切换到宽版
  • 广告投放
  • 稿件投递
  • 繁體中文
    • 899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
    5734
    光币
    22822
    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。 uF(k[[qaiN  
    '8`T|2   
    成像示意图
    /"AvOh*  
    首先我们建立十字元件命名为Target j\)H  
    x/TGp?\g  
    创建方法: w8M2N]&:  
    q|#MB7e/  
    面1 : _+QwREP  
    面型:plane ``4wX-y  
    材料:Air 9/TY\?U  
    孔径:X=1.5, Y=6,Z=0.075,形状选择Box Eek9|i"p  
    4I~i)EKy6  
    W|c.l{A5Q  
    辅助数据: <&#+ E%E4  
    首先在第一行输入temperature :300K, *K!++k!Ixa  
    emissivity:0.1; ~uaP$*B[  
    \P?ToTTV  
    hb^!LtF#Y  
    面2 : sOC&Q&eg  
    面型:plane Cw1( 5  
    材料:Air jz:gr=* z  
    孔径:X=1.5, Y=6,Z=0.075,形状选择Box iyM^[/-R6  
    |qUrEGjiSS  
    B4W\ t{  
    位置坐标:绕Z轴旋转90度, 3B9nP._  
    av'*u  
    5{l1A (b  
    辅助数据: (aKZ5>>cN  
    ZlR!s!vv  
    首先在第一行输入temperature :300K,emissivity: 0.1; S ~|.&0"\  
    T%I&txl  
    g()m/KS<  
    Target 元件距离坐标原点-161mm; tHI*,  
    D s-`  
    J/Q|uRpmqr  
    单透镜参数设定:F=100, bend=0, 位置位于坐标原点 Z;<ep@gy~  
    moO _-@i  
    LHi6:G"Y(  
    探测器参数设定: !WKk=ysFS  
    * BOBH;s  
    在菜单栏中选择Create/Element Primitive /plane )SiY(8y  
    {+=i?  
    $L{7%]7QC  
    iHz[Zw^.s  
    DP>mNE  
    g _ M-F  
    元件半径为20mm*20,mm,距离坐标原点200mm。 TETsg5#  
    0|C[-ppr  
    光源创建: 0j@IxEPs  
    T T"3^@  
    光源类型选择为任意平面,光源半角设定为15度。 i$O#%12l  
    QkX@QQ T?  
    V\zsDP  
    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。 N(R,8GF5G  
     c!D> {N  
    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 WEC-<fN|Y\  
    !#.vyBK#  
    %FS;>;i?  
    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。 MVAc8dS  
    7SHo%b A  
    创建分析面: r5)f82pQ  
    m|dF 30~A  
    Wf1-"Q  
    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。 0*{p Oe/u  
    ~~dfpW_"  
    yS"0/Rm}  
    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。 mh8nlB  
    EG1x  
    FRED在探测器上穿过多个像素点迭代来创建热图 qS82/e)7  
    S A3Y:(  
    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。 4`0;^K.  
    将如下的代码放置在树形文件夹 Embedded Scripts, f[M"EMy  
    ST4(|K  
    }q x(z^  
    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。 Bcm=G""  
    hGKdGu`0  
    绿色字体为说明文字, | VRq$^g  
    ;S =e%:zb  
    '#Language "WWB-COM" Y;PDZb K3  
    'script for calculating thermal image map faJ8zX  
    'edited rnp 4 november 2005 <M>#qd@c  
    h=mv9=x  
    'declarations -9i+@%{/  
    Dim op As T_OPERATION ;@O(z*14@  
    Dim trm As T_TRIMVOLUME Nuo<` 6mV@  
    Dim irrad(32,32) As Double 'make consistent with sampling lMPbLF%_  
    Dim temp As Double +{bh  
    Dim emiss As Double a!{hC)d*  
    Dim fname As String, fullfilepath As String N>T=L0`  
    vev8l\  
    'Option Explicit g&8.A(  
    {B v`i8e  
    Sub Main o}W7.7^2  
        'USER INPUTS Z~B+*HF  
        nx = 31 33S`aJ  
        ny = 31 4t(QvIydA  
        numRays = 1000 ";58B} ki  
        minWave = 7    'microns <#!8?o&i  
        maxWave = 11   'microns (N9`WuI  
        sigma = 5.67e-14 'watts/mm^2/deg k^4 :4b- sg#  
        fname = "teapotimage.dat" ;W =by2x*  
    f(W,m >.;  
        Print "" /XC;.dLA#  
        Print "THERMAL IMAGE CALCULATION" ^&e;8d|f{  
    @u7%B}q7:  
        detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 13]y)(  
    DOA[iT";4  
        Print "found detector array at node " & detnode $jDD0<F.#  
    ug>]U ~0  
        srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 ZW`HDrP`  
    ~c'\IM  
        Print "found differential detector area at node " & srcnode *GB$sXF  
    ook' u }h  
        GetTrimVolume detnode, trm qRWJ-T:!F  
        detx = trm.xSemiApe y0lLFe~  
        dety = trm.ySemiApe 1Z=;Uy\  
        area = 4 * detx * dety d u _O}x  
        Print "detector array semiaperture dimensions are " & detx & " by " & dety y;*My#  
        Print "sampling is " & nx & " by " & ny N>h]mX6  
    &7JEb]1C  
        'reset differential detector area dimensions to be consistent with sampling p` ^:Q*C"  
        pixelx = 2 * detx / nx nT(!HDH  
        pixely = 2 * dety / ny F5Cqv0H V  
        SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False k$Nx6?8E  
        Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 oKZ[0(4<  
    #zh6=.,7  
        'reset the source power 1 / F<T  
        SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) MX%|hIOpr  
        Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" 9iiU,}M`j  
    |v,}%UN2  
        'zero out irradiance array 4"`=huQ  
        For i = 0 To ny - 1 6uv'r;U]  
            For j = 0 To nx - 1 9} IVNZc  
                irrad(i,j) = 0.0 f4qS OVv  
            Next j \f ~u85  
        Next i b*9m2=6  
    #h}IUR  
        'main loop iGpK\oH  
        EnableTextPrinting( False ) x`b~ZSNJ%  
    ~QQEHx\4zZ  
        ypos =  dety + pixely / 2 `"-`D!U?$  
        For i = 0 To ny - 1 j@!BOL~?  
            xpos = -detx - pixelx / 2 CYY X\^hA  
            ypos = ypos - pixely m&;zLBA;  
    T= iZ9w  
            EnableTextPrinting( True ) loAfFK>g  
            Print i woC FN1W  
            EnableTextPrinting( False ) J?UZN^  
    +"*l2E]5  
    wt3Z?Pb  
            For j = 0 To nx - 1 ?ZD{e|:u  
    S0X.8Bq  
                xpos = xpos + pixelx Al;%u0]5  
    &eLQ;<qO*|  
                'shift source |R:v<  
                LockOperationUpdates srcnode, True xP|%rl4  
                GetOperation srcnode, 1, op ]-+.lR%vd9  
                op.val1 = xpos o>QFd x  
                op.val2 = ypos N23+1h  
                SetOperation srcnode, 1, op >"m@qkh  
                LockOperationUpdates srcnode, False Oa3=+_C~$1  
    96([V|5K  
    raytrace 9, sCJ5bb"  
                DeleteRays 3e!a>Gl*  
                CreateSource srcnode HquB*=^xh  
                TraceExisting 'draw e{#a{`?Uez  
    O_%PBgcJr  
                'radiometry : Oz7R:  
                For k = 0 To GetEntityCount()-1 av| 6r#  
                    If IsSurface( k ) Then ^`B##9g~  
                        temp = AuxDataGetData( k, "temperature" ) /oix tO)  
                        emiss = AuxDataGetData( k, "emissivity" ) 8M(|{~~3:  
                        If ( temp <> 0 And emiss <> 0 ) Then +p%5/ smfs  
                            ProjSolidAngleByPi = GetSurfIncidentPower( k ) 1zEZ\G  
                            frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) nP3;<*T P0  
                            irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi CzDR%vx  
                        End If SBYMDKZ  
    N4JqW  
                    End If dOYmt,  
    Ty,)mx){)  
                Next k 0;m$a=  
    4q 2=:"z4  
            Next j 4jyr\=42F'  
    \w@_(4")Qb  
        Next i ;JD3tM<  
        EnableTextPrinting( True ) M& BM,~  
    yADN_  
        'write out file ,VcD vZ7  
        fullfilepath = CurDir() & "\" & fname .]sIoB-54  
        Open fullfilepath For Output As #1 PU/Br;2A  
        Print #1, "GRID " & nx & " " & ny po](6V  
        Print #1, "1e+308" /B#lju!  
        Print #1, pixelx & " " & pixely O|7{%5h  
        Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 (8eNZ*+mO  
    ws=9u-  
        maxRow = nx - 1 i[BR(D&l_p  
        maxCol = ny - 1 g,GbaaXH  
        For rowNum = 0 To maxRow                    ' begin loop over rows (constant X) l!2Z`D_MD  
                row = "" 6/WK((Fd  
            For colNum = maxCol To 0 Step -1            ' begin loop over columns (constant Y) Pk?%PB ?Z  
                row = row & irrad(colNum,rowNum) & " "     ' append column data to row string SYW= L  
            Next colNum                     ' end loop over columns $rQFM[  
    qer'V  
                Print #1, row j7HlvoZV  
    }+RF~~H/  
        Next rowNum                         ' end loop over rows LK-6z w5=(  
        Close #1 _*?"[TYfX  
    }.|5S+J?[  
        Print "File written: " & fullfilepath g KmRjK  
        Print "All done!!" elHarey`f  
    End Sub 2;(iTPz +  
    !7a^8   
    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: E<G@LT  
    Sph"w08  
    P+%)0*W  
    找到Tools工具,点击Open plot files in 3D chart并找到该文件 Z6/~2S@  
      
    dK(%u9v  
    `6/Yf@b  
    打开后,选择二维平面图: +(P 43XO08  
    (>5VS  
     
    分享到