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    [分享]十字元件热成像分析 [复制链接]

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    离线infotek
     
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    只看楼主 倒序阅读 楼主  发表于: 2020-11-18
    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。 65`'Upu  
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    成像示意图
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    首先我们建立十字元件命名为Target p?`|CE@h7  
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    创建方法: w or'=byh\  
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    面1 : WNlSve)]ie  
    面型:plane @,>=X:7  
    材料:Air Cak/#1  
    孔径:X=1.5, Y=6,Z=0.075,形状选择Box yM#trqv5  
    NE>JtTF<  
     KHs{/  
    辅助数据: *a0I  Z  
    首先在第一行输入temperature :300K, Mpl,}Q!c  
    emissivity:0.1; JjTzq2'%  
    J-%PyvK$?  
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    面2 : )]>Y*<s }  
    面型:plane %_J/&{6G  
    材料:Air $j4?'-i=e  
    孔径:X=1.5, Y=6,Z=0.075,形状选择Box <"|<)BGeI  
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    位置坐标:绕Z轴旋转90度, WSB|-Qj}W  
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    辅助数据: 2T2#HP  
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    首先在第一行输入temperature :300K,emissivity: 0.1; fdEj#Ux<H  
    qx<zX\qI6n  
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    Target 元件距离坐标原点-161mm; UmI@":|-  
    qA_DQ):  
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    单透镜参数设定:F=100, bend=0, 位置位于坐标原点 HE<%d  
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    探测器参数设定: )mZy>45  
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    在菜单栏中选择Create/Element Primitive /plane g8 *|" {  
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    元件半径为20mm*20,mm,距离坐标原点200mm。 =ir;m  
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    光源创建:  KNyD}1  
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    光源类型选择为任意平面,光源半角设定为15度。 }Ml z\'{  
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    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。 9- <V%eNX  
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    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 w`Aw+[24  
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    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。 b,V=B{(~  
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    创建分析面: IIEU{},}z  
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    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。 aRKG)0=  
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    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。 cG"<*Xi<  
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    FRED在探测器上穿过多个像素点迭代来创建热图 *iN]#)3>  
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    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。 Gjh7cm>  
    将如下的代码放置在树形文件夹 Embedded Scripts, juZ3""  
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    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。 EqU[mqeF  
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    绿色字体为说明文字, 'V{k$}P2  
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    '#Language "WWB-COM" 4T^WRS  
    'script for calculating thermal image map P@? '@.e  
    'edited rnp 4 november 2005 kpUU'7Q  
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    'declarations z,P7b]KVe  
    Dim op As T_OPERATION wZb@VG}%  
    Dim trm As T_TRIMVOLUME PKG ,4v=  
    Dim irrad(32,32) As Double 'make consistent with sampling q &o=4  
    Dim temp As Double xf SvvCy  
    Dim emiss As Double gJv^v`X  
    Dim fname As String, fullfilepath As String Vjd =F.V+  
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    'Option Explicit 'gH#\he[Dh  
    ?P]md9$(+e  
    Sub Main kniMXeiu  
        'USER INPUTS p7tC~]r:L  
        nx = 31 eci\Q,   
        ny = 31 g >oLc6T  
        numRays = 1000 "MN'%"/  
        minWave = 7    'microns Agf!6kh  
        maxWave = 11   'microns U#4W"1~iX  
        sigma = 5.67e-14 'watts/mm^2/deg k^4 =w>QG{-N  
        fname = "teapotimage.dat" /q]@|5I  
    FX 3[U+  
        Print "" K`<P^XJr  
        Print "THERMAL IMAGE CALCULATION" L+CSF ]  
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        detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 y}`%I&]n  
    Ymvd= F   
        Print "found detector array at node " & detnode bhYaG i0  
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        srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 *k$&Hcr$  
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        Print "found differential detector area at node " & srcnode _v,n~a}&  
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        GetTrimVolume detnode, trm LlqhZetS  
        detx = trm.xSemiApe DdgFBO  
        dety = trm.ySemiApe Q4*cL5j  
        area = 4 * detx * dety UW3F)  
        Print "detector array semiaperture dimensions are " & detx & " by " & dety )]R8 $S  
        Print "sampling is " & nx & " by " & ny D bJ(N h  
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        'reset differential detector area dimensions to be consistent with sampling }J`Gm  
        pixelx = 2 * detx / nx 2XpGgG`2`C  
        pixely = 2 * dety / ny ".4^?d_^VF  
        SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False g!uhy}  
        Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 10 ^=1@U  
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        'reset the source power v\C+G[MV 7  
        SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) }S4Fy3)  
        Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" {HeMdGn9  
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        'zero out irradiance array P/ 5r(l5  
        For i = 0 To ny - 1 #'P&L>6 ;  
            For j = 0 To nx - 1 _6( =0::x  
                irrad(i,j) = 0.0 #oI`j q  
            Next j v\vn}/>*d  
        Next i :08UeEy  
    V ALYA=w/  
        'main loop mx2 Jt1  
        EnableTextPrinting( False ) }$ der  
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        ypos =  dety + pixely / 2 b3H;Ea?^^<  
        For i = 0 To ny - 1 s~CA @  
            xpos = -detx - pixelx / 2 BlCKJp{m$  
            ypos = ypos - pixely HZNX1aQ|Q#  
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            EnableTextPrinting( True ) t{9Ph]e  
            Print i X+iULr.^`~  
            EnableTextPrinting( False ) -_+0[Nb.  
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            For j = 0 To nx - 1 2Xosj(H  
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                xpos = xpos + pixelx Qi M>59[  
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                'shift source  NNX/2  
                LockOperationUpdates srcnode, True =*pu+o,?  
                GetOperation srcnode, 1, op IftPN6(Z  
                op.val1 = xpos H;8(y4;  
                op.val2 = ypos SWt"QqBU  
                SetOperation srcnode, 1, op We|*s2!  
                LockOperationUpdates srcnode, False O1A*-G:X  
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                'raytrace @gd-lcMYW  
                DeleteRays 9Bn dbS i  
                CreateSource srcnode eF9LZ"-s  
                TraceExisting 'draw lU?"\m  
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                'radiometry b\?`721BG  
                For k = 0 To GetEntityCount()-1 ^VQiq7 xm  
                    If IsSurface( k ) Then u4Sa4o  
                        temp = AuxDataGetData( k, "temperature" ) iZ UBw  
                        emiss = AuxDataGetData( k, "emissivity" ) S $Wd}2>  
                        If ( temp <> 0 And emiss <> 0 ) Then 8^T' a^Wt  
                            ProjSolidAngleByPi = GetSurfIncidentPower( k ) h W-[omr0  
                            frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) j>U.(K  
                            irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi <"-sN  
                        End If b$BUo8O}  
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                    End If A /MOY@%G  
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                Next k OA8pao~H  
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            Next j eWFlJ;=  
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        Next i 8/=2N  
        EnableTextPrinting( True ) =LC5o2bLy  
    '{|87kI  
        'write out file ?h5Y^}8Qg  
        fullfilepath = CurDir() & "\" & fname m+L:\mvA  
        Open fullfilepath For Output As #1 )}EwEM  
        Print #1, "GRID " & nx & " " & ny 7M4iBk4I  
        Print #1, "1e+308" 90q*V%cS  
        Print #1, pixelx & " " & pixely up`6IWlLE  
        Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 OSBE5  
    tlW}lN}  
        maxRow = nx - 1 tIg_cY_y  
        maxCol = ny - 1 U_:/>8})d  
        For rowNum = 0 To maxRow                    ' begin loop over rows (constant X) $wBUu   
                row = "" 7':|f"  
            For colNum = maxCol To 0 Step -1            ' begin loop over columns (constant Y) iaMZ37  
                row = row & irrad(colNum,rowNum) & " "     ' append column data to row string f}fM%0/5  
            Next colNum                     ' end loop over columns ]UNmhF!W>u  
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                Print #1, row wBr0s *1I  
     ;HW@ZI  
        Next rowNum                         ' end loop over rows Ft07>E$/Q^  
        Close #1 //`X+[bMG  
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        Print "File written: " & fullfilepath |{$Vk%cUE  
        Print "All done!!" $(GXlhA  
    End Sub y+c+/L8  
    :/u EPki  
    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: M;V2O;  
    T3bBc  
    I!{5*~ 3  
    找到Tools工具,点击Open plot files in 3D chart并找到该文件 c+q4sNnE  
      
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    打开后,选择二维平面图: s8R.?mhH=  
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    QQ:2987619807
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