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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。 s&1}^'| a(lmm@;V< 成像示意图 {43J'WsJ 首先我们建立十字元件命名为Target :D~J(Y2 P DwBSj 创建方法: lr ]C'dD .yB{+ 面1 : 2YK2t<EO 面型:plane Rd[^)q4d$w 材料:Air ?X$*8;==6 孔径:X=1.5, Y=6,Z=0.075,形状选择Box i':a|#e> |IDZMd0 !V-(K_\t 辅助数据: +asO4'r 首先在第一行输入temperature :300K, R# ZO<g%' emissivity:0.1; 7G%:ckg =3dd1n;8> 7m8(8$-6 面2 : 6[-[6%o#z 面型:plane onl,R{,`0 材料:Air CW
-[c 孔径:X=1.5, Y=6,Z=0.075,形状选择Box ZqXp f f o idneus Qh+zs^-? 位置坐标:绕Z轴旋转90度, 0+/ew8~$ (wf3HEb_ 0wt4C% .0 辅助数据: w<Bw2c pA6A*~QE 首先在第一行输入temperature :300K,emissivity: 0.1; 51;[R8'w F>eo.|' A_crK`3 Target 元件距离坐标原点-161mm; KxDp+]N]
Ey%KbvNv a\&g;n8jA 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 +[}<u- - ?in)kL D"exI] 探测器参数设定: 7"1]5\p^g \\;y W~ 在菜单栏中选择Create/Element Primitive /plane hD{
`j R?M>uaxn C7K]c4T Dt(xj}[tC =|dHD ij1YV2v 元件半径为20mm*20,mm,距离坐标原点200mm。 H4$f+ J$lfI^^ 光源创建: qg:EN~E# :6]qr 86 光源类型选择为任意平面,光源半角设定为15度。 ]E6r)C 0{ GJF &id 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。 j4u
["O3 (T%Ue2zlY 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。 $9@AwS@Uu P3nBxw" GWv i
功率数值设定为:P=sin2(theta) theta为光源半角15度。我们为什么要这么设定,在第二部分会给出详细的公式推导。 ,T$ GOjt '8[;
m_S 创建分析面: iB` EJftI! a ," BGHZL~ 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。 zRbY]dW `YqXF=- cICfV,j 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。 UZ#oaD8H6 x2'pl
(^ FRED在探测器上穿过多个像素点迭代来创建热图 lQEsa45 M&)\PbMc 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。 N,l"9>CF 将如下的代码放置在树形文件夹 Embedded Scripts, ~@(C+ 3, M93*"jA Y6Ux*vhK 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。 aNA]hl e\O-5hp7 绿色字体为说明文字, R_\o`v5 Cy*.pzCi '#Language "WWB-COM"
C|h Uyo 'script for calculating thermal image map (.X)= 'edited rnp 4 november 2005 jOzi89 (=%0$(S> 'declarations 57=d;Yg e Dim op As T_OPERATION ib~i ^_p Dim trm As T_TRIMVOLUME r-yUWIr
S Dim irrad(32,32) As Double 'make consistent with sampling %V+"i_{m Dim temp As Double SN]g4}K- Dim emiss As Double ('AAHq/ Dim fname As String, fullfilepath As String -/V(Z+dj (m6V)y 'Option Explicit o8|qT)O@U ifu!6_b. Sub Main dfKGO$}V 'USER INPUTS vbd)L$$20+ nx = 31 W)J MV ny = 31 IvlfX`(" numRays = 1000 V1pBKr)v minWave = 7 'microns LAH">E maxWave = 11 'microns 'nBP% sigma = 5.67e-14 'watts/mm^2/deg k^4 -
jCj_@n fname = "teapotimage.dat" L#uU.U= =5Nh}o(l? Print "" }WaZ+Mdg\ Print "THERMAL IMAGE CALCULATION" ar6+n^pi0] N-_APWA detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 jT}={[9b qw?(^uZNW Print "found detector array at node " & detnode j7lJ7BIr t$wbwP srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 `-OzjbM ^L)TfI_n Print "found differential detector area at node " & srcnode GBT|1c'i `GdH ,:S> GetTrimVolume detnode, trm K3M.ZRh\;` detx = trm.xSemiApe ^D6TeH dety = trm.ySemiApe q7f`:P9~ area = 4 * detx * dety 4(LLRzzW Print "detector array semiaperture dimensions are " & detx & " by " & dety GK!@|Kk8q7 Print "sampling is " & nx & " by " & ny xr7}@rq"U< M<d!j I9) 'reset differential detector area dimensions to be consistent with sampling tx~,7TMS/ pixelx = 2 * detx / nx i?;#ZNh pixely = 2 * dety / ny nq8XVT.m^\ SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False vdC0tax Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 d&raHF* pGjwI3_K 'reset the source power X% j`rQk` SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) 4=/jh:h Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" PJ0~ymE1~G R54ae:8 'zero out irradiance array GWWg3z.o"W For i = 0 To ny - 1 yxHo0U For j = 0 To nx - 1 >Zs! irrad(i,j) = 0.0 8=TC 3] Next j &1yJrj9y Next i wjwCs` D
5n\h5 'main loop 1W{ oj EnableTextPrinting( False ) &K[sb% TB* t^E ypos = dety + pixely / 2 G)%V 3h For i = 0 To ny - 1 kSzap+ nB? xpos = -detx - pixelx / 2 Sx'oa$J ypos = ypos - pixely _<#92v!F $"W[e"Q EnableTextPrinting( True ) wbAwmOiZ Print i IDT\hTPIs EnableTextPrinting( False ) -dA9x~o Pz{MYw m+;U,[%[*E For j = 0 To nx - 1 jVd`J *3fl}l xpos = xpos + pixelx (ct1i>g Mf#@8"l 'shift source oo\^}jb LockOperationUpdates srcnode, True N,-C+r5}<4 GetOperation srcnode, 1, op U&1O op.val1 = xpos Lv['/!DJ| op.val2 = ypos 5>.ATfAsV SetOperation srcnode, 1, op eN.6l2- LockOperationUpdates srcnode, False 7*+CX QUn!&55 'raytrace LYECX DeleteRays pNOE
KiJ CreateSource srcnode +;lDU}$ TraceExisting 'draw jH9PD8D\ b4cTn 6 'radiometry v4s4D1} For k = 0 To GetEntityCount()-1 t2)uJN`a$X If IsSurface( k ) Then 6Q7=6 temp = AuxDataGetData( k, "temperature" ) a<q9~QS emiss = AuxDataGetData( k, "emissivity" ) (0q`eO2 If ( temp <> 0 And emiss <> 0 ) Then .O1w-,= ProjSolidAngleByPi = GetSurfIncidentPower( k ) aOGoJCt
C frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) _Sfu8k>): irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi 4;J.$ End If H 4ELIF#@ F$tzsz,9n End If Mb2a;s 3-hcKE Next k >;,23X / ^d9At614 Next j A?#i{R 4AJT)I. Next i Nmz5:Rq EnableTextPrinting( True ) t;VMtIW+E fVgK6?<8^ 'write out file gU+yqT7= fullfilepath = CurDir() & "\" & fname X,l7>>L{g Open fullfilepath For Output As #1 [k\VUg:P Print #1, "GRID " & nx & " " & ny aSIb0`(3 Print #1, "1e+308" Yv]vl6< Print #1, pixelx & " " & pixely ]^>Inh! Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 W`9{RZ' C;HEvq7 maxRow = nx - 1 k{;?>=FH! maxCol = ny - 1 *Ci&1Mu^Z For rowNum = 0 To maxRow ' begin loop over rows (constant X) I2CI9,0 row = "" 2QbKh) For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) 9ns( F: row = row & irrad(colNum,rowNum) & " " ' append column data to row string d^RcJ3w Next colNum ' end loop over columns /} PdO Sy <E@1 Print #1, row yJC:
bD1xi 1$E [`` n Next rowNum ' end loop over rows +BtLd+)R Close #1 D? %*L YX,;z/Jw2 Print "File written: " & fullfilepath Z72%Bv Print "All done!!" qpe9?`vVX End Sub Uz_ob9l<#H y|O3*`&m 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: &77J,\C$: \[{8E}_"^ Z1q<) O1QX 找到Tools工具,点击Open plot files in 3D chart并找到该文件 }rmr0Bh A2\hmp@A@7 Xk%eU>d 打开后,选择二维平面图: K\Q4u4DjbJ W895@
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