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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。 <RXw M6G2 `<frgXu64 成像示意图 [k<1`z3 首先我们建立十字元件命名为Target =&nW~<- v (xpn`NA 创建方法: nw6pV% i=S~(gp 面1 : W7sn+g\ 面型:plane KP]"P*?
? 材料:Air uLR<FpM 孔径:X=1.5, Y=6,Z=0.075,形状选择Box (?0`d L|j%S m Y,|J\w@ 辅助数据: %aRT>_6" 首先在第一行输入temperature :300K, =r2]uW9 emissivity:0.1; L2UsqVU g}LAks fmX!6Kv 面2 : O`[aU%4b 面型:plane EgjR^A1W2 材料:Air |{>ER,<- 孔径:X=1.5, Y=6,Z=0.075,形状选择Box ^teq[l$; zUJZ`seF p4!:]0c 位置坐标:绕Z轴旋转90度, _}xd}QW ULJ mSe ^D%Za' 辅助数据: u\yVR$pQ )!:sFa
1 首先在第一行输入temperature :300K,emissivity: 0.1; avQJPB)}Sb g4p )kXhtjOl| Target 元件距离坐标原点-161mm; $;N* c H~ ^TY;Zp 'a6<ixgo0 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 \y`+B*\i W,5Hx1z R 8,P-
7^ 探测器参数设定: l7H
qo) b?X.U}62_ 在菜单栏中选择Create/Element Primitive /plane HBS\<} }@ Z56 t_^X$pL aT!'}GjL ~}EMk 3 1RcSTg 元件半径为20mm*20,mm,距离坐标原点200mm。 JF&$t} bV+(b9 光源创建: v{zMO:3 JxE53ev 光源类型选择为任意平面,光源半角设定为15度。 fWfk[(M'9 t7n(Qkrv zi R5:d3 我们将光源设定在探测器位置上,具体的原理解释请见本章第二部分。 wI]"U2L5 o1W:ox?kO 我们在位置选项又设定一行的目的是通过脚本自动控制光源在探测器平面不同划分区域内不同位置处追迹光线。 R'EUV0KX>Y %,Sf1fUJ c0B|F 功率数值设定为:P=sin2(theta) theta为光源半角15度。我们为什么要这么设定,在第二部分会给出详细的公式推导。 JWvjWY2+P ('wY9kvL& 创建分析面: <h%O?mkC poGc a1 Nkxmm/Z 到这里元件参数设定完成,现在我们设定元件的光学属性,在前面我们分别对第一和第二面设定的温度和发射系数,散射属性我们设定为黑朗伯,4%的散射。并分别赋予到面一和面二。 ;<yd^Xs m8'C_U^89 UcBe'r}G 到此,所有的光学结构和属性设定完成,通过光线追迹我们可以查看光线是否可以穿过元件。 `>0MNmu fkf1m:Ckh FRED在探测器上穿过多个像素点迭代来创建热图 \^ghdU *.L81er5~ FRED具有一个内置的可编译的Basic脚本语言。从Visual Basic脚本语言里,几乎所有用户图形界面(GUI)命令是可用这里的。FRED同样具有自动的客户端和服务器能力,它可以被调用和并调用其他可启动程序,如Excel。因此可以在探测器像素点上定义多个离轴光源,及在FRED Basic脚本语言里的For Next loops语句沿着探测器像素点向上和向下扫描来反向追迹光线,这样可以使用三维图表查看器(Tools/Open plot files in 3D chart)调用和查看数据。 1)
ta 将如下的代码放置在树形文件夹 Embedded Scripts, -F'b8:m "k]CW\H6z ?]D"k4 打开后清空里面的内容,此脚本为通用脚本适用于一切可热成像的应用。 yjfat&$ ~ P~ 绿色字体为说明文字, u6>?AW1~ S*j6OwZ '#Language "WWB-COM" lY|Jr{+Ln 'script for calculating thermal image map "Rn3lj0 'edited rnp 4 november 2005 ono4U.C9 =]:> "_jN 'declarations ;"(foY"L Dim op As T_OPERATION
NR;1z Dim trm As T_TRIMVOLUME f|O{#AC Dim irrad(32,32) As Double 'make consistent with sampling :ba5iMa Dim temp As Double K>*a*[t0Sy Dim emiss As Double ylt`*|$ Dim fname As String, fullfilepath As String \
[a%('} oc8:r 'Option Explicit N<QXmgqx O_Oj|'bBC Sub Main [9Ss#~ 'USER INPUTS &u#&@J nx = 31 LpR3BP@At ny = 31 PO6&bIr numRays = 1000 xg)v0y~ minWave = 7 'microns E b=}FuV maxWave = 11 'microns LX^u_Iu sigma = 5.67e-14 'watts/mm^2/deg k^4 ]`Oo%$Ue fname = "teapotimage.dat" 2WU@*%sk" 5 ~TdD6} Print "" jBegh9KHq Print "THERMAL IMAGE CALCULATION" R
{-5Etv zN
[2YJ$ detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 m!<\WN6g cJ54s} Print "found detector array at node " & detnode lP<:tR~K NH+(?TN srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 mdRU^n *zr(Zv Print "found differential detector area at node " & srcnode w8n|B?Sr =}.EY iD GetTrimVolume detnode, trm Mbb x` detx = trm.xSemiApe s`0QA!G{- dety = trm.ySemiApe DZi!aJ area = 4 * detx * dety 0qX3v<+[6 Print "detector array semiaperture dimensions are " & detx & " by " & dety {GC?SaK Print "sampling is " & nx & " by " & ny 3YVi"
k?2 ;VWAf;U;B 'reset differential detector area dimensions to be consistent with sampling }Hn/I,/ pixelx = 2 * detx / nx Q=]w !I\ pixely = 2 * dety / ny Y.*y9)#S6 SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False 0:+WO%z Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 YCP) %} *8LMn 'reset the source power ]Ux<aiY]a
SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) t+eVR8 Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" () j=5KDu 3+XOZh8 'zero out irradiance array ra
o[VZ For i = 0 To ny - 1 ';<0/U For j = 0 To nx - 1 7AObC4 g irrad(i,j) = 0.0 z_|/5$T>U Next j t25,0<iW Next i ['T:ea6B h=:Q-?n- 'main loop }I
:OsAw EnableTextPrinting( False ) "sG=wjcw^ 1;{Rhu7*
k ypos = dety + pixely / 2 -?0qf,W. For i = 0 To ny - 1 %@u;5qD& xpos = -detx - pixelx / 2 zRyuq1Zyc, ypos = ypos - pixely QDu 2?EYZq d!$Z(W0 EnableTextPrinting( True ) UXdUO@ Print i >k'c'7/ EnableTextPrinting( False ) #W|'1
OX4 .,OVzW [<6S%s For j = 0 To nx - 1 Z-l=\ekJ v#!%GEg1r xpos = xpos + pixelx ?#45wC v&=gF/$ 'shift source
~/P&Tub^ LockOperationUpdates srcnode, True <>8WQn,K GetOperation srcnode, 1, op GSRVe/[ op.val1 = xpos MgY0q?.S= op.val2 = ypos uH(f$A SetOperation srcnode, 1, op f`;j:O LockOperationUpdates srcnode, False t{.8|d@
](s'L8(x raytrace s#WAR]x0x DeleteRays 2Tagr1L CreateSource srcnode eN^qG
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TraceExisting 'draw ^3UGV*Ypk sNLs\4v 'radiometry [xGf,;Z For k = 0 To GetEntityCount()-1 [DF,^4g If IsSurface( k ) Then MerFZd 1 temp = AuxDataGetData( k, "temperature" ) |b)Y#)C; emiss = AuxDataGetData( k, "emissivity" ) ,.7*Hpa If ( temp <> 0 And emiss <> 0 ) Then @CT;g\4 ProjSolidAngleByPi = GetSurfIncidentPower( k ) !Y[lQXv frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) -&-Ma,M? irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi v^1pN>#%g End If 7BJzMlJ1Y c5u@pvSP End If kYjGj,m" MZT23[+ Next k
wwyPl J%,*isEL Next j egq67S <kx&w(= Next i sk=-M8;\ EnableTextPrinting( True ) E<Q
f!2s$ l\@)y4
+ 'write out file (G[
*|6m fullfilepath = CurDir() & "\" & fname FgB&b Open fullfilepath For Output As #1 dF2nEaN0% Print #1, "GRID " & nx & " " & ny LyAn&h} Print #1, "1e+308" uLWh| Print #1, pixelx & " " & pixely L2[f]J% Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 0Nnsjh [rSR:V?"a maxRow = nx - 1
.p e( lP maxCol = ny - 1 `0Oh_8" For rowNum = 0 To maxRow ' begin loop over rows (constant X) 7eV
di* row = "" pP*a For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) ;,?KI$K row = row & irrad(colNum,rowNum) & " " ' append column data to row string ;{U@qQD7 Next colNum ' end loop over columns d2H|LMhJ 2(#7[mgPI Print #1, row %3ICI f PM8f Next rowNum ' end loop over rows *q-['"f Close #1 HBu[gh;b @n{JM7ctJ Print "File written: " & fullfilepath k\NMy#]Zt Print "All done!!" i:OK8Q{VI End Sub \uaJ@{Vug CnG+Mc^ 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: Y07ZB'K TX&Jt% !qM=a3 找到Tools工具,点击Open plot files in 3D chart并找到该文件 kNobl F!]lU`z)= Q+W1lv8R 打开后,选择二维平面图: jAm3HI
8n*.).33
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