya:  
    将如下的代码放置在树形文件夹 Embedded Scripts, i`w&{WTRQ  
    0p*Oxsy  
    SU.$bsu  
    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。 wZj`V_3  
    e "Tr0k  
    绿色字体为说明文字, (J j'kW6G6  
    k+eeVy  
    '#Language "WWB-COM" h~Z:YY)4  
    'script for calculating thermal image map B\~(:(OPM]  
    'edited rnp 4 november 2005 IL%P\Zs  
    FJsM3|{2=d  
    'declarations IKp/xj[!  
    Dim op As T_OPERATION uJ3*AO  
    Dim trm As T_TRIMVOLUME ;"NW= P&  
    Dim irrad(32,32) As Double 'make consistent with sampling #V@vz#bo=  
    Dim temp As Double VF~kjH2>  
    Dim emiss As Double ypTH=]y  
    Dim fname As String, fullfilepath As String <4"Bb_U  
    h9&0"LHr  
    'Option Explicit T^2o' _:  
    @3?dI@i(  
    Sub Main `pd+as  
        'USER INPUTS suN}6C I  
        nx = 31 yM?jiy  
        ny = 31 P#,g5  
        numRays = 1000 l~x 6R~q  
        minWave = 7    'microns L,sXJ23.  
        maxWave = 11   'microns aBKJd  
        sigma = 5.67e-14 'watts/mm^2/deg k^4 YG#{/;^nm)  
        fname = "teapotimage.dat" 1L4v X  
    o4YF,c+>q  
        Print "" 6PLdzZ{  
        Print "THERMAL IMAGE CALCULATION" cu4|!s`#  
    Lv-M.  
        detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 fs, >X!l+  
    Co:Rg@i(F  
        Print "found detector array at node " & detnode 2bOFH6g  
    wqJ1^>TB  
        srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 S\@U3|Q5  
    A/~^4DR  
        Print "found differential detector area at node " & srcnode + ;B K|([#  
    %)y-BdSp.  
        GetTrimVolume detnode, trm ]q|U0(q9  
        detx = trm.xSemiApe J/c5)IB|  
        dety = trm.ySemiApe *>jJ<8!  
        area = 4 * detx * dety t#nRa Pzp  
        Print "detector array semiaperture dimensions are " & detx & " by " & dety cXt]55"  
        Print "sampling is " & nx & " by " & ny stq%Eg?  
    hhJs$c(  
        'reset differential detector area dimensions to be consistent with sampling W'Y#(N[ktP  
        pixelx = 2 * detx / nx KWn.  
        pixely = 2 * dety / ny B1J2m^  
        SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False e @|uG%  
        Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 ['aiNhlbt  
    *,Sa*-7(  
        'reset the source power mzn#4;m$  
        SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) dMa6hI{k  
        Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" ]KQBek#DD  
    eY(JU5{  
        'zero out irradiance array <1kK@m -E  
        For i = 0 To ny - 1 F>aaUj  
            For j = 0 To nx - 1 kp,$ NfD  
                irrad(i,j) = 0.0 i5czm?x  
            Next j lR5k1J1n  
        Next i +wm%`N;v<  
    ,BlNj^5f  
        'main loop &xS] ;Fr  
        EnableTextPrinting( False ) W9jxw4)  
    cTdX'5  
        ypos =  dety + pixely / 2 o AM)<#U>  
        For i = 0 To ny - 1 #M[%JTTn  
            xpos = -detx - pixelx / 2 LbnW(wr6:(  
            ypos = ypos - pixely  $kY ]HI  
    }%S#d&wh$_  
            EnableTextPrinting( True ) ;Lk07+3G  
            Print i 1-8 G2e  
            EnableTextPrinting( False ) 4u7^v1/  
    ]=(PtzVa  
    b4>1UZGW-  
            For j = 0 To nx - 1 Z (C0+A\  
    e0`5PVJ  
                xpos = xpos + pixelx LDj*~\vsq  
    8]l(D  
                'shift source 'E4}++\  
                LockOperationUpdates srcnode, True @ "/:Omh  
                GetOperation srcnode, 1, op c{})Z=  
                op.val1 = xpos Z4D[nPm$  
                op.val2 = ypos ]Tn""3#1g  
                SetOperation srcnode, 1, op kB_T9$0e#  
                LockOperationUpdates srcnode, False 6rN.)dL.#N  
    9+I /bl4  
    raytrace Ypx"<CKP}  
                DeleteRays 8]xYE19=  
                CreateSource srcnode i?'|}tK  
                TraceExisting 'draw ;AJ6I*O@+  
    8l >Xbz  
                'radiometry nc.:Wm6Mj  
                For k = 0 To GetEntityCount()-1 oGz5ZDa#  
                    If IsSurface( k ) Then Up\ k67  
                        temp = AuxDataGetData( k, "temperature" ) qR9!DQc'  
                        emiss = AuxDataGetData( k, "emissivity" ) @8 lT*O2j  
                        If ( temp <> 0 And emiss <> 0 ) Then @ [%K D  
                            ProjSolidAngleByPi = GetSurfIncidentPower( k ) *fQn!2}=(  
                            frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) y*#+:D]o*  
                            irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi TECp!`)j"  
                        End If 3?<LWrhV3  
    }hS$F  
                    End If *)s^+F 0  
    4z,/0  
                Next k F+ <Z%KuCu  
    4,?WNPqo  
            Next j %(:{TR  
    fY!9i5@'  
        Next i * 5(%'3  
        EnableTextPrinting( True ) Y {|is2M9'  
    n {..Q,z  
        'write out file [rReBgV  
        fullfilepath = CurDir() & "\" & fname Sn[/'V^$a  
        Open fullfilepath For Output As #1 @oQ"FLF.  
        Print #1, "GRID " & nx & " " & ny a.fdCI]%  
        Print #1, "1e+308" (9v%66y  
        Print #1, pixelx & " " & pixely Xx ou1l!  
        Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 <l<6W-I   
    | &/_{T  
        maxRow = nx - 1 #hXxrN  
        maxCol = ny - 1 cueaOtD  
        For rowNum = 0 To maxRow                    ' begin loop over rows (constant X) gPIl:, d(  
                row = "" t@q==VHF  
            For colNum = maxCol To 0 Step -1            ' begin loop over columns (constant Y) aq - |  
                row = row & irrad(colNum,rowNum) & " "     ' append column data to row string ?vQ:z{BO  
            Next colNum                     ' end loop over columns ?b\oM v5y  
    )Kq@ m1>@  
                Print #1, row HSEz20s  
    ku GaOO  
        Next rowNum                         ' end loop over rows i'[! 'HY  
        Close #1 =Jswd  
    Gyb|{G_  
        Print "File written: " & fullfilepath ~"r(PCa@  
        Print "All done!!" 3)hQT-)  
    End Sub 3zMaHh)mj  
    \6%`)p  
    在输出报告中,我们会看到脚本对光源的孔径和功率做了修改,并最终经过31次迭代,将所有的热成像数据以dat的格式放置于: I/go$@E"  
    Op:$7hv  
    %]N|?9L"=  
    找到Tools工具,点击Open plot files in 3D chart并找到该文件 +NVXFjPC  
      
    H{1'- wB  
    P<=1O WC  
    打开后,选择二维平面图: /ACau<U]t  
    6xx(o  
     
    分享到