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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。 GB;_!69I 0JKTwLhC 成像示意图 suYbD!`( 首先我们建立十字元件命名为Target g9=_^^Tg .*X=["
F 创建方法: J#q^CWN3R |>1#)cONW 面1 : !}5rd\ 面型:plane _xy[\X;9 材料:Air )3<>H!yG} 孔径:X=1.5, Y=6,Z=0.075,形状选择Box s%8,'3& A-J#$B i29a1nD4Hm 辅助数据: i r'C(zD= 首先在第一行输入temperature :300K, kB%.i%9\\ emissivity:0.1; n&a\mGF &|#,Bsk"@ @=
=) 面2 : TuaP 面型:plane 6L)7Q0Z 材料:Air )eqF21\ 孔径:X=1.5, Y=6,Z=0.075,形状选择Box hztqZ: F/[m.!Eo J1Az+m 位置坐标:绕Z轴旋转90度, /a9CqK Pjxj$>&;*j VvT7v] 辅助数据: _Vf>>tuW >YsM'.EF D 首先在第一行输入temperature :300K,emissivity: 0.1; 2E`mbT,v& 7%[ YX kP5G}Bp Target 元件距离坐标原点-161mm; cV_-Bcb x34GRe!! [LUqF?K& 单透镜参数设定:F=100, bend=0, 位置位于坐标原点 G
\Nnw==v )heHERbJ qJ<l$Ig 探测器参数设定: %<'.c9u5 ZLdIEBi= 在菜单栏中选择Create/Element Primitive /plane YU!s;h jSRi 5uOz #hN 0\s&;@xKk -M_>]ubG x9S9%JG : 元件半径为20mm*20,mm,距离坐标原点200mm。 %iJ}H6m ^zS;/% 光源创建: @8+v6z )CmHC3 光源类型选择为任意平面,光源半角设定为15度。 Zb|a\z8 ? 8?x:PkK pd& HC 我们将光源设定在探测器位置上,具体的原理解释请见本章第二部分。 >3&V"^r(|
U0srwt97S 我们在位置选项又设定一行的目的是通过脚本自动控制光源在探测器平面不同划分区域内不同位置处追迹光线。 pn){v {MTtj4$ eH[i<Z 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。 DyA/!%g e@ $|xa") 创建分析面: bR~5
:A^ R,=8)OI2 b&
-8/t 到这里元件参数设定完成,现在我们设定元件的光学属性,在前面我们分别对第一和第二面设定的温度和发射系数,散射属性我们设定为黑朗伯,4%的散射。并分别赋予到面一和面二。 VeZd\Oe IN;9p w KrHKM 3< 到此,所有的光学结构和属性设定完成,通过光线追迹我们可以查看光线是否可以穿过元件。 pjFj{ j]]5&u/l FRED在探测器上穿过多个像素点迭代来创建热图 o)x&|0_ Zk>m!F>,p FRED具有一个内置的可编译的Basic脚本语言。从Visual Basic脚本语言里,几乎所有用户图形界面(GUI)命令是可用这里的。FRED同样具有自动的客户端和服务器能力,它可以被调用和并调用其他可启动程序,如Excel。因此可以在探测器像素点上定义多个离轴光源,及在FRED Basic脚本语言里的For Next loops语句沿着探测器像素点向上和向下扫描来反向追迹光线,这样可以使用三维图表查看器(Tools/Open plot files in 3D chart)调用和查看数据。 @$
lX%p> 将如下的代码放置在树形文件夹 Embedded Scripts, O=lRI)6w@e XW@C_@*J {XUSw8W' 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。 C>mFylN W- nS{v( 绿色字体为说明文字, RrYNtc s0/m qZ]s '#Language "WWB-COM" jp@X,HES 'script for calculating thermal image map csxn"Dz\ 'edited rnp 4 november 2005 1$6
u |W@Ko%om 'declarations |$ZS26aYw} Dim op As T_OPERATION qt/6o|V Dim trm As T_TRIMVOLUME n<<arO"cv Dim irrad(32,32) As Double 'make consistent with sampling s{V&vRr Dim temp As Double .;.Zbhm Dim emiss As Double ^Jdg%U? Dim fname As String, fullfilepath As String \u(Gj]B#" oIIi_yc 'Option Explicit `T ^0&# Gm=&[?} Sub Main ggYi 7Wzsd 'USER INPUTS :`"-Jf nx = 31 Yl?s^]SFU ny = 31 ,# .12Q! numRays = 1000 rg]b$tL~ minWave = 7 'microns E<0Mluk maxWave = 11 'microns Cw kQhj? sigma = 5.67e-14 'watts/mm^2/deg k^4 qe(C>qjMbG fname = "teapotimage.dat" hNgT/y8 x_?K6[G&} Print "" A&%7Z^Pp Print "THERMAL IMAGE CALCULATION" .*>C[^ u|u)8;'9( detnode = FindFullName( "Geometry.Detector.Surface" ) '找到探测器平面节点 ~|ZAS] 3pL4Zhf Print "found detector array at node " & detnode M(C}2.20 )hoVB srcnode = FindFullName( "Optical Sources.Source 1" ) '找到光源节点 6"}F
KRR 7Q~W}`Qv' Print "found differential detector area at node " & srcnode KM"?l<x0Y i.?rom GetTrimVolume detnode, trm B4+u/hkbh? detx = trm.xSemiApe Nlwt}7 dety = trm.ySemiApe bJR\d0Z area = 4 * detx * dety 0]]OE+9<c Print "detector array semiaperture dimensions are " & detx & " by " & dety
vk( I7 Print "sampling is " & nx & " by " & ny v4uQ0~k~X "[7'i<,AI 'reset differential detector area dimensions to be consistent with sampling .'2I9P\! pixelx = 2 * detx / nx CtD<%v3` pixely = 2 * dety / ny \9od*y SetSourcePosGridRandom srcnode, pixelx / 2, pixely / 2, numRays, False <@+L^Ps~z Print "resetting source dimensions to " & pixelx / 2 & " by " & pixely / 2 ,pf\g[tz QyZ'%T5J 'reset the source power sE|8a SetSourcePower( srcnode, Sin(DegToRad(15))^2 ) ;b=7m#5 Print "resetting the source power to " & GetSourcePower( srcnode ) & " units" HJpx,NU' w-v8P`V 'zero out irradiance array k*F9&-rtN For i = 0 To ny - 1 !,5qAGi0 For j = 0 To nx - 1 $M4_"!
irrad(i,j) = 0.0 $-!7<a- Next j 6Rq +=X Next i aYHs35 ^"vmIC.h 'main loop :fy,%su EnableTextPrinting( False ) VAyAXN~ N}{V*H^0QU ypos = dety + pixely / 2 c*"P+ For i = 0 To ny - 1 ,lFzL3'_0x xpos = -detx - pixelx / 2 @$$J}~{ ypos = ypos - pixely > #9
a&O d& v 7l EnableTextPrinting( True ) 4Sdj#w Print i /;21?o EnableTextPrinting( False ) qxZf!NX5 ]2iIk=r$ 1L\r:mx3 For j = 0 To nx - 1 78?{;iNv >Kl_948
xpos = xpos + pixelx Ip8:~Fl] p_apVm\t_ 'shift source >Apa^Bp LockOperationUpdates srcnode, True 7suT26C GetOperation srcnode, 1, op I{%(G( op.val1 = xpos iF.f*3-NJB op.val2 = ypos J^~J& SetOperation srcnode, 1, op [<f9EeziB LockOperationUpdates srcnode, False 92b}N|u d$?+>t/ raytrace jC?l :m? DeleteRays BuC\Bd^0 CreateSource srcnode N"~P$B1X TraceExisting 'draw ^d(gC%+!u Bw[IW[(~! 'radiometry XZ8]se"C For k = 0 To GetEntityCount()-1 I_`NjJ;61 If IsSurface( k ) Then 37M,Os1( temp = AuxDataGetData( k, "temperature" ) X .K*</(g emiss = AuxDataGetData( k, "emissivity" ) 8Vt'X2 If ( temp <> 0 And emiss <> 0 ) Then RgM=g8}M ProjSolidAngleByPi = GetSurfIncidentPower( k ) ^ ~Tn[w W_ frac = BlackBodyFractionalEnergy ( minWave, maxWave, temp ) f&] !;) irrad(i,j) = irrad(i,j) + frac * emiss * sigma * temp^4 * ProjSolidAngleByPi ~ySsv End If -G=.3
bux TvRm 7 End If 6D{70onY+ ~=otdJ Next k
X]GodqL\ 2:yXeSeA Next j [w+1<ou;j O\%0D.HEz Next i v`6vc)>8 EnableTextPrinting( True ) OsYZa`$, 2IkyC` 'write out file E2S#REB4 fullfilepath = CurDir() & "\" & fname Ou
f \%E< Open fullfilepath For Output As #1 ]{ch]m Print #1, "GRID " & nx & " " & ny 2%H_%Zu9 Print #1, "1e+308" .I^Y[_.G Print #1, pixelx & " " & pixely }R hSt] Print #1, -detx+pixelx/2 & " " & -dety+pixely/2 : 'jVA 'I r maxRow = nx - 1 )$*B maxCol = ny - 1 `\=~
$&vjC For rowNum = 0 To maxRow ' begin loop over rows (constant X) ,bB}lU) row = "" -7Kstc- For colNum = maxCol To 0 Step -1 ' begin loop over columns (constant Y) =<ht@-1 row = row & irrad(colNum,rowNum) & " " ' append column data to row string l#p?lBm1 Next colNum ' end loop over columns ,1vFX$ N5x I;UV9' Print #1, row Q,ZV C B.gEV*@ Next rowNum ' end loop over rows xa{.hp? Close #1 MY(51)* |]Y6*uEX< Print "File written: " & fullfilepath W3R43>$ Print "All done!!" xZ QyH End Sub sLK$H|%>m FEV Ya#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: D<*)^^ /}5)[9GC !!~r1)zN 找到Tools工具,点击Open plot files in 3D chart并找到该文件 hN!{/Gc| WO^]bR J*^ i=y 打开后,选择二维平面图: P(LiH I3}I7oc_
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