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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。 dc1Zh
W4 .n YlYY' 成像示意图 to&,d`k=- 首先我们建立十字元件命名为Target s>L.V2!$0 Xz)F-C27h 创建方法: /Qr`au 5<v1v& 面1 : 9Scg:}Nj 面型:plane .o/uA 材料:Air ivq(eKy 孔径:X=1.5, Y=6,Z=0.075,形状选择Box ku]?"{Xx V|sV U *xsBFCRU 辅助数据: {R@V 首先在第一行输入temperature :300K, ZBY2,%nAo emissivity:0.1; @d 7V@F0d (Ll'j0]k> U887@-!3 面2 : +M_ _\7 面型:plane S-gO 材料:Air J9]cs?`) 孔径:X=1.5, Y=6,Z=0.075,形状选择Box Rky]F+J a4 N f\7 Is}kCf 位置坐标:绕Z轴旋转90度, -wg}X-'z0 >|kD(}Axf u|Mx} 辅助数据: 1eshuL (,QWK08 首先在第一行输入temperature :300K,emissivity: 0.1; v]F4o1ckk 1Pw1TO"Z
zEW+1-=)+7 Target 元件距离坐标原点-161mm; H~Vf;k> 9.M'FCd~M ~).D\Q\ 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 +#BOWz bK~Toz<k C7NSmZ 探测器参数设定: ]gcOMC &*+$38XE^ 在菜单栏中选择Create/Element Primitive /plane GK'p$`oJm ?%Nh4+3N> sV%DX5@ (M$>*O3SR *{fs{gFw9 4l%W]' 元件半径为20mm*20,mm,距离坐标原点200mm。
Fl=H5HR ~KMah 光源创建: Zc1x"j MU
a[}? 光源类型选择为任意平面,光源半角设定为15度。 ;j1E 6 mWaij]1> c5WMN.z 我们将光源设定在探测器位置上,具体的原理解释请见本章第二部分。 ~i%=1&K&` 4{zy)GE|W 我们在位置选项又设定一行的目的是通过脚本自动控制光源在探测器平面不同划分区域内不同位置处追迹光线。 q q&U)-` C){Q;`M-< 9_:"`)]3B 功率数值设定为:P=sin2(theta) theta为光源半角15度。我们为什么要这么设定,在第二部分会给出详细的公式推导。 bT2G
G S5TVfV5LI 创建分析面: = N*Jis pz['o JXU?'@QY 到这里元件参数设定完成,现在我们设定元件的光学属性,在前面我们分别对第一和第二面设定的温度和发射系数,散射属性我们设定为黑朗伯,4%的散射。并分别赋予到面一和面二。 YQG
l8E' %mT/y%&: %CiF;wJ 到此,所有的光学结构和属性设定完成,通过光线追迹我们可以查看光线是否可以穿过元件。 Ei @ ye$_=KARP FRED在探测器上穿过多个像素点迭代来创建热图 f- 9t m-
<y|3 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。 wX]$xZ!s 将如下的代码放置在树形文件夹 Embedded Scripts, Ju47} t%HB \Yr*x7! aH_c84DS 打开后清空里面的内容,此脚本为通用脚本适用于一切可热成像的应用。 `Fr ,,Q81\ lF!PiL 绿色字体为说明文字, '|ntwK*f diJpbR^JP '#Language "WWB-COM" WC~;t4 'script for calculating thermal image map )>FAtE 'edited rnp 4 november 2005
p)/e;q^ 08nh y[ 'declarations %BkE %ZcZ Dim op As T_OPERATION L4/ns@e Dim trm As T_TRIMVOLUME X#$ oV# Dim irrad(32,32) As Double 'make consistent with sampling ?(=|!`IoO Dim temp As Double apa&'%7 Dim emiss As Double 9#:nlu9 Dim fname As String, fullfilepath As String M+
%O-B WkA47+DsV 'Option Explicit ?Xypn#OPt 1 gjaTPwY Sub Main *%;A85V/ 'USER INPUTS Cb{D[ nx = 31 U U_0@V< ny = 31 xQvI$vP numRays = 1000 M,H8ZO:R minWave = 7 'microns UDi(7c0. maxWave = 11 'microns 9/0H,qZc sigma = 5.67e-14 'watts/mm^2/deg k^4 x/<]/D fname = "teapotimage.dat" ]C,j80+pK ~wW]ntZm Print "" C<^i`[&P$ Print "THERMAL IMAGE CALCULATION" tB>!1}v sX~E ~$_g detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 R|qrK t^":.}[Q Print "found detector array at node " & detnode \UK}B u/j\pDl. srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 HU?1>}4L lot`6] Print "found differential detector area at node " & srcnode j_90iP^5: h7E?7nR GetTrimVolume detnode, trm G^d3$7 detx = trm.xSemiApe [IOI&`?D dety = trm.ySemiApe |=IJ^y(x| area = 4 * detx * dety @3c'4O
Print "detector array semiaperture dimensions are " & detx & " by " & dety /Kli C\ Print "sampling is " & nx & " by " & ny d {U%q
d yP$esDP 'reset differential detector area dimensions to be consistent with sampling e5bXgmyil pixelx = 2 * detx / nx n}Z%D-b$ pixely = 2 * dety / ny G]aey>) SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False W'vek uM Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 ^x O](,H o
i'iZX 'reset the source power 6t; ;Fz SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) UiV#w#&P Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" h<&GdK2U+ ]}/Rl}_ 'zero out irradiance array 1<m`38' For i = 0 To ny - 1 m@+v6&, For j = 0 To nx - 1 D@uVb4uK irrad(i,j) = 0.0 :(US um Next j tjThQ Next i 87! jn'A ~F-knEvL 'main loop
ZJs~,Q EnableTextPrinting( False ) 'M6+(`x A;rk4)lij ypos = dety + pixely / 2 f{VV U/$ For i = 0 To ny - 1 lGYW[0dy xpos = -detx - pixelx / 2 }w4OCN\1
ypos = ypos - pixely [(*Eg!?W= 7#j.yf4 EnableTextPrinting( True ) QD%xmP Print i ~vDa2D<9% EnableTextPrinting( False ) =|AYT6z, P@UE.0NYX *ilh/Hd> For j = 0 To nx - 1 :u9'ZHkZ LI.WcI3uS xpos = xpos + pixelx Vc5>I_ !o`7$`%Wz\ 'shift source .:&`PaMt LockOperationUpdates srcnode, True J(}PvkA GetOperation srcnode, 1, op rGNa[1{kRs op.val1 = xpos V.
i{IW op.val2 = ypos LGuZp?" SetOperation srcnode, 1, op ,(q]
$eOZ LockOperationUpdates srcnode, False fD[O
tc Szt2 "AR raytrace rtAPkXJFM DeleteRays (
y!o CreateSource srcnode Zfk]Z9YO TraceExisting 'draw z0LspRaz G 3U[)(" 'radiometry 9l~D}5e7 For k = 0 To GetEntityCount()-1 b}NNkM If IsSurface( k ) Then ( gg )? temp = AuxDataGetData( k, "temperature" ) bj@sci(1? emiss = AuxDataGetData( k, "emissivity" ) stK}K-=` If ( temp <> 0 And emiss <> 0 ) Then ?l%4
P5 ProjSolidAngleByPi = GetSurfIncidentPower( k ) iw MxTty frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) W2rd[W irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi #b*4v&< End If P]n0L4c !dwZ` D End If s?;8h &]= 3);P!W4> Next k BAXu\a-C_ C~4SPCU Next j N{bg-%s10i
t* Ct* Next i ;SI (5rS? EnableTextPrinting( True ) Nzgi)xX0HX <vWP_yy 'write out file @4UX~=:686 fullfilepath = CurDir() & "\" & fname \{ | GK Open fullfilepath For Output As #1 #pPOQv:~ Print #1, "GRID " & nx & " " & ny "{vWdY|" Print #1, "1e+308" I1m[M? Print #1, pixelx & " " & pixely W7A!QS Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 U9T}iI k%gj maxRow = nx - 1 v#{Nh8n maxCol = ny - 1 [ x+-N7 For rowNum = 0 To maxRow ' begin loop over rows (constant X) ~vt*%GN3 row = "" eik_w(xPT For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) {.k IC@^O row = row & irrad(colNum,rowNum) & " " ' append column data to row string [err$ Next colNum ' end loop over columns gmH`XKi\ v@Eb[7Kq/1 Print #1, row PcA^ jBgGl bL* b>R[x Next rowNum ' end loop over rows ?XdvZf $ Close #1 @~s5 {4 {1Cnrjw Print "File written: " & fullfilepath >}F$6KM Print "All done!!"
9;%$
End Sub 0cKsGDm m-4#s 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: `lE&:) : 8>zo 4|&/#Cz^Y 找到Tools工具,点击Open plot files in 3D chart并找到该文件 :Ef!gpS}?R .S|T{DMQ[ _Ycz@Jn 打开后,选择二维平面图: 0~ nCT&V nI?*[y}
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