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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。 Ll, U>yo o8~<t]Ejw 成像示意图 -PTfsQk 首先我们建立十字元件命名为Target 6eb~Z6n&? %e(DPX 创建方法: 5,?^SK|'x Q9i[?=F:z 面1 : b-Ru UfUn0 面型:plane 1p8hn!V 材料:Air Z1{>"o:@ 孔径:X=1.5, Y=6,Z=0.075,形状选择Box I.it4~]H OoQLR mDO! o 辅助数据: U:bnX51D4 首先在第一行输入temperature :300K, QW_BT^d" emissivity:0.1; a\}`
f=T =yWdtBng FM7`q7d 面2 : :QC |N@C 面型:plane Y|buQQ| 材料:Air Zgo%Jo 孔径:X=1.5, Y=6,Z=0.075,形状选择Box I3u)y|Y= }s[`T 6FY.kN\
位置坐标:绕Z轴旋转90度, bnJ4Edy tVh"C%Vkr ;,s9jw 辅助数据: ZEso2|
A9MTAm{ 首先在第一行输入temperature :300K,emissivity: 0.1; z0Z1J8Qq6. FH%M5RD 'mZQ}U=< Target 元件距离坐标原点-161mm; qfjUJ/ r1 b"ta FIUQQQ\3 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 eJeL{`NS d4p6.3 !t}yoN
n| 探测器参数设定: p(nEcu "C?H:8W 在菜单栏中选择Create/Element Primitive /plane =.w~qL >`p?
CE d{"@<0i? <W+9h0c u60RuP& >dgz/n?:v 元件半径为20mm*20,mm,距离坐标原点200mm。 Hg$7[um v0?SN>fZ 光源创建: #\_8y`{x P](8Qrl 光源类型选择为任意平面,光源半角设定为15度。 >GLoeCRNu {h
PB% Pm,.[5uc 我们将光源设定在探测器位置上,具体的原理解释请见本章第二部分。 k SgE_W) *eX/ZCn 我们在位置选项又设定一行的目的是通过脚本自动控制光源在探测器平面不同划分区域内不同位置处追迹光线。 7O:g;UI# wJ7^)tTRF u:mndTpB6x 功率数值设定为:P=sin2(theta) theta为光源半角15度。我们为什么要这么设定,在第二部分会给出详细的公式推导。 4c[/%e:\- K)5j 创建分析面: Sp*4Z`^je CD%Cb53 Qqx!'fft 到这里元件参数设定完成,现在我们设定元件的光学属性,在前面我们分别对第一和第二面设定的温度和发射系数,散射属性我们设定为黑朗伯,4%的散射。并分别赋予到面一和面二。 [P6m8%Y|s w*&vH/D `WnsM;1Y" 到此,所有的光学结构和属性设定完成,通过光线追迹我们可以查看光线是否可以穿过元件。 xaVn.&Wl n$v4$_qS FRED在探测器上穿过多个像素点迭代来创建热图 K?r WdlGnFAWh FRED具有一个内置的可编译的Basic脚本语言。从Visual Basic脚本语言里,几乎所有用户图形界面(GUI)命令是可用这里的。FRED同样具有自动的客户端和服务器能力,它可以被调用和并调用其他可启动程序,如Excel。因此可以在探测器像素点上定义多个离轴光源,及在FRED Basic脚本语言里的For Next loops语句沿着探测器像素点向上和向下扫描来反向追迹光线,这样可以使用三维图表查看器(Tools/Open plot files in 3D chart)调用和查看数据。 '.M4yif\g 将如下的代码放置在树形文件夹 Embedded Scripts, v5@M 34 ('AAHq/ -/V(Z+dj 打开后清空里面的内容,此脚本为通用脚本适用于一切可热成像的应用。 (m6V)y o8|qT)O@U 绿色字体为说明文字, ifu!6_b. dfKGO$}V '#Language "WWB-COM" vbd)L$$20+ 'script for calculating thermal image map ;8dffsyq 'edited rnp 4 november 2005 >^GV
#z V)l:fUm2 'declarations JgA{1@h Dim op As T_OPERATION w%8y5v5 Dim trm As T_TRIMVOLUME @0]WMI9B"B Dim irrad(32,32) As Double 'make consistent with sampling d4*SfzB Dim temp As Double ir"t@"Y;o Dim emiss As Double fGqX
dlP Dim fname As String, fullfilepath As String g6;smtu_T aKWxL e 'Option Explicit >3@3~F%xAX J7^UQ Sub Main M=lU`Sm 'USER INPUTS y j#*H nx = 31 3ce$eZE ny = 31 ^X}r ^ numRays = 1000 9}m?E<6& minWave = 7 'microns \"))P1 maxWave = 11 'microns 2QM{e!9 sigma = 5.67e-14 'watts/mm^2/deg k^4 {-8Nq`w fname = "teapotimage.dat" %ut8/T #QIY+muN Print "" C\~}ySQc.e Print "THERMAL IMAGE CALCULATION" 6h2keyod J?yasjjgP detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点
{it}\[3 rq4g~e!S Print "found detector array at node " & detnode AvB=/p@] jC4>%!{m srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 Nw$OJ9$L>
ybw\^t Print "found differential detector area at node " & srcnode =gD)j&~}_ Q;w[o GetTrimVolume detnode, trm DXI4DM"15I detx = trm.xSemiApe !Q15qvRS dety = trm.ySemiApe l`ZL^uT area = 4 * detx * dety KFwuz()7 Print "detector array semiaperture dimensions are " & detx & " by " & dety T3@2e0u ) Print "sampling is " & nx & " by " & ny @#OL{yMy eZqEFMBTm 'reset differential detector area dimensions to be consistent with sampling vt2.
i$u pixelx = 2 * detx / nx OKlR`Vaty pixely = 2 * dety / ny lZL+j6Q SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False (${ #l Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 \t&! &R# n qO*z< 'reset the source power 5X=1a*2'] SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) ]vvA]e Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" xc 1d[dCdp [,,@>nyD 'zero out irradiance array xb3 G,F For i = 0 To ny - 1 bs?\
)R 5/ For j = 0 To nx - 1 rzIWQFv irrad(i,j) = 0.0 5L[imO M0 Next j $cHU, Next i oI/_WY[t ''@Tke3IG6 'main loop w01[oU$x= EnableTextPrinting( False ) [0y,K{8t Zf3(!
a[ ypos = dety + pixely / 2 *3`R W<Z For i = 0 To ny - 1 #p>&|I xpos = -detx - pixelx / 2 PL{lYexJ ypos = ypos - pixely [|oG}'Xz d{JI]
! EnableTextPrinting( True ) oSD=3DQ; Print i (WC
=om EnableTextPrinting( False ) JX&]>#6|E v#&;z_I+ 0*b8?e For j = 0 To nx - 1 A{T9-f@X @I?,!3`jS xpos = xpos + pixelx 7>y]uT@ar 4"kc(J`c 'shift source )VkVZf | S LockOperationUpdates srcnode, True ocWl]h]. GetOperation srcnode, 1, op e}yF2|0FD op.val1 = xpos v)_c*+6u op.val2 = ypos 9e
K~g0m SetOperation srcnode, 1, op m_oUl(pk LockOperationUpdates srcnode, False `aAE4Ry? m`-:j"]b$ 'raytrace <Hr<QiAK DeleteRays @[9 CreateSource srcnode j!i*& TraceExisting 'draw /)J]ItJlz >8I~i:hn 'radiometry :?zq! For k = 0 To GetEntityCount()-1 !AE;s}v)0{ If IsSurface( k ) Then jFdgFKc) temp = AuxDataGetData( k, "temperature" ) 0SYJ*7lPX
emiss = AuxDataGetData( k, "emissivity" ) Yq00<kIDJ If ( temp <> 0 And emiss <> 0 ) Then 1?H;
c5?d& ProjSolidAngleByPi = GetSurfIncidentPower( k ) rtz-kQ38R frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) VQH48{X irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi ^g6v#]&WA End If z3i`O
La Lm=EN%*#9 End If yg'CL/P ^UKY1Q. Next k XLpn3sX$ }EwE#sZ# Next j 1q!k#Cliu #M!$CGi ( Next i YQC.jnb2 EnableTextPrinting( True ) )yb~ kbe _0rt.NRD 'write out file ,jC~U s< fullfilepath = CurDir() & "\" & fname zqdkt ` Open fullfilepath For Output As #1 /ojwOJ Print #1, "GRID " & nx & " " & ny YT!iI Print #1, "1e+308" +BtLd+)R Print #1, pixelx & " " & pixely A'jL+dI. Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 18%$Z$K, >$rH,Er maxRow = nx - 1 qpe9?`vVX maxCol = ny - 1 Uz_ob9l<#H For rowNum = 0 To maxRow ' begin loop over rows (constant X) y|O3*`&m row = "" &77J,\C$: For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) 8/R$}b>< row = row & irrad(colNum,rowNum) & " " ' append column data to row string Z1q<) O1QX Next colNum ' end loop over columns }rmr0Bh :!Q(v(M Print #1, row hk5!$#^ jG`PyIgw Next rowNum ' end loop over rows .jP|b~ Close #1 1VFCK& +sn0bi/rG Print "File written: " & fullfilepath ""
^n^$ Print "All done!!" 1N $OXLu End Sub W#g!Usf:/ h& |