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    [技术]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: 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。 ?>5[~rMn  
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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 / PG+ s6  
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    创建方法: A<l8CWv[  
    } r$&"wYM  
    面1 : *LpEH,J  
    面型:plane lY/{X]T.(  
    材料:Air zWpJ\/k~  
    孔径:X=1.5, Y=6,Z=0.075,形状选择Box )orVI5ti  
    )&]gX  
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    辅助数据: M*FUtu  
    首先在第一行输入temperature :300K, P'f =r%  
    emissivity:0.1; ,#[0As29u  
    ~>&7~N8  
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    面2 : nf& P Dv1  
    面型:plane 1>P[3Y@}  
    材料:Air qd#?8  
    孔径:X=1.5, Y=6,Z=0.075,形状选择Box ntbl0Sk  
    \"Z^{Y[,;  
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    位置坐标:绕Z轴旋转90度, {Vw+~8  
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    辅助数据: v+uq  
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    首先在第一行输入temperature :300K,emissivity: 0.1; f =@'F=  
    Fb=(FQ2Y?  
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    Target 元件距离坐标原点-161mm; HA&7 ybl  
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    单透镜参数设定:F=100, bend=0, 位置位于坐标原点 I^"ou M9}Q  
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    探测器参数设定: `i5U&K. 7  
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    在菜单栏中选择Create/Element Primitive /plane TI4#A E  
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    元件半径为20mm*20,mm,距离坐标原点200mm。 -!MrG68  
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    光源创建: ~hK7(K  
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    光源类型选择为任意平面,光源半角设定为15度。 MU6|>{  
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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。 *69{#qN  
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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 MzjV>.  
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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。 ql"&E{u?  
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    创建分析面: o6`4y^Q{/  
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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。 PWeCk2xH  
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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。 _)|_KQQu  
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    FRED在探测器上穿过多个像素点迭代来创建热图 EWOS6Yg7  
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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。 dRw O t  
    将如下的代码放置在树形文件夹 Embedded Scripts, fM,!9}<  
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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。 HIiMq'H^  
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    绿色字体为说明文字, x_za R}WI  
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    '#Language "WWB-COM" G!]%xFwYa  
    'script for calculating thermal image map /$NDH]a  
    'edited rnp 4 november 2005 x)evjX=q  
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    'declarations E/bIq}R6  
    Dim op As T_OPERATION "FuOWI{in  
    Dim trm As T_TRIMVOLUME U@t" o3E  
    Dim irrad(32,32) As Double 'make consistent with sampling 0$=Uhi  
    Dim temp As Double EQQ/E!N8l  
    Dim emiss As Double 2n]UNC  
    Dim fname As String, fullfilepath As String 'I$-h<W  
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    'Option Explicit 7D'-^#S5  
    'XW[uK]w)  
    Sub Main -,xCUG<g  
        'USER INPUTS H~Z$pk%  
        nx = 31 y{ & k`H  
        ny = 31 \9;SOAv  
        numRays = 1000 :r4]8X-  
        minWave = 7    'microns %>,B1nt  
        maxWave = 11   'microns )1CYs4lp  
        sigma = 5.67e-14 'watts/mm^2/deg k^4 W&M=%  
        fname = "teapotimage.dat" XKp$v']u  
    JA]TO (x  
        Print "" Q1ox<-  
        Print "THERMAL IMAGE CALCULATION" oZM6%-@qi  
    $qz(9M(m#  
        detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 b5!\"v4c  
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        Print "found detector array at node " & detnode l>(w]  
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        srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 {?2jvv  
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        Print "found differential detector area at node " & srcnode (tZ#E L0  
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        GetTrimVolume detnode, trm Qu 7#^%=  
        detx = trm.xSemiApe v?AQ&'Fk  
        dety = trm.ySemiApe B#o/3  
        area = 4 * detx * dety 3K{XT),  
        Print "detector array semiaperture dimensions are " & detx & " by " & dety | aAu 4   
        Print "sampling is " & nx & " by " & ny 0wFa7PyG?  
    [_$r-FA  
        'reset differential detector area dimensions to be consistent with sampling ?(C(9vO  
        pixelx = 2 * detx / nx `/|S.a#g  
        pixely = 2 * dety / ny B: '}SA{  
        SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False Z`_`^ \"  
        Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 l7{]jKJue  
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        'reset the source power w)Rtt 9  
        SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) BIu%A]e"  
        Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" It5U=PU  
    nqp:nw  
        'zero out irradiance array ;Avz%2#c`  
        For i = 0 To ny - 1 {c 82bFiv  
            For j = 0 To nx - 1 os :/-A_m  
                irrad(i,j) = 0.0 6}V)\"u&   
            Next j .2K4<UOAbm  
        Next i MU  }<-1  
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        'main loop UxGr+q  
        EnableTextPrinting( False ) Mz?xvP?z  
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        ypos =  dety + pixely / 2 z XI [f  
        For i = 0 To ny - 1 >M}\_c=  
            xpos = -detx - pixelx / 2 For`rfR  
            ypos = ypos - pixely sl5y1W/]]  
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            EnableTextPrinting( True ) PZT]H?  
            Print i *\-R&8  
            EnableTextPrinting( False ) MC 8t"SB  
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            For j = 0 To nx - 1 ?&ow:OH+  
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                xpos = xpos + pixelx c `[,>  
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                'shift source @ij8AGE:  
                LockOperationUpdates srcnode, True @yGK $<R  
                GetOperation srcnode, 1, op fbl8:c)I  
                op.val1 = xpos uG5RE  
                op.val2 = ypos MD"a%H#p  
                SetOperation srcnode, 1, op $0kuR!U.N  
                LockOperationUpdates srcnode, False +hUS sR&  
    }NH\Q$IU  
    raytrace k$ ya.b<X/  
                DeleteRays 8!R +wy  
                CreateSource srcnode {r.KY  
                TraceExisting 'draw 2qA"emUM  
    ?{)sdJe  
                'radiometry ;^[VqFpeS  
                For k = 0 To GetEntityCount()-1 ?Aq \Gr  
                    If IsSurface( k ) Then P"Scs$NOU?  
                        temp = AuxDataGetData( k, "temperature" ) jX9{Ki"  
                        emiss = AuxDataGetData( k, "emissivity" ) (Xak;Xum1  
                        If ( temp <> 0 And emiss <> 0 ) Then @]{+9m8G@  
                            ProjSolidAngleByPi = GetSurfIncidentPower( k ) p)x*uqSd  
                            frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) =7e|e6  
                            irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi kVqRl%/3Tb  
                        End If }L!%^siG_  
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                    End If j O-H 1@;  
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                Next k +zl2| '  
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            Next j b`9J1p.;  
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        Next i i[+cNJ|$B0  
        EnableTextPrinting( True ) vqeWt[W v  
    9=l6NNe)|  
        'write out file ORc20NFy7  
        fullfilepath = CurDir() & "\" & fname F0D7+-9[  
        Open fullfilepath For Output As #1 hoj('P2a#n  
        Print #1, "GRID " & nx & " " & ny 8E/wUN,Lxj  
        Print #1, "1e+308" hja;d1yH  
        Print #1, pixelx & " " & pixely <[oPh(!V  
        Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 u%s@B1j  
    'Nqa=_<WW  
        maxRow = nx - 1 tM% f#O  
        maxCol = ny - 1 QE#Ar8tU  
        For rowNum = 0 To maxRow                    ' begin loop over rows (constant X) I7S#vIMXR.  
                row = "" G\;a_]Q  
            For colNum = maxCol To 0 Step -1            ' begin loop over columns (constant Y) ^D}]7y|fm  
                row = row & irrad(colNum,rowNum) & " "     ' append column data to row string C.#\ Pz0  
            Next colNum                     ' end loop over columns Li?_P5+a  
    1DTA Dh0  
                Print #1, row pBbfU2p  
    TwaK>t96[  
        Next rowNum                         ' end loop over rows TV['"'D&i  
        Close #1 hoDE*>i  
    4Y>J,c  
        Print "File written: " & fullfilepath 2 omKP,9,2  
        Print "All done!!" 2!Gb4V  
    End Sub O:I"<w9_1  
    8TH fFL  
    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: ->S# `"@$  
    ~^<1k-  
    B(t`$mC  
    找到Tools工具,点击Open plot files in 3D chart并找到该文件 gZW(z  
      
    5z=.Z\M`8  
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    打开后,选择二维平面图: +v{g'  
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