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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。 T/0cPn0> DS+BX`i%#p 成像示意图 e(?1`1 首先我们建立十字元件命名为Target Uw]o9 e0S {e$@i 创建方法: *~~J1.ja> ay
=B<|! 面1 : ~|[i64V<^ 面型:plane iSX HMp4V 材料:Air ]XcWGQv~ 孔径:X=1.5, Y=6,Z=0.075,形状选择Box 8`s*+.LI! IB$i^ 0nvT}[\H* 辅助数据: Sz:PeUr9h 首先在第一行输入temperature :300K, od$$g( emissivity:0.1; p-m\0tQ Ci 'V $VjMd f 面2 : QL @SE@" 面型:plane ^F
qs,^~W 材料:Air uJ=d!Kn 孔径:X=1.5, Y=6,Z=0.075,形状选择Box 2c51kG77E /eT9W[a z0x^HDAeC 位置坐标:绕Z轴旋转90度, (0l>P]"n qo}yEl1 |'lNR)5 辅助数据: o^/ fr&,9 U# IPYyV 首先在第一行输入temperature :300K,emissivity: 0.1; AHMvh 7O? "!&
o|!2 ~c55LlO> Target 元件距离坐标原点-161mm; #S]O|$&* XZQ-Ig18 _>)@6srC 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 -]-0]*oAp ++UxzUd fT{jD_Q+3 探测器参数设定: c(29JZ ;1s;" 在菜单栏中选择Create/Element Primitive /plane 4`'Rm/) c6 .j$6t 3sRI7g Unansk WZjR^6 {MN6JGb|' 元件半径为20mm*20,mm,距离坐标原点200mm。 ,<C~DSAyZ Bio QV47B 光源创建: ~}/_QlX` K Hq~SRc~ 光源类型选择为任意平面,光源半角设定为15度。 N"0>)tG I *f@M} a^^OI|? 我们将光源设定在探测器位置上,具体的原理解释请见本章第二部分。 dQFUQ =*.S<Ko) 我们在位置选项又设定一行的目的是通过脚本自动控制光源在探测器平面不同划分区域内不同位置处追迹光线。 c,]fw2 TwF.UL@G% )Jw$&%/{1 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。 6;@:/kl t
_,v>P2) 创建分析面: 9xK#(M
1D2RhM% *v: .]_; 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。 P(o>UDy C!nbl+75 /1m+iM^V 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。 ^jcVJpyT@R %tPy]{S.. FRED在探测器上穿过多个像素点迭代来创建热图 GO*D4<#u a[,p1}!_ 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。 VV#'d 将如下的代码放置在树形文件夹 Embedded Scripts, I.>8p]X 3[?;s}61 DwK$c^2q{. 打开后清空里面的内容,此脚本为通用脚本适用于一切可热成像的应用。 {9) HB: Q'hs,t1< 绿色字体为说明文字, sO!m,pK( * bhb=~ '#Language "WWB-COM" (dy:d^ 'script for calculating thermal image map 7VdxQ T 'edited rnp 4 november 2005 !aJ6Uf%R ]3Ibl^J 'declarations /n:Q>8^n'W Dim op As T_OPERATION g&Uu~;jq] Dim trm As T_TRIMVOLUME bA'N2~., Dim irrad(32,32) As Double 'make consistent with sampling yigq#h^ Dim temp As Double ^4p$@5zH Dim emiss As Double !w0=&/Y{R Dim fname As String, fullfilepath As String 'c]Pm,Ls jLY$P<u?%P 'Option Explicit 3<[q>7X Q4Qf/q;U Sub Main ;#8xRLW 'USER INPUTS I>6zX nx = 31 eLV[U ny = 31 ??LE0i numRays = 1000 w'y,$gtX/ minWave = 7 'microns oMYZ^b^ maxWave = 11 'microns *o!#5c sigma = 5.67e-14 'watts/mm^2/deg k^4 <(xro/ fname = "teapotimage.dat" x^cJ~e2 K$s{e0
79 Print "" ytV[x Print "THERMAL IMAGE CALCULATION" x2/ciC
8o).q}>& detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 6\VZ6oS e5"5 U7 Print "found detector array at node " & detnode T{N8 K K F7]8*[u srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 I*g[Y= EN,}[^Z Print "found differential detector area at node " & srcnode 7<K=G2_: {d)L0KXK GetTrimVolume detnode, trm LY#V)f detx = trm.xSemiApe xJFcW+ dety = trm.ySemiApe ;RQ}OCz9}8 area = 4 * detx * dety dYlVJ_0Zr Print "detector array semiaperture dimensions are " & detx & " by " & dety SP>&+5AydX Print "sampling is " & nx & " by " & ny 9/I
xh? MOi1+`kwh 'reset differential detector area dimensions to be consistent with sampling 3a}c'$F>_' pixelx = 2 * detx / nx 6JRFYgI pixely = 2 * dety / ny WY5HmNX3E SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False M!%|IKw Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 m& D#5C sWKdqs 'reset the source power ,Vof<,x0 SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) ~\<L74BB Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" ,,Ivey!kL m,}GP^<1i 'zero out irradiance array u%=2g'+)_ For i = 0 To ny - 1 Qv]rj]% For j = 0 To nx - 1 KYl!Iw67d irrad(i,j) = 0.0 ~8-xj6^ Next j glBS|b$\: Next i GNHW bC6_m ,s:viXk 'main loop dVn_+1\L EnableTextPrinting( False ) UA*Kuad SDk^fTV8x ypos = dety + pixely / 2 "{2niBx For i = 0 To ny - 1 Blj<|\igc xpos = -detx - pixelx / 2 l?Ibq} [~ ypos = ypos - pixely 9;L8%T
( 4[Wwm EnableTextPrinting( True ) ][YC.J Print i lB8gD EnableTextPrinting( False ) ::-*~CH) n?9FJOqi 1(e64w@ For j = 0 To nx - 1 +jKu^f6 F6>oGmLy xpos = xpos + pixelx VssWtL _g'x=VJF 'shift source 2h)Qz+|7 LockOperationUpdates srcnode, True ktp<o.f[ GetOperation srcnode, 1, op Q-1Xgw! op.val1 = xpos bU/YU0ZIT op.val2 = ypos NYzBfL
x SetOperation srcnode, 1, op D#^euNiWd LockOperationUpdates srcnode, False "z_},TCy Nx
E=^
v raytrace BPVOBL@ DeleteRays ^uPg71r: CreateSource srcnode OGG9f?? TraceExisting 'draw kdhwnO vI,T1%llu 'radiometry @Qp#Tg<' For k = 0 To GetEntityCount()-1 ViG>gMG v If IsSurface( k ) Then #wZH.i# temp = AuxDataGetData( k, "temperature" ) k~,
k@mR emiss = AuxDataGetData( k, "emissivity" ) /!`xqG# If ( temp <> 0 And emiss <> 0 ) Then I~;H'7|e ProjSolidAngleByPi = GetSurfIncidentPower( k ) 'ud[#@2 frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp )
;kT~&.,y irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi tk>J
mcTw End If wz BI<0]z )t CNp End If Dv&K3^~Rfb Sl@Ucc31 Next k [khXAf1{Q ff~1>=^
Next j "b%FkD Aq\K N. Next i MIb[}w= EnableTextPrinting( True ) | IS$Om q;7DH4;t 'write out file ;V?d;O4u fullfilepath = CurDir() & "\" & fname ~@#a*=" Open fullfilepath For Output As #1 :T<5Tq*+x Print #1, "GRID " & nx & " " & ny <y&&{*KW8m Print #1, "1e+308" 6RDy2JAOP Print #1, pixelx & " " & pixely Ba**S8{/` Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 2 gR*] ?C* H8 xhE~'t maxRow = nx - 1 Z[eWey_ maxCol = ny - 1 2<n@%'OQp For rowNum = 0 To maxRow ' begin loop over rows (constant X) 8;#yXlf row = "" cv7:5P For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) I0!]J{ row = row & irrad(colNum,rowNum) & " " ' append column data to row string !SIk9~rJ Next colNum ' end loop over columns sRqecG(n vTTXeS-b Print #1, row ia_lP VKf&}u/ Next rowNum ' end loop over rows 5}c8v2R:B Close #1 0N$FIw2 Lj3Pp$h Print "File written: " & fullfilepath
Lw%_xRn) Print "All done!!" p<,`l)o}~ End Sub Y*S:/b~y 1Kd6tnX 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: =itQ@``r t[@>u'YKt 0m"Ni:KEf 找到Tools工具,点击Open plot files in 3D chart并找到该文件 `csZ*$7 O%N. ;Ve AWKJ@&pA9m 打开后,选择二维平面图: 3dSC`K J_.cC
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