切换到宽版
  • 广告投放
  • 稿件投递
  • 繁體中文
    • 1917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。 -gS"pE^1  
    _%y4q%#  
    成像示意图
    DAdYg0efex  
    首先我们建立十字元件命名为Target -DP*q3  
    +4et7  
    创建方法: !:WW  
    X\Y}oa."A  
    面1 : V1B(|P  
    面型:plane P7:d ly[,q  
    材料:Air _;hf<|c  
    孔径:X=1.5, Y=6,Z=0.075,形状选择Box 3e%nA8?  
    mN*?%t  
    ;o0#(xVz  
    辅助数据: s~^}F+n  
    首先在第一行输入temperature :300K, m:uPEpcU  
    emissivity:0.1; [dB$U}SEj  
    k$N0lR4:p  
    Xc*U+M >U  
    面2 : u%3i0BajY  
    面型:plane yb2}_k.JG  
    材料:Air :^i^0dC  
    孔径:X=1.5, Y=6,Z=0.075,形状选择Box x5h~G  
    ,\YAnKn6_  
    d(-EcY>?  
    位置坐标:绕Z轴旋转90度, Y- )x Tn  
    1vnYogL   
    c6&Q^p|CF  
    辅助数据: Vi?q>:E:  
    =dZHYO^Cv  
    首先在第一行输入temperature :300K,emissivity: 0.1; Es!Q8.  
    aI3CNeav  
    tF7hFL5f  
    Target 元件距离坐标原点-161mm; xwi\  
    :>+\17tx  
    -MBV $:_R  
    单透镜参数设定:F=100, bend=0, 位置位于坐标原点 d%_OT0Ei  
    \]uV!)V5B  
    (UL4+ta  
    探测器参数设定: o*5U:'=5}  
    <lE?,jl  
    在菜单栏中选择Create/Element Primitive /plane 3B0PGvCI1  
    ,WD X(  
    GbI-SbE  
    c9wfsapJ  
    j$Ab>}g]  
    zmI]cD@G  
    元件半径为20mm*20,mm,距离坐标原点200mm。 k^\pU\J  
    i#/]KsSp  
    光源创建: - +> 1r  
    :|+Qe e  
    光源类型选择为任意平面,光源半角设定为15度。 S >yLqPp  
    $q$7^ r@  
    aNxAZMg  
    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。 58 bCUh#uw  
    GZip\S4Y  
    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 _oG&OJ@  
    x/!5K|c  
    q%Yn;g|_  
    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。 bD ^b  
    Hc^W%t~  
    创建分析面: *`_{  
    Hnk:K9u.B:  
    X5LBEOG  
    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。 bi[IqU!9  
    6eFp8bANN#  
    (o5j'2:.  
    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。 ,:LA.o}h  
    }%7 NF*  
    FRED在探测器上穿过多个像素点迭代来创建热图 @$9'@")  
    T*g:# ^4  
    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。 1y#D?R=E  
    将如下的代码放置在树形文件夹 Embedded Scripts, 6;'dUGvH  
    Gg Jf7ie4  
    f| _u7"OX  
    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。 t>=fTkB  
    _g%TSumvq<  
    绿色字体为说明文字, }}v9 `F  
    &>d:R_Q]  
    '#Language "WWB-COM" #7ohQrP  
    'script for calculating thermal image map a=cvCf  
    'edited rnp 4 november 2005 k:jSbbQ  
    tW WWx~k  
    'declarations hj'(*ND7z  
    Dim op As T_OPERATION &xRo^iV?  
    Dim trm As T_TRIMVOLUME Gx`Lks  
    Dim irrad(32,32) As Double 'make consistent with sampling *Kdda} J+  
    Dim temp As Double c\a_VRN>r  
    Dim emiss As Double >leU:7  
    Dim fname As String, fullfilepath As String /xtq_*I1S  
    [8tL"G6s  
    'Option Explicit WSuww  
    y;_% W  
    Sub Main i&{DOI%w  
        'USER INPUTS MxT-1&XL  
        nx = 31 p w8 s8?  
        ny = 31 ]a5 f2lE  
        numRays = 1000 C74a(Bk}H  
        minWave = 7    'microns o2<#s)GpY  
        maxWave = 11   'microns (=7Cs  
        sigma = 5.67e-14 'watts/mm^2/deg k^4 Z#rB}  
        fname = "teapotimage.dat" 6DH~dL_",%  
    &=VDASEu  
        Print "" sI{ M  
        Print "THERMAL IMAGE CALCULATION" qkiI/nH3  
    s"t$0cH9  
        detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 0PlO(" ,a  
    v`M3eh@$A  
        Print "found detector array at node " & detnode z`:lcF{V  
    %Dwk  
        srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 Y "/]|'p  
    o!)3?  
        Print "found differential detector area at node " & srcnode [VE8V-  
    +E{|63~q  
        GetTrimVolume detnode, trm I:mr}mv=i  
        detx = trm.xSemiApe Hy^N!rBxfO  
        dety = trm.ySemiApe 17`1SGZ  
        area = 4 * detx * dety ZIQ [bE7  
        Print "detector array semiaperture dimensions are " & detx & " by " & dety y&V@^ "`  
        Print "sampling is " & nx & " by " & ny =3L;Z[^9  
    ]*AR,0N&  
        'reset differential detector area dimensions to be consistent with sampling V#iPj'*   
        pixelx = 2 * detx / nx p6;OL@ \~  
        pixely = 2 * dety / ny r-Pkfy(  
        SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False r,h%[JKM  
        Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 /Njd[= B  
    [PDNwh0g5  
        'reset the source power ))"6ern  
        SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) 9b9$GyI  
        Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" XCBL}pNkR  
    "g1)f"pL  
        'zero out irradiance array O6LS(5j2  
        For i = 0 To ny - 1 7eAX*Kgt<_  
            For j = 0 To nx - 1 Eea*s'  
                irrad(i,j) = 0.0 sVOyT*GY  
            Next j G|!on<l&  
        Next i ]x(!&y:h  
    'h,VR=e<  
        'main loop EwvoQ$#jv  
        EnableTextPrinting( False ) c}2jmwq  
    ]GW]dM  
        ypos =  dety + pixely / 2 ivN&HAxI@  
        For i = 0 To ny - 1 ~5}* d  
            xpos = -detx - pixelx / 2 )8$=C#qC[  
            ypos = ypos - pixely sM `DL  
    ;EP:o%r  
            EnableTextPrinting( True ) <nT +$  
            Print i }khV'6"'|  
            EnableTextPrinting( False ) 5Ou`z5S\k  
    oYm[V<nIl  
    DK: o]~n  
            For j = 0 To nx - 1 Na]:_K5Dp  
    ddJe=PUb  
                xpos = xpos + pixelx <+?7H\b  
    GkQpELO:  
                'shift source ]H+8rY%+  
                LockOperationUpdates srcnode, True %D\[*  
                GetOperation srcnode, 1, op 7%x[q}  
                op.val1 = xpos /}b03  
                op.val2 = ypos n'E(y)9|  
                SetOperation srcnode, 1, op Bf~vA4  
                LockOperationUpdates srcnode, False r{L> F]Tw  
    %N>%!m  
    raytrace Lh!J >  
                DeleteRays S.-TOE  
                CreateSource srcnode C26>BU<  
                TraceExisting 'draw -"' j7t:  
    w"-Lc4t+  
                'radiometry 'h|DO/X~L  
                For k = 0 To GetEntityCount()-1 128EPK  
                    If IsSurface( k ) Then KBx6NU?;PO  
                        temp = AuxDataGetData( k, "temperature" ) ~j}cyHg  
                        emiss = AuxDataGetData( k, "emissivity" ) g| I6'K!<  
                        If ( temp <> 0 And emiss <> 0 ) Then :V RNs  
                            ProjSolidAngleByPi = GetSurfIncidentPower( k ) keL&b/@  
                            frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) v$?+MNks  
                            irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi mwHB(7YS,  
                        End If 8]/bK5`  
    Vc\MV0lr  
                    End If chM%]|gey  
    <Tzrj1"Q3  
                Next k Yg%I?  
    1 ySk;;3  
            Next j Vc&! OE  
    3no%E03p  
        Next i V5V bJBpf  
        EnableTextPrinting( True ) S9]'?|  
    cQCSe,$ W  
        'write out file 4i)1'{e  
        fullfilepath = CurDir() & "\" & fname I_} SB|  
        Open fullfilepath For Output As #1 %Nlt H/I  
        Print #1, "GRID " & nx & " " & ny ^c"jH'#.L  
        Print #1, "1e+308" [8 ]z|bM  
        Print #1, pixelx & " " & pixely xpV|\2C  
        Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 BC&S>#\  
    .o(fe\KHf  
        maxRow = nx - 1 wh$sn:J  
        maxCol = ny - 1 X( \ AB  
        For rowNum = 0 To maxRow                    ' begin loop over rows (constant X) LM~[@_j  
                row = "" qeVfE_<  
            For colNum = maxCol To 0 Step -1            ' begin loop over columns (constant Y) 4;e5H_}Oo  
                row = row & irrad(colNum,rowNum) & " "     ' append column data to row string md)c0Bg8~  
            Next colNum                     ' end loop over columns ^oBtfN>4  
    N.,X<G.H  
                Print #1, row {f3YsM;]C  
    4VJ-,Z  
        Next rowNum                         ' end loop over rows HVR /7&g  
        Close #1 Aza /6OL  
    s4X>.ToMC  
        Print "File written: " & fullfilepath i1ixi\P{0  
        Print "All done!!" T*Y~\~Jhu  
    End Sub Kr gFKRgGj  
    ~7*.6YnI  
    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: KKj a/p  
    \ub7`01  
    UOv+T8f=  
    找到Tools工具,点击Open plot files in 3D chart并找到该文件 '}ptj@,  
      
    > kG GR  
    JFcLv=U  
    打开后,选择二维平面图: S'Q@ScJ  
    Vz~{UHH6  
     
    分享到