切换到宽版
  • 广告投放
  • 稿件投递
  • 繁體中文
    • 2399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
    7377
    光币
    31026
    光券
    0
    只看楼主 正序阅读 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在探测器上,并显示其热成像图。 l!D}3jD  
    3#LlDC_WC  
    成像示意图
    Z@4Ar fl  
    首先我们建立十字元件命名为Target Vr3Zu{&2  
    lU8l}Ndz"  
    创建方法: ?>7[7(|  
    W: z6Koc0  
    面1 : Zu*F#s!tUI  
    面型:plane j*|VctM  
    材料:Air yuh *  
    孔径:X=1.5, Y=6,Z=0.075,形状选择Box owVX*&b{  
    &l}^iP'%!  
    2=*H 8'k  
    辅助数据: 1KU! tL  
    首先在第一行输入temperature :300K, ;YaQB#GK%  
    emissivity:0.1; tHU2/V:R  
    Ki;*u_4{  
    Akq2 d;  
    面2 : ) ;EBz  
    面型:plane 1.}d.t  
    材料:Air { a =#B)6  
    孔径:X=1.5, Y=6,Z=0.075,形状选择Box mVj9, q0  
    9Gvd&U  
    l[dK[4  
    位置坐标:绕Z轴旋转90度, sU=H&D99  
    =O~_Q-  
    w2?3wrP3  
    辅助数据: H%[eV8  
    Lc}y<=P@  
    首先在第一行输入temperature :300K,emissivity: 0.1; })'B<vq  
    i}cRi&2[  
    % aP!hy  
    Target 元件距离坐标原点-161mm; l5~os>  
    4VHn  \  
    u2tfF  
    单透镜参数设定:F=100, bend=0, 位置位于坐标原点 YX!iL6?~  
    T~-ycVc  
    t$`r4Lb9/  
    探测器参数设定: >>,e4s,  
    9[#pIPxNK  
    在菜单栏中选择Create/Element Primitive /plane aEB_#1  
    91/Q9xY  
    )7hqJa-V  
    )j6~Wy@4  
    n3WlZ!$  
    ::`HQ@^  
    元件半径为20mm*20,mm,距离坐标原点200mm。 !n`fTK<$  
    M*0]ai|;  
    光源创建: 7 W5@TWM  
     -uS!\  
    光源类型选择为任意平面,光源半角设定为15度。 Zj(AJ*r  
    x5pdS:  
    j/DzCcp7  
    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。 ;[ZEDF5H  
    @@f"%2ZR[  
    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。 yWmJ~/*lG  
    nkPh,X\N0  
    [+Iz@0q  
    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。 Q3'llOx  
    6bg ;q(*7  
    创建分析面: hW<%R]^|  
    PrqlTT}Px  
    Lj({[H7D!  
    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。 cZ,b?I"Q%  
    !|(-=2`  
    ROI7eU  
    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。 }CSDV9).S  
    &C_j\7Dq  
    FRED在探测器上穿过多个像素点迭代来创建热图 RH W]Z Pr<  
    X0HZH?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。 b! t0w{^w  
    将如下的代码放置在树形文件夹 Embedded Scripts, h4gXvPS&r  
    : $1?i)  
    G[PtkPSJ  
    打开后清空里面的内容,此脚本为通用脚本适用于一切可热成像的应用。 @?sRj&w  
    z(ONv#}p  
    绿色字体为说明文字, =jN.1}  
    .^`{1%  
    '#Language "WWB-COM" T=DbBy0-  
    'script for calculating thermal image map <_L,t 1H{  
    'edited rnp 4 november 2005 ~ah~cwmpS  
    LE Nq_@$  
    'declarations w{8xpAqm  
    Dim op As T_OPERATION DeVv4D:}@  
    Dim trm As T_TRIMVOLUME J3V= 46Yc  
    Dim irrad(32,32) As Double 'make consistent with sampling tAd%#:K  
    Dim temp As Double XSB"{H>&  
    Dim emiss As Double dlh)gp;  
    Dim fname As String, fullfilepath As String 5Pc;5 o0C  
    XT%nbh&y  
    'Option Explicit g{)dP!}  
    :LQYo'@yB  
    Sub Main  tU5zF.%  
        'USER INPUTS QW~E&B%  
        nx = 31 KAJi  
        ny = 31 1ba~SHi  
        numRays = 1000 !qQl@j O  
        minWave = 7    'microns 1t~G|zhX  
        maxWave = 11   'microns WDYeOtc  
        sigma = 5.67e-14 'watts/mm^2/deg k^4 C[AqFo  
        fname = "teapotimage.dat" ! I:%0D  
    9<?M8_  
        Print "" oH?b}T=9jz  
        Print "THERMAL IMAGE CALCULATION" bHnT6Icom  
    $99n&t$Y  
        detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 }"H,h)T  
    qBQ?HLK-  
        Print "found detector array at node " & detnode 3pROf#M  
    &m7]v,&  
        srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 i^&~?2  
    <$$yw=ef  
        Print "found differential detector area at node " & srcnode $rBq"u=,0+  
    2a)xTA#  
        GetTrimVolume detnode, trm Lg+Ac5y}`  
        detx = trm.xSemiApe F,F4nw<W  
        dety = trm.ySemiApe pU}(@oy  
        area = 4 * detx * dety 7F7 {)L  
        Print "detector array semiaperture dimensions are " & detx & " by " & dety s c,Hq\$&  
        Print "sampling is " & nx & " by " & ny iuW[`ou X  
    Q8tL[>Xt  
        'reset differential detector area dimensions to be consistent with sampling U}[d_f  
        pixelx = 2 * detx / nx H2\;%K 2  
        pixely = 2 * dety / ny |A~jsz6pI  
        SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False ^/>(6>S^M  
        Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 f}ji?p  
    d"mkL-  
        'reset the source power n,(sBOQ  
        SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) %(#y 5yJ]  
        Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" i>A s;*  
    {6|G@ ""O  
        'zero out irradiance array gCS<iBT(7  
        For i = 0 To ny - 1 myQagqRx  
            For j = 0 To nx - 1 D/xbF`  
                irrad(i,j) = 0.0 #Y`~(K47  
            Next j Fnv;^}\z  
        Next i (`>+zT5aH  
    %lhEM}Sm  
        'main loop \ a<h/4#|  
        EnableTextPrinting( False ) Qj.#)R  
    @V sG'  
        ypos =  dety + pixely / 2 .V/Rfq  
        For i = 0 To ny - 1 A RuA<vQ  
            xpos = -detx - pixelx / 2 286;=rN]*  
            ypos = ypos - pixely bHYy}weZ  
    Yui3+}Ms  
            EnableTextPrinting( True ) hbDXo:  
            Print i iL&fgF"'  
            EnableTextPrinting( False ) O, wJR  
    .t-4o<7 3  
    WRbj01v  
            For j = 0 To nx - 1 Tbih+# ?  
    $y&E(J  
                xpos = xpos + pixelx +F` S>U  
    ;-lXU0}&  
                'shift source Wx}8T[A}  
                LockOperationUpdates srcnode, True .Iw AK/QS  
                GetOperation srcnode, 1, op Ecefi pG  
                op.val1 = xpos @Zu5VpJ  
                op.val2 = ypos w~A{(- dx  
                SetOperation srcnode, 1, op YeL#jtC  
                LockOperationUpdates srcnode, False BWa,f8  
    X6X $Pve  
    raytrace QB uMJm  
                DeleteRays |Q6.299  
                CreateSource srcnode _\G"9,)u '  
                TraceExisting 'draw }Yzco52  
    I\{ 1u  
                'radiometry Q5`*3h6p=  
                For k = 0 To GetEntityCount()-1 ~{g [<Qi  
                    If IsSurface( k ) Then @7]yl&LZ  
                        temp = AuxDataGetData( k, "temperature" ) 5E;qM|Ns  
                        emiss = AuxDataGetData( k, "emissivity" ) - t'jNR'  
                        If ( temp <> 0 And emiss <> 0 ) Then xb~yM%*c  
                            ProjSolidAngleByPi = GetSurfIncidentPower( k ) )e+>w=t  
                            frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) Y0@"fU35  
                            irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi 4N_R:B-V u  
                        End If HGs $*  
    85:=4N%  
                    End If DDP/DD;n}r  
    TH&U j1  
                Next k u(>^3PJ+  
    rk2j#>l$4  
            Next j 2d #1=+V  
    <I\/n<*  
        Next i kR-SE5`Jk  
        EnableTextPrinting( True ) 5|j<`()H :  
    <4si/=  
        'write out file fI}to&qk  
        fullfilepath = CurDir() & "\" & fname 36Zf^cFJ  
        Open fullfilepath For Output As #1 ^e_hLX\SW  
        Print #1, "GRID " & nx & " " & ny feDlH[$  
        Print #1, "1e+308" |O|V-f{l  
        Print #1, pixelx & " " & pixely ]Kt6^|S$a  
        Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 {0wIR_dGX  
    O|{d[eX  
        maxRow = nx - 1 4K#>f4(U`g  
        maxCol = ny - 1 5h=}j  
        For rowNum = 0 To maxRow                    ' begin loop over rows (constant X) .+3g*Dv{&  
                row = "" Q:G4Z9Kt  
            For colNum = maxCol To 0 Step -1            ' begin loop over columns (constant Y) qs6]-  
                row = row & irrad(colNum,rowNum) & " "     ' append column data to row string :Uzm  
            Next colNum                     ' end loop over columns D rUO-  
    RUnSCOdX  
                Print #1, row d9f C<Tp  
    I(L,8n5  
        Next rowNum                         ' end loop over rows 0WW2i{7`U  
        Close #1 }(J}f)  
    rxvx  
        Print "File written: " & fullfilepath {tuYs:  
        Print "All done!!" h6D<go-b56  
    End Sub kzQ+j8.,U  
    8oy^Xc+  
    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: 3=P]x ;[ba  
    45@ I*`  
    u"cV%(#  
    找到Tools工具,点击Open plot files in 3D chart并找到该文件 +K:Dx!9  
      
    N]Y d9tn{  
    y*jp79G  
    打开后,选择二维平面图: T= y}y  
    vAF "n  
     
    分享到