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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。 xYUC|c1Q9 z;#]xCV 成像示意图 wq@{85 首先我们建立十字元件命名为Target XD=p:Ezh i,z^#b7JQ 创建方法: 8n1<nS< 6<
T@\E 面1 : zs<2Ozv 面型:plane ?wpS 材料:Air :,'yHVG\ 孔径:X=1.5, Y=6,Z=0.075,形状选择Box S(\<@S& ,6iXl ch U6/$CH<pe 辅助数据: n#Y=y# 首先在第一行输入temperature :300K, N!#0O.6 emissivity:0.1; X}@'FxIF +8#hi5e E[8R
)xC@ 面2 : 6*uWRjt 面型:plane T}55ZpSC& 材料:Air ,N`cH\ 孔径:X=1.5, Y=6,Z=0.075,形状选择Box
e#/SFI0m 9H6%\#rw +IkL=/';# 位置坐标:绕Z轴旋转90度, -Y=o }S_#*N)i a2!;$B% 辅助数据: bnYd19> |h6u%t2AY 首先在第一行输入temperature :300K,emissivity: 0.1; BdQ/kXZu+ % r>v^1Vo )@,zG(t5; Target 元件距离坐标原点-161mm; WnkI i,< dtDT^~ 2k]Jkd,E 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 s-"oT= OKO+(>AQ Ak'=/`+ p 探测器参数设定: |iLf;8_: RAUD8Z 在菜单栏中选择Create/Element Primitive /plane ucwUeRw, Sz'H{?" XKQ\Ts2<k wk[4Qsk< H
b}(.` =_:Mx'7 元件半径为20mm*20,mm,距离坐标原点200mm。 > %B7/l$ Y4j%K~lsY 光源创建: aP}30E*Y ,GTIpPj 光源类型选择为任意平面,光源半角设定为15度。 L2}p<?f dZIruZ)x l/6$BPU` 我们将光源设定在探测器位置上,具体的原理解释请见本章第二部分。 .jK,6't^ 3@8Zy:[8< 我们在位置选项又设定一行的目的是通过脚本自动控制光源在探测器平面不同划分区域内不同位置处追迹光线。 fB"It~ p 9J4gDw4< l37)
Q 功率数值设定为:P=sin2(theta) theta为光源半角15度。我们为什么要这么设定,在第二部分会给出详细的公式推导。 1}XESAX;0 [MI ? 创建分析面: "IuPg=|# -?Kd[Ma ^W* 3S[-`g 到这里元件参数设定完成,现在我们设定元件的光学属性,在前面我们分别对第一和第二面设定的温度和发射系数,散射属性我们设定为黑朗伯,4%的散射。并分别赋予到面一和面二。 >V|KS(}s #y>q)Ph \yKYBfp-p 到此,所有的光学结构和属性设定完成,通过光线追迹我们可以查看光线是否可以穿过元件。 t=BXuFiu GX,)~Syw* FRED在探测器上穿过多个像素点迭代来创建热图 ,/Usyb,` W>cHZ. _ FRED具有一个内置的可编译的Basic脚本语言。从Visual Basic脚本语言里,几乎所有用户图形界面(GUI)命令是可用这里的。FRED同样具有自动的客户端和服务器能力,它可以被调用和并调用其他可启动程序,如Excel。因此可以在探测器像素点上定义多个离轴光源,及在FRED Basic脚本语言里的For Next loops语句沿着探测器像素点向上和向下扫描来反向追迹光线,这样可以使用三维图表查看器(Tools/Open plot files in 3D chart)调用和查看数据。 \_|g}&}6Y 将如下的代码放置在树形文件夹 Embedded Scripts, D9/PVd V:*6R/Ft "^&Te%x_b 打开后清空里面的内容,此脚本为通用脚本适用于一切可热成像的应用。 ?
e<D + T'${*NVn 绿色字体为说明文字, d*tn&d~k, /P
koqA, '#Language "WWB-COM" Q8?:L<A 'script for calculating thermal image map Uxb>)36I 'edited rnp 4 november 2005 ['JIMcD |Q*OA 'declarations * G0I2 Dim op As T_OPERATION I|/\ L|vo Dim trm As T_TRIMVOLUME @0&KM|+ Dim irrad(32,32) As Double 'make consistent with sampling 0*F<tg,+] Dim temp As Double /j$`Cq3I Dim emiss As Double ujan2'YT Dim fname As String, fullfilepath As String \wM8I-f! 6u[
B}%l 'Option Explicit -W'T3_ ,]H2F']4Z Sub Main sMNhD/bb 'USER INPUTS `w
K6B5> nx = 31 zya2 O?s ny = 31 wq
=Ef numRays = 1000 >}) W5Y+ minWave = 7 'microns :>3/*"vx?G maxWave = 11 'microns n1PV/ Z sigma = 5.67e-14 'watts/mm^2/deg k^4 AZf$XHP2 fname = "teapotimage.dat" 7 DW_G ?my2dd,| Print "" C|-QU Print "THERMAL IMAGE CALCULATION" `g^b Qx Dt glPo_( detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 [I2vg<my nk.j7tu Print "found detector array at node " & detnode j:P(,M[ R>y/Y<5= srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 QUKv :; <}('w/ Print "found differential detector area at node " & srcnode "pTU&He v!6IH GetTrimVolume detnode, trm
kAnK1W> detx = trm.xSemiApe B'8T+qvA dety = trm.ySemiApe v&r\Z @% area = 4 * detx * dety 2f0qfF Print "detector array semiaperture dimensions are " & detx & " by " & dety r O-=):2 Print "sampling is " & nx & " by " & ny [iUy_ C=qp PS'SI X 'reset differential detector area dimensions to be consistent with sampling ^
RIWW0 pixelx = 2 * detx / nx 6S&OE k pixely = 2 * dety / ny )JXy>q# SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False !~fy".|x Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 0@/C5 v (g3@3.Kk) 'reset the source power ,?(U4pzX SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) g66x;2Q Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" ^k5# {?I 9^1li2z k{ 'zero out irradiance array bT c^huP For i = 0 To ny - 1 "5b4fQ;x For j = 0 To nx - 1 n0%5mTUN irrad(i,j) = 0.0 >?|c>HGX Next j ]:}x 4O# Next i Rg%Xy`gS a,eJO ?? 'main loop tJ9gwx7Pg EnableTextPrinting( False ) -fT}Nj\ X3R:^ff\ ypos = dety + pixely / 2 }dpE> For i = 0 To ny - 1 bEB9J-
Q xpos = -detx - pixelx / 2 Xz\ X 8I ypos = ypos - pixely Rgb&EnVW S0H|:J EnableTextPrinting( True ) 9O|k|FD Print i +@qIDUiF3 EnableTextPrinting( False ) sOhKMz Wiere0 2* o(eh. For j = 0 To nx - 1 rj/1AK y,Z2`Zmu xpos = xpos + pixelx CG]/. uxbLoE 'shift source iH>IV0
< LockOperationUpdates srcnode, True Iwe GetOperation srcnode, 1, op Ib2n Bg>j op.val1 = xpos #Q$e%VJ(c1 op.val2 = ypos Z. ,pcnaQb SetOperation srcnode, 1, op (kL(:P/ LockOperationUpdates srcnode, False @BMuov !112u#V raytrace NfND@m{/ DeleteRays hr`,s!0Y CreateSource srcnode b]g#mQ TraceExisting 'draw hQwUwfoe@ hp$1c 'radiometry .$a|&P=S For k = 0 To GetEntityCount()-1 9gac7(2`) If IsSurface( k ) Then l._g[qa temp = AuxDataGetData( k, "temperature" ) }gKY_e3 emiss = AuxDataGetData( k, "emissivity" ) o ]@'R<F(u If ( temp <> 0 And emiss <> 0 ) Then cv-;fd>' ProjSolidAngleByPi = GetSurfIncidentPower( k ) D*t[5,~j frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) vQ8$C 3 irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi -%TwtO<$'] End If J+l#!gk$! H
$mZ? End If ;E0x#JUrw z?W kHQ9 Next k lm|s% /Nns3oE Next j V\=%u<f T[kS;-x Next i ~(]'ah, EnableTextPrinting( True ) 8@r>`c [~ !9t9+~ 'write out file "rHPcp"m fullfilepath = CurDir() & "\" & fname c3(0BSv Open fullfilepath For Output As #1 \-D[C+1( Print #1, "GRID " & nx & " " & ny =yZ6 $ hK Print #1, "1e+308" {EJ+
Print #1, pixelx & " " & pixely ?MOjtAG0_~ Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 2]V8- 3j2d&*0 maxRow = nx - 1 SK5__Ix maxCol = ny - 1 r=# v@]zB For rowNum = 0 To maxRow ' begin loop over rows (constant X) K0Lc~n/ row = "" #g~]2x For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) VVqpzDoXG row = row & irrad(colNum,rowNum) & " " ' append column data to row string Ymm*p,` Next colNum ' end loop over columns +de5y]1H,| [a7S?%>Bh Print #1, row A>6_h1 ;iz3Bf1o Next rowNum ' end loop over rows WS"v"J% Close #1 #M<u^$Jz |nY+Nen7 Print "File written: " & fullfilepath 5hfx2O) Print "All done!!" 2{S*$K[M End Sub 5")BCA wsgT`M'J[ 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: 'y7<!uo? 0aGAF ] U["IXR# 找到Tools工具,点击Open plot files in 3D chart并找到该文件 z8
K#G%,: 40$9./fe) n1)]. ` 打开后,选择二维平面图: %>t4ib_8 `+(4t4@ew
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